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ADVANCED POWER ELECTRONIC CONVERTERS AND APPLICATIONS
ADVANCED POWER ELECTRONIC CONVERTERS AND APPLICATIONS
ADVANCED POWER
ELECTRONICS
CONVERTERS
IEEE Press
445 Hoes Lane
Piscataway, NJ 08854
IEEE Press Editorial Board
Tariq Samad, Editor in Chief
George W. Arnold Mary Lanzerotti Linda Shafer
Dmitry Goldgof Pui-In Mak MengChu Zhou
Ekram Hossain Ray Perez George Zobrist
Kenneth Moore, Director of IEEE Book and Information Services (BIS)
Technical Reviewers
Marcelo Godoy Simões, Colorado School of Mines
Hamid A. Toliyat, Texas A&M University
ADVANCED POWER
ELECTRONICS
CONVERTERS
PWM Converters Processing
AC Voltages
EUZELI CIPRIANO DOS SANTOS JR.
EDISON ROBERTO CABRAL DA SILVA
Copyright © 2015 by The Institute of Electrical and Electronics Engineers, Inc.
Published by John Wiley & Sons, Inc., Hoboken, New Jersey. All rights reserved
Published simultaneously in Canada
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Library of Congress Cataloging-in-Publication Data is available.
ISBN: 9781118880944
Printed in the United States of America
10 9 8 7 6 5 4 3 2 1
CONTENTS
PREFACE xi
CHAPTER 1 INTRODUCTION 1
1.1 Introduction 1
1.2 Background 3
1.3 History of Power Switches and Power Converters 4
1.4 Applications of Power Electronics Converters 6
1.5 Summary 9
References 9
CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER
CONVERTERS 10
2.1 Introduction 10
2.2 Power Electronics Devices as Ideal Switches 11
2.2.1 Static Characteristics 12
2.2.2 Dynamic Characteristics 12
2.3 Main Real Power Semiconductor Devices 16
2.3.1 Spontaneous Conduction/Spontaneous Blocking 17
2.3.2 Controlled Conduction/Spontaneous Blocking Devices 18
2.3.3 Controlled Conduction/Controlled Blocking Devices 19
2.3.4 Spontaneous Conduction/Controlled Blocking Devices 22
2.3.5 List of Inventors of the Major Power Switches 24
2.4 Basic Converters 25
2.4.1 dc–dc Conversion 28
2.4.2 dc–ac Conversion 33
2.4.3 ac–dc Conversion 43
2.4.4 ac–dc Conversion 49
2.5 Summary 50
References 52
CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING ac
VOLTAGE AND POWER BLOCKS GEOMETRY 56
3.1 Introduction 56
3.2 Principles of Power Blocks Geometry (PBG) 58
3.3 Description of Power Blocks 62
3.4 Application of PBG in Multilevel Configurations 67
3.4.1 Neutral-Point-Clamped Configuration 68
v
vi CONTENTS
3.4.2 Cascade Configuration 72
3.4.3 Flying Capacitor Configuration 75
3.4.4 Other Multilevel Configurations 79
3.5 Application of PBG in ac–dc–ac Configurations 81
3.5.1 Three-Phase to Three-Phase Configurations 82
3.5.2 Single-Phase to Single-Phase Configurations 85
3.6 Summary 85
References 87
CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION 88
4.1 Introduction 88
4.2 Three-Level Configuration 89
4.3 PWM Implementation (Half-Bridge Topology) 93
4.4 Full-Bridge Topologies 95
4.5 Three-Phase NPC Converter 98
4.6 Nonconventional Arrangements by Using Three-Level Legs 101
4.7 Unbalanced Capacitor Voltage 108
4.8 Four-Level Configuration 112
4.9 PWM Implementation (Four-Level Configuration) 115
4.10 Full-Bridge and Other Circuits (Four-Level Configuration) 118
4.11 Five-Level Configuration 119
4.12 Summary 124
References 124
CHAPTER 5 CASCADE CONFIGURATION 125
5.1 Introduction 125
5.2 Single H-Bridge Converter 126
5.3 PWM Implementation of A Single H-Bridge Converter 129
5.4 Three-Phase Converter—One H-Bridge Converter Per Phase 140
5.5 Two H-Bridge Converters 144
5.6 PWM Implementation of Two Cascade H-Bridges 146
5.7 Three-Phase Converter—Two Cascade H-Bridges Per Phase 149
5.8 Two H-Bridge Converters (Seven- and Nine-Level Topologies) 162
5.9 Three H-Bridge Converters 164
5.10 Four H-Bridge Converters and Generalization 169
5.11 Summary 169
References 170
CHAPTER 6 FLYING-CAPACITOR CONFIGURATION 172
6.1 Introduction 172
6.2 Three-Level Configuration 173
6.3 PWM Implementation (Half-Bridge Topology) 177
6.4 Flying Capacitor Voltage Control 179
6.5 Full-Bridge Topology 181
6.6 Three-Phase FC Converter 183
6.7 Nonconventional FC Converters with Three-Level Legs 186
CONTENTS vii
6.8 Four-Level Configuration 189
6.9 Generalization 196
6.10 Summary 197
References 198
CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS 199
7.1 Introduction 199
7.2 Nested Configuration 200
7.3 Topology with Magnetic Element at the Output 205
7.4 Active-Neutral-Point-Clamped Converters 211
7.5 More Multilevel Converters 214
7.6 Summary 218
References 219
CHAPTER 8 OPTIMIZED PWM APPROACH 221
8.1 Introduction 221
8.2 Two-Leg Converter 222
8.2.1 Model 222
8.2.2 PWM Implementation 223
8.2.3 Analog and Digital Implementation 228
8.2.4 Influence of 𝜇 for PWM Implementation 231
8.3 Three-Leg Converter and Three-Phase Load 233
8.3.1 Model 233
8.3.2 PWM Implementation 235
8.3.3 Analog and Digital Implementation 236
8.3.4 Influence of 𝜇 for PWM Implementation in a Three-Leg Converter 236
8.3.5 Influence of the Three-Phase Machine Connection over Inverter
Variables 238
8.4 Space Vector Modulation (SVPWM) 243
8.5 Other Configurations with CPWM 247
8.5.1 Three-Leg Converter—Two-Phase Machine 247
8.5.2 Four-Leg Converter 249
8.6 Nonconventional Topologies with CPWM 252
8.6.1 Inverter with Split-Wound Coupled Inductors 252
8.6.2 Z-Source Converter 254
8.6.3 Open-End Winding Motor Drive System 257
8.7 Summary 261
References 261
CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS 264
9.1 Introduction 264
9.2 Basic Control Principles 265
9.3 Hysteresis Control 271
9.3.1 Application of the Hysteresis Control for dc Motor Drive 275
9.3.2 Hysteresis Control for Regulating an ac Variable 278
viii CONTENTS
9.4 Linear Control—dc Variable 279
9.4.1 Proportional Controller: RL Load 279
9.4.2 Proportional Controller: dc Motor Drive System 280
9.4.3 Proportional-Integral Controller: RL Load 283
9.4.4 Proportional-Integral Controller: dc Motor 285
9.4.5 Proportional-Integral-Derivative Controller: dc Motor 286
9.5 Linear Control—ac Variable 288
9.6 Cascade Control Strategies 289
9.6.1 Rectifier Circuit: Voltage-Current Control 289
9.6.2 Motor Drive: Speed-Current Control 290
9.7 Summary 293
References 293
CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK
CONVERTER 295
10.1 Introduction 295
10.2 Full-Bridge Converter 296
10.2.1 Model 296
10.2.2 PWM Strategy 297
10.2.3 Control Approach 298
10.2.4 Power Analysis 299
10.2.5 dc-link Capacitor Voltage 301
10.2.6 Capacitor Bank Design 304
10.3 Topology with Component Count Reduction 307
10.3.1 Model 307
10.3.2 PWM Strategy 308
10.3.3 dc-link Voltage Requirement 309
10.3.4 Half-Bridge Converter 310
10.4 Topologies with Increased Number of Switches (Converters in Parallel) 310
10.4.1 Model 311
10.4.2 PWM Strategy 315
10.4.3 Control Strategy 316
10.5 Topologies with Increased Number of Switches (Converters in Series) 318
10.6 Summary 321
References 321
CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK
CONVERTERS 324
11.1 Introduction 324
11.2 Full-Bridge Converter 325
11.2.1 Model 325
11.2.2 PWM Strategy 327
11.2.3 Control Approach 328
11.3 Topology with Component Count Reduction 330
11.3.1 Model 330
11.3.2 PWM Strategies 331
11.3.3 dc-link Voltage Requirement 332
11.3.4 Half-Bridge Converter 332
CONTENTS ix
11.4 Topologies with Increased Number of Switches (Converters in Parallel) 332
11.4.1 Model 333
11.4.2 PWM 338
11.4.3 Control Strategies 339
11.5 Topologies with Increased Number of Switches (Converters in Series) 340
11.6 Other Back-To-Back Converters 340
11.7 Summary 344
References 344
INDEX 347
ADVANCED POWER ELECTRONIC CONVERTERS AND APPLICATIONS
PREFACE
This book deals with a new methodology to present an important class of electri-
cal devices, that is, power electronics converters. The common approach to teaching
converters is to consider each type individually, in a separate and isolated fashion.
The direct consequence is that the learning process becomes passive since the power
electronics configurations are presented without consideration of their origin and
development. Since the teaching process is based on the topology itself, students do
not develop the ability to construct new topologies from the conventional ones.
A systematic approach is taken to the presentation of multilevel and
back-to-back converters, instead of showing them separately, which is normally done
in a conventional presentation. Another special aspect of this book is that it covers
only subjects related to the converters themselves. This will give more room for
exploring the details of each topology and its concept. In this way, the method of con-
ceptual construction of power electronics converters can be highlighted appropriately.
While presenting the basics of power devices, as well as an overview of the
main power converter topologies in Chapter 2, this book focuses primarily on con-
figurations processing ac voltage through a dc-link stage. This text is ideally suited
for students who have previously taken an introductory course on power electronics.
It serves as a reference book to senior undergraduate and graduate students in elec-
trical engineering courses. However, due to the content in Chapter 2, it is expected
that even students who the lack knowledge of power devices and basic concepts of
converters can understand the subject.
Although the primary market for this text is heavily academic, electrical engi-
neers working in the field of power electronics, motor drive systems, power systems,
and renewable energy systems will also find this book useful.
The organization of the book is as follows: Chapter 1 is the introductory
chapter. Chapter 2 presents the basics of power devices as well as an overview of
the main power converter topologies. Chapter 3 provides a brief review of the main
power electronics converters that process ac voltage; additionally, it furnishes the
introduction to the power blocks geometry (PBG), which will be used to describe the
power converters described in this book. In fact, this chapter brings up a compilation
of the topologies explained throughout this book. The fundamentals of PBG and
its correlation to the development of power electronics converters are presented
in a general way. Multilevel configurations are presented from Chapters 4–7.
Neutral-point-clamped, cascade, flying capacitor, and other multilevel configura-
tions are presented in Chapters 4–7, respectively. Chapter 8 deals with techniques
for optimization of the pulse width modulation (PWM), considering the fact that the
number of pole voltages is higher than the number of voltages demanded by the load.
After describing many topologies throughout Chapters 2–7, highlighting the circuits
xi
xii PREFACE
themselves, as well as PWM strategies in Chapter 8, Chapter 9 handles control
actions needed to keep a specific variable of the converter under control. Chapter 9 is
strategically placed before the presentation of the back-to-back converters (Chapters
10 and 11) due to their need for regulation of electrical variables. Single-phase
to single-phase back-to-back converters are presented in Chapter 10, and the final
chapter deals with three-phase to three-phase back-to-back converters.
Euzeli Cipriano Dos Santos Jr.
Edison Roberto Cabral Da Silva
CHAPTER 1
INTRODUCTION
1.1 INTRODUCTION
Power electronics may be considered a revolutionary field in electrical engineer-
ing because of the new insights obtained during its development. This has actually
been the case from the beginning, when mercury arc rectifiers and thyratrons were
employed in grid-controlled circuits. After this first generation of power devices and
converters, power electronics with silicon power diodes and thyristors was developed
to overcome many of the problems of the first generation, such as the operation in low
efficiency. As mentioned in Reference 1, the so-called power electronics, with gas
tube and glass-bulb electronics, was known as industrial electronics, and the power
electronics with silicon-controlled rectifiers began emerging in the market in the early
1960s.
The different definitions of power electronics lead to the same concept or idea:
that the control of power flow between an apparatus that furnishes electrical energy
and another one that demands electrical energy. For instance, the definition given
in References 2 and 3 say, respectively: “ … power electronics involves the study of
electronic circuits intended to control the flow of electrical energy. These circuits can
handle power flow at levels much higher than the individual devices ratings … ” and
“ … power electronics deal with conversion and control of electrical power with the
help of electronic switching devices.”
Power electronics involves several academic disciplines creating a complex
system, including semiconductor physics, control theory, electronics, power systems,
and circuit principles. The comprehensive aspect of power electronics makes the pre-
sentation of its contents difficult. The interdisciplinary nature of power electronics
requires the integration of the practices and assumptions of all the academic dis-
ciplines involved, as well as calling for significant prerequisites on the part of the
students enrolled for the course. Figure 1.1 illustrates this by analogy, with the pre-
requisite skills needed for a power electronics course being shown as the roots of a
tree, the various power electronics devices as the trunk, and the resulting technologies
and applications (power quality, renewable energy systems, etc.) as the branches.
Since the dawn of solid-state power electronics, the use of semiconductor
devices has been the major technology to drive power processors. A comparison
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
1
2 CHAPTER 1 INTRODUCTION
Power
quality
Motor
drive
Renewable
energies
Computer
Control
Electronics
Circuits
Math
Physics
Hybrid
electric
vehicles
Power
systems
Figure 1.1 Interdisciplinary nature
and new insights obtained from
power electronics.
of the semiconductor devices formerly used in controlled rectifiers with new
technologies underlines this dramatic development. In addition to the improvement
of power switches, there has also been great activity in terms of circuit topology
innovations.
A power electronic converter is the centerpiece of many electrical systems.
Common applications include, but are not limited to, motor drive systems, renew-
able energies, robotics, electrical and hybrid vehicles, and circuits promoting power
quality. These applications have required considerable research worldwide to develop
semiconductor devices, configurations that process ac and dc variables, control and
diagnosis, fault-tolerant systems, and the like.
In addition to the technical side mentioned already, the educational aspects have
considerable importance, as students usually consider power electronics courses to
be particularly difficult, perhaps because of their interdisciplinary nature. Achieving
student motivation is thus a fundamental task of educators involved in the field of
power electronics.
In this context, this book discusses a novel methodology for presenting an
important set of power electronics converters, that is, topologies that process ac
voltage. The common approach to teaching converters is to consider each type
individually, in a separated and isolated manner. The direct consequence is that the
learning process becomes passive as the power electronics configurations are pre-
sented without any consideration of their origin and development. Since the teaching
process is based on the topology itself, students develop no ability to construct
new topologies, different from the conventional ones. Section 1.2 outlines this new
methodology.
1.2 BACKGROUND 3
1.2 BACKGROUND
Although presenting the basics of power devices as well as an overview of the main
power converter topologies in Chapter 2, this book focuses primarily on configura-
tions processing ac voltage through a dc-link stage. This book is ideally suited for
students who have already taken an introductory course in power electronics. It also
serves as a reference book to senior undergraduate and graduate students in electrical
engineering courses. However, students can easily manage despite the lack of knowl-
edge of power devices and basic concepts of converters, because they are explained
in Chapter 2.
Systems with power electronics conversion have been used to guarantee grid
and load requirements in terms of controllability and efficiency of the electrical
energy demanded, especially in industrial applications. Power electronics topologies
convert energy from a primary source to a load (or to another source) requiring any
level of processed energy.
Classifications of the power electronics topologies can be done in terms of the
type of variable under control (i.e., ac or dc), as well as the number of stages of
power conversions used, as observed in Fig. 1.2. Figure 1.2(a) shows, in a general
way, many of the possibilities related to energy conversion. Figure 1.2(b) highlights
a direct ac–ac conversion, which converts an ac voltage (v1) with a specific frequency
(f1) to another ac voltage with a different (or same) voltage (v2) and frequency (f2);
this converter is normally called a cycle converter. Figure 1.2(c) depicts the ac–dc
or dc–ac conversion, while Fig. 1.2(d) shows a dc–dc converter. Even admitting
ac
(ν1,f1)
dc
(V3)
(a) (b) (c)
(d) (e) (f)
dc
(V3)
dc
(V4)
dc
(V3)
dc
(V4)
dc
(V4)
ac
(ν2,f2)
ac
(ν1,f1)
ac
(ν2,f2)
ac
(ν1,f1)
ac
(ν2,f2)
ac
(ν1,f1)
dc
(V3)
dc
(V3)
dc
(V4)
dc
(V3)
dc
(V4)
dc
(V4)
ac
(ν2,f2)
ac
(ν1,f1)
ac
(ν2,f2)
ac
(ν1,f1)
ac
(ν2,f2)
Figure 1.2 Power conversion: (a) all possibilities of conversion, (b) cycle converter,
(c) rectifier or inverter, (d) chopper, (e) ac–dc–ac, and (f) dc–ac–dc.
4 CHAPTER 1 INTRODUCTION
that Fig. 1.2(e) and 1.2(f) could be considered as extended versions of the previous
cases, those conversion systems (ac–dc–ac and dc–ac–dc) are presented in Fig. 1.2
because of the large use in different applications.
Special attention is given to the conversion systems presented in Fig. 1.2(c)
and 1.2(e), dealing with configurations that process ac voltage (at input and/or output
converter sides) with one dc stage. A systematic approach is taken for the presenta-
tion of those configurations, instead of just showing them separately, as is normally
done in a conventional presentation. Another aspect of this book is that only the sub-
jects related to the converters themselves will be considered, which means that the
contents dealing with either ac filters or transformers will be omitted. This will give
more room for exploring the details of each topology and its concept. In this way, the
method of conceptual construction of power electronics converters can be highlighted
appropriately.
1.3 HISTORY OF POWER SWITCHES
AND POWER CONVERTERS
Configurations of power electronics converters have provided an attractive alterna-
tive for the applications needing energy processing, considering the acceptable level
of losses associated with the conversion process itself, as well as improvement in
reliability. As previously mentioned, power electronics converters must control the
power flow, which means that the development of the devices used in those convert-
ers is crucial to guarantee the expected features. In this section, a historic view of
the power electronics devices will be furnished, highlighting the main events that
contributed to the current development.
The history of power electronics predates the development of the semiconduc-
tor devices employed nowadays. The first converters were conceived in the early
1900s, when the mercury arc rectifiers were introduced. Until the 1950s the devices
used to build power electronics converters were grid-controlled vacuum tube recti-
fier, ignitron, phanotron, and thyratron. There were two important events in the power
electronics development: (i) in 1948, when Bell Telephone Laboratories invented the
silicon transistor, with applications in very low power devices such as in portable
radios and (ii) in 1958, when the General Electric Company developed the thyristors
or SCR, first using germaniums and later silicon. It was the first semiconductor power
device.
Besides these two events, many developments have been achieved in terms
of switching development. Between 1967 and 1977, the gate turnoff (GTO)
(gate-controlled switch) and gate-assisted turnoff thyristor (GATT) (gate-assisted
turnoff switch) were invented. Power transistors, MOSFETs (metal oxide semi-
conductor field-effect-transistors), MCTs (MOS-controlled thyristor) and IGBTs
(insulated-gate-bipolar transistors) have been invented since the end of 1970s. In
addition, it is worth mentioning that the area of power electronics was deeply
influenced by microelectronics development, and the history of power electronics is
closely related to advances in integrated circuits to control switching power supplies.
1.3 HISTORY OF POWER SWITCHES AND POWER CONVERTERS 5
Power transistors,
MOSFETs (metal oxide semiconductors Field-Effect-Transistors),
MCTs (MOS controlled thyristor) and
IGBTs (Insulated-gate-bipolar transistor)
were invented since the end of 1970s
1977
1980
GTO (gate-controlled switch) and
GATT (gate-assisted-turnoff switch)
were invented
First semiconductor power device.
General Electric Company
developed the thyristor or SCR
1967
Bell Telephone Laboratories
invented the silicon transistor
with former applications in very
low power applications such as
in portable radios
1958
1948
The first investigators
to study controlled
rectification in gas
tubes
The mercury arc rectifier was
invented by Peter Cooper Hewitt.
Before the advent of solid-state
devices, mercury-arc rectifiers
were one of the most efficient
rectifiers
1914
1900
Figure 1.3 Timeline of historical events in the power electronics devices evolution.
Figure 1.3 depicts the timeline showing the development of power electronics
devices.
An important chapter in the history of power electronics converters was the
development of switching power suppliers. In 1958, the IBM 704 computer, which
was developed for large-scale calculations, used as a switching power supplier the
primitive vacuum tube-based switching regulator. But the revolution in power sup-
plier concepts came in the late 1960s, when the switching power supplies replaced the
linear ones. In a linear power supply, regulated dc voltages are obtained from the ac
utility grid throughout the following sequence of steps: (i) 60 Hz power transformer,
to converter 120 ac voltage at the primary transformer side to low voltage at secondary
transformer side; (ii) such voltage is converted to dc with a simple diode rectifier; and
(iii) a linear regulator drops the voltage to a desired value. Indeed, it is possible to
identify many problems related to this technology, such as low efficiency (50–65%
of the power is wasted as heat), and it was heavy and large (mainly due to the low
frequency transformer, heatsink and fans to deal with the heat). The advantages are
that it has a very stable output voltage and the conversion system is noise-free.
To overcome the disadvantages of the linear regulators, General Electric pub-
lished a design of an early stage switching power supply in 1959.
The concept of switching power suppliers is very different from linear regula-
tors. Instead of conducting power 100% of the time (i.e., turning excess power into
heat), the switches and passive elements are connected to rapidly turn the power on
and off. Unlike linear regulators, the ac utility voltage is converted directly to dc volt-
age, and the gating signal controls the time of the switching, regulating the average
voltage desired at the output converter end.
6 CHAPTER 1 INTRODUCTION
Another important development in power electronics configurations was the
controlled rectifiers, especially with the production of the silicon-controlled rectifier
(SCR or thyristor). Such a device allowed the control of high power by just changing
the signal applied to its gating circuit with higher efficiency rather than the older
technology of employing a mercury arc rectifier.
1.4 APPLICATIONS OF POWER ELECTRONICS
CONVERTERS
The range of applications for power electronics converters is so large that it goes
from low power residential applications to high power transmission lines. Many of
those applications can be considered as traditional ones (e.g., rectification circuits and
motor drive systems). On the other hand, a few emerging applications have generated
wide interest (e.g., renewable energy systems). A brief discussion matching the power
electronics converters with those applications will be introduced here, with the details
of those applications being presented throughout the chapters.
Figures 1.4 and 1.5 summarize some examples that demonstrate the presence
of power electronics in a wide range of applications. Figure 1.4(a) shows schemati-
cally the application of power electronics in hybrid/electric vehicles. From the power
Power electronics
apparatus
Memory
CPU
Source
Nano-grid
house
Energy-control-
center
PV
PV
Outlet
ECC
Single-phase
utility grid
Hard
drive
DC
DC
DC
dc
dc
DC
(a)
(c)
(b)
(d)
Figure 1.4 Applications of power electronics using converters that process ac voltage.
1.4 APPLICATIONS OF POWER ELECTRONICS CONVERTERS 7
Macro grid
Micro grid
Power
converter
C
C
ac motor
Wind
generation
C
C C
dc motor
PV generation
C
HEV
Energy Control
Center (ECC)
Loads
T
T
ac
DC
ac
or
Coal-fired
generation
Single-phase
utility grid
Long-distance
transmission
lines
Hydroelectric generation
Centralized
generation
Transformer
Figure 1.5 Application of power electronics in a distributed generation system. C stands for
converter.
electronics point of view, the hybrid and fully electric automobiles differ one from
another, mainly due to the power ratings of the inverters used. While a typical inverter
rating is about 50 kW for the hybrid vehicle, the inverter rating for a fully electric
vehicle is about 200 kW. The inverter motor drive system that furnishes energy to the
power-train is by far the most important power electronics system used in this kind of
8 CHAPTER 1 INTRODUCTION
application, but the battery charge and other peripheral systems are also crucial. The
main features expected in this application are high efficiency performance, compact
on-board energy storage, and low manufacturing cost for market competition with
conventional thermal-engine vehicles.
Desktop and laptop computers can be considered as systems with on-board
distribution schemes where different dc bus voltages are required. Inside these equip-
ment can be found many power electronics converters, as seen in Fig. 1.4(b). An
ac–dc converter produces a dc voltage bus from an ac utility grid, which will be
employed by different dc–dc converters to supply the microprocessor, disk drive,
memory, and so on. In the case of laptops, a battery charger is added with a power
management system to control sleep modes, which guarantees extension in battery
life via power consumption reduction.
Figure 1.4(c) shows the application of the power electronics converters in
renewable energy systems, which nowadays is a hot topic in the political agenda
of many industrialized countries, mainly due to environmental issues and as an
alternative way to establish a decentralized generation system. It is worth mentioning
that, besides the advantages of renewable energy, this kind of system presents a high
price energy generation, especially when it is compared to conventional sources such
as hydroelectric power and coal. In this sense, power electronics converters must
deal with efficiency, reliability, and cost reduction, in order to make those alternative
sources of energy more competitive.
Figure 1.4(d) shows a trolley bus, which is an electric bus that receives electrical
energy directly from overhead wires (generally suspended from roadside posts) by
using spring-loaded trolley poles.
A well-defined traditional power distribution system has a radial topology and
unidirectional power flow to feed end-users. However, in the last few years, there has
been research and development in replacing this paradigm by a new and complex
multisource system with active functions and bidirectional power flow capability. In
this new scenario, the utility grid is supposed to guarantee load management and
demand side management, as well as using market price of electricity, and forecasting
of energy (e.g., based on wind and solar renewable sources) in order to optimize the
distribution system as a whole.
A microgrid can be defined as a localized grouping of electricity generation,
energy storage, and loads that are normally connected to a traditional centralized
grid (macrogrid), as seen in Fig. 1.5. Figure 1.5 shows a microgrid with a dc bus,
where the power converters (represented generically by the letter C) interface dis-
tributed sources and loads with the dc bus. The point of common coupling (PCC)
between micro- and macrogrid can be disconnected, which means that the microgrid
can then operate autonomously. In this case, an island detection system is necessary,
which safely disconnects the microgrid. The interface between micro- and macrogrid
is possible due to advances made in the power electronics
The important equipment in this scenario is the Energy-Control-Center (ECC),
consisting of a bidirectional ac–dc (or dc–ac) power conversion converter used to
interface the utility ac grid and dc bus. The multiple dispersed generation sources
and the ability to isolate the microgrid from a larger network would provide highly
reliable electric power.
REFERENCES 9
Another important area in which power electronics is becoming more and more
common is in aerospace industry. Many loads classically powered by hydraulic net-
works were replaced by electrical power loads (e.g., pumps and braking). Besides
facing the common challenges, the power electronics converters must deal with harsh
environment constraints in terms of temperature, low pressure, humidity, and vibra-
tions.
1.5 SUMMARY
Following the introduction, this chapter presents in Section 1.2 the background of the
book, highlighting the type of configurations that this book will deal with (i.e., dc–ac
and ac–dc–ac converters). Section 1.3 gives a brief history of the power electronics
devices and power electronics converters, focusing on the development of switch-
ing power suppliers and SCR rectifiers. Finally, some applications are considered in
Section 1.4 to show the wide range of applications of power electronics converters.
Readers can find further discussion from References 4 to 13.
REFERENCES
[1] Liserre M. Dr. Bimal K. Bose: a reference for generations [editor’s column]. IEEE Ind Electron Mag
2009;3(2):2–5.
[2] Rashid MH. Power Electronics Handbook: Devices, Circuits, and Applications. San Diego, CA:
Elsevier; 2007. p 1–2.
[3] Bose BK. Power Electronics and Motor Drives: Advances and Trends. San Diego, CA: Elsevier;
2006. p 1–3.
[4] Blaabjerg F, Consoli A, Ferreira JA, van Wyk JD. The future of electronic power processing and
conversion. IEEE Trans Ind Appl 2005;41(1):3–8.
[5] Gutzwiller FW. Thyristors and rectifier diodes - the semiconductor workhorses. IEEE Spectr
1967;4:102–111.
[6] Elasser A, Kheraluwala MH, Ghezzo M, Steigerwald RL, Evers NA, Kretchmer J, Chow TP.
A comparative evaluation of new silicon carbide diodes and state-of-the-art silicon diodes for power
electronic applications. IEEE Trans Ind Appl 2003;39(4):915–921.
[7] dos Santos EC Jr, Jacobina CB, da Silva ERC, Rocha N. Single-phase to three-phase power convert-
ers: state of the art. IEEE Trans Power Electron 2012;27(5):2437–2452.
[8] Goldman A. Magnetic Components for Power Electronics. Kluwer Academic Publishers; 2002.
[9] IBM Customer Engineering Reference Manual: 736 Power Supply, 741 Power Supply, 746 Power
Distribution Unit; 1958. p 60–17.
[10] Karcher EA. Silicon controlled rectifiers in monolithic integrated circuits. Electron Devices Meeting,
1965 International; vol. 11; 1965. p 6–17.
[11] Mohan N, Undeland TM, Robbins WP. Power Electronics: Converters, Applications, and Design.
3rd ed. John Wiley & Sons; 2002.
[12] Rashid MH. Power Electronics: Circuits, Devices, and Applications. Prentice Hall; 1993.
[13] El-Hawary ME. Principles of Electric Machines with Power Electronic. Wiley: IEEE Press; 2002.
CHAPTER 2
POWER SWITCHES
AND OVERVIEW OF BASIC
POWER CONVERTERS
2.1 INTRODUCTION
The basic principles and characteristics of the main power switches are presented
in this chapter. Furthermore, an overview of the principal power electronics
converters is furnished, highlighting the main characteristics for each type of
topology. Semiconductor power devices are the center piece of the power elec-
tronics converters. While the knowledge about such devices is crucial to design
a power converter with specific characteristics for a given application, the study
of different topologies brings up new possibilities to improve the energy process
system.
Before dealing specifically with pulse-width modulation (PWM) converters
processing ac voltage, which is the core of this book, this chapter considers a large
variety of power conversion possibilities. The converters studied in this chapter
include dc–dc, dc–ac, ac–dc, and ac–ac converters, as well as voltage-, and
current-source converters.
As the objective is to furnish an overview of the different types of switches
and converters, a deep analysis of the converters described in this chapter is omit-
ted. However, the following chapters present a systematic description of both power
converters, called Power Block Geometry, and the advanced PWM converters pro-
cessing ac voltage (e.g., multilevel converters and back-to-back converters) to the
smallest detail.
This chapter is organized as follows: Section 2.2 presents the ideal charac-
teristics of the major power switches available in the market, highlighting their
static and dynamic features; Section 2.3 shows the real characteristics of such
semiconductor devices, sorted in terms of dynamic characteristics; Section 2.4
describes basic power electronics converters, and finally, Section 2.5 summarizes the
chapter.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
10
2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES 11
2.2 POWER ELECTRONICS DEVICES AS IDEAL
SWITCHES
The design and construction of power semiconductor devices focus on how to
improve their performance toward the hypothetical concept of an ideal switch.
Figure 2.1 shows the power switches and the year of development of each switch.
The performance of a given power switch is normally measured by its static and
dynamic characteristics. An ideal switch must have the following characteristics:
(i) infinite blocking voltage capability, (ii) no current while the switch is off,
(iii) infinite current capability when on, (iv) drop voltage equal to zero while on, (v)
no switching or conduction losses, and (vi) capability to operate at any switching
frequency.
There are different ways to classify a power switch. In this book, two differ-
ent ways are considered: static characteristics and dynamic controllability. The main
Ideal switch
GalliumARsenide (GAAS)
technology
Silicon carbide (SiC)
technology
BCT - Bilateral conduction
thyristor (1999)
IGCT – Integrated gate-
commutated thyristor (1996)
SITH static induction thyristor,
normally “on” (1983)
MOSFET – metal-oxide field
effect transistor (1975)
TRIAC (1963)
SCR – silicon-controlled
rectifier, thyristor (1956)
Magnetic
amplifier
(1947)
Mercury arc
rectifier (1902)
Thyratron (1920)
Ignitron (1930)
BJT – bipolar
junction transistor (1950)
GTO (1960)
RCT (1963)
IGBT – insulated gate
bipolar transistor (1983)
MTO – MOS turn-off
(1995)
ETO – emitter turn-off
(1998)
Figure 2.1 Development of the power switches toward the concept of the ideal switch.
12 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
figures of merit for the static characteristics are the graphs describing the current
versus voltage behaviors (I–V). On the other hand, for the dynamic features, the
capability to change the states on and off through either an external signal (gat-
ing command) or by the variables of the circuit in which the switch is connected
is considered. For example, there is no gating signal to turn on and off a diode,
its conduction or blocking depends upon the voltage and current imposed by the
circuit.
2.2.1 Static Characteristics
The static characteristics of the power semiconductor devices are related to their abil-
ity to either conduct or block one or two polarities, as shown in Fig. 2.2.
Figure 2.2(a) and 2.2(b) shows the ideal I–V characteristic for the blocking
and conducting states, respectively. Figure 2.2(c)–2.2(g) depicts the voltage versus
current (I–V) ideal characteristics for the main devices found in the market.
The semiconductor devices can, therefore, operate with either unidirectional or
bidirectional (UniC or BidC) current, and with either unidirectional or bidirectional
voltage (UniV or BidV). For example: (i) diode, bipolar junction transistor (BJT),
and insulated bipolar junction transistor (IGBT) are unidirectional voltage and cur-
rent type of devices, (ii) SCR is an unidirectional current and bidirectional voltage
device, (iii) TRIAC and bidirectional controlled thyristor (BCT) are bidirectional in
current and voltage, and (iv) MOSFET is unidirectional in voltage and bidirectional
in current.
The characteristics presented in Fig. 2.2(c)–2.2(g) play an important role for
the specification and design of the power electronics converters. These graphs are
in fact approximations of the real I–V characteristics of the device. For example,
Fig. 2.2(c) is an approximation of the real characteristics of a power diode, which is
presented later in this chapter.
2.2.2 Dynamic Characteristics
The dynamic characteristics of a specific device are related to the behavior of voltage
and current when there is a change either from conduction to blocking state or from
blocking to conduction. Such a change is known as commutation or switching. The
commutation (or switching) from the blocking state to the conduction state is referred
to as either turn-on or conduction. The commutation from the conduction state to the
blocking state is referred to as either turn-off or blocking. For the I–V characteristic
curves (shown in Fig. 2.2), the commutation process corresponds to going from the
operating point on an axis to another one. For example, for a switch UniC/UniV with
direct voltage as in Fig. 2.2(c), the blocking procedure makes the variables of the
switch (voltage and current) go from the I-axis to the V-axis.
In fact, the commutation process can be spontaneous or controlled, as shown
in Fig. 2.3. Four cases are presented as follows:
• Spontaneous conduction (SC)—see Fig. 2.3(a);
• Spontaneous blocking (SB)—see Fig. 2.3(b);
2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES 13
Blocking state
(a)
Conducting state
(b)
Unidirectional current (UniC)
Unidirectional (reverse) voltage
(UniV-r)
(c)
Unidirectional current (UniC)
Unidirectional voltage(UniV)
(d)
Unidirectional current (UniC)
Bidirectional voltage (BidC)
(e)
Bidirectional current (BidC)
Unidirectional voltage (UniV)
(f)
Bidirectional current (BidC)
Bidirectional voltage (BidV)
(g)
i
ν
i
ν
i
ν
i
ν
i
ν
i
ν
i
ν
Figure 2.2 Ideal I–V characteristics for blocking and conduction states of the power
switches available in the market.
• Controlled conduction (CC)—see Fig. 2.3(c);
• CB—see Fig. 2.3(d).
In the case of spontaneous commutation (i.e., conduction and blocking), the
change of state is defined by the variables of the power circuit, while for the controlled
14 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
SC
ν
i
SB
ν
i
CC
ν
i
CB
ν
i
(a)
(c) (d)
(b)
Figure 2.3 Dynamic
characteristics of an ideal device
considering its commutation
process. (a) Spontaneous turn on,
(b) spontaneous turn off, (c)
controlled turn on, and (d)
controlled turn off.
commutation, the change of state is guaranteed via a gating signal (command
signal).
Figure 2.4 shows the behavior of the voltage and current in time-domain (left
side) and dynamic characteristics (right side) for SC, SB, CC, and CB. The points (P1,
P2, and P3) along with the axes in Fig. 2.4 illustrate the behavior of the variables when
the switching process occurs for both spontaneous and controlled commutation. For
example, in Fig. 2.4(a) P1 indicates the operation point when the switch is blocked,
which means that such a device is submitted to a negative voltage while its current is
zero. The operation point P2 shows the device’s behavior while its voltage has been
reduced. Finally, P3 shows the values of voltage and current when the switch is turned
on. This commutation process occurs, for example, in a rectifier circuit with diodes
where the circuit itself allows the state change from blocking to conduction. A similar
analysis can be done for SB in Fig. 2.4(b).
On the other hand, a controlled commutation device must have a control elec-
trode, usually called a gate or base, in addition to the two main terminals. A control
signal applied to the gate or base, while the voltage applied between the main termi-
nals is positive, results in change of state in a desirable manner, that is, from one axis
to another, as shown in Fig. 2.4(c) and 2.4(d).
In terms of dynamic characteristics, the ideal power devices can be classified
as follows:
• SC/SB;
• CC/SB;
• CC/CB;
• SC/CB.
2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES 15
(b)
(a)
(c)
(d)
P3
P3
P3
P2
P2
SC
P2
P1
P1
P1
t
t
i
i
ν ν
P3
P3
P3
P2
P2
SB
P2
P1
P1
P1
t
t
i
i
ν
ν
P2
P2
CC
P2
P1
P1
P1
t
t
i
i
ν ν
P2
P2
CB
P2
P1
P1
P1
t
t
i
i
ν ν
Figure 2.4 Comparison on time-domain
and dynamic characteristics during the
commutation process. (a) SC, (b) SB,
(c) CC, and (d) CB.
16 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES
The most common power electronics devices are diodes, thyristors, and power tran-
sistors. Usually they have two power terminals (anode/cathode, or collector/emitter or
drain/source) and one or more command terminals ( gate/ base). Unlike the ideal char-
acteristics presented earlier, real devices have practical limits for rated voltage and
current, as well as for their operation frequency. Such limits are normally specified by
the datasheet furnished by manufacturers. Therefore, the device characteristics and
their specification are crucial to choose a particular power device instead of others.
The most common nonideal device characteristics are
(a) The Forward and Reverse Voltage Capability. The main limiting ratings are as
follows:
i. Forward Blocking Voltage. The maximum repetitive forward voltage that
can be applied to the power terminals of the device (normally from anode to
cathode, from collector to emitter, from drain to source) so that the device
blocks the current flow (blocking state) in the direct sense, unless com-
manded to turn on.
ii. Reverse Blocking Voltage. The maximum repetitive reverse voltage that can
be applied to the power terminals of the device (from cathode to anode, for
instance) so that the device blocks the current flow in the reverse sense.
iii. Maximum Peak Nonrepetitive Forward and Reverse Voltage. The maximum
nonrepetitive forward and reverse voltages, respectively, under transient
conditions.
iv. Vdc and VR. Maximum continuous direct (forward) and reverse blocking
voltages, respectively. This is the maximum dc voltage that the diode can
withstand in reverse-bias mode on a continual basis.
v. Forward Voltage Drop. This is the instantaneous value of the drop voltage,
which is normally dependent on the temperature.
(b) The current capability while the device is on (conducting) is junction
temperature-dependent. The main limiting ratings are the following:
i. On-State Current. It is the average value of the conduction current.
ii. On-State Root Mean Square (RMS) Current. It is the RMS value of the
conduction current.
iii. Peak Repetitive Forward Current. It is the maximum repetitive current that
can flow through the device.
iv. Peak Surge Forward Current. It is the maximum nonrepetitive forward cur-
rent that can flow through the device under transient conditions.
It should be noted that when blocked, the device still conducts a leakage current
that can be forward or reverse, depending on the device state.
(c) The switching is not instantaneous, so there are limits in the switching fre-
quency, as follows:
i. Turn-On Time. It is the time required to complete the turn-on process.
2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 17
ii. Turn-Off Time or Recovery Time (trr). it is the minimum interval of time
required from the instant the conduction current is decreased to zero so that
the device is capable of withstanding the forward voltage without turning
on.
iii. d𝑣∕dt. It is the maximum variation rate of the forward voltage that can
be applied to the device in the blocking state without starting a nonpro-
grammed turn-on.
iv. di∕dt. It is the maximum variation rate of the forward current during turn-on
that can be applied to the device; higher di∕dt than the one specified by the
manufacturer may destroy the component.
(d) The maximum switching frequency depends on the recovery time of the device.
(e) Power Losses. There are three main components of losses in a semiconductor
device: (i) switching losses (turn-on and turn-off), (ii) conduction losses, and
(iii) reverse conduction losses.
The most used devices in industrial applications are considered in the following
section. Such switches are sorted in terms of their dynamic characteristics.
2.3.1 Spontaneous Conduction/Spontaneous Blocking
The conventional diode and the Schottky diode have the characteristic of SC and SB,
as presented in the sequence.
The Conventional Diode The conventional diode is a silicon p–n junction device
with two terminals, anode (A) and cathode (K), that conducts current from A to K and
blocks the reverse current. The rating of the voltage goes up to 9 kV with 4.8 kA and
5 kV with 13 kA. Its symbol is presented in Fig. 2.5(a) and its real I–V characteristic
is given in Fig. 2.5(b). The diode conducts when 𝑣AK > 0, the current being limited by
the external circuit, its typical direct voltage drop is 0.7 V. Generally speaking, it can
be said that they recover their reverse blocking capability when the forward current iA
goes to zero and a reverse voltage is applied across its terminals, for an interval of time
longer than the reverse recovery time trr obtained in its technical data sheet. In reality,
after reaching zero, the current reverses its direction, reaching a reverse peak called
“peak reverse recovery current” that is comparable to the forward current. Snubber
K
νAK
A
iA
iA
(a) (b)
Figure 2.5 The diode: (a) symbol and
(b) I–V characteristic.
18 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
circuits are essential for the adequate protection of the diode. The snubber circuit will
protect it from overvoltage spikes, mainly due to the junction capacitance and leakage
inductance from terminals and circuit connections. The basic snubber circuit is com-
posed of a capacitor in series with a resistor connected in parallel with the diode. The
size of the snubber circuit is reduced for the fast (trr < 1 μs) and ultrafast recovery
diode (trr < 100 ns), with ratings reaching: (i) 600 V, 30 A and trr = 50 ns, and (ii)
1200 V, 120 A, trr = 85 ns. Recent development in the silicon carbide material allows
reducing the diode reverse recovery time up to 16 ns.
The Schottky Diode Unlike the standard diode presented previously, the Schottky
diode is formed by a metal–semiconductor junction (the p material is replaced by
metal). It has a lower conduction drop voltage (typically 0.5 V) and faster switching
time than the standard diode (less than 100 ps), which allows its operation in higher
frequency. However, it has lower blocking voltage (typically up to 200 V) and higher
leakage current. Its silicon carbide (SiC) version is promising and has been already
tested to withstand 1.2 kV with 60 A.
2.3.2 Controlled Conduction/Spontaneous Blocking Devices
The main devices in this group are the silicon-controlled rectifier (SCR) and the TRI-
ode AC (TRIAC).
The SCR The SCR is a silicon p–n–p–n device with three terminals: two power
terminals, anode (A) and cathode (K) through which the current flows, and a control
terminal, named the gate terminal (G). It is unidirectional in current and blocks in
both forward and reverse directions (UniC/BidV). The device is triggered by a posi-
tive gate current pulse. When the gate is not triggered the SCR blocks the current in
the forward direction even with 𝑣AK > 0. If iGK > 0 while 𝑣AK > 0, the SCR conducts
the current from anode to cathode imposed by the circuit in which the SCR is inserted.
Its voltage drop in conduction is from 1 to 4 V. Once in conduction, the SCR behaves
like a diode and it can only be turned off when the anode current becomes zero. After
the current reaches zero, a reverse voltage should be applied across its terminals in
order to accelerate the capability of forward blocking. Note that the gate loses con-
trol over the SCR during its conduction. The symbol and real I–V characteristics are
shown in Fig. 2.6(a) and 2.6(b), respectively. The direct and reverse voltages across
its terminals are symmetrical in the conventional SCR (there are SCRs with asym-
metrical voltage characteristics, the ASCR) and can reach 5 kV with 5 kA and 12 kV
with 2.3 kA, or even 5 kV with 8 kA. Unexpected turn-on can occur due to a high
d𝑣∕dt. For these reasons a snubber circuit with a capacitor can be used to avoid both
triggering by d𝑣∕dt and overvoltage spikes, a resistor that limits the current peak, and
an inductor that limits the di∕dt rate.
The TRIAC The TRIAC is a thyristor that operates as two SCRs monolithically
integrated connected in antiparallel. Such a device can conduct and block in both
forward and reverse directions (BidC/BidV). It has two power terminals, T1 and T2,
and one gate G. Its symbol and its I–V characteristic are presented in Fig. 2.7(a) and
2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 19
K
G
νAK
A
iA
iA
(a) (b)
Figure 2.6 The SCR: (a)
symbol and (b) I–V
characteristic.
2.7(b), respectively. When 𝑣T = 𝑣T1 − 𝑣T2 is positive (quadrant I) and the TRIAC is
turned on by a positive gate current pulse. But when the 𝑣T is negative (quadrant III)
it is turned on by a negative gate current pulse. The operation in quadrants II and IV
is also possible but the gate triggering is less sensitive in these cases. Also, the d𝑣∕dt
is poorer than that of SCRs.
Other CC/SB devices are the light-activated SCR (LASCR), the reverse con-
ducting thyristor (RCT), which functions as an SCR with an inverse-parallel diode
(BidC/UniV), and the BCT, in which two SCRs are also connected in antiparallel,
but differently from the TRIAC, each one acting independently with its independent
gate control (BidC/BidV).
2.3.3 Controlled Conduction/Controlled Blocking Devices
The main CC and CB devices are (1) basic transistors, like the BJT and the metal oxide
semiconductor field-effect transistor (MOSFET); (2) basic thyristors, like the gate
turn-off (GTO); (3) mixed transistors, like the IGBT; and (4) mixed thyristors, like
the MOS-controlled thyristor (MCT) and the Integrated gate commutation thyristor
(IGCT).
Bipolar Junction Transistor (BJT) Unidirectional in current, the BJT can be
either n–p–n or p–n–p and it has asymmetric blocking, only withstanding some
tens of reverse blocking voltage (UniC/UniV). Its symbol and static characteristics
T2
T1
G
νT
iT
iT
(a) (b)
Figure 2.7 The TRIAC: (a)
symbol and (b) I–V
characteristic.
20 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
B
E
C
iB = 0
iC
iB
iC
iB
νCE
(a) (b)
Figure 2.8 The BJT: (a)
symbol and (b) I–V
characteristic.
are shown in Fig. 2.8. It has three terminals, the collector (C) and emitter (E) through
which the current (ic) flows and the base (B) that controls the amplitude of ic. Unlike
lower power BJT devices, the power devices operate in the quasi-saturated region,
which reduces the stored charge, avoiding the long recovery time obtained when
operated in the saturated region. As its dc current gain (hfe) is much lower than its
signal level counterpart (in general as low as 5), the Darlington connection is more
common because its dc current gain is higher. A disadvantage of this arrangement
is its drop voltage and leakage current. BJTs with forward blocking voltage up to
1 kV are available.
The MOSFET Application of the metal oxide semiconductor (MOS) technology to
the field-effect transistor resulted in the power MOSFET. It has three terminals, the
drain (D), the source (S), and the gate (G).
Its symbol and I–V characteristics are shown in Fig. 2.9. It is an n–p–n, or
p–n–p, device in which its two p–n, or n–p, layers are connected through a metal,
so that a capacitor is formed between G and D. The MOSFET is turned on by a
voltage pulse. The MOSFET acts as a resistance while conducting and behaves
like a transistor before being turned on. Similar devices have been developed
under different names, depending on the manufacturer, such as the HEXFET
(“hexagonal-field-effect-transistor”), SIPMOS (“Siemens-Power Metal Oxide
Silicon”) and TMOS (“T flowing current metal oxide silicon”). Its forward blocking
voltage is in the range of 1 kV and it can operate in high frequency. Since it has
an intrinsic diode in antiparallel connection, it operates with forward and reverse
current and can be classified as a BidC/UniV device. It has replaced the BJT in the
range of low voltage and high frequency but its disadvantage comes from its high
conduction resistance that increases with the voltage.
G
S
D
νGS = 0
iD
iD
νGS
νDS
(a) (b)
Figure 2.9 The MOSFET:
(a) symbol and (b) I–V
characteristic.
2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 21
G
E
C iC
iC
νGE
νCE
(a) (b)
Figure 2.10 The IGBT: (a)
symbol and (b) I–V
characteristic.
However, it has been demonstrated that SiC MOSFET can have extremely low
on-resistance, thus saving energy. It has been predicted that in some applications the
SiC MOSFET will replace the Si-IGBT in the voltage range of more than 1 kV.
The IGBT The IGBT promoted a great revolution in power electronics as it uses
a mixed bipolar-MOSFET technology. It combines the advantages of the MOSFET
and the BJT Darlington, with controlled turn-on and turn-off. Like the MOSFET it
has a high input impedance and needs low energy to be switched on. Its symbol and
I–V characteristics are given in Fig. 2.10. The IGBT conduction drop voltage is small
(from 2 to 3 V in a device of 1 kV). The conventional device is unidirectional in cur-
rent and only blocks forward voltage (UniI/UniV) with a voltage of 6.5 kV for 750 A,
or 1.7 kV for 3.6 kA for d𝑣∕dt of order from 50, 000 V∕μs to 100, 000 V∕μs. The type
NPT (“nonpunch-through”) can reach 3.5 kV and 2 kA. Its typical turn on and turn
off time is from 200 ns to 1 μs. It is possible to design it to block the voltage in both
directions, forward and reverse voltages. Such a device has been recently introduced
in the market with the name of reverse blocking IGBT but for lower voltage (1.7 kV)
and current (25 A), 1200 V∕40 A, 600 V∕200 A. As for the MOSFET, the SiC tech-
nology is also designing SiC–IGBT, which has reached the high blocking voltage
of 15 kV.
The GTO The GTO did appear to give thyristors the option to control its turn-off.
Its symbol and I–V characteristics are given in Fig. 2.11 and it is, normally, a
UniC/UniV device. For turning on, it only needs a small pulse of positive current at
the gate. However, its turn-off current gain of the negative current pulse is typically
3–5, which means that for turning off a 6 kV∕6 kA GTO, it needs a negative gate
A K
G
iA
iA
νAK
(a) (b)
Figure 2.11 The GTO: (a)
symbol and (b) I–V
characteristic.
22 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
current pulse of 1.5 kA. The reverse blocking GTO can withstand reverse voltage
of 4.5 kV with 3 kA. Also, the GTO needs snubbers when used with inductive
load.
The MCT The MCT is also called MOS-GTO and combines the characteristics of
the FET integrated with the p–n–p–n structure of a thyristor. It is a UniC/UniV
device. When designed, it was expected that it would be able to handle more than
200 kVA and more than 1 MVA in subsequent years. In conduction, it approximates
to the SCR characteristics. Its blocking is obtained through the turn-off gate. How-
ever, even though it reached values of 2 and 3 kV and hundreds of amperes, its
acceptance by the market is still undefined at the moment. Its symbol is given in
Fig. 2.12(a).
The IGCT The IGCT was introduced in 1997 and it is a high voltage, high power,
asymmetric blocking device, with a structure very similar to a GTO thyristor. As it is
designed with a monolithically integrated antiparallel diode, it is a BidC/UniV type
of device. Its symbol is given in Fig. 2.12(b). It is a device with unity turn-off current
gain. This means that a 4.5 kV IGCT with a controllable anode current of 3000 A
requires a turn-off negative gate current of 3 kA. So it needs a great amplification
for turn off and, also, the gate driver must have an ultralow leakage inductance in
order to have short duration and very large di∕dt. With this purpose, the gate drive
circuit is built in and such integration between the command and the device results
in high turn-off speed (1 μs) and basically eliminates the problem of d𝑣∕dt found in
GTOs permitting snubberless operation. In IGCTs the cathode current is diverted to
the gate before any distribution of current between gate and anode is observed so that
the structure p–n–p–n can be converted to a p–n–p structure. As a result, the IGCT
conducts as a GTO but turns off as an IGBT, combining the characteristics of these
devices. Other parameters superior in the IGCT as compared to the GTO are the con-
duction drop voltage and gate-driver loss. Its typical frequency is around 500 Hz it can
reach 1 kHz. The device has been applied in power system installations of 100 MVA
and medium power (up to 5 MW) industrial drives. Like the GTO and IGCT, the
reverse blocking IGCT (RBIGCT), symmetric, has been recently developed, and can
withstand 5 kV.
2.3.4 Spontaneous Conduction/Controlled Blocking Devices
Two devices can be classified as SC/CB, that is, the static induction transistor (SIT)
normally-on and the Static Induction Thyristor (SITH) normally-on.
K
K
A
G
G
A
(a) (b)
Figure 2.12 Symbol of the: (a) MCT and
(b) IGCT.
2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 23
K
S
D
G
G
A
(a) (b)
Figure 2.13 Symbol of: (a) SIT and
(b) SITH.
The SIT The SIT, also known as Junction Field-Effect Transistor (J-FET), is an
n-type field-effect transistor, voltage driven. Its symbol is given in Fig. 2.13(a). It is a
UniC/UniV device with ratings of 1.2 kV and 300 A and can operate up to 100 kHz.
It conducts when 𝑣GS = 0 and its drain current can be controlled by the gate-source
voltage, 𝑣GS. However, the gate-source voltage required for turning off the device is
high and it is not uncommon that a voltage as high as 40 V (negative) is needed. This
characteristic of normally turned on with controlled turn-off classifies the device as
SC/CB (the SIT normally-off has been already developed, with limited performance).
However, its high forward voltage makes it unsuitable for most power electronics
applications, unless radio frequency operation is needed. Additionally, the difficulty
in manufacturing it raises concerns about its mass production. This device has been
shown to be more promising with the SiC technology reaching ratings of 1.2 kV∕17 A
and 6.5 kV∕5 A. Its range of power operation is up to 50 kW. It has been shown
that a SiC SIT of 125 V∕2.2 kW can operate in the ultrahigh frequency range up to
450 MHz. However, the gate-source voltage required for turning this device off is
about VGS = −30 V. Although SiC SIT is a normally-on device, recently a SiC SIT
normally-off has been developed with ratings of 1.2 kV and 35 A, with a turn-off VGS
of only −2.5 V.
The SITH The SITH, or SIThy, a device unidirectional in voltage, is a combination
of an n-channel SIT and a p–n–p transistor. Its symbol is given in Fig. 2.13(b). It is
a normally-on device with turn-off controlled by negative gate voltages and it does
not have reverse blocking capability. It can handle currents in the range of 300 A to
2 kA with a recovery time from 2 to 4 μs and it is a device rated with 1.5 kV∕300 A
and has a rated frequency of 10 kHz but it is expected to be applied to power sources
up to 10 MHz. Although it can operate at higher frequencies compared to the GTO,
its higher drop voltage and lower current gain are its main disadvantages. As for the
SIT, the complexity of the manufacture process and the high negative gate voltage
for turning it off are its major drawbacks.
Exercise 2.1
The simple circuit presented below allows the power flow control between the
voltage source (Vdc = 1 kV) and the resistive load (Ro), by turning-on and -off
the switch S with switching frequency equal to fs. From the ratings of the
24 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
switches given in this chapter determine the appropriate power device to be
employed as the switch S, considering the following conditions:
(a) fs = 1 kHz and Ro = 0.6
(b) fs = 50 kHz and Ro = 2.5
(c) fs = 200 kHz and Ro = 10.
Vdc
S
Ro
2.3.5 List of Inventors of the Major Power Switches
The list of inventors of the major power devices available in today’s market is pre-
sented here:
• Diode pn. The first semiconductor diode, a germanium-made device, was cre-
ated in 1952, 200 V/35 A, by R.N. Hall. Its counterpart in silicon was invented
by Russell Ohl at Bell Laboratories, 500 V.
• BJT. In 1947, W. Shockley, J. Bardeen, and W. Brattain built a germanium
point-contact transistor. The BJT was created by W. Shockley from Bell Lab-
oratory in 1948 and developed in 1950 for 500 V/20 A. The first commer-
cially available silicon devices (grown junction) were manufactured in 1954 by
Gordon Teal.
• SCR (Thyristor). The SCR or thyristor was proposed by William Shockley in
1950. It was theoretically described in 1954 and 1955 by J.L. Moll from Bell
Laboratory but it was not well accepted until GE manufactured a feasible device
in 1957. Its commercial version was available in 1958 and was championed by
G. E.’s Frank W. “Bill” Gutzwiller (300 V/16 A).
• GTO. The GTO thyristor was created in 1962 by R. Aldrich and N. Holonyak
from GE. It was used until the 1970s when it was replaced by the silicon power
MOSFET and IGBT. This happened because the GTO was limited to low cur-
rent. For instance, in 1967 its maximum rates were 500 V/10 A. However, an
improved Hitachi GTO was developed in 1981 allowing for higher voltage and
current (2500 V/1000 A).
• TRIAC. The bidirectional triode thyristor was created by F. W. Gutzwiller, from
GE, in 1963. It reached 40 A experimentally but the first commercial Triacs
were the SC40 and SC45, rated 200 V, 6 A, and 10 A, in 1965 and 1966,
respectively, following basic research steps developed by GE’s Aldrich and
Nick Holonyak (1958), and Finis E. Gentry and Tuft (1963).
• RCT. The RCT was created in 1970 by Kokosa and B. Tuft from GE.
2.4 BASIC CONVERTERS 25
• MOSFET. The first metal-oxide field-effect transistor was created in 1958 and
reported in 1960 by D. Kahng and M.M. Atalla, from Bell Laboratory. How-
ever, the first successfully commercialized power MOSFET was from Interna-
tional Rectifier.
• SITH or FCT (Field-Controlled Thyristor). The SITH was proposed by
J. Nishizawa from Mitsubishi Electric Corporation in 1975 (700 V); in the
same year a similar device that received the name of FCT was reported by
D.E. Houston.
• IGBT. The first IGBT with substantial current ratings was developed in 1982
by J. Baliga, from GE, with a symmetric blocking voltage of 600 V for 10 A
(6 kVA). It was also reported by J.P. Russel in 1983 under the name of COM-
FET, reaching 400 V and 30 A.
• SIT (normally “on” or JFET) was introduced by J. Nishizawa in 1975, 300 V,
2 A, with an output power of 5 W at 1 GHz, 36W at 200 kHz and 40 W at
100 MHz.
• BCT. The bilateral controlled thyristor was created by ABB in 1998, having
voltage and current ratings of 6.5 kV and 1390 A.
• IGCT. The IGCT was conceived in 1993 at ABB and reported in 1996 by P.K.
Steimer, H. Gruning et al. from ABB for 4.5 kV and 3 kA. It was also reported
in 1996 by J. Sakano et al. from Hitachi and was able to block 4 kV.
• MTO. The MOS turn-off thyristor was invented in 1995 by D.E. Piccone et al.
from Silicon Power Corporation, with rated values of 6000 V and 500 A.
2.4 BASIC CONVERTERS
As mentioned earlier, a power electronics converter interfaces a source and a load
(or another source). The source can be either of voltage type or current type. Also,
the load can be of either voltage type (e.g., a capacitive load) or current type (e.g.,
an inductive load). The connection between a source and a load should obey the
following sequences: (i) voltage (V)–current (I)–voltage (V)–current (I), or (ii)
current (I)–voltage (V)–current (I)–voltage (V). Four connections between source
and load are then possible, as shown in Fig. 2.14, which establishes the following
connections, V –I, I–V, V − V and I–I. Notice that, for the V –V connection
as in Fig. 2.14(c), the power converter interfacing load and source are expected
Power
converter
Power
converter
Power
converter
Power
converter
(d)
(c)
(b)
(a)
+
–
+
–
+
–
+
–
Figure 2.14 Four possibilities of connection between source and load.
26 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
to have an inductor element inside that block. The same rationale applies for
Fig. 2.14(d).
Only sources and loads of different types can be directly connected, that is: (i)
a voltage source can be directly connected to a current-type load and (ii) a current
source can be directly connected to a voltage-type load. Such a restriction comes
from the need to avoid, for example, a parallel connection between two voltage-type
elements, and so preventing short-circuit between these two elements.
Except for the case of resistive load, the minimal number of switches that
allows interconnecting a source and a load is two, which is called basic commutation
cell. In fact such a commutation cell can be obtained with two different arrange-
ments, as seen in Figs 2.15 (Cell I) and 2.16 (Cell II). Cell I in Fig. 2.15(a), also
known as leg when it is arranged as presented in Fig. 2.15(b), can be used to con-
nect a voltage source to an inductive load. In Fig. 2.15(c), the source is connected
between points M and N while the load is connected to the point A, named as pole.
Instead, in Cell II in Fig. 2.16(a), or its leg representation [Fig. 2.16(b)], the cur-
rent source connected to point A allows feeding a capacitive load connected between
points M and N (voltage-type load), as shown in Fig. 2.16(c). It should be noticed
that while one of the switches is conducting, the other one is turned off. Note that
the pole (point A) can be connected to either point M or point N, so that it can only
assume the potential of those points. For this reason, both cells are said to be two-level
cells.
S1
S1 S1
S2 S2 S2
A
A A
N N
(a) (b) (c)
M
M
N
M
Figure 2.15 Basic cell employed to connect voltage source to current-type load.
S1
S1
S2 S2
A A
N N
(a) (b)
M
M
S1
S2
A
N
(c)
M
Figure 2.16 Basic cell
employed to connect
current source to
voltage-type load.
2.4 BASIC CONVERTERS 27
(a) (b)
(c) (d)
C
S1
S2
+
–
S1
S2
+
–
+ –
S1 S2
L
+
–
+
–
Figure 2.17 Principles for building power converters.
Figure 2.17 shows how different types of sources and loads can be connected
through the basic cells presented in Figs 2.15 and 2.16. As mentioned earlier,
sources and loads of the same type can only be connected through an intermediate
coupling circuit. For example, to connect a voltage source to a voltage-type load,
it is necessary to employ a current-type element (inductor) between the source
and load [see Fig. 2.17(c)]. For duality, the voltage-type element is a capacitor
that is used to connect both current source and current-type load, as shown in
Fig. 2.17(d).
The basic cells permit the basic converters used to convert energy from
dc-to-dc, dc-to-ac, ac-to-dc, and ac-to-ac (or simply dc–dc, dc–ac, ac–dc, and
ac–ac) and also to extend them to more complex structures, in a more systematic
way. This will be in fact the approach employed in this book.
Depending of the application, it is possible to define two scenarios: (i) one
load supplied by one or more sources and (ii) one source supplying one or more
loads. Consider first the case in which there is only one load supplied from one or
more sources. Each source can be connected to either a switch (corresponding to the
point M in Fig. 2.15, for example), as shown in Fig. 2.18(a)–2.18(d), or to the pole
(midpoint of the leg, i.e., point A), as shown in Fig. 2.18(e) and 2.18(f). Similarly, for
the second scenario, when there is only one source and the load is constituted by one
or more elements, each part of the load can be connected to either a switch (point M,
for example), as shown in Fig. 2.19(g) or to the midpoint of the leg (A), as shown in
Fig. 2.18(h) and 2.18(i).
Notice from Figs 2.15–2.18 that the power switches, sources, and loads are
represented generically. The procedure to choose first the appropriate power switch
and the converter with desirable characteristics depends on the type of source and
load that have been considered, as well as the requirements for a specific application.
28 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
(a) (b) (c)
(d) (e) (f)
(g) (h) (i)
Figure 2.18 Different ways to connect source(s) to the load(s).
The following technical characteristics are used for choosing the appropriate switch
and converter: (i) UniC or BidC, (ii) UniV or BidV, (iii) SC or CC, and (iv) SB or CB.
Other essential features are switching frequency, voltage and current ratings, and cost.
2.4.1 dc–dc Conversion
Buck Converter The buck converter is presented in Fig. 2.19(a), which comprises
(i) a dc voltage source (Vdc), (ii) a basic cell as in Fig. 2.15(a) with switches S1 and
S2, (iii) energy storage component (L) due to the interface between two voltage-type
elements, and (iv) a resistive load with voltage Vo. As demanded for this application,
both switches S1 and S2 should be (a) UniC and UniV and (b) CC and CB. However,
notice that S2 must be complementary to S1 to avoid a short circuit of the dc source
(Vdc), which means that when S1 is on, S2 should be off, and when S2 is on, S1 should
be off.
2.4 BASIC CONVERTERS 29
(a) (b)
(c) (d)
(e)
S2
Vdc
+
–
Vo
+
–
S1 L
C
Vdc
+
–
Vo
+
–
C
off
on
L
iL
Vdc
νD
Toff
Ton
t
Vdc
+
–
Vo
+
–
C
off
on
L
iL
Vdc
+
–
Vo
+
–
Q L iL
C
D
Figure 2.19 Buck converter with: (a) basic cell and (b) real switches. (c) TS 1. (d) TS 2. (e)
Diode voltage.
This means that the circuit will have the same functionality if a SC/SB type
of switch (i.e., diode) is employed for S2. Then, the circuit will be as shown in
Fig. 2.19(b).
There are two topological states (TSs) for the buck converter:
TS 1—The switch Q is on and conducts the inductor current, while the diode
is off, as shown in Fig. 2.19(c).
TS 2—When Q is turned off, the diode conducts the inductor current, as shown
in Fig. 2.19(d).
Example 2.1
Explain why a buck converter such as the one presented in Fig. 2.19 requires
two power switches with UniC and UniV characteristics.
Solution
As the output voltage is dc, the load current is also dc, which leads to a dc
current for IL. During the TS 1, the switch Q will carry this unidirectional
type of current (UniC) and during the TS 2 the diode will carry IL. When both
30 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
switches are turned off their current will be zero. In terms of the voltage applied
to those devices, it is also UniV, as the voltage will be either zero or Vdc for Q
and either zero or −Vdc for D.
Figure 2.19(e) shows the diode voltage, which is the voltage applied to the LC
filter. While the time domain representation—as in Fig. 2.19(e)—provides a good
understanding of the topology itself, the frequency domain with the Fourier series
allows identification of the frequency components. In general terms, the expansion
of a periodical waveform f(t) in Fourier series is given by
f(t) = Fo +
∞
∑
n=1
fn(t) =
1
2
ao +
∞
∑
n=1
{an cos(n𝜔t) + bn sin(n𝜔t)} (2.1)
where Fo = 1∕2(ao) is the average value and
an =
1
𝜋 ∫
2𝜋
0
f(t) cos(n𝜔t)d(𝜔t) for n = 0, … , ∞ (2.2)
bn =
1
𝜋 ∫
2𝜋
0
f(t) sin(n𝜔t)d(𝜔t) for n = 1, … , ∞ (2.3)
In the case of Fig. 2.19(e), the average value Fo in (2.1) is given by
Vo =
TonVdc
Ts
= dVdc with d = Ton∕Ts (2.4)
where Ton is the interval of time with the switch S1 on, Ts is the switching period
(Ton + Toff), and d is known as duty cycle.
Notice that the input voltage of the LC filter has infinite components of fre-
quency [see equation (2.1)], which must be filtered allowing, ideally, an output volt-
age Vo with only the zero frequency component, as in equation (2.4).
Example 2.2
Assume the inductor voltage waveform and the information that this energy
storage component is in fact a passive element to deduce equation (2.4) without
the expansion in Fourier series.
Solution
The graphs below show the inductor waveforms (voltage and current) assum-
ing a continuous conduction mode (i.e., iL is always higher than zero). As the
inductor is a passive component, the average power on this device is zero, lead-
ing to an average voltage also equal to zero. It turns out that:(Vdc − Vo)Ton =
VoToff and consequently: Vo∕Vdc = Ton∕T = d.
2.4 BASIC CONVERTERS 31
t
t
iL
ILmax
–Vo
νL
Ton Toff
Vdc–Vo
ILmin
IL
Exercise 2.2
By using equations (2.2) and (2.3) calculate the Fourier coefficients an and bn
from 0 to the seventh harmonic for two waveforms of the diode voltage with
buck converter operating with d = 0.5 and 0.75. Also, consider a switching
frequency equal to 50 kHz. If the LC filter in Fig. 2.19 is designed with a cut
frequency equal to 20 kHz (3dB), find out if this filter can cut the switching
frequency of the buck converter for both cases: d = 0.5 and 0.75?
Boost Converter The boost converter with the representation of the real semi-
conductor devices is presented in Fig. 2.20(a). Its TSs are given in Fig. 2.20(b) and
2.20(c).
TS 1—In this mode, the switch is on and the diode is off. The input voltage
is then applied to the inductor with a consequent increase in its current iL.
Since D is off, the load current is provided by the capacitor C.
TS 2—This mode starts when the switch is turned off and consequently the
diode is on. At this moment, the energy stored at the magnetic field of the
inductor is released to the capacitor and load.
The average output voltage of the boost converter is given by
Vo =
Vdc
(1 − d)
(2.5)
32 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
(a)
(b) (c)
Vdc
+
–
Vo
+
–
C
Q
L D
iL
Vdc
+
–
Vo
+
–
C
on
L off
iL
Vdc
+
–
Vo
+
–
C
on
L
off
iL
Figure 2.20 Boost converter and its topological states.
The characteristics of the boost converter are the following:
1. Its output average voltage value is greater than the input voltage source.
2. Its input current is continuous with a ripple that depends on the value of the
input inductance and switching frequency.
3. The output voltage is positive.
Exercise 2.3
A boost converter as in Fig. 2.20 aims to obtain a dc output voltage of 120 V
from a voltage source with 24 V. The resistive load is 120 Ω, switching fre-
quency is equal to 50 kHz and the converter operates at continuous conduction
mode (iL > 0). Determine: (a) duty cycle d, (b) average load current, (c) aver-
age source current, and (d) inductor value to guarantee a current ripple less
than 5%.
Other Basic dc–dc Converters In addition to the buck and boost converters pre-
sented previously, there are four other basic nonisolated dc–dc converters that can
control the output voltage, as shown in Fig. 2.21. The absolute value of their average
output voltage is given by
Vo =
dVdc
(1 − d)
(2.6)
For all of the topologies in Fig. 2.21, the average of the output voltage can be
either smaller or greater than that of the voltage source, depending on the value of d.
The main characteristics of the configurations presented in Fig. 2.21 are presented in
the sequence.
2.4 BASIC CONVERTERS 33
(a) (b)
(c) (d)
Vdc
+
–
Vo
+
–
Vdc
+
–
Vo
+
–
Vdc
+
–
Vo
+
–
Vdc
+
–
Vo
+
–
Figure 2.21 Four basic dc–dc converters: (a) buck-boost, (b) cuk, (c) zeta, and (d) SEPIC.
(i) Buck-Boost Converter. This converter is shown in Fig. 2.21(a) and can connect
a voltage source to a voltage type load. The characteristics of the buck-boost
converter are the following:
1. Both input current and the current iD are discontinuous.
2. The output voltage is negative.
(ii) Cuk Converter. This converter is shown in Fig. 2.21(b) and can connect a cur-
rent source to a current-type load. The characteristics of the Cuk converter are
the following:
1. Both input current and output current are continuous.
2. The output voltage is negative.
(iii) Zeta Converter. This converter is shown in Fig. 2.21(c) and can connect a volt-
age source to a current-type load. The characteristics of the Zeta converter are
the following.
1. The input current is discontinuous and the output current is continuous.
2. The output voltage is positive.
(iv) Single-Ended Primary-Inductor Converter (SEPIC) Converter. The SEPIC
converter is based on the scheme of Fig. 2.21(d) and can connect a current
source to a voltage type load. The characteristics of the Zeta converter are the
following:
1. The input current is continuous and the current iD is discontinuous;
2. The output voltage is positive.
2.4.2 dc–ac Conversion
The circuits that permit a conversion from dc to ac are also known as inverters.
They can be voltage-source inverters (VSIs), current-source inverters (CSIs)
and impedance-source inverters (ZSIs). The fundamental concepts and main
34 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
νo
io
+Vdc/2
–Vdc/2
q1 q2
d1 d1
t
d2
Vdc
2
R L
a
+
–
νo
io
Vdc
2
q2
q1 d1
d2
0
(a) (b)
Figure 2.22 (a) Half-bridge inverter and (b) its output voltage and current waveforms for
d = 0.5.
characteristics of the VSI and CSI are given in the sequence, while the ZSI is
considered in Chapter 8 (Section 8.6.2).
Voltage Source Inverter (VSI) The simplest way to generate an ac voltage from a
dc source is with the arrangement as in Fig. 2.18(b) with the load connected between
the basic cell and two sources. Figure 2.22 shows the same converter with the repre-
sentation of real switches.
Half-Bridge When the switch q1 is on, the voltage source +Vdc∕2 is applied
to the load. The load current then increases exponentially. When q1 is turned off (q2 is
on), the current is obliged to decrease via diode d2, and a negative voltage is applied
to the load. A similar operation but related to d1 and q1 starts when q2 is turned
off. When d = Ton∕Ts = 0.5, a square wave is generated at the inverter output. The
output voltage is depicted in Fig. 2.22(b) along with the load current. The expansion
in Fourier series of the output voltage is given by
𝑣a0 =
4
𝜋
Vdc
2
[
sin (𝜔t) +
1
3
sin(3𝜔t) +
1
5
sin(5𝜔t) +
1
7
sin(7𝜔t) + …
]
(2.7)
Equation (2.7) allows calculating the amplitude of the output fundamental volt-
age as well as the existing odd harmonics.
The sinusoidal variation of the duty cycle d inside the switching interval Ts
allows shifting the harmonics to the high frequency region. The order of the most
significant ones is around the frequency modulation index, defined as
mf =
fs
fm
(2.8)
where fs is the frequency of the carrier signal that defines the switching frequency
(e.g., triangular waveform) and fm is the frequency of the modulating signal (e.g.,
sinusoidal signal).
This technique is known as sinusoidal pulse-width modulation (SPWM). Its
implementation is achieved by comparing a sinusoidal (modulating signal) with a
2.4 BASIC CONVERTERS 35
+Vt νt
νa0
0
+Va0
*
+Vdc/2
–Vdc/2
+Va0(1)
Va0(1) fundamental of νa0
–Va0(1)
Va0
*
–Vt
–Va0
*
Figure 2.23 Sinusoidal modulation: reference (top) and pole voltage waveform (bottom).
triangle waveform (carrier signal), the frequency of the modulating signal being the
fundamental one and the carrier frequency defining the switching frequency. The
main waveforms of the SPWM are presented in Fig. 2.23 (top), while Fig. 2.23 (bot-
tom) shows the waveforms for the output voltage.
The relationship between the amplitude of modulating signal, V∗
a0
, and that of
the carrier signal, Vt, defines the amplitude modulation index, ma, that is
ma =
V∗
a0
Vt
(2.9)
For the sinusoidal modulation (SPWM), the amplitude of the fundamental volt-
age is given by
Va0(1) =
V∗
a0
Vt
Vdc
2
= ma
Vdc
2
(2.10)
This means that the amplitude of the fundamental is directly proportional to the
amplitude modulation index (ma) for a given dc bus value (Vdc).
Example 2.3
For a half-bridge inverter as presented in Fig. 2.22(a) supplying a resistive
load of 5Ω, switching frequency of 10 kHz and Vdc = 100 V (duty cycle equal
to 50%), calculate: (a) the RMS of the output voltage assuming all harmonic
frequencies, (b) the RMS of the output voltage at the fundamental frequency,
and (c) output power as well as voltage and current processed by each
switch.
36 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
Solution
(a) By definition, the RMS value of a periodic function f(t) with period T is
given by
fRMS =
√
1
T ∫
T
0
[f(t)]2dt
Applying this equation for the waveform of the voltage presented in
Fig. 2.22(b), gives an output RMS voltage equal to
VoRMS = 50 V
(b) As observed in equation (2.7), the fundamental component of the output
voltage is given by𝑣ao1 = 2Vdc∕𝜋(sin(𝜔t)), consequently the RMS value
of the fundamental voltage will be given by Vo1RMS = 2Vdc∕𝜋
√
2 =
45.15 V.
(c) The output power is given by Po = V2
oRMS
∕R = 500 W. The blocking volt-
age and current processed by each switch is given by 100 V and 20 A,
respectively.
Exercise 2.4
Repeat the last example with a converter operating with a switching frequency
equal to 20 kHz and a RL load with R = 5Ω and L = 15 mH.
Full-Bridge The circuit of the single-phase full-bridge inverter is given in
Fig. 2.24(a). The output voltage can be written as a function of the pole voltages, as
𝑣ab = 𝑣a0 − 𝑣b0 (2.11)
The main waveforms of the converter are shown in Fig. 2.24(b). In this case the
pole voltages 𝑣a0 and 𝑣b0 are phase-shifted by180 electrical degrees.
As in the half-bridge with duty cycle equal to 50%, the output voltage includes
odd harmonics components, that is, third, fifth, seventh, and so on, as d = 0.5.
When the pole voltages are phase-shifted of 𝜃 degrees, as shown in Fig. 2.25(a),
four of the eight modes of operation are given in Fig. 2.25(b)–2.25(e). In Mode 1,
switches q1 and q2 conduct the increasing positive load current (t0 < t < t1), then q2
is turned off forcing q1 to conduct the load current along with d3 in a free-wheeling
mode (Mode 2, t1 < t < t2) until q1 is turned off (t2). From this moment on, Mode
3 starts with d3 and d4 conducting together; the load voltage becomes negative and
the load current is then forced to zero (t2 < t < t3). The zero crossing determines
the beginning of Mode 4, in which the current increases in the negative direction.
2.4 BASIC CONVERTERS 37
io
q1 q3
q2
d2
d3
d1
d4
q4
0 νo
Vdc
2 R L
a
b
Vdc
2
+
–
q1
d1 d1
q4
d4
q2
d2 d2
q3
d3
νa0
νb0
νo io
+Vdc/2
+Vdc/2
+Vdc
–Vdc
t
t
t
–Vdc/2
–Vdc/2
(a) (b)
Figure 2.24 (a) Single-phase full-bridge inverter. (b) Main waveforms.
(b) (c)
(a)
(d) (e)
q1 q1 0 a
b
R L
q3
q2
t0 t1 t2 t3 t4 t5 t6
t
q2
d2 d2
d3
d1
d1
θ
d4
q4
νo
io
+Vdc
–Vdc
νo
io
+
–
Vdc
2
q1
q2
Vdc
2
0 a
b
R L
νo
io
+
–
Vdc
2
d3
d4
Vdc
2
0 a
b
R L
νo
io
+
–
Vdc
2
q1
d3
Vdc
2
0 a
b
R L
νo
io
+
–
Vdc
2
q3
q4
Vdc
2
Figure 2.25 Single-phase full-bridge inverter. (a) Gating signals and main waveforms. (b)
Mode 1. (c) Mode 2. (d) Mode 3. (e) Mode 4.
When q4 is turned off, q3 starts conducting with d1, and so on, until the cycle is
completed.
The strategy of adding the phase-shift angle 𝜃 modifies the amplitude of the
fundamental and harmonics of the load voltage, which is given in equation (2.12)
38 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
0.1
0 20 40 60 80 100 120 140 160 180
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1.0
νab(1,n)
4Vdc
π
νab(3,n)
4Vdc
π νab(5,n)
4Vdc
π
νab(7,n)
4Vdc
π
Figure 2.26 Behavior of
the fundamental and
harmonics of the output
voltage as a function of 𝛾.
as a function of 𝛾 = 𝜋 − 𝜃. Figure 2.26 depicts the behavior of the fundamental and
harmonics components of the load voltage as a function of 𝛾. It can be observed that
for 𝛾 = 120∘ the amplitude of the third harmonic is zero, although the 5th, 7th, 11th,
13th harmonics are still present.
Vo(n) =
4Vdc
n𝜋
sin
(n𝛾
2
)
(2.12)
Another way to reduce the low frequency harmonic components for the out-
put voltage is to apply a PWM strategy for the gating signals, as previously done
for the half-bridge converter. There are different ways to generate the PWM signals
for the full-bridge converter, such as: (i) bipolar modulation—when the sinusoidal
references for pole 1 and pole 2 are in phase, (ii) unipolar modulation—when the
sinusoidal reference voltages are phase-shifted by 180∘, and (iii) a third possibility
is to operate one of the legs with PWM signal while the other one is operated at the
fundamental frequency; this corresponds to the unipolar modulation with clamped
voltage. Details about the PWM for the full-bridge converter are furnished in Chapters
5 and 8.
Three-Phase Inverter A dc–ac three-phase converter is shown in Fig. 2.27.
The gating signal generation for the power switches can be obtained as done pre-
viously by either changing 𝛾 to eliminate specific harmonics components or with a
PWM approach, which will push the harmonics to higher frequencies components.
First, assuming the pole voltages with phase-shift equal to 120∘ from each other, the
2.4 BASIC CONVERTERS 39
Vdc
Vdc
2
0
Vdc
2
a
b
c
Figure 2.27 Three-phase
inverter.
line-to-line voltages can be calculated as
𝑣ab = 𝑣a0 − 𝑣b0
𝑣bc = 𝑣b0 − 𝑣c0 (2.13)
𝑣ca = 𝑣c0 − 𝑣a0
As the load is Y-connected, it turns out that
𝑣an =
1
3
(2𝑣a0 − 𝑣b0 − 𝑣c0)
𝑣bn =
1
3
(2𝑣b0 − 𝑣c0 − 𝑣a0)
(2.14)
𝑣cn =
1
3
(2𝑣c0 − 𝑣a0 − 𝑣b0)
Also, it can be shown that the relationship between the load neutral and the
midpoint of the dc bus for a balanced three-phase system is given by
𝑣n0 =
1
3
(𝑣a0 + 𝑣b0 + 𝑣c0) (2.15)
The corresponding waveforms for equations (2.13)–(2.15) are shown in
Fig. 2.28.
As the line-to-line voltage in Fig. 2.28(b) was obtained with 𝛾 = 120∘, then
neither third harmonic nor its multiples are measured in these voltages. This is an
important characteristic for three-phase systems, as the natural phase angle displace-
ment among the phases (120∘) allows elimination of harmonics.
It can be seen from Fig. 2.28 that there are six modes of operation. These modes
are highlighted in Fig. 2.29(a)–2.29(f). In addition to these six modes of operation,
there are two other modes of operation that apply zero voltage to the loads. These
are the free-wheeling configurations presented in Fig. 2.29(g) and 2.29(h), where
three bottom or upper switches conduct at the same time. Note that for simplifica-
tion purposes the operation modes of the three-phase circuit are presented with ideal
switch.
40 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
νa0
νab
νan
νb0
νc0
+Vdc/2
–Vdc/2
+Vdc/2
+2/3Vdc
+1/3Vdc
–1/3Vdc
(c)
(b)
(a)
(d)
t
t
t
t
t
t
+1/6Vdc
–1/6Vdc
–2/3Vdc
–Vdc/2
+Vdc/2
+Vdc
–Vdc
–Vdc/2
Figure 2.28 Waveforms of
three-phase inverter. (a) Pole
voltages; (b) line-to-line
voltage; (c) load phase voltage;
and (d) zero-sequence voltage.
Another way to eliminate harmonics for the output voltage is to generate a
SPWM signal for the gating of the switches, as presented in Fig. 2.30, which shows
three reference signals phase-shifted by 120∘ compared to a carrier signal. This figure
shows also the pole voltages as a result of the sine-triangular comparison.
Example 2.4
Draw the waveforms of the pole voltages (𝑣a0, 𝑣b0, and 𝑣c0), line-to-line volt-
age (𝑣ab), and load phase voltage (𝑣an) considering a SPWM strategy applied
2.4 BASIC CONVERTERS 41
to dc–ac three-phase converter with the switching frequency and modulating
frequency equal to 10 kHz and 60 Hz, respectively. Also prove that ma → ∞.
Solution
As the amplitude modulation index (ma) is infinite, from equation (2.9) it
means that the amplitude of the modulating signal is infinitely higher than the
amplitude of the carrier signal, which leads to a pole voltage and load voltages
as presented in Fig. 2.28.
(a) (b)
(c) (d)
(e) (f)
(g) (h)
Vdc
+
–
Vdc
+
–
Vdc
+
–
Vdc
+
–
Vdc
+
–
Vdc
+
–
Vdc
+
–
Vdc
+
–
Figure 2.29 Modes of operation
of the three-phase inverter.
42 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
νt νa0
∗
νa0
νb0
νc0
νb0
∗ νc0
∗
Figure 2.30 Three-phase
inverter waveforms with
PWM approach.
Exercise 2.5
The three-phase inverter in Fig. 2.27 (Vdc = 300 V) is operated with a sinu-
soidal PWM approach with a modulation index ma = 0.9. The ratio between
the frequency of the carrier and modulating signals (mf ) is high enough to
guarantee sinusoidal load currents when the three-phase load is constituted by
R = 5 Ω and L = 20 mH (per phase). The frequency of the modulating signal
is 50 Hz.
(a) What is the RMS value of the voltage 𝑣a0 at the fundamental frequency?
(b) What is the RMS value of the voltage 𝑣ab at the fundamental frequency?
(c) What is the RMS value of the current in each phase?
(d) CSI
The three-phase version of the CSI is shown in Fig. 2.31. As the current source
is unidirectional, the switches are of UniC type. However, due to the bidirectional
load voltage type, the switches must be of BidV type. In fact, the CSI is dual to the
VSI. Because of this, the line-to-line output voltage waveform of a VSI is equiva-
lent to the line output current waveform of a CSI. Using this knowledge, the CSI
can be controlled by the same PWM techniques used to control the VSI. However,
practical aspects such as dead-time generation follows different rules for both types
of converters.
2.4 BASIC CONVERTERS 43
a
b
c
Figure 2.31 Current source
inverter (CSI).
2.4.3 ac–dc Conversion
Ac–dc converters are also known as rectifiers. Such converters can be sorted as
uncontrolled or controlled rectifiers. An overview about this type of converter is pre-
sented here.
Uncontrolled Rectifiers Notice that a sinusoidal waveform as those obtained on
the utility grid has average voltage equal to zero. Some applications, such as dc motor
drive systems, require a waveform with average voltage different from zero.
If a resistive load is employed, the simplest way to satisfy the condition of
non-null average voltage is to use a power converter able to cut, for instance, the
negative part of the sinusoidal waveform, as presented schematically in Fig. 2.32(a).
A power switch series connected between the source and load will implement this
rectifier circuit with no need to use the basic cells as in Figs 2.15 and 2.16. It is
evident that the output voltage and output current are unidirectional, which leads to
a device with the following characteristics SC/SB/UniC/UniV-r, that is, diode. There
are two TSs defined by the variables of the circuit as there is no gating signal control.
The TSs are shown in Fig. 2.32(b).
However, for an RL type of load [see Fig. 2.33(a)] the sinusoidal input volt-
age obliges the current to become zero somewhere between 𝜔t = 𝜋 and 𝜔t = 3𝜋∕2
(a) (b)
νac
+
–
νo
+
+
– –
Figure 2.32 Single-phase half-bridge diode rectifier with resistive load: (a) circuit; (b)
operation modes.
44 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
(a) (b)
νac
+
–
νo
i
+
–
Figure 2.33 Single-phase half-bridge diode rectifier with inductive load: (a) circuit; (b)
operation modes.
(depending of the load power factor), thus turning off the diode. During the diode con-
duction after 𝜔t = 𝜋, the negative input voltage is applied to the load. Even dealing
with negative voltage, the diode will turn off only when both conditions are satisfied:
reverse voltage and zero current [see section “The Conventional Diode”]. In this case,
the average of the output voltage will vary with the load power factor, which is some-
times an undesirable condition. The output voltage varying with the power factor of
the load can be avoided by using a diode in parallel with the load (free-wheeling
diode), that, in fact, clamps the negative part of the load voltage at zero, as shown
in Fig. 2.34. The arrangement of two diodes as presented in this figure is indeed a
particular case of the basic cell shown in Fig. 2.15. In this case, the output voltage
will be equal to
Vo =
Vm
𝜋
(2.16)
where Vm is the amplitude of the sinusoidal waveform.
Example 2.5
Deduce equation (2.16).
Notice from Fig. 2.34 that due to the inductive load, the arrangement of diodes
is in fact a basic cell (as in Fig. 2.16) constituted by diodes.
While a single-phase full-bridge diode rectifier is presented in Fig. 2.35(a), the
three-phase version is presented in Fig. 2.35(b). Both circuits are also one of the cases
presented in Fig. 2.18 with higher output dc voltage than the half-bridge, as in Figs
2.32–2.34.
2.4 BASIC CONVERTERS 45
(a) (b)
νac
+
–
νo
+
–
Figure 2.34 Single-phase half-bridge diode rectifier with inductive load and free-wheeling
diode: (a) circuit; (b) operation modes.
(a) (b)
Figure 2.35 Diode rectifier: (a) single-phase and (b) three-phase circuits.
Controlled Rectifiers The controlled rectifiers can also be either half-bridge or
full-bridge topologies. Their control can be obtained either by phase control or by
PWM control, depending on the type of switch employed in the circuit.
Phase Control Considering a sinusoidal (bidirectional) voltage source
feeding a unidirectional inductive load, as shown in Fig. 2.36(a), the type of
switch for S1 and S2 can be given respectively by: CC/SB/UniC/BidV (SCR) and
SC/SB/UniC/UniV-r (diode), as in Fig. 2.36(b). The SCR is turned on at a given
angle 𝛼 in relation to the moment that the SCR voltage becomes positive on its
terminals. Unlike the previous rectifiers, the angle control allowed by the gating
circuit of the SCR permits varying the output average voltage by changing 𝛼. This
technique is known as phase control.
46 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
(a) (b)
νac
+
–
νac
+
–
νo
+
S2
D
T
S1
–
νo
+
–
Figure 2.36 (a) Controlled ac–dc converter using a switching cell. (b) Single-phase rectifier
with SCR.
The average of the output voltage (Vo𝛼), as a function of both 𝛼 and the ampli-
tude of the sinusoidal voltage, is given by
Vo𝛼 =
Vm
2𝜋
(1 + cos 𝛼) (2.17)
It can be seen from equation (2.17) that when 𝛼 = 0∘, the value of the output
voltage is the same as in equation (2.16), as the SCR is equivalent to the diode when
𝛼 = 0.
Exercise 2.6
Deduce the expression for the average of the output voltage as in
equation (2.17) of the controlled rectifier as presented in Fig. 2.36.
The single split-phase half-bridge rectifier is shown in Fig. 2.37(a), in which
the sinusoidal voltage sources 𝑣ac1 and 𝑣ac2 are phase-shifted 180o to each other, as
shown in Fig. 2.37(b). Suppose that the load current is continuous (i.e., always above
zero) and that the SCR T1 is turned on at a given angle 𝛼 after 𝑣ac1 becomes positive.
This voltage is then applied to the load. From 𝜔t = 𝜋, 𝑣ac1 becomes negative while
𝑣ac2 becomes positive allowing T2 to be turned on when 𝜔t = 𝜋 + 𝛼. Until this time
the load current is furnished by 𝑣ac1, as shown in Fig. 2.37(c). From 𝜔t = 𝜋 + 𝛼 on,
𝑣ac2 feeds the load current, as shown in Fig. 2.37(d).
Note that when a free-wheeling diode is added as in Fig. 2.38(a), the negative
part of the output waveform is clamped to zero as in Fig. 2.38(b) and the output
average voltage is calculated from equation (2.17).
The three-phase and six-phase half-bridge rectifiers are shown in Figs 2.39 and
2.40, respectively. In the results presented in Figs 2.39(b) and 2.40(b) their output
voltages are obtained for 𝛼 = 30∘. The general expression for the average output
voltage for a n-phase half-bridge rectifier considering 𝛼 = 0∘ is given by (2.18).
2.4 BASIC CONVERTERS 47
(a) (b)
(c) (d)
νac
+
–
νac
+
+
+
–
–
–
νac
+
–
νo
io
νo
νg2
νg1
νac1,νac2
νac1
νac2
+
+
–
–
νac1
νac2
io
+
–
νo
+
–
νo
+
–
T2
T1
T1
T2
Figure 2.37 Single split-phase rectifier: (a) power circuit, (b) waveforms, and (c) and (d)
modes of operation.
Vo =
nVm
𝜋
sin
(
𝜋
n
)
(2.18)
Examples of the full-bridge rectifiers for single-phase and three-phase circuits
are presented in Fig. 2.41(a) and 2.41(b), respectively. The output voltage wave-
form of the full-bridge single-phase bridge is similar to that of the single split-phase
half-bridge rectifier. The output voltage waveform of the three-phase bridge is similar
to that of the six-phase half-bridge.
PWM Control A three-phase PWM converter with bidirectional power flow
capability, sinusoidal grid current, and power factor control is presented in Fig. 2.42.
Each phase can employ the boost principle so that the output voltage is higher than
the amplitude of the input voltage. This topology is discussed in detail in Chapter 9.
48 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
(a) (b)
νac
+
–
νo
νo
νac1,νac2
+
–
T1
D
T2
Figure 2.38 Single split-phase rectifier with a free-wheeling diode: (a) power circuit and (b)
main waveforms.
(a) (b)
νo
νa
νb
νc
+
–
νa νb νc
– t
Figure 2.39 (a) Three-phase half-bridge controlled rectifier and (b) output waveform.
(a)
(b)
νo
+
–
νa νb νc
t Figure 2.40 (a) Six-phase
half-bridge controlled
rectifier and (b) output
waveform.
2.4 BASIC CONVERTERS 49
(a) (b)
Figure 2.41 Full-bridge controlled:
(a) single-phase and (b) three-phase
rectifiers.
Figure 2.42 Three-phase
controlled rectifier.
2.4.4 ac–dc Conversion
An example of a simple ac–ac converter is presented in Fig. 2.43(a), where the switch
is a TRIAC (or two SRCs in antiparallel), for a resistive load. By varying the switch
turn-on angle 𝛼, the RMS value of the fundamental component of the output voltage
is varied as well. During the positive semicycle of the input voltage, when turned
on, the TRIAC conducts from M1 to M2 and during the negative semicycle of the
input voltage, when turned on, it conducts from M2 to M1. The voltages are shown in
Fig. 2.43(b). The need for a device of BidV type is confirmed from the waveform of
the voltage across the device. The RMS of the output voltage is given by
Vo𝛼 =
Vm
√
2
√
1
𝜋
(
𝜋 − 𝛼 +
sin 2𝛼
2
)
(2.19)
The circuit shown in Fig. 2.44(a) is a single-phase ac–ac converter, referred to
as a cycloconverter. The switches must be of the type CC/SB and BidV/UniC as in
this figure. The positive (P) and negative (N) converters are controlled to achieve an
output voltage with variable amplitude and a variable frequency, as in Fig. 2.44(b).
Another ac–ac converter is the matrix converter, which consists of an array of
bidirectional switches that directly connect the load to the source. The three-phase
to three-phase conversion is given in Fig. 2.45(a) with ideal switches. The practical
realization of the matrix converter is presented in Fig. 2.45(b).
50 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
(a) (b)
νo
νo
νac
νac
M1 M2
Figure 2.43 Simple ac–ac
converter: (a) circuit and
(b) phase control.
P N
(a) (b)
N N N N N N
P P P P P P
Figure 2.44 (a) Single-phase cycloconverter. (b) Waveforms of the circuit: (top) grid
voltage and (bottom) load voltage with dashed line.
The back-to-back converter is another way to generate a controlled ac voltage
from the utility grid voltage. Such a converter is also known as indirect ac–dc–ac
conversion, as there is a dc link between both ac stages, as in Fig. 2.46. This converter
is described in detail in Chapters 10 and 11. The ac–dc–ac converter can also be
implemented with a current source configuration.
2.5 SUMMARY
This chapter first classified the static (unidirectional or bidirectional features in
terms of current and voltage) and dynamic (spontaneous or controlled turn-on and/or
turn-off) characteristics of the ideal power switches. Then a summary of the main
2.5 SUMMARY 51
(a)
a
b
c
a
b
c
A B C
A
B
C
(b)
Figure 2.45 (a) Three-phase switching matrix. (b) Practical implementation of the matrix
converter.
Figure 2.46 Indirect converter: ac–dc–ac conversion.
real power semiconductor devices available in the market was given, taking into
account the static and dynamic characteristics. It was outlined their limit values for
current, voltage, and switching frequency. The bedrock for the following chapters
was given by introducing the concept of basic switching cell, from which it is pos-
sible to generate the basic converter topologies used in power electronics. By using
these switching cells, a general discussion on the principles of power conversion
52 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS
from dc sources (dc–dc and dc–ac conversion) and ac sources (ac–dc and ac–ac)
is furnished. Also the principle of operation of the main converter topologies is
explained. It is expected from this chapter to provide the reader a systematic way of
deciding which type of power semiconductor is the most appropriate choice for a
given application based on: (i) the static and dynamic characteristic, (ii) voltage and
current ratings, and (iii) on the frequency of operation. In addition to the generation
of conventional power electronics topologies, the concept of cell can be applied
to conceive other topologies used by researchers and by related industry. These
other topologies, named in this book as advanced power electronics converters,
are introduced in the following chapters. Details on the topics can be found from
References 1 to 77. As will be presented from Chapter 3 onwards, this text will focus
on advanced power electronics converters that process AC voltage by using PWM
strategies as the gating signal control of the power switches.
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1972.
[2] Burns WB III, Kociecki J. Power electronics in the minicomputer industry. Proc IEEE
1988;76(4):311–324.
[3] Hower PL. Power semiconductor devices: an overview. Proc IEEE 1988;76(4):335–342.
[4] Baliga BJ. Evolution of MOS-bipolar power semiconductor technology. Proc IEEE 1988;76(4):
409–418.
[5] Chen DY. Power semiconductors: fast, tough, and compact. IEEE Spect 1987;24.
[6] Thomson-C.S.F. Le transistor de puissance dans son environement. Paris: Thomson-CSF-DSD, 1978.
[7] Ferrieux JP, Forest F, Lienart P. The insulated gate bipolar transistor: switching modes. Proceedings
of European Power Electronics Conference; 1969. p 171–175.
[8] Heumann K, Papp G, Jung M. Comparative study on new power transistors with respect to high
frequency inverter applications. Ibid; 1989. p 99–104.
[9] Muraoka K, Kawamura Y, Ohtsubo Y, Sugawara S, Tamamushi T, Nishizawa J. Characteristics of
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CHAPTER 3
POWER ELECTRONICS
CONVERTERS PROCESSING
ac VOLTAGE AND POWER
BLOCKS GEOMETRY
3.1 INTRODUCTION
This chapter provides a brief review of the main power electronics converters that pro-
cess ac voltage and an introduction to power blocks geometry (PBG), to understand
the power converters described later in this book. In fact, this chapter has a compi-
lation of the topologies studied throughout this book. The fundamentals of PBG and
its correlation to the development of power electronics converters are presented in a
general way; details regarding each converter are presented in the following chapters.
This approach is called geometry because it deals with interconnection of geometric
shapes following specifics axioms and conjectures.
The main goal of the PBG is to provide an alternative and systematic approach
for the presentation of the power converters used to process ac voltage. This strategy
employs formal methods based on a simple geometrical representation with estab-
lished rules. A universe with axioms and conjectures is defined in order to establish
a formation law. Through this method, which is called PBG, power electronics con-
figurations observed in the technical literature, especially the traditional ones, can be
obtained by following the proposed rules with a high level of abstraction. The PBG
method is a general approach that can be employed for the creation and develop-
ment of dc–ac and ac–dc–ac converters from two levels to n levels. It is demon-
strated that different types of converters processing ac voltage can be easily built by
using PBG.
The converters studied in this book have at least one stage that synthesizes
ac voltage (𝑣o), as observed in Fig. 3.1(a). This kind of converter should be able to
create ac waveforms from a dc voltage, with at least two levels, as in Fig. 3.1(b).
Figure 3.1(c) shows a pulse width modulation (PWM) waveform for the output con-
verter, also with two levels, but with reduced harmonic distortion compared to that in
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
56
3.1 INTRODUCTION 57
(a)
(b)
Pulsed-
voltage
source
PWM
PBG LEG
Model
Table of
Variables
(d)
(c)
t t
Converter
processing
ac voltage
νo
νo
νo
Figure 3.1 (a) Power converter able to synthesize ac voltage. (b) ac Output voltage with two
levels. (c) PWM ac output voltage with two levels. (d) Approach employed to determine the
pulsed voltage source.
Fig. 3.1(b). The focus of this book is topologies dealing with PWM voltages with two
or more levels obtained from a dc stage. Indeed, the block in Fig. 3.1(a) that processes
a PWM ac voltage can also be referred to as a pulsed voltage source. Figure 3.1(d), in
turn, shows the approach employed throughout this book to obtain the pulsed voltage
sources systematically. First, the PBG is considered to define what a single leg looks
like (LEG in Fig. 3.1(d) – circuit constituted by a set of switches able to generate
a waveform with two or more levels). Then the table of variables will be employed
to define both the model of the converter and the PWM strategy. Such a leg can be
defined from the PBG, considering different figures of merit, for example, number of
levels, quantity of semiconductors and passive elements desired.
This chapter is organized as follows: Section 3.2 introduces the concept of
PBG with the concepts, axioms, and postulates defining a systematic way to present
power electronics converters; Section 3.3 describes each power block (PB) used in
the PBG; Sections 3.4 and 3.5 describe the application of the PBG for multilevel and
58 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
back-to-back configurations, respectively. Finally, Section 3.6 summarizes the entire
chapter.
3.2 PRINCIPLES OF POWER BLOCKS
GEOMETRY (PBG)
By definition, engineering is the application of science to practical uses, and one of the
most important approaches employed in engineering is the act of abstracting, that is,
simplifying a complex system in a simple statement or simple equation. An example
of abstraction is in analog and digital electronics where
OpAmp and Inverter Logic symbols are considered abstract elements that
describe the behavior of electrical variables. There is a high level of abstraction from
the physical elements to the symbols. Such a level of abstraction is crucial to the
development of important devices such as computers and satellites, as the designer
can focus on the functionality of each element (high level consideration) instead of,
for instance, either the interactions of atoms or operation of internal transistors (low
level consideration).
Also, the presentation of power electronics converters can involve some level
of abstraction, with the power switches (e.g., insulated-gate-bipolar transistor (IGBT)
and metal oxide semiconductor field-effect-transistors (MOSFETs)) being consid-
ered as a simple and ideal (loss-free) two-state switch, on (1) or off (0). In this sense,
the goal of the PBG is to bring a higher level of abstraction to the concept of convert-
ers by furnishing a set of concepts, axioms, and postulates, as presented in the rest of
this chapter.
Propositions, as considered in general statements of geometry relationships, are
basically divided into two types: (i) those assumed to be true, and (ii) those proven
to be true. The former are called (in Euclid’s terminology) axioms if they deal with
quantities and postulates if they deal with geometrical figures, while the latter are
called theorems. In this way, to axiomatize a particular system is to show that its
influences can be defined by a short set of sentences. Hence, it is possible to use
some concepts, axioms, and postulates to define a formation law for many power
electronics converters that process ac voltage as follows.
Concepts
Concept 1. PB is a basic unit of the power electronics configurations. There are
six different PBs, which are able to represent a large number of topologies
by just changing their arrangement.
Concept 2. Shape is either a slot or tooth with triangular or square geome-
try. Each block is constituted by either three or four shapes. Triangular and
square shapes are used to represent specific types of variables, that is, dc or
ac. On the other hand, slot and tooth are employed in the PBG to bring up
the intuitive aspect of mechanical connection among blocks.
Concept 3. PB–dc (PB which processes dc variables) is a PB with at least
one triangular shape. If a PB presents one or more triangular shapes, it is
considered a unit that processes dc voltage.
3.2 PRINCIPLES OF POWER BLOCKS GEOMETRY (PBG) 59
Concept 4. PB–ac (PB which processes ac variables) is a PB without any tri-
angular shape. If a PB presents only square shapes, it is considered a unit
that processes ac voltage.
Axioms
Axiom 1. Every PB is constituted of at least three shapes.
Axiom 2. Every mechanical connection between PBs is an electrical connection.
Axiom 3. A dashed line denotes ac variable and a solid line denotes dc variable.
Postulates
Postulate 1. A triangular shape connects only with another triangular shape.
Postulate 2. A square shape connects only with another square shape.
Postulate 3. The triangular shape is associated with dc variables.
Postulate 4. The square shapes could be associated with either dc or ac
variables.
Regarding these concepts, the axioms and postulates described above, it is pos-
sible to construct a large number of configurations proposed in the technical literature
that process ac voltage.
Normally, power switches are considered the basic elements or cells for
construction of power electronics converters. Figure 3.2 shows different topologies
conceived for different applications, but with the same number of controlled power
switches (i.e., four power switches).
While Fig. 3.2(a) depicts an H-bridge configuration, Fig. 3.2(b) and 3.2(c) show
a leg for the three-level NPC and flying capacitor topologies, respectively; finally
Fig. 3.2(d) shows an ac–dc–ac single-phase half-bridge (at both sides) configura-
tion. It is worth mentioning that the configurations in Fig. 3.2 also process ac voltage
(a) (b) (c) (d)
Figure 3.2 Configurations employing four controlled switches: (a) H-bridge, (b) three-level
NPC, (c) three-level flying capacitor, and (d) ac–dc–ac single-phase half-bridge.
60 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
(a) (b) (c)
(d) (e)
Figure 3.3 Configurations employing
six controlled switches: (a) three-phase
inverter, (b) four-level NPC, (c)
four-level flying capacitor, (d) ac–dc–ac
single-phase shared leg, and (e) nested
configuration.
through a dc stage and have the same number of switches. The conventional way to
present power converters with the switches as basic cells assumes the configurations
in Fig. 3.2 as distinct categories. As a consequence, students are unable to under-
stand how those configurations were created. A similar situation can be observed in
Fig. 3.3.
Also, in this figure, an isolated presentation hides the understanding of creation
of the topologies. In this case the configurations have six controlled power switches
and Fig. 3.3(e) shows a different type of topology (as compared to those presented in
Fig. 3.2) named nested converter.
To overcome such a difficulty, the conception of topologies by using the prin-
ciples of the PBG brings up a systematic presentation with a simple and familiar
concept of connecting blocks. Such an approach guarantees a formal outline needed
for a generalized and didactic presentation. It is worth emphasizing that with PBG it
is possible to create a large number of topologies from two- to n-level, just following
simple rules. The PBs used in the PBG is shown in Fig. 3.4. Figure 3.4(a) and 3.4(b)
shows three PB-dc and three PB-ac, respectively. See Concepts 3 and 4.
Each PB constitutes a set of power switches, which guarantees specific char-
acteristics for the blocks. Figure 3.5 shows what is obtained inside each PB. Dur-
ing the process of creation of the configurations the PBs are considered in their
3.2 PRINCIPLES OF POWER BLOCKS GEOMETRY (PBG) 61
(a) (b)
Figure 3.4 Basic units (power blocks – PB) used in the power blocks geometry (PBG):
(a) PB-dc and (b) PB-ac.
(a) (b)
(c) (d)
(e) (f)
Figure 3.5 Basic units
(power blocks – PBs) used
in the power blocks
geometry (PBG): (a) first
PB-dc, (b) second PB-dc, (c)
third PB-dc, (d) first PB-ac,
(e) second PB-ac, and (f)
third PB-ac.
62 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
(a) (b)
(c) (d)
Figure 3.6 Configurations in
Fig. 3.2 obtained from the PBs.
higher level (i.e., with strong abstraction from the details inside the blocks). The
connections among the PBs, considering the postulates mentioned previously, will
be employed for construction of the classical and nonconventional configurations, as
considered in the next sections. In fact, the topologies showed in Figs 3.2 and 3.3 are
obtained from the PBs following the rules presented in Section 3.2, as observed in
Fig. 3.6.
3.3 DESCRIPTION OF POWER BLOCKS
The first PB-dc [see Fig. 3.5(a)] is constituted only by diodes, which means that there
is no generation of gating signals.
On the other hand, there is at least one controlled power switch inside all other
PBs, which requires some understanding. Figure 3.7 shows the variables associated
with the second PB-dc, as well as the table with their related variables, called Table
of Variables. In this table, q is the state of the controlled switch (q = 1 means closed
switch, while q = 0 means open switch), 𝑣o, Vp, and Vn are the output voltage,
3.3 DESCRIPTION OF POWER BLOCKS 63
q
q
Vp
Vp
Vn
Vn
νo
io
νo
νo
io
(a) (b)
row q
1 1
2 1
3 0
4 0
> 0
< 0
> 0
< 0
Vp
Vp
Vp
Vn
Figure 3.7 Variables associated with the
second PB-dc and Table of Variables.
positive terminal of the input voltage, and negative terminal of the input voltage,
respectively.
In principle, considering Postulate 4, it is possible to generate an ac output
voltage, since a square tooth is observed at the output of this block. Since the desir-
able scenario indicates that the output voltage could be defined by the switching
state independent of the load current, there is no full control associated with the first
PB-dc.
Hence, taking into account the possibilities shown in the Table of Variables (see
Fig. 3.7), some restrictions related to the controllability of the output voltage (𝑣o) are
observed. When the output current is negative (rows 2 and 4) the output voltage is
always Vp, independent of q, which means that there is no control of the output voltage
in this case (i.e., io < 0). Then, considering the PB-dc operating alone, as depicted in
Fig. 3.7, the full controlled cell is obtained only when io > 0. Equation (3.1) describes
the behavior of the output voltage for the second PB-dc when io > 0.
𝑣o = qVp + (1 − q)Vn (3.1)
A similar restriction is observed in the third PB-dc, when io > 0, which means
that the full controlled output voltage is obtained when io < 0, as observed in Fig. 3.8.
In this case it turns out that
𝑣o = qVn + (1 − q)Vp (3.2)
Although such current restriction observed in Figs 3.7 and 3.8 can prohibit the
application of those blocks to process ac voltage, their associations will guarantee the
use of these blocks to generate multilevel circuits able to process ac voltage.
64 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
q q
Vp
Vp
Vn
Vn
νo
io
νo
νo
io
(a) (b)
row q
1 1
2 1
3 0
4 0
> 0
< 0
> 0
< 0
Vn
Vn
Vp
Vn
Figure 3.8 Variables associated with
the third PB-dc and Table of Variables.
q
q q
Vp
Vp
Vn
Vn
νo
io
νo
νo
io
(a) (b)
row q
1 1
2 1
3 0
4 0
> 0
< 0
> 0
< 0
Vp
Vp
Vn
Vn
Figure 3.9 Variables associated with
the first PB-ac and Table of Variables.
On the other hand, the current restriction does not appear in the PBs that process
ac voltage (PB-ac). Figure 3.9 shows the variables associated with the first PB-ac, as
well as its Table of Variables. Since there are two controlled switches, there is no
restriction in terms of the controllability of the output voltage, even in the case of
3.3 DESCRIPTION OF POWER BLOCKS 65
q2
q1
q1
q1
q2
Vp
Vp
Vn
Vn
νo
io
νo
νo
io
(a) (b)
row q1
1 0
2 0
3 0
4
5
6
7
8
0
1
1
1
1
q2
0
0
0
0
0
0
1
1
0
0
1
1
> 0
> 0
> 0
> 0
< 0
< 0
< 0
< 0
Vn – Vp
Vn – Vp
Vp – Vn
Vp – Vn
q2
Figure 3.10 Variables associated with
the first PB-ac and Table of Variables.
positive and negative currents. In this case, equation (3.1) is valid for any value of
io, and q is complementary to q (i.e., q = 1 − q) to avoid a short-circuit between Vp
and Vn. The second PB-ac [see Fig. 3.5(e)] is in fact a particular case of the first
instance with the ability to control positive and negative currents due to the antiseries
connection of the switches.
The third PB-ac [see Fig. 3.5(f)] has four controlled switches q1 and q2 and
their complementary switches q1 and q2. Like the first PB-ac, the output voltage is
a function of only the state of switches (q1 and q2). But unlike the case in Fig. 3.9,
Fig. 3.10 shows that the output voltage has three different values, or three levels (Vn −
Vp, 0, Vp − Vn), and in this case the output voltage is given by
𝑣o = (q1 − q2)Vp + (q2 − q1)Vn (3.3)
The process of building power electronics converters processing ac voltage
by using the PBG does not take into account the switching states, just the geom-
etry of the blocks and the connections among them, which make possible the
process of topologies creation. The Table of Variables presented in Figs 3.7–3.10
and equations (3.1)–(3.3) will be employed for the generation of the PWM
waveforms, discussed in the following chapters. The next section of this chapter
will deal only with the creation of the configurations by using the axioms and
postulates.
66 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
Example 3.1
Assume a dc motor drive system requires a converter with controlled voltage at
the output converter side and demanding positive currents only. (a) Choose one
of the PBs with minimum components able to deal with these requirements.
(b) If the motor average current is given by Io = 50A and the dc-link voltage
is given by Vpn = 200V (with Vpn = Vp − Vn) specify the switches employed
in this converter in terms of voltage and current values.
Solution
(a) Since the output has a positive dc current and there is a need for a
controlled output voltage, the PB with fewer components will be the
first PB-dc [i.e., configuration constituted by a controlled switch q and a
diode – see Fig. 3.7(a)].
(b) Considering the operation of this PB: (1) when q = 1 the output current (Io)
will be going through the controlled switch, the diode current will be zero,
the controlled switch voltage will be zero and the reserve diode voltage
will be Vpn; (2) when q = 0 the output current (Io) will be going through
the diode, the controlled switch current will be zero, the controlled switch
voltage will be Vpn and the diode voltage will be zero. The specification of
the voltage and current for both devices (controlled switch and diode) are
200 V and 50 A.
Example 3.2
A battery formation apparatus is constituted by circuits that aim to generate a
specific voltage waveform in order to guarantee the charge and discharge pro-
cess until the battery is considered formed. Sometimes the discharge process is
obtained by burning the stored energy with resistors (i.e., inefficient process).
To overcome this problem, it is possible to employ power electronics solutions
to charge and discharge the battery by sending energy back to the primary
source of energy with higher efficiency, as observed below. Choose one of the
PBs with minimum components that can deal with these requirements.
Primary
source of
energy
Power
electronics
converter
Vp
IBat
IBat
VBat
Battery
under
formation
Vpn Vo
+
–
+
–
Vn
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 67
Solution
The power electronics converter for this particular application must generate
controlled output voltage either for positive or negative current, which means
that both PB-ac (half-bridge or H-bridge configurations) could be used.
3.4 APPLICATION OF PBG IN MULTILEVEL
CONFIGURATIONS
Multilevel converters were first conceived for high voltage and high power appli-
cations, beginning with the neutral-point-clamped (NPC) inverter. Since that time,
many configurations have been proposed to establish the highly desirable character-
istics for high power applications such as low blocking voltage by switching devices
and reduced waveform distortion. The number of levels can be increased as far as
necessary, limited by both the complexity of the control and the price of the con-
verter itself, due to the increased number of semiconductor devices. To figure out
the advantages of waveforms with increased number of levels, Fig. 3.11 shows the
total harmonic distortion (THD) versus modulation index (or amplitude-modulation
ratio) for two-, three-, and four-level waveforms. As defined in the previous chapter,
Two-level
Three-level
Four-level
1.0
0.9
0.8
0.7
m (modulation index)
0.6
0.5
0.4
0.3
0.2
THD
(total
harmonic
distortion)
Figure 3.11 THD versus modulation index for voltages with two, three, and four levels.
68 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
(a) (b) (c)
Figure 3.12 Output converter voltage with two-, three-, and four-level.
the modulation index (ma) is a relationship between the amplitude of the sinusoidal
waveform (also called modulating or control voltage – Vm) and triangular waveform
(also called carrier voltage – Vt), that is, ma = Vm∕Vt. It can be seen from Fig. 3.11
that the increase in the number of levels results in THD reduction for a given value
of ma. Figure 3.12 depicts the waveforms produced by converters with two-, three-
and four-levels, respectively. From this figure it is easy to understand the behavior
shown in Fig. 3.11 with better THD for a higher number of levels – notice that the
waveforms in Fig. 3.12 become closer to a sinusoidal voltage.
The most employed multilevel configurations, with industry interest, are
diode-clamped (or NPC), cascade, and flying capacitor multilevel inverters. Those
multilevel configurations will be considered throughout this book as the conven-
tional ones, while different multilevel topologies presented in the technical literature
will be treated as nonconventional solutions. The nonconventional converters are
important in power electronics basically because they may provide an alternative
solution to improve a specific aspect of the conversion system. Furthermore, such
nontraditional power electronics converters play an important role in teaching
students due to the extra effort required in modeling and dealing with specific
requirements.
3.4.1 Neutral-Point-Clamped Configuration
Considering the PBG, the constructions of the NPC configurations can be presented
in a systematic way, as described briefly in this subsection. Chapter 4, however, will
provide details of this configuration. With two PBs-dc cells [see Fig. 3.5(b) and 3.5(c)]
and the first PB-ac cell [see Fig. 3.5(d)], and connecting them following the Postulates
1 and 2 presented previously, it is possible to generate the three-level NPC configu-
ration, as observed in Fig. 3.13(a). This is a three-level converter because the blocks
(and consequently the switches) are connected in such a way that one of the three
inputs can be selected to appear at the output converter side.
Other levels can be obtained following the same strategy, that is, connecting
a triangular slot (or tooth) with a triangular tooth (or slot) (i.e., following Postulate
1); and connecting a square slot (or tooth) to a square tooth (or slot) (i.e., following
Postulate 2).
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 69
(a)
(b)
(c)
1
2
3
1
2
3
4
5
1
2
6
7
3
4
5
Figure 3.13 Construction of NPC multilevel legs using PBs: (a) three-levels, (b) four-levels,
and (c) five-levels.
From the four-level NPC configuration onward there are always two or more
possibilities of connections among the triangle slots and teeth. For instance, consid-
ering the configuration in Fig. 3.13(b), the triangle slot of PB 1 is connected to the
triangle tooth of PB 4, while the slot of PB 3 is connected to the tooth of PB 2. There
are other ways to connect the blocks differently from that shown in Fig. 3.13. These
different ways and the PWM approach are considered in Chapter 4.
70 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
Example 3.3
Write the Table of Variables for the three-level NPC configuration; see
Fig. 3.13(a). Prove that the switching devices can be represented by a binary
variable, with qj = 1 used when the switch is on and qj = 0 when the switch
is off (with j = 1, 2, 3, and 4), as highlighted below.
Vn
Vp
q1 = {0,1}
q2 = {0,1}
νo
q3 = {0,1}
q4 = {0,1}
Solution
Since there are four switches with two states each, there are sixteen (22 = 16)
possibilities for the total switching states, as shown below:
row q1 q2 q3 q4 𝑣o
1 0 0 0 0 Undefined
2 0 0 0 1 Undefined
3 0 0 1 0 Undefined
4 0 0 1 1 Vn
5 0 1 0 0 Undefined
6 0 1 0 1 Undefined
7 0 1 1 0 0
8 0 1 1 1 Short-circuit
9 1 0 0 0 Undefined
10 1 0 0 1 Undefined
11 1 0 1 0 Undefined
12 1 0 1 1 0
13 1 1 0 0 Vp
14 1 1 0 1 Vp
15 1 1 1 0 Short-circuit
16 1 1 1 1 Short-circuit
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 71
Notice that many of the states obtained in this Table are prohibited since
they are either undefined or short-circuit, and so must be avoided. In this
context, undefined means that the output voltage is not defined exclusively by
the switching states. Without taking into account the prohibited states, this
converter can generate three different voltages at its output (i.e., Vn, 0, Vp) for
either positive or negative currents.
Example 3.4
Many of the switching states in Example 3.3 cannot be applied since they are
prohibited states. Since there are only three inputs and those inputs should be
selected to appear at the output converter side (𝑣o), determine: (a) the mini-
mum number of independent switching states to select any input voltage at the
output converter side (b) how those switching states can be associated with the
converter in Fig. 3.13(a) with four switches to generate a three-level output
voltage.
Solution
(a) As there are three inputs and the requirement is to use the switching states
to select each of these inputs at the output, the minimum number of inde-
pendent switching states is 2, since 22 = 4.
(b) As observed in Fig. 3.13(a), the three-level NPC topology requires four
switches to guarantee an output with three levels. On the other hand, with
two independent switching states (as concluded previously) it is possible to
select three inputs available (Vn, 0, Vp), defining the complementary switch-
ing states as q1 and q2, where q1 = 1 − q1 and q2 = 1 − q2. Below is pre-
sented the three-level NPC topology, using only two independent switches,
as well as its Table of Variables. The converter as presented below is able to
select any input by using two independent switches.
Vp
Vn
q1
q2
νo
q2
q1
72 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
State q1 q2 𝑣o
1 0 0 Vn
2 0 1 0
3 1 0 Undefined
4 1 1 Vp
3.4.2 Cascade Configuration
As the number of levels increases, the practical control limits observed in the NPC
multilevel converter restrict its use, due to capacitor voltage control issues. Such oper-
ation limits are presented in Chapter 4. Another topology that deals with generation
of multilevel voltages without dramatically increasing the control complexity is the
cascade configuration, since it normally uses isolated dc sources. A high power motor
drive system with high level reliability is one of the applications where this kind of
converter is popular.
The construction of the cascade multilevel configurations are observed in
Fig. 3.14, with the direct use of the third PB-ac (see Fig. 3.5) following Postulate 2
with the connection of the teeth in a series arrangement. Dashed lines at the output
of these converters mean that they will deal with ac variables, while solid lines at the
input side of the converter mean dc variables. Details of the cascade configuration
are furnished in Chapter 5.
Example 3.5
For the converter presented below [as in Fig. 3.14(a)], write the Table of Vari-
ables for the case in which the dc-link voltage of the converters are given by
Vdc1 = Vdc and Vdc2 = 2Vdc and then determine how many levels will be gen-
erated at the output converter side with qj = 1 − qj and j = 1, 2, 3, 4.
Vdc1
Vdc2
q1 q2
q3 q4
νo
q1 q2
q3 q4
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 73
(a)
(b)
Figure 3.14 Construction of cascade multilevel legs using PBs with: (a) two power blocks
and (b) three power blocks.
74 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
Solution
The Table of Variables for this converter is presented below. The output voltage
will have seven levels given by 0, ±Vdc, ±2Vdc and ±3Vdc.
row q1 q2 q3 q4 𝑣o
1 0 0 0 0 0
2 0 0 0 1 2Vdc
3 0 0 1 0 −2Vdc
4 0 0 1 1 0
5 0 1 0 0 Vdc
6 0 1 0 1 3Vdc
7 0 1 1 0 −Vdc
8 0 1 1 1 Vdc
9 1 0 0 0 −Vdc
10 1 0 0 1 Vdc
11 1 0 1 0 −3Vdc
12 1 0 1 1 −Vdc
13 1 1 0 0 0
14 1 1 0 1 2Vdc
15 1 1 1 0 −2Vdc
16 1 1 1 1 0
Example 3.6
Considering two cells of the first PB-ac, as presented in Fig. 3.5(d) and Pos-
tulates 2 and 4, draw a different configuration from the ones presented so far
with three inputs and one output and write the possible output voltages.
Solution
The postulates applied for two cells of the first PB-ac as presented in Fig. 3.5(d)
allow a possible solution as depicted below.
V1
V2
V3
νo
After the process of defining the topology, it is possible to write the out-
put voltages, taking into account the switches inside each block, as shown
below.
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 75
V1
V2
V3
q1
q2
q3
νo
q4
Here, the output voltages are given respectively by
• 𝑣o = V1 when q1 = q3 = 1 and q2 = q4 = 0
• 𝑣o = V2 when q2 = q3 = 1 and q1 = q4 = 0
• 𝑣o = V3 when q4 = 1 and q1 = q2 = q3 = 0
3.4.3 Flying Capacitor Configuration
There are some drawbacks associated with both multilevel topologies (NPC and cas-
cade) presented earlier. One of the disadvantages of the NPC topology is the need
to control dc-link capacitor voltages. On the other hand, an obvious drawback for a
cascade topology is the high number of dc voltage sources required.
The flying capacitor converter is another topology that can generate multilevel
voltages. Although needing additional flying capacitors (FCs), the capacitance values
are smaller than the dc-link capacitor and there are two switching states to control
the charging and discharging of FC. Unlike the NPC topology, in which just one
switching state is available to obtain zero voltage at the output converter side, the FC
converter has two states to generate zero voltage at the output.
In practical implementation of the NPC topology there is only one dc voltage
available; so two dc-link capacitors are normally used to guarantee three voltages
at the input converter side, as in Fig. 3.15(a). Figure 3.15(b) shows the Table of
Variables when two capacitors are used to generate three levels. For a symmetrical
three-level output voltage [as in Fig. 3.12(b)] each capacitor voltage should be
the same, for example, VC1 = VC2 = Vpn∕2. A control scheme should be added
to guarantee this requirement, but as shown in Fig. 3.15(b), there is a missing
switching state (State 3) q1 = 1 and q2 = 0, which reduces the degree of freedom
for controlling capacitor voltage. This problem is minimized for the capacitor
flying topologies since there are two switching states to generate zero voltage at the
output.
The PBG approach can also be employed to systematically obtain the flying
capacitor converters. For example, Fig. 3.16(a) brings up the three-level flying
76 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
(a)
State
1 0
q1 q2
0
2 0 1 0
3 1 0
4 1 1
(b)
q2
q1
Vpn
νo νo
–VC2
VC2
VC1
VC1
q2
q1
–
–
+
+
0
Figure 3.15 (a) NPC topology with a single dc voltage source and two dc-link capacitors.
(b) Table of Variables.
capacitor topology under PBs representation. The converters with four and five
levels are depicted in Fig. 3.16(b) and 3.16(c), respectively. Details about this circuit
are given in Chapter 6.
Example 3.7
Write the Table of Variables for the converter given below, which is based on
the three-level flying capacitor topology, with a dc voltage source instead of
flying capacitor. Prove also that the switching devices can be represented by a
binary variable, that is, qj = 1 is used when the switch is on and qj = 0 when
the switch is off (with j = 1, 2, 3, and 4).
Vdc
Vdc
Vdc
q1 = {0,1}
q2 = {0,1}
νo
q3 = {0,1}
0
q4 = {0,1}
Solution
Since there are four switches with two states each, there exist sixteen possibil-
ities for the total switching states, as shown below:
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 77
1
2
C C
1
3
2
C
C
4
1 2
3
C C
C
C C
C
C C
(a)
(b)
(c)
Figure 3.16 Construction of flying capacitor multilevel legs using PBs: (a) three-level, (b)
four-level, and (c) five-level.
78 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
row q1 q2 q3 q4 𝑣o
1 0 0 0 0 Undefined
2 0 0 0 1 Undefined
3 0 0 1 0 Undefined
4 0 0 1 1 −Vdc
5 0 1 0 0 Undefined
6 0 1 0 1 0
7 0 1 1 0 Short-circuit
8 0 1 1 1 Short-circuit
9 1 0 0 0 Undefined
10 1 0 0 1 Undefined
11 1 0 1 0 0
12 1 0 1 1 −Vdc
13 1 1 0 0 Vdc
14 1 1 0 1 Vdc
15 1 1 1 0 Short-circuit
16 1 1 1 1 Short-circuit
Notice that many of the states obtained in this table are prohibited,
that is, either undefined or short-circuit, and so must be avoided. Without
taking into account the prohibited states, this converter can generate three
different voltages at its output (i.e., −Vdc, 0, Vdc) for either positive or negative
currents.
Example 3.8
(a) Considering Example 3.7, what is the minimum number of independent
switching states that still allows three levels at the output converter side?
b) Draw the power converter with this minimum number of independent
switches to guarantee a three-level output voltage.
Solution
(a) If there are three input voltages and the requirement is to use the switching
states to select each input, the minimum number of independent switching
states is 2, since 22 = 4.
(b) As observed in Fig. 3.16(a), the three-level flying capacitor topology
requires four switches to guarantee an output with three levels. Moreover,
as shown earlier, with two independent switching states (q1 and q2) it
is possible to select the three inputs available (Vdc, 0, −Vdc), which ends
up with the definition of the complementary switching states q1 and q2
(q1 = 1 − q1 and q2 = 1 − q2). Below is presented the three-level flying
3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 79
capacitor configuration, using only two independent switching states and
the complementary switching states, as well as the Table of Variables.
Comparing this Table with that in Fig. 3.15, there is no prohibited state for
this topology, and this degree of freedom is used to control the voltage of
the flying capacitor.
Vdc
Vdc
Vdc
q1
q2
νo
0
q1
q2
State q1 q2 𝑣o
1 0 0 −Vdc
2 0 1 0
3 1 0 0
4 1 1 Vdc
3.4.4 Other Multilevel Configurations
Although the configuration obtained in Example 3.6 can generate an output voltage
with three levels, it is clearly a nonconventional topology, since it is not identified
as NPC, cascade, or flying capacitor converter. This section presents briefly some
nonconventional converters and Chapter 7 provides the necessary details.
Figure 3.17(a) shows a possible four-level topology by using the first and
second PBs-ac. Since this is a four-level converter, one of its counterparts is the
four-level NPC configuration shown in Fig. 3.13(b). Considering just the number of
semiconductor devices employed for both circuits, it favors the nonconventional one
in Fig. 3.17(a) due to the elimination of four diodes.
In addition to the drawbacks of the NPC converters mentioned earlier, such
topologies present unequal loss distribution among the semiconductor power devices.
The active NPC (ANPC) achieves a better loss distribution and wider semiconductor
devices utilization. ANPC configurations can also be presented following the PBG
approach (basically considering Postulates 2 and 4), as depicted in Fig. 3.17(b) for
three-level and in Fig. 3.17(c) for four-level output voltage.
Many of the nonconventional configurations proposed in the technical literature
can be obtained by following the axioms and postulates of the principles of the PBG,
as in Fig. 3.18.
80 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
V2
V1
V3
V4
V2
V1
V3
V4
νo
νo
V2
V1
V3
V2
V1
V3
νo
νo
V1
V1
V4
V4
V2
V2
V3
V3
V1
V4
V2
V3
νo νo νo
(a)
(b)
(c)
Figure 3.17 Construction of nonconventional converters. (a) Nested multilevel converter. (b)
Three-level ANPC multilevel legs using PB. (c) Four-level ANPC multilevel legs using PB.
3.5 APPLICATION OF PBG IN ac–dc–ac CONFIGURATIONS 81
(a)
(b)
(c)
Figure 3.18 Construction of multilevel legs using PBs.
3.5 APPLICATION OF PBG IN ac–dc–ac
CONFIGURATIONS
Another important class of configuration that processes ac voltage is the one with
two conversion stages, that is, with both rectification (ac–dc conversion) and
inversion (dc–ac conversion) stages connected through a dc-link capacitor link.
Such topologies are normally called ac–dc–ac configurations (or back-to-back
82 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
configurations) and are usually described as three-phase to three-phase (3ph–3ph),
single-phase to single-phase (1ph–1ph), and single-phase to three-phase (1ph–3ph)
conversions. Although each power conversion system (3ph–3ph, 1ph–1ph or
1ph–3ph) presents many possibilities of implementation in terms of the topology
structure employed, the ac–dc–ac configurations can be formulated considering the
principles of the PBG.
Many applications require this kind of converter: (i) three-phase motor drive
system with active power factor correction [see Fig. 3.19(a)], (ii) universal active
power filter with a combination of series and shunt active filters [see Fig. 3.19(b)],
and (iii) wind generation system [see Fig. 3.19(c)].
3.5.1 Three-Phase to Three-Phase Configurations
A three-phase back-to-back converter feeds a three-phase load from a three-phase
grid employing six legs (twelve switches) with one leg connected to each phase of
the system, as shown in Fig. 3.20(a). Considering the PBs and the geometry involving
them, the dashed line means that all input and output variables are of ac type, while
the solid line represents the dc variables of the dc-link voltage.
Some other topologies can be derived from the conventional one in Fig. 3.20(a),
especially when it is necessary to reduce the number of semiconductor devices. In
this way, both dc-link midpoint and shared-leg connections have been employed as
an approach to reduce the power switches. It means that at least one of the legs,
constituted by two power switches, is no longer used for the solutions presented in
Three-phase
utility grid
Three-phase
utility grid
ac–dc–ac three-phase to
three-phase converter
ac–dc–ac three-phase to
three-phase converter
Three-phase
ac motor
Induction
machine
Wind turbine
Gearbox
(a)
(c)
Three-phase
utility grid
ac–dc–ac three-phase to
three-phase converter
Non-linear
load
(b)
Figure 3.19 Applications of the ac–dc–ac three-phase to three-phase converter: (a) ac
motor drive system, (b) active power filter, and (c) double-fed induction generation system
used in wind turbines.
3.5 APPLICATION OF PBG IN ac–dc–ac CONFIGURATIONS 83
(a)
(b)
(c)
(d)
(e)
Figure 3.20 Three-phase to three-phase ac–dc–ac power conversion topology: (a) Direct
solution with six legs, (b) one shared leg, (c) one dc-link midpoint connection, (d) two
dc-link midpoint connections, and (e) shared-leg and dc-link midpoint connections.
84 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
Fig. 3.20(b)–3.20(e). However, regarding cost reduction, this approach make sense
if what is saved by the number of power semiconductor devices is not lost in higher
device ratings and higher values of electrolytic capacitor.
Figure 3.20(b) shows a solution with a shared leg between input-output con-
verter sides. Figure 3.20(c) presents a full-bridge configuration at the input side (left
side), and a half-bridge configuration at the output side (right side).
Although using the same number of power switches, the configuration in
Fig. 3.20(e) has advantages compared to that in Fig. 3.20(d). Notice from Fig. 3.20(e)
that one of the converter sides presents full-bridge characteristics (no connection
with the dc-link midpoint capacitors). On the other hand, in Fig. 3.20(d), both
converter sides are half-bridge. The topologies presented in Fig. 3.20 are discussed
in detail in Chapter 11.
Exercise 3.1
The common principle behind the topologies proposed in Fig. 3.20 is the inher-
ent redundancy of the three-phase systems. For a set of balanced three-phase
voltages, the relationship among the voltages is given by 𝑣1 + 𝑣2 + 𝑣3 = 0,
which means that if two voltages are defined, the third one will be indirectly
defined (they are linearly dependent). Considering the three-phase load con-
nected to a voltage source with only two phases [𝑣A = VAcos(𝜔t + ΦA) and
𝑣B = VBcos(𝜔t + ΦB)], as depicted below, define the amplitude of the volt-
ages (VA and VB) and the values of phases (ΦA and ΦB) to guarantee a balanced
three-phase load voltage given by 𝑣1 = V cos(𝜔t), 𝑣2 = V cos(𝜔t + 120), and
𝑣3 = V cos(𝜔t − 120).
ν1
VA
VB
ν2
ν3
+ –
–
– + –
+
+
+
–
In addition to reducing the number of power switches to reduce costs, it is also
possible to increase the number of semiconductor devices, as depicted in Fig. 3.21
paralleling back-to-back converters, to reduce the amount of power processed
by each conversion stage and improve the quality of the waveform generated by
converters.
3.6 SUMMARY 85
(a) (b)
Figure 3.21 Paralleling back-to-back converters: (a) PB representation and (b)
representation with switches.
3.5.2 Single-Phase to Single-Phase Configurations
As in the three-phase to three-phase ac–dc–ac configurations, it is possible to
establish a systematic presentation for generation of single-phase to single-phase
ac–dc–ac configurations, as in Fig. 3.22. Note that the approach of using shared-leg
and dc-link capacitor midpoint are still used to guarantee the component count
reduction. The single-phase back-to-back converters, including their model, PWM
strategy, and analysis are addressed in Chapter 10.
3.6 SUMMARY
This chapter shows that the proposed PBG strategy could be used to establish a sys-
tematic method for the presentation of many of the power electronics converters that
process ac voltage through a dc stage. A compilation of the main configurations was
done under the PBG point of view. Instead of considering power switches as the basic
elements in the process of converter construction, the PBs are employed as a higher
level component, with descriptions of the details inside the blocks. The connection
among the PBs, using the postulates and axioms, furnishes a simple and familiar con-
cept of geometrical blocks. Such a strategy was employed for construction of classical
and nonconventional configurations.
As a result of the PBG approach, different configurations are now presented as
a part of the same set of converters (i.e., topologies dealing with ac voltage with at
least one dc stage). Besides bringing a systematic presentation, the PBG technique
will play an important role in the process of topology construction. Even in the case
in which practical applications are not directly addressed for a specific configuration
obtained with PBG, this configuration still will be considered in this book since it
provides challenges in terms of converter understanding itself and creativity in devel-
oping its model and control strategies.
Each configuration presented in this chapter is deeply studied in the following
chapters, with the development of comprehensive model and PWM strategies. Further
details can be found in References from 1 to 21.
86 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING
(a)
(b)
(c)
(d)
(e)
Figure 3.22 Single-phase to single-phase ac–dc–ac power conversion topology: (a) Direct
solution with four legs, (b) one shared leg, (c) one dc-link midpoint connection, (d) two
dc-link midpoint connections, and (e) shared-leg and dc-link midpoint connections.
REFERENCES 87
REFERENCES
[1] Escaud B, Marty P. Introduction à l’étude des structures des convertisseurs statiques. Electron Ind
1983;56:65–71.
[2] Marty and Escaud B. La commutation dans les convertisseurs statiques, Ibid., No. 60; 1983. p 69–73.
[3] M. V. Miranda, A. M. N. Lima, Formal verification and controller redesign of power electronic con-
verters, Proc IEEE Int Symp Ind Electron, 2004. v. 1. p. 1–6.
[4] E. C. dos Santos Jr, E. R. C. da Silva. Power block geometry applied to the building of power elec-
tronics converters, IEEE Trans Educ, v. 2, pp. 191–198, 2013.
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of IECON’04; 2004. p 2290–2294.
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CHAPTER 4
NEUTRAL-POINT-CLAMPED
CONFIGURATION
4.1 INTRODUCTION
In this chapter, the neutral-point-clamped (NPC) configuration, also known as
diode-clamped configuration, is considered under the power blocks geometry (PBG)
point of view. The introduction and fundamental concepts of NPC configurations
from three-level to n-level, as well as a detailed description of these circuits,
including its model, pulse width modulation (PWM), and control strategies, are
addressed in this chapter.
The three-level NPC configuration is one of the most common topologies for
medium and high voltage applications, especially in motor drive systems, because
of reduced dv/dt, reduced total harmonic distortion (THD), and especially its ability
to deal with high voltage demand without connecting switches in series. However,
it is also possible to employ this kind of topology in lower power applications, as in
photovoltaic energy systems where other factors such as voltage with low distortion
and reduced leakage current are important factors.
This chapter is organized as follows: in Section 4.2 the three-level NPC
topology is once again obtained from the PBs and also treated in the level of power
switches. Its model is obtained by deducing an equation to describe the voltage
behavior at the ac side. Such an equation is achieved from the Table of Variables,
which also plays an important role in the PWM development. In Section 4.3 the
simplest PWM approach is detailed for the half-bridge single-phase three-level con-
verter. The concepts presented previously are expanded to full-bridge single-phase
and three-phase converters in Sections 4.4 and 4.5, respectively. Section 4.6 brings
up nonconventional converters demonstrating how those topologies can be easily
constructed by using PBG. The inherent problem of the unbalanced capacitor
voltages in NPC topologies is addressed in Section 4.7. NPC configurations with
number of levels higher than three are presented from Section 4.8–4.11. Section 4.12
provides a summary of the chapter.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
88
4.2 THREE-LEVEL CONFIGURATION 89
(a)
2
1
3
V1
V2
vo
V2
(b)
2
1
3
V1
vo
(c)
2
1
3
V2
vo
(d)
2
1
3
V3
vo
Figure 4.1 (a) Three-level (V1, V2, V3) NPC configuration with PBs. Activation of the PBs
to obtain the level: (b) 𝑣o = V1. (c) 𝑣o = V2. (d) 𝑣o = V3.
4.2 THREE-LEVEL CONFIGURATION
As already seen, the power blocks (PBs), can be connected following a systematic
approach to guarantee the creation of NPC multilevel configurations. The first
and direct arrangement of the blocks is repeated in Fig. 4.1(a), with triangular
shape connected to triangular shape and square shapes connected to each other.
Figure 4.1(b)–4.1(d) show the ways used to obtain each specific level (V1, V2, V3) at
the output converter side. Figure 4.1(b) illustrates that it is necessary to activate PBs
1 and 3 to obtain 𝑣o = V1, while 𝑣o = V3 is obtained when PBs 2 and 3 are activated
[see Fig. 4.1(d)]. On the other hand, the voltage V2 appears at the output side (𝑣o),
when just PB 3 is fully activated, as observed in Fig. 4.1(c). To generate an output
waveform with three levels, it is necessary to activate the PBs in a sequence as
observed in Fig. 4.2.
Since 𝑣o can assume just one input voltage V1, V2, or V3 at any time, it is pos-
sible to write an equation to describe the output voltage 𝑣o as a function of input
voltages and two independent binary variables (q1 and q2). Since there are three inputs
to be selected, the minimum number of binary variables employed to select those
inputs is two. These three inputs must appear at the output converter side through the
use of two binary variables, which means that one possible combination to achieve
this goal is given in Table 4.1.
Defining complementary variables (q1 and q2) as q1 = 1 − q1 and q2 = 1 − q2,
the output voltage can be defined as follows:
𝑣o = q1q2V3 + q1q2V2 + q1q2V1 (4.1)
Developing (4.1) we get
𝑣o = (1 − q1)(1 − q2)V3 + (1 − q1)q2V2 + q1q2V1 (4.2)
𝑣o = (1 − q2 − q1)V3 + q2V2 + q1q2(V3 − V2 + V1) (4.3)
90 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
1
2
1
2
3 3
V1
V1
V2
V3
t
V2
vo
vo
vo
1
2
3
V3
vo
Figure 4.2 Generation of a three-level output voltage for generic values of V1, V2 and V3.
TABLE 4.1 Table of Variables for the Converter
in Fig. 4.1(a)
State q1 q2 𝑣o
1 0 0 V3
2 0 1 V2
3 1 0
4 1 1 V1
Normally the waveform presented in Fig. 4.2 must be symmetrical, which
means that V1 = Vdc, V2 = 0 and V3 = − Vdc, and then it turns out that
𝑣o = (q1 + q2 − 1)Vdc (4.4)
It is worth mentioning that the binary variables considered in Table 4.1 are
related to the switching states inside the blocks in Fig. 4.1. Figure 4.3 shows the
same topology presented in Fig. 4.1 along with the binary variables describing the
state of the switches for both positive and negative output currents (io).
Notice that, unlike PB-dc operating alone (see Figs 3.7 and 3.8), the NPC
topology is able to generate the desired output voltage for both positive and nega-
tive currents, which means that each voltage value V1, V2, and V3 can be obtained
at the output converter side independent of the current values. In other words any
4.2 THREE-LEVEL CONFIGURATION 91
(a)
V1
V2
q1
q2
V3
io
q1
q2
(b)
V1
V2
q1
q2
V3
io
q1
q2
(c)
V1
V2
q1
q2
V3
io
q1
q2
Figure 4.3 Generation of levels: (a) V1, (b) V2, and (c) V3 independent of the output current.
desired output voltage is obtained for both cases io > 0 and io < 0, as observed in
Fig. 4.3.
Example 4.1
Considering the Tables of Variables presented below, place each switch (q1,
q2, q1, and q2) in the correct position in the circuit below to guarantee the
generation of the levels as demanded in the following tables.
State q1 q2 𝑣o State q1 q2 𝑣o
1 0 0 1 0 0
2 0 1 2 0 1
3 1 0 3 1 0
4 1 1 4 1 1
V1
V2
V3
Position 1
Position 2
Position 3
Position 4
vo
Solution
To guarantee an output voltage 𝑣o as demanded in the first Table of Variables,
the switches q1, q2, q1, and q2 should be placed, respectively, in the positions
3, 4, 1, and 2 as below. There is no possible combination for the second table.
92 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
State q1 q2 𝑣o State q1 q2 𝑣o
1 0 0 V1 1 0 0 V1
2 0 1 – 2 0 1 V2
3 1 0 V2 3 1 0 V3
4 1 1 V3 4 1 1 –
Example 4.2
Build the Table of Variables for the circuits presented below, with respect to
the position of each switch.
V1
V2
V3
q1
q2
q1
q2
vo
V1
V2
V3
q1
q2
q1
q2
vo
Solution
The Table of Variables for each circuit is given, respectively, by
State q1 q2 𝑣o State q1 q2 𝑣o
1 0 0 V3 1 0 0 V2
2 0 1 undefined 2 0 1 undefined
3 1 0 undefined 3 1 0 undefined
4 1 1 V3 4 1 1 undefined
Exercise 4.1
Considering the tables presented in Example 4.2, show through equivalent cir-
cuits and assuming positive and negative currents, why some of the states are
undefined.
4.3 PWM IMPLEMENTATION (HALF-BRIDGE TOPOLOGY) 93
Notice that for the two arrangements in Example 4.2 there are more than one
undefined states, which means that there is no way to obtain three levels at the output
converter side, as seen in Fig. 4.3. Such a characteristic is not desirable for a power
converter processing ac voltage.
4.3 PWM IMPLEMENTATION
(HALF-BRIDGE TOPOLOGY)
If the aim is to generate an ac voltage at the output converter side with both ampli-
tude and frequency controllable, a PWM strategy is applied to generate the switching
gating signals. From a converter processing ac voltage, ideally an output sinusoidal
voltage is expected. However, due to the characteristics of the NPC converter pre-
sented in Fig. 4.2, the number of levels is limited to three. Hence, the aim of the
PWM strategy is to guarantee that the three-level voltage at the output of the converter
emulates the desirable sinusoidal voltage. The average value of the square output
waveform must be equal to a sinusoidal reference (inside the switching period) as
presented in the figure below.
vl
∗
vl
∗
vl
∗
vl
vl
vl
Switching
frequency
Normally, the switching frequency is kept high (compared to the modulating
signal) to increase the accuracy of 𝑣l ≈ 𝑣∗
l
. In fact many works in the technical lit-
erature have proposed solutions in terms of modulation approaches applied for NPC
converters to improve different aspects of the converter. In this chapter, the simplest
way to generate the PWM waveforms is considered. However, an optimized PWM
approach is derived in Chapter 8.
Figure 4.4 shows a simple analog solution, in which the states of the four
switches are determined by a comparison among a sinusoidal waveform (𝑣∗
sin
) and
two high frequency triangular waveforms (𝑣∗
t1
and 𝑣∗
t2
). Such PWM can be expanded
for NPC converters with higher levels, which uses N − 1 (N is the number of levels)
triangular carrier signals with just one modulating signal. The sinusoidal waveform
is given by 𝑣∗
sin
= Vl sin(𝜔lt), where Vl is the amplitude and 𝜔l is the angular fre-
quency desired to the load. The block mentioned as driver must guarantee the levels
of voltage and current in the switch’s gate circuit needed to operate the power devices
adequately as well as guarantee galvanic isolation.
Notice from Fig. 4.4(c) and 4.4(d) that when the switches q1 and q1 are chang-
ing their states (during the positive half cycle of 𝑣∗
sin
), switch q2 is on and switch q2
94 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
driver
+
–
driver
q1
q2
q1
q2
vsin
*
vt1
*
1
0
1
0
1
0
0.2 0.225 0.25
–1
q1
q1
vsin
* vt1
*
0.2 0.225 0.25
1
0
1
0
1
0
–1
q1
q2
vsin
*
vt2
*
driver
+
–
driver
q1
q2
q1
q2
vsin
*
vt2
*
(a)
(b)
(c)
(d)
Figure 4.4 (a) PWM generation circuit for switches: (a) q1 and q1; and (b) q2 and q2.
(c) Variables associated with switches q1 and q1 (from top to bottom) – reference voltages,
gating signal of switch q1 and gating signal of switch q1. (d) Variables associated with
switches q2 and q2 (from top to bottom) reference voltages, gating signal of switch q2 and
gating signal of switch q2.
is consequently off for the entire half cycle, while in the negative half cycle of 𝑣∗
sin
,
when switches q2 and q2 are changing their states, switch q1 is off and switch q1
is on.
The modulation presented in Fig. 4.4 describes the states in Table 4.1, when q2
is on and q1 can be either off (State 2 in Table 4.1) or on (State 4 in Table 4.1). In the
same way, when q1 is off, q2 can be either off (State 4.1 in Table 4.1) or on (State 2
in Table 4.1). Also, this modulation approach avoids the undesired State 3.
Figure 4.5(a) shows the half-bridge three-level configuration, in which the
load is connected between the dc-link midpoint and the center point of the leg.
4.4 FULL-BRIDGE TOPOLOGIES 95
q2
q1
q1
q1
q2
Vdc
Vdc
R
+ –
L
q2
vo
vo
io
io
0
0
1
–1
1
0
200
50
–200
–50
0.2 0.225 0.25
1
(a)
(b)
Figure 4.5 (a) Three-level NPC half-bridge converter. (b) (from top to bottom) 𝑣∗
sin
, 𝑣∗
t1
, 𝑣∗
t2
;
gating signal of switch q1; gating signal of switch q2; load voltage and load current.
Figure 4.5(b) depicts (from top to bottom) PWM reference waveforms, gat-
ing signal of switches q1 and q2, load voltage, and load current, respectively.
The parameters employed in these simulation tests were: Vdc = 200 V, R = 5Ω
and L = 5mH, and switching frequency equal to 500Hz. For the sake of com-
parison, the same parameters are used for the other simulation results in this
chapter.
Sometimes in practical applications just one dc source is available, which
means that both dc sources shown in Fig. 4.5(a) are changed by capacitors connected
to a single dc source. In this sense, it is necessary to guarantee the control voltage
for both capacitors. This specific issue is considered later on in this chapter.
4.4 FULL-BRIDGE TOPOLOGIES
The three-level NPC topology with two legs, that forms a full-bridge single-phase
converter, can be obtained from PBG by connecting the PBs given in Fig. 4.1 appro-
priately, as seen in Fig. 4.6(a). Following this approach it is also possible to build
96 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
a
(a)
b
V2
V1
V3
1
2
3
a
(b)
b
c
V2
V1
V3
1
2
3
a
(c)
b
c
d
V2
V1
V3
1
2
3
Figure 4.6 NPC three-level topology with: (a) two legs (full-bridge single-phase load),
(b) three legs (three-phase load), and (c) four legs (three-phase four-wire load).
configurations with n legs. Figure 4.6(b) shows a three-level NPC topology with
three legs for applications demanding a three-phase system (e.g., three-phase motor
drive systems or three-phase rectifier converter), while Fig. 4.6(c) shows a three-level
NPC topology with four legs to be employed, for instance, in a three-phase four-wire
system. These three configurations in Fig. 4.6 are described in the following
sections.
Figure 4.7(a) presents the full-bridge single-phase converter [as in Fig. 4.6(a)]
highlighting the connections of the switches. It is worth mentioning that even though
the full-bridge topology in Fig. 4.7(a) is constituted by three-level legs, the output
voltage has five levels.
Figure 4.7(b) shows (from top to bottom) pole voltage (voltage between the
midpoint of the leg and the dc-link capacitor midpoint 𝑣a0) of the first leg with three
levels, pole voltage of the second (𝑣b0) also with three levels, load voltage, and load
current, respectively. Comparing Figs 4.5 and 4.7, it is evident that the increased
number of levels observed on the load voltage of the full-bridge topology guarantees
a ripple reduction on the load current for the full-bridge topology. In this case the
output voltage is given by
𝑣o = (q1a + q2a − q1b − q2b)Vdc (4.5)
The number of levels considered in this chapter for conventional topologies is
defined by the pole voltages. For instance, both converters in Figs 4.5 and 4.7 are
4.4 FULL-BRIDGE TOPOLOGIES 97
q2a
q1a
q2b
q1b
q1a
q2a
a
b
0
q1b
q2b
Vdc
Vdc
R
+ –
L
vo
va0
vb0
vo
io
io
200
–200
200
500
–500
100
–100
0.2 0.225 0.25
–200
(a)
(b)
Figure 4.7 (a) Three-level NPC full-bridge converter. (b) (from top to bottom) pole voltage
of the first leg (𝑣a0), pole voltage of the second (𝑣b0), load voltage and load current.
considered as single-phase three-level NPC topologies, although they present differ-
ent number of levels for the load voltages.
Example 4.3
Considering the topology presented in Fig. 4.7(a), find a solution for the PWM
generation circuit to guarantee the waveforms shown in Fig. 4.7(b).
Solution
A set with a reference sinusoidal and two triangular waveforms plus two
OpAmps for each leg (as seen in Fig. 4.4 for the half-bridge topology) can be
employed for the PWM signal generation for the full-bridge topology. Since
the control of both legs is independent, those sinusoidal waveforms should
have 180∘ of phase apart to guarantee a maximum output voltage.
98 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
Example 4.4
What happens if different phase displacements are employed for both reference
sinusoidal waveforms?
Solution
The figure below shows a phase or diagram representation for the pole voltages
𝑣a0 and 𝑣b0 (just for the sinusoidal components) as well as for the load voltage
𝑣o = 𝑣a0 − 𝑣b0. The output voltage is a function of the phase displacement of
the pole voltages, meaning that the maximum output voltages will be obtained
when this phase displacement angle is equal to 180∘.
180°
90° 0°
va0
va0
vb0
vl = va0 – vb0 vl = va0 – vb0
vl = 0
va0 = vb0
vb0
4.5 THREE-PHASE NPC CONVERTER
A three-phase three-level full-bridge NPC configuration is depicted in Fig. 4.8(a) by
employing switches. Notice that this circuit was easily obtained by just connecting
the PBs as seen in Fig. 4.6(b). Figure 4.8(b), in turn, shows some variables associated
with this converter, that is, (from top to bottom): pole voltage, voltage between the
load neutral point (NP) (n) and dc-link midpoint connection (0), load phase voltage,
and load current, respectively. The pole voltages can be written as follows:
𝑣a0 = (q1a + q2a − 1)Vdc (4.6)
𝑣b0 = (q1b + q2b − 1)Vdc (4.7)
𝑣c0 = (q1c + q2c − 1)Vdc (4.8)
The load phase voltages are given by
𝑣a = 𝑣a0 − 𝑣n0 (4.9)
𝑣b = 𝑣b0 − 𝑣n0 (4.10)
𝑣c = 𝑣c0 − 𝑣n0 (4.11)
Considering a balanced three-phase condition (𝑣a + 𝑣b + 𝑣c = 0), the voltage
between the NP of the three-phase load (n) and the dc-link midpoint can be defined
4.5 THREE-PHASE NPC CONVERTER 99
q2a
q1a
q2b
q1b
q2c
q1c
q1a
q2a
a
b
c
n
0
q1b
q2b
q1c
q2c
Vdc
Vdc
R L
R L
R L
va0
vn0
van
ia
ia
500
0
0
0
0
–500
500
500
–500
100
–100
0.2 0.225
(b)
(a)
0.25
–500
Figure 4.8 (a) Three-phase NPC converter. (b) (from top to bottom) pole voltage, voltage
𝑣n0, load voltage, and load current.
analytically by
𝑣n0 =
1
3
(𝑣a0 + 𝑣b0 + 𝑣c0) (4.12)
Substituting (4.10)–(4.12) into (4.13), we have
𝑣n0 =
Vdc
3
(q1a + q2a + q1b + q2b + q1c + q2c) − Vdc (4.13)
From (4.13), the voltage for each phase of the three-phase load can be written
as follows:
𝑣a =
(
2
3
q1a +
2
3
q2a −
1
3
q1b −
1
3
q2b −
1
3
q1c −
1
3
q2c
)
Vdc
(4.14)
𝑣b =
(
−
1
3
q1a −
1
3
q2a +
2
3
q1b +
2
3
q2b −
1
3
q1c −
1
3
q2c
)
Vdc
(4.15)
𝑣c =
(
−
1
3
q1a −
1
3
q2a −
1
3
q1b −
1
3
q2b +
2
3
q1c +
2
3
q2c
)
Vdc (4.16)
In the case of a balanced three-phase load, the load voltages depend only of the
state of the switches and of the dc-link voltage as considered in (4.15)–(4.17).
100 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
The control circuit for the three-phase converter can be obtained as seen in
Fig. 4.4. The difference is the number of modulating signals needed; in this case
there are three references: 𝑣∗
sin 1
= Vl sin(𝜔t), 𝑣∗
sin 2
= Vl sin(𝜔t + 120∘) and 𝑣∗
sin 3
=
Vl sin(𝜔t + 240∘), where Vl and 𝜔l are the desired peak voltage and frequency for the
load, respectively.
Exercise 4.2
Create a table relating all states of the switches (64 possibilities) to find the
number of levels for 𝑣n0 and the number of levels for the phase voltage 𝑣a for
the converter shown in Fig. 4.8.
Application (High Voltage Motor Drive System)
The three-phase NPC multilevel configuration can be employed in medium voltage
(MV) drives to reach a high voltage level without using switching devices in series
connection. The switching frequency for MV high power application is normally low
as compared to the two-level converter in order to reduce the power losses (it is
usually limited to a few hundred hertz) without compromising the quality of the wave-
forms generated due to the number of levels. Normally, special modulation tech-
niques are needed to produce the minimum harmonic distortion for the motor cur-
rent for a large range of speed and torque. The main applications are in pumps,
fans/exhausts, compressors, mixers, agitators, conveyors, cement mills, steel mills,
winders/unwinders, sugar mills, refiners, banburys, and extruders. The figure below
shows a common scheme with an NPC topology employed in MV drives.
Utility
grid
Switch gear Transformer
Mv inverter
MV induction
motor
M
3~
Y
Δ
Δ
4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 101
q2a
q1a
q2b
q1b
q2c
q1c
q1a
q2a
a
b
c
0
q1b
q2b
q1c
q2c
Vdc
Vdc
R
L
R
L
R
L
Figure 4.9 Three-level NPC converter supplying a three-phase load connected in Δ
arrangement.
Exercise 4.3
An MV three-phase motor has line-to-line and active power given, respectively,
by 2.3 kV and 150 kW (with power factor 0.85). Assuming that this motor will
be supplied by a three-leg NPC topology, determine the voltage and current
ratings of the switches for this configuration.
Figure 4.9 shows the NPC three-phase power converter topology supplying
a Δ- connected three-phase load. The main difference between Figs 4.9 and 4.8(a)
is related to the values of voltages and current demanded by the load, as well as
the number of levels measured on the load voltages. In this case (Δ-connected)
the load phase voltage has only five levels, as seen from the equations given
below:
𝑣a = (q1a + q2a − q1b − q2b)Vdc (4.17)
𝑣b = (q1b + q2b − q1c − q2c)Vdc (4.18)
𝑣c = (q1c + q2c − q1a − q2a)Vdc (4.19)
4.6 NONCONVENTIONAL ARRANGEMENTS BY
USING THREE-LEVEL LEGS
It is possible to combine the NPC leg with two-level legs already presented in this
chapter to establish a nonconventional single-phase multilevel converter, as seen in
Fig. 4.10. In this case, it is used four PBs with the output load connected between
blocks 3 and 4. Since the output of block 3 has three levels (V1, V2, and V3) and the
102 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
V1
V2
V3
2
1
3
4
vo
Figure 4.10 Five-level single-phase converter
obtained by the combination of NPC and
conventional legs – block representation.
TABLE 4.2 Table of Variables for the Converter in Fig. 4.10
State q1a q2a q1b Output of PB 3 Output of PB 4 𝑣o
1 0 0 0 − Vdc − Vdc 0
2 0 0 1 − Vdc Vdc − 2Vdc
3 0 1 0 0 − Vdc Vdc
4 0 1 1 0 Vdc − Vdc
5 1 1 0 Vdc − Vdc 2Vdc
6 1 1 1 Vdc Vdc 0
output of block 4 has two levels (V1 and V3), it leads to an output voltage with five
levels (0, V1 − V3, V2 − V1, V2 − V3, V3 − V1).
For a symmetrical output voltage generation, the input voltages should have the
following parameters: V1 = Vdc, V2 = 0, and V3 = − Vdc, meaning that the output volt-
age will be with the following values 0, ± Vdc, ± 2Vdc. For the converter in Fig. 4.10
it is necessary for three independent binary signals (q1a, q2a, and q1b) to synthesize
the desired output voltage since there are five levels. Table 4.2 shows the voltage 𝑣o
as a function of q1a, q2a, and q1b.
Equations to describe the pole voltages (𝑣a0 and 𝑣b0) and output voltage 𝑣o as a
function of the input voltages and as a function of three independent binary variables
(q1a, q2a, and q1b) are given below, respectively:
𝑣a0 = (q1a + q2a − 1)Vdc
(4.20)
𝑣b0 = (2q1b − 1)Vdc
(4.21)
𝑣o = (q1a + q2a − 2q1b)Vdc (4.22)
The binary variables considered in both Table 4.2 and in equation (4.22) are in
fact the switching states inside the blocks, which means that the topology presented
in Fig. 4.10 can be considered in its lower level representation (switches instead of
blocks), as in Fig. 4.11.
4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 103
q2a
q1a
q1b
q1a
q1b
q2a
a b
0
Vdc
Vdc
+ –
vo
io
Figure 4.11 Five-level
single-phase converter obtained by
the combination of NPC and
conventional legs with switches.
Exercise 4.4
Assuming all switching states given in Table 4.2, write a Table showing
the blocking voltages and current through the switches for the six switches
employed in Fig. 4.11.
It is also possible to generate a four-level topology with the same PBs as in
Fig. 4.10, but with a different arrangement as presented in Fig. 4.12. Notice that
the capacitors in Fig. 4.12(a) are used to guarantee the NP needed by the NPC leg.
Figure 4.12(b) shows the same configuration with the switches. In this case, it needs
three dc sources with the advantage of using all switches with the same blocking
voltage, as discussed in this section.
q2a
q1a
q1b
q1b
q1a
q2a
a
b
V1
1
2
3
4
V2
V3
V1
V2
V3
+
– vo
vo
io
Figure 4.12 Four-level single-phase converter: (a) block representation and (b) circuit with
switches.
104 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
TABLE 4.3 Table of Variables for the Converter in Fig. 4.12
State q1a q2a q1b 𝑣o
1 0 0 0 − V3
2 0 0 1 − V3 − V2
3 0 1 0 − V2/2
4 0 1 1 V2/2
5 1 1 0 V1 + V2
6 1 1 1 V1
The converter in Fig. 4.12 has six switches (q1a, q1a, q2a, q2a, q1b, and q1b),
two clamping diodes, three dc sources, and two dc-link capacitors. Considering all
possible switching states available and eliminating the prohibited ones, the output
voltage is determined in Table 4.3. To guarantee that all power switches will oper-
ate under the same blocking voltage as well as a symmetrical output voltage, it is
necessary to establish V1 = V3 = Vdc/4 and V2 = Vdc/2.
The modulation strategy for the converter shown in Fig. 4.12 can be determined
assuming a combination of the two-level and three-level PWM approaches, which
means that, for the two-level leg [PB 4 in Fig. 4.12(a)] only one triangular carrier
signal will be employed, while for the three-level leg [PBs 1, 2, and 3 in Fig. 4.12(a)]
two triangular carrier signals will be employed, as observed in Fig. 4.13(a). Since the
triangular waveform is proportional to the dc-link voltage associated with each leg,
the voltages 𝑣∗
t1
, 𝑣∗
t2
, and 𝑣∗
t3
can be obtained as shown in Fig. 4.13(b). In this sense,
the two-level leg will deal with one-third of the output voltage while the three-level
leg will deal with two-third of the desired output voltage.
The pole voltage for the three-level, two-level legs and output voltage is given
respectively by
𝑣a0 = (q1a + q2a − 1)2Vdc (4.23)
𝑣b0 = (2q1b − 1)Vdc (4.24)
𝑣o = (q1a + q2a − 2q1b − 1)Vdc (4.25)
Figure 4.14(a) and 4.14(b) shows the output voltage and current for a switching
frequency equal to 500 Hz and 1 kHz, respectively.
Although the configuration shown in Fig. 4.12 can generate a four-level output
voltage, it needs either three independent dc voltages or an auxiliary circuit to obtain
three controlled voltages from a unique dc voltage source, as in Fig. 4.14(c) – top.
Figure 4.14(c) – bottom shows the equivalent topological states when the switches
in the auxiliary circuit are turned on and off simultaneously. A duty cycle of 50%
should be generated to guarantee a desired capacitor voltage in the dc-link of the
converters.
Using the three-level NPC topologies and a three-phase load type, it is possible
to create a three-phase NPC topology with both two- and three-level characteristics
4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 105
q2a
qb
qb
q1a
q1a
q2a
vsin
*
2
3
+
–
vt1
*
vsin
*
2
3
+
–
+
–
–
2/3vsin –1/3vsin
* *
vt1
*
vsin
*
1
3
vt2
*
vt2
*
vt1
*
vt3
*
1
–1
0
0.66
–0.66
0
0.2 0.225 0.25
Figure 4.13 PWM generation: (a) analog implementation and (b) waveforms.
for the pole voltage. In this case, the dc-link of the three-phase converter is connected
to two PB-dc blocks, as depicted in Fig. 4.15. Figure 4.15(a) shows such hybrid topol-
ogy with the PBs perspective, while Fig. 4.15(b) depicts this topology by using power
switches. For a symmetrical waveform generation, it is necessary to define the input
voltages as follows: V1 = Vdc, V2 = 0, and V3 = − Vdc.
The operation of this converter takes into account the fact that it is possible to
obtain different levels per phase, depending on the values for the reference voltages.
For instance, Fig. 4.16(a) – top shows the desired phase voltages (𝑣∗
a, 𝑣∗
b
, and 𝑣∗
c )
divided by sectors. The first sector is defined by the interval of time in which 𝑣∗
a is
106 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
(a)
(b)
(c)
–30
–150
150
0
30
0
0.2 0.225 0.25
vo
io
–30
–150
150
0
30
0
0.2 0.225 0.25
vo
io
q1a
q2a
q1a
qb
qb
q2a
a
b
Vdc
Auxiliary
circuit
Equivalent circuit 1 Equivalent circuit 2
C1
C2
C3
C4
+
– vo
io
Figure 4.14 Output
voltage and current for the
configuration in Fig. 4.12
with: (a) 500 Hz and (b)
1 kHz. (c) (top) Auxiliary
circuit and (bottom)
equivalent topological
circuit.
4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 107
q2
q1a
qb
qa
q1
qb
qc
qc
qa
a
b
c
0
Vdc
Vdc
V1
c
b
a
V2
1
2
(a)
(b)
3
V3
Figure 4.15 Hybrid topology: (a) power blocks and (b) switching representation.
maximum, 𝑣∗
b
is minimum, and 𝑣∗
c is in-between. It means that: (i) phase a can be
modulated as a three-level leg (with pole voltage 𝑣a0 between Vdc and 0), since it
is expected to generate the maximum voltage; (ii) phase b can be modulated as a
three-level leg (with pole voltage 𝑣b0 between 0 and − Vdc); and finally (iii) phase c
can be modulated as a two-level leg (with the pole voltage between Vdc and − Vdc).
The modulation strategy for the leg dealing with the highest and smallest
voltages (three levels) are obtained by comparing the desired waveforms with two
triangular waveforms (with level-shift approach) as shown in Fig. 4.4, while the
modulation for the leg dealing with middle voltages (two levels) is obtained through
a comparison between the reference voltage and one triangular waveform.
Still considering nonconventional configurations, a half-bridge three-phase
NPC topology is shown in Fig. 4.17(a).
108 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
va
* vb
* vc
*
1
–1
0
50
–50
0
50
–50
0
50
–50
–15
15
0
0
0.77 0.8
0.77 0.8
va0
vb0
vc0
ia ib ic
(a)
(b)
Figure 4.16 (a) Desired reference voltage and pole voltages. (b) Load current.
As in the case of previous nonconventional topologies, it is necessary to adapt
the PWM strategy [see Fig. 4.17(b) and 4.17(c)] employed to guarantee the gener-
ation of a balanced three-phase load voltage. The challenge in this case is that the
three-phase currents of the load must be regulated in a balanced way, even though
there are only two legs available to do it. Two load currents are directly controlled
by these two legs, and the third one is indirectly controlled, since ia + ib + ic = 0. The
maximum amplitude of the line-to-line reference voltages (𝑣∗
ac = 𝑣∗
a − 𝑣∗
c ) and (𝑣∗
bc
=
𝑣∗
b
− 𝑣∗
c) is limited by the amplitude of the triangular waveforms, as in Fig. 4.17(c).
In these, the triangular waveforms have a frequency of 1 KHz.
As this topology cannot be considered conventional, there are some restrictions
in its practical application. However, it could be employed in fault-tolerant systems,
as a backup configuration in the case of a fault of the three-leg conventional topology
(Fig. 4.8).
4.7 UNBALANCED CAPACITOR VOLTAGE
If there is only one dc voltage source available, the NP required for the NPC con-
figuration can be obtained with two capacitors in a series connection, as seen in
Fig. 4.18(a). When a leg of the converter is connected (or clamped) to the NP, as in
4.7 UNBALANCED CAPACITOR VOLTAGE 109
q2b
q1a
driver
driver
driver
driver
driver
driver
driver
driver
q1a
q2a
q2a
q1b
q1b
q2b
q2b
q1b
q1b
q2b
q2a
q1a
q1a
q2a
Vdc
Vdc
R
R
R
L
L
L
va
* vac
*
vt1
*
vt2
*
vc
*
vb
*
Σ
Σ
+
–
+
–
+
–
–
–
+
–
vac
*
vac
*
vt1
*
vt1
1
–1
0
1
–1
0
40
–40
0
0.2 0.225 0.25
*
vt2
*
vt2
*
vbc
*
vt1
*
ia ib ic
vt2
*
vb
*
(a)
(b)
(c)
Figure 4.17 (a) Half-bridge three-level three-phase NPC converter. (b) PWM strategy.
(c) (from top to bottom) reference waveforms for leg a (𝑣∗
a − 𝑣∗
c , 𝑣∗
t1
, and 𝑣∗
t2
), reference
waveforms for leg b (𝑣∗
b
− 𝑣∗
c , 𝑣∗
t1
, and 𝑣∗
t2
) and load currents.
110 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
a
b
c Three-phase
load
215
200
185
0 0.5 1
Vdc
Vdc
C1
0
(NP) 0
(NP)
+
–
+
–
C2
C1
C2
iC1
iC1
iNP
vC1
vC2
iC2
vC2
vC1
iC2
ic
ib
ia
iNP
iNPa
iNPb
iNPc
(a) (b)
(c)
Figure 4.18 (a) NPC three-level topology with one dc voltage source. (b) Circuit showing
the currents in the capacitors. (c) Capacitor voltages.
Fig. 4.18(b), its current is injected at this point. The NP current (iNP) can be expressed
by the following equation
iNP = q2aq1aia + q2bq1bib + q2cq1cic (4.26)
Notice that the NP is a floating point. In an open-loop operation and without
a specific PWM strategy, there is no guarantee that 𝑣C1 and 𝑣C2 will converge to the
desired voltage, that is, Vdc/2. Considering the simple modulation strategy presented
in this chapter, the capacitor voltages are unbalanced, as in Fig. 4.18(c), which brings
up asymmetry at the output voltage of the converter.
To explain this capacitor voltage behavior it is necessary to observe the vari-
ables responsible for charging and discharging C1 and C2 highlighting the start-up
transient. From equation (4.25) it is seen that each component of the NP current
iNPx = q2xq1xix (with x = a, b, c) is a function of load current and switching states.
For example, Fig. 4.19(a) shows two currents associated with phase a, (i.e., ia
and iNPa). Notice that iNPa [the first portion of equation (4.26)] is actually the current
ia multiplied by the state of the switches q2a and q1a. As expected, such a current has
4.7 UNBALANCED CAPACITOR VOLTAGE 111
(a)
(b)
(c)
0.2
100
–100
0
100
–100
0
100
–100
0
100
–100
0
100
–100
0
0.225 0.25
0.2 0.225 0.25
100
–100
0
100
–100
0
0.2 0.225 0.25
iC2
iC1
iNPa
iNPa
iNPb
iNPc
ia
Figure 4.19 (a) ia and iNPa. (b) iNPa, iNPb, and iNPc. (c) iC1 and iC2.
an average value equal to 0. The behavior of the currents iNPa, iNPb, and iNPc is shown
in Fig. 4.19(b).
The capacitor currents iC1 and iC2 are functions of iNPa, iNPb, and iNPc, as seen in
Fig. 4.19(c). The reason why the capacitor voltage 𝑣C1 goes down and 𝑣C2 goes up in
Fig. 4.18(c) is because iC1 starts with a negative value while iC2 starts with a positive
value, that is, initially C1 is discharged and C2 is charged but always maintaining the
𝑣C1 + 𝑣C2 constant and equal to Vdc. There are different strategies to regulate 𝑣C1 and
𝑣C2 by either using feedback controllers or with specific PWM approaches.
112 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
(a)
(b) (c)
(d) (e)
2
1
4
5
3
V1
V2
vo
2
1
4
5
3
V1
vo
2
1
4
5
3
V2
vo
2
1
4
5
3
V3
vo
2
1
4
5
3
V4
vo
V3
V4
Figure 4.20 (a) Four-level NPC configuration with PBs. (b) 𝑣o = V1. (c) 𝑣o = V2. (d) 𝑣o = V3.
(e) 𝑣o = V4.
4.8 FOUR-LEVEL CONFIGURATION
Following the axioms and postulates involving the PBs, presented in the previous
chapter, the four-level (NPC) leg can be easily obtained as seen in Fig. 4.20(a).
Figure 4.20(b)–4.20(e) shows the ways used to obtain each specific level (V1, V2, V3,
and V4) at the output converter side. Figure 4.20(b) illustrates that it is necessary to
activate the PBs 1, 3 and 5 to obtain 𝑣o = V1, while 𝑣o = V4 is obtained when PBs 2,
4, and 5 are activated [see Fig. 4.20(e)]. On the other hand, the intermediate voltages
V2 and V3 are obtained at the output side when PBs 3 and 5, and PBs 4 and 5 are
activated, respectively. In general terms, to generate an output waveform with four
levels as in Fig. 4.21 (bottom), it is necessary to activate the PBs in a sequence as
observed in Fig. 4.21 (top).
Since 𝑣o is supposed to assume just one input voltage V1, V2, V3, or V4 at a
time, an equation to describe the output voltage 𝑣o as a function of the input voltages
can be obtained from the independent binary variables (q1, q2, and q3). As in the
4.8 FOUR-LEVEL CONFIGURATION 113
2
1
4
5
3
V1
V1
vo
vo
2
1
4
5
3
V2
V2
vo
2
1
4
5
3
V3
V3
vo
2
1
4
5
3
V4
V4
t
vo
Figure 4.21 Generation of a general four-level output voltage.
TABLE 4.4 Table of Variables for the Converter in Fig. 4.20(a)
State q1 q2 q3 𝑣o
1 0 0 0 V4
2 0 0 1 V3
3 0 1 0
4 0 1 1 V2
5 1 0 0
6 1 0 1
7 1 1 0
8 1 1 1 V1
three-level NPC topology, the binary variables considered in Table 4.4 are related to
the switching states inside the blocks in Fig. 4.20.
In this case, the output pole voltage is given by
𝑣o = q1q2q3V4 + q1q2q3V3 + q1q2q3V2 + q1q2q3V1 (4.27)
where q1 = 1 − q1, q2 = 1 − q2, and q3 = 1 − q3.
Normally the waveform shown in Fig. 4.21 must be symmetrical, which means
that V1 = Vdc, V2 = Vdc/3, V3 = − Vdc/3, and V4 = − Vdc, and
𝑣o =
(
−q1q2q3 −
q1q2q3
3
+
q1q2q3
3
+ q1q2q3
)
Vdc (4.28)
If any other combination of output voltages associated with the switching states
is considered, instead of the Table of Variables presented in Table 4.4, it will lead to
undesired states, as presented shown in Example 4.2.
114 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
q1
V1
q2
(a) (b)
(c)
(d)
q3
io
q1
V3
q2
q3
io
q1
V4
q2
q3
io
q1
V2
q2
q3
io
Figure 4.22 Generation of the level: (a) V1, (b) V2, (c) V3, and (d) V4 independent of the
output current.
The four-level NPC configuration has no restriction in terms of the generation
of desired output voltage and the values of currents, which means that each desired
voltage value V1, V2, V3, and V4 can be obtained at the output converter side for any
values of current (io > 0 or io < 0) as in Fig. 4.22.
4.9 PWM IMPLEMENTATION (FOUR-LEVEL CONFIGURATION) 115
driver
driver
+
–
q1
q2
q3
q1
q1
q2
q3
vsin
*
vt1
*
vt1
*
driver
driver
+
–
q1
q2
q3
q1
q2
q3
vsin
*
vt2
*
driver
driver
+
–
q1
q2
q3
q1
q2
q3
vsin
*
vt3
*
1
0
1
0
1
0
0.2 0.225 0.25
–1
q1
vsin
*
q2
vt2
*
1
0
1
0
1
0
0.2 0.225 0.25
–1
q2
vsin
*
q3
vt3
*
1
0
1
0
1
0
0.2 0.225 0.25
–1
q3
vsin
*
(a) (b) (c)
(d)
(e)
(f)
Figure 4.23 Four-level NPC topology – control circuit and signals for the switches.
4.9 PWM IMPLEMENTATION (FOUR-LEVEL
CONFIGURATION)
Figure 4.23 shows the analog solution for the PWM generation of one leg. The states
of the six switches are determined by a comparison among three high frequency tri-
angular waveforms (𝑣∗
t1
, 𝑣∗
t2
, and 𝑣∗
t3
) and a sinusoidal waveform (𝑣∗
sin
).
116 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
It can be seen from Fig. 4.23 that these three triangular waveforms (𝑣∗
t1
, 𝑣∗
t2
, and
𝑣∗
t3
) are intentionally level-shifted to guarantee four levels at the output converter side.
During the interval of time in which q1 and q1 are in operation (i.e., turning on and
off) q2 and q3 are always on and consequently q2 and q3 are always off. This is exactly
what is expected from Table 4.4, rows 8 and 4, that is, when the switching sequence
is changed from (q1,q2,q3) = (1,1,1) to (q1,q2,q3) = (0,1,1) the output voltage will
change from V1 to V2. On the other hand, during the interval of time in which q2 and
q2 are in operation (turning on and off) q1 is always off and q3 is always on, which
is expected from Table 4.4, rows 2 and 4. In this case, when the switching sequence
is changed from (q1,q2,q3) = (0,0,1) to (q1,q2,q3) = (0,1,1) the output voltage will
change from V3 to V2. Finally, for the interval of time in which q3 and q3 are in
operation (turning on and off) q1 and q2 are always off, which is also expected from
Table 4.4, rows 1 and 2. When the switching sequence is changed from (q1,q2,q3) =
(0,0,0) to (q1,q2,q3) = (0,0,1) the output voltage will change from V4 to V3.
Figure 4.24 shows the power converter and waveforms for a half-bridge
four-level configuration. If only one dc source is available, as in Fig. 4.18, additional
R L
q1
Vdc1
Vdc2
Vdc3
Vdc4
q2
q3
q1
q2
q3
(a)
1
1
0
1
0
1
0
200
–200
50
–50
0.2 0.225 0.25
–1
q1
q2
q3
vo
io
(b)
Figure 4.24 (a) Four-level NPC half-bridge converter. (b) (from top to bottom) 𝑣∗
sin
, 𝑣∗
t1
, 𝑣∗
t2
,
𝑣∗
t3
; gating signal of switch q1; gating signal of switch q2; gating signal of switch q3; load
voltage and load current.
4.9 PWM IMPLEMENTATION (FOUR-LEVEL CONFIGURATION) 117
capacitors can be employed to obtain four voltage levels. However, the challenge to
control the capacitor voltages from a single dc source increases with the number of
levels of the converters. From four levels onwards, an auxiliary circuit is normally
needed to guarantee the control of such capacitors for a large range of load power
factor.
It is worth mentioning that the number of triangular waveforms increases pro-
portionally to the number of levels. For a converter with n levels n − 1 triangular
waveforms are needed at the output of the converter. As a consequence of the high
number of triangular waveforms, such converters must be designed to operate at high
modulation index to guarantee the desired amount of levels at the output converter
side. Figure 4.25 shows the influence of the modulation index (ma) in the converter
waveforms. Such a figure highlights the control (top) and output converter (middle
and bottom) waveforms for three different values of ma. When ma is decreased, the
(a)
(b)
1
0
–1
200
0
–200
40
0
0 0.02 0.04
0 0.02 0.04
–40
1
0
–1
200
0
–200
40
0
–40
Figure 4.25 (top) Sinusoidal and triangular waveforms, (middle) load voltage and (bottom)
load current: (a) ma = 0.8, (b) ma = 0.45, and ma = 0.2.
118 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
(c)
0 0.02 0.04
1
0
–1
200
0
–200
40
0
–40
Figure 4.25 (Continued)
number of levels reduces as well, as observed in the sequence of Fig. 4.25(a), 4.25(b),
and 4.25(c), respectively. The output voltage is reduced to a two-level waveform when
the modulation index is equal to 0.2.
4.10 FULL-BRIDGE AND OTHER CIRCUITS
(FOUR-LEVEL CONFIGURATION)
The full-bridge single-phase converter using four-level NPC legs is shown in
Fig. 4.26(a). This topology could be of interest in single-phase applications when
the quality of the output voltage is an important aspect of the design since the load
voltage (𝑣o = 𝑣a0 − 𝑣b0) has almost sinusoidal behavior. Figure 4.26(b) shows (from
top to bottom) pole voltage 𝑣a0, pole voltage 𝑣b0, load voltage, and load current,
respectively.
A three-phase three-level full-bridge NPC configuration is depicted in
Fig. 4.27(a), while Fig. 4.27(b) shows some variables associated with this converter,
that is, (from top to bottom) pole voltage (𝑣a0), voltage between load NP and
dc-link midpoint connection (𝑣n0), load phase voltage (𝑣an), and load current (ia),
respectively.
Figure 4.28 shows a half-bridge three-phase four-level NPC topology. In this
case, a similar approach employed for the three-level topology, in terms of the PWM
circuit, is also considered for this configuration.
A four-level topology can be obtained for a three-phase machine with
open-end windings following the pattern of the circuit given in Fig. 4.12, and shown
in Fig. 4.29. This is an open-end winding motor drive system, which requires access
to six terminals of the machine. A four-level voltage appears in each phase of the
machine.
4.11 FIVE-LEVEL CONFIGURATION 119
R L
q1a
Vdc1
Vdc2
a
0 b
Vdc3
Vdc4
q2a
q3a
q1a
q2a
q3a
q1b
q2b
q3b
q1b
q2b
q3b
(a)
200
0
0.2 0.225 0.25
–200
200
0
–200
500
0
–500
100
0
–100
vo
vb0
va0
io
(b)
Figure 4.26 (a) Four-level NPC full-bridge converter. (b) (from top to bottom) pole voltage
𝑣a0, pole voltage 𝑣b0, load voltage, and load current.
4.11 FIVE-LEVEL CONFIGURATION
Following the same approach presented before for the three- and four-level configura-
tions, the five-level converter is shown in Fig. 4.30(a). As done for the previous NPC
topologies. Notice that just two types of PBs are employed. Figure 4.30(b) shows the
five-level configuration with the traditional representation, using switches.
In addition to the capacitor voltage balancing problem, another challenge
appears when the number of levels increases for an NPC topology. The blocking
voltage for each clamping diode changes and it depends on its position in the circuit.
The diode voltage can be written as
𝑣D = (N − 1 − x)(N − 1)−1
Vdc (4.29)
120 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
R L
R L
R
+ –
L
n
q1a
Vdc1
Vdc2
a
0 b
Vdc3
Vdc4
q2a
q3a
q1a
q2a
q3a
q1b
q2b
q3b
q1b
q2b
q3b
q1c
q2c
q3c
q1c
q2c
q3c
(a)
500
0
0.2 0.225 0.25
–500
500
0
–500
500
0
–500
100
0
–100
van
vn0
va0
van
ia
ia
(b)
Figure 4.27 (a) Four-level three-phase NPC converter. (b) (from top to bottom) pole voltage,
voltage between load NP and dc-link midpoint connection, load voltage, and load current.
R L
R L
R L
b
c
q1b
q2b
q3b
q1b
q2b
q3b
q1c
q2c
q3c
q1c
q2c
q3c
Vdc1
Vdc2
0
Vdc3
Vdc4
Figure 4.28 Half-bridge
four-level three-phase NPC
converter.
4.11 FIVE-LEVEL CONFIGURATION 121
q1a
C1
C2
C3
C4
qc
c
b
a a+
q2a
q1a
q2a
q1b
b+
q2b
q1b
q2b
q1c
c+
q2c
q1c
q2c
qc
qb
qb
qa
Phase 1
Phase 2
Phase 3
Three-phase
machine
qa
Figure 4.29 Four-level open-end motor drive system.
(a)
(b)
2
1
4
5
7
6
3
V1
V2
vo
V3
V4
V5
q1
q2
q3
q4
q1
q2
q3
q4
Vdc1
Vdc2
Vdc3
0
Vdc4
Figure 4.30 Five-level NPC
converter: (a) PB representation and
(b) representation with switches.
122 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
(a)
(b)
V1
V2
vo
V3
V4
V5
q1
q2
q3
q4
q1
q2
q3
q4
Vdc1
Vdc2
Vdc3
0
Vdc4 Figure 4.31 Five-level NPC
converter with pyramid structure:
(a) PB representation and
(b) representation with switches.
where N is the number of levels, x changes from 1 to N − 2 and Vdc is the dc-link
voltage of the whole dc source. For high voltage applications, such different blocking
voltage characteristics could bring up operational limits for the converter. To solve
this problem and guarantee the same blocking voltages for all diodes, it is necessary
to add more clamping diodes in series.
By adding the first PB-dc shown in Fig. 4.31(a), it is possible to find a topology
with the same blocking voltages for all diodes with a pyramid structure as proposed
by Yuan and Barbi [14] and depicted in Fig. 4.31(b).
Theoretically, the number of levels in an NPC topology can be increased as
necessary, and to do so the PB-cc blocks must be stacked as in Fig. 4.32.
4.11 FIVE-LEVEL CONFIGURATION 123
3
1
2
1
3
5
4
2
1
3
5
7
6
4
2
(a)
(b)
(c)
(d)
Figure 4.32 Generation of the n-level NPC topologies: (a) three-level, (b) four-level,
(c) five-level, and (d) n-level.
124 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION
4.12 SUMMARY
This chapter is dedicated to NPC configurations. Further details about NPC topolo-
gies can be found in References from 1 to 14. The topologies are presented in a
systematic way in the following sequence: (i) PBs connections obtained from the
rules presented in Chapter 3; (ii) once the topology is established, the Table of Vari-
ables is obtained; (iii) the next step is modeling the converter by writing the output
voltage to describe what was obtained in the Table of Variables; and (iv) and finally
the PWM approach is developed from the Table of Variables. The same systematic
approach has been applied for both conventional and nonconventional topologies.
More than bringing new possibilities for power electronics converters in differ-
ent applications, nonconventional converters play an important role in the learning
process and ensure a deep understanding of the subject.
REFERENCES
[1] Baker RH. Bridge converter circuit. US patent 4270163. 1981 May (filed in Aug. 79).
[2] Nabae A, Takahashi I, Akagi H. A new neutral-point-clamped PWM inverter. IEEE Trans Ind Appl
1981;IA-17(5):518–523.
[3] Steinke JK. Control of a neutral-point-clamped PWM inverter for high power AC traction drives.
Int’l Conf on Power Electron and Variable-Speed Drives on; 1988 Jul 13–15. p 214–217.
[4] Holtz J. Self-commutated inverters with a stepped output-voltage waveform suitable for high powers
and frequencies. Siemens Forsch-U Entwick1-Ber 1977;6(3):164–171.
[5] Carrara G, Gardella S, Marchesoni M, Salutari R, Sciutto G. A new multilevel PWM method: a
theoretical analysis. IEEE Trans Power Electron 1992;7:497–505.
[6] Lin B-R, Wei T-C. Space vector modulation strategy for an eight-switch three-phase NPC converter.
IEEE Trans Aerosp Electron Syst 2004;40(2):553–566.
[7] Holmes DG, Lipo TA. Pulse Width Modulation for Power Converters. Piscataway: IEEE/Wiley Inter-
science; 2003.
[8] E. C. dos Santos Jr., Muniz JHG, and da Silva ERC. 2L3L inverter. Proc of Brazilian Power Electron
Conf (COBEP); 2011, p 924–929
[9] Mihalache L. A hybrid 2/3 level converter with the minimum switch count. Industry Applications
Conference. 41st IAS Annual Meeting. Conference Record of the 2006 IEEE; 2006; vol. 2.
p 611–618.
[10] da Silva ER, Muniz JG, da Nobrega RB, dos Santos Jr. EC. An improved pulse-width-modulation
for the modified hybrid 2/3-level converter. Proc of Brazilian Power Electron Conf (COBEP); 2013,
p 248–253.
[11] Choi NS, Cho JG, Cho GH. A general circuit topology of multilevel inverter. Proc. Rec. IEEE PESC;
1991. p 96–103.
[12] Carpita M, Tenconi S. A novel multilevel structure for voltage source inverter. Proc. Rec. EPE Conf.;
1991. p 1.90–1.94.
[13] Hammond PW. Medium voltage PWM drive and method. US patent 5,625,545. 1997.
[14] Yuan X, Barbi I. A new diode clamping multilevel inverter. Proceedings of APEC99; 1999.
p 495–501.
CHAPTER 5
CASCADE CONFIGURATION
5.1 INTRODUCTION
The PBG is employed in this chapter to describe the cascade multilevel configura-
tions, also known as H-bridge series connected configurations. The introduction and
fundamental concepts are furnished for a single H-bridge topology, followed by the
connection of other H-bridge converters for generation of topologies with more lev-
els. Such configurations deal with attractive characteristics common for multilevel
circuits, such as low electromagnetic interference (EMI), reduced total harmonic dis-
tortion and high relationship between the number of levels per number of switches.
Comparing this multilevel configuration with the neutral point clamped (NPC) topol-
ogy described earlier, it is possible to sort some advantages such as (i) simple pack-
aging and physical structure with no neutral point clamping circuits, (ii) modular
structure (more or fewer H-bridge cells can be cascaded depending on the desired
power quality), and (iii) possibility to operate even with partial failure. On the other
hand, the main disadvantages are associated with (i) greater number of dc sources
and (ii) control complexity.
The previous chapter was organized with the sections divided in terms of the
number of levels of the converter, that is, three levels, four levels, and so on. In
this chapter, on the other hand, the organization (labeling scheme) of the sections
considers the number of H-bridge converters instead of number of levels. The main
reason for that is, depending on the values of the dc voltage sources and modulation
approach, the same topology can generate different number of levels.
Accordingly, Section 5.2 presents the description of a single H-bridge converter
along with its Table of Variables. The pulse width modulation (PWM) implementa-
tion is derived from the Table of Variables, as highlighted in Section 5.3. The fol-
lowing section presents the three-phase version with a single H-bridge converter per
phase. Sections 5.5, 5.6, and 5.7 deal with two H-bridge converters in series, with the
sequence given respectively by power converter construction, PWM approach, and
three-phase version. After showing how it is possible to guarantee post-fault oper-
ation with this type of converter in Section 5.7, Section 5.8 demonstrates that two
H-bridge converters can be employed to generate an output voltage with either seven
or nine levels, by employing the correct relationship between the dc-link voltages.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
125
126 CHAPTER 5 CASCADE CONFIGURATION
V1
V2
(a) (b)
(c) (d)
vo
V1
V2
vo
V1
V2
vo
V1
V2
vo
Figure 5.1 (a) One H-bridge configuration with PBs. (b) 𝑣o = V1 − V2. (c) 𝑣o = V2 − V1.
(d) 𝑣o = 0.
Section 5.9 presents different arrangements and PWM solutions for three H-bridge
converters connected in series. Finally, Section 5.10 introduces the generalization and
other possible converters characterized by series arrangements of H-bridge circuits.
This chapter has been written with the help of References from 1 to 14.
5.2 SINGLE H-BRIDGE CONVERTER
Considering the power blocks (PBs), no connection is needed among PBs to obtain
an H-bridge topology, since there is a block that represents this converter directly,
as observed in Fig. 5.1(a). Figure 5.1(b), 5.1(c) and 5.1(d) illustrates the methods
used to obtain three levels at the output converter side (V1 − V2, V2 − V1, 0). In
general terms, to generate an output waveform with three levels as in Fig. 5.2 (bot-
tom), it is necessary to activate the PBs in a sequence as observed in this figure
(top).
Notice that instead of selecting one of the input voltages V1, V2, and V3 as
done for the NPC topology considered in the previous chapter, the three-level output
voltage in Fig. 5.2 is a combination of two voltages V1 and V2 available at the input
converter side. Despite the three-level voltage in Fig. 5.2, it is convenient to start the
analysis of the cascade multilevel topologies by assuming just two levels (V1 − V2,
V2 − V1) at the output converter side, as in Fig. 5.1(b) and 5.1(c).
Since 𝑣o can assume just one combination of the input voltages each time, it is
reasonable to write an equation to describe the output voltage 𝑣o as a function of both
input voltages and an independent binary variable. As the number of input voltages
to be selected is two, the minimum number of binary control variable is one. This
binary variable should be used to select one combination of the inputs to appear at
the output converter side, which means that one possible solution to achieve this goal
is given in Table 5.1.
From q1 and its complementary signal q1 = 1 − q1, the output voltage can be
obtained as follows:
𝑣o = q1(V1 − V2) + q1(V2 − V1) (5.1)
5.2 SINGLE H-BRIDGE CONVERTER 127
V1
V1 – V2
V2 – V1
t
0
V2
vo
vo
V1
V2
vo
V1
V2
vo
Figure 5.2 General three-level output voltage.
TABLE 5.1 Converter in Fig. 5.1(a) Operating as
a Two-Level Converter
State q1 𝑣o
1 1 V1 − V2
2 0 V2 − V1
If V1 − V2 = Vdc, then (5.1) can be written as follows:
𝑣o = (2q1 − 1)Vdc (5.2)
As seen in the previous chapter, these control variables (q1 and q1) are in fact the
states of the switches inside the blocks. Comparing Table 5.1 with Fig. 5.2 (bottom)
it is evident that just one binary control variable (q1) and its complementary signal
(q1) are not enough to select three levels at the output converter side.
If the number of levels for the output voltage is expected to be three (±Vdc,0),
the minimum number of binary variables in this case should be two, which are used
to select a desired output voltage, meaning that one possible combination to achieve
this goal is given in Table 5.2.
The output voltage can be written as
𝑣o = −q1q2Vdc + q2q1Vdc (5.3)
where q2 = 1 − q2. Substituting the complementary variables, the previous equation
becomes
𝑣o = −(1 − q1)q2Vdc + (1 − q2)q1Vdc (5.4)
𝑣o = (q1 − q2)Vdc (5.5)
128 CHAPTER 5 CASCADE CONFIGURATION
TABLE 5.2 Converter in Fig. 5.1(a) Operating as
a Three-Level Converter
State q1 q2 𝑣o
1 0 0 0
2 0 1 −Vdc
3 1 0 Vdc
4 1 1 0
Figure 3.10 shows the same configuration presented in Fig. 5.1, along with
binary variables describing the state of the switches for positive and negative
output currents (io). Notice that there is no restriction in terms of state of the
switches and the values of currents, which means that each voltage value can be
obtained at the output converter independent of the current values (io > 0 and
io < 0).
Example 5.1
Considering the previous analysis, place each switch (q1, q1, q2, and q2) in
the correct position in the following circuit to guarantee the generation of the
levels as shown in Table 5.2.
Vdc
Position 1
+
–
Position 3
Position 2
Position 4
vo
Solution
For the generation of a voltage 𝑣o with three levels, as in Table 5.2, q1 should
be placed, for example, in position 2, while q2 should be placed in position 1.
Consequently q1 and q2 should be placed in positions 4 and 3, respectively.
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 129
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE
CONVERTER
If a single H-bridge converter is operating with two or three levels independently,
the ultimate control goal is to guarantee a regulated voltage at its output side. The
output voltage is regulated in terms of amplitude and frequency, obtained through
PWM strategies. Many works in the technical literature have proposed solutions in
terms of modulation approach applied to cascade converters. A simple sinusoidal
carrier-based PWM strategy is considered in this chapter.
Figure 5.3 shows an analog solution for implementation of PWM, in which
the states of the four switches are determined by a comparison between one high
frequency triangular waveform (𝑣∗
t ) and a sinusoidal waveform (𝑣∗
sin
). Note that this
modulation strategy generates the waveforms with two levels as seen in Table 5.1.
In Fig. 5.3(a) (top) the same gating signals are sent to q1 and q2, while the same
complementary signals are sent to q2 and q1, which implies that the pair of switches
q1 − q2 and q2 − q1 are always turned on and off simultaneously. Figure 5.3(a) (bot-
tom) shows the power part of the converter, and Fig. 5.3(b) shows the waveforms of
the PWM and gating signals.
While Fig. 5.4(a) shows an H-bridge converter supplying a single-phase RL
load, Fig. 5.4(b) shows (from top to bottom) PWM reference waveforms (𝑣∗
sin
and 𝑣∗
t ),
gating signal of switch q1, gating signal of switch q2, load voltage and load current,
respectively. The parameters employed in these simulation results were Vdc = 200V,
R = 5Ω, and L = 5mH, and switching frequency was equal to 1000Hz. These same
parameters have been used for other simulation outcomes in this chapter.
The modulation strategy presented in Figs 5.3 and 5.4 seems to have low prac-
tical interest due to a two-level voltage generation, which means reduced THD as
compared to the three-level option. However, it permits applicability in photovoltaic
systems due to common mode voltage and current reduction.
As indicated by Fig. 5.2 and Table 5.2, an H-bridge converter is also able to
generate a three-level voltage by just changing the PWM control signals.
Figure 5.5 shows two PWM approaches used to control the H-bridge converter.
A direct comparison between the results obtained in Fig. 5.5 highlights some advan-
tages and drawbacks for each method used to generate three levels at the output
converter side. For instance, with two high frequency waveforms (𝑣∗
t1
and 𝑣∗
t2
) [see
Fig. 5.5(a) and 5.5(c) – Method 1] it is possible to operate the converter with reduced
power converter losses, since one leg will modulate (turning the switches on and off)
while the other one will be clamped. Method 1 is also known as level-shift PWM strat-
egy. On the other hand, the operation with one high frequency waveform (𝑣∗
t ) and two
modulating signals (𝑣∗
sin 1
and 𝑣∗
sin 2
) [see Fig. 5.5(b) and 5.5(d) – Method 2] guaran-
tees lower harmonic distortion, which can be verified by the reduced current ripple.
In this case, both legs modulate during the whole period of the sinusoidal waveforms;
as a consequence, the harmonic content of the high frequency components is twice
that of the switching frequency.
In Method 1 [Fig. 5.5(a) and 5.5(c)] just two states in Table 5.2 are employed
per half of the sinusoidal period, that is, states 1 and 3 for the positive half of the
130 CHAPTER 5 CASCADE CONFIGURATION
driver
driver
+
–
q1
q2
q1
q2
q1
q2
q2
q1
q1
q2
vsin
*
vt2
*
vsin
* vt
*
(a)
1
1
–1
0
0
1
1 1.025 1.05
0
(b)
Figure 5.3 (a) PWM generation for switches q1, q2, q1, and q2. (b). (from top to
bottom) – reference voltages, gating signal of switch q1, and gating signal of switch q2.
sine, and states 1 and 2 for the negative half of the sine. In this method, state 4 with
both switches on is never employed. On the other hand, in Method 2 all states are
employed.
Figures 5.4 and 5.5 highlight that the same average voltage and consequently
the same amplitude (in terms of average values) of the load current is obtained at the
output converter side, independent of the modulation strategies employed.
The frequency-domain representation, using the Fourier transformation of the
output voltage, is an important tool to understand the differences between the PWM
strategies in Fig. 5.5.
Figure 5.6(a) and 5.6(b) shows the waveforms presented in Fig. 5.5, with both
time- and frequency-domain for Methods 2 and 1, respectively. Notice that the pole
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 131
(a)
q1
q2
vsin
*
vo
io
vt
*
1
1
–1
0
0
1
1 1.025 1.05
0
200
–200
50
–50
(b)
q1 q2
R
+
–
L
q2
2
1
0
q1
io
vo
Vdc
2
Vdc
2
Figure 5.4 (a) Two-level H-bridge converter. (b) (from top to bottom) 𝑣∗
sin
, 𝑣∗
t ; gating signal
of switch q1; gating signal of switch q2; load voltage and load current.
voltages for Method 2 have two main frequency components, that is, one related to
the sinusoidal and another related to the triangular waveform. Since 𝑣o = 𝑣10 − 𝑣20
and there is just one triangular waveform, such a frequency component is cancelled
for 𝑣o. Although not shown in this figure, there are higher frequency components. On
the other hand, there are two sinusoidal waveforms with phase shift equal to 180∘ for
Method 2, which explains why the amplitude of the sine frequency component for 𝑣o
is twice that for 𝑣10 and 𝑣20. Such a characteristic also explains the higher switching
frequency observed for 𝑣o in the time domain. For Method 1 [Fig. 5.6(b)], each pole
voltage has dc components that are cancelled for 𝑣o, but the triangular frequency com-
ponents are not cancelled. Since this waveform was obtained by employing different
carrier signals, it is clear why the switching frequency components for 𝑣o in Method
1 are equal to the switching frequency component observed in the pole voltages.
Exercise 5.1
Determine all topological states (equivalent circuits) for the switching states
in both strategies presented in Fig. 5.5. Assume both positive and negative
currents.
132 CHAPTER 5 CASCADE CONFIGURATION
driver
driver
driver
driver
+
–
+
–
q1
q1
q2
q2
q1
q1
q2
q2
vsin
*
vt1
*
vt1
*
v10
v20
vo
io
vt2
*
vt2
*
driver
driver
driver
driver
+
–
+
–
q1
q1
q2
q2
q1
q1
q2
q2
vsin1
*
vsin
*
vsin2
*
vt
*
(a)
(b)
1
–1
100
–100
100
–100
200
–200
50
–50
1 1.025 1.05
0
vt
*
v10
v20
vo
io
vsin1
* vsin2
*
1
–1
100
–100
100
–100
200
–200
50
–50
1 1.025 1.05
0
(c)
(d)
Figure 5.5 PWM strategy: (a) Method 1 and (b) Method 2. (c) Waveforms for method 1:
(from top to bottom) 𝑣∗
sin
, 𝑣∗
t1
, and 𝑣∗
t2
; pole voltage 𝑣10; pole voltage 𝑣20, load voltage 𝑣o; and
load current io. (d) Waveforms for method 2: (from top to bottom) 𝑣∗
sin 1
, 𝑣∗
sin 2
, and 𝑣∗
t ; pole
voltage 𝑣10; pole voltage 𝑣20, load voltage 𝑣o; and load current io.
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 133
(a)
(b)
v10
Time domain
v20
Time domain
v10
Frequency domain
Sine freq. Triangular freq.
Sine frequency
Sine frequency
Triangular frequency
Frequency domain
Time domain Frequency domain
v20
vo
v10
Time domain
v20
Time domain
v10
Frequency domain
Sine frequency
Triangular frequency
Sine frequency
Sine frequency
Triangular frequency
Triangular frequency
Frequency domain
Time domain Frequency domain
v20
vo
vo
vo
Figure 5.6 Waveforms for time and frequency domains for: (a) Method 2 and (b) Method 1.
In general terms, for a PWM strategy obtained from a comparison between
sinusoidal and triangular waveforms as presented in Figs 5.3 and 5.5(b), the peak
amplitude of the fundamental component for the pole voltage V10(1) [see equation
(2.10)] is given by
V10(1) =
V∗
sin
Vt
Vdc
2
= ma
Vdc
2
(5.6)
134 CHAPTER 5 CASCADE CONFIGURATION
It turns out that the fundamental component can be written by 𝑣10(1)(t) =
ma(Vdc∕2) sin(𝜔t) with ma ≤ 1. The harmonic components can be calculated using
the Fourier series as follows:
𝑣10(t) = V10(0) +
∞
∑
h=1
𝑣10(h)(t) (5.7)
with
∞
∑
h=1
𝑣10(h)(t) =
∞
∑
h=1
{ah cos(h𝜔t) + bh sin(h𝜔t)}. Note that ah are the cosine
components in the Fourier series, while bh are the sine components, see equations
(2.1)–(2.3).
Indeed the harmonic for the pole voltage comes out as side-bands centered on
the switching frequency and its multiples. The figure below shows the amplitude of
the normalized harmonic component V10(h)∕(Vdc∕2) versus the harmonics, obtained
from equation (5.6) for three values of modulation indexes: ma = 1, 0.6, and 0.4, and
with mf > 21 for all cases.
1
1
0.02 0.03 0.03
0.13
1.00
0.13
0.07
0.37 0.37
0.07 0.04 0.04
0.08
0.20
0.20
0 0
0.06 0.06 0.02 0.02 0.01 0.01
0.12
0.13
0.13
0.32
0.32
1.15
0.40
0 0 0 0 0 0
0 0 0
0
0.04
0.15 0.11 0.15
0.06
0.06
0.04
Harmonic
mf–4
2mf–5 2mf+5
2mf+3
2mf–3
2mf+1
3mf+4
3mf–4
3mf–6 3mf+6
3mf–2 3mf+2
3mf
2mf–1
mf+4
mf–2 mf+2
ma=1.0 mf>21
ma=0.6 mf>21
ma=0.4 mf>21
mf
1 Harmonic
mf–4
2mf–5 2mf+5
2mf+3
2mf–3
2mf+1
3mf+4
3mf–4
3mf–6 3mf+6
3mf–2 3mf+2
3mf
2mf–1
mf+4
mf–2 mf+2
mf
1 Harmonic
mf–4
2mf–5 2mf+5
2mf+3
2mf–3
2mf+1
3mf+4
3mf–4
3mf–6 3mf+6
3mf–2 3mf+2
3mf
2mf–1
mf+4
mf–2 mf+2
mf
0.02
0.32 0.32 0.21 0.21
0.18 0.18
0.60
0.60
v10
v10
v10
It can be seen from this figure that the pole voltage has an interesting charac-
teristic, that is, there is only odd harmonics. The even harmonics disappear if mf is
an odd integer bigger than 9. This is due to odd symmetry with 𝑣10(−t) = −𝑣10(t).
Also, the ah (cosine elements in the Fourier series) are equal to zero, while the terms
bh (sine elements) can be different from zero.
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 135
The pole voltage is plotted below to demonstrate the effect of an even value
for mf as compared to an odd one. Note that when mf = 8, an asymmetric waveform
is obtained at the pole voltage, since the comparison of the peaks and valleys
of the sinusoidal voltage along with the triangular one is different. On the other
hand, when mf = 9 (an odd number for mf ) a symmetric waveform is obtained
since the comparison is symmetric for all periods, as highlighted in the peaks and
valleys.
• ma = 0.9 and mf = 8
vsin
* vt
v10
Asymmetrical waveform
ma = 0.9 and mf = 8
• ma = 0.9 and mf = 9
vsin
* vt
v10
Symmetrical waveform
ma = 0.9 and mf = 9
Other harmonic component elimination can be obtained when both sinusoidal
(𝑣∗
sin
) and triangular (𝑣t) waveforms are synchronized for mf < 21. If mf > 21, no
synchronization is needed due to low gain.
Application (Photovoltaic Systems)
A typical photovoltaic (PV) power system is composed of a set of PV arrays with one
central inverter, which can be implemented transformerless or with an isolated trans-
former as shown below. The last solution is sometimes avoided due to size, weight,
and price of the low frequency transformer.
136 CHAPTER 5 CASCADE CONFIGURATION
Inverter
1
2
PV arrays
Transformerless
Utility
grid
Due to high frequency on the inverter, a common mode voltage (𝑣CM ) is gener-
ated with respect to the ground, which will induce a circulating current between the
PV panels and the grid through the inverter. Notice that such a current does not exist
when a transformer is used.
Due to safety requirements the PV module frame is connected to the ground,
as represented in figure below (left side). Since the panels have a planar structure
and module glass, it results in capacitance to the ground. In fact, the individual PV
cells have distributed stray capacitance to the ground, as depicted in the middle of the
figure below. The distributed capacitance throughout the module can be characterized
by an equivalent lumped capacitance highlighted in the right figure below.
PV panel
Individual
PV cell
CPV
CPV
PV
Panel
PV panel
Distributed
stray
capacitance
Lumped
stray
capacitance
P(+)
P(+) P(+)
N(–)
N(–)
N(–)
Assuming this equivalent circuit for the PV along with the stray capacitances, it
is possible to obtain the circuit below (top). Without an isolated transformer there is a
galvanic connection between the grid and PV arrays represented in this figure by the
circulating current iLeakage. The bottom-left-side figure below shows a simplification
of this circuit with a block representing the panels and the inverter. In this case,
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 137
for simplification purposes, just one CPV is considered between the point N and
the ground. If an H-bridge topology (bottom-right-side figure below) is chosen to
implement the grid-tie inverter, it is possible to define two voltages as function of
𝑣1N = q1VPN and 𝑣2N = q2VPN as follows:
• Differential voltage: 𝑣DM = 𝑣1N − 𝑣2N;
• Common mode voltage: 𝑣CM = (𝑣1N + 𝑣2N)∕2.
Dc-link
capacitances P
P
q1 q2
L1
L2
L1
L2
1
1
2
2
1
2
Grid-tie
Inverter
PV array +
inverter
CPV
CPV
CPV
N
N
N
Stray
capacitance
iLeakage
iLeakage
Using both voltages 𝑣DM and 𝑣CM it is possible to model the block describing
PV array + Inverter above with the circuit presented below.
PV array + inverter
L1
L2
1
2
CPV
vCM
–vDM/2
vDM/2
N
iLeakage
138 CHAPTER 5 CASCADE CONFIGURATION
As observed in the figures above, the leakage current varies particularly with
𝑣CM, or by using other words, iLeakage is a function of the common mode voltage given
by 𝑣CM = (q1 + q2)VPN∕2. From the Table presented in the sequence, it is quite clear
that if the modulation strategy selects only states 2 and 3, 𝑣CM is always equal to
VPN∕2, which means constant voltage applied to the capacitor CPV and consequently
null circulating current (i.e., iLeakage = 0). The direct consequence of cancelling iCM
is that the number of levels at the output converter side will be two, instead of three.
See Table 5.1 as well as Fig. 5.3.
State q1 q2 𝑣CM
1 0 0 0
2 0 1 VPN∕2
3 1 0 VPN∕2
4 1 1 VPN
Example 5.2
For the H-bridge topology shown in Fig. 5.4(a) with Vdc = 600V, ma = 0.6,
switching frequency: 1950 Hz and 𝑣∗
sin
= 180 sin(2𝜋50t), calculate the root
mean square (RMS) values of the fundamental and most important harmonics
(with at least 10% of the amplitude of the biggest harmonic) for the pole
voltage 𝑣10 assuming Method 2 in Fig. 5.5.
Solution
The amplitude of the fundamental and harmonics can be obtained from the
figure below that shows the relationship between V10(h)∕(Vdc∕2) and the har-
monics.
0.13
1.00
0.13
0.07
0.37 0.37
0.07 0.04 0.04
0.08
0.20
0.20
0 0 0 0 0
0
ma=0.6 mf>21
1 Harmonic
mf–4
2mf–5 2mf+5
2mf+3
2mf–3
2mf+1
3mf+4
3mf–4
3mf–6 3mf+6
3mf–2 3mf+2
3mf
2mf–1
mf+4
mf–2 mf+2
mf
0.60
v10
So, the amplitude of the harmonic hV10(h) is given by
V10(h) =
(
V10(h)
Vdc∕2
)
Vdc
2
The RMS value can be obtained directly as follows:
V10(h)RMS
=
1
√
2
(
V10(h)
Vdc∕2
)
Vdc
2
5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 139
Since ma = 0.6 and mf = ft∕fsin = 1950∕50 = 39, it is possible to
write:
h = 1 → V10(1)RMS
= 1
√
2
⋅ 0.6 ⋅ 600
2
= 127V
h = 39 → V10(39)RMS
= 1
√
2
⋅ 1 ⋅ 600
2
= 212V
h = 37, 41 → V10(37,41)RMS
= 1
√
2
⋅ 0.13 ⋅ 600
2
= 27V
h = 77, 79 → V10(77,79)RMS
= 1
√
2
⋅ 0.37 ⋅ 600
2
= 78V
h = 115, 119 → V10(115,119)RMS
= 1
√
2
⋅ 0.2 ⋅ 600
2
= 42V
All the other harmonics will not be considered since their amplitude is
less than 10%.
Example 5.3
Determine the RMS voltage value for the fundamental and for the harmonic
number 39 of the output voltage assuming the conditions of the last example;
assume both PWM strategies shown in Figs 5.4 and 5.5(b).
Solution
Since the output voltage of the PWM approach shown in Fig. 5.4 has the same
shape of the pole voltage [see Fig. 5.4(b)] it is possible to keep using the tem-
plate furnished in the figure
V10(h)
Vdc∕2
versus harmonics. However, the RMS values
are given by
Vo(h) =
(
V10(h)
Vdc∕2
)
Vdc
h = 1 → Vo(1)RMS
= 1
√
2
⋅ 0.6 ⋅ 600 = 254V
h = 39 → Vo(39)RMS
= 1
√
2
⋅ 1 ⋅ 600 = 424V
On the other hand, for the PWM technique given in Fig. 5.5(b) the out-
put voltage presents a different shape from the pole voltage, which means
that it is possible to use the template in figure V10(h)∕(Vdc∕2) versus harmon-
ics. Although 𝑣o has three levels instead of two, the fundamental component
(h = 1) should be the same as for the PWM in Fig. 5.3 since in both cases the
converter is operating under the same conditions in terms of Vdc, ma, and mf .
Then: h = 1 → Vo(1)RMS
= 254V.
For the harmonic 39, it turns out that Vo(39)RMS
= 0, [see Fig. 5.6(a)].
140 CHAPTER 5 CASCADE CONFIGURATION
Exercise 5.2
Repeat Examples 5.1 and 5. with ma = 1.0 instead of 0.6. The other operation
conditions are the same as in the previous examples.
5.4 THREE-PHASE CONVERTER—ONE H-BRIDGE
CONVERTER PER PHASE
A three-phase configuration by using one H-bridge converter per phase is depicted in
Fig. 5.7(a). It is worth mentioning that both converter and three-phase load are con-
nected in a Y arrangement. The converter pole voltages can be written as a function
of the states of switches, as follows:
𝑣a0 = (q1a − q2a)Vdc (5.8)
𝑣b0 = (q1b − q2b)Vdc (5.9)
𝑣c0 = (q1c − q2c)Vdc (5.10)
Considering a balanced three-phase system, it turns out that the voltage between
the neutral of the load and the point “0” is given by
𝑣n0 =
Vdc
3
(q1a − q2a + q1b − q2b + q1c − q2c) (5.11)
Compiling equations (5.8)–(5.11), it is possible to write the load voltages 𝑣an,
𝑣bn, and 𝑣cn in a matrix representation, as shown below:
⎡
⎢
⎢
⎣
𝑣an
𝑣bn
𝑣cn
⎤
⎥
⎥
⎦
= Vdc
⎡
⎢
⎢
⎢
⎢
⎢
⎢
⎣
2
3
−2
3
−1
3
−1
3
1
3
2
3
−1
3
1
3
−1
3
1
3
−1
3
1
3
−2
3
−1
3
1
3
1
3
2
3
−2
3
⎤
⎥
⎥
⎥
⎥
⎥
⎥
⎦
⎡
⎢
⎢
⎢
⎢
⎢
⎢
⎣
q1a
q2a
q1b
q2b
q1c
q2c
⎤
⎥
⎥
⎥
⎥
⎥
⎥
⎦
(5.12)
The power converter constituted by the arrangement of H-bridges topologies,
as in Fig. 5.7(a) allows different connections for the H-bridge converters. Such a
characteristic is not observed for the converters shown in the previous chapter. In fact,
for a given three-level NPC topology, different arrangements can be addressed for the
load side with either Y or Δ connections of the three-phase load, but the connections
of the converter itself cannot be changed, since all legs are connected to the same
dc-link source. On the other hand, due to its modular feature, H-bridge converters
can be changed in order to deal with specific requirements. In this sense, Fig. 5.7(b)
5.4 THREE-PHASE CONVERTER—ONE H-BRIDGE CONVERTER PER PHASE 141
q1a
a
b
n
L R
L
0
(a) (b)
R
Vdc
va0
vb0
vc0
van
vbn
c
L R
vcn
vab
q1a
q2a q2a
q1b q1b
q2b q2b
q1c q1c
q2c q2c
q1a
n
L R
L R
Vdc
Vdc
Vdc
van
vbn
L R
vcn
q1a
q2a q2a
q1b q1b
q2b q2b
q1c q1c
q2c q2c
Figure 5.7 (a) Three-phase H-bridge configuration connected in a Y arrangement.
(b) Three-phase H-bridge configuration connected in a Δ arrangement.
shows a solution in which the converters are arranged in a Δ connection. There is
also a possibility to connect a three-phase load in Δ for the converters depicted in
Fig. 5.7(a) and 5.7(b).
Exercise 5.3
Fill a table to show the number of levels of the load phase voltage 𝑣an for both
topologies given in Fig. 5.7 as a function of the switching states.
To highlight the influence of the PWM strategies presented in Fig. 5.5
(Methods 1 and 2) for the three-phase configuration as in Figs 5.7(a), 5.8(a), 5.8(b)
show the waveforms related to Methods 1 and 2, respectively. In the three-phase
case, the waveforms for the line-to-line voltage obtained through Method 1 have
an interesting characteristic with the same d𝑣∕dt, while Method 2 presents a
line-to-line voltage with the levels not well defined as in Fig. 5.8(a). As a conse-
quence 𝑣an in Fig. 5.8(a) is closer to a sine waveform than in Fig. 5.8(b). Note that
Fig. 5.8(c) highlights the advantages of Method 1 with a voltage presenting the
same d𝑣∕dt.
142 CHAPTER 5 CASCADE CONFIGURATION
va0
va0
vab
vab
van
van
ia ib ic
vab
vab
ib ic
–200
0
200
–200
0
200
–50
1 1.025
(a)
(b)
(c)
1.05
1 1.025
Method 1
Method 2
Same
dv/dt
Different
dv/dt
1.05
0
50
–400
0
400
–200
0
200
–200
0
200
–50
0
50
–400
0
400
Figure 5.8 (from top to bottom) Voltages: 𝑣a0, 𝑣ab, and 𝑣an and load currents for (a)
Method 1, (b) Method 2, and (c) levels of line-to-line voltage.
5.4 THREE-PHASE CONVERTER—ONE H-BRIDGE CONVERTER PER PHASE 143
As described in the previous chapter, there is a possibility to supply a
three-phase load by using a converter able to supply only two phases, since the third
phase will be indirectly controlled, due to the redundancy inherent in the balanced
three-phase systems (ia + ib + ic = 0 and 𝑣a + 𝑣b + 𝑣c = 0).
Exercise 5.4
Assuming all possibilities in terms of converter and three-phase load connec-
tions as given in the table below, specify the switches of the converters in terms
of voltage and current requirement, assuming the same RL load and dc-link
voltage for all connections below. Also, disregard any safety margin while
specifying the components.
Converter Load
Connection Connection Figure
Y Y 5.7(a)
Δ Y 5.7(b)
Y Δ –
Δ Δ –
Figure 5.9(a) shows the configuration with only two H-bridges connected to
phases a and b, while Fig. 5.9(b) shows the waveforms related to this configuration.
This kind of topology seems to have low practical interest, but in a fault-tolerant
system it could be interesting due to its ability to maintain the three-phase voltage
applied to the load on the post-fault operation. In this scenario, the “healthy” config-
uration is changed to the post-fault one after fault identification in the third phase of
the converter.
The PWM control of the configuration presented in Fig. 5.9(a) needs to be
adapted. The amplitude of voltage applied to the load is reduced by
√
3 and its dis-
tortion harmonic increased. However, the converter is still able to supply a three-phase
load with balanced currents as in Fig. 5.9(b) with ia, ib, and ic having the same ampli-
tude and a phase shift equal to 120∘.
Exercise 5.5
Does the connection shown in Fig. 5.9 affect the number of levels of the load
phase voltage? To answer this question, write a table to show the load voltages
as a function of the switching states and compare with the results obtained in
Exercise 5.3.
144 CHAPTER 5 CASCADE CONFIGURATION
ia ib ic
vcn
vbn
van
1 1.025 1.05
0
200
–200
0
200
–200
0
200
–200
50
0
–50
q1a
R
a
b
c
L
R
L
R
L
van
vbn
vcn
Vdc
q1a
q2a q2a
q1b q1b
q2b q2b
(a)
(b)
Figure 5.9 (a) Configuration supplying only two phases of the three-phase load. (b) (from
top to bottom) 𝑣an, 𝑣bn, 𝑣cn, and load currents.
5.5 TWO H-BRIDGE CONVERTERS
Connecting H-bridge converters in series, as in Fig. 5.10(a), allows the generation
of voltage with a higher number of levels. Such a cascade converter is in fact a very
popular topology in high voltage motor drive applications, especially due to its mod-
ular characteristic.
As discussed previously, each H-bridge converter can generate a maximum of
three levels at its output, which means a maximum of nine levels at the output of two
connected H-bridges series. All levels are considered in Table 5.3 for each switch-
ing state. The levels are: {0, ±Va, ±Vb, −Va − Vb, −Va + Vb, Va − Vb, Va + Vb}.
Figure 5.10(b)–5.10(j) show the combination used to obtain each specific level at
the output converter side.
5.5 TWO H-BRIDGE CONVERTERS 145
va
vb
vo
(a)
va
vb
vo
(b)
va
vb
vo
(c)
va
vb
vo
(d)
va
vb
vo
(e)
va
vb
vo
(f)
va
vb
vo
(g)
va
vb
vo
(h)
va
vb
vo
(i)
va
vb
vo
(j)
Figure 5.10 (a) Two H-bridges configuration with PBs. (b) 𝑣o = Va + Vb. (c)
𝑣o = −Va − Vb. (d) 𝑣o = Va − Vb. (e) 𝑣o = −Va + Vb. (f) 𝑣o = Va. (g) 𝑣o = −Va. (h) 𝑣o = Vb.
(i) 𝑣o = −Vb. (j) 𝑣o = 0.
From the expression for the output voltage of one H-bridge converter given in
(5.5), the output voltage 𝑣o of the converter presented in Fig. 5.10(a) can be written
as a function of the binary variables presented in Table 5.3, as follows:
𝑣o = (q1a − q2a)Va + (q1b − q2b)Vb (5.13)
146 CHAPTER 5 CASCADE CONFIGURATION
TABLE 5.3 Table of Variables for the Converter in Fig. 5.10
State q1a q2a q1b q2b 𝑣o
1 0 0 0 0 0
2 0 0 0 1 −Vb
3 0 0 1 0 Vb
4 0 0 1 1 0
5 0 1 0 0 −Va
6 0 1 0 1 −Va − Vb
7 0 1 1 0 −Va + Vb
8 0 1 1 1 −Va
9 1 0 0 0 Va
10 1 0 0 1 Va − Vb
11 1 0 1 0 Va + Vb
12 1 0 1 1 Va
13 1 1 0 0 0
14 1 1 0 1 −Vb
15 1 1 1 0 Vb
16 1 1 1 1 0
Although it is possible to generate nine levels at the output of the converter in
Fig. 5.10, this section will start with the analysis to obtain five levels followed by
seven and nine.
Example 5.4
What should be the relationship between Va and Vb to reach the maximum nine
levels (the maximum number of levels) at the output converter side?
Solution
To generate the maximum number of levels at the output converter side it is nec-
essary to guarantee either V1 = 3V2 or V2 = 3V1. Other numbers of levels can
be obtained with other relationships of the input voltages. For instance, seven
levels is obtained with V1 = 2V2 or V2 = 2V1, while five levels is obtained with
V1 = V2.
5.6 PWM IMPLEMENTATION OF TWO CASCADE
H-BRIDGES
PWM control strategies are also employed for a converter with two cascade H-bridge
topology to guarantee controlled voltage and frequency at its output. Since there
5.6 PWM IMPLEMENTATION OF TWO CASCADE H-BRIDGES 147
are more switches to generate the desired output voltage as compared to the single
H-bridge topology, it is also expected to have ways to implement the PWM strategies.
This section explores some of these PWM approaches.
Figure 5.11 shows the analog solution with phase shift multicarrier modulation
technique, in which the states of the eight switches are determined by a comparison
between two high frequency triangular waveforms (𝑣∗
t1
and 𝑣∗
t2
, carrier signals) and
two sinusoidal waveforms (𝑣∗
sin
and −𝑣∗
sin
, control signals) for the case where Va =
Vb = Vdc. The voltages 𝑣∗
t1
and 𝑣∗
t2
are shifted by 90∘. In this case the converter is
able to generate a five-level waveform at its output. As mentioned previously, the
(a)
(b)
driver
driver
driver
driver
90°
Phase
shift
driver
driver
driver
driver
+
–
+
+
+
1
0
–1
200
0
–200
–
–
–
q1a
q1a
q2a
q2a
q1a
q1a
q2a
q2a
q1b
q1b
q2b
q2b
q1b
q1b
q2b
q2b
vsin
*
vsin
*
vsin
*
–vsin
*
–vsin
*
vo
vt1
*
vt1
*
vt2
*
vt2
*
(a)
Figure 5.11 (a) PWM strategy with phase-shift method. (b) (top) PWM waveforms and
(bottom) output converter voltage.
148 CHAPTER 5 CASCADE CONFIGURATION
block named driver must guarantee the levels of voltage and current needed to operate
(turning on and off) the power switches adequately, as well as isolate the control
(signal) and the power circuits.
It is evident that the phase shift between 𝑣∗
t1
and 𝑣∗
t2
plays an important role in
the PWM approach as in Fig. 5.11. In fact, the influence of this parameter is depicted
in Fig. 5.12, which shows triangular (𝑣∗
t1
and 𝑣∗
t2
) and sinusoidal (𝑣∗
sin
) voltages (top);
load voltage (middle); and load current (bottom). The parameters employed in these
simulation results were: input voltage – Va = 100V and Vb = 100V; load – R = 5Ω
and L = 5mH; and switching frequency – 1kHz. Figure 5.12(a) shows those vari-
ables with phase shift between 𝑣∗
t1
and 𝑣∗
t2
equal to 0∘. Other phase shifts are consid-
ered, that is, 45∘, 90∘, and 180∘, as in Fig. 5.12(b), 5.12(c) and 5.12(d), respectively.
Considering the waveforms of the load voltage and load current, it is evident that 90∘
reduces the harmonic distortion for both voltage and current. Although changing the
high frequency components and consequently the THD of the variables, the phase
shift does not influence the value of voltage applied to the load.
In fact, the phase angle displacement of 90∘ between 𝑣∗
t1
and 𝑣∗
t2
guarantees an
optimum output voltage because it generates a sequence of switching states with the
(a) (b)
(c) (d)
1
–1
200
0
–200
50
0
–50
0
1
–1
200
0
–200
50
0
–50
0
1
–1
200
0
–200
50
0
–50
0
1
–1
200
0
–200
50
0
–50
0
Figure 5.12 Triangular (𝑣∗
t1
, 𝑣∗
t2
) and sinusoidal (𝑣∗
sin
) waveforms (top); load voltage
(middle); and load current (bottom): with phase shift of (a) 0∘, (b) 45∘, (c) 90∘, and
(d) 180∘.
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 149
vsin
*
–vsin
*
vt2
*
vt1
*
2Vdc
State 11 State 11
State 3 State 9 State 15 State 12
State 11 State 11 State 11
Vdc
Figure 5.13 Switching
states when 𝑣∗
sin
is in its
peak with 90∘of the phase
displacement between
𝑣∗
t1
and 𝑣∗
t2
.
levels well defined as in Fig. 5.8. For instance, during the peaks it is expected that the
output voltages change from Vdc to 2Vdc, while during the valleys the voltages should
change from −2Vdc to −Vdc. Figure 5.13 shows the sequence of the switching states
when 𝑣∗
sin
is around its peak. Since Va = Vb = Vdc, States 3, 9, 15, and 12 in Table 5.3
generate the same output voltage equal to Vdc. On the other hand, there is only one
way to generate 2Vdc, which is through State 11. Note that any other phase shift will
generate a sequence different from the one in Fig. 5.13.
Another way to implement the PWM strategy for the converter employing two
H-bridge cells in series is presented in Fig. 5.14. Such a technique is called level-shift
(or level dispositions), where all carrier signals are in phase but with different offsets.
For a symmetrical (same dc-link voltages) cascade multilevel converter, the
quantity of the carrier signals is defined by the number of levels desired at the output
converter side, that is, for N levels (N − 1) triangular carriers are required.
Figure 5.15 shows a comparison between two-level shift PWM approaches.
Note that other outcomes are obtained when all triangular carriers have the same
peak-to-peak voltage, but there is a phase shift of 180∘ between any two adjacent
carrier waves.
5.7 THREE-PHASE CONVERTER—TWO CASCADE
H-BRIDGES PER PHASE
A three-phase configuration employing two H-bridge converters per phase is depicted
in Fig. 5.16(a), with both converter and load connected in a Y arrangement. The
waveforms associated with this configuration are depicted in Fig. 5.16(b). These load
voltages present high quality with reduced THD due to the high number of levels. The
PWM strategy employed in the results of Fig. 5.16 were obtained with the level shift
approach, as in Fig. 5.14.
The converter voltages can be written as a function of the states of switches, as
follows:
𝑣a0 = (q1a − q2a + q3a − q4a)Vdc (5.14)
𝑣b0 = (q1b − q2b + q3b − q4b)Vdc (5.15)
150 CHAPTER 5 CASCADE CONFIGURATION
driver
driver
driver
driver
+
–
+
–
q1a
q1a
q1a
q1a
q2a
q2a
q2a
q2a
driver
driver
driver
driver
q1b
q1b
q1b
q1b
q2b
q2b
q2b
q2b
vsin
*
vt1
*
vsin
*
vo
vt2
*
vt3
*
vt4
*
+
–
+
–
(a)
(b)
1
–1
100
0
–200
0
Figure 5.14 (a) PWM strategy with phase disposition (PD) method. (b) (top) PWM
waveforms and (bottom) output converter voltage.
𝑣c0 = (q1c − q2c + q3c − q4c)Vdc (5.16)
Considering a balanced three-phase system, the voltage between the neutral of
the load “n” and the point “0” is given by
𝑣n0 =
Vdc
3
c
∑
x=a
(q1x − q2x + q3x − q4x) (5.17)
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 151
(a) (b)
50
0
1 1.016
0
200
–200
0
1
–1
–50
50
0
1 1.016
0
200
–200
0
1
–1
–50
Figure 5.15 Comparison between two-level shift PWM techniques.
Compiling equations (5.14)–(5.17), and assuming a balanced scenario, it is
possible to write the load voltages 𝑣an, 𝑣bn, and 𝑣cn as a function of both switching
states and dc-link voltages.
As mentioned previously, one of the main advantages of the cascade configura-
tions is their modularity, which brings benefits in terms of fault tolerance capability.
The fault compensation is achieved by reconfiguring the power converter topology to
keep the system in operation, even with a different number of H-bridges per phase.
Figure 5.17(a) shows one phase of the three-phase converter as in Fig. 5.16(a) under
“healthy” operation and generating a five-level voltage at the output. For the sake
of illustration, let us assume that a fault occurs in the switch q1a, as highlighted in
Fig. 5.17(b). Such a fault can be characterized as either a permanent short-circuit [see
Fig. 5.17(c)] or a permanent open-circuit [see Fig. 5.17(d)]. The fault detection sys-
tem must be able to identify where the fault has occurred (determining which switch
is at fault), and also the type of fault (short- or open-circuit). Sometimes it is necessary
to use fuses to deal with the reconfiguration of the power converter, which will help
to isolate part of converter under fault. For simplification purposes, the fuse devices
are not presented in Fig. 5.17.
The first action to be taken for a short-circuit failure [Fig. 5.17(c)] in the switch
q1a is to keep the complementary switch q1a open. As a consequence, the voltage
generated at the output of this H-bridge converter 𝑣1a2a = 𝑣1a − 𝑣2a can assume only
two values 0 or Vdc, that is, 𝑣1a2a = {0, Vdc}. Another scenario is with an open-circuit
failure as shown in Fig. 5.17(d). In this case, the complementary switch q1a must be
on to avoid current discontinuity. Consequently, the voltage generated at the output of
this H-bridge converter can also assume only two values, that is, 𝑣1a2a = {0, −Vdc}.
Both cases of failure lead to a voltage generation at the output of the H-bridge under
fault with just one polarity: positive polarity {0, Vdc} for short-circuit failure and neg-
ative polarity {0, −Vdc} for open-circuit failure. This represents a restriction for the
amount of voltage generated by the phase under fault. However, a sinusoidal voltage
with smaller amplitude and only three levels {0, ±Vdc} can still be generated by these
two H-bridge converters in series.
Although the faults presented in Fig. 5.17, there are some failures that
damage the whole H-bridge converter. For example, it is quite common to have
152 CHAPTER 5 CASCADE CONFIGURATION
(a)
q1a
q1a
Vdc Vdc
q2a
q2a
q3a
q3a
q4a
q4a
q1b
q1b
Vdc Vdc
a
b
c
L R
L
n
R
L R
q2b
q2b
q3b
q3b
q4b
q4b
q1c
q1c
Vdc Vdc
q2c
q2c
q3c
q3c
q4c
q4c
van
vbn
vcn
(b)
200
–200
0
200
–200
0
200
–200
0
50
–50
0
1 1.025 1.05
van
vbn
vcn
ia ib ic
Figure 5.16 (a) Three-phase H-bridge configuration connected in a Y arrangement
(b) Voltages and currents.
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 153
(a)
(b)
(c)
(d)
q1a
q1a
2a
1a
a
0
Vdc Vdc
q2a
q2a
q3a
q3a
q4a
q4a
q1a
q1a
2a
1a
a
Permanent
short-circuit
Permanent
short-circuit
0
Vdc Vdc
q2a
q2a
q3a
q3a
q4a
q4a
q1a
q1a
2a
1a
a
0
+
–
Vdc Vdc
q2a
q2a
q3a
q3a
q4a
q4a
v1a2a
q1a
q1a
2a
1a
a
0
+
–
Vdc Vdc
q2a
q2a
q3a
q3a
q4a
q4a
v1a2a
Figure 5.17 (a) “Healthy”
operation for the leg of the
cascade topology. (b) Fault
occurring in the switch q1a.
(c) Short-circuit type of fault.
(d) Open-circuit type of fault.
154 CHAPTER 5 CASCADE CONFIGURATION
two switches inserted in the same package constituting a leg, and likely one
switch will be affected if a malfunction has happened to another switch in the
same leg. Another example of malfunction that deteriorates the whole H-bridge
cell (in terms of capacity to generate any voltage) is when a fault occurs in
the dc-link. There is no way to generate any desired voltage at the output of
any H-bridge without dc-link voltage. The fault compensation when the entire
H-bridge is suffering from a fault is achieved by reconfiguring the power converter
topology along with additional devices, such as triacs, as shown in Fig. 5.18(a).
The triacs t1 and t2 are open under “healthy” operation and must be turned on
if a fault is detected, to isolate the whole H-bridge under fault. Figure 5.18(b)
shows the post-fault topology with the H-bridge converter isolated by using the
triac t1.
The post-fault operation requires a new PWM approach to keep a set of bal-
anced three-phase voltages applied to the load. There exist different ways to generate
the PWM signals for the post-fault topology as in Fig. 5.18(b), since there are two
converters per phase (in phases b and c) and just one converter in the phase a to synthe-
size the desire three-phase load voltage. One possibility to maintain the three-phase
balanced voltage is to turn on the triacs t3 and t5 to make this topology equal to that
presented in Fig. 5.7(a). This means that the two H-bridge per phase configuration
will be changed to a single H-bridge per phase. Also the rated voltage is reduced to
half of the pre-fault operation. Another possibility is to keep the post-fault topology
as presented in Fig. 5.18(b), that is, phase a with one H-bridge and phases b and c
with two H-bridges. To guarantee a balanced three-phase voltage among the phases,
the modulation index for phases b and c should be reduced to 50% of the modulation
index employed for phase a.
Exercise 5.6
Determine the number of levels of the post-fault topology in Fig. 5.18(b) con-
sidering the case in which the modulation index for phases b and c is reduced
by 50%.
As done before, the connection of the converters can be changed in order
to deal with specific requirements of the load. For instance, Fig. 5.19 shows a
solution in which the converters are arranged in a Δ connection. There is also
a possibility to connect a three-phase load in the Δ connection.
If the three-phase load is an electrical machine, it is also possible to connect
this machine with an open-end winding arrangement as seen in Fig. 5.20. Open-end
winding motor structure is obtained by opening the neutral point of the conventional
induction or synchronous machine and does not require any design change for the
machine itself. In fact, a three-phase machine with six terminals available is needed.
In this case the model of the converter is given by
𝑣a1n1 = (q1a − q2a)Vdc (5.18)
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 155
(a)
q1a
q1a
2a
1a
a
0
Vdc Vdc
q2a
q2a
t1 t2
q3a
q3a
q4a
q4a
(b)
q1b
q1b
b
L R
L R
n
0
Vdc Vdc
q2b
q2b
t3
t4
q3b
q3b
q4b
q4b
a
Vdc
t2
q3a
q3a
q4a
q4a
q1c
q1c
c
Vdc Vdc
q2c
q2c
t5
t6
q3c
q3c
q4c
q4c
van
vbn
L R
vcn
Figure 5.18 (a) Fault-tolerant converter with triacs. (b) Post-fault topology.
156 CHAPTER 5 CASCADE CONFIGURATION
a
L R
n
Vdc
q1a
q1a
q2a
q2a
Vdc
q3a
q3a
q4a
q4a
van
b
L R
Vdc
q1b
q1b
q2b
q2b
Vdc
q3b
q3b
q4b
q4b
vbn
c
L R
Vdc
q1c
q1c
q2c
q2c
Vdc
q3c
q3c
q4c
q4c
vcn
Figure 5.19 (a) Three-phase with two H-bridges connected in Δ.
𝑣b1n1 = (q1b − q2b)Vdc (5.19)
𝑣c1n1 = (q1c − q2c)Vdc (5.20)
and
𝑣a2n2 = (q3a − q4a)Vdc (5.21)
𝑣b2n2 = (q3b − q4b)Vdc (5.22)
𝑣c2n2 = (q3c − q4c)Vdc (5.23)
Then the voltage applied to the machine’s phases are given by
𝑣a1a2 = 𝑣a1n1 − 𝑣a2n2 + 𝑣n1n2 (5.24)
𝑣b1b2 = 𝑣b1n1 − 𝑣b2n2 + 𝑣n1n2 (5.25)
𝑣c1c2 = 𝑣c1n1 − 𝑣c2n2 + 𝑣n1n2 (5.26)
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 157
(a)
(b)
a2
a1
b2
n2
n1
b1
c2
c1
200
0
–200
200
0
–200
200
0
–200
50
0
1 1.01 1.02 1.03 1.04 1.05
–50
Three-phase
machine
Vdc
q1a
q1a
q2a
q2a
Vdc
q3a
q3a
q4a
q4a
Vdc
q1b
q1b
q2b
q2b
Vdc
q3b
q3b
Phase 1
Phase 2
Phase 3
q4b
q4b
Vdc
q1c
q1c
q2c
q2c
Vdc
q3c
q3c
q4c
q4c
Figure 5.20 (a) Motor drive system with open-end winding topology. (b) Voltages
and currents.
158 CHAPTER 5 CASCADE CONFIGURATION
with 𝑣n1n2 given by
𝑣n1n2 = 𝑣a1n1 + 𝑣b1n1 + 𝑣c1n1 − 𝑣a2n2 − 𝑣b2n2 − 𝑣c2n2 (5.27)
The open-end winding arrangement of the three-phase machine allows another
series connection of the converter, as presented in Fig. 5.21(a). This is a three-phase
motor drive system employing two three-leg inverters. Since the three-phase machine
is in series with both converters, this is also considered a series connection arrange-
ment among converters and machine. One of the advantages of the system presented
in Fig. 5.21(a) is its fault tolerance capability. Two cases can be considered:
Case I. The fault compensation is achieved by reconfiguring the power con-
verter topology without any additional devices such as triacs. The post-fault
configuration guarantees a Y connection of the motor.
Case II. The fault compensation is achieved by reconfiguring the power con-
verter topology with devices such as triacs. The post-fault configuration
guarantees a delta connection of the motor.
Both fault-tolerant strategies (Cases I and II) are based on the open-end winding
machine and can be compensated for (i) dc-link capacitor failure; (ii) short-circuit
failure; and (iii) open-circuit failure of the power switches. As previously presented,
fault compensation is achieved by reconfiguring the power converter topology when
a failure is detected.
Vdc
q1a
Fuse
Inverter 1
01
q1b
1b
1a
1c
q1c
q1a q1b q1c
ia ib ic
va vb vc
Vdc
q2a
Fuse
Inverter 2
(a) (b)
02
q2b
2b
2a
2c
q2c
+ + +
– – –
q2a q2b q2c
va
* vt1
*
va
vt2
*
Figure 5.21 (a) Pre-fault configuration—open-end winding motor drive system. (b) PWM
waveforms (top) and motor phase voltage (bottom).
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 159
A modulator with two carriers can be used for the PWM generation of the
“healthy” open-end winding motor drive system [Fig. 5.21(a)], as observed in
Fig. 5.21(b). The comparison between 𝑣∗
a and 𝑣∗
t1
defines the state of the switch q1a,
while the comparison between 𝑣∗
a and 𝑣∗
t2
defines the state of the switch q2a. Each
inverter also has a fuse for isolation purposes. As seen in Fig. 5.21(b) the motor
phase voltage (𝑣a) has also multilevel characteristics.
For Case I, the reconfiguration approach is obtained by using the other power
switches not affected by the fault to create a neutral for the machine. Figure 5.22(a),
5.22(b), and 5.22(c) show the procedure to create a post-fault configuration in the
case of open-circuit failure, short- circuit failure, and dc-link failure, respectively.
Note that, in the case of dc-link failure, the creation of the neutral of the machine
can be accomplished by either upper or lower switches of the converter under
fault. In this strategy (Case I) the motor voltage value after the fault is reduced
by 50%.
Open-circuit failure
Short-circuit failure
Fuse Fuse
Fuse
Fuse
Y connection
Y connection
Fuse
Fuse
Fuse
(a)
(b)
Figure 5.22 Post-fault configuration for: (a) open-circuit failure, (b) short-circuit failure,
and (c) dc-link failure.
160 CHAPTER 5 CASCADE CONFIGURATION
DC-link failure
Fuse
Fuse
Fuse
Fuse
Y connection
(c)
Figure 5.22 (Continued).
On the other hand, for Case II, the fault compensation is achieved by reconfig-
uring the power converter topology along with reconfiguration devices (triacs). The
pre-fault configuration is depicted in Fig. 5.23(a). In order to increase the voltage
applied to the machine, the reconfiguration approach aims to guarantee a delta con-
nection of the motor after the fault. Two actions must be managed by the control
system: isolate the source of the converter under fault and turn on all triacs, as depicted
in Fig. 5.23(b). Despite using more devices (three triacs – ta, tb, and tc) than the solu-
tion presented in Case I, the values for the motor phase voltage after the fault are
reduced by just 13.4%, due to the Δ connection.
Fuse
q1a
1a
1b
1c
Vdc
01
q1b
q1c
q1a
q1b
q1c
Inverter 1
Inverter 2
(a)
Fuse
q2a
2a
2b
2c
Vdc
02
q2b
q2c
q2a
q2b
q2c
ia ib ic
ta tb tc
va vb vc
+ + +
– – –
Figure 5.23 Fault-tolerant strategy—Case II. (a) Pre-fault configuration. (b) Fault
reconfiguration procedure to make a delta connection of the machine considering a
short-circuit failure.
5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 161
Delta
connection
Source
isolation
Fuse Fuse
Fuse
(b)
Figure 5.23 (Continued).
(a)
(b)
vb
*
va
*
PWM
Inverter 1
Three-phase
open-end
winding
machine
Inverter 2
vc
*
Fault
detection
vb
*
va
*
PWM
Inverter 1
Three-phase
open-end
winding
machine
Inverter 2
vc
*
Fault
detection
Figure 5.24 Control block diagram. (a) Case I. (b) Case II.
162 CHAPTER 5 CASCADE CONFIGURATION
(a)
(b)
v
a
(V)
50
–50
0.05 0.06 0.07 0.08
Fault Reconfiguration
0.09 0.1 0.11 0.12 0.13 0.14 0.15
0
i
a,
i
b,
i
c
(A)
50
–50
0.05 0.06 0.07 0.08
Fault
t (s)
Reconfiguration
0.09 0.1 0.11 0.12 0.13 0.14 0.15
0
v
a
(V)
50
–50
0.05 0.06 0.07 0.08
Fault Reconfiguration
0.09 0.1 0.11 0.12 0.13 0.14 0.15
0
i
a,
i
b,
i
c
(A)
50
–50
0.05 0.06 0.07 0.08
Fault
t (s)
Reconfiguration
0.09 0.1 0.11 0.12 0.13 0.14 0.15
0
Figure 5.25 Motor phase voltage (top) and current (bottom) with a fault occurring at
t = 0.1 s. (a) Case I and (b) Case II.
Figure 5.24 shows a simplified schematic of the control strategy for Cases
I and II. The fault can be identified by comparing the reference voltage with the
measured ones. After the fault occurrence, the reconfiguration procedure changes
from the open-end winding motor (“healthy” configuration) to a post-fault converter.
Figure 5.25 shows simulated results with a fault (open-circuit failure) occurring in
switch q2b at t = 0.1s. The variables in this figure are motor phase voltage (𝑣a) and
motor currents (ia, ib, and ic). Figure 5.25(a) shows the results for Case I, while
Fig. 5.25(b) shows the results for Case II. In this case, the switching frequency was
2 kHz and the dc-link voltage of each dc source was 50 V.
5.8 TWO H-BRIDGE CONVERTERS (SEVEN- AND
NINE-LEVEL TOPOLOGIES)
The PWM approach previously presented for two H-bridge converters connected in
series generates the gating signals to guarantee a five-level voltage at the output of the
converter. Such a converter structure is also known as symmetric cascade multilevel
5.8 TWO H-BRIDGE CONVERTERS (SEVEN- AND NINE-LEVEL TOPOLOGIES) 163
TABLE 5.4 Table of Variables for the Cascade Converter Operating with Seven Levels
State q1a q2a q1b q2b 𝑣o
1 0 0 0 0 0
2 0 0 0 1 −Vb
3 0 0 1 0 Vb
4 0 0 1 1 0
5 0 1 0 0 −2Vb
6 0 1 0 1 −3Vb
7 0 1 1 0 −Vb
8 0 1 1 1 −2Vb
9 1 0 0 0 2Vb
10 1 0 0 1 Vb
11 1 0 1 0 3Vb
12 1 0 1 1 2Vb
13 1 1 0 0 0
14 1 1 0 1 −Vb
15 1 1 1 0 Vb
16 1 1 1 1 0
inverter, since it uses the same dc-link voltages. An asymmetric cascade multilevel
inverter using unequal dc sources in each phase can be employed to generate either a
seven-level or a nine-level waveform.
From Table 5.3 and considering Va = 2Vb, it turns out that the number of lev-
els for 𝑣o will be seven: {0,±Vb,±2Vb,±3Vb}, as presented in Table 5.4. Note that
equation (5.28) describes the voltage at the output converter side as a function of the
switching states.
𝑣o = (2q1a − 2q2a + q1b − q2b)Vb (5.28)
Although increasing the number of levels, asymmetric cascade multilevel
inverters operate with switches dealing with different blocking voltages and also
require different dc-link voltages, which could restrict their applications.
A higher number of levels can be obtained when Va = 3Vb. Table 5.5 shows
nine levels for the output voltage as a function of the state of the switches. In this
case the nine levels are {0,±Vb,±2Vb,±3Vb,±4Vb}. Another possible restriction of the
unsymmetrical cascade multilevel topology is related to the lack of redundancy for
generation of each level. Such a redundancy brings a degree of freedom to optimize
the converter’s operation.
A comparison between Tables 5.4 and 5.5 shows the generation of the level 2Vb
is obtained with two switching states (States 9 and 12 in Table 5.4) for the seven-level
configuration, while the generation of the same level for a nine-level configuration is
done with just one switching state (State 10 in Table 5.5).
164 CHAPTER 5 CASCADE CONFIGURATION
TABLE 5.5 Table of Variables for the Cascade Converter Operating with Nine Levels
State q1a q2a q1b q2b 𝑣o
1 0 0 0 0 0
2 0 0 0 1 −Vb
3 0 0 1 0 Vb
4 0 0 1 1 0
5 0 1 0 0 −3Vb
6 0 1 0 1 −4Vb
7 0 1 1 0 −2Vb
8 0 1 1 1 −3Vb
9 1 0 0 0 3Vb
10 1 0 0 1 2Vb
11 1 0 1 0 4Vb
12 1 0 1 1 3Vb
13 1 1 0 0 0
14 1 1 0 1 −Vb
15 1 1 1 0 Vb
16 1 1 1 1 0
TABLE 5.6 Different Switching States to Generate the Same Output Level 2Vdc
State q1a q2a q1b q2b q1c q2c 𝑣o
1 1 0 1 0 0 0 2Vdc
2 1 0 1 0 1 1 2Vdc
3 1 0 1 1 1 0 2Vdc
4 1 0 0 0 1 0 2Vdc
5 0 0 1 0 1 0 2Vdc
6 1 1 1 0 1 0 2Vdc
5.9 THREE H-BRIDGE CONVERTERS
Multilevel configurations with three H-bridges can be obtained easily just
following the axioms and postulates of the power blocks geometry (PBG).
Figure 5.26(a) shows a single-phase topology with three H-bridges series connected.
Figure 5.26(b), 5.26(c), and 5.26(d) present three-phase solutions with H-bridges
Y-connected, Δ-connected, and with open-winding machine arrangement, respec-
tively. Figure 5.26(e) shows another possibility of connections with Δ arrangements
for the outer converters.
With the increase of the number of H-bridge cells, the number of switching
states and levels increases. For example, assuming that Va, Vb, and Vc have the same
value Vdc, there are six ways to generate the level 2Vdc, as presented in Table 5.6.
5.9 THREE H-BRIDGE CONVERTERS 165
(a)
(b)
(c)
(d)
(e)
Va
Vb
Vc
Va1
Vb1
Vc1
Va2
Vb2
Vc2
Va3
Vb3
Vc3
n
vo
1 2 3
Va1
Vb1
Vc1
Va2
Vb2
Vc2
Va3
Va1 Va2 Va3
Vb1
Three-phase
machine
Phase 1
Phase 2
Phase 3
Vb2 Vb3
Vc1 Vc2 Vc3
Va1 Va2 Va3
Vb1
Three-phase
machine
Phase 1
Phase 2
Phase 3
Vb2 Vb3
Vc1 Vc2 Vc3
Vb3
Vc3
1 2 3
Figure 5.26 Three H-bridge configuration: (a) single-phase, (b) three-phase Y-connected,
(c) three-phase Δ-connected, and (d) open-winding machine. (e) Δ connections for the outer
converters.
166 CHAPTER 5 CASCADE CONFIGURATION
(a)
(b)
200
0
–200
50
0
–50
300
0
–300
1
0
–1
0.03 0.05 0.07
0.055 0.06
200
0
–200
vo
vo
vsin
* vt1
* vt6
* vt3
* vt2
* vt5
* vt4
*
io
vsin
*
Figure 5.27 (a) Phase-shift modulation with (top) PWM signals, (middle) output voltage
and (bottom) output current. (b) Zoom of the PWM and output voltages.
In a general way, the output voltage of the three symmetrical H-bridge config-
uration can be written as
𝑣o = (q1a − q2a)Va + (q1b − q2b)Vb + (q1c − q2c)Vc (5.29)
Figure 5.27 shows the waveforms for the configuration in Fig. 5.26(a) supplying
a single-phase RL load. Figure 5.27(a) top presents the PWM signals with phase-shift
multicarrier modulation. Six triangular carrier signals (𝑣∗
t1
, 𝑣∗
t2
, 𝑣∗
t3
, 𝑣∗
t4
, 𝑣∗
t5
, and 𝑣∗
t6
)
are required since 7 levels are expected at the output. There is a phase shift between
any two adjacent carrier waveforms given by 360∘/(N – 1), where N is the number
of levels.
Figure 5.27(b) shows details (zoom) for the voltages presented in Fig. 5.27(a).
The control circuitries as well as the power part of the converter (with the power
switches) are presented in Fig. 5.28.
Note that the control waveforms (𝑣∗
sin
and 𝑣∗
t1
, 𝑣∗
t6
, 𝑣∗
t3
, 𝑣∗
t2
, 𝑣∗
t5
, 𝑣∗
t4
) and the ana-
log circuit as presented in Fig. 5.28 generate a desired sequence of pulses at the output
5.9 THREE H-BRIDGE CONVERTERS 167
driver
driver
driver
driver
driver
driver
driver
driver
driver
driver
driver
driver
+
+
–
–
+
–
+
–
q1a
q1a
q2c
q1b
q1a
q1a
q2a
q2a
q1b
q1b
q2b
q2b
q1c
q1c
q2c
q2c
q2c
q1b
q2a
q1c
q2b
q2a
q1c
q2b
vsin
*
vt1
*
vt6
*
vt3
*
vt2
*
+
–
+
–
vt5
*
vt4
*
Figure 5.28 Analog
control circuitries (left side)
and the power part of the
converter (right side).
voltage with seven levels, all of them with the same d𝑣∕dt. If another PWM signal is
employed (different from that presented in Fig. 5.27), changes are also expected in
the analog circuit solution. For example, Fig. 5.29 shows the level-shift multicarrier
PWM modulation for the three H-bridge converter with six triangular carrier signals
vertically disposed. In this case, all carrier signals are in phase with each other. Such a
technique is also known as in-phase disposition (IPD). In addition to the approach pre-
sented in Fig. 5.29 there are other possibilities: alternate phase opposite disposition
(APOD) and phase opposite disposition (POD). In the APOD approach all carriers
are alternately in opposite disposition, while for the POD all carriers below zero are
in phase, but in phase opposition with those above the zero axis.
Figure 5.30 shows the control and power part of the converter to generate a
seven-level output voltage as presented in Fig. 5.29. A direct comparison between
phase shift and level shift strategies (presented in Figs 5.27 and 5.29, respectively)
reveals that the phase shift approach has advantages in terms of reduced harmonic
distortions.
It is also possible to combine the solutions presented in Figs 5.27 and 5.29,
as presented in Fig. 5.31. Such a combination results in a phase shift and level shift
multicarrier approach.
168 CHAPTER 5 CASCADE CONFIGURATION
200
0
–200
50
0
–50
0.03 0.05 0.07
1
0
–1
vo
io
vsin
*
Figure 5.29 Level shift multicarrier modulation: (top) PWM signals (from top to bottom):
𝑣t1, 𝑣t3, 𝑣t5, 𝑣t6, 𝑣t4, and 𝑣t2. (middle) output voltage 𝑣o, and (bottom) output current io.
driver
driver
driver
driver
driver
driver
driver
driver
driver
driver
driver
driver
+
+
–
–
+
–
+
–
q1a
q1a
q1b
q1c
q1a
q1a
q2a
q2a
q1b
q1b
q2b
q2b
q1c
q1c
q2c
q2c
q1b
q1c
q2c
q2b
q2a
q2c
q2b
q2a
vsin
*
vt1
*
vt3
*
vt5
*
vt6
*
+
–
+
–
vt4
*
vt2
*
Figure 5.30 Analog control circuitries (left side) and the power part of the converter (right
side) for the level-shift modulation.
5.11 SUMMARY 169
200
0
–200
50
0
–50
0.03 0.05 0.07
1
0
–1
vo
io
vsin
*
Figure 5.31 Phase shift/level shift multicarrier modulation: (top) PWM signals: 𝑣t1, 𝑣t3, 𝑣t5,
𝑣t6, 𝑣t4, and 𝑣t2. (b) Output voltage 𝑣o, and (c) output current io.
5.10 FOUR H-BRIDGE CONVERTERS AND
GENERALIZATION
A converter with four H-bridges and also the generalization of the cascade converters
are presented in Fig. 5.32(a). Figure 5.32(b) shows another type of series connection
converter with a combination of the conventional three-phase converter and H-bridges
topologies.
5.11 SUMMARY
This chapter dealt with configurations and PWM techniques for connected H-bridge
converters series. After discussing the single-phase converter, the three-phase version
was presented using a single H-bridge converter per phase. Also, it was shown how to
increase the number of levels with two H-bridge converters connected in series, bring-
ing up the sequence given respectively by power converter construction, model, PWM
approach, and three-phase version. Different multicarrier based schemes were pre-
sented and various associated aspects discussed. For instance, the direct comparison
between phase shift and level shift strategies revealed that the phase shift approach
has advantages in terms of reduced harmonic distortions. One special issue treated
in this chapter was the possibility of guaranteeing post-fault operation with cascaded
H-bridge converters. In addition, it was shown that two H-bridge converters can be
employed to generate an output voltage with seven and nine levels, employing the
correct relationship between the dc-link voltages. Finally, different arrangements and
PWM solutions for three connected H-bridge converter series were introduced based
on the PBG approach. The chapter is enriched with Table of Variables and analog
control circuitries for most cases.
170 CHAPTER 5 CASCADE CONFIGURATION
a
L R
van
b
n
L R
vbn
c
L R
vcn
(b)
(a)
Figure 5.32 Four H-bridges and generalization. (b) Hybrid topology combining H-bridge
and conventional three-phase inverter.
REFERENCES
[1] L. M. Tolbert, F. Z. Peng, and T. G. Habetler, Multilevel converters for large electric drives, IEEE
Trans Ind Appl, vol. 35, no. 1, pp. 36–44, 1999.
[2] R. Rabinovici, D. Baimel, J. Tomasik, A. Zuckerberger, Series space vector modulation for
multi-level cascaded H-bridge inverters, IEE Proc IET, vol. 3, no. 10, pp. 843–857, 2010.
REFERENCES 171
[3] Rodriguez J, Hammond PW, Pontt JO, Musalem R, Escobar Mj. Operation of a medium-voltage
drive under faulty conditions. IEEE Trans Ind Electron 2005;52(4):1080–1085.
[4] Wu B. High Power Converters and AC Drives. New Jersey: John Wiley and Sons; 2006.
[5] J. Rodriguez, J. Lai and F. Z. Peng, Multilevel inverters: a survey of topologies, controls, and appli-
cations, IEEE Trans Ind Electron, 49, No. 4, 2002, 724–738.
[6] J Rodriguez, S. Bernet, Bin Wu, J. O. Pontt, S. Kouro, Multilevel voltage-source-converter topologies
for industrial medium-voltage drives, IEEE Trans Ind Electron, vol. 54, no. 6, pp. 2930–2945, 2007.
[7] Rashid MH. Power Electronics Handbook. New York: Academic; 2001.
[8] Peng FZ, Lai J-S. Multilevel cascade voltage source inverter with separate DC sources. US patent
5,642,275. Jun 1997.
[9] Hammond PW. Medium voltage PWM drive and method. US patent 5,625,545. Apr 1997.
[10] Corzine Keith, Familiant Yakov. A new cascaded multilevel H-bridge drive. IEEE Trans Power Elec-
tron, 2002, Vol. 17, No. 1, pp.125–131.
[11] Manjrekar MD, Lipo TA. Hybrid multilevel power conversion system: a competitive solution for
high-power applications. IEEE Trans Ind Appl 2000;36(3):834–841.
[12] Lund R, Manjrekar MD, Steimer P, Lipo TA. Control strategies for a hybrid seven-level Inverter,
Conference Record of EPE, pp. 1–10, 1999.
[13] Manjrekar MD, Lipo TA. A hybrid multilevel inverter topology for drive applications. IEEE APEC;
1998, 523–529.
[14] Carrara G, Gardella S, Marchenosi M, Salutari R, Sciutto G. A new multilevel PWM method:
a theoretical analysis. IEEE Trans Power Electron, July 1992;7:497–505.
CHAPTER 6
FLYING-CAPACITOR
CONFIGURATION
6.1 INTRODUCTION
A type of multilevel configuration known as flying capacitor (FC) converter is
presented in this chapter under powerblock geometry (PBG) point of view. The
introduction and fundamental concepts of configurations with three and more
levels employing a FC approach, as well as a detailed description of these circuits,
are addressed in this chapter. FC converters present higher degrees of freedom
(redundant states) to synthesize a specific output voltage and employ a lesser number
of semiconductor power devices than the neutral point clamped (NPC) topology.
Such redundant states are used to regulate the FC voltage. Unlike the cascade
configuration presented in Chapter 5, there is no need for isolated dc sources.
The main challenge of the FC configuration is to keep the FC voltage under a
desired level, avoiding distortion at the ac part of the converter. Part of this chapter will
be dedicated to discussing strategies to balance the FC voltage. For the sake of illustra-
tion, the analysis starts with the FC being substituted by a dc voltage source. A simple
pulse width modulation (PWM) approach is employed to generate a three-level out-
put voltage. It is demonstrated that the PWM approach affects the voltage ripple of
the FC voltage. In fact, there are different strategies to regulate the capacitor voltage,
which can be sorted into two main types: natural-balancing and active schemes. The
natural-balancing approach employs solutions in terms of PWM strategies without
any voltage and current sensors, while the active method employs feedback regula-
tion and control algorithms to maintain the voltage constant. It is worth mentioning
that different aspects affect the capacitor voltage balancing, for example, the type of
load (linear or nonlinear). This chapter is organized considering the number of levels
generated by each circuit, as done in Chapter 4 for NPC circuits.
Subsequent to this introduction, Section 6.2 presents the power blocks (PBs)
and the circuit with switches for the FC three-level topology, as also the model and
Table of Variables. Section 6.3 deals with a simple PWM strategy applied for the
three-level circuit. The FC voltage regulation is presented in Section 6.4. Sections 6.5
and 6.6 show the FC topologies for single-phase (full-bridge) and three-phase appli-
cations, respectively. Other circuits of three-phase converters appear in Section 6.7.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
172
6.2 THREE-LEVEL CONFIGURATION 173
Four-level topologies are considered in Section 6.8. Finally, Section 6.9 presents the
generalization and Section 6.10 summarizes this chapter.
6.2 THREE-LEVEL CONFIGURATION
The PBs, as described in the Chapter 3, can be connected in a systematic appro-
ach to guarantee the creation of FC multilevel configurations. An arrangement
using two PB-ac blocks is depicted in Fig. 6.1(a), which follows Postulate 2.
Figure 6.1(b)–6.1(e) shows the ways used to obtain each specific level at the output
converter side 𝑣o referred to as the point “0”, that is, V1, (V1 − V2), (V2 − V3), −V3,
respectively. Figure 6.1(c) and 6.1(d) illustrates that it is necessary to activate two
PBs to obtain 𝑣o = (V1 − V2) and 𝑣o = (V2 − V3), while 𝑣o = V1 and 𝑣o = −V3 are
obtained activating only one PB as in Fig. 6.1(b) and 6.1(e), respectively.
(a)
0
2
1
V1
V3
vo
V2
(b)
0
2
1
V1
vo
(c)
0
2
1
V1
V2
vo
(d)
0
2
1
V3
V2
vo
(e)
0
2
1
V3
vo
Figure 6.1 (a) Three levels FC configuration with PBs. Arrangement to obtain: (b) 𝑣o = V1.
(c) 𝑣o = V1 − V2. (d) 𝑣o = V2 − V3. (e) 𝑣o = −V3.
174 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
or
0
2
1
V1
vo
V2
0
2
1
V1
V1
–V3
t
vo
vo
0
2
1
V3
V2
vo
0
2
1
V3
vo
V1 – V3
2
Figure 6.2 Generation of a general three-level output voltage.
In general terms, to generate an output waveform with three levels it is nec-
essary to activate the PBs in a sequence as observed from the waveform of 𝑣o in
Fig. 6.2 (bottom). Since this is a three-level converter, V1 − V2 = V2 − V3, which
means V2 = (V1 + V3)∕2. It is worth emphasizing that with FC topology it is possi-
ble to generate the V2 level with two different circuit arrangements (i.e., topological
states), as observed in Fig. 6.2 (top). This is an important characteristic of the FC
topologies, which will be explored later in this chapter.
Since 𝑣o can assume just one voltage value V1, (V1 − V3)∕2 or −V3 at each
instant of time, it is possible to establish an equation to describe the output voltage
𝑣o as a function of the input voltages V′
1
, V′
2
, V′
3
[where V′
1
= V1, V′
2
= (V1 − V3)∕2,
and V′
3
= −V3] as well as a function of two independent binary variables (q1 and q2).
Following the same approach employed previously in this book, these binary vari-
ables define the states of the switches inside the blocks. In this sense, since there are
three inputs to be selected (V′
1
, V′
2
, and V′
3
), the minimum number of binary variables
employed to select those inputs is two. Considering that there are three input voltages
to be selected by using these binary variables, the output voltage can be obtained as
presented in Table 6.1.
6.2 THREE-LEVEL CONFIGURATION 175
TABLE 6.1 Table of Variables for the Converter in Fig. 6.1(a)
State q1 q2 𝑣o 𝑣o
1 0 0 −V3 V′
3
2 0 1
V1 − V3
2
V′
2
3 1 0
V1 − V3
2
V′
2
4 1 1 V1 V′
1
An equation used to describe the behavior presented in this table is given below:
𝑣o = q1q2V′
3
+ q1q2V′
2
+ q1q2V′
2
+ q1q2V′
1
(6.1)
where q1 = 1 − q1 and q2 = 1 − q2. In this case, (6.1) becomes
𝑣o = (1 − q1)(1 − q2)V′
3
+ (1 − q1)q2V′
2
+ q1(1 − q2)V′
2
+ q1q2V′
1
(6.2)
Normally, there are some requirements associated with total harmonic
distortion (THD) minimization for the output voltage, which ends up with a sym-
metrical waveform at the converter output, and consequently V′
1
= Vdc, V′
2
= 0, and
V′
3
= −Vdc. In this case it is possible to write equation (6.2) as follows:
𝑣o = (q1 + q2 − 1)Vdc (6.3)
The binary variables considered in Table 6.1 are in fact the switching states
inside the blocks, which means that the topology presented in Fig. 6.1 can be treated
at its lower level presentation (switches instead of blocks), as in Fig. 6.3.
Note that the FC configuration is bidirectional, which means that each voltage
value V′
1
, V′
2
, V′
3
can be obtained at the output converter side independent of the cur-
rent, that is, any desired output value is obtained for both cases io > 0 and io < 0, as
observed in Fig. 6.3.
(a) (b) (c) (d)
Vdc
Vdc
Vdc
q1
q2
io
q1
q2
Vdc
Vdc
Vdc
q1
q2
io
q1
q2
Vdc
Vdc
Vdc
q1
q2
io
q1
q2
Vdc
Vdc
Vdc
q1
q2
io
q1
q2
Figure 6.3 Generation of levels: (a) V′
1
, (b) and (c) V′
2
, and (d) V′
3
independent of the output
current.
176 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
Exercise 6.1
(a) Assuming the FC configuration with four independent switches (q1, q2, q3,
and q4) as presented below, fill the table below eliminating the prohibited states
caused by either undefined states (e.g., all switches off) or short-circuit of the
dc-link source (or FC). (b) Eliminate all undefined states in this table and find
a logic relationship among q1, q2, q3, and q4.
vo
Vdc
Vdc
Vdc
q1
q2
q3
q4
State q1 q2 q3 q4 𝑣o
1 0 0 0 0
2 0 0 0 1
3 0 0 1 0
4 0 0 1 1
5 0 1 0 0
6 0 1 0 1
7 0 1 1 0
8 0 1 1 1
9 1 0 0 0
10 1 0 0 1
11 1 0 1 0
12 1 0 1 1
13 1 1 0 0
14 1 1 0 1
15 1 1 1 0
16 1 1 1 1
6.3 PWM IMPLEMENTATION (HALF-BRIDGE TOPOLOGY) 177
6.3 PWM IMPLEMENTATION
(HALF-BRIDGE TOPOLOGY)
A desired output voltage with regulation of both voltage and frequency can be
obtained for the FC converter with PWM strategies. As considered for the other
topologies, such a strategy is able to synthesize a square waveform with an average
value (at the switching frequency) equal to a sinusoidal waveform.
Figure 6.4 shows one possible analog solution for the PWM implementation
known as level-shift, in which the states of the four power switches are determined
by a comparison among two high frequency triangular waveforms (𝑣∗
t1
and 𝑣∗
t2
)
and a sinusoidal waveform (𝑣∗
sin
). The block marked “driver” must guarantee the
(a) (b)
(c)
(d)
driver
driver
1
0
1
0
1
0
0.2 0.225 0.25
–1
+
–
q1
q1
q2
q1
q1
q2
vsin
*
vt1
*
vt1
*
driver
driver
+
–
q1
q2
q1
q2
vsin
*
vsin
*
1
0
1
0
1
0
0.2 0.225 0.25
–1
q2
q2
vt2
*
vsin
*
vt2
*
Figure 6.4 (a) PWM generation for switches q1 and q1. (b) PWM generation for switches q2
and q2. (c) Variables associated with switches q1 and q1 (from top to bottom) – reference
voltages, gating signals of switches q1 and q1. (d) Variables associated with switches q2 and
q2 (from top to bottom) – reference voltages, gating signals of switches q2 and q2.
178 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
levels of voltage and current at the gate circuit needed to operate the power switches
adequately.
Note that when the switches q1 and q1 are in operation (on and off during the
positive half cycle of 𝑣∗
sin
) the switch q2 is on and consequently the switch q2 is off
for the whole half period. This is equivalent to states 2 and 4 in Table 6.1, which
generates the levels V′
2
and V′
1
, respectively. On the other hand, on the negative half
cycle of 𝑣∗
sin
, when the switches q2 and q2 are in operation (alternating on and off)
the switch q1 is off and consequently the switch q1 is on. This is equivalent to states
1 and 2 in Table 6.1, which generates the levels V′
3
and V′
2
, respectively.
The PWM presented in Fig. 6.4(a) is able to generate the output voltage with
the desired number of levels (V′
1
, V′
2
, and V′
3
) using such a simple implementation.
However, State 3 in Table 6.1 has not been used in this simple strategy, which means
that there is still a degree of freedom to be explored, as seen in the following sections.
Figure 6.5(a) shows the half-bridge three-level configuration, in which the
load is connected between the dc-link mid-point and the center point of the leg.
Figure 6.5(b) depicts (from top to bottom) PWM reference waveforms, gating signals
of switches q1 and q2, load voltage, and load current, respectively. The parameters
employed in these simulation tests were: Vdc = 200 V, R = 5 Ω, and L = 5 mH, and
switching frequency equal to 500 Hz.
(a)
(b)
vo
io
vt1
*
vt2
*
vsin
*
0.2 0.225 0.25
0
200
–200
0
0
0
1
1
–1
1
50
0
–50
q1
q2
q1
L
R
+ –
vo
io
Vdc
Vdc
Vdc
q2
q2
q1
Figure 6.5 (a) Three-level FC half-bridge converter. (b) (from top to bottom) 𝑣∗
sin
, 𝑣∗
t1
, 𝑣∗
t2
;
gating signal of switch q1; gating signal of switch q2; load voltage and load current.
6.4 FLYING CAPACITOR VOLTAGE CONTROL 179
6.4 FLYING CAPACITOR VOLTAGE CONTROL
In order to simplify the analysis of an FC converter, the FC was substituted by a dc
voltage source, as in Fig. 6.5(a). However, in practical circuits the center dc voltage
source in Fig. 6.5(a) is replaced by a capacitor, as in Fig. 6.6(a). In this case, it is
necessary to guarantee the control voltage of this capacitor.
For example, if the level-shift PWM approach presented in Fig. 6.4 is applied
to the half-bridge converter presented in Fig. 6.6(a), the results for the capacitor vari-
ables (𝑣C and iC) are as presented in Fig. 6.6(b). Even with the average value of 𝑣C
equal to 200 V (as desired), there are variations for the voltage 𝑣C which will bring
up low frequency distortion at the output converter side.
From the node between the switches q1 and q2 in Fig. 6.6(a) it is possible to
determine the capacitor current as follows: iC = iq1 − iq2, and assuming the level-shift
modulation approach, it can be seen that:
When 𝑣∗
sin
> 0:
q2 = 1
iq2 = io
iq1 = q1io
∴iC = (q1 − 1)io
(a)
(b)
vC
vC
iC
io
vt1
*
vt2
*
vsin
*
vsin
*
1.01
1 1.02
0
200
150
250
50
0
0
1
1
–1
1
–50
q1
q2
q1
L
R
+ –
vo
io
Vdc
Vdc
q2
q2
q1
Figure 6.6 (a) Half-bridge
converter with flying
capacitor. (b) Control and
power variables for the
half-bridge circuit with
level-shift PWM.
180 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
When 𝑣∗
sin
< 0:
q1 = 0
iq1 = 0
iq2 = q2io
∴iC = −q2io
From the current iC obtained previously, it is possible to determine directly the
capacitor voltage, since: 𝑣C = 1
C
∫ iCdt.
Exercise 6.2
In order to deeply understand the mechanism behind the FC voltage control,
draw the topological states considering the switching signals and capacitor
waveforms in steady-state operation for the circuit in Fig. 6.6(a), as highlighted
below. Consider each of the intervals of time below (from 1 to 17).
vC
iC
q1
q2
1 2
3 5 7 11
4 6 8 9
13 15
10 12 14 16 17
To guarantee the capacitor voltage control with reduced variation, another
PWM strategy can be considered, as seen in Fig. 6.7. A phase-shift has been
considered in this case, which leads to a capacitor charging and discharging at the
switching frequency. This plays an important role in keeping 𝑣C with reduced ripple.
The polarity of the capacitor current in Fig. 6.6(b) has changed with the sinusoidal
frequency, which increases the ripple for 𝑣C. Note from Fig. 6.6(b) that the FC is
discharged during the entire positive half of the sinusoidal voltage (𝑣∗
sin
) since iC is
either zero or negative. On the other hand, the FC during the negative half of the
sinusoidal voltage is charged because iC is either zero or positive.
6.5 FULL-BRIDGE TOPOLOGY 181
vC
iC
io
vt1
*
vt2
*
vsin
*
vsin
*
1.01
1 1.02
0
200
150
250
50
0
0
–1
1
–1
1
–50
q1
q2
Figure 6.7 Control and power waveforms for the half-bridge circuit with level-shift PWM.
On the other hand, in the PWM technique shown in Fig. 6.7, the charging/
discharging occurs on the switching frequency; this keeps the capacitor voltage ripple
smaller.
The PWM techniques able to reduce the ripple on the FC are fundamental for
reducing the distortion of the output voltages. Figure 6.8(a) and 6.8(b) shows the load
voltage for the level-shift and phase-shift approaches, respectively. Figure 6.9 in turn
shows the start-up transient for the FC voltage.
6.5 FULL-BRIDGE TOPOLOGY
Full-bridge three-level FC converters for both single-phase and three-phase loads are
obtained by connecting the blocks in Fig. 6.1 as observed in Figs 6.10(a) and 6.10(b),
respectively. Figure 6.10(c) shows the option in which the three-phase four-wire sys-
tem is required.
The full-bridge single-phase three-level FC converter is presented in
Fig. 6.11(a) by using switches instead of blocks (lower level representation).
Figure 6.11(b) shows (from top to bottom) pole voltage of the first leg (with switches
q1a and q2a), pole voltage of the second (with switches q1b and q2b), load voltage,
and load current, respectively.
Comparing the load voltage in Figs 6.5(b) and 6.11(b), it is quite clear that the
increased number of levels observed in the load voltage of the full-bridge topology
guarantees the ripple reduction of the current and consequently a better quality of the
voltage delivered by the converter.
In this case the output voltage is given by
𝑣o = (q1a + q2a − q1b − q2b)Vdc (6.4)
182 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
(a)
(b)
vo
250
0
–250
1 1.025 1.05
vo
250
0
–250
1 1.025 1.05
Figure 6.8 Influence of the PWM technique for distortion reduction at the output voltage.
vC
200
100
0
0 3 6
Figure 6.9 Start-up transient for
the flying capacitor voltage (𝑣C).
As mentioned previously, the number of levels considered in this chapter is
defined by the voltage between the midpoint of the leg and the dc-link midpoint,
that is, through the pole voltage. For instance, both converters in Figs 6.6 and 6.11
are considered as single-phase three-level FC configurations, even though the load
voltage in the full-bridge topology presents five levels.
6.6 THREE-PHASE FC CONVERTER 183
(a)
0
1
2
Vdc
a
b
Vdc
(b)
0
1
2
Vdc
a
b
c
Vdc
(c)
0
1
2
Vdc
a
b
c
d
Vdc
Figure 6.10 (a) Single-phase full-bridge three-level FC converter. (b) Three-phase
full-bridge three-level FC converter. (c) Three-phase four-wire three-level FC converter.
6.6 THREE-PHASE FC CONVERTER
A three-phase three-level FC configuration is depicted in Fig. 6.12(a), while
Fig. 6.12(b) shows some variables associated with this converter, that is, (from top to
bottom) pole voltage, voltage between the load neutral point and dc-link mid-point
connection, load phase voltage, and load current, respectively.
The pole voltages for the three-phase converter can be written as follows:
𝑣a0 = (q1a + q2a − 1)Vdc (6.5)
𝑣b0 = (q1b + q2b − 1)Vdc (6.6)
𝑣c0 = (q1c + q2c − 1)Vdc (6.7)
Considering a balanced three-phase load, the voltage 𝑣n0 can be defined ana-
lytically by
𝑣n0 =
Vdc
3
(q1a + q2a + q1b + q2b + q1c + q2c) − Vdc (6.8)
From (6.8), and considering all 64 switching states, the voltage 𝑣n0 depicted
in Fig. 6.12(b) is responsible for increasing the number of levels in 𝑣an. The phase
184 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
io
vo
vb0
va0
0.225
0.2 0.25
200
–200
200
–200
500
–500
100
–100
q1a
L
R
a
b
0
+ –
vo
io
Vdc
Vdc
q2a
q2a
q1a
q1b
q2b
q2b
q1b
(a)
(b)
Figure 6.11 (a) Three-level NPC full-bridge converter. (b) (from top to bottom) pole voltage
of the first leg (q1a and q2a), pole voltage of the second (q1b and q2b), load voltage, and load
current.
voltage for each phase of a balanced three-phase load is given by
𝑣a =
(
2
3
q1a +
2
3
q2a −
1
3
q1b −
1
3
q2b −
1
3
q1c −
1
3
q2c
)
Vdc (6.9)
𝑣b =
(
−
1
3
q1a −
1
3
q2a +
2
3
q1b +
2
3
q2b −
1
3
q1c −
1
3
q2c
)
Vdc (6.10)
𝑣c =
(
−
1
3
q1a −
1
3
q2a −
1
3
q1b −
1
3
q2b +
2
3
q1c +
2
3
q2c
)
Vdc (6.11)
In this case (balanced three-phase load) the load voltages depend only on state
of the switches and dc-link voltage.
Notice that the control circuit is obtained as seen in Fig. 6.4, replicating the
PWM control for the other two phases with the following sinusoidal references:
𝑣∗
sin 1
= Vp sin(𝑤t), 𝑣∗
sin 2
= Vp sin(𝑤t + 120∘), and 𝑣∗
sin 3
= Vp sin(𝑤t + 240∘), where
Vp is the peak voltage desired for the load.
6.6 THREE-PHASE FC CONVERTER 185
ia
van
vn0
va0
0.225
(a)
(b)
0.2 0.25
500
–500
0
500
–500
0
500
–500
0
100
–100
0
q1a
n
a
b
c
0
+ –
vc
ic
+ –
vb
ib
+ –
va
ia
Vdc
Vdc
q2a
q2a
q1a
q1b
q2b
q2b
q1b
q1c
q2c
q2c
q1c
Figure 6.12 (a) Three-level NPC converter. (b) (from top to bottom) pole voltage, voltage
𝑣n0, load voltage and load current.
Figure 6.13(a) shows the same power converter topology supplying a
three-phase load connected in Δ arrangement. The way the load is connected to the
FC topology plays an important role for the converter’s design and specification.
Figure 6.13(b) shows the impact of the load’s connection (i.e., Δ or Y) on the FC
voltage ripple of the phase a (𝑣Ca) with Fig. 6.13(b) – top showing the result for
Y connection and Fig. 6.13(b) – bottom showing the same result under the same
conditions for Δ connection. A FC of 100 μF was considered for both cases in
Fig. 6.13. Since the Δ connection implies higher load currents, it also leads to higher
FC voltage fluctuation, as highlighted in Fig. 6.13(b) – bottom. Another significant
difference expected with the type of load connection (Y or Δ) is in terms of the
number of levels obtained on the load phase as follows:
𝑣a = (q1a + q2a − q1b − q2b)Vdc (6.12)
𝑣b = (q1b + q2b − q1c − q2c)Vdc (6.13)
𝑣c = (q1c + q2c − q1a − q2a)Vdc (6.14)
186 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
0 0.1 0.2 0.3
t (s)
v
Ca
(V
)
0.4 0.5
240
220
200
180
160
0 0.1 0.2 0.3
t (s)
v
Ca
(V)
0.4 0.5
240
220
200
180
160
q1a
a
b
c
0
+
–
vc
+
–
vb
+ –
va
Vdc
Vdc
q2a
q2a
q1a
q1b
q2b
q2b
q1b
q1c
q2c
q2c
q1c
Figure 6.13 (a) Three-level FC converter supplying a three-phase load connected in Δ
arrangement (b) FC voltage with (top) wye and (bottom) delta load connection.
6.7 NONCONVENTIONAL FC CONVERTERS
WITH THREE-LEVEL LEGS
The goal in this section, as in other chapters in this book, is to present different power
circuits obtained by changing the way the switches are arranged. Even assuming that
those configurations may not be considered as traditional ones, they are useful in pro-
viding a learning intervention. In this sense, following the possibilities regarding the
6.7 NONCONVENTIONAL FC CONVERTERS WITH THREE-LEVEL LEGS 187
connection between the blocks that define a conventional two-level leg and those for
FC three-level leg, it is possible that five- and four-level topologies can be obtained,
as in Fig. 6.14(a) and 6.14(b), respectively.
In fact, despite using three dc voltage sources and having lesser levels at the out-
put converter side, the converter in Fig. 6.14(b) has the advantage of operating with
switches under the same blocking voltage. To guarantee that all power switches oper-
ate under the same blocking voltage and to guarantee a symmetrical output voltage,
it is necessary to make V1 = V3 = Vdc and V2 = 2Vdc.
Considering all possibilities of switching states available (that is, eliminating
the prohibited states), the output voltage is determined by Table 6.2. From this
table and avoiding the undesired states, there are four levels for 𝑣o. It is evident that
Fig. 6.14(a) is a particular case of the converter with four levels with V1 = V3 = 0,
which will lead necessarily to a converter with irregular blocking voltage among the
switches.
As can be observed in Fig. 6.14(b), the single-phase load is connected between
the points a and b of the converter, which leads to an output voltage given by
𝑣o = (2q1a + 2q2a − 2qb − 1)Vdc (6.15)
The modulation strategy for this converter can be decided, assuming a com-
bination of the two-level and three-level PWM approaches, which means that one
triangular carrier signal (𝑣∗
t2
) is employed for the two-level leg, and two triangular
carrier signals (𝑣∗
t1
and 𝑣∗
t3
) are used for a three- level leg. Since each leg is capable of
synthesizing different values of voltages, that is, 2Vdc for the two-level leg and 4Vdc
for the three-level leg, the sinusoidal waveforms employed to define PWM signals
should follow the same ratio. Indeed, there are two requirements: the reference volt-
age for the three-level leg must be twice as big as the two-level leg and their difference
must be the desired voltage (𝑣∗
sin
), which leads to
𝑣∗
a =
(
2
3
)
𝑣∗
sin (6.16)
𝑣∗
b = −
(
1
3
)
𝑣∗
sin (6.17)
Figure 6.14(c) shows the analog implementation of the PWM approach for
the proposed converter. Note that the level-shift technique has been applied to the
FC three-level leg. Figure 6.14(d) shows the PWM signals with three triangular
waveforms (𝑣∗
t1
and 𝑣∗
t3
employed for the three-level leg and 𝑣∗
t2
used for the two-level
leg) and two sinusoidal waveforms, as in equations (6.16) and (6.17).
Figure 6.15(a) shows the three-phase version of the FC four-level converter
presented in Fig. 6.14(b) by using an open-end motor drive system. Again, this
configuration presents all switches processing the voltage with the same blocking
voltage. The model and PWM strategy for this topology can be adapted directly
from Fig. 6.14(c). Figure 6.15(b) presents the machine phase voltage for phase 1
(𝑣a). The three-phase two-leg FC topology is depicted in Fig. 6.16.
188 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
b a
vo vC
+
+
+
–
–
–
+
–
+
–
io
Vdc
q2a
q2a
q1a
qb
qa
qb
b a
vo vC
+
+
–
–
io
V2
V1
V3
q2a
q2a
q1a
qb
q1a
q2a
q2a
q1a
qb
qb
q1a
qb
va
* vsin
*
2
3
=
vt1
*
va
* vsin
*
2
3
=
vt3
*
vb
* vsin
*
1
3
=
1
0
–1
1
0
–1
0.2 0.225
(d)
0.25
vt2
*
vt2
*
vt3
*
vb
*
va
*
vt1
*
(a) (b)
(c)
Figure 6.14 (a) Five-level FC topology. (b) Four-level FC topology. (c) PWM strategy for
the four-level circuit and (d) its waveforms.
6.8 FOUR-LEVEL CONFIGURATION 189
TABLE 6.2 Output Voltage Considering All
Switching States Available
State {q1aq2aqb} 𝑣o
1 {0 0 0} −Vdc
2 {0 0 1} −3Vdc
3 {0 1 0} −Vdc
4 {0 1 1} Vdc
5 {1 0 0}
6 {1 0 1}
7 {1 1 0} 3Vdc
8 {1 1 1} Vdc
q1a
V1
V2
V3
200
(a)
(b)
–200
0
qc
c
b
a a+
q2a
q1a
q2a
q1b
b+
q2b
q1b
q2b
q1c
c+
q2c
q1c
q2c
qc
qb
qb
qa
Phase 1
Phase 2
Phase 3
Three-phase
machine
qa
v
a
(V)
Figure 6.15 (a) Three-phase version of the four-level FC converter with open-end winding
three-phase motor. (b) Machine phase voltage.
6.8 FOUR-LEVEL CONFIGURATION
Following the axioms and postulates involving the PBs, presented in the Chapter 3,
the four-level FC leg can be obtained as seen in Fig. 6.17(a). Figure 6.17(b)–6.17(i)
shows the methods used to obtain the levels at the output converter side, specified in
Table 6.3. Figure 6.17(b) illustrates that it is necessary to activate the PBs 2 and 3 to
obtain 𝑣o = −V4, while 𝑣o = V1 is obtained when PBs 1 and 2 are activated.
190 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
b
c
0
vc
ic + –
vb
ib + –
va
ia + –
Vdc
Vdc
q1b
q2b
q2b
q1b
q1c
q2c
q2c
q1c
Figure 6.16 Three-phase
two-leg FC converter.
TABLE 6.3 Table of Variables for the Converter in Fig. 6.17(a)
State q1 q2 q3 𝑣o
1 0 0 0 −V4
2 0 0 1 V3 − V4
3 0 1 0 −V3 + V2 − V4
4 0 1 1 V2 − V4
5 1 0 0 −V2 + V1
6 1 0 1 V3 − V2 + V1
7 1 1 0 −V3 + V1
8 1 1 1 V1
The other levels are: 𝑣o = V3 − V4 [Fig. 6.17(c)], 𝑣o = −V3 + V2 − V4
[Fig. 6.17(d)], 𝑣o = V2 − V4 [Fig. 6.17(e)], 𝑣o = −V2 + V1 [Fig. 6.17(f)], 𝑣o = V3 −
V2 + V1 [Fig. 6.17(g)], 𝑣o = −V3 + V1 [Fig. 6.17(h)], and 𝑣o = V1 [Fig. 6.17(i)].
In general terms, to generate an output waveform with four symmetrical levels as
in Fig. 6.18, it is necessary to activate the PBs in a sequence as observed in the
same figure, with V1 = 1.5Vdc, V2 = 2Vdc, V3 = 1Vdc, and V4 = 1.5Vdc. Table 6.4
shows the symmetrical levels as a function of the switching states. The interme-
diate levels (−0.5Vdc and 0.5Vdc) can be obtained with three different circuits;
such a characteristic can be employed to guarantee the FC voltage with reduced
ripple.
The equation employed to describe the output voltage 𝑣o as a function of both
the input voltages and the binary variables (q1, q2, and q3) is presented below. The-
oretically, it is possible to guarantee each input voltage at 𝑣o using only two binary
variables, since 22 = 4. However, it is necessary to associate each binary variable to
a switching state of the four-level configuration, which means a minimum of three
binary variables (q1, q2, and q3).
6.8 FOUR-LEVEL CONFIGURATION 191
0
1
3
(a)
(b)
2 vo
V1
V4
V2 V3
1
3
2 vo
V4
(c)
1
3
2
vo
V4
V3
(d)
1
3
2 vo
V4
V3
V2
(e)
1
3
2 vo
V4
V2
(h)
1
3
2
vo
V1
V3
(i)
1
3
2
0
vo
V1
(f)
1
3
2
vo
V1
V2
(g)
1
3
2
vo
V1
V3
V2
Figure 6.17 (a) Four-level FC configuration with PBs. (b) 𝑣o = −V4. (c) 𝑣o = V3 − V4.
(d) 𝑣o = −V3 + V2 − V4. (e) 𝑣o = V2 − V4. (f) 𝑣o = −V2 + V1. (g) 𝑣o = V3 − V2 + V1. (h)
𝑣o = −V3 + V1. (i) 𝑣o = V1.
In this sense, the output pole voltage is given by
𝑣o = q1q2q3(−1.5Vdc) + q1q2q3(−0.5Vdc) + q1q2q3(−0.5Vdc)
+ q1q2q3(0.5Vdc) + q1q2q3(−0.5Vdc) + q1qq3(0.5Vdc)
+ q1q2q3(0.5Vdc) + q1q2q3(1.5Vdc) (6.18)
where q1 = 1 − q1, q2 = 1 − q2, and q3 = 1 − q3.
192 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
1
3
2
vo
V1
V3
1
3
2
vo
V1
V3
V2
1
3
2
0
vo
V1
1
3
2 vo
vo
vo
V2
V4
1.5Vdc
0.5Vdc
–0.5Vdc
–1.5Vdc
1
3
2
V4
t
V3
vo
1
3
2
V4
1
3
2 vo
V4
V3
V2
1
3
2
vo
V1
V2
Figure 6.18 Generation of a general four-level output voltage.
TABLE 6.4 Table of Variables for the Converter in Fig. 6.18(a)
with 1.5Vdc, 0.5Vdc, −0.5Vdc, or −1.5Vdc
State q1 q2 q3 𝑣o
1 0 0 0 −1.5Vdc
2 0 0 1 −0.5Vdc
3 0 1 0 −0.5Vdc
4 0 1 1 0.5Vdc
5 1 0 0 −0.5Vdc
6 1 0 1 0.5Vdc
7 1 1 0 0.5Vdc
8 1 1 1 1.5Vdc
Developing (6.18) it is possible to write 𝑣o as follows:
𝑣o = (q1 + q2 + q3)Vdc − 1.5Vdc (6.19)
As in the three-level FC configuration, the four-level one is able to generate the
desired output voltage either for positive or negative voltage.
6.8 FOUR-LEVEL CONFIGURATION 193
(a) (b)
(c)
driver
driver
+
–
q1
q2
q3
vsin
*
vt1
* +
–
vsin
*
vt1
*
q1
q2
q3
driver
driver
q1
q2
q3
q1
q2
q3
+
–
vsin
*
vt1
*
driver
driver
q1
q2
q3
q1
q2
q3
Figure 6.19 Modulation strategy for gating signal generation.
Considering the need for generation of an output waveform with reduced har-
monic distortion, Fig. 6.19 shows the analog solution for the PWM signal gener-
ation. The states of the six switches are determined by a comparison among three
high frequency triangular waveforms (𝑣∗
t1
, 𝑣∗
t2
, and 𝑣∗
t3
) and a sinusoidal waveform
(𝑣∗
sin
). Such a comparison will allow the generation of the levels as in Table 6.4.
Figure 6.20 shows the power converter and waveforms for a half-bridge four-level
configuration.
Although the topologies in Figs 6.17–6.20 present the conventional way to
obtain a four-level voltage by using FC configuration, it is also possible to obtain a
four-level output voltage with only two PBs, that is, with four switches per leg, as
seen in Fig. 6.21(a). In this case, it is necessary to guarantee the following relation-
ship among the input voltage sources: V1 = V3 = 2Vdc and V2 = Vdc and adapt the
PWM generation to assure an output voltage with four levels. The pole voltage is
given by
𝑣o = (3q1 + q2 − 2)Vdc (6.20)
Figure 6.21(b) shows the desired sinusoidal voltage that must be synthesized
by the studied converter. This waveform is intentionally separated into four sectors.
To synthesize the desired voltage in each sector it is necessary to activate the switches
q1 and q2 as described in Fig. 6.21(b) – bottom. While Fig. 6.22(a) shows the analog
194 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
(a)
(b)
R L
io
io
vo
vo
+ –
1.5Vdc
1.5Vdc
1
1
1
0
0
1
0
200
–200
0.2 0.225 0.25
50
–50
–1
2Vdc
Vdc
q1
q1
q1
q2
q2
q3
q3
q2
q3
Figure 6.20 (a) Four-level FC half-bridge converter. (b) (from top to bottom) 𝑣∗
sin
, 𝑣∗
t1
, 𝑣∗
t2
,
𝑣∗
t3
; gating signal of switches q1, q2, and q3; load voltage and load current.
(a)
va0
2Vdc
–2Vdc
–Vdc
Vdc
2Vdc
0
2Vdc
Vdc a
0 0
0 1
1 0
1 1
q1
q2
q2
q1
q1 q2
Figure 6.21 (a) Four-level FC
converter with four switches
(b) Desired waveform divided
in sectors.
6.8 FOUR-LEVEL CONFIGURATION 195
(b)
va0 = {Vdc, –Vdc} va0 = {Vdc, –Vdc}
va0 = {Vdc, 2Vdc} va0 = {Vdc, –2Vdc}
q1 = 1
Desired
sinusoidal
voltage
q2 = {0,1}
q1 = {0,1}
q2 = {0,1}
q1 = 0
q2 = {0,1}
q1 = {0,1}
q2 = {0,1}
Sector 1 Sector 2 Sector 3 Sector 4
Figure 6.21 (Continued)
(a)
(b)
+
–
q1
q2
vsin1
*
vsin1
*
vcarrier1
*
vcarrier1
vsin2
*
vcarrier2
+
–
vsin2
*
vcarrier2
*
q1
q2
Figure 6.22 (a) Four-level FC converter with four switches (b) Desired waveform divided in
sectors.
196 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
(a)
0
1
2
3
V1
V4
V2 V3
a
b
(b)
0
1
2
3
V1
V4
V2 V3
a
b
c
(c)
0
1
2
3
V1
V4
V2 V3
a
b
c
d
Figure 6.23 (a) Single-phase full-bridge four-level FC converter. (b) Three-phase four-level
FC converter. (c) Three-phase four-wire four-level FC converter.
circuit for the four-level topology in Fig. 6.21(a), Fig. 6.22(b) shows its PWM signals.
Notice that the voltages 𝑣∗
sin 1
, 𝑣∗
sin 2
, 𝑣carrier1, and 𝑣carrier2 furnish the switching states
necessary for a symmetrical output voltage with four levels.
Full-bridge four-level FC converters for both single-phase and three-phase
loads are obtained by connecting the PBs as in Fig. 6.23(a) and 6.23(b), respectively.
Figure 6.23(c) shows the option in which a three-phase four-wire system is required.
6.9 GENERALIZATION
Following the same approach as for the three- and four-level configurations, the
N-level converter can be obtained as in Fig. 6.24(e) for an odd value for N, and
in Fig. 6.24(f) for an even value for N. Theoretically, the number of levels in an
FC topology can be increased as far as necessary, although practical limitations do
appear when the number of levels is higher than five. Note that the evolution from
three to N levels is presented in Fig. 6.24(a) to Fig. 6.24(f). It is worth mentioning
that the PBG brings a simple and intuitive aspect of connecting blocks for creation
of FC topologies from three to N levels. The model and PWM strategy applied for
6.10 SUMMARY 197
(a)
0
1
2
V1
V3
V2
(b)
0
1
2
3
V1
V4
V2 V3
(c)
0 0
0
1
4
2
3
V1
V5
V4
V2 V3
(d)
(e) (f)
0
1
4
5
2
3
V1
V6
V4 V5
V2 V3
Figure 6.24 Generation of the n-level FC topologies: (a) three-level, (b) four-level, (c)
five-level, (d) six-level, (e) N-level (with N odd), and (f) N-level (with N even).
the configurations with number of levels higher than four can be easily adapted from
the previous discussion in this chapter.
6.10 SUMMARY
This chapter was dedicated to the multilevel topologies that are characterized by the
presence of the FC employed to generate different levels. For the sake of simplifica-
tion, first the FC was substituted by a DC source and then the circuit with capacitor
was presented along with the analysis to keep 𝑣c with minimum ripple. As in the
case of other configurations in this book, such as neutral-point-clamped and cas-
cade arrangements, FC topologies were presented in a systematic way following this
sequence: (i) PB connections obtained from the rules presented in Chapter 3, (ii)
once the topology was established the Table of Variables was obtained, (iii) model-
ing the converter by writing the output voltage to describe what was obtained in the
Table of Variables, and (iv) developing the PWM approach from the Table of Vari-
ables. As a learning intervention, nonconventional converters were also employed in
198 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION
this chapter. There is an extensive technical literature on this topic some of which is
given as References from 1 to 9.
REFERENCES
[1] Meynard TA, Foch H. Multilevel conversion: high voltage chopper and voltage source inverters. Pro-
ceedings of IEEE PESC’92; 1992. p 397–403.
[2] Meynard TA, Foch H, Thomas P, Courault J, Jakob R, Nahrstaedt M. Multicell converters: basic con-
cepts and industry applications. IEEE Trans Ind Electron 2002;49(5):955–964.
[3] Jeon J-H, Kim T-J, Kang D-W, Hyun D-S. A symmetric carrier technique of CRPWM for voltage
balance method of flying capacitor multi-level inverter. IEEE Trans Ind Electron 2005;52(3):879–888.
[4] Lin B-R, Hung T-L, Huang C-H. “Single-phase AC/AC converter with capacitor-clamped scheme”.
IEE Proc-Electr Power Appl 2003;150(4):464–470.
[5] Lin BR, Huang CH. Single-phase switching-mode rectifier with capacitor-clamped topology. IEE
Proc-Electr Power Appl 2005;152(1):9–16.
[6] Lin B-R, Huang C-H. Three-phase capacitor-clamped converter with fewer switches for use in power
factor correction. IEE Proc-Electr Power Appl 2005;152(3):596–604.
[7] Kou X, Corzine KA, Familiant Y. Full binary combination schema for floating voltage source
multi-level inverters. IEEE Trans Power Electron 2002;17(6):891–897.
[8] Jing Huang, Keith Corzine. Extended operation of flying capacitor multilevel inverters. Proceedings
of IEEE IAS’ 04; 2004. p 813–819.
[9] Radermacher H, Schmidt B, De Doncker R. Determination and comparison of losses of single
phase multi-level inverters with symmetric supply. Proceedings of IEEE PESC’04; vol. 6; 2004. p
4428–4433.
CHAPTER 7
OTHER MULTILEVEL
CONFIGURATIONS
7.1 INTRODUCTION
After dealing with either conventional power circuits for multilevel topologies or non-
traditional configurations based on the three most used circuits (neutral point clamped
(NPC), cascade, and flying capacitor (FC)), this chapter presents some other topolo-
gies obtained independently. Such power circuits are also easily obtained from the
axioms and postulates of the power blocks geometry (PBG) presented in Chapter 3.
Although many of the circuits presented in this chapter have not been con-
sidered in industrial applications, such converters have characteristics that bring up
specific advantages as compared to the traditional circuits. Furthermore, the noncon-
ventional multilevel configurations presented in this chapter have an important role
in helping to understand how new topologies have been conceived in the literature.
Such NPCs are presented, following the same procedure as before, with the following
steps: (i) consider the PBs and the rules to determine the connection of blocks and
consequently the connection of the power switches, (ii) determine a Table of Variables
to associate the output voltage with binary variables (switching states), (iii) find an
equation to describe the Table of Variables and consequently model the converter,
and (iv) determine a simple pulse width modulation (PWM) approach to obtain the
gating signals of the switches.
The sections in this chapter deal with different types of nontraditional con-
verters and are organized as follows: Section 7.2 presents the nested configuration
achieved by connecting only the first and second PB-ac in an appropriate way. Section
7.3 shows an alternate way to obtain a multilevel output voltage with a coupled
inductor placed at the output of the converter, as well as a topology known as mod-
ular multilevel converter (MMC). Section 7.4 presents the ANPC topology, high-
lighting its thermal stress reduction among the power switches. A series of other
topologies are included in Section 7.5, which brings up a review stressing how the
multilevel circuits proposed in the technical literature can be in fact obtained eas-
ily from the Power Block Geometry approach. Finally, Section 7.6 summarizes this
chapter.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
199
200 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
(a) (b)
(c) (d)
V1
V2
V3
V1
V2
V4
V3
V1
V2
V4
V3
V5
V1
V2
V4
V3
V6
V5
vo
vo vo
vo
Figure 7.1 Nested multilevel configurations with the block representation: (a) three-level,
(b) four-level, (c) five-level, and (d) six-level.
7.2 NESTED CONFIGURATION
This section presents multilevel topologies based on the concept of nested arrange-
ment. Such topologies are called nested multilevel converters because the external
connections of the blocks involve the internal ones. Figure 7.1(a) shows a three-level
circuit obtained with the first PB-ac and second PB-ac. Figure 7.1(b), 7.1(c), and
7.1(d) depict a four-, five-, and six-level converters, respectively. Once the topolo-
gies are obtained via the power blocks, the circuits can be considered in their lower
level (representation with switches), as presented in Fig. 7.2. Figure 7.2(a) and 7.2(b)
show three- and four-level converters, respectively. The converters presented in this
figure show both single-leg and three-phase versions of the nested configuration.
Figure 7.2(c) shows the evolution from five to seven levels.
When compared to the NPC topologies, the nested configurations can be con-
sidered as an interesting option due to the reduced number of power diodes. A draw-
back would be different blocking voltage per switch.
Although Figs 7.1 and 7.2 present topologies able to generate a number of lev-
els between 3 and 7, the analysis in this section will be focused on the four-level
converter, which is enough to give the reader a comprehensive idea of how to deal
with this family of multilevel converters.
The converter leg in Fig. 7.2(b) (left side) is constituted by two controlled
switches (q1 and q4) and two bidirectional controlled switches (q2 and q3). For the
version of the converter with three legs, required in three-phase systems, there are six
controlled switches (q1x and q4x – x = a, b, and c) and six bidirectional controlled
7.2 NESTED CONFIGURATION 201
(a)
(b)
(c)
V1
V1
V1
V1
V1
V1
V4 V4
V4
V4
V4
V5
V5
V5
V6
V6
V7
V2
V2
V2
V2
V2
V3
V3
V3
V3
V3
V2
V3
V1
V2
V3
q2
q1
q1
q1
q5
q2
q2
q3
q4
q4
q4
q1a q1b q1c
q2a q2b q2c
q3a
q3a
q3
q3
q2
q2
q1
q1
q3b
q3b
q3c
q3c
q4a
q4
q4
q5
q5
q6
q6
q7
q4b q4c
q2a q2b q2c
q1a q1b q1c
q3
vo
vo
vo
vo
vo
vc
vb
va
vc
vb
va
Figure 7.2 Nested multilevel configurations with the switches representation: (a)
three-level, (b) four-level, and (c) evolution from five- to seven-level.
switches (q2x and q3x). The Table of Variables for the leg of the nested topology with
four levels is presented in Table 7.1.
Such a table can be described by the following equation:
𝑣o = q1q2q3q4V1 + q1q2q3q4V2 + q1q2q3q4V3 + q1q2q3q4V4 (7.1)
with qy = 1 − qy for y = 1, 2, 3, and 4.
202 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
TABLE 7.1 Table of Variables for the Four-Level
Nested Converter
State q1 q2 q3 q4 𝑣o
1 1 0 0 0 V1
2 0 1 0 0 V2
3 0 0 1 0 V3
4 0 0 0 1 V4
For the generation of a symmetrical waveform with the maximum output volt-
age given by Vdc, the input voltage can be obtained as follows: V1 = 3Vdc∕4, V2 =
Vdc∕4, V3 = −Vdc∕4, and V4 = −3Vdc∕4. In this case, it turns out that equation (7.1)
becomes
𝑣o =
(3q1q2q3q4 + q1q2q3q4 − q1q2q3q4 − 3q1q2q3q4)Vdc
4
(7.2)
Figure 7.3(a)–7.3(d) shows the positive and negative currents through the
switches q1, q2, q3, and q4 when these switches are turned on, respectively. Notice
that the bidirectional controlled switches (q2 and q3) have been employed on the
inner leg, while the switches (q1 and q4) have been used on the outer leg.
Exercise 7.1
Explain what would happen if the positions of the switches placed on the inner
and outer legs are switched, for example, if the figure below is used instead
of Fig. 7.1(b). Justify your answer by using equivalent circuits such as in
Fig. 7.3.
V1
V2
V3
vo
From the Table of Variables (Table 7.1), it is possible to determine a PWM
solution as shown in Fig. 7.4. Notice that the PWM approach for the nested topology
can be obtained with only one modulating signal and three carrier signals with a level
shift technique.
Figure 7.5 shows the simulated results for the nested configuration with four
levels for a three-phase application. The waveforms presented in Fig. 7.5(a) and 7.5(b)
7.2 NESTED CONFIGURATION 203
(a) (b)
(c) (d)
q1
Vdc
3
4
+
–
Vdc
1
4
Vdc
1
4
+
+
0
–
–
Vdc
3
4
+
–
q2
Vdc
3
4
+
–
Vdc
1
4
Vdc
1
4
+
+
0
–
–
Vdc
3
4
+
–
q3
Vdc
3
4
+
–
Vdc
1
4
Vdc
1
4
+
+
0
–
–
Vdc
3
4
+
–
q4
Vdc
3
4
+
–
Vdc
1
4
Vdc
1
4
+
+
0
–
–
Vdc
3
4
+
–
Figure 7.3 Current flows
through the switches when
(a) q1 = 1, (b) q2 = 1, (c)
q3 = 1, and (d) q4 = 1.
are: (a) pole voltages; (b) from top to bottom: output line voltage, pole voltage, and
phase current.
Exercise 7.2
Compare the nested and the NPC topologies in terms of the blocking voltage
for the switches employed in one leg. Assume that both topologies have four
levels and are generating the same output voltage. Disregard any safety margin
while specifying the voltages for each power switch.
204 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
driver
driver
driver
driver
+
–
+
–
+
–
q1
V1
V4
V2
V3
q1
q2
q2
q3
q3
q4
q4
vsin
*
vt1
*
vt2
*
vo
vt3
*
Figure 7.4 PWM approach for the nested configuration.
(a)
(b)
0.1 0.15
0
100
–100
0
100
–100
0
100
–100
v
c0
(V)
t(s)
v
b0
(V)
v
a0
(V)
0.1 0.15
0
0.105 0.11 0.12 0.13 0.14 0.15
0.115 0.125 0.135 0.145
0.105 0.11 0.12 0.13 0.14 0.15
0.115 0.125 0.135 0.145
100
–100
0
100
–100
0
1
–1
i
b
(A)
t(s)
v
b0
(V)
v
ac
(V)
Figure 7.5 Three-phase
four-level nested
configurations: (a) pole
voltages and (b) line-to-line
voltage (top), pole voltage
(middle), and load current
(bottom).
Although sometimes there are practical limits for the converters with a higher
number of levels, the nested topology allows its generation with N levels for both
cases, N being an odd and an even number. Figure 7.6 presents a generalization of
the nested multilevel converters for an odd [see Fig. 7.6(a)] and even [see Fig. 7.6(b)]
number of levels.
7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT 205
(a) (b)
vo vo
Figure 7.6 Generalization of nested multilevel converter with (a) odd and (b) even number
of levels.
7.3 TOPOLOGY WITH MAGNETIC ELEMENT
AT THE OUTPUT
A three-level voltage can be obtained either by using the nested topology (as described
in Section 7.2) or by employing any of the conventional circuits (described in previous
chapters). All circuits considered so far for generation of a three-level voltage at
the output of the converter have been achieved by placing switches, sources, and/or
capacitors appropriately, as seen in Fig. 7.7(a)–7.7(c).
The figures of the NPC, H-bridge, and FC configurations are repeated here
in order to compare their principles with an alternate way to generate a three-level
voltage. Observing such topologies, it is possible to use different strategies to generate
the same number of levels at the output converter side. For instance, Fig. 7.7(a) shows
an NPC topology that creates three different paths to connect the input voltages V1,
V2, and V3 to the output (𝑣o). The H-bridge circuit shown in Fig. 7.7(b) combines both
inputs to obtain the desirable three-level output voltage, that is, V1 − V2, 0, V2 − V1.
On the other hand, the FC topology in Fig. 7.7(c) associates sources (or sources and
capacitors) in series to obtain the desirable levels at the output.
By employing a different approach, Fig. 7.7(d) shows another way to imple-
ment a three-level power converter. Such an arrangement, using a split-wound cou-
pled inductor at the output converter side, guarantees a three-level output voltage
with only two PBs-dc. The lower level representation of this converter is furnished
206 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
(a) (c)
(b)
(d) (e)
2
2
1
1
0
+
–
q1
q2
0
V1 V1
V3
V2
V1
V1
V2
V2
V2
V3
vo
vo
vo
vo
io
iCM
vo
2
Vdc
+
–
2
Vdc
Figure 7.7 Three-level configurations: (a) NPC, (b) cascade, (c) flying capacitor, (d)
configuration with two PB-dc and split-wound coupled inductors, and (e) representation of
the converter in Fig. 7.7(d) with switches.
in Fig. 7.7(e), which highlights the connections of the power switches and coupled
inductor.
It is assumed that the currents through the coupled inductor are in continuous
conduction mode, that is, the current is always higher than zero. Figure 7.8(a), 7.8(b),
7.8(c), and 7.8(d) shows the equivalent circuit for the leg when (q1,q2) are given by
(0,0), (0,1), (1,0), and (1,1), respectively. Table 7.2 shows the Table of Variables for
this converter. Notice that the output voltage has three levels, as explained later.
The voltages 𝑣10 and 𝑣20 [voltages from the points 1 and 2 to the dc-link capac-
itor midpoint – “0” in Fig. 7.7(e)] can be expressed as a function of the state of the
switches q1 and q2, as follows:
𝑣10 = (2q1 − 1)
Vdc
2
(7.3)
𝑣20 = (2q2 − 1)
−Vdc
2
(7.4)
The pole voltages as in equations (7.3) and (7.4) lead to the model presented in
Fig. 7.9(a). Then the output voltage 𝑣o with respect to “0” can be in turn written as
𝑣o =
1
2
(𝑣10 + 𝑣20) (7.5)
Substituting (7.3) and (7.4) in (7.5) it is possible to write 𝑣o as a function only
of the state of the switches and dc-link voltage
𝑣o = (q1 − q2)
Vdc
2
(7.6)
7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT 207
(a)
1
2
0
+
–
off
off
vo
io
2
Vdc
+
–
2
Vdc
(b)
1
x2
0
+
–
off
off
vo
io
2
Vdc
+
–
2
Vdc
(c)
1
2
0
+
–
off
on
vo
io
2
Vdc
+
–
2
Vdc
(d)
1
2
0
+
–
on
on
vo
io
2
Vdc
+
–
2
Vdc
Figure 7.8 Equivalent
circuits for the topology
presented in Fig. 7.7(d): (a)
q1 = q2 = 0, (b) q1 = 0 and
q2 = 1, (c) q1 = 1 and q2 = 0,
and (d) q1 = q2 = 1.
TABLE 7.2 Pole Voltage as a Function of the
Switching States
q1 q2 𝑣10 𝑣20 𝑣o
0 0 −Vdc∕2 Vdc∕2 0
0 1 −Vdc∕2 −Vdc∕2 −Vdc∕2
1 0 Vdc∕2 Vdc∕2 Vdc∕2
1 1 Vdc∕2 −Vdc∕2 0
From the Table of Variables presented in Table 7.2 it is possible to define the
PWM strategies as in Fig. 7.9(b). Figure 7.9(c) shows the main waveforms associated
with this circuit.
208 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
driver
driver
+
+
–
–
q1
q2
q2
qx1
q1
vsin
*
vsin
*
vt1
*
vt1
*
+
–
vsin
*
vt2
*
vt2
*
vo
vo
vo
v10
+
–
v20
0
(a) (b)
(c)
1
2
q2
qx2
qx2
Figure 7.9 (a) Model of converter in Fig. 7.7(e). (b) PWM circuit. (c) Waveforms for
generation of a three-level voltage.
Example 7.1
Deduce equation (7.5) for the three-level topology presented in Fig. 7.7(e).
Solution
The output voltage 𝑣o can be written with respect to the point “0” in two differ-
ent ways, 𝑣o = −𝑣x1 + 𝑣10 and 𝑣o = 𝑣x2 + 𝑣20, where 𝑣x1 and 𝑣x2 are the drop
voltages on the coupled inductor for the upper and lower parts of the inductor,
respectively. Adding both equations 𝑣o is easily obtained as (𝑣10 + 𝑣20)∕2 for
the symmetrical case (𝑣x1 = 𝑣x2).
7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT 209
(a)
(c)
(b)
Vp
Vn
0
0 0 0
vo
vo1 vo2 vo3
vo
Figure 7.10 Five-level topology with coupled inductor placed at the output converter side:
(a) PBG representation, (b) representation with switches, and (c) three-phase version.
More levels can be obtained by combining the solution with coupled inductor
and NPC converter. The circuit depicted in Fig. 7.10 is a five-level topology with a
PBG representation [see Fig. 7.10(a)] and with a representation using switches [see
Fig. 7.10(b)]. Its three-phase version is presented in Fig. 7.10(c). Notice that in this
converter the number of levels is higher than the input voltages available (Vp, 0, Vn),
which follows the same characteristics of the three-level version in Fig. 7.7(e) – in
the three-level case there are three levels obtained from only two voltages.
Although many of the converters presented so far in this and previous chapters
are suitable for high voltage high power applications, the MMC combines excellent
210 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
V1
V2
vc vb va
Figure 7.11 Modular multilevel
converter with PBs.
output voltage waveforms, very high efficiencies and an overall high blocking
voltage capability with reduced stress on the switching devices of each submodule.
Those characteristics are desirable in applications such as high power motor drives.
Figures 7.11 and 7.12 show this configuration with power blocks and switches,
respectively. There are some challenges related to the operation point of view of
this converter. They are capacitor voltage ripple control for each module as well as
circulating current regulation.
Each phase of the converter shown in Figs. 7.11 and 7.12 constitutes two
branches of half-bridge converters (also known as submodules), series connected
to dc terminals V1 and V2. Those branches are connected through inductors. The
ac terminals (𝑣a, 𝑣b, and 𝑣c) are connected to the middle point of the inductors. In
general terms, the ac voltage is controlled by changing the number of half-bridge
converters connected to each leg. From Fig. 7.12 ia and the circulating current (icc)
can be written, respectively, by
ia = ia1 − ia2 (7.7)
icc =
ia1 + ia2
2
(7.8)
Consequently the currents ia1 and ia2 can be expressed as a function of both
circulating current and output ac current as follows:
ia1 =
icc + ia
2
(7.9)
ia2 =
icc − ia
2
(7.10)
The circulating current is associated to the energy exchange between the phase
leg and the dc-link source. In fact, the control strategy applied for this converter
should guarantee the capacitor voltage control for each submodule as well as desired
output voltages 𝑣a, 𝑣b, and 𝑣c.
7.4 ACTIVE-NEUTRAL-POINT-CLAMPED CONVERTERS 211
V1
V2
vc vb
ia1 ia
ia2
va
Figure 7.12 Modular
multilevel converter –
representation with switches.
7.4 ACTIVE-NEUTRAL-POINT-CLAMPED CONVERTERS
The converter presented in Fig. 7.13 shows another arrangement using only the first
PB-ac, which is called ANPC configuration. Figure 7.13(a) shows the three-level
topology, while Fig. 7.13(b) presents the four-level version of the ANPC circuit. Yet
more levels can be reached by adding more blocks as done in Chapter 4 for the NPC
converter. Notice that for this family of multilevel converters controlled switches are
employed instead of power diodes (as in NPC configurations) to obtain zero voltage
212 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
(a)
(b)
(c) (d) (e)
q1 d1
d2
q2
d
io
io
io
Figure 7.13 ANPC configuration: (a) three-level circuit, (b) four-level circuit, (c) zero
output voltage with positive current, (d) second path for zero output voltage with positive
current, and (e) zero output voltage with positive current for NPC converter.
7.4 ACTIVE-NEUTRAL-POINT-CLAMPED CONVERTERS 213
at the output of the converter. The main advantages as compared to the conventional
NPC topology [see Fig. 7.7(a)] is a better balance distribution of losses, which allows
an increase in the maximum output power.
In general terms, the design of a multilevel power electronics converter can be
established by limiting the switching frequency in order to meet the maximum allow-
able losses. In this sense and assuming a high power density scenario, a topology such
as NPC, with irregular power losses distribution, presents unequal junction tempera-
ture distribution on the power converter circuit. As a direct consequence, some power
devices become hotter than others, restricting the switching frequency even more.
On the other hand, due to the presence of controlled power switches, the ANPC
topology can allow alternative paths to obtain the same zero voltage at the output
converter side. It turns out that it is possible to manage the losses distribution of
the switches by changing these paths. For example, Fig. 7.13(c) depicts the ANPC
topology for the case in which a zero voltage is obtained for positive output current.
On the other hand, Fig. 7.13(d) shows the same case as before (zero voltage obtained
at the output with positive current) reached by using an alternative circuit. Finally,
Fig. 7.13(e) shows that for the NPC converter there is only one path to obtain zero
level voltage at the output of the converter with a positive current.
Since the heat sink is essential for the thermal stability and lifetime of the
semiconductor devices and for operation of the power converter as a whole, its specifi-
cation must guarantee heat transfer capability for the switches, especially those under
the highest thermal stress. Indeed, such a characteristic of the ANPC topology pre-
sented in Fig. 7.13(c) and 7.13(d) plays an important role in the thermal design of this
converter. The irregular junction temperature among diodes and power switches of the
NPC topology is presented in Fig. 7.14(a). The components d, q1, q2, d1, and d2 are
the semiconductor devices in Fig. 7.13(e). To avoid such irregular junction tempera-
ture among the power switches while synthesizing the desired voltage, Fig. 7.14(b)
shows one leg of the ANPC topology with a PWM defined by the temperature of the
devices, which means that the hot points can be avoided by using alternative paths
highlighted in Fig. 7.13(c) and 7.13(d).
(a) (b)
q1
q1
q1 T2,T4
T3,T6
d1
d
Junction
temperature
PWM
Approach
d2
q2
q2
q2
q3
q3
q4
q4
q5
q5
q6
q6
vsin
*
Figure 7.14 (a) Junction temperature among the semiconductor devices. (b) PWM strategy
for the ANPC topology.
214 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
TABLE 7.3 Table of Variables for the ANPC Topology
q1 q2 q3 q4 q5 q6 𝑣o
1 1 0 0 0 0 Vdc
0 1 0 0 1 0 0
0 0 1 0 0 1 0
0 0 0 1 0 1 −Vdc
As mentioned previously, such irregular losses distribution can be avoided with
the ANPC topology and a regulated loss-balancing system. This loss control strategy
can be achieved by either measuring or estimating the junction temperature. From
Table 7.3 it is possible to establish a PWM strategy, depending on the temperature
either measured or estimated from each semiconductor device.
7.5 MORE MULTILEVEL CONVERTERS
Since the goal of this section is to demonstrate that many topologies can be repre-
sented by PBG, their presentation is limited to the description of the circuits with both
blocks and switches. All analysis in terms of Table of Variables, model, and PWM can
be obtained by the reader following a similar approach as in the previous chapters.
Also, this section aims to reiterate that the power blocks and the rules and
postulates presented in Chapter 3 are an interesting way to understand how the mul-
tilevel configurations have been presented in the technical literature. By following
the rules and using specific blocks, it is possible to, for example, obtain the config-
uration depicted in Fig. 7.15, which has been named by the authors as active switch
NPC (ASNPC). Figure 7.15(a) shows this converter under PBG representation, which
employs four PBs-ac. The equivalent lower-level representation using power switches
is presented in Fig. 7.15(b). The improvement brought up by this converter lies on
the reduction of the average switching frequency for all power devices.
The three-level configuration obtained using just the second PB-ac comes
up with two different implementations as presented in Fig. 7.16(a) and 7.16(c).
(a) (b)
V1
V2
V3
V1
V2
V3
vo vo
Figure 7.15 Three-level configuration ASNPC (a) blocks and (b) switches.
7.5 MORE MULTILEVEL CONVERTERS 215
(a)
(c) (d) (e)
(b)
V1
V3
V1
V2
V2
V1
V3
V3 V3
V2
V1
V2
V2
V3
V1
vo
vo
vo
vo
vo
Figure 7.16 Three-level topologies using the second PB-ac only.
Figure 7.16(b) shows the same topology with switches. Considering the representa-
tion with the power switches as in Fig. 7.16(d), it is evident that the four switches
between the 𝑣o and V2 can be simplified by only two antiseries switches as in
Fig. 7.16(e). Indeed, Fig. 7.16(a) and 7.16(c) end up with the same topology, as
presented in Fig. 7.16(b) and 7.16(e).
Figure 7.17 shows a family of multilevel topologies known as mixed NPC/FC
converters. Figure 7.17(a) depicts such a mixed three-level converter using both
PB-dc and PB-ac, while Fig. 7.17(b) shows it with only PBs-ac. The representa-
tion with switches for those converters is presented in Fig. 7.17(c) and 7.17(d),
respectively. Higher levels can be easily obtained by stacking more elements as in
Fig. 7.17(e)–7.17(h).
Another way to merge a FC with the first PB-ac is presented in Fig. 7.18.
Figure 7.19 depicts a similar configuration using a second PB-ac instead of the first
one. Finally, Fig. 7.20(a) shows that two PBs-ac can be vertically stacked, which
creates a differential converter, and Fig. 7.20(b) and 7.20(c) present different ways to
generate a four-level converter.
216 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
(a) (b)
(c) (d)
(e) (f)
(g) (h)
V1
V1
V1
V1
V1
V2
V3
V4
V2
V3
V4
V2
V3
V4
V2
V3
V1
V2
V3
V2
V3
vo
vo
vo
vo vo
V1
V2
V3
V4
vo
vo
V1
V2
V3
vo
Figure 7.17 Mixed NPC/FC converter.
7.5 MORE MULTILEVEL CONVERTERS 217
(a) (b)
V1
V2
V3 V3
V2
V1
vo
vo
Figure 7.18 Mixed NPC/FC converter using flying capacitor and first PB-ac.
(a) (b)
V2
V3 V3
V2
V1
V1
vo
vo
Figure 7.19 Mixed NPC/FC
converter using flying capacitor
and first/second PB-ac.
218 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS
(a)
(b)
(c)
Figure 7.20 (a) Differential converter. (b) Four-level converter obtained with the first PB-ac.
(c) Asymmetrical four-level topology.
7.6 SUMMARY
This chapter dealt with of nontraditional multilevel converters. The approach used,
with the PBG, shows that there is a high number of possibilities for generation
of multilevel topologies and such an approach helps to understand how many of
these topologies have been desscribed in the technical literature. Although not
REFERENCES 219
all possibilities have been deeply examined, three of them have been analyzed,
considering the PBs and the rules to determine the connection of blocks, Table of
Variables and model of the converter. There is an extensive number of possibilities of
multilevel topologies to which this technique can be used. Some of them, indicated
in References from 1 to 26 have been used in this chapter.
REFERENCES
[1] Bhagwat PM, Stefanovic VR. Generalized structure of a multilevel PWM inverter. IEEE Trans Ind
Appl 1983;IA-19(6):1057–1069.
[2] Holmes D, Lipo T. Pulse Width Modulation for Power Converters: Principles and Practice.
Wiley-IEEE Press; 2003.
[3] dos Santos Jr. EC, Muniz JHG, da Silva ERC. 2L3L inverter. Proceedings of COBEP; 2011.
p 924–929.
[4] dos Santos Junior EC, Muniz JHG, da Silva ERC, Jacobina CB. Nested multilevel configurations.
IEEE Energy Conversion Congress and Exposition (ECCE); 2012. p 324–329.
[5] Matsui K, Murai Y, Watanabe M, Kaneko M, Ueda F. A pulsewidth modulated inverter with
parallel-connected transistors by using current sharing reactors. IAS Annual Meeting Conference
1985; 1985. p 1015–1019.
[6] Fratta A, Griffero G, Nieddu S, Pellegrino G Villata F. Inductive three-level V.-supplied conversion
cell by new hybrid coupling reactor family. Proceedings of IAS’02; 2002. p 2378–2385.
[7] Salmon J, Ewanchuk J, Knight AM. PWM inverters using split-wound coupled inductors. IEEE Trans
Ind Appl 2009;45(6):2001–2009.
[8] Teixeira CA, McGrath BP, Holmes DG, Topologically reduced multilevel converters using comple-
mentary unidirectional phase-legs. IEEE International Symposium on Industrial Electronics (ISIE);
2012. p 2007–2012.
[9] Brückner T, Bernet S, Güldner H. The active NPC converter and its loss-balancing control. IEEE
Trans Ind Electron 2005;52(3):855–868.
[10] Bruckner T, Bernet S, Steimer PK. Feedforward loss control of three-level active NPC converters.
IEEE Trans on Ind Appl 2007;43(6):1588–1596.
[11] Andrejak JM, Lescure M. High voltage converters promising technological developments. Proc. Rec.
EPE Conf.; 1987. p 1.159–1.162.
[12] Choi NS, Cho JG, Cho GH. A general circuit topology of multilevel inverter. Proc. Rec. IEEE PESC;
1991. p 96–103.
[13] Carpita M, S Tenconi. A novel multilevel structure for voltage source inverter. Proc. Rec. EPE Conf.;
1991. p 1.90–1.94.
[14] Floricau D, Gateau G, Leredde A. New active stacked NPC multilevel converter: operation and fea-
tures. IEEE Trans Ind Electron 2010;57(7):2272–2278.
[15] Gateau G, Meynard TA, Foch H. Stacked multicell converter (SMC): properties and design. IEEE
32nd Annual Power Electronics Specialists Conference, PESC 2001; 2001 Jun 17–22; Vancouver,
Canada; 2001.
[16] Suh B-S, Hyun D-S. A new n-level high voltage inversion system. IEEE Trans Ind Electron
1997;44(1):107–115.
[17] Peng F. A generalized multilevel inverter topology with self voltage balancing. IEEE Trans Ind Appl
2001;37(2).
[18] Barbosa P, Steimer P, Steinke J, Winkelnkemper M, Celanovic N. Active-neutral-point-clamped mul-
tilevel converters. Proc. IEEE Power Electron. Spec. Conf.; 2005. p 2296–2301.
[19] da Silva ERC, Muniz JHG, dos Santos EC, Silva RNA, Barreto LH. Capacitor balance in a five-level
based halfbridge converter by use of a mixed active-cell. IEEE Energy Conversion Congress and
Exposition (ECCE); 2013. p 414–419.
[20] Meilil J, Ponnaluri S, Serpa L, Steimer PK, Kolar JW. Optimized pulse patterns for the 5-level ANPC
converter for high speed high power applications. IEEE IECON 06; 2006. p 2597–2592.
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[21] Meynard T, Lienhardt AM, Gateau G, Haederli Ch, Barbosa P. Flying capacitor multiCell converters
with reduced stored energy. Proceedings of IEEE ISIE; 2006. p 914–918.
[22] Ramos RR, Ruiz-Caballero D, Ortmann MS, Mussa SA. New symmetrical hybrid multilevel
dc-ac converters. Proceedings of Power Electronics Specialists Conference (PESC2008); 2008.
p 1916–1922.
[23] Ratnayake KR, Ishikawa H, Wang D, Yoshida M, Watanabe T. Novel hybrid five level inverter. IPEC;
2000. p 2025–2028.
[24] Chen A, Hu L, and He X. A novel type of combined multilevel converter topologies. The 30th Annual
Conference of the IEEE Industrial Electronics Society; 2004. p 2290–2294.
[25] Haque MT. Series sub-multilevel voltage source inverters (MLVSIs) as a high quality MLVSI. Pro-
ceedings of SPEEDAM; 2004. p F1B-1–F1B-4.
[26] Babaei E. A cascade multilevel converter topology with reduced number of switches. IEEE Trans
Power Electron 2008;23(6):2657–2664.
CHAPTER 8
OPTIMIZED PWM APPROACH
8.1 INTRODUCTION
Many pulse width modulation (PWM) approaches have been proposed by authors
throughout the years for the systems studied in this book, that is, dc–ac and ac–dc–ac
power conversions. In general terms, it is possible to sort the PWM strategies into
two main categories: (i) sinusoidal pulse width modulation (SPWM) and (ii) space
vector modulation (SVPWM). In SPWM, introduced by Schonnung in 1964 [1], to
produce the output voltage waveform, a sinusoidal control signal (modulating signal)
is compared to a triangular signal (carrier signal). SVPWM uses a complex voltage
vector to define the pulse widths. Although one of the first suggestions for employing
complex voltage vectors in a PWM control was made by Jardan [2], the SVPWM
technique was first published by Busse and Holtz [3] followed by Pfaff et al. [4], in
the same year.
The majority of the PWM approaches presented in the previous chapters of this
book can be classified as SPWM. For each of the configurations studied so far, inten-
sive research has developed PWM strategies, bringing different levels of optimization
in terms of the THD of the waveforms generated and also in terms of the efficiency
of the converter. As a direct consequence of the high volume of research devoted
to this topic, several improvements have been observed since the first studies. For
instance, modification of the modulating signal has introduced many improvements
to the SPWM technique, resulting in nonsinusoidal carrier-based PWM (CPWM)
techniques [5–8]. After the reports by Buja and Indri [9] it has been gradually rec-
ognized that the addition of an adequate third-harmonic zero-sequence component
to each of the reference pole voltage increases 15.5% of the fundamental component
of the output voltages in a three-phase converter. As concluded by Depenbrock [10],
more than introducing the benefit of 15.5%, the zero sequence component can be used
to reduce the number of times the switches are turned on and off, by clamping each
pole voltage during 60∘ of the sinusoidal waveform.
This chapter presents some techniques for optimization of the PWM approach
considering the fact that the number of pole voltages is higher than the number of
voltages demanded by the load, and then there is a degree of freedom to be explored.
For instance, in Fig. 8.1 there is one degree of freedom for the H-bridge converter
supplying a single-phase load. There are two pole voltages available (𝑣10 and 𝑣20)
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
221
222 CHAPTER 8 OPTIMIZED PWM APPROACH
Vdc
0
1
2
iq1 iq2
+
–
+
vo
io
–
q1 q2
q1 q2
Figure 8.1 Converter with two
legs supplying a single-phase load.
at the converter side and just one voltage (𝑣o) must be controlled. Following this
introduction, this chapter is organized in seven sections. Sections 8.2 and 8.3 show
an optimized PWM strategy for converters with two and three legs, respectively. For
both sections, a PWM approach is presented with both analog and digital implemen-
tations, and finally the influence of the parameter 𝜇 is addressed for the quality of
the waveform generated as well as for the losses of the converter. Section 8.4 deals
with space vector modulation for a three-phase converter, while Section 8.5 presents
the CPWM for both a three-leg converter feeding a two-phase symmetrical machine
and a four-leg converter supplying a three-phase four-wire load. The CPWM is also
employed in non-conventional converters (Section 8.6), such as split-wound coupled
inductors, Z-source converter, and open-end winding motor.
8.2 TWO-LEG CONVERTER
8.2.1 Model
A two-leg converter, as seen in Fig. 8.1, consists of four power switches q1, q1, q2,
and q2. Note that the circuitry necessary to generate the gating signals is not presented
in this figure. The upper (q1 and q2) and bottom (q1 and q2) switches are complemen-
tary, which means that q1 = 1 − q1 and q2 = 1 − q2. As considered in the previous
chapters, the conduction state of all switches can be represented by the binary vari-
able with qx = 1 indicating a closed switch and qx = 0 indicating an open one (with
x = 1 and 2).
The pole voltages 𝑣10 and 𝑣20 can be defined as a function of the switching
states, as follows:
𝑣10 = (2q1 − 1)
Vdc
2
(8.1)
𝑣20 = (2q2 − 1)
Vdc
2
(8.2)
8.2 TWO-LEG CONVERTER 223
TABLE 8.1 Voltages and Currents of the Switches as a Function of the
Switching States
Switching Voltages Across the Currents through the
States Switches Switches
q1 q2 𝑣q1 𝑣q1 𝑣q2 𝑣q2 iq1 iq1 iq2 iq2
0 0 Vdc 0 Vdc 0 0 io 0 io
0 1 Vdc 0 0 Vdc 0 io io 0
1 0 0 Vdc Vdc 0 io 0 0 io
1 1 0 Vdc 0 Vdc io 0 io 0
The output voltage is given by
𝑣o = 𝑣10 − 𝑣20 (8.3)
𝑣o = (q1 − q2)Vdc (8.4)
Note that there are two control variables (switching states q1 and q2) to define
just one output voltage (𝑣o). While the load voltage is generated by the converter, the
load current (io) depends on the load connected to the converter (io = 𝑣o∕Z, where
Z is the impedance for a linear load). The voltages across the switches and currents
through the switches are presented in Table 8.1.
From Table 8.1, the following equations can be used to define the voltage and
currents of the switches:
𝑣qx = (1 − qx)Vdc (8.5)
𝑣qx = qxVdc (8.6)
iqx = qxio (8.7)
iqx = (1 − qx)io (8.8)
with x = 1, 2.
8.2.2 PWM Implementation
From equation (8.3) it is possible to define the desired output voltage as a function of
the reference pole voltages, as follows:
𝑣∗
o = 𝑣∗
10 − 𝑣∗
20 (8.9)
A reference voltage [𝑣∗
o = V∗
o cos(𝜔ot)] must be synthesized through two refer-
ence pole voltages (𝑣∗
10
and 𝑣∗
20
), which means one degree of freedom to be explored.
Then, an auxiliary variable (𝑣∗
h
) can be defined to allow some level of improvement.
In this case it is possible to write:
𝑣∗
10 = 𝑣∗
o + 𝑣∗
h (8.10)
𝑣∗
20 = 𝑣∗
h (8.11)
224 CHAPTER 8 OPTIMIZED PWM APPROACH
Equation (8.9), in principle, is satisfied for any value of 𝑣∗
h
. However, the aux-
iliary voltage must be obtained in order to guarantee that the reference pole voltages
are limited as follows:
−Vdc
2
≤ 𝑣∗
10 ≤
Vdc
2
(8.12)
−Vdc
2
≤ 𝑣∗
20 ≤
Vdc
2
(8.13)
When equations (8.12)–(8.13) are satisfied, it is said that the converter is oper-
ating in its linear region. The following development in this subsection aims to deter-
mine an analytical expression for 𝑣∗
h
, and consequently defining 𝑣∗
10
and 𝑣∗
20
for PWM
implementation.
Substituting (8.10) and (8.11) into (8.12) and (8.13), it is possible to write:
(a) Inequality 1. 𝑣∗
h
≥
−Vdc
2
− 𝑣∗
o;
(b) Inequality 2. 𝑣∗
h
≥
−Vdc
2
;
(c) Inequality 3. 𝑣∗
h
≤
Vdc
2
− 𝑣∗
o;
(d) Inequality 4. 𝑣∗
h
≤
Vdc
2
.
As long as 𝑣∗
o is a sinusoidal waveform, it can assume either positive or neg-
ative values; then we have two cases, Case 1: when 𝑣∗
o > 0 and Case 2: for 𝑣∗
o < 0.
Figure 8.2 shows the hatched area (feasible region) relative to inequalities 1 and 2 for
Case 1, while Fig. 8.3 shows the same inequalities for Case 2. Even with 𝑣∗
o being a
sinusoidal waveform, it appears in the following analysis (Figs 8.2–8.5) as a constant
due to the short interval of time considered.
Note that in Case 1 (Fig. 8.2) the inequality 1 is predominant over inequality 2
(since satisfying inequality 1, the inequality 2 will be necessarily satisfied), while in
Case 2 inequality 2 is predominant.
Then, equation (8.14) is enough to succinctly describe both scenarios presented
in Figs 8.2 and 8.3:
𝑣∗
h ≥
−Vdc
2
− MAX{𝑣∗
o, 0} (8.14)
Equation (8.14) is a generic way to present inequalities 1 and 2, and it is equiv-
alent to the graphical analysis depicted in Figs 8.2 and 8.3.
A similar approach can be used for inequalities 3 and 4. Figure 8.4 shows the
hatched area (feasible region) related to inequalities 3 and 4 for Case 1, while Fig. 8.5
shows the same inequalities for Case 2. Note that in Case 1 inequality 4 is predomi-
nant, while in Case 2 inequality 3 must be satisfied. Then, it is possible to write 𝑣∗
h
in
a short way as presented in
𝑣∗
h ≤
Vdc
2
− MIN{𝑣∗
o, 0} (8.15)
8.2 TWO-LEG CONVERTER 225
(a)
(b)
vo
*
t
t t
*
(Case 1: vo >0)
–Vdc
2
Inequality 1:
Feasible region
Inequality 2:
Feasible region
0
Vdc
2
–Vdc
2
0
Vdc
2
0
–Vdc
2
Vdc
2
vo
*
–
–
Vdc
2
Figure 8.2 (a) Limits of 𝑣∗
h
when 𝑣∗
o > 0 (Case 1). (b) Feasible region for inequality 1 (left)
and inequality 2 (right).
(a)
(b)
vo
*
t
t t
*
(Case 2: vo <0)
–Vdc
2
Inequality 1:
Feasible region
Inequality 2:
Feasible region
0
Vdc
2
–Vdc
2
0
Vdc
2
0
–Vdc
2
Vdc
2
vo
*
+
–
Vdc
2
Figure 8.3 (a) Limits of 𝑣∗
h
when 𝑣∗
o < 0 (Case 2). (b) Feasible region for inequality 1 (left)
and inequality 2 (right).
226 CHAPTER 8 OPTIMIZED PWM APPROACH
(a)
(b)
vo
*
t
t t
*
(Case 1: vo >0)
–Vdc
2
Inequality 3:
Feasible region
Inequality 4:
Feasible region
0
Vdc
2
–Vdc
2
0
Vdc
2
–Vdc
2
0
Vdc
2
vo
*
–
Vdc
2
Figure 8.4 (a) Limits of 𝑣∗
h
when 𝑣∗
o < 0. (b) Feasible region for inequality 3 (left) and
inequality 4 (right).
(a)
(b)
vo
*
t
t t
*
(Case 2: vo <0)
–Vdc
2
Inequality 3:
Feasible region
Inequality 4:
Feasible region
0
Vdc
2
–Vdc
2
0
Vdc
2
–Vdc
2
0
Vdc
2
vo
*
+
Vdc
2
Figure 8.5 (a) Limits of 𝑣∗
h
when 𝑣∗
o < 0. (b) Feasible region for inequality 3 (left) and
inequality 4 (right).
8.2 TWO-LEG CONVERTER 227
As in equation (8.14), equation (8.15) can be used instead of employing
the graphical analysis depicted in Figs 8.4 and 8.5. Hence, it is possible to write
equations (8.14) and (8.15) together, as:
−Vdc
2
− MAX{𝑣∗
o, 0} ≤ 𝑣∗
h ≤
Vdc
2
− MIN{𝑣∗
o, 0} (8.16)
or
−Vdc
2
− Vmax ≤ 𝑣∗
h ≤
Vdc
2
− Vmin (8.17)
where Vmax = MAX{𝑣∗
o, 0} and Vmin = MIN{𝑣∗
o, 0}.
For the operation inside a linear region [see equations (8.12) and (8.13)] 𝑣∗
h
must be considered between the limits presented in equation (8.17) and observed in
Fig. 8.6(a). Note from this figure that the lower and upper values for 𝑣∗
h
are V1 and
V2, respectively. These voltages are defined as follows: V1 = (−Vdc∕2) − Vmax and
V2 = (Vdc∕2) − Vmin. It is possible to create an index 𝜇 (distribution factor) in such a
way that the voltage 𝑣∗
h
can be changed proportionally as a function of 𝜇, as observed
in Fig. 8.6(b), with 0 ≤ 𝜇 ≤ 1. Therefore, the equation of the line in Fig. 8.6(b) can
be defined as follows:
𝑣∗
h(𝜇) = V1 + (V2 − V1)𝜇 (8.18)
By developing equation (8.18),
𝑣∗
h = Vdc
(
𝜇 −
1
2
)
+ (𝜇 − 1)Vmax − 𝜇Vmin (8.19)
0
0
(a)
(b)
0.5 1
vh
*
vh
*
μ
V2
V1
t
–Vdc
2
– Vmax
V1 =
–Vdc
2
– Vmin
V2 =
Figure 8.6 (a) Limits of 𝑣∗
h
. (b) 𝑣∗
h
as a
function of the distribution factor.
228 CHAPTER 8 OPTIMIZED PWM APPROACH
With 𝑣∗
h
defined as in (8.19), the reference pole voltages (𝑣∗
10
and 𝑣∗
20
) presented
in (8.10), (8.11) are used either to compare with a high frequency triangular waveform
(in the analog solution) or to generate timer counters (in the digital solution).
Example 8.1
Determine the waveforms for 𝑣∗
10
and 𝑣∗
20
when 𝜇 = 0.5 (distribution factor)
and assuming 𝑣∗
o = V∗
o cos(𝜔ot).
Solution
To determine the waveforms for 𝑣∗
10
and 𝑣∗
20
, from (8.10) and (8.11), it is nec-
essary to find 𝑣∗
h
, as in equation (8.19). Equation (8.19) with 𝜇 = 0.5 becomes
𝑣∗
h
= −1∕2(V∗
min
+ V∗
max). As defined earlier, Vmax = MAX{𝑣∗
o, 0} and Vmin =
MIN{𝑣∗
o, 0}, which means that:
(a) When 𝑣∗
o > 0, Vmax = 𝑣∗
o and Vmin = 0
(b) When 𝑣∗
o ≤ 0, Vmax = 0 and Vmin = 𝑣∗
o.
Hence, 𝑣∗
h
is equal to −1∕2(𝑣∗
o) for both cases 𝑣∗
o > 0 and 𝑣∗
o ≤ 0.
Therefore, 𝑣∗
10
= 1
2
𝑣∗
o and 𝑣∗
20
= −1
2
𝑣∗
o. The waveforms for 𝑣∗
10
and 𝑣∗
20
are two
sinusoidal waves with the same amplitude but 180∘ apart.
8.2.3 Analog and Digital Implementation
Figure 8.7 shows the analog implementation of the PWM solution for the two-leg
converter as depicted in Fig. 8.1. Note that the reference pole voltages, obtained from
equations (8.10)–(8.11) are compared to the carrier signal 𝑣∗
t with amplitude equal
to Vt. The relationship between the amplitude of the modified voltages 𝑣∗
j0
(i.e., V∗
j0
–with j = 1, 2) and Vt defines the amplitude modulation ratio (ma = V∗
j0
∕Vt). On the
other hand, the relationship between the switching frequency (fs – frequency of the
carrier signal) and the frequency of the sinusoidal waveform (fo) defines the frequency
modulation ratio (mf = fs∕fo).
v10
*
v20
*
0
vo
*
vh
* vt
*
μ
q1
Equation
(8.19)
–
+
–
+
Vdc
*
VMAX
MAX
MIN
*
VMIN
q1
q2
q2
Figure 8.7 Analog PWM
implementation.
8.2 TWO-LEG CONVERTER 229
Example 8.2
Considering 𝜇 = 0.5, determine the load voltage 𝑣o assuming the amplitude
modulation ratio (ma) equal to infinite.
Solution
By definition ma is given by V∗
j0
∕Vt, which means that for a modulation ratio
equal to infinite the amplitude of the sinusoidal waveform is always higher
than the carrier signal amplitude. Then, qj = 1 if 𝑣∗
j0
> 0 and qj = 0 if 𝑣∗
j0
< 0
with j = 1, 2. Then the load voltage will be a square waveform with the same
frequency of 𝑣∗
o and with amplitude equal to Vdc.
The equivalent digital solution can be obtained as an alternative for the analog
PWM implementation by defining the time in which the switches (q1 and q2) are on.
For determination of the pulse widths, used to define when the switches are either
on or off (i.e., emulating the OpAmp operation in Fig. 8.7), it is assumed that the
modified reference voltages 𝑣∗
10
and 𝑣∗
20
are constants over the switching period Ts.
From Fig. 8.8, this hypothesis (i.e., 𝑣∗
10
and 𝑣∗
20
constants over Ts) becomes more
accurate as the switching frequency becomes much higher than the frequency of the
modulating signal (i.e., fs ≫ fo).
Then, assuming that the triangular frequency is high enough to guarantee the
condition in Fig. 8.8(b), the average values of 𝑣10 and 𝑣20 over Ts should be equal to
the medium values of 𝑣∗
10
and 𝑣∗
20
, respectively. Figure 8.9 shows the waveforms for
the first leg highlighting that the medium values of 𝑣∗
10
and 𝑣10 must be equal. Hence,
it is possible to write
1
Ts ∫
t+Ts
t
𝑣∗
10(t)dt =
1
Ts ∫
t+Ts
t
𝑣10(t)dt (8.20)
1
Ts ∫
t+Ts
t
𝑣∗
20(t)dt =
1
Ts ∫
t+Ts
t
𝑣20(t)dt (8.21)
Since 𝑣∗
10
and 𝑣∗
20
are assumed to be constant over Ts,
𝑣∗
10
=
[
Vdc
2
𝜏1 −
Vdc
2
(
Ts − 𝜏1
)
]
1
Ts
(8.22)
𝑣∗
20 =
[
Vdc
2
𝜏2 −
Vdc
2
(
Ts − 𝜏2
)
]
1
Ts
(8.23)
where 𝜏1 and 𝜏2 are the time in which the switches q1 and q2 are on.
230 CHAPTER 8 OPTIMIZED PWM APPROACH
zoom
zoom
vt
* vt
*
vt
*
v10
* v10
*
v10
* vt
* v10
*
(a) (b)
Figure 8.8 Comparison of high frequency triangular and sinusoidal waveforms: (a) low
frequency modulation ratio and (b) high frequency modulation ratio.
v10
Ts
A1
A2
A3
vt
*
avg {v10} = A2–A1–A3
*
v10
*
τ1
Figure 8.9 Average value of 𝑣∗
10
equal to the average value 𝑣10.
From expressions (8.22)–(8.23) it is possible to calculate the time intervals in
which the switches q1 and q2 are on, that is
𝜏1 =
(
𝑣∗
10
Vdc
+
1
2
)
Ts (8.24)
𝜏2 =
(
𝑣∗
20
Vdc
+
1
2
)
Ts (8.25)
After the definition of the pulse widths (𝜏1 and 𝜏2), it is necessary to pro-
gram timers for implementation with either a digital signal processing (DSP) or a
field-programmable gate array (FPGA) device, for instance.
8.2 TWO-LEG CONVERTER 231
Exercise 8.1
Assume a single-phase dc–ac converter as in Fig. 8.1 with Vdc = 100V. Also
consider two ways to generate the PWM signals: (i) analog implementation
with OpAmps with maximum voltage allowed equal to 15V (due to operation
restrictions of the OpAmps), that is, maximum voltage for 𝑣∗
10
, 𝑣∗
20
, and 𝑣∗
t ,
must be equal to 15V; and (ii) digital implementation with the code written in
C++ for a DSP, with 𝑣∗
10
= 50 sin(𝜔t) and 𝑣∗
20
= 50 sin(𝜔t + 180∘). Question:
Is it possible to generate a desirable ac output voltage with amplitude
equal to 100V for both analog and digital implementations as described
before?
8.2.4 Influence of 𝝁 for PWM Implementation
The parameter 𝜇 and consequently 𝑣∗
h
play an important role in the PWM imple-
mentation described already. As mentioned earlier, the distribution factor (𝜇) can be
employed to optimize the converter operation. For instance, to emphasize such an
vt
*
vh
*
vo
*
v10
*
v10
–1
0.1 0.11 0.12
0
1
–1
0
1
io
vo
v20
*
v20
–1
0.1 0.11 0.12
0
1
–1
0
1
Figure 8.10 Waveforms obtained with 𝜇 = 0.5.
vt
*
vh
*
vo
*
v10
*
v10
–1
0.1 0.11 0.12
0
1
–1
0
1
io
vo
v20
*
v20
–1
0.1 0.11 0.12
0
1
–1
0
1
Figure 8.11 Waveforms obtained with 𝜇 = 0.0.
232 CHAPTER 8 OPTIMIZED PWM APPROACH
vt
*
vh
*
vo
*
v10
*
v10
–1
0.1 0.11 0.12
0
1
–1
0
1
io
vo
v20
*
v20
–1
0.1 0.11 0.12
0
1
–1
0
1
Figure 8.12 Waveforms obtained with 𝜇 = 1.0.
optimization, a set of the main converter’s variables are shown in Figs 8.10, 8.11, and
8.12 for 𝜇 equal to 0.5, 0.0, and 1.0, respectively. Notice that those results are normal-
ized and the maximum value is always one for both power and control waveforms.
Figure 8.10 shows the case with symmetrical waveforms (𝑣∗
10
and 𝑣∗
20
) obtained with
𝜇 = 0.5, which represents the best option in terms of the total harmonic distortion
(THD).
Note that the ripple of the current in this result is lower than that shown in Figs
8.11 and 8.12. On the other hand, 𝜇 = 0 and 𝜇 = 1 generate asymmetrical waveforms
(see Figs 8.11 and 8.12) with the main advantage related to the switching losses reduc-
tion. There is a large period of time (180∘ of the modulating signal) in which there is
no switching for either 𝑣10 or 𝑣20.
It is important to highlight that although 𝜇 plays an important role creating
waveforms with distortions to deal with either THD improvement or loss reduction,
these parameters (𝜇 and consequently 𝑣∗
h
) will not change the lengths of the active
states, as observed in Fig. 8.13.
Example 8.3
Why does the load current (io) for all values of 𝜇 have the same average value?
Does it change if another value for 𝜇 is chosen rather than 0.5, 0.0, or 1.0, for
example 𝜇 = 0.3?
Solution
Even with different instantaneous load voltages due to different values of 𝑣∗
h
,
as observed in Figs 8.10–8.12, the average values of 𝑣o should be the same
since the common term 𝑣∗
h
is cancelled [see equation (8.9)]. That is why the
amplitude value of the load current is kept constant. Another explanation can
be obtained from Fig. 8.13, which shows the unchanged active vector length
by either using 𝑣∗
h
or not, that is, if the same active vectors are applied, the
same amplitude for the currents is expected.
8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 233
v10
vh
*
vh
*
vt
v10
*
v20
*
v20
Active states
Ts
Figure 8.13 Influence of 𝑣∗
h
on the active states generation.
Vdc n
0
1
2
3
iq1 iq2 iq3
–
+
+
v1
i1
i2
i3
–
+ v2
–
+ v3
–
q1 q2 q3
q1 q2 q3
Figure 8.14 Three-leg converter supplying a three-phase load.
8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD
8.3.1 Model
A three-leg converter, as seen in Fig. 8.14, is constituted by six power switches q1,
q1, q2, q2, q3, and q3. For simplification purposes, the circuitry necessary to generate
the gating signals is not presented in this figure; instead just the power part of the
circuit has been presented. The upper (q1, q2, and q3) and bottom (q1, q2, and q3)
switches are complementary, which means that qx = 1 − qx (with x = 1, 2, 3). The
conduction state of all switches can also be represented by a binary variable with
qx = 1 indicating a closed switch and qx = 0 indicating an open one.
234 CHAPTER 8 OPTIMIZED PWM APPROACH
The pole voltages 𝑣10, 𝑣20, and 𝑣30 can be defined as a function of the switching
states, as follows:
𝑣10 = (2q1 − 1)
Vdc
2
(8.26)
𝑣20 = (2q2 − 1)
Vdc
2
(8.27)
𝑣30 = (2q3 − 1)
Vdc
2
(8.28)
The output voltages (𝑣1, 𝑣2, and 𝑣3) are given by
𝑣1 = 𝑣10 − 𝑣n0 (8.29)
𝑣2 = 𝑣20 − 𝑣n0 (8.30)
𝑣3 = 𝑣30 − 𝑣n0 (8.31)
Considering a balanced three-phase system (i.e., 𝑣1 + 𝑣2 + 𝑣3 = 0) and from
(8.29)–(8.31), it is possible to define 𝑣n0 as in equation (8.32):
𝑣n0 =
1
3
(𝑣10 + 𝑣20 + 𝑣30) (8.32)
Substituting (8.32) into (8.29)–(8.31), we get
𝑣1 =
2
3
𝑣10 −
1
3
𝑣20 −
1
3
𝑣30 (8.33)
𝑣2 = −
1
3
𝑣10 +
2
3
𝑣20 −
1
3
𝑣30 (8.34)
𝑣3 = −
1
3
𝑣10 −
1
3
𝑣20 +
2
3
𝑣30 (8.35)
Note that it is possible to explore the redundancy inherent in a three-phase sys-
tem. When two voltages are controlled, the third is indirectly controlled, such as:
𝑣3 = −(𝑣1 + 𝑣2).
Substituting (8.26)–(8.28) into (8.33)–(8.35), it is possible to write the output
voltages only as a function of the state of the switches:
𝑣1 =
[
2
3
q1 −
1
3
q2 −
1
3
q3
]
Vdc (8.36)
𝑣2 =
[
−
1
3
q1 +
2
3
q2 −
1
3
q3
]
Vdc (8.37)
𝑣3 = −𝑣1 − 𝑣2 (8.38)
The three-leg converter supplying a three-phase load (Fig. 8.14) also presents
a degree of freedom. Note that there are only two output voltages to be controlled (𝑣1
and 𝑣2 – or any other combination of two voltages among 𝑣1, 𝑣2, and 𝑣3) throughout
three controlled variables q1, q2, and q3.
While the load voltages are generated by the converter, the load currents (i1, i2,
and i3) depend on the load connected to the converter. In the case of a linear load, it can
be written as ix = 𝑣x∕Zx, where Zx is the load impedance for phase x; with x = 1, 2, 3.
The voltages and currents through the switches are presented in Table 8.2.
8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 235
TABLE 8.2 Voltages and Currents of the Switches as a
Function of the Switching States
Switching Voltages of the Currents of the
States Switches Switches
qx 𝑣qx 𝑣qx iqx iqx
0 Vdc 0 0 il
1 Vdc 0 il 0
From Table 8.2, the following equations can be used to define the voltage and
currents of the switches, respectively.
𝑣qx = (1 − qx)Vdc (8.39)
𝑣qx = qxVdc (8.40)
iqx = qxix (8.41)
iqx = (1 − qx)ix (8.42)
with x = 1, 2, 3.
8.3.2 PWM Implementation
From equations (8.29)–(8.31) it is possible to define the desired output voltages as a
function of both reference pole voltages and voltage 𝑣∗
n0
, as follows:
𝑣∗
1 = 𝑣∗
10 − 𝑣∗
n0 (8.43)
𝑣∗
2 = 𝑣∗
20 − 𝑣∗
n0 (8.44)
𝑣∗
3 = 𝑣∗
30 − 𝑣∗
n0 (8.45)
The voltage 𝑣∗
n0
can be considered as an auxiliary variable (𝑣∗
h
) which is
expected to bring a level of optimization for the converter, as for the single-phase
converter presented previously. If the desired balanced three-phase voltages are
given by 𝑣∗
1
= V∗
o cos(𝜔ot), 𝑣∗
2
= V∗
o cos(𝜔ot + 120∘), and 𝑣∗
3
= V∗
o cos(𝜔ot − 120∘),
the reference pole voltages can be defined by:
𝑣∗
10 = 𝑣∗
1 + 𝑣∗
h (8.46)
𝑣∗
20 = 𝑣∗
2 + 𝑣∗
h (8.47)
𝑣∗
30
= 𝑣∗
3
+ 𝑣∗
h (8.48)
with
𝑣∗
h = Vdc
(
𝜇 −
1
2
)
+ (𝜇 − 1)Vmax − 𝜇Vmin (8.49)
where Vmax = MAX{𝑣∗
1
, 𝑣∗
2
, 𝑣∗
3
} and Vmin = MIN{𝑣∗
1
, 𝑣∗
2
, 𝑣∗
3
}; 𝜇 is the distribution
factor and determines how the free-wheeling time interval can be distributed through-
out the switching period.
236 CHAPTER 8 OPTIMIZED PWM APPROACH
Equations (8.19) and (8.49) are identical equations, just changing the terms
Vmax and Vmin. In fact, 𝑣∗
h
is a generalized expression that can be employed in different
power converters processing ac voltage, as discussed later in this chapter.
8.3.3 Analog and Digital Implementation
Figure 8.15 shows the analog implementation of the PWM solution for the three-leg
converter depicted in Fig. 8.14. The reference pole voltages are obtained as in
equations (8.46)–(8.48) and compared to the carrier signal 𝑣∗
t .
Following the same approach employed for the single-phase converter, it is
possible to calculate the time intervals in which the switches q1, q2, and q3 are on,
that is
𝜏1 =
(
𝑣∗
10
Vdc
+
1
2
)
Ts (8.50)
𝜏2 =
(
𝑣∗
20
Vdc
+
1
2
)
Ts (8.51)
𝜏3 =
(
𝑣∗
20
Vdc
+
1
2
)
Ts (8.52)
After defining the pulse widths (𝜏1, 𝜏2, and 𝜏3), it is necessary to program three
timers associated with each leg.
8.3.4 Influence of 𝝁 for PWM Implementation in a Three-Leg
Converter
As considered for the two-leg converter, the voltage 𝑣∗
h
can be used to optimize spe-
cific parameters such as weighted total harmonic distortion (WTHD) and losses.
v1
* v10
*
v20
*
v30
*
v2
*
v3
*
vh
*
vt
*
μ
q1
Equation
(8.49)
–
+
–
+
–
+
Vdc
*
VMAX
MAX
MIN
*
VMIN
q1
q2
q2
q3
q3
Figure 8.15 Analog PWM implementation for the three-leg converter.
8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 237
vt
* v1
*
v10
i3
0.09
–1
0
1
–1
0
0
1
–1
1
0.105
(a)
(b)
0.12
i2 i1
vt
* v1
*
v10
i3
0.09
–1
0
1
–1
0
0
1
–1
1
0.105 0.12
i2 i1
Figure 8.16 Waveforms obtained with: (a) 𝜇 = 0.5 and (b) 𝜇 = 1.0.
0
WTHD
0.5 1
μ
Figure 8.17 WTHD versus 𝜇.
Figure 8.16(a) and 8.16(b) shows the main waveforms for 𝜇 equal to 0.5 and 0, respec-
tively. While Fig. 8.17 shows the WTHD of the load phase voltage as a function of
𝜇, Fig. 8.18 shows the same waveforms as in Fig. 8.16 with 𝜇 changing from 0 to
1 six times per period. Note that 𝜇 = 0.5 generates symmetrical waveforms with the
benefit of better WTHD. On the other hand, 𝜇 = 0 leads to benefits in terms of loss
reduction due to the clamped pole voltages. One way to bring up the benefits of both
𝜇 = 0.5 and 𝜇 = 1.0 is to change the parameter 𝜇 from 0 to 1 many times inside
the sine period. This will guarantee an average value of 0.5 while keeping the pole
voltages clamped.
238 CHAPTER 8 OPTIMIZED PWM APPROACH
vt
* vl1
*
v10
i3
0.09
–1
0
1
–1
0
1
–1
1
0.105 0.12
i2 i1
Figure 8.18 Waveforms with 𝜇 changing from 0 to 1.
8.3.5 Influence of the Three-Phase Machine Connection
over Inverter Variables
Traditionally, a three-phase machine is designed to be connected in a wye (Y) or delta
(Δ) arrangement depending on the voltage level available from the utility grid. In a
motor drive system, the connections of the three-phase machine can still be defined
as a function of the voltage level available on the dc-link capacitor. If the dc-link
voltage for a given application is not restrictive, the choice between both possibil-
ities of machine connections [Y – see Fig. 8.19(a) or Δ – see Fig. 8.19(b)] favors
the Y connection, as shown. The following analysis is obtained with the assumption
that the same power switches and dc-link capacitors are employed for both motor
Vdc
C
C
0
1
2
3
i1
i2
i3
v1
v2
+
+
+
v3
q1 q2 q3
q1 q2 q3
Vdc
C
C
0
1
2
3
i1
i2
i3
v1
v2
+
+
+
v3
q1 q2 q3
q1 q2 q3
(a)
(b)
Figure 8.19 Ac motor drive
system with a three-phase machine
in a: (a) Y connection and
(b) Δ connection.
8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 239
drive systems (Y and Δ), which is reasonable due to the range of IGBTs available
in the market. For instance, there is a class of IGBTs that operates at 600 V, the fol-
lowing IGBT available deals with 1200 V. As a consequence, the same IGBT can be
employed for a three-phase system with 220Vrms (phase voltage) for both Y and Δ,
since a Y arrangement would require power switches with 539 V (peak), while a Δ
arrangement 311 V (peak).
This section aims to show the advantages and disadvantages of the Y and Δ
connections of the three-phase machine in a motor drive system, highlighting the
influence of these connections on the converter variables. Some parameters of the
inverter will be considered in this analysis, that is, (i) dc-link voltage requirement,
(ii) RMS current of the dc-link capacitor, (iii) WTHD of the motor voltages, (iv)
converter losses, and (v) fault tolerance capability.
The dc-link voltage of a voltage source inverter (VSI) can be defined as a func-
tion of the rated voltage demanded by the motor, as given in (8.53) and (8.54) for wye
and delta connection, respectively
Vdc =
√
3Vph (8.53)
Vdc = Vph (8.54)
where Vph is the amplitude of the motor phase voltage.
The dc-link voltage requirement of the motor drive system in Fig. 8.19(a) is
√
3 times higher than that in the Fig 8.19(b), considering the motor phase voltage is
the same.
On the other hand, the dc-link capacitor current of the system with Y and Δ
connections are given by (8.55) and (8.56), respectively:
ic = q1i1 + q2i2 + q3i3 (8.55)
ic = q1(i3 − i1) + q2(i1 − i2) + q3(i2 − i3) (8.56)
0
0
0.5
1
i
c
(mA)
1.5
2
20 40 60 80 100
Fig. 8.19(a)
0
0
0.5
1
i
c
(mA)
Frequency (kHz)
1.5
2
20 40 60 80 100
Fig. 8.19(b)
Figure 8.20 Capacitor current spectrum: (a) Y connection and (b) Δ connection.
240 CHAPTER 8 OPTIMIZED PWM APPROACH
Figure 8.20 shows the spectra of the dc-link capacitor current. As expected in
(8.55) and (8.56), the amplitude of the harmonic components is higher in Δ, which
means that the dc-link capacitor losses will be also higher and consequently the lifes-
pan is expected to be lower for a Δ connection.
The quality of the waveform generated at the output converter side can be mea-
sured by WTHD, which can be calculated by
WTHD =
100
a1
√
√
√
√
p
∑
i=2
(ai
i
)2
(8.57)
(a)
(b)
–400
0.01
0.1
0.2
0.4
0.6
0.8
1
0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
0.015 0.02
0
1
2
4
3 +
+
+
+
–
–
–
–
t (s)
v
1
(V)
WTHD
−
v
1
0.03
0.025
–200
0
200
400
–400
0.01 0.015 0.02
t (s)
ma
v
1
(V)
0.03
0.025
–200
0
200
400
Fig. 8.19(b)
Fig. 8.19(b)
Fig. 8.19(a)
Fig. 8.19(a)
q1 q2 q3
n
q1 q2 q3
q4
q4
Three-phase
Machine
v2
vC2
+
–
vC1
v3
v1
i1
i2
i3
Figure 8.21 (a) (top) WTHD of the phase voltage (𝑣1) as a function modulation index.
(bottom) Phase voltages with ma = 0.5. (b) Solution with two dc voltages available. (c) THD
of the motor current as a function of the modulation index.
8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 241
–2
–1
0
1
2
–2
4
10 20 30 40 50
Percent of the voltage (%)
60 70 80 90 100
6
8
10
THD
(%)
12
14
16
–1
0
1
2
–2
–1
0
1
2
–2
–1
0
1
2
–2
–1
0
1
2
Figure 8.21 (Continued)
where a1 is the amplitude of the fundamental voltage component, ai is the amplitude
of the ith harmonic, and p is the highest harmonic taken into consideration.
An interesting result is shown in Fig. 8.21(a) (top). This figure shows the
WTHD of the phase voltage (𝑣1) as a function of the modulation index (ma) for
both systems shown in Fig. 8.19. Note that independent of the three-phase motor
connections (wye or delta) the WTHD of the phase voltages are exactly the same,
although the waveforms of the motor phase voltages are different, as seen in
Fig. 8.21(b) (bottom). Even with the phase voltage of a three-phase machine, Y
connection presents five levels instead of three in a Δ connection; such levels have
higher d𝑣∕dt in their peaks and valleys as compared to the three-level voltage,
which reduces the WTHD. Therefore, even with higher levels, both voltages are
242 CHAPTER 8 OPTIMIZED PWM APPROACH
equal under the WTHD point of view. A VSI able to drive a three-phase induction
motor with reduced THD for a wide range of ma is shown in Fig. 8.21(b). When
the range of the motor voltage is from 100% to 50%, the switch q4 must be turned
on to guarantee the dc-link voltage equal to 𝑣C1 + 𝑣C2 and the modulation index
goes from 1 to 0.5 (1 ≤ ma ≤ 0.5). On the other hand, when the range of the
motor voltage is from 50% to 0%, the switch q4 must be turned off to guarantee
the dc-link voltage equal to 𝑣c2 and the modulation index range goes back to
1 ≤ ma ≤ 0.5. It is worth mentioning that, even considering the operation at reduced
output voltage range, the power converter in Fig. 8.21(b) operates with a high
modulation index, which means reduced THD. Figure 8.21(c), in turn, shows the
THD behavior of the motor current from 10% to 100% of rated voltage applied to the
machine.
Another important feature affected by the connection of the machine is the con-
verter’s losses. Figure 8.22 shows the comparison of conduction, switching, and total
(conduction + switching) losses of the VSI. In this figure the switching frequency of
the converter is 10 kHz. The converter power losses are higher when the machine is
connected in a Δ arrangement, due to the higher level of currents. Figures 8.20 and
8.22 indicate why a Y connection is the primary option for a three-phase machine
connection in a motor drive system.
Exercise 8.2
When the machine is Δ connected, the reference pole voltages for the PWM
generation can be defined as follows:
𝑣∗
10 = −𝑣∗
1 + 𝑣∗
h
𝑣∗
20 = 𝑣∗
h
𝑣∗
30 = 𝑣∗
2 + 𝑣∗
h
with 𝑣∗
1
= V∗
o cos(𝜔ot) and 𝑣∗
2
= V∗
o cos(𝜔ot + 120∘) and 𝑣∗
h
given by
equation (8.49) with VMAX = {−𝑣∗
1
, 0, 𝑣∗
2
} and VMIN = {−𝑣∗
1
, 0, 𝑣∗
2
}. Explain
why these equations guarantee a balanced three-phase voltage applied to the
machine. What would happen if equations (8.46)–(8.48) are applied for the
three-leg converter with a three-phase machine in a Δ arrangement?
Y connection
Conduction
losses
Switching
losses
Total
losses
Conduction
losses
Switching
losses
Total
losses
Δ connection
10 kHz 10 kHz
0
100
Losses
(W)
200
0
100
Losses
(W)
200
Figure 8.22 Converter
losses of the ac motor drive
system with a switching
frequency equal to 10 kHz.
8.4 SPACE VECTOR MODULATION (SVPWM) 243
8.4 SPACE VECTOR MODULATION (SVPWM)
The nonsinusoidal CPWM techniques described earlier in this chapter could be
implemented in either an analog or a digital way. On the other hand, the space
vector modulation is an inherent digital way to generate the gating signals for q1,
q2, and q3. These three independent gating signals lead to eight possible switching
combinations for a three-phase inverter.
From the electrical machine and reference-frame theory analyses, it is possible
to define a transformation to represent the original three-phase variables in a sim-
ple system with variables in quadrature. Such a transformation changes the variables
with no physical connotation. Hence, a three-phase system can be considered to form
stationary vectors in the dq complex plane. The transformation of variables can be
defined as
𝑣
s
odq = P𝑣
s
123 (8.58)
where 𝑣
s
123 are the voltages in the original three-phase system, 𝑣
s
odq are the voltages in
the dq complex plane plus zero sequence component represented by “o”; the super-
script “s” stands for stationary reference-frame, as the stator variables in a three-phase
ac machine. P is the transformation of variables with
𝑣
s
odq =
⎡
⎢
⎢
⎢
⎣
𝑣s
o
𝑣s
d
𝑣s
q
⎤
⎥
⎥
⎥
⎦
, 𝑣
s
123 =
⎡
⎢
⎢
⎢
⎣
𝑣s
1
𝑣s
2
𝑣s
3
⎤
⎥
⎥
⎥
⎦
, and P =
√
2
3
⎡
⎢
⎢
⎢
⎢
⎣
1
√
2
1
√
2
1
√
2
1 −1
2
−1
2
0
√
3
2
−
√
3
2
⎤
⎥
⎥
⎥
⎥
⎦
.
The dq voltages in the stationary reference-frame can be obtained from 𝑣s
1
, 𝑣s
2
and 𝑣s
3
, by using the matrix P, as follows:
𝑣s
d =
√
2
3
(
𝑣s
1
−
1
2
𝑣s
2
−
1
2
𝑣s
3
)
(8.59)
𝑣s
q =
1
√
2
(𝑣s
2
− 𝑣s
3
) (8.60)
Since it is assumed a balanced case (𝑣s
1
+ 𝑣s
2
+ 𝑣s
3
= 0) the term 𝑣s
o is null.
Equations (8.59)–(8.60) can be written as functions of the states of the switches [see
equations (8.36)–(8.38)], as follows:
𝑣s
d =
√
2
3
(
q1 −
1
2
q2 −
1
2
q3
)
Vdc (8.61)
𝑣s
q =
1
√
2
(q2 − q3)Vdc (8.62)
Table 8.3 shows the vectors in the dq plane Vs
x = Vs
d
+ jVs
q (x = 1, 2, … , 8)
associated with each switching state. Each vector means a topological circuit for the
converter, as shown in Fig. 8.23.
Note from Table 8.3 that there are two null (0 and 7) and six non-null (1, 2,
3, 4, 5, and 6) vectors – active vectors, which will be used to synthesize the desired
244 CHAPTER 8 OPTIMIZED PWM APPROACH
TABLE 8.3 PWM Vectors as a Function of the
Switching States
Vector q1 q2 q3 Vs
x
0 0 0 0 0
1 1 0 0
√
2∕3Vdc
2 1 1 0 Vdc∕
√
6 + jVdc∕
√
2
3 0 1 0 −Vdc∕
√
6 + jVdc∕
√
2
4 0 1 1 −
√
2∕3Vdc
5 0 0 1 −Vdc∕
√
6 − jVdc∕
√
2
6 1 0 1 Vdc∕
√
6 − jVdc∕
√
2
7 1 1 1 0
(a) (b) (c)
(d) (e) (f)
(g) (h)
V1
V2
V3
V1
q1
V2
V3
V1
q2
V2
V3
V1
q1 q1 q2 q3
q3
V2
V3
V1
V2
V3
V1
q2 q3
V2
V3
V1
q3
V2
V3
V1
q1 q2
V2
V3
Figure 8.23 Topological circuits as a function of the switching states: (a) Vector 0, (b)
Vector 1, (c) Vector 2, (d) Vector 3, (e) Vector 4, (f) Vector 5, (g) Vector 6, (h) Vector 7.
8.4 SPACE VECTOR MODULATION (SVPWM) 245
(a)
(c)
(d) (e)
(b)
V3
s
V2
s
V1
s
V0
s
V6
s
V5
s
V2
s
t2/T
V2
s
t2/T
V3
s
t3/T
V1
s
t1/T
V4
s
V7
s
Vector 2
Vector 1
Vector 0
vswitch vswitch
iswitch
vdq
s*
vdq
s*
Pcond
Pblock
iswitch
Sector 3 Sector 1
Sector 1
Sector 4 Sector 6
Sector 2
Sector 2
Sector 5
θ
θ
Figure 8.24 Graphical analysis for the space vector PWM showing the (a) vectors and (b)
sectors (c) Losses associated to the switching states change A reference voltage in (d) Sector
1, and (e) Sector 2.
load voltage. All vectors Vs
x (x = 0, 2, … , 7) are shown in Fig. 8.24(a) as a graphical
representation of Table 8.3. The area between two adjacent non-null vectors defines
a sector as depicted in Fig. 8.24(b), which leads to six vectors.
It is possible to go from one vector to its adjacent one with just a single change
for the switching state. For instance, from Vector 1 to Vector 2, q2 is changed from
0 to 1, while q1 and q3 are kept constant. In the same way, from Vector 2 to Vector
3, q1 is changed from 1 to 0, while q2 and q3 are kept constant. It means that it is
possible to reduce the number of changes in the switching states by using adjacent
246 CHAPTER 8 OPTIMIZED PWM APPROACH
vectors to synthesize a specific value of the desired voltage. The strategy of applying
adjacent vectors plays an important role for converter losses reduction, since losses
appear each time it is necessary to change the switching states, as seen in Fig. 8.24(c).
To reduce the switching losses, if the desired voltage is inside Sector 1, the
Vectors 1 and 2 should be chosen [see Fig. 8.24(d)]. In the same way, if the desired
voltage is inside Sector 2, Vectors 2 and 3 should be chosen [see Fig. 8.24(e)], and
so on.
All pairs of adjacent vectors available in a three-leg converter are: (Vs
1
and Vs
2
),
(Vs
2
and Vs
3
), (Vs
3
and Vs
4
), (Vs
4
and Vs
5
), (Vs
5
and Vs
6
), and (Vs
6
and Vs
1
). Notice that
it is possible to define such a set of adjacent vectors in a generic way by using (Vs
k
and Vs
l
), with k = 1, … , 6, and l = k + 1 if k ≤ 5; and l = 1 if k = 6. The vectors
Vs
k
and Vs
l
have their dq components (see Table 8.3), that is, Vs
k
= Vs
dk
+ jVs
qk
and
Vs
l
= Vs
dl
+ jVs
ql
. The reference voltage 𝑣s∗
dq
can be obtained from a set of three-phase
reference voltages (𝑣s∗
123
) by using the transformation P given in (8.58). As mentioned
earlier, a switching sequence for q1, q2, and q3 should be chosen to allow the converter
to synthesize a given reference voltage 𝑣s∗
dq
, which is constant in the switching period
(Ts). In terms of average values, it is possible to write
1
Ts ∫
Ts
0
𝑣s∗
dqdt =
1
Ts ∫
tk
0
Vs
kdt +
1
Ts ∫
tl
0
Vs
l dt (8.63)
𝑣s∗
dq =
tk
Ts
Vs
k +
tl
Ts
Vs
l (8.64)
where tk and tl are intervals of time for application of the vectors Vs
k
and Vs
l
, respec-
tively. Rewriting (8.64) in terms of dq components, we get
𝑣s∗
d =
tk
Ts
Vs
kd +
tl
Ts
Vs
ld (8.65)
𝑣s∗
q =
tk
Ts
Vs
kq +
tl
Ts
Vs
lq (8.66)
Equations (8.65) and (8.66) show that the reference voltages can be obtained
from the interval of time for application of two adjacent vectors. From (8.65) and
(8.66) it is possible to write
tk =
𝑣s∗
d
Vs
lq
− 𝑣s∗
q Vs
ld
Vs
kd
Vs
lq
− Vs
ld
Vs
qk
Ts (8.67)
tl =
𝑣s∗
q Vs
kd
− 𝑣s∗
d
Vs
kq
Vs
kd
Vs
lq
− Vs
ld
Vs
qk
Ts (8.68)
To keep the switching frequency of the converter constant, it is necessary to
guarantee that the sum of the time for the application of the vectors is equal to Ts.
Then, the null vectors (Vectors 0 and 7 in Table 8.3) can be used to keep the switch-
ing frequency constant, that is, tk + tl + to = Ts, and then to = Ts − tk − tl. Note that
8.5 OTHER CONFIGURATIONS WITH CPWM 247
V0
s
V1
s
V1
s
V0
s
V2
s
V2
s
V7
s
V7
s
v10
Vdc/2
–Vdc/2
toi tof
Ts
v20
Vdc/2
–Vdc/2
v30
Vdc/2
–Vdc/2 Figure 8.25 Pulses defining how
the null vectors are divided at the
beginning and end of the switching
period.
there is a degree of freedom for to, meaning that this time could be divided between
the beginning (toi = 𝜇to) and the end [tof = (1 − 𝜇)to, 0 ≤ 𝜇 ≤ 1] of the sampling
interval, as presented in Fig. 8.25. Note that this approach brings benefits in terms of
THD reduction, since the pulse can be centered inside the sampling period.
A summary of the SPWM is presented in Fig. 8.26, which also shows the
algorithm for the implementation of the space vector modulation by using a MAT-
LAB code.
8.5 OTHER CONFIGURATIONS WITH CPWM
Although the SPWM approach represents one of the most popular options in indus-
trial applications, the CPWM is able to generate PWM signals with the same benefits
as in the SPWM. Furthermore, the expression derived in (8.19) is a generic way to
represent the auxiliary voltage 𝑣∗
h
. Such expressions can be employed in different con-
verters with at least one degree of freedom, that is, the number of voltages available
at the converter side higher than the number of voltage(s) demanded by the load. In
the following sections, a symmetrical two-phase motor drive system and a converter
for application in three-phase four-wire systems are employed as examples of the
comprehensiveness of the CPWM.
8.5.1 Three-Leg Converter—Two-Phase Machine
Two-phase motors can be found in home appliances, industrial tools, or small power
applications. Such a motor is often used in fixed speed drives. However, a dc–ac
power converter can be used when a variable motor speed operation is required. The
248 CHAPTER 8 OPTIMIZED PWM APPROACH
v123
s*
vdq
s*
Transformation
of variables
Definition
of sectors
and obtaining
k and l
Calculate
Calculate
Table 8.3
Equations
(8.67) and (8.68)
Vdk,Vqk,Vdl and Vql
s s s s
tk and tl
Figure 8.26 Algorithm for implementation of the SVPWM.
symmetrical two-phase motor can be considered as an interesting alternative for frac-
tional horsepower variable-speed drive, due to its characteristic of no pulsating torque
produced as observed in single-phase motors.
Since a symmetrical two-phase motor is a three-terminal electrical apparatus, a
three-leg converter can be used to supply it. Figure 8.27 shows a three-leg converter
supplying a two-phase symmetrical machine. Since this type of machine demands
two voltages in quadrature (𝑣∗
𝛼 and 𝑣∗
𝛽
), the reference pole voltages are as follows:
𝑣∗
10 = 𝑣∗
𝛼 + 𝑣∗
h (8.69)
𝑣∗
20 = 𝑣∗
𝛽 + 𝑣∗
h (8.70)
𝑣∗
30 = 𝑣∗
h (8.71)
where 𝑣∗
h
can be obtained directly from equation (8.49) with Vmax = MAX{𝑣∗
𝛼, 𝑣∗
𝛽
, 0}
and Vmin = MIN{𝑣∗
𝛼, 𝑣∗
𝛽
, 0}.
8.5 OTHER CONFIGURATIONS WITH CPWM 249
Vdc
0
1
2
3
iq1 iq2 iq3
–
+
+
vα
iα
iβ
in
–
+ vβ
–
q1 q2 q3
q1 q2 q3
n
Figure 8.27 Three-leg
converter supplying a
symmetrical two-phase
machine.
Exercise 8.3
Comparing the three-leg converter supplying a three-phase load (as in
Fig. 8.14) with the same converter supplying a two-phase load (as in
Fig. 8.27), determine the changes in the specification of the power switches
assuming that both machines have the same phase voltage, active power,
and power factor. Disregard any safety margin while specifying the power
switches.
8.5.2 Four-Leg Converter
Note that the three-phase and two-phase motor drive systems require the same topol-
ogy in terms of the number of switches employed. The difference is related to the
load (e.g., type of machine) connected to the converter and also in terms of control
considered for PWM and feedback strategies (if needed).
Similarly, the same CPWM approach can be employed for dc-ac converters
with four legs considered in different applications. Figure 8.28 shows a four-leg
converter feeding a three-phase four-wire system. In this type of application, there
Vdc
0
1
2
3
4
iq1 iq2 iq3 iq4
–
+
+
v1
i1
i2
i3
iN
–
+v2
–
+v3
–
q1 q2 q3 q4
q1 q2 q3 q4
Figure 8.28 Four-leg converter supplying a three-phase four-wire load.
250 CHAPTER 8 OPTIMIZED PWM APPROACH
Load
Source
υ1
Three-phase
load
–
+
υ2 –
+
υ3 –
+
υ1 –
+
υ2 –
+
υ3 –
+
1
2
3
4
1
2
3
4
Figure 8.29 Three-phase four-wire systems with: (left) balanced and (right) unbalanced
waveforms.
Vdc
0
1
2
3
4
iq1 iq2 iq3 iq4
–
+
+
v1
i1
i2
i3
i4
–
+v2
–
+v3
–
+v4
–
q1 q2 q3 q4
q1 q2 q3 q4
Figure 8.30 Four-leg converter supplying four-phase machine.
are two different scenarios: balanced three-phase voltages, as in Fig. 8.29 (left-hand
side), and unbalanced three-phase voltages, as in Fig. 8.29 (right-hand side). The
latter case is employed for applications such as dynamic-voltage-restorer and
series-active-power-filter.
On the other hand, Fig. 8.30 shows the same four-leg converter supplying a
four-phase machine. The PWM strategy with the inclusion of the voltage 𝑣∗
h
is still
valid for the converter with four legs, even considering the different applications
highlighted previously. The use of a four-phase machine drive system brings some
advantages such as eliminating the common mode, reducing the ratings of the power
switches, and providing fault tolerance characteristics for the drive system.
8.5 OTHER CONFIGURATIONS WITH CPWM 251
Exercise 8.4
(a) Write the PWM equations (reference pole voltages) for the four-leg con-
verter presented in Fig. 8.28 assuming both cases with balanced and unbal-
anced requirement. (b) Write the PWM equations for the four-leg converter
supplying a four-phase machine with balanced voltages. (c) Also, draw a block
diagram as in Fig. 8.15 for the (a) and (b) questions.
Application (Dynamic Voltage Restorer)
Dynamic voltage restorer (DVR) can be used to minimize the effect of operational
malfunction of the electric power grid, which can lead to sags or swells. The DVR’s
benefits of sustaining and restoring the voltage supply are especially important in
applications with critical loads requiring a regulated voltage. The operation principle
of this electrical apparatus is as follows: during the normal operation of the grid, the
static switch Q3 is turned on, while during sags or swells the switches Q1 and Q2 are
turned on to either add or subtract the grid voltage, as compensation voltage from
the DVR.
0
25%
35%
45%
55%
65%
100 200
ms
Sags
300 400 500
The figure below shows the compensation requirement for a typical situation
that shows a trend of deeper voltage sags with shorter duration, while moderate sags
Q3
Q1
Distribution
bus
Control
Charger
Load
Bus
Q2
LPF
252 CHAPTER 8 OPTIMIZED PWM APPROACH
occur for a longer period of time. The information provided in the graph below plays
an important role for designing the charger of the DVR.
The figure below presents the dynamic operation of the DVR highlighting the
grid voltage with a 100 ms sag duration. Note that this figure shows a sag with bal-
anced voltages, but it is quite common to have an unsymmetrical sag, which requires
a DVR implemented by a three-phase four-wire dc-ac converter.
Load voltage
DVR voltage
Grid voltage
100 ms
8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM
8.6.1 Inverter with Split-Wound Coupled Inductors
A converter having the same number of controlled power devices (six IGBTs) as in
the conventional three-leg converter (Fig. 8.14) but with higher number of levels is
presented in Fig. 8.31. Such a converter was presented in Section 7.3 with another
PWM approach, consisting of two carrier and one modulating signal per phase. The
Vdc
a1 c1
b1
a2 c2
b2
a
c
b
0
qa1
da1 db1 dc1
a
da2 db2 dc2
qb1 qc1
qa2 qb2 qc2
–
+va
–
+vb
–
+vc
Figure 8.31 Three-phase PWM inverter with split-wound coupled inductors.
8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 253
CPWM is presented in this section for the converter in Fig. 8.31 as an alternative
option. The main advantages of this converter when compared to the solutions pre-
sented in the technical literature are higher number of levels for the pole voltages and
no dead-time requirement for the converter’s operation.
Such a PWM inverter with split-wound coupled inductors is constituted by
switching power devices (qx1 − qx2, with x = a, b, c), six diodes (dx1 − dx2), and three
split-wound coupled inductors. The characteristics and the operation modes of this
converter are presented in Section 7.3.
The voltages 𝑣x10 and 𝑣x20 (voltages from the points x1 and x2 to the dc-link
capacitor midpoint) can be expressed as a function of the state of the switches qx1 and
qx2, respectively as follows:
𝑣x10 = (2qx1 − 1)
Vdc
2
(8.72)
𝑣x20 = (2qx2 − 1)
−Vdc
2
(8.73)
It means that each leg can be modeled as in Fig. 8.32(a). Then the pole voltages
𝑣x0 will be given by
𝑣x0 =
1
2
(𝑣x10 − 𝑣x20) (8.74)
Hence from (8.72)–(8.74) it is possible to write 𝑣x0 as a function only of the
state of the switches and dc-link voltage, as follows:
𝑣x0 = (qx1 − qx2)
Vdc
2
(8.75)
or
𝑣x0 = 𝑣x1 − 𝑣x2 (8.76)
where 𝑣x1 = qx1Vdc∕2 and 𝑣x2 = qx2Vdc∕2.
From (8.76) it is possible to model the three-phase converter as depicted in
Fig. 8.32(b).
If the desired voltage in the three-phase load is given by 𝑣∗
a, 𝑣∗
b
, and 𝑣∗
c , then
the reference pole voltage can be written as
𝑣∗
a0 = 𝑣∗
a + 𝑣∗
h (8.77)
𝑣∗
b0 = 𝑣∗
b + 𝑣∗
h (8.78)
𝑣∗
c0
= 𝑣∗
c + 𝑣∗
h (8.79)
where 𝑣∗
h
can be obtained directly from equation (8.49). Once the reference pole volt-
ages 𝑣∗
a0
, 𝑣∗
b0
, and 𝑣∗
c0
are defined from (8.77)–(8.79), the voltages from the points x1
and x2 (with x = a, b, c) with respect to 0 are given by
𝑣∗
x1
=
𝑣∗
x0
2
(8.80)
𝑣∗
x2 = −
𝑣∗
x0
2
(8.81)
The PWM signals generation from equations (8.80) and (8.81) can be done as
presented in Fig. 8.32(c).
254 CHAPTER 8 OPTIMIZED PWM APPROACH
(a) (b)
(c)
0 0
–
–
+
+
vx10 vb1
– +
vc1
–
–
–
–
+
+
+
+
va1
vb2
vc2
va2 –
+ va
–
+ vb
–
+ vc
ix
x
a
b
n
c
–
+
vx20
va
* va0
* va1
*
va2
*
vb0
*
vc0
*
vb
*
vc
*
vh
*
μ
vb1
*
vb2
*
vc1
*
vc2
*
vt
*
qa1
qa2
qb1
qb2
qc1
qc2
1/2
–1/2
1/2
–1/2
1/2
–1/2
Equations
(8.49)
–
+
–
+
–
+
–
+
–
+
–
+
Vdc
*
VMAX
MAX
MIN
*
VMIN
Figure 8.32 (a) Leg model. (b) Model of the three-phase PWM inverter with split-wound
coupled inductors. (c) Analog PWM implementation.
8.6.2 Z-Source Converter
The PWM dc–ac power converters presented in this book are predominantly char-
acterized as a voltage-source converter. However, in general terms, dc–ac power
converters can be divided into two main groups: voltage-source and current-source
converters, each one with its particular characteristics. The impedance-source con-
verter is an alternative type of power converter, which provides the unique feature of
buck and boost operation capability with the same number and same arrangement of
the semiconductor devices. Such a converter employs an impedance circuit to con-
nect the converter to the primary energy source, as seen in Fig. 8.33, and it is also
known as Z-source inverter.
Unlike the conventional dc–ac converter in which there is a need for dead time
to avoid short-circuit of the dc-link source, in the Z-source converter such short-circuit
(named as shoot-through zero state) is required to guarantee the boost operation of
the converter. In fact the Z-source converter is a buck-boost dc-ac converter with the
operation mode (buck or boost) defined by the PWM strategy.
8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 255
Vdc
L2
L1
C1 C2 a
b
c
Z-source
3 ~
motor
–
+
–
+
vi
vd
qa1 qb1 qc1
qa2 qb2 qc2
Figure 8.33 Z-source converter.
The circuit operates, boosting the input voltage (Vdc) if there is a short-circuit
time between two switches of the same leg for one, two, or three legs. On the other
hand, if there is no short-circuit time (as in a conventional converter) the circuit
will operate as a buck converter. Figure 8.34(a) and 8.34(b) show the equivalent
circuits considering the dc source (Vdc) point of view when the inverter is creating
a short-circuit and without a short-circuit, respectively. Note that when there is no
short-circuit, the inverter is represented by a current source ii, since it is assumed that
the load has inductive characteristics.
Considering an ideal and symmetrical circuit with L1 = L2 = L and C1 = C2 =
C, it leads to
VC1 = VC2 = VC (8.82)
𝑣L1 = 𝑣L2 = 𝑣L (8.83)
From Fig. 8.34(a), that is, during the short-circuit time (𝜏o), it is seen that
𝑣L = VC (8.84)
𝑣d = 2VC (8.85)
𝑣i = 0 (8.86)
On the other hand, from Fig. 8.34(b), during the conventional operation (𝜏N),
it yields
𝑣L = Vdc − VC (8.87)
𝑣d = Vdc (8.88)
𝑣i = 2VC − Vdc (8.89)
From equations (8.84)–(8.86) and (8.87)–(8.89) and since the average value
of the inductor voltage into one switching period (Ts) should be zero, it leads to
VL =
1
Ts ∫
t+Ts
t
𝑣Ldt =
𝜏oVC + 𝜏N(Vdc − VC)
Ts
= 0 (8.90)
where Ts = 𝜏N + 𝜏o.
256 CHAPTER 8 OPTIMIZED PWM APPROACH
(a)
(b)
Vdc Vdc
L1 iL1
iL2
vC1
vC2
L2
C1 C2
Diode
open
–
–
–
+
+
+
–
+
v
i
=
0
vd
Vdc
L1
L2
C1 C2
Diode
close
–
+
–
+
vd
vi
ii
Figure 8.34 (a) Equivalent circuit during the short-circuit. (b) Equivalent circuit during the
conventional operation.
Working on equation (8.90) it becomes
VC
Vdc
=
𝜏N
𝜏N − 𝜏o
(8.91)
The average voltage of the input converter side is given by
Vi =
𝜏N
𝜏N − 𝜏o
Vdc (8.92)
Finally, the peak dc-link voltage can be obtained as follows:
𝑣i = VC − 𝑣L (8.93)
𝑣i = 2VC − Vdc (8.94)
𝑣i =
1
1 − 2𝜏o∕Ts
Vdc = B ⋅ Vdc (8.95)
where B is the boost factor of the Z-source converter. Equation (8.95) means that for
any 𝜏o different from 0 the voltage value of the input side of the converter will be
higher than the voltage at the source side (Vdc), that is, boost operation. The capacitor
8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 257
voltages can also be obtained as a function of the shoot-through time (𝜏o):
VC1 = VC2 =
1 − 𝜏o∕Ts
1 − 2𝜏o∕Ts
Vdc (8.96)
To generate the PWM signals for the Z-source converter allowing the boost
operation it is necessary to include the short-circuit time (shoot-through). The CPWM
technique presented throughout this chapter can be applied to this type of converter as
well. In this case, in order to facilitate the demonstration of the PWM signal genera-
tion, the voltage of the input converter side (𝑣i) is divided into two parts, thus creating
a virtual zero point (“0”), as observed in Fig. 8.35(a).
Then, the pole voltages are defined as the voltage from the central point of the
leg to the point “0”. The pole voltages are: 𝑣a0, 𝑣b0, and 𝑣c0. Figure 8.35(b) shows the
generation of pole voltages through the comparison between the triangular and sinu-
soidal waveforms for the conventional (left-side) and Z-source (right-side) inverters.
The shoot-through zero states can be evenly distributed among the three-phase legs,
while the equivalent active vectors are unchanged. It can be seen from Fig. 8.35(b)
that 𝜏1 and 𝜏2 (time intervals of active vectors) have the same values for the conven-
tional and Z-source converters. During the shoot-through zero state intervals of time
the pole voltages are equal to zero, since 𝑣i = 0.
Exercise 8.5
Assuming that the circuit in Fig. 8.33 (Z-source topology) should be designed
to operate boosting this input voltage from 100V to 150V, what is the maxi-
mum modulation index (ma) obtained in this scenario?
8.6.3 Open-End Winding Motor Drive System
As mentioned in previous chapters of this book, besides the Δ and Y connections
there is another way to connect a three-phase machine in motor drive systems, which
is called open-end winding connection. Such a connection consists of a series arrange-
ment of two conventional two-level converters (inverters 1 and 2 in Fig. 8.36) through
the open-end windings of a three-phase machine. Note that in this case it is necessary
to have access to six terminals of the machine.
The converter pole voltages depend on the conduction states of the power
switches, that is
𝑣al0l
= (2qal − 1)
Vdcl
2
(8.97)
𝑣bl0l
= (2qbl − 1)
Vdcl
2
(8.98)
𝑣cl0l
= (2qcl − 1)
Vdcl
2
(8.99)
where l = 1 and 2.
258 CHAPTER 8 OPTIMIZED PWM APPROACH
(a)
(b)
Vdc1
Ts Ts
t
t
t
t
t
t
+ +
+
–
–
–
“Virtual”
zero point
vi = E
vt
* va
* vb
* vc
* vt
* va
* vb
* vc
*
τa
τo
τb
τ1 τ2 τ1 τ2
τc
τa
τb
τc
E
2
E
2
0
–
vb0
vc0
va0
E
2
3
τo
3
τo
6
τo
6
E
2
0
–
E
2
E
2
0
–
E
2
E
2
0
–
vb0
vc0
va0
E
2
E
2
0
–
E
2
E
2
0
–
E
2
E
2
0
qa1
a
b
c
qb1 qc1
qa2 qb2 qc2
Figure 8.35 (a) Inverter highlighting the virtual zero point “0”. (b) Generation of pole
voltages through sine-triangle modulation for conventional (left-side) and Z-source
(right-side) inverters.
8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 259
Vdc1 Vdc2
Inverter 1 Inverter 2
Three-phase
machine
a1 a2
c1 c2
b1 b2
01 02
qa1 qb1 qc1
qa1 qb1 qc1
qc2
–
+
qb2 qa2
qc2 qb2 qa2
va
–
+vb
–
+vc
Figure 8.36 Open-end winding machine supplied by two inverter series connected.
The motor phase voltages can be written as a function of the pole voltages and
as a function of the difference between the dc-link capacitor midpoints:
𝑣a = 𝑣a101
− 𝑣a202
+ 𝑣0102
(8.100)
𝑣b = 𝑣b101
− 𝑣b202
+ 𝑣0102
(8.101)
𝑣c = 𝑣c101
− 𝑣c202
+ 𝑣0102
(8.102)
where, for a balanced case it becomes
𝑣0102
= −
1
3
( c
∑
j=a
𝑣j101
−
c
∑
j=a
𝑣j202
)
(8.103)
Both power converters must generate appropriate reference voltages (𝑣∗
a, 𝑣∗
b
,
and 𝑣∗
c) for the three-phase machine. Due to the inherent redundancy of the voltages
demanded by a three-phase machine, the converters actually need to generate inde-
pendently two line-to-line voltages (e.g., 𝑣ab = 𝑣a − 𝑣b and 𝑣ca = 𝑣c − 𝑣a). For the
system presented in Fig. 8.36 there are four degrees of freedom in terms of the PWM
generation, since the converter has six legs and it needs to generate just two voltages.
Considering that the voltages 𝑣∗
ab
and 𝑣∗
ca should be imposed by the converter, four
auxiliary variables are introduced as presented in equations (8.104)–(8.109)
𝑣∗
ab = 𝑣∗
a101
− 𝑣∗
b101
− 𝑣∗
a202
+ 𝑣∗
b202
(8.104)
𝑣∗
ca = −𝑣∗
a101
+ 𝑣∗
c101
+ 𝑣∗
a202
− 𝑣∗
c202
(8.105)
𝑣∗
h0 = 𝑣∗
a101
− 𝑣∗
a202
(8.106)
𝑣∗
h1 = 𝑣∗
a202
(8.107)
𝑣∗
h2 = 𝑣∗
b202
(8.108)
𝑣∗
h3 = 𝑣∗
c202
(8.109)
It can be seen from these equations that both desired and auxiliary voltages
have been written as a function of the reference pole voltages. However, for the PWM
generation purposes, it is necessary to define the reference pole voltages as a function
260 CHAPTER 8 OPTIMIZED PWM APPROACH
of the desired and auxiliary voltages as follows:
𝑣∗
a101
= 𝑣∗
h0 + 𝑣∗
h1 (8.110)
𝑣∗
b101
= −𝑣∗
ab + 𝑣∗
h0 + 𝑣∗
h2 (8.111)
𝑣∗
c101
= 𝑣∗
ca + 𝑣∗
h0 + 𝑣∗
h3 (8.112)
𝑣∗
a202
= 𝑣∗
h1 (8.113)
𝑣∗
b202 = 𝑣∗
h2 (8.114)
𝑣∗
c202
= 𝑣∗
h3 (8.115)
It is also possible to define effective reference pole voltages since
𝑣∗
a120 = 𝑣∗
a101
− 𝑣∗
a202
(8.116)
𝑣∗
b120 = 𝑣∗
b101
− 𝑣∗
b202
(8.117)
𝑣∗
c120 = 𝑣∗
c101
− 𝑣∗
c202
(8.118)
Another convenient way to write the effective reference pole voltages is as
follows:
𝑣∗
a120 = 𝑣∗
h0 (8.119)
𝑣∗
b120 = −𝑣∗
ab + 𝑣∗
h0 (8.120)
𝑣∗
c120 = 𝑣∗
ca + 𝑣∗
h0 (8.121)
Equations (8.122)–(8.124) lead to a straightforward way to write the PWM
equations:
𝑣∗
a101
= 𝑣∗
a120 + 𝑣∗
h1 (8.122)
𝑣∗
b101
= 𝑣∗
b120 + 𝑣∗
h2 (8.123)
𝑣∗
c101
= 𝑣∗
c120 + 𝑣∗
h3 (8.124)
𝑣∗
a202
= 𝑣∗
h1 (8.125)
𝑣∗
b202
= 𝑣∗
h2 (8.126)
𝑣∗
c202
= 𝑣∗
h3 (8.127)
To finally define the reference pole voltages, it remains to determine the auxil-
iary voltages 𝑣∗
h0
, 𝑣∗
h1
, 𝑣∗
h2
, and 𝑣∗
h3
, as presented in the sequence:
The auxiliary voltage (𝑣∗
h0
) involves the desired line-to-line and effective pole
voltages. It is possible to define 𝑣∗
h0
respecting the following restriction
V0MIN ≤ 𝑣∗
h0 ≤ V0MAX (8.128)
with
V0MIN = MIN
{
−
Vdc1 + Vdc2
2
, −
Vdc1 + Vdc2
2
− 𝑣∗
ab, −
Vdc1 + Vdc2
2
+ 𝑣∗
ca
}
V0MAX = MAX
{
Vdc1 + Vdc2
2
,
Vdc1 + Vdc2
2
− 𝑣∗
ab,
Vdc1 + Vdc2
2
+ 𝑣∗
ca
}
REFERENCES 261
The voltages 𝑣∗
h0
can be defined as a function of 𝜇0 as in equation (8.129), which
is an adaption from equation (8.49):
𝑣∗
h0 = (1 − 𝜇0)V0MIN + 𝜇0V0MAX (8.129)
Using the auxiliary voltage 𝑣∗
h0
and the desired line-to-line voltage it is possible
to define the effective reference pole voltages. Finally to define the reference pole
voltages (8.122)–(8.127) it is necessary to find 𝑣∗
h1
, 𝑣∗
h2
, and 𝑣∗
h3
as in the sequence:
The auxiliary voltages (𝑣∗
h1
, 𝑣∗
h2
, and 𝑣∗
h3
) can be considered as three
single-phase auxiliary voltages, which are also restricted by
VkMIN ≤ 𝑣∗
hk ≤ VkMAX (8.130)
with k = 1, 2, 3; where the minimum and maximum values are given respectively by
𝑣∗
kMIN = MIN
{
−
Vdc1
2
− 𝑣∗
l120, −
Vdc2
2
}
𝑣∗
kMAX = MAX
{
Vdc1
2
− 𝑣∗
l120,
Vdc2
2
}
when k = 1 → l = a, k = 2 → l = b, and k = 3 → l = c.
The remaining auxiliary voltages (𝑣∗
hk
) can be calculated as presented below:
𝑣∗
hk = (1 − 𝜇k)VkMIN + 𝜇kVkMAX (8.131)
Equation (8.131) was obtained by following the same strategy as in
equation (8.19).
8.7 SUMMARY
This chapter presented a systematic way to implement an optimized PWM applied
to dc–ac converters [1–23]. It has been demonstrated that if the converter presents
a number of pole voltages higher than the number of desired output voltages, a
parameter 𝑣∗
h
can be added to improve either THD or efficiency of the converter.
Section 8.2 introduced such an optimization for the H-bridge converter along with
its model. Sections 8.3, 8.5, and 8.6 showed the same PWM technique for other
converters [24–32], that is: (i) three-leg converter feeding a two-phase load, (ii)
four-leg converter supplying a three-phase four-wire load, (iii) split-wound coupled
inductor converters, (iv) Z-source converter, and (v) open-end winding motor
drive system. Section 8.4 described the space vector modulation applied to the
conventional three-phase dc–ac converter.
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1969;5(6):672–679.
262 CHAPTER 8 OPTIMIZED PWM APPROACH
[3] Jardan KR. Modes of operation of three-phase inverters. IEEE Trans Ind Appl 1969;5(6):680–685.
[4] Busse A, Holtz J. Multiloop control of a unity power factor fast-switching AC to DC Converter.
Conference Record of IEEE Power Electronics Specialists Conference (PESC’82); 1982. p 171–179.
[5] Pffaf G, Weschta A, Wick A. Design and experimental results of a brushless AC servo drive. Con-
ference Record of IEEE/IAS Annual Meeting; 1982. p 692–697.
[6] Zubek J, Abbondanti A, Nordby CJ. Pulsewidth modulated inverter motor drives with improved mod-
ulation. IEEE Trans Ind Appl 1975;IA-11(6):1224–1228.
[7] Bowes SR, Mount MJ. Microprocessor control of PWM inverters. IEE Proc B 1981:293–305.
[8] Holtz J. Pulsewidth modulation for electronic power conversion. Proc IEEE 1994;82:1194–1214.
[9] Buja G, Indri G. Improvement of pulse width modulation techniques. Arch Elektrotech
1977;57:281–289.
[10] Depenbrock M. Pulse width control of a 3-phase inverter with non-sinusoidal phase voltages. Pro-
ceedings of the IEEE International Semiconductor Power Converter Conference, ISPCC’07; 1977.
p 399–403.
[11] Houldsworth JA, Grant DA. The use of harmonic distortion to increase the output voltage of a
three-phase PWM inverter. IEEE Trans Ind Appl 1984;IA-20(5):1224–1228.
[12] Agelidis VG, Ziogas PD, Joos G. Dead-band PWM switching patterns. IEEE Trans Power Electron
1996;11:523–531.
[13] Boost MA, Ziogas PD. State-of-the-art carrier PWM techniques: a critical evaluation. IEEE Trans
Ind Appl 1988;24:271–280.
[14] Ziogas PD, Moran L, Joos G, Vincenti D. A refined PWM scheme for voltage and current source
converter. Proceedings IEEE PESC’90; 1990. p 977–983.
[15] Seixas P. Commande numérique d’une machine synchrone autopilotée [D.Sc. Thesis]. L’Intitut
Nationale Polytechnique de Toulouse, INPT; 1988.
[16] Hava AM, Kerkman R, Lipo TA. A high-performance generalized discontinuous PWM algorithm.
IEEE Trans Ind Appl 1998;34:1059–1071.
[17] Holmes DG. The significance of zero space vector placement for carrier-based PWM schemes. IEEE
Trans Ind Appl 1996;32:1122–1129.
[18] Taniguchi K, Ogino Y, Irie H. PWM technique for power MOSFET inverter. IEEE Trans Power Elect
1988;3(3):328–334.
[19] Jacobina CB, Lima AMN, da Silva ERC, Alves RNC, Seixas PF. Digital scalar pulse-width mod-
ulation: a simple approach to introduce non-sinusoidal modulating waveforms. IEEE Trans Power
Electron 2001;16:351–359.
[20] Blasko V. A hybrid PWM strategy combining modified space vector and triangle comparison meth-
ods. Proc Conf. Rec. PESC; 1996. p 1872–1878.
[21] Trzynadlowski A, Legowski S. Minimum-loss vector PWM strategy for three-phase inverter. IEEE
Trans Power Electron 1994;9:26–34.
[22] van der Broeck HW, Skudelny HC, Stanke GV. Analysis and realization of a pulsewidth modulator
based on voltage space vector. IEEE Trans Ind Appl 1988;24(1):142–150.
[23] Holmes DG. The general relationship between regular-sampled pulse-width-modulation and space
vector modulation for hard switched converters. Conf. Rec. IEEE-IAS Annual Meeting; 1992.
p 1002–1009.
[24] Matsui K, Murai Y, Watanabe M, Kaneko M, Ueda F. A pulsewidth modulated inverter
with parallel-connected transistors by using current sharing reactors. IEEE Trans Ind Appl
1993;8(2):186–191.
[25] Salmon J, Ewanchuk J, Knight AM. PWM inverters using split-wound coupled inductors. IEEE Trans
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CHAPTER 9
CONTROL STRATEGIES FOR
POWER CONVERTERS
9.1 INTRODUCTION
After describing many topologies in Chapters 2–7, highlighting the circuits them-
selves, as well as optimized pulse width modulation (PWM) strategies in Chapter 8,
this chapter deals with the control actions needed to keep a specific variable of the
converter under control, for instance, in a motor drive system where the speed must be
controlled electronically through a power converter, or in a circuit designed to correct
the power factor actively. This chapter is strategically placed before the description
of back-to-back converters, due to the need for regulation of some variables, such
as grid current and dc-link capacitor voltage. It is worth mentioning that all power
converters previously presented were without any feedback control.
The types of controllers employed in applications with power converters
as controlled source can be basically classified into two main groups: lin-
ear and nonlinear controllers. Hysteresis and sliding-modes are examples of
nonlinear controllers, while proportional (P), proportional–integral (PI), and
proportional–integral–derivative (PID) regulators are examples of linear controllers.
The principle and characteristics of both types of controllers are introduced here.
Rather than providing deep analysis for each controller, this chapter aims to prepare
the reader for the next chapters, where the converters demand feedback control.
A dynamic simulation is an important aspect to test and validate control strate-
gies, since the behavior of the variables can be verified to predict the dynamics of
the system. MATLAB codes are presented for the control strategies developed in
this chapter as an effective way to verify the actions of the studied controllers. Also,
Euler’s integration method is employed to simulate the behavior of the state space
variables, due to its simplicity.
Following this introduction, Section 9.2 presents some principles of the con-
trollers for systems using power converters as actuators. Section 9.3 deals with a
nonlinear control technique called hysteresis control, highlighting some advantages
and disadvantages of this technique. Two applications are also considered in this
section: dc motor drive system and regulation of an ac variable. Although this book
deals with PWM converters processing ac voltage, the dc motor drive system plays an
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
264
9.2 BASIC CONTROL PRINCIPLES 265
important role in understanding a critical feature of the hysteresis control, switching
frequency changing with the load. The classic linear controllers (P, PI, and PID) are
presented in Section 9.4 for dc variables, while Section 9.5 presents a linear type of
controller for ac variables. A more complex control technique is presented in Section
9.6 with a cascade strategy for systems dealing with control of two variables with
different dynamic responses. The cascade control strategy is applied to regulate both
power factor and dc-link voltage in back-to-back converters for the next chapters.
Finally, Section 9.7 summarizes this chapter.
9.2 BASIC CONTROL PRINCIPLES
The system presented in Fig. 9.1(a) shows a Controlled Voltage Source supplying an
RL load. Let us assume that the control objective in this system is to guarantee the
load current regulation, that is, the measured output current (io) must follow a specific
reference value (i∗
o). Since the output voltage (𝑣o) has been employed to reach this
goal, a simple control block diagram can be obtained, as in Fig. 9.1(b). In this figure,
C(s) and H(s) are the controller and the RL load in the s-domain, respectively. The
transfer function of the H(s) is given by 1
Ls + R
.
A discretization method can be employed in order to simulate this system in a
digital way (e.g., by using a MATLAB code). One of the simplest ways to discretize a
specific process or system is to use the Euler discretization method. This is equivalent
of approximating the integrals by using the left-point rule. Hence, the first integral is
approximated as the product of the integrand at time t and the integration range dt,
which is called step size (h) for the digital implementation.
In the system of Fig. 9.1(a), for a given 𝑣o and considering a specific RL load,
the following equations can be obtained:
𝑣o = Rio + L
dio
dt
(9.1)
dio
dt
=
𝑣o − Rio
L
(9.2)
Considering the left-point rule, the discrete version of equation (9.2) can be
written as
io(t + h) = io(t) +
𝑣o − Rio
L
h (9.3)
C(s)
R
L
(a)
Controlled
voltage
source
(b)
–
–
+
H(s)
Σ
vo
vo
io
*
io
io
ei
Figure 9.1 (a) Controlled
voltage source feeding an RL
load. (b) Control block
diagram.
266 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
%Simulation of a RL load connected to a Controlled-
Voltage-Source
R=5; %Resistance of the RL load
L=0.05; %Inductance of the RL load
io=0; %state variable (load current)
vo=100; %input variable (load voltage)
h=1e-4; %step size
j=0; %variable used to storage the outcomes
t=0; %initial value of the digital time
tmax=1; %maximum simulation time
while t<=tmax, %begining of the simulation loop
t = t + h; %time incrementation
io = io + (vo-R*io)*h/L; %state space variable 1
% storage of the variables
j = j + 1;
time(j)=t;
current(j)=io;
voltage(j)=vo;
end
figure(1),plot(time,voltage)
figure(2),plot(time,current)
Figure 9.2 MATLAB code for the system presented in Fig. 9.1(a) for open loop operation.
Figure 9.2 shows the MATLAB code for the system presented in Fig. 9.1(a),
which simulates the behavior of the variables dynamically as well as plots their vari-
ables in the time domain. The output current for the open-loop operation has the
expected exponential behavior for a step voltage response, as observed in Fig. 9.3.
Note that the load current (io) is a function of both the load itself (which is normally
not controllable) and the output voltage 𝑣o, which is a variable used to control the
load current.
To implement the control block diagram presented in Fig. 9.1(b), and con-
sidering the digital implementation as done in the MATLAB code of Fig. 9.2, it is
necessary to add the code lines related to the controller C(s). For the sake of illustra-
tion let us consider a simple proportional controller for C(s), which means that the
output of this controller will define the voltage 𝑣o as follows:
𝑣o = Kei (9.4)
where K is the gain of the controller and ei is the current error.
Assuming a reference current as depicted in Fig. 9.4(a) with a desired step tran-
sient, the control system allows that the measured current io will follow its reference,
as observed in Fig. 9.4(b). Those waveforms were obtained with K = 200.
Due to the inductive characteristics of the load, the value of voltage to allow
this step transient of current is expected to be huge at the moment of the step
transient (theoretically an infinite voltage is needed to allow such a variation of
current). Figure 9.5(a) shows the output voltage of the controller, while Fig. 9.5(b)
highlights the instant of the step transient [zoom of Fig. 9.5(a) between t = 0.49 s
and t = 0.51 s]. Note that to guarantee a current step transient from 5 to −5 A as in
Fig. 9.4, the value of voltage almost reaches −2000 V.
9.2 BASIC CONTROL PRINCIPLES 267
100
0 0.05 0.1 0.15
50
0
v
o
(V)
t (s)
(a)
10
0 0.05 0.1 0.15
5
15
20
25
0
i
o
(A)
t (s)
(b)
Figure 9.3 (a) Output voltage.
(b) Output current.
5
0 0.2 0.4 0.6 0.8 1
0
–5
i
o
(A)
*
t (s)
(a)
5
0 0.2 0.4 0.6 0.8 1
0
–5
i
o
(A)
t (s)
(b)
Figure 9.4 (a) Reference load current
(b) Measured load current.
268 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
0
0 0.2 0.4 0.6 0.8 1
1000
–1000
–2000
v
o
(V)
*
t (s)
(a)
0
0.49 0.495 0.5 0.505 0.51
–1000
–2000
v
o
(V)
t (s)
(b)
Figure 9.5 (a) Load voltage needed
for a current step transient in
Fig. 9.4. (b) Zoom of the voltage
shown in Fig. 9.5(a).
Exercise 9.1
Write a MATLAB code to implement the control strategy shown in Fig. 9.1(b)
for an RL load (the reader is encouraged to use the code furnished in Fig. 9.2).
Plot the waveforms as in Figs 9.4 and 9.5. Additionally, explain the behavior
of the output voltage shown in Fig. 9.5 through the equations of the inductor
voltage.
In a real system, with the controlled voltage source having the maximum limit
well defined in terms of voltage and power deliverable to the load, the situation
observed in Fig. 9.5 is likely not possible. Even if a controller requires that amount
of voltage to guarantee a small current error (ideally zero) during the step transient,
there are practical limits for the voltage source, which will not allow such a condition.
Indeed, the control scheme presented in Fig. 9.1(b) does not show the controlled
voltage source (actuator) needed to implement this control scheme in a real-world
scenario. Note from Fig. 9.1(b) that the controller’s output defines the load voltage
directly. A more realistic system is considered in Fig. 9.6, in which the controlled
voltage source is added for the system through block G(s).
C(s) G(s) H(s)
Σ
*
vo vo io
*
io ei
–
Figure 9.6 Control block diagram
with inclusion of the controlled
voltage source.
9.2 BASIC CONTROL PRINCIPLES 269
if t>tpwm, % begin of the pwm loop simulation
tpwm=tpwm+hpwm; %definition of discrete time
cont=0; %auxiliar variable
v10r = vor/2; %pole voltage - leg 1
v20r = -vor/2; %pole voltage - leg 2
tal1 = (v10r/Vdc + 1/2)*hpwm; %Eq. (24) – Chapter 8
tal2 = (v20r/Vdc + 1/2)*hpwm; %Eq. (25) – Chapter 8
end% end of the pwm loop
cont=cont+h; % updating auxiliary variable
%Definition of the state of the switches
if(cont<tal1)
q1=1;
else
q1=0;
end
if(cont<tal2)
q2=1;
else
q2=0;
end
v10=(2*q1-1)*(Vdc/2); %Expression for the pole volt. 1
v20=(2*q2-1)*(Vdc/2); %Expression for the pole volt. 2
vo = v10 - v20; %Load voltage
Figure 9.7 MATLAB code for implementation of the digital PWM.
Block G(s) could be implemented with one of the PWM converters described
previously, but an H-bridge topology has been chosen and it will be used through-
out this chapter. Applications in a dc motor drive system and in a controlled rectifier
circuit will be considered later on in this chapter with the H-bridge converter imple-
menting G(s). Under the control point of view, the H-bridge converter must generate
a voltage at the load side (𝑣o) that represents accurately the voltage required by the
controller 𝑣∗
o. For an ideal controlled voltage source, it turns out that 𝑣o = 𝑣∗
o with
G(s) = 1. However, in terms of average value, the H-bridge topology G(s) can be
represented more realistically by a first order transfer function, with its time con-
stant equal to the switching period, G(s) = 1
Tss + 1
, where Ts = 1∕fs, and fs being the
switching frequency of the H-bridge topology.
A MATLAB code for an H-bridge converter can be written as in Fig. 9.7. The
expressions (9.24), (9.25) deduced in Chapter 8 have been considered in this code for
the digital implementation of the pulse widths (𝜏1 and 𝜏2). Note from this code that
there is a digital loop to emulate the interrupt in systems like Digital Signal Processors
(DSP). In order to implement a control system as seen in Fig. 9.6, the code lines for
the converter (Fig. 9.7) should be added in the program presented in Fig. 9.2.
Exercise 9.2
(a) Make a step transient for the reference voltage (𝑣∗
o) applied to the H-bridge
converter, that is, 𝑣∗
o = −80 V for t < 0.1 s and 𝑣∗
o = 80 V for t ≥ 0.1 s.
270 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
Compare this reference with the average of the output voltage to demonstrate
that this kind of converter can be represented approximately by a transfer
function given by G(s) = 1
Tss+1
. (b) Combine the code lines presented in Figs
9.2 and 9.7 to implement the closed-loop system as in Fig. 9.6, that is, with
the controlled voltage source as actuator; assume Vdc = 100 V.
The results of the closed-loop transfer function considering the H-bridge topol-
ogy as the controlled voltage source [G(s)] in Fig. 9.6 is presented in Fig. 9.8. When
the controller requires a voltage higher than the maximum voltage available through
the converter, the controlled voltage source (H-bridge topology) cannot follow this
requirement due to physical limitations/restrictions. In this particular case, the maxi-
mum and minimum voltages available on the H-bridge topology are 100 and −100 V,
respectively. As a consequence of using a non-ideal controlled voltage source, the
0
0 0.2 0.4 0.6 0.8 1
1000
–1000
–2000
–100
–5
0
5
0
100
v
o
(V)
i
o
(A)
v
o
(V)
*
t (s)
(a)
(b)
0 0.2 0.4 0.6 0.8 1
t (s)
(c)
0 0.2 0.4 0.6 0.8 1
t (s)
Figure 9.8 (a) Controller’s output
voltage (b) Converter’s output voltage
(c) Load current.
9.3 HYSTERESIS CONTROL 271
0
0.49 0.495 0.5 0.505 0.51
1000
–1000
–2000
–100
–5
0
5
0
100
v
o
(V)
v
o
(V)
i
o
(A)
*
t (s)
(a)
(b)
(c)
0.49 0.495 0.5 0.505 0.51
t (s)
0.49 0.495 0.5 0.505 0.51
t (s)
Figure 9.9 Zoom of the waveforms
presented in Fig. 9.8 around the
transient time (t = 0.5 s).
control actions will be delayed since instead of applying the necessary voltage to
guarantee that transient for the current, that is, 𝑣o ≅ −2000 V, the converter will
employ its minimum voltage of −100 V. The time transient will be affected, but
the control action is still active, as observed in Fig. 9.9, which shows a zoom of the
waveforms presented in Fig. 9.8 around the transient instant.
The proportional controller along with other linear regulators will be presented
with more details later on in this chapter. However, prior to analyzing deeply the linear
controllers, in the following section a hysteresis control strategy will be considered,
due to its simplicity.
9.3 HYSTERESIS CONTROL
The hysteresis control is one of the simplest ways to guarantee a current control in
systems as shown in Fig. 9.1(a). Unlike the linear controllers, such as the proportional
272 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
one considered in Section 9.2 in which the gains should be designed to obtain specific
characteristics, the hysteresis control will define directly the state of the switches of
the H-bridge topology to make the current follow its reference with a fixed value
for the maximum error given by Δi. Notice that the dynamics of the results (and
consequently the error) obtained in Figs 9.8 and 9.9 can be changed if another gain for
K is employed. Details of how to design the gains of linear controllers are furnished
in Section 9.4.
Figure 9.10 shows the implementation of the hysteresis-type current controller,
highlighting (i) the power and control parts of the circuit [Fig. 9.10(a)], (ii) the wave-
form of the variable under control (io) [Fig. 9.10(b) - top], and (iii) the switching
states q1 and q2 [Fig. 9.10(b) - middle and bottom]. In this case, the states of the
switches are defined as follows:
If io > i∗
o + Δi, the load current must be reduced, hence
q2 = on
(a)
(b)
0
0
5
0.01 0.02 0.03 0.04 0.05
Vdc
Hysteresis
loop
L R
–
–
+
io
*
io
ei
vo
io
q1
q2
q1 q2
q1 q2
i
o
,
i
o
(A)
*
0
0
1
0.5
0.01 0.02 0.03 0.04 0.05
q
1
0
0
1
0.5
0.01 0.02 0.03 0.04 0.05
q
2
t (s)
Figure 9.10 (a) Hysteresis controller defining the state of the switches. (b) Reference and
measured currents (top), and the state of the switches q1 and q2 (middle and bottom).
9.3 HYSTERESIS CONTROL 273
and
q1 = off
If io < i∗
o − Δi, the load current must be increase, hence
q1 = on
and
q2 = off
where Δi defines the hysteresis width below and above i∗
o. In steady state opera-
tion conditions, the load current ripple is constant. The results of the hysteresis control
for the same current transient presented before are shown in Fig. 9.11.
The startup condition for the hysteresis control is highlighted in Fig. 9.12 where
tr – interval of time in which io changes from 0 to i∗
o;
(a)
–5
5
0
0 0.5 1
t (s)
i
o
(A)
*
(b)
–5
5
0
0 0.5 1
t (s)
i
o
(A)
Figure 9.11 Hysteresis control:
reference load current and (b) measured
load current.
io
io
*
Δi
Δi
q1
tr
Ts
tα tβ
Figure 9.12 Startup transient for
the hysteresis control.
274 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
t𝛼 – time in steady state operation in which q1 is on;
t𝛽 – time in steady state operation in which q2 is on;
Ts – switching period.
During tr the behavior of the load current can be described as in equation (9.5)
io(t) =
Vdc
R
(
1 − e
−R
L
t
)
(9.5)
when t = tr the load current will be io = i∗
o, then
i∗
o =
Vdc
R
(
1 − e
−R
L
tr
)
(9.6)
tr = −
L
R
ln
(
1 −
Ri∗
o
Vdc
)
(9.7)
The rising time (tr) as well as the switching period (Ts = t𝛼 + t𝛽; in steady state
operation) are functions of the load parameters (R and L). Ts is also a function of the
hysteresis width (Δi).
Exercise 9.3
(a) Write a code in MATLAB to implement the hysteresis control as in
Fig. 9.10(a). (b) Validate the expression given in equation (9.7) for two differ-
ent RL loads. (c) By using the same simulation code show that the switching
frequency of the hysteresis control is dependent of the RL parameters by
filling the Table below.
R 5 Ω 10 Ω 50 Ω
L 5 mH 5 mH 5 mH
fs
SKSHS
Such a dependency of the switching period with the load can restrict the appli-
cation of this type of controller. For instance, in dc motor drive applications, in addi-
tion to the static components as in the RL load presented in Fig. 9.1(a), the load (dc
motor) has also a dynamic component, back electromotive force (emf), which is a
function of the rotor speed. This type of load affects directly the performance of the
hysteresis controller. This topic is addressed in Section 9.3.1.
Another characteristic of the hysteresis control is the constant ripple for the
load current, which is defined by 2Δi, that is, the instantaneous error is not zero in
the steady state operation. Ideally, to reach null error, Δi should be zero, which implies
a hypothetical scenario with infinite switching frequency.
9.3 HYSTERESIS CONTROL 275
Despite this disadvantage, it is possible to see some advantages of the hysteresis
control, such as simple implementation and there is no need to define the gains of the
controller as done for linear control approaches.
9.3.1 Application of the Hysteresis Control
for dc Motor Drive
The model of the dc motor is presented in this section in order to understand the
influence of a dynamic load in the switching frequency in a hysteresis control
approach.
A dc motor is constituted by two main magnetic circuits: (i) field circuit located
at the stator and (ii) armature circuit placed at the rotor. A sketch of this motor is
presented in Fig. 9.13(a), while Fig. 9.13(b) shows the electrical model for the motor,
which can be obtained as in equations (9.8) and (9.9):
𝑣f = Rf if + Lf
dif
dt
(9.8)
𝑣a = Raia + La
dia
dt
+ ea (9.9)
(a)
(b)
λf
λa
if
if
ia
υf
υf
υa
υa ea
Te
Tm
ωr
Tl
Field
circuit
R L
ia R L
M
e
c
h
a
n
i
c
a
l
l
o
a
d
Armature
circuit
+
+
–
+
–
+
–
+
–
–
Figure 9.13 (a)
Representation of a dc
motor. (b) Equivalent
circuit of the field (top) and
armature (bottom) circuits.
276 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
where ea = kc𝜆f 𝜔m is the back emf (electromotive force); kc is the coupling constant,
𝜆f is the field flux and 𝜔m is the mechanical speed. The electromagnetic torque is
produced due to the trend of the armature flux to align with the field flux, and then
the magnitude of this torque is obtained as follows:
Te = k′
c𝜆a𝜆f (9.10)
or
Te = kc𝜆f ia (9.11)
Applying Newton’s second law for rotation, that is, the net external torque is
equal to the moment of inertia times angular acceleration, then:
Te − Tl = Bm𝜔m + Jm
d𝜔m
dt
(9.12)
where Tl is the load torque, Bm is the damping coefficient and Jm is the moment of
inertia.
From equations (9.8), (9.9), and (9.12) it is possible to write the state space
representation for this type of machine, as in the following equations:
d
dt
[
ia
𝜔m
]
=
[
−Ra∕La − kc𝜆f ∕La
kc𝜆f ∕Jm −Bm∕Jm
] [
ia
𝜔m
]
+
[
1∕La 0
0 −1∕Jm
] [
𝑣a
Tl
]
(9.13)
𝜔m =
[
0 1
]
[
ia
𝜔m
]
+ [0]
[
𝑣a
Tl
]
(9.14)
where ia and 𝜔m are the state space variables.
Figure 9.14 shows the MATLAB code for the motor equations presented in
(9.13) and (9.14) with the Euler’s integration method.
Figure 9.15, in turn, shows the simulation results highlighting the state space
variables, that is, armature current and rotor angular speed. Besides the simplification
brought up by this model, it describes the dynamics of the system reasonably well.
Considering the hysteresis control described in this chapter, let us observe the
influence of the motor speed in the switching frequency for a constant hysteresis
width (2Δi).
For low speed, when the amplitude of the back emf is small (ea = kc𝜆f 𝜔m), the
switching frequency of the converter is high. On the other hand, for high speed, when
the amplitude of the back emf is high, the switching frequency is low. To explain this
behavior, a simulation has been performed with a dc motor connected to a mechani-
cal load, which presents a variable characteristic, that is, the torque demand increases
with speed squared. Examples of loads that exhibit this variable load torque charac-
teristic are centrifugal fans, pumps, and blowers.
Also, to illustrate how the switching frequency of the H-bridge converter can be
influenced by the motor speed with hysteresis control, a reference armature current is
set equal to 10 A for operation in high speed, and set up equal to 2.5 A for low speed
operation. The outcomes for the measured and reference currents are presented in
9.3 HYSTERESIS CONTROL 277
%constants
ra=0.06;
Laa=0.0018;
kf=0.1;
Bm=0.01;
Jm=0.001;
lambdaf=1;
%state variables
wm=0;
ia=0;
%input variables
va=1; %Armature voltage
Tl=.1; %Load torque
h=1e-4;%step size
j=0;
t=0;
tmax=2;
while t<=tmax,
t = t + h; % simulation time
ia=ia+(va/Laa-ra*ia/Laa-kf*lambdaf*wm/Laa)*h;%state
space 1
wm = wm + (kf*lambdaf*ia/Jm-Tl/Jm-Bm*wm/Jm)*h;%state
space 2
% storage the variables
j = j + 1;
time(j)=t;
armature_current(j)=ia;
rotor_speed(j)=wm;
end
figure(1),subplot(2,1,1),plot(time,armature_current)
subplot(2,1,2),plot(time,rotor_speed)
Figure 9.14 MATLAB code for implementation of the dc motor.
0.5 1
0
–2
0
2
4
6
8
10
t (s)
i
a
(A)
0.5 1
0
0
2
4
6
8
10
12
t (s)
(a) (b)
ω
m
(rad/s)
Figure 9.15 Dynamics of the dc
motor showing (a) armature
current and (b) rotor speed.
Fig. 9.16. As expected, the switching frequency is higher in low speed operation,
since T′′
s < T′
s then f′′
s > f′
s .
It is worth mentioning that the emphasis that has been given to show the vari-
ation of switching frequency in the hysteresis control approach is because it could
278 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
2.3
0
2
4
6
8
10
12
2.35 2.4 2.45 2.5 2.55 2.6 2.65 2.7
t (s)
Ts
' Ts
''
High speed
operation
Low speed
operation
i
a
,
i
a
(A)
Figure 9.16 Waveforms for reference and measured motor current for operation in high and
low speeds.
represent a problem in terms of the power electronics converter design. The specifica-
tions for the power switch normally consider current, blocking voltage, and switching
frequency. Such a power switch may not operate adequately if it is outside the fre-
quency range furnished by the manufacturer.
9.3.2 Hysteresis Control for Regulating an ac Variable
The previous discussions dealt with the hysteresis approach applied to control a dc
variable, that is, a dc current for both RL load and dc machine. The hysteresis control
is also useful for controlling ac variables with sinusoidal or non-sinusoidal wave-
forms. Examples of control systems requiring sinusoidal and non-sinusoidal wave-
forms are ac motor control systems (induction and synchronous motors) and active
power filters, respectively.
Figure 9.17 shows the implementation of the hysteresis-type current controller,
illustrating the circuit itself in Fig. 9.17(a) and the waveforms of the reference (i∗
o)
and measured (io) variables in Fig. 9.17(b) and 9.17(c), respectively. Figure 9.17(a) is
repeated here for convenience. Note in Fig. 9.17(a) that the definition of the states of
the switches is exactly the same as seen previously for the dc control. In Fig. 9.17(b)
there is an intentional transient in the current amplitude at t = 0.5 s to show the effec-
tiveness of this control strategy.
Exercise 9.4
With the approach established earlier to control the dc load current (see the def-
inition of the switching states in Section 9.3), the output voltage had only two
levels. Determine and simulate a hysteresis method to guarantee the current
control as well as to generate an output voltage with three levels.
9.4 LINEAR CONTROL—dc VARIABLE 279
(a)
(b)
0
–5
0
5
0.5 1
Vdc
Hysteresis
loop
L R
–
–
+
io
*
io
ei
vo
io
q1
q2
t (s)
q1 q2
q1 q2
i
o
(A)
(c)
0
–5
0
5
0.5 1
t (s)
i
o
(A)
Figure 9.17 (a) Hysteresis controller defining the state of the switches (b) Reference current
(c) Measured current.
9.4 LINEAR CONTROL—dc VARIABLE
9.4.1 Proportional Controller: RL Load
In Section 9.2 (Basic Control Principles) was presented a simple control approach
with a proportional controller, which is the simplest example of linear control. As pre-
viously presented in Fig. 9.4, for an ideal, controlled voltage source, and in Fig. 9.8,
for a nonideal controlled voltage source, it seems that the proportional controller is
able to guarantee error equal to zero. However, this type of controller cannot reach
280 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
null error for a system with a first order transfer function, like an RL load. Indeed,
analyzing in detail the waveforms in Figs 9.4 and 9.8 it is possible to realize that
those errors are not zero even for an ideal, controlled voltage source. The reader is
encouraged to plot those results by using his/her own simulation codes and observe
the error between the measured and reference currents.
Assuming an ideal controlled voltage source, as in Fig. 9.1(b), the open-loop
transfer function [F(s)] and closed-loop transfer function [M(s)] are given respec-
tively by
F(s) =
kp
R + sL
(9.15)
M(s) =
kp
(R + kp) + sL
(9.16)
Equation (9.16) shows that in the steady state operation M(s) is not equal to one.
When t → ∞ (steady state), s = jω → 0 – meaning that M(s) is equal to kp∕(R + kp).
It is evident that null error will be obtained when M(s) = 1, which is only possible if
kp → ∞. Also, for the case of using a non-ideal controlled voltage source (H-bridge
topology) represented by G(s) = 1
Tss+1
, null error will be obtained only when kp → ∞.
Unlike the hysteresis control, for which there is no need to specify gains, for
the linear approach, the gains of the controller must be obtained to guarantee specific
dynamic characteristics. A graphical analysis known as root locus can be used to
determine stability of the system, as well as to visualize the poles and zeros behavior
of the closed loop transfer function as a function of the proportional gain parameter,
as in Fig. 9.18. These graphs are helpful to determine the design of the proportional
controller (kp). For this simple example presented in Fig. 9.18 (i.e., proportional con-
troller plus a first order transfer function), the gain should be selected as large as
possible to minimize the error. Higher values of proportional gains (kp) guarantee
smaller steady-state error and faster response as well, see Fig. 9.18 for kp equal to
1, 5, and 20.
9.4.2 Proportional Controller: dc Motor Drive System
To analyze the proportional controller acting as a speed regulator in a dc motor drive
system, it is useful to find the transfer function for the motor, as it was done for
the RL load. Additionally, a detailed control block diagram will provide important
information about how the motor variables and control actions interact among
themselves.
From the state-space representation in equations (9.13) and (9.14), the transfer
function can be obtained as follows:
(s)
U(s)
= C(sI − A)−1
B + D (9.17)
where (s) and U(s) are the Laplace transformation for 𝜔m and input variables (𝑣a
and Tl), respectively. The matrices for the state-space representation are given by:
9.4 LINEAR CONTROL—dc VARIABLE 281
0
0
2
4
i
o
,
i
o
(A)
i
o
,
i
o
(A)
*
6
1 2
t (ms)
3 4 5 0
0
2
4
i
o
,
i
o
(A)
*
6
1 2
t (ms)
3 4 5
0
0
2
4
6
1 2
t (ms)
3 4 5
kp = 1
Re
Im
kp = 5
kp = 20
Figure 9.18 Root locus of the system in Fig. 9.1(b).
A =
[
−Ra
∕La
− kc
𝜆f
∕La
kc
𝜆f
∕Jm
−Bm
∕Jm
]
, B =
[
1∕La
0
0 −1∕Jm
]
, C =
[
0 1
]
and D = 0. The matrix I is a 2 × 2
identity matrix. Developing equation (9.17)
(s) = Ga(s)Va(s) + Gm(s)Tl(s) (9.18)
where Ga(s) =
ka
s2 + (sa + sm)s + k
=
ka
(s + s1)(s + s2)
with ka =
kc𝜆f
JmLa
. The poles of the system
can be written as follows:
s1 =
[
−
(
sa + sm
)
+
√
(sa + sm)2 − 4k
]
∕2
s2 =
[
−
(
sa + sm
)
−
√
(sa + sm)2 − 4k
]
∕2
with sa = ra∕La, sm = Bm∕Jm, and k = (raBm + k2
c𝜆2
f
)∕(JmLa).
Considering the model for a dc machine developed in equations (9.13) and
(9.14) it is possible to determine its block diagram, as presented in Fig. 9.19, where
kc is the coupling constant. This block diagram helps to understand how the variables
interact with each other. A simplified block diagram representation for this system
282 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
kc
kc
If
Ia Ia
Te
Ea
+
+
–
–
Lf
Vf
Va
Tl
Ω
Ω
Λf
+
1
Rf + sLf
1
Ra + sLa
1
Bm + sJm
×
Figure 9.19 Detailed block
diagram representation for a
dc-motor.
with one output (Ω) and two inputs (Va and Tl) is shown in Fig. 9.20(a). From the
speed controller perspective, the term Gm(s)Tl(s) can be considered as a disturbance
which must be compensated by the feedback control system.
Figure 9.20(b) shows the speed closed-loop control block diagram, while
Fig. 9.20(c) shows the same loop control without the disturbance term. The simplifi-
cation brought up by Fig. 9.20(c) means that it has been assumed that the controller
will be designed in such way that the disturbance term will be compensated by the
controller itself, then for simplification purposes, the disturbance can be neglected.
For a proportional controller [C(s) = kp] and assuming an ideal controlled volt-
age source, the open-loop transfer function [F(s)] and closed-loop transfer function
[M(s)] for the system presented in Fig. 9.20(c) are given respectively by
F(s) =
kpka
(T1s + 1)(T2s + 1)
(9.19)
M(s) =
kpka
(T1s + 1)(T2s + 1) + kpka
(9.20)
where T1 = 1∕s1 and T2 = 1∕s2.
Considering the steady state analysis (t → ∞ ⇒ s = jω → 0) for equation
(9.20), it turns out that M(s) = kpka∕(1 + kpka), which is different from a desirable
M(s) = 1 (i.e., null error). The error is not null, unless when kp → ∞, which goes to
an unrealistic scenario of infinite voltage needed to keep error equal to zero.
As observed in the root locus analysis presented in Fig 9.20(d), the consequence
of increasing kp (to reduce the steady state error) is that the imaginary parts of poles
will be much higher than the real part of the poles, bringing oscillation issues for
response.
9.4 LINEAR CONTROL—dc VARIABLE 283
(a)
(b)
(c)
(d)
Va
Tl
Va
Tl
–
–
Ω
Ω
Ω* EΩ
Ga(s)
Ga(s)
C(s)
Va
Im
Ω
Ω* EΩ
Ga(s)
C(s)
Gm(s)
Gm(s)
+
+
+
+
–S2
–S1 Re
Increasing kp
Increasing kp
Figure 9.20 (a) Simple block
diagram representation for a dc
machine drive system (b) Speed
closed-loop control (c) Speed
closed-loop control without the
disturbance term. (d) Root locus of the
dc motor drive system with
proportional controller.
9.4.3 Proportional-Integral Controller: RL Load
For a system with a first order transfer function (e.g., RL), the simplest linear con-
troller to guarantee null error is the proportional-integral one. For this type of con-
troller, the F(s) is given by
F(s) =
(
kp +
ki
s
) (
1
R + sL
)
(9.21)
Equation (9.21) can be conveniently rewritten as below:
F(s) =
ki
s
(
kp
ki
s + 1
) (
1∕R
L
R
s + 1
)
(9.22)
From equation (9.22) it is evident that the open-loop transfer function has a
pole placed at the origin of the complex plane, due to the ki∕s term, which means null
284 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
error at steady state operation. It also suggests that it is possible to cancel the zero of
the controller with the pole of the system (RL load), making
ki
kp
=
R
L
(9.23)
The zero-pole cancellation furnishes one possible design criterion for determin-
ing the gains of the proportional-integral controller. Then, considering equation (9.22)
and the zero-pole cancellation, the F(s) and M(s) are given respectively by
ki
sR
and
ki
sR+ki
. The root locus of the system is given in Fig. 9.21, which highlights three-step
responses for ki equal to 0.5, 1.5, and 2.5. Once one of the characteristics is picked
up from Fig. 9.21 for a specific value of ki, the gain kp will be defined from (9.23).
If the zero-pole cancellation is not employed to determine the gains of the
controller, the root locus will be clearly different, which could bring up an unde-
sired complex situation. Also, the determination of the gains of the controller is not
straightforward. Without zero-pole cancellation M(s) will be clearly a more complex
0
0
2
4
i
o
,
i
o
(A)
i
o
,
i
o
(A)
*
6
0.2 0.4
t (s)
0.6 0.8 1
0
0
2
4
6
0.2 0.4
t (s)
0.6 0.8 1
0
0
2
4
i
o
,
i
o
(A)
*
ki = 0.5
Re
Im
ki = 1.5
ki = 2.5
6
0.2 0.4
t (s)
0.6 0.8 1
Figure 9.21 Root locus for a PI controller and RL load.
9.4 LINEAR CONTROL—dc VARIABLE 285
system, as below:
M(s) =
skp + ki
s2L + s(R + kp) + ki
(9.24)
To test the proportional-integral controller by using the dynamic simulation (as
done previously with the MATLAB code), it is necessary to discretize the controller
itself. A discretization method using the Euler approach can also be used for simu-
lation of the controller. The block diagram model for the PI controller is shown in
Fig. 9.22, from which it is possible to determine the state space representation, as
below:
̇
x = kie (9.25)
y = x + kpe (9.26)
Exercise 9.5
Write a MATLAB code to implement a PI controller. Test this code by control-
ling an RL load current with both an ideal voltage source and with an H-bridge
topology as actuator.
For the case where a non-ideal controlled voltage source is considered, the F(s)
obtained in (9.22) is now given by:
ki
s
(kp
ki
s + 1
) (
1
Tss+1
) (
1∕R
L
R
s+1
)
. In this case, the
zero of the controller can be used to cancel one of the two poles, that is, s = −1∕Ts and
s = −R∕L. Normally, due to the high switching frequency of the power converters, the
dominant pole is s = −R∕L, which must be cancelled if a faster response is desired.
9.4.4 Proportional-Integral Controller: dc Motor
As in the case of the RL type of load, a proportional-integral controller is employed
to guarantee null error for a dc motor fed by an H-bridge converter. The control block
diagram presented in Fig. 9.20(c) and the transfer function of the motor given by
Output
of the
controller
e(t) y(t)
x(t)
x(t)
1
s
State space
variable
Error
kp
ki
Figure 9.22 Block diagram
representation for a PI
controller.
286 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
Ga(s) =
ka
(T1s+1)(T2s+1)
are considered in this analysis. In this case, unlike the RL load,
the system has two poles; one of these poles can be cancelled to obtain specific char-
acteristics, such as guarantee of faster dynamic response in a closed loop operation.
The open-loop transfer function F(s) after the zero-pole cancelation kp∕ki = T2 is
obtained as follows:
F(s) =
kika
s(T1s + 1)
(9.27)
With the dominant pole cancelled (s = −1∕T2), the M(s) is obtained as
M(s) =
kika
s(T1s + 1) + kika
(9.28)
Figure 9.23(a) and 9.23(b) shows the speed response for two cases, when the
slowest (dominant) pole is cancelled [Fig. 9.23(a)] and when fastest pole is can-
celled [Fig. 9.23(b)]. These results were obtained considering the parameters of the
dc machine in Fig. 9.14 assuming the same ki gain for both results, that is, ki = 2 and
kp = T1ki for Fig. 9.23(a); and with ki = 2 and kp = T2ki for Fig. 9.23(b).
Although the waveforms presented in Fig. 9.23(a) and 9.23(b) were obtained
with the same number for the integral gain ki = 2, it is also possible to determine the
gains of the controllers analytically by using a specific design criterion. For example,
Fig. 9.23(c) depicts the root locus of the dc motor with a PI controller after the cancel-
lation of the dominant pole. Despite the fact that this controller guarantees null error,
its limitation lies in the dynamics of the close-loop transfer function that is limited
by −1∕2T1 regardless of the rise of the gain ki. One possible analytical solution for
designing the gains of the PI controller can be identical poles for close-loop transfer
function, as in
ki =
1
4kaT1
(9.29)
kp = T2ki (9.30)
9.4.5 Proportional-Integral-Derivative Controller: dc Motor
As presented in the last section, the dc motor drive system with a PI controller has
one of its poles placed at the origin of the complex plane (i.e., s = 0), which assures
null error in steady state operation. From Fig. 9.23(c), however, it is evident that the
fastest response obtained with this controller is reached when it leads to the real part
of the dominant pole equal to −1∕(2T1).
If a faster response is needed, another controller must be employed. Note that
for the PI controller applied in this system, the dominant pole is always located on
the right side of the pole −1∕T1. A PID controller is able to obtain faster response for
a dc motor drive system than a PI type of controller, which has the following transfer
function:
C(s) = kp +
ki
s
+ kds (9.31)
9.4 LINEAR CONTROL—dc VARIABLE 287
(a)
(b)
(c)
0
0
2
4
6
8
0.2 0.4
t (s)
Rotor
speed
0.6 0.8 1
0
–1/2T1
–1/T1
0
2
4
6
8
0.2 0.4
t (s)
Rotor
speed
Im
Re
Increasing ki
Increasing ki
0.6 0.8 1
Figure 9.23 Speed dynamic
response for cancellation of (a)
slowest and (b) fastest pole (c) Root
locus of the dc motor with a PI
controller.
In fact, the derivative term of the controller cannot be implemented as it appears
in (9.31), as the transfer function of the PID controller will be:
C(s) = kp +
ki
s
+
kds
sTd + 1
(9.32)
or
C(s) =
(Tdkp + kd)s2 + (Tdki + kp)s + ki
s(Tds + 1)
(9.33)
where Td indicates the quality of the derivative part. Ideally Td must be equal to zero,
but its real value depends on the physical limitation of both actuator and system as a
whole.
The expression (9.33) shows that C(s) presents two poles: s = 0 and s = −1∕Td,
and two zeros. The zeros can be used to cancel both poles of the dc motor (as done
288 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
with the PI for cancellation of one pole). Moreover, the parameters kp and kd can be
employed to allocate the closed loop poles anywhere in the complex plane.
The following design of the controllers can be obtained for the condition of two
real identical poles:
ki =
1
Ti
=
1∕ka
4Td
(9.34)
kp =
T1 + T2 − Td
Ti
(9.35)
kd =
T1T2 − (T1 + T2 − Td)Td
Ti
(9.36)
9.5 LINEAR CONTROL—ac VARIABLE
Note that the linear regulators considered so far in this chapter have been employed
to control dc variables whether it is RL load or dc machine, current or speed. Two
of these controllers were able to guarantee null steady state error (i.e., PI and PID),
while the proportional one was not. Indeed, the integral part of the PI and PID con-
trollers goes to infinite for dc variables; since the operation frequency is zero, s = 0
and consequently ki∕s → ∞. Such a characteristic leads to a desirable zero error char-
acteristic.
However, for ac variables, which means s ≠ 0, there is no term in the controller
that tends to infinite, which leads to an error different from zero. For the case of ac
variables, it is necessary to use another PI type of controller, such as presented below:
C(s) =
kas2 + kbs + kc
(s2 + 𝜔2)
(9.37)
where ka, kb and kc are the gains of the controller. In this case, the controller presents
an infinite value for the rated frequency 𝜔.
The state space representation of this controller can be obtained as in
equations (9.38)–(9.40)
̇
x1 = x2 + kbe (9.38)
̇
x2 = −𝜔2
x1 + kde (9.39)
y = x1 + kae (9.40)
where x1 and x2 are state variables and kd = kc − 𝜔2ka.
After presenting controllers able to deal with dc and ac variables, it is important
to present other control approaches for systems that have more than one variable
to be regulated. For instance, a controlled rectifier circuit aims to guarantee power
factor correction with sinusoidal current as well as keep the output voltage constant.
The following section presents a control strategy regulating two variables known as
cascade control.
9.6 CASCADE CONTROL STRATEGIES 289
9.6 CASCADE CONTROL STRATEGIES
The control strategies described in this chapter have considered a schematic as pre-
sented in Fig. 9.1(b). This leads to a controlled voltage source implemented by a
dc–ac converter. For both types of loads (RL and dc motor) considered previously,
there is just one variable to be regulated, either current or speed. However, in some
applications there is a need to control two variables to reach specific requirements.
In this section a control approach called cascade control is presented for two appli-
cations, that is, power factor rectifier and dc motor drive system.
9.6.1 Rectifier Circuit: Voltage-Current Control
Figure 9.24(a) shows the circuit for a single-phase controlled rectifier, which has two
control objectives. They are: guarantee a regulated dc voltage (𝑣o) at the output and a
sinusoidal grid current (ig) with power factor close to one at input converter side. Both
control objectives are obtained simultaneously through the H-bridge power converter.
Before showing details about the control operation of the rectifier circuit pre-
sented in Fig. 9.24(a), it is convenient and simple to show the operation of a similar
(a)
(b)
L
C R
– – –
+ +
+
iq1 iq2
ig
eg vg
iC
vo
L
C R
– – –
+
+
+
iq1 iq2
Ig
Eg
Vg
iC
vo
Figure 9.24 (a) Rectifier circuit. (b)
Dc–dc converter.
290 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
circuit in terms of the control strategy, as in Fig. 9.24(b). This topology deals with
a dc to dc conversion [instead of ac to dc, as in Fig. 9.24(a)] and the principal goal
is to control the output voltage. Besides, there is no need to control the power fac-
tor; since the primary source of energy is dc, the control strategies for both circuits
in Fig. 9.24 can be established following the same principle, that is, using control
cascade scheme.
Equations (9.41) and (9.42) show that the capacitor current, and consequently
the capacitor voltage, can be regulated through Ig.
iC = −iq1 − iq2 −
𝑣o
R
(9.41)
iC = Ig(q1 − q2) −
𝑣o
R
(9.42)
Figure 9.25(a) depicts a control block diagram for the converter in Fig. 9.24(b).
The control structure for the controlled power factor rectifier in Fig. 9.24(a) is pre-
sented in Fig. 9.25(b). The difference between both control approaches for the con-
verters in Fig. 9.24(a) and 9.24(b) is the synchronization method for the power factor
correction.
9.6.2 Motor Drive: Speed-Current Control
The speed control of a dc motor, as presented in Fig. 9.20(c), was obtained directly
by defining the armature voltage (Va) as the output of the speed controller. Indeed,
(a)
(b)
– –
Ig
* Vg
* Vg Ig
eg
iC vo
Ig
Vo
*
Vo
Voltage
controller
Voltage
controller
Current
controller
Current
controller
TF of the
inductor
TF of the
inductor
Controlled
voltage
source
Controlled
voltage
source
1
Cv(s) G(s)
PLL
H(s)
sC
Eq.
(9.42)
Ci(s)
ev
Σ
Σ Σ
ei
– –
–
Ig
* vg
θ
* vg iC
ig vo
vo
*
vo 1
Cv(s) G(s)
sin(θ)
H(s)
sC
Eq.
(9.42)
Ci(s)
ev ei
eg
Eg
Σ
Σ Σ
X
*
ig
ig
Figure 9.25 Control block diagrams: (a) for the converter in Fig. 9.24(b). (b) for the
converter in Fig. 9.24(a).
9.6 CASCADE CONTROL STRATEGIES 291
+
–
+
–
–
–
Ia
* Va
* Va
Vf
Tl
If
1
Ω*
Ω
Ω
Ea
Te
Λf
×
×
Cω(s) Ci(s) Gv(s)
Ra + sLa
+
+
kc
kc
Lf
Ia Ia
1
Bm + sJm
1
Rf + sLf
Figure 9.26 Cascade control for a dc machine.
this control strategy was possible because Ω is a function of Va as shown in Fig. 9.19.
However, there are two blocks between these two variables (Fig. 9.19), which repre-
sent the electrical and mechanical dynamics for the motor. Fig. 9.26 suggests another
solution along with just one block in between the variable used to control (Va) and
the variable under control (Ia).
The control scheme using an outer controller for the speed (Ω) and an inner
controller for the armature current (Ia) is also known as a cascade control, which is in
fact the same principle as applied for the rectifier circuit presented in Section 9.6.1.
The cascade control is possible in this case because the mechanical and electrical
dynamics are completely different, with the internal loop much faster than the external
one. Both controllers C𝜔(s) and Ci(s) are PI type of controllers, since it is enough to
guarantee null error for the dc variables (Ia and Ω). Although using two controllers,
instead of just one as in Fig. 9.20, the main advantage of the cascade control is the
possibility to limit the armature current, which brings additional protection for the
machine.
Assuming that the mechanical variables are constants for the electrical variables
perspective, the internal control loop can be simplified as in Fig. 9.27. In this case,
the open loop transfer function is given by
Fi(s) =
ki
s
(
s
kp
kI
+ 1
) (
1
Tss + 1
) ⎛
⎜
⎜
⎝
1∕ra
La
ra
s + 1
⎞
⎟
⎟
⎠
(9.43)
+ +
–
–
Ia
*
Va
* Va Ia
Ea
1
Ci(s) Cv(s)
Ra + sLa Figure 9.27 Internal
control scheme for the
block diagram of Fig. 9.26.
292 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS
Canceling the zero of the controller with the pole of the motor, it yields
Fi(s) =
ki
s
(
1∕ra
Tss + 1
)
(9.44)
Consequently the close loop transfer function for the current control is given by
Mi(s) =
ki∕ra
Tss2 + s + ki∕ra
(9.45)
As seen before, the gain ki can be obtained by using either a root locus approach
or making identical poles, which means ki = ra∕(4Ts); then
Mi(s) =
1
(2Tss + 1)2
(9.46)
Since Ts is a small value, Mi(s) becomes
Mi(s) =
1
4Tss + 1
(9.47)
The external loop of the block diagram shown in Fig. 9.26 is given in Fig. 9.28.
Considering Tl as a perturbation to be compensated by the controller, the open loop
transfer function for the speed controller is given by
F𝜔(s) =
ki𝜔kc𝜆f
Bm
(kp𝜔
ki𝜔
s + 1
)
s
(
Jm
Bm
s + 1
)
(4Tss + 1)
(9.48)
Cancelling the zero with the pole we have
F𝜔(s) =
ki𝜔kc𝜆f
Bm
1
s(4Tss + 1)
(9.49)
Then the close loop transfer function is given by
M𝜔(s) =
ki𝜔kc𝜆f
Bm
4Tss2 + s +
ki𝜔kc𝜆f
Bm
(9.50)
Making identical poles we have
M𝜔(s) =
1
(8Tss + 1)2
(9.51)
Ia
+
–
* Ia
1
Ω
Ω* Te
Kc Λf
Mi(s)
Cω(s)
Bm + sJm
+
–
Tl
Figure 9.28 External loop of the controller in Fig. 9.26.
REFERENCES 293
From this approach it is possible to design the gains of the controller as follows:
kp𝜔
ki𝜔
=
Jm
Bm
with ki𝜔 =
Bm
16Tskckf
.
9.7 SUMMARY
This chapter presented the basic principles of controllers for systems using power
converters as actuators. This is indeed a preparation for the next chapters that will
need feedback control actions to guarantee the correct operation of the back-to-back
converters. This chapter is divided into two parts: nonlinear and linear control tech-
niques. Section 9.3 dealt with a nonlinear control technique, that is, hysteresis control,
highlighting some advantages and disadvantages. Two applications were also con-
sidered in this section: dc motor drive system and regulation of an ac variable. The
classic linear controllers (P, PI, and PID) were presented in Section 9.4 for dc vari-
ables, while Section 9.5 presented a linear type of controller for ac variables. A more
complex control technique was presented in Section 9.6 with a cascade strategy to
introduce back-to-back converters, which are described in the following chapters.
More details on the control techniques described can be found from 1 to 18.
REFERENCES
[1] L. Shang, D. Sun, J. Hu, Sliding-mode-based direct power control of grid-connected voltage-sourced
inverters under unbalanced network conditions, Power Electron, IET, vol. 4, no. 5, pp. 570–579, May
2011.
[2] R.-J. Wai, C.-Y. Lin, Dual active low-frequency ripple control for clean-energy power-conditioning
mechanism, IEEE Trans Ind Electron, vol. 58, no. 11, pp. 5172–5185, Nov. 2011.
[3] B. Labbe, B. Allard, X. Lin-Shi, D. Chesneau, An integrated sliding-mode buck converter with
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CHAPTER 10
SINGLE-PHASE
TO SINGLE-PHASE
BACK-TO-BACK CONVERTER
10.1 INTRODUCTION
Single-phase two-stage energy conversion systems are considered in this chapter.
Such conversion systems, also known as back-to-back converters, deal with recti-
fication and inversion through a dc-link capacitor. The control goals are high power
factor and sinusoidal current at the input side of the converter and regulated voltage
at its output side. Several applications require this type of conversion system, such
as line voltage regulators, universal active power filters, standby power supplies, and
uninterruptible power supplies.
Power blocks are again employed in this chapter as an effective way to under-
stand how the topologies presented in the technical literature have been conceived.
Furthermore, many of the subjects considered in the previous chapters (e.g., opti-
mized PWM and control strategies) are used to improve the converter’s operation
in terms of total harmonic distortion (THD) and efficiency, as well as to regulate the
variables of the back-to-back converter, such as grid power factor and dc-link voltage.
This chapter describes the full-bridge topology for single-phase ac–dc–ac con-
version in Section 10.2. In addition to the model, pulse width modulation (PWM),
and control strategies, a power analysis and an expression for the dc-link capaci-
tor oscillation are also presented in the section. Three sections of this chapter deal
with nonconventional topologies, that is, topologies with reduced (Section 10.3) and
increased (Sections 10.4 and 10.5) number of power semiconductor devices. Semi-
conductor component count reduction is obtained by either sharing a leg or by using
the dc-link mid-point connection. On the other hand, topologies with increased num-
ber of components are addressed by connecting back-to-back converters both in par-
allel and series. This will allow THD improvements and reducing power processed by
each converter. A summary of the chapter is presented in Section 10.6, while Section
10.7 shows the references.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
295
296 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
10.2 FULL-BRIDGE CONVERTER
10.2.1 Model
By connecting two PBs back-to-back, it is possible to build a single-phase to
single-phase ac–dc–ac as presented in Fig. 10.1(a). The representation using
switches is given in Fig. 10.1(b).
The conversion system consists of a single-phase utility grid, input inductor
(with reactance Xg), capacitor bank at the dc-link with two capacitors (each one with
capacitance equal to C), rectifier, inverter, and a single-phase load. Technically, the
dc-link capacitor bank in Fig. 10.1 could be implemented with just one capacitance.
However, for the sake of modeling, it is convenient to draw this circuit with two capac-
itors to have access to the point “0.” The inductive element (Lg) between the utility
grid and the input converter side is needed to avoid short-circuit between both volt-
age source type of element (grid and input converter side). Also, the dc-link bank is
needed to decouple input and output converter sides. Moreover, it is expected that the
input side of the converter in Fig. 10.1 operates as boost converter since the dc-link
voltage should be bigger than the grid voltage to guarantee grid current control. The
rectifier circuit constitutes switches qg1 and qg2, and their complementary switches
given respectively by qg1 and qg2. The inverter, in turn, constitutes switches ql1 and
ql2 and their complementary switches ql1 and ql2. As considered in previous chapters,
the conduction state of the switches is represented by a binary variable, where q = 1
indicates a closed switch while q = 0 is an open one with = g1, g2, l1, and l2. From
Fig. 10.1(b), the following equations can be derived for both input and output con-
verter sides as in equations (10.1) and (10.2), respectively:
𝑣g = 𝑣g10 − 𝑣g20 (10.1)
(a)
(b)
–
+
–
–
+ –
+
+
ig
iC
vC
il
vl
eg
vg
Xg
qg1 qg2
g1
g2
ql2
ql1
ql2
ql1
l1
l2
0
2
qg2
qg1
vC
vl
2
Figure 10.1 Two-leg converter supplying a single-phase load: (a) blocks and (b) switch
representation.
10.2 FULL-BRIDGE CONVERTER 297
𝑣l = 𝑣l10 − 𝑣l20 (10.2)
where the pole voltages can be written as a function of the states of the switches, as
follows:
𝑣g10 = (2qg1 − 1)
𝑣C
2
(10.3)
𝑣g20 = (2qg2 − 1)
𝑣C
2
(10.4)
𝑣l10 = (2ql1 − 1)
𝑣C
2
(10.5)
𝑣l20 = (2ql2 − 1)
𝑣C
2
(10.6)
Equation (10.7) furnishes the dynamic model for the variables of the grid con-
verter side:
𝑣g = eg − rgig − lg
dig
dt
(10.7)
where rg and lg represent the resistances and inductances of the input inductor.
The capacitor voltage can be obtained as follows:
𝑣c =
1
C∫
[(qg1 − qg2)ig + (ql2 − ql1)il]dt (10.8)
with the interval of integration equal to the switching frequency.
It is worth mentioning that the same approach used earlier in this book is con-
sidered in this chapter: (i) modeling the system by writing the voltage generated by
the converter as a function of the switching states, (ii) defining the switching states by
using a PWM technique, and (iii) obtaining the desired voltages for the PWM with
closed-loop operation.
10.2.2 PWM Strategy
The optimized PWM strategy presented in Chapter 8 can be employed for the
full-bridge configuration presented in Fig. 10.1 to improve either THD or efficiency
at both sides (input and output) of the converter.
If the desired input and output voltages are given respectively by 𝑣∗
g and 𝑣∗
l
, the
reference pole voltages can be written as follows:
𝑣∗
g10 = 𝑣∗
g + 𝑣∗
gh (10.9)
𝑣∗
g20 = 𝑣∗
gh (10.10)
𝑣∗
l10 = 𝑣∗
l + 𝑣∗
lh (10.11)
𝑣∗
l20 = 𝑣∗
lh (10.12)
298 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
The auxiliary voltages 𝑣∗
gh
and 𝑣∗
lh
are given respectively by
𝑣∗
gh = 𝑣C
(
𝜇g −
1
2
)
+ (𝜇g − 1)V∗
gmax − 𝜇gV∗
gmin
(10.13)
𝑣∗
lh = 𝑣C
(
𝜇l −
1
2
)
+ (𝜇l − 1)V∗
lmax − 𝜇lV∗
lmin
(10.14)
where Vgmax = MAX{𝑣∗
g, 0}, Vgmin = MIN{𝑣∗
g, 0} and Vlmax = MAX{𝑣∗
l
, 0}, Vlmin =
MIN{𝑣∗
l
, 0}; 𝜇g and 𝜇l are the distribution factor and determine how the free-wheeling
time can be distributed throughout the switching period. Note that 𝑣∗
gh
and 𝑣∗
lh
are
independent of each other. Equations (10.13) and (10.14) were deduced in Section
8.2.2.
Once the reference pole voltages have been defined in equations (10.9)–(10.12),
the pulse widths 𝜏g1, 𝜏g2, 𝜏l1, and 𝜏l2 can be calculated by equations (10.15)–(10.18),
as follows:
𝜏g1 =
(
𝑣∗
g10
𝑣C
+
1
2
)
Ts (10.15)
𝜏g2 =
(
𝑣∗
g20
𝑣C
+
1
2
)
Ts (10.16)
𝜏l1 =
(
𝑣∗
l10
𝑣C
+
1
2
)
Ts (10.17)
𝜏l2 =
(
𝑣∗
l20
𝑣C
+
1
2
)
Ts (10.18)
where Ts is the switching period.
10.2.3 Control Approach
Figure 10.2 presents the control block diagram for the system in Fig. 10.1. The input
power factor and the dc-link capacitor voltage are both controlled by using this control
approach. The output voltage is obtained by open-loop operation just setting up the
PWM signals for the legs l1 (i.e., switches ql1 –ql1) and l2 (i.e., switches ql2 –ql2).
Note that a cascade control approach is employed since the dynamics of the capacitor
voltage is completely different from the inner loop that deals with grid current.
The dc-link voltage 𝑣C is adjusted to its reference value 𝑣∗
C
using the controller
RC, which is implemented with a standard PI controller. This controller provides the
amplitude of the reference grid current I∗
g . To maintain the power factor close to one
with a sinusoidal grid current, the instantaneous reference current i∗
g must be syn-
chronized with the input voltage eg. Such a synchronization scheme can be obtained
via a PLL algorithm. The block Ge –ig is responsible for generating the reference
sinusoidal grid current in phase with the grid voltage i∗
g = I∗
g sin(𝜔gt + Φg), which
means that Φg is the phase angle of the grid voltage and 𝜔g is the grid frequency. The
current controller loop must deal with sinusoidal waveforms, which means that the
10.2 FULL-BRIDGE CONVERTER 299
–
–
+
+
ig
* vg
*
vgh
*
vlh
*
vl
*
ig
*
*
vC
vC
eg
Σ Σ
ig
μg
μl
RC Ri
PWM
Load
Rectifier/Inverter
Voltage
sensor
Voltage
sensor
Current
sensor
Grid
Ge-ig
Equation
(13)
Equation
(14)
qg1
qg2
ql2
ql1
Figure 10.2 Control strategy for the single-phase to single-phase converter.
conventional PI controller will not guarantee null error in steady-state operation – a
modified PI controller can be employed instead (see Section 9.5). As presented in
Fig. 10.2 and mentioned earlier, the output voltage control is obtained by open-loop
operation.
The PWM block presented in Fig. 10.2 can be implemented either from
equations (10.15)–(10.18) or by comparing these reference pole voltages with high
frequency carrier signals.
Exercise 10.1
Draw a block diagram system with a hysteresis current control instead of using
the linear controller Ri in Fig. 10.2. Is there any change for the number of
current and voltage sensors employed with the hysteresis control scheme?
10.2.4 Power Analysis
To find an expression of the capacitor voltage as a function of the system’s vari-
ables including the power demanded by the load, let us assume the following general
scenario:
Grid Voltage. eg(t) = Eg cos(𝜔gt)
Low Frequency Voltage of the Input Converter Side. 𝑣g(t) = Vg cos(𝜔gt − 𝜃g)
Grid Current. ig(t) = Ig cos(𝜔gt + Φg)
300 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
vg
eg
ig
vl
il
ϕg
ε
θg
ϕl
Figure 10.3 Phasor diagram for the low frequency
converter variables of Fig. 10.1.
Low Frequency Voltage of the Output Converter Side. 𝑣l(t) = Vl cos(𝜔lt + 𝜀)
Load Current. il(t) = Il cos(𝜔lt + 𝜀 + Φl)
All these variables are depicted in the phasor diagram presented in Fig. 10.3.
The effect of the high frequency voltages generated by the converters are neglected
to simplify the analysis. Also, for the sake of simplification, the phasors of the input
and output variables are considered in the same figure, which means that they have
the same frequencies.
The input and output powers are given by pg(t) = 𝑣g(t)ig(t) and pl(t) = 𝑣l(t)il(t),
respectively. Neglecting the converter power losses, the dc-link capacitor power can
be obtained as
pc(t) = pg(t) − pl(t) (10.19)
or
pc(t) =
[
VgIg
2
cos
(
𝜃g + Φg
)
−
VlIl
2
cos(Φl)
]
+
[
VgIg
2
cos
(
2𝜔gt − 𝜃g + Φg
)
−
VlIl
2
cos(2𝜔lt + 2𝜖 + Φl)
]
(10.20)
As long as the converter losses are neglected, the active power demanded by
the load is generated by the single-phase grid without losses through the conversion
stage, that is,
VgIg cos(𝜃g + Φg) = VlIl cos(Φl) (10.21)
Substituting (10.21) into (10.20), the capacitor power is given by
pc(t) =
VgIg
2
cos(2𝜔gt − 𝜃g + Φg) −
VlIl
2
cos(2𝜔lt + 2𝜖 + Φl) (10.22)
or
pc(t) = Nl
cos(Φl)
cos(𝜃g + Φg)
cos(2𝜔gt − 𝜃g + Φg) − Nl cos(2𝜔lt + 2𝜖 + Φl) (10.23)
where Nl = VlIl∕2.
10.2 FULL-BRIDGE CONVERTER 301
Equation (10.23) suggests that the pulsating powers inherent from single-phase
systems (at input and output sides of the converter) appear on the dc-link capaci-
tor bank.
One of the desired operation conditions is input power factor close to one,
which is obtained imposing Φg = 0 (see Fig. 10.3). Although there is no control for
some of the parameters in equation (10.23), such as Nl and Φl, the phase angle 𝜖 can
be employed to reduce the pulsating power on the dc-link capacitors if both input and
output converter sides have the same frequencies.
Exercise 10.2
Considering the input converter side modeled as a controlled voltage source
(𝑣g), as depicted in the figure below, determine the value of Xg for an
input power factor equal to one and assuming the following conditions:
eg(t) = 170 cos(2𝜋60t + 12∘), 𝑣g(t) = 204 cos(2𝜋60t) and with the amplitude
of the grid current equal to 10A. Assume an ideal inductance.
vg
ig
Xg
+
–
eg
+
–
10.2.5 dc-link Capacitor Voltage
The capacitor voltage can be achieved from capacitor power. Notice that
pc(t) = 𝑣cic = C𝑣c
d𝑣c
dt
(10.24)
this leads to
𝑣c
d𝑣c
dt
=
Nl
C
[
cos
(
Φl
)
cos(𝜃g + Φg)
cos(2𝜔gt − 𝜃g + Φg) − cos(2𝜔lt + 2𝜖 + Φl)
]
(10.25)
Applying an integral at both sides of equation (10.25), it is possible to write
𝑣2
c = Nl
⎡
⎢
⎢
⎣
cos
(
Φl
)
cos(𝜃g + Φg)
Xcg sin(2𝜔gt − 𝜃g + Φg)−
Xcl sin(2𝜔lt + 2𝜖 + Φl)
⎤
⎥
⎥
⎦
+ 𝑣c (10.26)
where Xcg = 1
𝜔gC
, Xcl = 1
𝜔lC
and 𝑣c is a dc value of 𝑣c.
302 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
vc
Δvc
t
0
Vc
Figure 10.4 Typical dc-link
voltage in single-phase
back-to-back converters.
Therefore, the capacitor voltage can be written as follows:
𝑣c =
√
𝑣c + ̃
𝑣c (10.27)
where ̃
𝑣c = NlXcl
[
cos(Φl)
cos(𝜃g+Φg)
fl
fg
sin(2𝜔gt − 𝜃g + Φg) − sin(2𝜔lt + 2𝜖 + Φl)
]
Once the dc-link voltage is well known as being composed of a dc value
overlapped by a small ac component, as in Fig. 10.4, it is possible to expand
equation (10.27) in a Taylor series around Vc. Since the Taylor series represents
a function as an infinite sum of terms that are calculated from the values of the
functions derivatives at a single point, the dc-link voltage can be expressed as
follows:
𝑣c = Vc +
̃
𝑣c
2Vc
−
̃
𝑣2
c
8Vc
+
∞
∑
n=3
[
(−1)n+1
n!
̃
𝑣n
c
2ñ
𝑣 2n−1
c
n
∏
j=2
(2j − 3)
]
(10.28)
The power series in (10.28) shows that the capacitor voltage consists of a dc
component and an ac component with infinite number of elements. However, for
practical values of the capacitor size and the dc-link reference voltage, the capaci-
tor voltage is well represented by the first two terms in (10.28) (i.e., Vc + (̃
𝑣c∕2Vc)).
This approximation results in the following expression:
𝑣c ≃ Vc +
NlXcl
2Vc
[
cos
(
Φl
)
cos(𝜃g + Φg)
fl
fg
sin(2𝜔gt − 𝜃g + Φg) − sin(2𝜔lt + 2𝜖 + Φl)
]
(10.29)
In order to analyze the voltage fluctuation, it is convenient to define the maxi-
mum (peak-to-peak) capacitor voltage as Δ𝑣c = 𝑣cmax − 𝑣cmin, where 𝑣cmax and 𝑣cmin
are the maximum and minimum values of 𝑣c in (10.29). The maximum value (𝑣cmax)
occurs when sin(2𝜔gt − 𝜃g + Φg) = 1 and sin(2𝜔lt + 2𝜖 + Φl) = −1 happen simulta-
neously, and the minimum value (𝑣cmin) occurs when sin(2𝜔gt − 𝜃g + Φg) = −1 and
sin(2𝜔lt + 2𝜖 + Φl) = 1 happen simultaneously. Hence,
𝑣cmax ≃ Vc +
NlXcl
2Vc
[
cos
(
Φl
)
cos(𝜃g + Φg)
fl
fg
+ 1
]
(10.30)
10.2 FULL-BRIDGE CONVERTER 303
𝑣cmin ≃ Vc −
NlXcl
2Vc
[
cos
(
Φl
)
cos(𝜃g + Φg)
fl
fg
+ 1
]
(10.31)
The dc-link voltage fluctuation is given by
Δ𝑣c ≃
NlXcl
Vc
[
cos
(
Φl
)
cos(𝜃g + Φg)
fl
fg
+ 1
]
(10.32)
From (10.32), it can be seen that the increase of the capacitance size reduces the
peak-to-peak voltage. For same grid and load frequencies (𝜔g = 𝜔l = 𝜔) and unitary
input power factor (cos Φg = 1), (10.29) can be written as follows:
𝑣c(t) ≃ Vc +
NlXc
2Vc
k𝜖 cos(2𝜔 + 𝛽) (10.33)
where
k𝜖 =
√
k2
Φ
− 2kΦ cos(𝜃g + 2𝜖 + Φl) + 1
kΦ = cos(Φl)∕ cos(𝜃g), Xc = 1∕𝜔C and
𝛽 = tan−1
[
cos Φl − cos
(
2𝜖 + Φl
)
cos Φl tan 𝜃g + sin(2𝜖 + Φl)
]
The term k𝜖 plays an important role for reduction of the pulsating voltage (Δ𝑣c)
on the capacitor voltage. If both grid and load have the same frequencies (e.g., unin-
terrupted power supply (UPS)) it is possible to use synchronization of the input and
output voltages to reduce k𝜖 and consequently reduce Δ𝑣c.
The maximum, minimum, and fluctuation values of 𝑣c are given respectively by
𝑣cmax ≃ Vc +
NlXc
2Vc
k𝜖 (10.34)
𝑣cmin ≃ Vc −
NlXc
2Vc
k𝜖 (10.35)
Δ𝑣c ≃
NlXc
Vc
k𝜖 (10.36)
The term k𝜖 reaches its maximum and minimum values for 𝜖 = −(𝜃g + 𝜙l +
𝜋)∕2 and 𝜖 = −(𝜃g + 𝜙l)∕2, respectively. Figure 10.5 shows k𝜖 as a function of the
load power factor 𝜙l for the following conditions: Nl = 1pu and Vl = Eg =
√
2pu.
𝜖 = 0 also guarantees a considerable reduction for k𝜖. In Fig. 10.5, 𝜙l < 0 means a
lagging power factor, while 𝜙l > 0 means a leading power factor.
Exercise 10.3
UPS is an electrical apparatus that is designed to provide power to a load even
when the input utility grid is not available. Such a device normally employs
304 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
ε = 0
k
ε
ε = –(θg + ϕl)/2
–90
0
0.5
1
1.5
2
2.5
–60 –30 0 30 60 90
ε = –(θg + ϕl + π)/2
ϕl (°)
Figure 10.5 k𝜀 as a function of the load power factor 𝜙l.
energy storage elements like batteries to furnish energy to the load when the
mains power fails. Assuming a single-phase to single-phase back-to-back con-
verter (as in Fig. 10.1) employed as an UPS with a set of batteries connected
to the dc-link voltage, and with a load frequency equal to the grid frequency,
determine the phase angle of the load voltage (𝜀) to obtain the minimum value
for the capacitor voltage oscillation. Consider that 𝜃g = 12∘, and that the input
and output power factors are given respectively by 1 and 0.85.
10.2.6 Capacitor Bank Design
In order to apply the input voltage with amplitude Vg and the output voltage with
amplitude Vl, the dc-link voltage 𝑣c should be larger than both Vg and Vl at any
instant of time. Figure 10.6(a) shows a case where an ideal scenario is considered
with a dc-link voltage without any fluctuation. The grid reference voltage is also pre-
sented in this figure. On the other hand, Fig. 10.6(b) depicts the case in which the
desired grid voltage cannot be generated appropriately because of the dc-link volt-
age fluctuation. Therefore, the minimum value of 𝑣c given in (10.35) must satisfy the
following equation:
𝑣cmin ≥ max{Vg, Vl} (10.37)
By choosing equation (10.37) as a minimum value for 𝑣c, the impedance Xcl
can be written from (10.31) as
Xcl =
Vc − max{Vg, Vl}
Nl
2Vc
(
cos(Φl)
cos(𝜃g + Φg)
fl
fg
+ 1
) (10.38)
10.2 FULL-BRIDGE CONVERTER 305
vc
Δvc
vg
*
vg
*
t
t 0
0
Vc
vc
Vc
(a) (b)
Figure 10.6 dc-Link voltage in
single-phase back-to-back
converters: (a) ideal scenario with no
oscillation and (b) real scenario with
a pulsating voltage on 𝑣c.
Once load and grid voltages are specified, the average value of the capacitance
must be chosen, based on the acceptable voltage fluctuation. Hence, the impedance
Xcl, and consequently the capacitor C, can be calculated from (10.38).
Exercise 10.4
For a single-phase back-to-back converter supplying a load with apparent
power equal to 2000 V-A, determine the capacitance value for the dc-link
assuming: 𝜃g = 12∘ with input and output power factors given respectively by
1 and 0.85. It is also known that the input and output voltages are the same
and are given by 120 V(RMS)–60Hz. Assume a maximum dc-link voltage
oscillation equal to 10 V.
Application (Uninterrupted Power Supply – UPS)
As mentioned earlier in this chapter, the single-phase back-to-back converter can
be employed as a UPS. The figure below (top) shows a simplified schematic of an
online UPS highlighting the operation modes, while the bottom part of the figure
shows the implementation of the online UPS with the configuration presented in
Fig. 10.1. This system is characterized by its ability to supply conditioned and regu-
lated power to a critical load during the normal and backup operations. Note that the
inverter is between the primary source of energies (grid or battery) and the load – this
system is also known as inverter-preferred or double-conversion UPS. In the case of
malfunction of the inverter, the bypass switch is turned on.
Normal
operation
Backup
operation
Load
Inverter
Rectifier
Grid
Bypass
switch
dc–dc
Battery
306 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
Bypass switch
Bidirectional
dc–dc converter
dc–dc
LPF
+
–
vl
+
–
eg
Another type of UPS is the line-interactive with the schematic presented in
the figure below. During the normal operation, the grid is connected to the load
directly through static switches. These switches are connected to multiple taps on
the secondary transformer to compensate grid voltage variation. Also, during nor-
mal operation, the circuit should be able to charge the battery without any additional
hardware – such a condition is obtained when the grid is feeding the load and con-
sequently there is voltage at the primary transformer. If both bottom switches of the
H-bridge converter are turned on simultaneously (i.e., short-circuit of the transformer
at the primary side) the current iBat will increase quickly. If the bottom switch is
turned off iBat will flow through the antiparallel diode of the top switch to the battery
and consequently charge it. The charging process is a high-frequency operation that
allows the current to go from the grid to the battery without any additional compo-
nent. During the backup operation, the load voltage is furnished with the following
parts: battery, H-bridge configuration, transformer, and capacitor. In this case the
static switches are all turned off.
Normal
operation
Backup
operation
Load
Grid
dc–ac
Battery
Static
switch
10.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 307
Static switch
1:n
+
–
vl
+
–
eg
iBat
10.3 TOPOLOGY WITH COMPONENT
COUNT REDUCTION
10.3.1 Model
Another single-phase back-to-back power converter is obtained by combining the
first and third PB-ac as in Fig. 10.7(a). Figure 10.7(b) shows the same configuration
with the switches represented. Note that the leg constituted by the switches qs –qs is
shared between the input and output sides of the converter.
As compared to the topology in Fig. 10.1 there is a reduction of 25% of the
number of power switches employed in the shared-leg converter. However, it is evi-
dent that the leg constituted by the switches qs and qs will handle a current that is
dependent on the input and output currents (ig − il). Also, as discussed later in this
section, the shared-leg plays an important role in the voltage capability of the con-
verter. It is worth mentioning that the cost reduction will be effective if what is saved
by reducing the number of semiconductor devices is not lost in higher device ratings
and more electrolytic capacitor energy storage to keep the same conditions as in the
full-bridge converter. The following equations can be derived from Fig. 10.7(b) for
both input and output converter sides:
𝑣g = 𝑣g0 − 𝑣s0 (10.39)
𝑣l = 𝑣l0 − 𝑣s0 (10.40)
The pole voltages can be written as a function of the states of the switches:
𝑣g0 = (2qg − 1)
𝑣C
2
(10.41)
𝑣s0 = (2qs − 1)
𝑣C
2
(10.42)
𝑣l0 = (2ql − 1)
𝑣C
2
(10.43)
308 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
(a)
(b)
–
–
+
+
–
–
+
+
ig
vg
iC
vC
il
vl
eg
vg
Xg
qg qs ql
qg qs ql
ql1
s
l
0 vl
Figure 10.7 Shared-leg single-phase to single-phase back-to-back converter: (a) block and
(b) switch representation.
Equation (10.7) is still valid for modeling the input converter side. However,
the capacitor voltage is given by
𝑣c =
1
C∫
[igqg + (il − ig)qs − ilql]dt (10.44)
with the interval of integration equal to the switching period.
10.3.2 PWM Strategy
If the desired input and output voltages are given respectively by 𝑣∗
g and 𝑣∗
l
, one option
for the reference pole voltages is as follows:
𝑣∗
g0
= 𝑣∗
g + 𝑣∗
h (10.45)
𝑣∗
s0 = 𝑣∗
h (10.46)
𝑣∗
l0
= 𝑣∗
l + 𝑣∗
h (10.47)
Unlike the previous full-bridge converter that has employed two auxiliary volt-
ages 𝑣∗
gh
and 𝑣∗
lh
to optimize both converter sides independently, the PWM strategy
presented in (10.45)-(10.47) uses just one variable 𝑣∗
h
due to the coupling between
the input and output sides of the converter through the leg constituted by the switches
10.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 309
qs –qs. 𝑣∗
h
is given by
𝑣∗
h = 𝑣C
(
𝜇 −
1
2
)
+ (𝜇 − 1)V∗
max − 𝜇V∗
min
(10.48)
with Vmax = MAX{𝑣∗
g, 0, 𝑣∗
l
} and Vmin = MIN{𝑣∗
g, 0, 𝑣∗
l
}.
Once the reference pole voltages have been defined, pulse widths 𝜏g, 𝜏s, and 𝜏l
are given by
𝜏g =
(
𝑣∗
g0
𝑣C
+
1
2
)
Ts (10.49)
𝜏s =
(
𝑣∗
s0
𝑣C
+
1
2
)
Ts (10.50)
𝜏l =
(
𝑣∗
l0
𝑣C
+
1
2
)
Ts (10.51)
Exercise 10.5
Draw the control block diagram for the converter shown in Fig. 10.7 by adapt-
ing the cascade control strategy shown in Fig. 10.2.
10.3.3 dc-link Voltage Requirement
As aforementioned, the shared-leg presented in Fig. 10.7 will affect the dc-link volt-
age needed to guarantee the same input and output voltages as in the full-bridge
circuit. To simplify the analysis let us assume that the dc-link capacitance is large
enough to have Δ𝑣c ≃ 0. The dc-link voltage for the converter shown in Fig. 10.1
must obey the requirement of 𝑣c ≥ max{𝑣g, 𝑣l}, where 𝑣g and 𝑣l are the voltage desir-
able at the input and output converter sides, respectively. Indeed, 𝑣c is obtained from
the statement that the maximum value of the difference between any combinations
of pole voltages will define the dc-link voltage. For the topology with shared-leg in
Fig. 10.7 it yields
𝑣c ≥ max{𝑣∗
g0 − 𝑣∗
s0, 𝑣∗
l0 − 𝑣∗
s0, 𝑣∗
g0 − 𝑣∗
l0} (10.52)
or
𝑣c ≥ max{𝑣∗
g, 𝑣∗
l , 𝑣∗
g − 𝑣∗
l } (10.53)
If the load and grid frequencies are different, the term 𝑣∗
g − 𝑣∗
l
will be bigger
than either 𝑣∗
g or 𝑣∗
l
and consequently will define 𝑣c. However, if both sides of the
converter require the same frequency, the output voltage can be generated to minimize
the effect of the term 𝑣∗
g − 𝑣∗
l
. This will allow the shared-leg converter to operate with
the same dc-link voltage as the full-bridge converter.
310 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
(a)
(b)
–
–
+
+
–
–
+
+
ig
vg
iC
vC
il
vl
eg
vg
Xg
qg
g
ql
l
l2
0
qg ql
vl
Figure 10.8 Half-bridge
single-phase to single-phase
back-to-back converter: (a)
block and (b) switch
representation.
10.3.4 Half-Bridge Converter
A back-to-back configuration with half-bridge at both converter sides (as in Fig. 10.8)
guarantees another level of component count reduction as compared to the topology
in Fig. 10.7. However, in this case there is a low frequency current flowing through
the capacitors due to the dc-link midpoint connection to the load and grid, which will
increase the voltage fluctuation on these elements and affect their losses.
The voltage at the input and output converter sides are determined directly from
the pole voltages 𝑣g0 and 𝑣l0, which are defined by equations (10.41) and (10.43),
respectively. Also, the PWM equations are straightforward since there is no degree
of freedom, that is, there are only two legs to process two voltages. In this case, it is
not possible to use auxiliary voltage to optimize some parameters of the circuit.
10.4 TOPOLOGIES WITH INCREASED NUMBER
OF SWITCHES (CONVERTERS IN PARALLEL)
The search for topologies with a reduced number of components continued over a
considerable period of time. This can be, in part, explained by the high cost of the
power switch when compared to other elements of the converter. However, as the
price of the semiconductor was going down, this tendency changed, and recently
10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 311
Figure 10.9 Single-phase to single-phase back-to-back converter with switches in parallel.
the configurations with an increased number of components appear as an interesting
option, especially in terms of reliability, efficiency, and distortions improvement.
Particularly, the connection of converters in parallel can be justified if the rat-
ings of the power switches available in the market cannot handle the level of current
demanded for a specific application. Indeed, connecting switches in parallel is the
simplest solution when the currents needed are higher than the rated currents of the
switches, as shown in Fig. 10.9 for the single-phase back-to-back converter.
Although the number of power switches is twice as compared to that in
Fig. 10.1, the characteristics of the converter in Fig. 10.9 in terms of quality of the
waveform generated are the same as in the conventional solution. As described in
the following sections, connecting back-to-back converters in parallel instead of
switches in parallel have the following benefits: (i) increase the current capability
of the converter and (ii) improve the quality of the waveforms generated by the
converter at the input and output sides.
10.4.1 Model
Connecting converters in parallel allows reducing the level of current and conse-
quently power processed by each converter. Another advantage is reducing outer
current ripple with interleaved technique. Figure 10.10 shows a single-phase to
single-phase energy conversion unit with two back-to-back converters in parallel.
Such a conversion unit consists of four PBs-ac [see Fig. 10.10(a)], or in other words,
the converters 1, 2, 3, and 4 [see Fig. 10.10(b)], single-phase load, four inductive
filters (L1a, L1b, L3a, and L3b) at the grid side, four more inductive filters (L2a, L2b,
L4a, and L4b) at the load side, and two dc-link capacitor banks.
Considering converters 1 and 3 (converters at the grid side), it is possible to
write the following equations:
eg = z1ai1a − z1bi1b + 𝑣1 (10.54)
eg = z3ai3a − z3bi3b + 𝑣3 (10.55)
ig = i1a + i3a (10.56)
312 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
(a)
(b)
–
+
+
–
+
–
ig
eg
iC
il
vl
vg
L1a
i1a
i1b
L1b
L2a
i2a
i2b
L2b
q1a q1b
1a
1b
2a
2b
01
q2b q2a
Converter 1 Converter 2
vl
vC1
2
+
–
vC1
2
q1a q1b q2b q2a
+
–
iC
L3b
i3b
i3a
L3a
L4b
i4b
i4a
L4a
q3a q3b
3a
3b
4a
4b
02
q4b q4a
Converter 3 Converter 4
vC2
2
+
–
vC2
2
q3a q3b q4b q4a
Figure 10.10 Single-phase to single-phase back-to-back converter connected in parallel: (a)
block and (b) switch representation.
where z1a = r1a + l1ap, z1b = r1b + l1bp, z3a = r3a + l3ap, and z3b = r3b + l3bp are the
impedances of the inductors L1a, L1b, L3a, and L3b, respectively; with p = d∕dt. The
voltages 𝑣1 and 𝑣3 are given by 𝑣1a01
− 𝑣1b01
and 𝑣3a02
− 𝑣3b02
, respectively.
For the converters at the load side, it yields:
𝑣l = −z2ai2a + z2bi2b + 𝑣2 (10.57)
𝑣l = −z4ai4a + z4bi4b + 𝑣4 (10.58)
il = i2a + i4a (10.59)
where z2a = r2a + l2ap, z2b = r2b + l2bp, z4a = r4a + l4ap, and z4b = r4b + l4bp are the
impedances of the inductors L2a, L2b, L4a, and L4b, respectively. The voltages 𝑣2 and
𝑣4 are given by 𝑣2a01
− 𝑣1b01
and 𝑣4a02
− 𝑣4b02
, respectively.
10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 313
i1o i2o
i3o i4o
io
io
io
0
io
Figure 10.11 Circulating current between both back-to-back converters in parallel.
Since there is no transformer for isolation purpose, there exists a circulation
current between both back-to-back converters as highlighted in Fig. 10.11. The fol-
lowing equations can be written from the circuit in Fig. 10.10:
z1ai1a − z3ai3a + z2ai2a − z4ai4a + 𝑣1a01
− 𝑣3a02
− 𝑣2a01
+ 𝑣4a02
= 0 (10.60)
z1ai1a − z3ai3a + z2bi2b − z4bi4b + 𝑣1a01
− 𝑣3a02
− 𝑣2b01
+ 𝑣4b02
= 0 (10.61)
z1bib − z3bi3b + z2ai2a − z4ai4a + 𝑣1b01
− 𝑣3b02
− 𝑣2a01
+ 𝑣4a02
= 0 (10.62)
z1bi1b − z3bi3b + z2bi2b − z4bi4b + 𝑣1b01
− 𝑣3b02
− 𝑣2b01
+ 𝑣4b02
= 0 (10.63)
Equations (10.60)–(10.63) were obtained with the following meshes (see
Fig. 10.10) 1a–2a–4a–3a, 1a–2b–4b–3a, 1b–2a–3b–4a, and 1b–2b–3b–4b,
respectively.
An expression for the circulating voltage can be obtained by adding
equations (10.60)–(10.63):
𝑣o = z1ai1a + z1bi1b − z3ai3a − z3bi3b + z2ai2a
+ z2bi2b − z4ai4a − z4bi4b (10.64)
with
𝑣o = −𝑣1a01
− 𝑣1b01
+ 𝑣3a02
+ 𝑣3b02
+ 𝑣2a01
+ 𝑣2b01
− 𝑣4a02
− 𝑣4b02
(10.65)
314 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
The circulating currents in Fig. 10.11 are given by
i1o = i1a + i1b (10.66)
i3o = i3a + i3b (10.67)
i2o = i2a + i2b (10.68)
i4o = i4a + i4b (10.69)
As seen in Fig. 10.11, the circulating current is in fact a single current that
circulates among the converters. Such a current can be written as
io = i1o = −i3o = i2o = −i4o (10.70)
Then substituting equations (10.66)–(10.69) into (10.54)–(10.59), it is possi-
ble to model the parallel converter as follows:
eg = (z1a + z1b)i1a − z1bio + 𝑣1 (10.71)
eg = (z3a + z3b)i3a + z3bio + 𝑣3 (10.72)
el = −(z2a + z2b)i2a + z2bio + 𝑣2 (10.73)
el = −(z4a + z4b)i4a + z4bio + 𝑣4 (10.74)
𝑣o = (z1a − z1b)i1a − (z3a − z3b)i3a − (z2a − z2b)i2a + (z4a − z4b)i4a
+ (z1b + z3b + z2b + z4b)io (10.75)
There are two components for the circulating current, that is, high and low
frequencies components. The high-frequency component is due to the difference of
the deadtime for each converter and also due to asymmetry of the power switches
employed in both stages. Such high-frequency components are not modeled in
equation (10.75). However, the model furnished in (10.75) considers the low fre-
quency component for the circulating current. For instance, any level of imbalance
between Lxa and Lxb (with x = 1, 2, 3, and 4) can be identified from this model.
The current io can be compensated (tracking a zero reference) with an additional
controller, as described in Section 10.4.3. Also, the dynamic model obtained from
equations (10.71)–(10.75) suggests that the voltage 𝑣1 is employed to control i1a,
and the voltage 𝑣3 is employed to control i3a. With these two currents (i1a and i3a)
under control, the grid current is also controlled [see equation (10.56)]. The voltage
𝑣o is employed to control io.
Considering a balanced case where z1a = z1b = z3a = z3b = z1 and z2a = z2b =
z4a = z4b = z2, the dynamic model is simplified by the following equations:
eg = 2z1i1a − z1io + 𝑣1 (10.76)
eg = 2z1i3a + z1io + 𝑣3 (10.77)
el = −2z2i2a + z2io + 𝑣2 (10.78)
el = −2z2i4a − z2io + 𝑣4 (10.79)
𝑣o = 2(z1 + z2)io (10.80)
10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 315
10.4.2 PWM Strategy
From the model presented earlier, it is possible to write the reference voltages as a
function of the reference pole voltages:
𝑣∗
1 = 𝑣∗
1a01
− 𝑣∗
1b01
(10.81)
𝑣∗
2 = 𝑣∗
2a01
− 𝑣∗
2b01
(10.82)
𝑣∗
3 = 𝑣∗
3a02
− 𝑣∗
3b02
(10.83)
𝑣∗
4 = 𝑣∗
4a02
− 𝑣∗
4b02
(10.84)
𝑣∗
o = −𝑣∗
1a01
− 𝑣∗
1b01
+ 𝑣∗
3a02
+ 𝑣∗
3b02
+ 𝑣∗
2a01
+ 𝑣∗
2b01
− 𝑣∗
4a02
− 𝑣∗
4b02
(10.85)
There are eight pole voltages and just five variables to control, two variables
associated to the grid current (𝑣∗
1
and 𝑣∗
3
), one variable to deal with the circulating
current (𝑣∗
o), and finally two more variables to handle load voltage control (𝑣∗
2
and
𝑣∗
4
). There exist, therefore, three degrees of freedom, that is, three auxiliary variables.
Those auxiliary variables can be defined as follows:
𝑣∗
x =
𝑣∗
1a01
+ 𝑣∗
1b01
2
(10.86)
𝑣∗
y =
𝑣∗
2a01
+ 𝑣∗
2b01
2
(10.87)
𝑣∗
z =
𝑣∗
4a02
+ 𝑣∗
4b02
2
(10.88)
From equations (10.86)–(10.88) it is possible to define the reference pole volt-
ages as follows:
𝑣∗
1a01
=
𝑣∗
1
2
+ 𝑣∗
x (10.89)
𝑣∗
1b01
= −
𝑣∗
1
2
+ 𝑣∗
x (10.90)
𝑣∗
3a02
=
𝑣∗
3
2
+
𝑣∗
o
2
− 𝑣∗
y + 𝑣∗
z + 𝑣∗
x (10.91)
𝑣∗
3b02
= −
𝑣∗
3
2
+
𝑣∗
o
2
− 𝑣∗
y + 𝑣∗
z + 𝑣∗
x (10.92)
𝑣∗
2a01
=
𝑣∗
2
2
+ 𝑣∗
y (10.93)
𝑣∗
2b01
= −
𝑣∗
2
2
+ 𝑣∗
y (10.94)
𝑣∗
4a02
=
𝑣∗
4
2
+ 𝑣∗
z (10.95)
𝑣∗
4b02
= −
𝑣∗
4
2
+ 𝑣∗
z (10.96)
The reference pole voltages are defined as a function of the desirable voltages
(defined by the controllers) 𝑣∗
1
, 𝑣∗
2
, 𝑣∗
3
, and 𝑣∗
4
as well as the auxiliary voltages 𝑣∗
x , 𝑣∗
y ,
316 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
and 𝑣∗
z . Note that the auxiliary voltages can be defined independently as follows, if
equations (10.100)–(10.105) are satisfied:
𝑣∗
x = 𝜇x𝑣∗
xMAX + (1 − 𝜇x)𝑣∗
xMIN (10.97)
𝑣∗
y = 𝜇y𝑣∗
yMAX + (1 − 𝜇y)𝑣∗
yMIN (10.98)
𝑣∗
z = 𝜇z𝑣∗
zMAX + (1 − 𝜇z)𝑣∗
zMIN (10.99)
where
𝑣∗
xMAX =
𝑣∗
c1
2
− max|V∗
x | (10.100)
𝑣∗
xMIN = −
𝑣∗
c1
2
− min|V∗
x | (10.101)
𝑣∗
yMAX =
𝑣∗
c1
2
− max|V∗
y | (10.102)
𝑣∗
yMIN = −
𝑣∗
c1
2
− min|V∗
y | (10.103)
𝑣∗
zMAX
=
𝑣∗
c2
2
− max|V∗
z | (10.104)
𝑣∗
zMIN = −
𝑣∗
c2
2
− min|V∗
z | (10.105)
with V∗
x =
{𝑣∗
1
2
,
−𝑣∗
1
2
,
𝑣∗
3
2
+
𝑣∗
o
2
− 𝑣∗
y + 𝑣∗
z , −
𝑣∗
3
2
+
𝑣∗
o
2
− 𝑣∗
y + 𝑣∗
z
}
, V∗
y =
{𝑣∗
2
2
, −
𝑣∗
2
2
}
and V∗
z =
{𝑣∗
4
2
, −
𝑣∗
4
2
}
; and 0 ≤ 𝜇x ≤ 1, 0 ≤ 𝜇y ≤ 1, and 0 ≤ 𝜇z ≤ 1.
The gating signals of the power switches can be obtained by either comparing
the reference pole voltages (10.89)–(10.96) with carrier waveforms or in a digital
way by programming timers. Since there are two converters connected in parallel,
an interleaved technique can be employed to reduce the current ripple. Figure 10.12
shows the carrier signals (𝑣∗
t1
and 𝑣∗
t2
) for the interleaved technique. In this case, 𝑣∗
t1
is employed for converters 1 and 2, while 𝑣∗
t2
is employed for converters 3 and 4.
Figure 10.13 shows the output of the parallel topology highlighting the influence of
the interleaved technique. Notice that since the ripple of i2a is shifted by 180 electri-
cal degrees (considering the switching frequency) from the ripple of i4a, the output
current will have a smoother ripple since il = i2a + i4a.
10.4.3 Control Strategy
The control block diagram for the parallel back-to-back converter is given in
Fig. 10.14. The dc-link voltages are regulated by the controllers Rc1 and Rc3. The
output of these controllers defines the amplitude of the currents in converters 1 and
3, respectively. The block Gi creates sinusoidal currents (i∗
1a
and i∗
3a
) in phase with
the grid voltage; this is a PLL-based block. The controllers Ri1 and Ri3 regulate the
currents i1a and i3a, and the output of these controllers define the voltages (𝑣∗
1
and 𝑣∗
3
)
employed in the PWM technique described previously. The circulating current is
10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 317
vt1
* vt2
*
t
Figure 10.12 Carrier signals for the
interleaved technique applied to the
parallel converters.
i2a
i4a
i2a
2a
L2a
i4a
4a
L4a
il
il
il
Figure 10.13 Output of the parallel back-to-back converter with interleaved technique.
regulated by using the controller Ro. The block k𝑣 can be employed to compensate
imbalance among the inductors; for a balanced case k𝑣 = 0.5.
Exercise 10.6
Assuming well-designed controllers for the parallel topology presented in
Fig. 10.10, that is, power factor equal to one, circulating current equal to
zero, and dc-link capacitor voltages under control, specify the power switches
employed in this configuration in terms of current and voltage with: (i) the
active power of the load is Pl = 1700W with cos(Φl) = 0.85, load voltage
with 120Vrms – 60 Hz, (ii) dc-link voltage fluctuation equal to zero, and (iii) a
drop voltage due to the inductors Lxa and Lxb (x = 1, 2, 3, 4) equal to 5Vrms on
each inductor.
318 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
–
–
+
–
+
–
–
–
–
vC1
*
vC1
–
+ vl
–
+ vC2
v1
*
v3
*
v2
*
v4
*
vo
*
I1
* i1a
*
io
i3a
i1a q1a
L1a L1b L3b L3a
L2a L2b L4b L4a
q3a
q3b
q1b
q2a
Conv. 2
Conv. 3
Conv. 1
Conv. 4
q4a
q4b
q2b
i1a
i1b
i3a
*
io
*
vl
*
I3
*
vC2
*
vC1
eg
vC2
Rc1
Gi
Ri1
Ri3
Ro1
PWM
kv
(1 – kv)
Rc3
Σ
Σ
Σ
Σ
Σ
Σ
Figure 10.14 Control block diagram of the parallel single-phase back-to-back converter.
10.5 TOPOLOGIES WITH INCREASED NUMBER
OF SWITCHES (CONVERTERS IN SERIES)
Connecting single-phase to single-phase converters in parallel brings up interest-
ing characteristics such as reduction of the current processed by each power switch
and interleaved PWM, which allows current ripple reduction. Following a similar
approach, it is also possible to connect single-phase to single-phase back-to-back
converters in series as seen in Fig. 10.15. Figure 10.15(a) shows the power block
representation while Fig. 10.15(b) depicts the representation with switches. In this
case, it is necessary for half of the dc-link voltage to have the same voltage capability
of the conventional single back-to-back converter. Also the load and grid will give
the back-to-back converters an H-bridge cascade configuration, that is, as a multi-
level converter (see Chapter 5). The only difference between the input/output of the
converter in Fig. 10.15 and the cascade topology in Chapter 5 is a circulating current
between both back-to-back units since there is no isolation. Such a circulating current
can be determined from the model, as described in the later. It is worth mentioning
that the majority of the topologies presented in Chapter 5 have isolated dc sources.
The following equations can be derived from the converter in Fig. 10.15(b).
eg = z1ig + 𝑣1ab + z2i′
g + 𝑣2ab (10.106)
𝑣l = 𝑣1cd + 𝑣2cd (10.107)
10.5 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN SERIES) 319
(a)
(b)
+
–
+
–
ig
io
eg
vl
vg
L1
q1a q1b q1c q1d
q1a q1b q1c q1d
1a
01
1b
1c
1d
Converter 1
Converter 2
vC1
2
+
–
+
–
vC1
2
+
–
L2
q2a
q2a
q2b q2c q2d
q2b q2c q2d
2a
02
2b
2c
2d
vC2
2
+
–
vC2
2
ig
′
il
′
il
vl
Figure 10.15 Series connection of the single-phase to single-phase back-to-back converters.
where z1 = r1 + pl1, z2 = r2 + pl2 with p = d∕dt; 𝑣1ab = 𝑣1a01
− 𝑣1b01
, 𝑣2ab =
𝑣2a02
− 𝑣2b02
, 𝑣1cd = 𝑣1c01
− 𝑣1d01
, and 𝑣2cd = 𝑣2c02
− 𝑣2d02
.
Since this is a transformerless configuration, there are circulating meshes,
which can be modeled by equations (10.108) and (10.109):
eg = z1ig + 𝑣1ac + 𝑣l − 𝑣2bd (10.108)
0 = 𝑣1bd − 𝑣2ac − z2i′
g (10.109)
320 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER
Adding (10.108) and (10.109), it is possible to define the circulating voltage as
follows:
𝑣o = eg − z1ig + z2i′
g = 𝑣1ac + 𝑣1bd − 𝑣2ac − 𝑣2bd + 𝑣l (10.110)
Ideally ig = i′
g and il = −i′
l
. However, due to the circulating current we have
i′
g = ig − io (10.111)
i′
l = −il + io (10.112)
The dynamic model of the converter can be rewritten from (10.106) as follows:
eg = z1ig + z2ig − z2io + 𝑣g (10.113)
where 𝑣g = 𝑣1ab + 𝑣2ab. From equation (10.110), the model for the circulating voltage
can be written in terms of io as
𝑣o = eg + (z2 − z1)ig − z2io (10.114)
For a balanced case with z1 = z2 we have
eg = 2z1ig − z1io + 𝑣g (10.115)
𝑣o = eg − z2io (10.116)
The PWM approach described for the series back-to-back converter can be
adapted from the solution employed in the parallel converter presented in the previous
section.
–
–
–
–
–
+
–
+
Ig
*
vg
*
vg
*
vo
*
vl
*
vl
–
+vC2
–
+vC1
io
*
io
v1ab
*
v2ab
*
v1cd
*
v2cd
*
ig
*
vC1+vC2
vC1
* *
vC1+vC2
*
vC1
eg ig
Σ
Σ
Σ
Σ
Rc
Rc1
Ro
½
½
Gi Rg
k1
L1
L2
k1
(1–k1)
PWM
Conv. 1
(Rectif.)
Conv. 1
(Invert.)
Conv. 2
(Invert.)
Conv. 2
(Rectif.)
q1a
q2a
q1b
q2b
q1c
q2c
q1d
q2d
Figure 10.16 Control block diagram of the single back-to-back converter series connected.
REFERENCES 321
The control strategy is shown in Fig. 10.16. Since the current ig affects both
dc-link voltages 𝑣C1 and 𝑣C2, the controller Rc has been employed to regulate (𝑣C1 +
𝑣C2). The output of this controller defines I∗
g , the instantaneous sinusoidal current i∗
g
synchronized with the grid voltage (in order to obtain high power factor) is deter-
mined by the PLL-based block Gi. The inner control loop should be designed to
guarantee grid current control; the output of the block Rg defines 𝑣∗
g. It is impor-
tant to highlight that 𝑣g is the voltage generated by both rectifiers in converters 1 and
2 to guarantee grid current control [see equation (10.115)]. In fact, although 𝑣g is
viewed from the grid as only one-component voltage, it is constituted by two terms,
that is, 𝑣g = 𝑣1ab + 𝑣2ab. The term k1 determines the level of voltage that should be
processed by the rectifiers of converters 1 and 2 to keep the voltage 𝑣C1 under con-
trol. Hence, the controllers Rc and Rc1 are employed to control the dc-link voltages
(𝑣C1 and 𝑣C2), while the controller Rg along with the block Gi are used to control grid
power factor. The circulating current must track a zero reference (i∗
g = 0) with the
controller Ro, and the output voltage 𝑣∗
l
defines the voltages 𝑣∗
1cd
and 𝑣∗
2cd
. Although
the load voltage control in Fig. 10.16 is done in open-loop operation, a closed-loop
can be easily obtained from this control block diagram.
Exercise 10.7
Repeat Exercise 10.6 with the same conditions for the series topology in
Fig. 10.15.
10.6 SUMMARY
This chapter presented several circuits able to implement a single-phase back-to-back
converter. A comprehensive analysis for the full-bridge topology was presented in
Section 10.2. The following aspects were considered for this topology: (i) model, (ii)
PWM, (iii) control, (iv) power analysis, and (v) dc-link capacitor voltage, and (vi)
capacitor bank design. Section 10.3 dealt with topologies with reduced number of
power switches. Two strategies were considered: utilization of shared-leg and dc-link
capacitor midpoint connections as valid ways to reduce the number of switches. On
the other hand, the topologies with increased number semiconductor devices were
presented in Sections 10.4 and 10.5, with configurations in parallel and series, respec-
tively. The model, PWM and control approaches highlighting the presence of the
circulating current were also presented for both topologies. More information can be
found in references from 1 to 35.
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[14] Xu Z, Li R, Zhu H, Xu D, Zhang C. Control of parallel multiple converters for direct-drive
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[19] Park HW, Park SJ, Park JG, Kim CU. A novel high-performance voltage regulator for single-phase
AC sources. IEEE Trans Ind Electron 2001;48(3):554–562.
[20] Choi J-H, Kwon J-MB, Jung J-H, Kwon B-H. Highperformance online UPS using three-leg-type
converter. IEEE Trans Ind Electron 2005;52(3):889–897.
[21] Rocha N, Jacobina CB, dos Santos EJ, de Cavalcanti RMB. Parallel connection of two single-phase
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[22] Holtz J. Pulsewidth modulation for electronic power conversion. Proc IEEE 1994;82(8):1194–1214.
[23] Ojo O, Kshirsagar PM. Concise modulation strategies for four-leg voltage source inverters. IEEE
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algorithms for ups applications. IEEE Trans Ind Electron 2008;55(8):2923–2932.
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[30] Dong G, Ojo O. Current regulation in four-leg voltage-source converters. IEEE Trans Ind Electron
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electrical systems. IEEE Trans Ind Electron 2001;48(3):517–525.
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[34] Kolar J, Round S. Analytical calculation of the rms current stress on the dc-link capac-
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CHAPTER 11
THREE-PHASE TO THREE-PHASE
AND OTHER BACK-TO-BACK
CONVERTERS
11.1 INTRODUCTION
A three-phase back-to-back converter is an important electrical apparatus with a
wide range of applications on systems demanding a processed three-phase voltage.
Although the operation principle is similar to the single-phase to single-phase
back-to-back converter presented in the previous chapter, the characteristics of
the three-phase version are quite different, especially due to the nonexistent
pulsating power on the dc-link capacitor voltages. Note that the power at the
input (grid-side) and output (load-side) of the converter are constant for a bal-
anced case. The concept of power blocks is considered to provide a broader
perception of how the topologies presented in the technical literature have been
conceived.
Following the introduction, this chapter is organized in six sections. Section11.2
deals with the full-bridge ac–dc–ac converter presenting its model, pulse width
modulation (PWM), and control strategies. Topologies with component count
reduction are presented in Section 11.3, while Sections 11.4 and 11.5 describe the
model, PWM, and control for configurations with an increased number of semi-
conductor devices. A similar approach as in the previous chapter is employed for
the three-phase back-to-back converters, that is, shared-leg and dc-link capacitor
midpoint connections for reducing the number of semiconductor devices, while con-
necting back-to-back converters in parallel and series are considered in Sections 11.4
and 11.5, respectively. Section 11.6 presents other converters, especially for
single-phase to three-phase conversion and for a six-phase motor drive system.
Finally, Section 11.7 summarizes the chapter.
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
324
11.2 FULL-BRIDGE CONVERTER 325
11.2 FULL-BRIDGE CONVERTER
11.2.1 Model
Since the control goals are active power factor and regulation of the dc-link capac-
itor voltage, the equations derived in this section highlight both grid current and
capacitor voltage variables. Although an open loop operation is assumed for the out-
put of the converter, a closed loop control can be easily implemented for the output
converter side.
The three-phase back-to-back converter can be obtained directly by using
two PBs back-to-back connected per phase as presented in Fig. 11.1(a). The
representation of the three-phase back-to-back converter using switches is furnished
in Fig. 11.1(b). The conversion system is composed of a three-phase utility grid,
input inductors (with reactance equal to Xg1, Xg2, and Xg3), capacitor bank at the
dc-link with two capacitors (each one with capacitance equal to C), controlled
rectifier, inverter, and a three-phase load. The rectifier circuit comprises the switches
qg1, qg2, and qg3 and their complementary switches: qg1, qg2, and qg3. Similarly, the
inverter comprises the switches ql1, ql2, and ql3 and their complementary switches
ql1
, ql2
, and ql3
. Binary variables are employed to define the conduction states of the
switches.
The model of the back-to-back converter can be obtained from Fig. 11.1(b) as
follows:
𝑣g1 = 𝑣g10 − 𝑣ng0 (11.1)
(a)
(b)
+
–
+
–
+
–
+
–
+
–
–
+
ig1
ig2
ig3
iC
vC
il1
il2
il3
vl3
vl2
vl1
eg1
eg2
eg3
vg3
vg2
vg1
Xg1
Xg2
Xg3
qg1 qg2 qg3
g1
ng g2
g3
ql2 ql3
nl
ql1
ql2
ql1
l1
l2
l3
0
2
qg2 qg3
qg1
ql3
vC
vl1
–
+vl2
–
+vl3
2
Figure 11.1 Three-phase to three-phase back-to-back converter: (a) block and (b) switch
representation.
326 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
𝑣g2 = 𝑣g20 − 𝑣ng0 (11.2)
𝑣g3 = 𝑣g30 − 𝑣ng0 (11.3)
𝑣l1 = 𝑣l10 − 𝑣nl0 (11.4)
𝑣l2 = 𝑣l20 − 𝑣nl0 (11.5)
𝑣l3 = 𝑣l30 − 𝑣nl0 (11.6)
where the pole voltages can be written as a function of the states of the switches, as
below:
𝑣g10 = (2qg1 − 1)
𝑣C
2
(11.7)
𝑣g20 = (2qg2 − 1)
𝑣C
2
(11.8)
𝑣g30 = (2qg3 − 1)
𝑣C
2
(11.9)
𝑣l10 = (2ql1 − 1)
𝑣C
2
(11.10)
𝑣l20 = (2ql2 − 1)
𝑣C
2
(11.11)
𝑣l30 = (2ql3 − 1)
𝑣C
2
(11.12)
with 𝑣ng0 = 1
3
(𝑣g10 + 𝑣g20 + 𝑣g30) and 𝑣nl0 = 1
3
(𝑣l10 + 𝑣l20 + 𝑣l30) for a balanced case.
Equations (11.13)–(11.15) furnish the dynamic model for the variables at the
grid side:
𝑣g1 = eg1 − rgig1 − lg
dig1
dt
(11.13)
𝑣g2 = eg2 − rgig2 − lg
dig2
dt
(11.14)
𝑣g3 = eg3 − rgig3 − lg
dig3
dt
(11.15)
where rg and lg represent the resistances and inductances of the input inductor.
The capacitor voltage can be obtained as
𝑣c =
1
C∫
(qg1ig1 + qg2ig2 + qg3ig3 − ql1il1 − ql2il2 − ql3il3)dt (11.16)
with the interval of integration equal to the switching period.
11.2 FULL-BRIDGE CONVERTER 327
11.2.2 PWM Strategy
The optimized PWM strategy presented in Chapter 8 can be employed for the
full-bridge configuration presented in Fig. 11.1 to improve either total harmonic
distortion (THD) or efficiency at both sides.
If the desired input and output voltages are given respectively by 𝑣∗
g1
, 𝑣∗
g2
, 𝑣∗
g3
and 𝑣∗
l1
, 𝑣∗
l2
, 𝑣∗
l3
, the reference pole voltages can be written as follows:
𝑣∗
g10 = 𝑣∗
g1 + 𝑣∗
gh (11.17)
𝑣∗
g20
= 𝑣∗
g2
+ 𝑣∗
gh (11.18)
𝑣∗
g30 = 𝑣∗
g3 + 𝑣∗
gh (11.19)
𝑣∗
l10 = 𝑣∗
l1 + 𝑣∗
lh (11.20)
𝑣∗
l20 = 𝑣∗
l2 + 𝑣∗
lh (11.21)
𝑣∗
l30 = 𝑣∗
l3 + 𝑣∗
lh (11.22)
The auxiliary voltages 𝑣∗
gh
and 𝑣∗
lh
are given respectively by
𝑣∗
gh = 𝑣C
(
𝜇g −
1
2
)
+ (𝜇g − 1)V∗
gmax − 𝜇gV∗
gmin
(11.23)
𝑣∗
lh = 𝑣C
(
𝜇l −
1
2
)
+ (𝜇l − 1)V∗
lmax − 𝜇lV∗
lmin
(11.24)
where Vgmax = MAX{𝑣∗
g1
, 𝑣∗
g2
, 𝑣∗
g3
}, Vgmin = MIN{𝑣∗
g1
, 𝑣∗
g2
, 𝑣∗
g3
} and Vlmax =
MAX{𝑣∗
l1
, 𝑣∗
l2
, 𝑣∗
l3
}, Vlmin = MIN{𝑣∗
l1
, 𝑣∗
l2
, 𝑣∗
l3
}; 𝜇g and 𝜇l are the distribution factor
and determine how the free-wheeling time can be distributed throughout the switch-
ing period. Note that, since the grid and load sides of the converter are decoupled by
the dc-link capacitor bank, 𝑣∗
gh
and 𝑣∗
lh
are independent of each other.
Once the reference pole voltages have been defined, pulse widths 𝜏g1, 𝜏g2, 𝜏g3,
𝜏l1, 𝜏l2, and 𝜏l3 can be calculated from equations (11.25)–(11.30), as below:
𝜏g1 =
(
𝑣∗
g10
𝑣C
+
1
2
)
Ts (11.25)
𝜏g2 =
(
𝑣∗
g20
𝑣C
+
1
2
)
Ts (11.26)
𝜏g3 =
(
𝑣∗
g30
𝑣C
+
1
2
)
Ts (11.27)
𝜏l1 =
(
𝑣∗
l10
𝑣C
+
1
2
)
Ts (11.28)
𝜏l2 =
(
𝑣∗
l20
𝑣C
+
1
2
)
Ts (11.29)
328 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
𝜏l3 =
(
𝑣∗
l30
𝑣C
+
1
2
)
Ts (11.30)
where Ts is the switching period. The state of the switches qg1, qg2, qg3, ql1, ql2, and
ql3 can be defined directly from the previous equations by programming timers in a
digital implementation of the PWM.
Note that the reference voltages 𝑣∗
g1
, 𝑣∗
g2
, and 𝑣∗
g3
employed in (11.25)–(11.27)
are obtained as the output of controllers (as presented in Section 11.2.3.) Although
the voltages 𝑣∗
l1
, 𝑣∗
l2
, and 𝑣∗
l3
can be defined with either open-loop or closed-loop, the
open loop operation is considered in this section.
11.2.3 Control Approach
Figure 11.2 presents the control block diagram for the three-phase back-to-back con-
verter. While the output voltage is controlled by open-loop operation, the dc-link
capacitor voltage and the grid power factor are regulated by the controllers RC and
Ri1, Ri2, Ri3, respectively. Since the dynamic of the capacitor voltage is slow as com-
pared to the grid current, a cascade control approach has been employed to guarantee
regulation of both variables.
The dc-link voltage 𝑣C is adjusted to its reference value 𝑣∗
C
by using the con-
troller RC, which could be implemented with a standard PI controller. This controller
–
+
–
–
–
+
+
+
Ig
*
vgh
*
vl10
*
vg30
*
vg20
*
vg10
*
vl20
*
vl1
*
vl2
*
vl3
*
vlh
*
vl30
*
ig1
* vg1
*
vg2
*
vg3
*
ig1 ig2 ig3
ig2
*
ig3
*
*
vc
vc
eg1
Σ
Σ
Σ
Σ
Σ
Σ
Σ
Σ
Σ
Σ
μl
μg
Rc
Ri1
Ri2
Ri3
PWM
Load
Rectifier/Inverter
Voltage
sensor
Voltage
sensor
Current
sensor Grid
Ge-ig
Eq.(11.23)
Eq.(11.24)
qg1
qg2
qg3
ql1
ql2
ql3
Figure 11.2 Control strategy for the three-phase back-to-back converter.
11.2 FULL-BRIDGE CONVERTER 329
provides the amplitude of the reference grid current I∗
g . To maintain the power fac-
tor close to one with a sinusoidal grid current, the instantaneous reference currents
i∗
g1
, i∗
g2
and i∗
g3
must be synchronized with the input voltage eg1, eg2, and eg3, respec-
tively. Such a synchronization scheme can be obtained through a phase locked loop
(PLL)-based control. The block Ge − ig is responsible for generating the reference
sinusoidal grid current in phase with the grid voltage, that is, i∗
g1
= I∗
g sin(𝜔gt + Φg),
i∗
g2
= I∗
g sin(𝜔gt + Φg + 120∘), i∗
g3
= I∗
g sin(𝜔gt + Φg + 240∘). The current controller
loop must deal with sinusoidal waveforms, which means that a conventional PI con-
troller will not guarantee null error in steady-state operation – a modified PI controller
can be employed instead.
The PWM block shown in Fig. 11.2 can be implemented either from
equations (11.17)–(11.22) or by comparing these reference pole voltages with
high-frequency carrier signals.
Application (Universal Active Power Filter)
Also known as Universal Power Quality Conditioner (UPQC), the Universal Active
power filter uses the back-to-back schematic circuit to improve the quality of both
voltage and current in a three-phase electrical system. The electrical energy gen-
erators in power plants furnish voltages nearly sinusoidal. However, the quality of
this voltage can be deteriorated due to steady-state and/or transient phenomena at
a given point of the electrical system. Examples of these phenomena are nonlinear
loads and faults in part of the power circuit resulting in current distortion and voltage
sags/swells. The universal active power filter can be employed to compensate dynam-
ically such disturbances for both steady-state and transient problems, with the ability
to deal with the correction of grid voltage disturbance and fluctuation. As presented
in the figure below, one side (grid side) of the back-to-back converter is employed to
compensate the voltage disturbance by adding voltage through a three-phase trans-
former, while the other side is used to inject the current at the load side to guarantee
sinusoidal grid current with power factor close to one. The universal active power
filter is especially recommended to protect critical loads at the point of installation as
well as compensate the grid from current harmonics generated at the load side. The
voltage 𝑣g is used to compensate any disturbance on eg, since 𝑣l = eg + 𝑣ngnl
− 𝑣g.
The current if has been employed to guarantee a sinusoidal grid current in phase
with the grid voltage, since ig = il + if .
Although several techniques are presented in the literature for active power
filter control, the main structure is based on two control loops: a dc-link voltage
outer loop and a current inner loop. The outer loop regulates the dc-link voltage
while the inner loop tracks the reference current necessary to compensate harmonics
and/or fundamental reactive power. Two basic methods are considered in the litera-
ture to generate current reference signal: direct method and indirect method. In the
direct method the disturbance to be compensated is sensed directly from the load and
employed as the filter reference current signal. In the indirect method the disturbance
to be compensated is sensed on the grid and controlled to a minimum value through
a closed-loop. The last method has reduced cost since it uses less number of sensors,
while the first one is more accurate.
330 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
+
– + –
–
+
eg vg ig
if
il
nl
vl
ng
11.3 TOPOLOGY WITH COMPONENT COUNT
REDUCTION
11.3.1 Model
Another three-phase to three-phase ac–dc–ac power converter is obtained by remov-
ing one of the PBs-ac as shown in Fig. 11.3(a). Figure 11.3(b) shows the same con-
figuration with switch representation. Note that the leg constituted by the switches
qs − qs is shared between the input and output sides of the converter, and conse-
quently such a leg will handle a current that is a sum of input and output currents
(il3 − ig3). Also, the shared-leg will play an important role for the voltage capability
of the converter. Unlike the previous back-to-back converter where both input and
output converter sides are decoupled, the shared-leg topology in Fig. 11.3 presents
coupling due to the leg qs − qs.
The following equations can be derived from Fig. 11.3(b) for both input and
output converter sides:
𝑣g1 = 𝑣g10 − 𝑣ng0 (11.31)
𝑣g2 = 𝑣g20 − 𝑣ng0 (11.32)
𝑣g3 = 𝑣s0 − 𝑣ng0 (11.33)
𝑣l1 = 𝑣l10 − 𝑣nl0 (11.34)
𝑣l2 = 𝑣l20 − 𝑣nl0 (11.35)
𝑣l3 = 𝑣s0 − 𝑣nl0 (11.36)
11.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 331
(a)
(b)
+
–
+
–
+
–
+
–
–
+
ig1
ig2
ig3
iC
vC
il1
il2
il3
vl3
vl2
vl1
eg1
eg2
eg3
vg3
vg2
vg1
Xg1
Xg2
Xg3
qg1 qg2 qs
g1
ng
g2
s
ql2
nl
ql1
ql2
ql1
l1
l2
0
2
qg2 qs
qg1
+
–
vC
2
vl1
–
+vl2
–
+vl3
Figure 11.3 Shared-leg three-phase back-to-back converter: (a) block and (b) switch
representation.
The pole voltages can be written as in equations (11.7)–(11.12) with 𝑣ng0 =
1
3
(𝑣g10 + 𝑣g20 + 𝑣s0) and 𝑣nl0 = 1
3
(𝑣l10 + 𝑣l20 + 𝑣s0). Also, equations (11.13)–(11.15)
are still valid for modeling the input converter side. However, the capacitor voltage
for the shared-leg topology in Fig. 11.3 is given by
𝑣c =
1
C∫
[qg1ig1 + qg2ig2 + qs(ig3 − il3) − ql1il1 − ql2il2]dt (37)
with the interval of integration equal to the switching period.
11.3.2 PWM Strategies
If the desired input and output voltages are given respectively by 𝑣∗
g1
, 𝑣∗
g2
, 𝑣∗
g3
and 𝑣∗
l1
,
𝑣∗
l2
, 𝑣∗
l3
, one option for the reference pole voltage is given below:
𝑣∗
g10 = 𝑣∗
g1 − 𝑣∗
g3 + 𝑣∗
h (11.38)
𝑣∗
g20 = 𝑣∗
g2 − 𝑣∗
g3 + 𝑣∗
h (11.39)
𝑣∗
s0 = 𝑣∗
h (11.40)
𝑣∗
l10 = 𝑣∗
l1 − 𝑣∗
l3 + 𝑣∗
h (11.41)
𝑣∗
l20 = 𝑣∗
l2 − 𝑣∗
l3 + 𝑣∗
h (11.42)
Due to the shared-leg, which connects both input and output sides of the con-
verter, there is only one voltage 𝑣∗
h
that optimizes both converter sides. The 𝑣∗
h
can be
332 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
defined as follows:
𝑣∗
h = 𝑣C
(
𝜇 −
1
2
)
+ (𝜇 − 1)V∗
max − 𝜇V∗
min
(11.43)
where Vmax = MAX{𝑣∗
g1
− 𝑣∗
g3
, 𝑣∗
g2
− 𝑣∗
g3
, 0, 𝑣∗
l1
− 𝑣∗
l3
, 𝑣∗
l2
− 𝑣∗
l3
} and Vmin =
MIN{𝑣∗
g1
− 𝑣∗
g3
, 𝑣∗
g2
− 𝑣∗
g3
, 0, 𝑣∗
l1
− 𝑣∗
l3
, 𝑣∗
l2
− 𝑣∗
l3
}.
Once the reference pole voltages have been defined, pulse widths can be
obtained as in equations (11.25)–(11.30). In this case, instead of defining 𝜏g3 and
𝜏l3, the pulse width 𝜏s is defined by (𝑣∗
s ∕𝑣C + 1∕2)Ts.
11.3.3 dc-link Voltage Requirement
To guarantee the same input and output voltages as in the full-bridge converter, the
minimum dc-link voltage for the shared leg topology must obey the following require-
ment:
𝑣c ≥ max{𝑣∗
gx0 − 𝑣∗
gy0, 𝑣∗
gx0 − 𝑣∗
s0, 𝑣∗
lx0 − 𝑣∗
ly0, 𝑣∗
lx0 − 𝑣∗
s0, 𝑣∗
gx0 − 𝑣∗
ly0} (44)
with x = 1, 2; y = 1, 2; and x ≠ y.
If the load frequency is different from the grid frequency, the term 𝑣∗
gx0
− 𝑣∗
ly0
is dominant and defines 𝑣c. However, if both sides of the converter require the same
frequency, the output voltage can be generated, synchronized to the input voltage to
minimize the effect of the term 𝑣∗
gx0
− 𝑣∗
ly0
. This will allow the shared-leg converter
to operate with the same dc-link voltage as the full-bridge converter.
11.3.4 Half-Bridge Converter
The half-bridge configuration at both converter sides is presented in Fig. 11.4). In this
case there is a low frequency current flowing through the capacitors due to the dc-link
midpoint connection, which increases the voltage fluctuation on these elements and
consequently affects their losses.
The voltage at the input and output converter sides is defined directly from the
poles voltages 𝑣g10, 𝑣g20 and 𝑣l10, 𝑣l20, which are defined by equations (11.7), (11.8),
(11.10), and (11.11), respectively. Also, the PWM equations are defined straightfor-
ward since there is no degree of freedom to be explored, that is, there are only two
legs to process two voltages.
11.4 TOPOLOGIES WITH INCREASED NUMBER OF
SWITCHES (CONVERTERS IN PARALLEL)
The connection of converters in parallel can be employed when the power ratings of
the switches available do not handle the level of current needed by the circuit. The
simplest solution when the currents demanded by the load are higher than the rated
currents of the switches is connecting switches in parallel, as shown in Fig. 11.5 for
the three-phase back-to-back converter. Although the number of power switches is
twice as compared to those in Fig. 11.1, the characteristics of this converter in terms
11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 333
(a)
(b)
+
–
+
–
+
–
+
–
–
+
ig1
ig2
ig3
iC
vC
il1
il2
il3
vl3
vl2
vl1
eg1
eg2
eg3
vg3
vg2
vg1
Xg1
Xg2
Xg3
qg1 q2g
g1
ng
g2
ql2
nl
ql1
ql2
ql1
l1
l2
0
2
qg2
qg1
+
–
vC
2
vl1
–
+ vl2
–
+ vl3
Figure 11.4 Half-bridge three-phase back-to-back converter: (a) block and (b) switch
representation.
Figure 11.5 Three-phase back-to-back converter with switches in parallel.
of quality of the waveform generated are the same as in the conventional solution (see
Fig. 11.1).
As considered in Chapter 10 for the single-phase back-to-back converters, con-
necting converters in parallel instead of switches in parallel will bring the following
benefits: (i) increase the current capability of the conversion system, (ii) improve the
quality of the waveforms generated at the input and output sides of the converter, and
(iii) reduce the stress on the dc-link capacitors.
11.4.1 Model
Although connecting converters in parallel allows reducing the level of power
processed by each converter, as well as current ripple reduction, a circulating current
334 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
(a)
(b)
Converter 1 Converter 2
Converter 3 Converter 4
+
–
+
–
+ –
+ –
+ –
l
vl3
vl2
vl1
eg1
vC1
iC1
+
–
eg2
+
–
eg3
vg3
vg2
vg1
X1a
q1a q1b q1c q2c q2b q2a
i2a
il1
vl1
vl2
vl3
il2
il3
i2b
i2c
1a 2a
01
1b 2b
1c 2c
i1a
i1b
i1c
X1b
X1c
X2a
X2b
X2c
g
2
+
–
vC1
2
q1a q1b q1c q2c q2b q2a
+
–
vC2
iC2
X3c
q3a q1b q1c q4c q4b q4a
i4c
i4b
i4a
3a 4a
02
3b 4b
3c 4c
i3c
i3b
i3a
X3b
X3a
X4a
X4b
X4c
2
+
–
vC2
2
q3a q3b q3c q4c q4b q4a
Figure 11.6 Parallel three-phase back-to-back converter: (a) block and (b) switch
representation.
exists between both back-to-back converters. To model such a circulating current
it is necessary to write down all equations of the system. Figure 11.6 shows a
three-phase to three-phase energy conversion unit with two back-to-back converters
connected in parallel. Note that, although increasing the complexity of the system,
other back-to-back converters can be added in parallel, which reduces the power
processed by each unit. Such a conversion unit can be represented by either power
blocks [Fig. 11.6(a)] or power switches [Fig. 11.6(b)]. This conversion system
consists of a three-phase load, six inductance filters (Xja, Xjb, and Xjc with j = 1, 3)
at the grid side, six inductance filters (Xma, Xmb, and Xmc with m = 2, 4) at the load
side, and two dc-link capacitor banks.
Considering converters 1 and 3 (converters connected at the grid side), it is
possible to write the following equations:
eg1 = z1ai1a + 𝑣1a01
− 𝑣g01
(11.45)
11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 335
eg2 = z1bi1b + 𝑣1b01
− 𝑣g01
(11.46)
eg3 = z1ci1c + 𝑣1c01
− 𝑣g01
(11.47)
eg1 = z3ai3a + 𝑣3a02
− 𝑣g02
(11.48)
eg2 = z3bi3b + 𝑣3b02
− 𝑣g02
(11.49)
eg3 = z3ci3c + 𝑣3c02
− 𝑣g02
(11.50)
for a balanced case 𝑣g01
and 𝑣g02
are given respectively by:
𝑣g01
=
1
3
(𝑣1a01
+ 𝑣1b01
+ 𝑣1c01
) (11.51)
𝑣g02
=
1
3
(𝑣3a02
+ 𝑣3b02
+ 𝑣3c02
) (11.52)
where z1a = r1a + l1ap, z1b = r1b + l1bp, z1c = r1c + l1cp, z3a = r3a + l3ap,
z3b = r3b + l3bp, and z3c = r3c + l3cp are the impedances of the elements X1a,
X1b, X1c, X3a, X3b, and X3c, respectively; with p = d∕dt. 𝑣g01
and 𝑣g02
are the
voltages between the neutral of the grid and the dc-link midpoints 01 and 02,
respectively. Similar equations are obtained for converters 2 and 4 connected to the
load, as follows:
𝑣l1 = −z2ai2a + 𝑣2a01
− 𝑣l01
(11.53)
𝑣l2 = −z2bi2b + 𝑣2b01
− 𝑣l01
(11.54)
𝑣l3 = −z2ci2c + 𝑣2c01
− 𝑣l01
(11.55)
𝑣l1 = −z4ai4a + 𝑣4a02
− 𝑣l02
(11.56)
𝑣l2 = −z4bi4b + 𝑣4b02
− 𝑣l02
(11.57)
𝑣l3 = −z4ci4c + 𝑣4c02
− 𝑣l02
(11.58)
for a balanced case 𝑣l01
and 𝑣l02
are given respectively by:
𝑣l01
=
1
3
(𝑣2a01
+ 𝑣2b01
+ 𝑣2c01
) (11.59)
𝑣l02
=
1
3
(𝑣4a02
+ 𝑣4b02
+ 𝑣4c02
) (11.60)
As expected, due to the connection of both converters in parallel, there is a cir-
culating mesh that originates a circulating current between both ac–dc–ac conversion
units, as highlighted in Fig. 11.7.
z1ai1a + z2ai2a − z4ai4a − z3ai3a + 𝑣1a01
− 𝑣2a01
+ 𝑣4a02
− 𝑣3a02
= 0 (11.61)
z1ai1a + z2bi2b − z4bi4b − z3ai3a + 𝑣1a01
− 𝑣2b01
+ 𝑣4b02
− 𝑣3a02
= 0 (11.62)
z1ai1a + z2ci2c − z4ci4c − z3ai3a + 𝑣1a01
− 𝑣2c01
+ 𝑣4c02
− 𝑣3a02
= 0 (11.63)
z1bi1b + z2ai2a − z4ai4a − z3bi3b + 𝑣1b01
− 𝑣2a01
+ 𝑣4a02
− 𝑣3b02
= 0 (11.64)
z1bi1b + z2bi2b − z4bi4b − z3bi3b + 𝑣1b01
− 𝑣2b01
+ 𝑣4b02
− 𝑣3b02
= 0 (11.65)
z1bi1b + z2ci2c − z4ci4c − z3bi3b + 𝑣1b01
− 𝑣2c01
+ 𝑣4c02
− 𝑣3b02
= 0 (11.66)
336 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
i1o i2o
i3o i4o
io
io
io
io
Figure 11.7 Circulating current between both back-to-back converters in parallel.
z1ci1c + z2ai2a − z4ai4a − z3ci3c + 𝑣1c01
− 𝑣2a01
+ 𝑣4a02
− 𝑣3c02
= 0 (11.67)
z1ci1c + z2bi2b − z4bi4b − z3ci3c + 𝑣1c01
− 𝑣2b01
+ 𝑣4b02
− 𝑣3c02
= 0 (11.68)
z1ci1c + z2ci2c − z4ci4c − z3ci3c + 𝑣1c01
− 𝑣2c01
+ 𝑣4c02
− 𝑣3c02
= 0 (11.69)
Note that equations (11.61)–(11.69) exist due to the parallel connection of the
back-to-back converters. If a transformer is employed for isolation purposes, the cur-
rent io would be zero and equations (11.61)–(11.69) would no longer exist.
An expression for the circulating voltage can be obtained by adding
equations (11.61)–(11.69), to give the following expression:
𝑣o =
c
∑
n=a
z1ni1n +
c
∑
n=a
z2ni2n −
c
∑
n=a
z4ni4n −
c
∑
n=a
z3ni3n (11.70)
with
𝑣o = −
c
∑
n=a
𝑣1n01
+
c
∑
n=a
𝑣2n01
+
c
∑
n=a
𝑣3n02
−
c
∑
n=a
𝑣4n02
(11.71)
From the currents of the converters it is possible to define the circulating current
as follows:
i1o =
1
√
3
(i1a + i1b + i1c) (11.72)
i2o =
1
√
3
(i2a + i2b + i2c) (11.73)
i3o =
1
√
3
(i3a + i3b + i3c) (11.74)
i4o =
1
√
3
(i4a + i4b + i4c) (11.75)
11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 337
As presented in Fig. 11.7, the circulating current can be represented as a single
current that circulates among the converters. Such a current can be written as
io = i1o = −i3o = i2o = −i4o (11.76)
Since the parallel back-to-back converter deals with three-phase systems at both
sides of the converter (i.e., grid and load sides), it is convenient to use the transfor-
mation of variables from 123 to odq as follows:
xg123 = Pxgodq (11.77)
xl123 = Pxlodq (11.78)
xkabc = Pxkodq (11.79)
with xg123 = [xg1 xg2 xg3]T , xl123 = [xl1 xl2 xl3]T and xkabc = [xka xkb xkc]T, where x
can be either voltage or current and k = 1, 2, 3, 4.
Defining the voltages 𝑣1n = 𝑣1n01
− 𝑣g01
, 𝑣2n = 𝑣2n01
− 𝑣l01
, 𝑣3n = 𝑣3n02
−
𝑣g02
, and 𝑣4n = 𝑣4n02
− 𝑣l02
, with n = a, b, c, it is possible to determine the model of
the system as follows:
egdq = z1odqi1odq + 𝑣1dq (11.80)
egdq = z3odqi3odq + 𝑣3dq (11.81)
eldq = −z2odqi2odq + 𝑣2dq (11.82)
eldq = −z4odqi4odq + 𝑣4dq (11.83)
where egdq = [egd egq]T, eldq = [eld elq]T, ikodq = [iko ikd ikq]T, 𝑣kdq = [𝑣kd 𝑣kq]T , and
zkodq = 1
6
[√
2
(
2zka − zkb − zkc
)
(4zka + zkb + zkc)
√
3(zkc − zkb)
√
6(zkb − zkc)
√
3(zkc − zkb) 3(zkb + zkc)
]
Then it is possible to write the equation for the circulating current as follows:
𝑣o =
√
3
[( 4
∑
k=1
zko
)
io +
∑
j=d,q
z1oji1j +
∑
j=d,q
z2oji2j −
∑
j=d,q
z3oji3j −
∑
j=d,q
z4oji4j
]
(11.84)
with zko = 2
6
(zka + zkb + zkc), zkod =
√
2
6
(2zka − zkb − zkc), and zkoq =
√
6
6
(zkb − zkc)
It is also convenient to write the model in dq components since: (i) the voltages
𝑣1dq and 𝑣3dq will be employed to control the currents i1odq and i3odq and consequently
the grid power factor, (ii) the load variables will be controlled by the voltages 𝑣2dq
and 𝑣4dq, and (iii) the circulating current will be regulated by 𝑣o.
Assuming a balanced case: z1n = z3n = z1 and z2n = z4n = z2 with n = a, b, c,
it is possible to rewrite the model as follows:
egdq = z1i1dq + 𝑣1dq (11.85)
egdq = z1i3dq + 𝑣3dq (11.86)
eldq = z2i2dq + 𝑣2dq (11.87)
eldq = z2i4dq + 𝑣4dq (11.88)
338 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
with z1 =
[
z1 0
0 z1
]
and z2 =
[
z2 0
0 z2
]
From equations (11.80), (11.81) it is possible to obtain dq grid current:
𝑣gd =
𝑣1d + 𝑣3d
2
= egd −
z1
2
igd (11.89)
𝑣gq =
𝑣1q + 𝑣3q
2
= egq −
z1
2
igq (11.90)
By following the same strategy, 𝑣ld and 𝑣lq are given by:
𝑣ld =
𝑣2d + 𝑣4d
2
= eld −
z2
2
ild (11.91)
𝑣lq =
𝑣2q + 𝑣4q
2
= elq −
z2
2
ilq (11.92)
Defining zg = z1∕2 and zl = z2∕2, yields
𝑣gd = egd − zgigd (11.93)
𝑣gq = egq − zgigq (11.94)
𝑣ld = eld − zlild (11.95)
𝑣lq = elq − zlilq (11.96)
11.4.2 PWM
As described in the model of the three-phase back-to-back converter, the reference
voltages 𝑣∗
kd
, 𝑣∗
kq
, and 𝑣∗
o (k = 1, 2, 3, 4) are furnished by the controllers to regulate the
input, output, and circulating variables, respectively. By employing a transformation
of variables, it is possible to write the 123 voltages as a function of odq as follows:
𝑣∗
ka =
√
2
3
𝑣∗
kd (11.97)
𝑣∗
kb =
√
2
3
(
1
2
𝑣∗
kd +
√
3
2
𝑣∗
kq
)
(11.98)
𝑣∗
kc =
√
2
3
(
−
1
2
𝑣∗
kd −
√
3
2
𝑣∗
kq
)
(11.99)
The reference pole voltages employed for the PWM techniques can be defined
as a function of auxiliary voltages as follows:
𝑣∗
1a01
= 𝑣∗
1a + 𝑣∗
x (11.100)
𝑣∗
1b01
= 𝑣∗
1b + 𝑣∗
x (11.101)
𝑣∗
1c01
= 𝑣∗
1c + 𝑣∗
x (11.102)
11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 339
𝑣∗
2a01
= 𝑣∗
2a + 𝑣∗
y (11.103)
𝑣∗
2b01
= 𝑣∗
2b + 𝑣∗
y (11.104)
𝑣∗
2c01
= 𝑣∗
2c + 𝑣∗
y (11.105)
𝑣∗
3a02
= 𝑣∗
3a +
𝑣∗
o
3
− 𝑣∗
y + 𝑣∗
z + 𝑣∗
x (11.106)
𝑣∗
3b02
= 𝑣∗
3b +
𝑣∗
o
3
− 𝑣∗
y + 𝑣∗
z + 𝑣∗
x (11.107)
𝑣∗
3c02
= 𝑣∗
3c +
𝑣∗
o
3
− 𝑣∗
y + 𝑣∗
z + 𝑣∗
x (11.108)
𝑣∗
4a01
= 𝑣∗
4a + 𝑣∗
z (11.109)
𝑣∗
4b01
= 𝑣∗
4b + 𝑣∗
z (11.110)
𝑣∗
4c01
= 𝑣∗
4c + 𝑣∗
z (11.111)
The voltages 𝑣∗
x , 𝑣∗
y and 𝑣∗
z can be defined by following the same approach as
in equations (11.23) and (11.24).
11.4.3 Control Strategies
Figure 11.8 shows the control block diagram of the parallel three-phase back-to-back
converter. The dc-link voltages 𝑣C1 and 𝑣C2 are regulated by the controllers Rc1 and
Rc2, respectively. These controllers furnish the amplitudes of the reference currents
I∗
1
and I∗
3
required at the input side of the converters 1 and 3. The power factor control,
in turn, is obtained by synchronization of the reference grid current i∗
1abc
(i∗
1a
, i∗
1b
, i∗
1c
)
–
–
+
–
+
–
–
–
+
+
+
+
I1
*
I3
* i3abc
*
i1abc
*
eldq
*
eldq
i1dq
* v1dq
*
vo1
*
vdq
*
el123
eldq
v2dq
*
v4dq
*
vξ
*
vc12
i1dq
i1abc
q1abc
q3abc
q2abc
q4abc
eg123
i3abc
i1odq
i3dq
*
v3dq
*
io1
*
io1
i3dq
i3dq
*
vc1
vc1
vc2
*
vc2
eg1
Σ
Σ
Σ
Σ
Σ
Σ
Rc1
Rvdq Gv24
Ri1dq
Ri3dq
Ro1
PWM
Converters
1
and
3
Converters
2
and
4
Rc2
Gir
dq
123
dq
123
dq
123
dq
123
Figure 11.8 Control block diagram of the parallel three-phase converter.
340 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
and i∗
3abc
(i∗
3a
, i∗
3b
, i∗
3c
) with the three-phase voltages. Such a synchronization is done
in block Gir, which employs a PLL-based technique.
The output of block Gir are instantaneous reference currents that are converted
to dq variables through the transformation 123/dq, based on the block dq. As a con-
sequence, the output of these blocks are the reference currents i∗
1dq
(i∗
1d
, i∗
1q
) and i∗
3dq
(i∗
3d
, i∗
3q
). A double-sequence type of controller is employed on Ri1dq and Ri3dq to reg-
ulate the sinusoidal currents i∗
1dq
and i∗
3dq
. The output of the controllers Ri1dq and Ri3dq
define the reference voltages 𝑣∗
1dq
and 𝑣∗
3dq
.
The circulating current is regulated by Ro1 with i∗
o1
= 0. The output of block
Ro1 is circulating voltage 𝑣∗
o1
. The load voltage controller is obtained via block R𝑣dq.
The output of this controller defines 𝑣∗
dq
(𝑣∗
d
and 𝑣∗
q).
The voltage applied for each converter can be considered as half of the voltage
𝑣dq, the block G𝑣24 gives 𝑣∗
2dq
= 𝑣∗
4dq
= 𝑣∗
dq
∕2. Finally the reference voltages gener-
ated by the controllers 𝑣∗
1dq
, 𝑣∗
3dq
, 𝑣∗
o1
, 𝑣∗
2dq
, and 𝑣∗
4dq
, and the auxiliary voltages (𝑣∗
𝜉
with 𝜉 = x, y, and z) are applied to the PWM block. The output of this block generates
the state of the switches.
11.5 TOPOLOGIES WITH INCREASED NUMBER OF
SWITCHES (CONVERTERS IN SERIES)
The series connection (i.e., cascade connection) of the three-phase back-to-back con-
verters can be obtained as shown in Fig. 11.9(a) for the power blocks representation,
while Fig. 11.9(b) shows the same conversion system with power switches. Note that
the line-to-line voltages viewed by both grid and load sides will be two connected
H-bridge converter series. The same advantages as described for the single-phase
back-to-back converter are observed in this topology. Also, it is necessary to regulate
the circulating current among the conversion units to increase the efficiency of the
converter.
11.6 OTHER BACK-TO-BACK CONVERTERS
In the power distribution systems, the single-phase grid has been considered as an
alternative for either rural or remote areas, due to its lower cost feature, especially
when compared with the three-phase solution. Hence, the single-phase voltage avail-
able as the power supply is quite common where there is a large area to be covered.
On the other hand, loads connected in a three-phase arrangement present some advan-
tages when compared to single-phase loads. This is especially true when a motor is
the load connected to the converter, due to its reduced size, constant torque and con-
stant power at balanced conditions. In this scenario, there is a need for single-phase to
three-phase power conversion systems. The back-to-back converter, able to interface
a three-phase load and a single-phase grid, is presented in Fig. 11.10.
Such a single-phase to three-phase power conversion presents an inherent
asymmetry, that is, constant power at the output converter side (three-phase load)
11.6 OTHER BACK-TO-BACK CONVERTERS 341
(a)
(b)
Converter 1
Converter 2
Converter 3
+
–
+
–
+ –
+ –
+ –
nl
vl3
vl2
vl1
eg1
vC1
+
–
eg2 ig2
ig3
ig1
+
–
eg3
vg3
vg2
vg1
X1a X1a
q1a
1a
1b
1d
1c
q1b q1c q1d
il1
vl1
vl2
vl3
il2
il3
01
X2a X2a
X3a X3a
ng
2
+
–
vC1
2
q1a q1b q1c q1d
+
–
vC2
q2a
2a
2b
2d
2c
q2b q2c q2d
02
2
+
–
vC2
2
q2a q2b q2c q2d
+
–
vC3
q3a
3a
3b
3d
3c
q3b q3c q3d
03
2
+
–
vC3
2
q3a q3b q3c q3d
Figure 11.9 Three-phase configuration with back-to-back converter series connected: (a)
block and (b) switch representation.
342 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
Figure 11.10 Single-phase to three-phase back-to-back converter.
+
+
–
–
(a)
(b)
Rectifier
Pulsating
power Constant
power
Inverter
iin
iout
υin
υout
Figure 11.11 (a) Power asymmetry of the single-phase to three-phase converter (b) a
potential solution to deal with the asymmetry.
11.6 OTHER BACK-TO-BACK CONVERTERS 343
Figure 11.12 Three-phase to three-phase four-wire back-to-back converter.
is6
vs6
is2
vs2
is4
vs4
is3
vs3
vs3
is5
vs5
is1
vs1
–
–
–
–
–
+
+
vs2 –
+
vs1 –
+
vs4 –
+
vs5 –
+
vs6 –
+
+
+
+
+
+
Six-phase machine
Six-phase
machine
n
n
m
m
Figure 11.13 (a) Six-phase machine drive system based on three-phase back-to-back
converters (b) model of the motor drive system.
344 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS
and a pulsating power at the input converter side (single-phase grid), as highlighted
in Fig. 11.11(a). The direct consequence of this asymmetry is the low frequency
voltage oscillation observed in the dc-link capacitors; also, the power switches of the
rectifier and inverter operate with different current ratings. Normally, the three-phase
motor rated voltage is higher than that furnished by the single-phase grid, which
means that the rectifier circuit must boost the grid voltage to guarantee the motor
rated voltage. Consequently, the current relationship between input and output
converter sides also implies converter asymmetry with the input current higher than
the output current. There are different ways to deal with this challenge; one way is
to employ the topology presented in Fig. 11.11(b) with a parallel converter used at
the rectifier stage.
Another example of three-phase back-to-back converters is presented in
Fig. 11.12, which deals with a load demanding a three-phase system with four wires.
Note that this configuration is able to generate a regulated three-phase voltage at the
load side where both three-phase and single-phase loads can be connected.
Lastly, Fig. 11.13(a) shows a six-phase machine drive system based on
ac–dc–ac converter topologies connected in paralleled without isolation trans-
former. Note that unlike the previous parallel configurations presented in this
chapter, the motor drive system in Fig. 11.13(a) does not have circulating current
since the neutrals (n and m) of the six-phase machine are not connected between
themselves, as highlighted in the model in Fig. 11.13(b). The six-phase machine is
in fact constituted by two sets of three-phase windings, which present benefits such
as reduced ripple on the torque. Another advantage of the six-phase motor drive
system compared to the three-phase one is the fact that the currents processed by
each switch of the inverter are lower.
11.7 SUMMARY
This chapter dealt with three-phase back-to-back converters. Section 11.2 presented
the full-bridge ac–dc–ac converter, its model, PWM, and control strategies.
Topologies with component count reduction were presented in Section 11.3, while
Sections 11.4 and 11.5 showed the model, PWM, and control for configurations with
an increased number of semiconductor devices. Shared-leg and dc-link capacitor
midpoint connections were also considered for reducing the number of semiconduc-
tor devices, while connecting back-to-back converters in parallel and series. Other
three-phase arrangements were considered in Section 11.6. Readers can find more
details from References 1 to 8.
REFERENCES
[1] H. W. van der Broeck and J. D. van Wyk, A comparative investigation of a three-phase induction
machine drive with a component minimized voltage-fed inverter under different control options, IEEE
Trans Ind Appl, vol. IA-20, no. 2, pp. 309–320, Mar./Apr. 1984.
[2] P. Enjeti and A. Rahman, A new single phase to three phase converter with active input current shaping
for low cost AC motor drives, IEEE Trans Ind Appl, vol. 29, no. 4, pp. 806–813, Jul./Aug. 1993.
REFERENCES 345
[3] Blaabjerg F, Freysson S, Hansen HH, and Hansen S. Comparison of a space-vector modulation strategy
for a three phase standard and a component minimized voltage source inverter. Proceedings EPE; 1995.
p. 1806–1813.
[4] Kim GT and Lipo TA. VSI-PWM rectifier/inverter system with a reduced switch count. Conference.
Rec. IEEE IAS Annual Meeting; 1995. p. 2327–2332.
[5] C. B. Jacobina, M. B. R. Correa, E. R. C. da Silva, and A. M. N. Lima, Induction motor drive system
for low-power applications, IEEE Trans Ind Appl, vol. 35, no. 1, pp. 52–61, Jan./Feb. 1999.
[6] F. Blaabjerg, D. O. Neacsu, and J. K. Pedersen, Adaptive SVM to compensate dc-link voltage ripple
for four-switch three-phase voltage-source inverters, IEEE Trans Power Electron, vol. 14, no. 4, pp.
743–752, Jul. 1999.
[7] E. Ledezma, B. McGrath, A. Muñoz, and T. A. Lipo, Dual AC-drive system with a reduced switch
count, IEEE Trans Ind Appl, vol. 37, no. 5, pp. 1325–1333, Sep./Oct. 2001.
[8] J. R. Rodríguez, J. W. Dixon, J. R. Espinoza, J. Pontt, and P. Lezana, PWM regenerative rectifiers:
State of the art, IEEE Trans Ind Electron, vol. 52, no. 1, pp. 5–22, Feb. 2005.
ADVANCED POWER ELECTRONIC CONVERTERS AND APPLICATIONS
INDEX
A
ac–dc conversion, 43–50
controlled rectifiers, 45
full-bridge controlled, 49
PWM control, 47
single split-phase rectifier with
free-wheeling diode, 48
three-phase controlled rectifier, 49
three-phase half-bridge controlled
rectifier, 48
uncontrolled rectifiers, 43
ac–dc–ac configurations, 81–85
PBG application in, 81–85
single-phase to single-phase
configurations, 85
three-phase to three-phase configurations,
82–85
ac–dc–ac converter, 3
active switch ANPC converters, 214
active-neutral-point-clamped (ANPC)
converters, 211–214
configuration, 211–212
alternate phase opposite disposition
(APOD), 167
analog PWM implementation, 228
applications of power electronics converters,
6–9
in a distributed generation system, 7
Energy-Control-Center (ECC), 8
field, 8–9
that process ac voltage, 6
B
back-to-back converters, 324–344, See also
three-phase to three-phase converters
single-phase to three-phase back-to-back
converter, 342
power asymmetry of, 342
Advanced Power Electronics Converters: PWM Converters Processing AC Voltages,
Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva.
© 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc.
three-phase to three-phase four-wire
back-to-back converter, 343
basic power converters, 25–43, See also
ac–dc conversion; dc–ac conversion;
dc–dc conversion; power
semiconductor devices
building, principles for, 27
connecting source to load, ways to, 28
bidirectional controlled thyristor (BCT), 12
bipolar junction transistor (BJT), 12, 19
bipolar modulation, 38
boost converter, 31
topological states for, 32
buck converter, 28
with basic cell switch, 29
with real switches, 29
topological states for, 29
buck-boost converter, 33
C
capacitor bank design, 304–307
capacitor current spectrum, 239
carrier-based PWM (CPWM), 221
configurations with, 247–252
our-leg converter, 249–252
three-leg converter, two-phase machine,
247–249
nonconventional topologies with,
252–261
cascade configuration, 72–75, 125–170
single H-bridge converter, 126–128
three-phase Converter
one H-bridge converter per phase,
140–144
two cascade H-bridges per phase,
149–162
347
348 INDEX
cascade configuration (Continued)
two H-bridge converters, 144–146
cascade control strategies, 289–293
motor drive, speed-current control,
290–293
rectifier circuit, voltage-current control,
289–290
chopper, 3
classifications of power electronics
topologies, 3
component count reduction, topology with,
307–310
dc-link voltage requirement, 309–310
half-bridge converter, 310
model, 307–308
PWM strategy, 308–309
control approach
full-bridge converter, 328–330
controlled conduction/controlled blocking
devices, 19–22
bipolar junction transistor (BJT), 19
IGBT, 21
gate turn-off (GTO), 21–22
IGCT, 22
reverse blocking IGCT (RBIGCT), 22
MOSFET, 19, 20–21
controlled conduction/spontaneous blocking
devices, 18–19
silicon-controlled rectifier (SCR), 18
TRIode AC (TRIAC), 18–19
controlled rectifiers, 45
controlled ac–dc converter using
switching cell, 46
phase control, 45
single-phase rectifier, 46–47
conventional diode, 17–18
cuk converter, 33
current-source inverters (CSIs), 33, 43
cycle converter, 3
D
dc–ac conversion, 33–40
current-source inverters (CSIs), 33
impedance-source inverters (ZSIs), 33
three-phase inverter, 38
voltage-source inverters (VSIs), 33, 34
dc–ac–dc converter, 3
dc–dc conversion, 28–33
boost converter, 31
buck converter, 28
buck-boost converter, 33
cuk converter, 33
single-ended primary-inductor converter
(SEPIC) converter, 33
zeta converter, 33
dc-link capacitor voltage, 301–304
dc-link voltage requirement, 309–310
differential converter, 218
digital PWM implementation, 228–231
dynamic controllability, ideal switches,
12–15
controlled turn off, 14
controlled turn on, 14
spontaneous turn off, 14
spontaneous turn on, 14
dynamic voltage restorer (DVR), 251–252
E
electromotive force (emf), 276
Energy-Control-Center (ECC), 8
F
five-level FC topology, 188
five-level NPC configuration, 119–123
PB representation, 121
with pyramid structure, 122
flying capacitor (FC) converter, 172–197
configuration, 75–79
four-level configuration, 189–196, See
also individual entry
full-bridge topology, 181–183
generalization, 196–197
nonconventional FC converters with
three-level legs, 186–189
three-level configuration, 173–176
three-phase FC converter, 183–186
voltage control, 179–181
forward blocking voltage, 16
forward voltage capability, 16
forward voltage drop, 16
four H-bridge converters and generalization,
169
four-leg converter, 249–252
dynamic voltage restorer (DVR), 251–252
supplying a three-phase four-wire load,
249
supplying four-phase machine, 250
four-level FC configuration, 189–196
converter with four switches, 194–195
four-level FC configuration with PBs, 191
INDEX 349
four-level FC half-bridge converter, 194
gating signal generation, modulation
strategy for, 193
general four-level output voltage,
generation of, 192
single-phase full-bridge four-level FC
converter, 196
three-phase two-leg FC converter, 190
four-level NPC configuration, 112–115
open-end motor drive system, 121
three-phase NPC converter, 120
four-wire back-to-back converter, 343
full-bridge converter, 36, 296–307, 325–330
capacitor bank design, 304–307
control approach, 298–299, 328–330
dc-link capacitor voltage, 301–304
model, 296–297, 325
power analysis, 299–301
PWM strategy, 297–298, 327–328
single-phase full-bridge inverter, 36–37
full-bridge single-phase converter, 95–98
using four-level NPC legs, 118–119
full-bridge topology, flying capacitor (FC)
converter, 181–183
G
gate turn-off (GTO), 4, 21–22
gate-assisted turnoff thyristor (GATT), 4
gating signal generation, modulation
strategy for, 193
generalization, FC converter, 196–197
H
half-bridge converter, 310, 332
half-bridge inverter, 34
half-bridge topology, 93–95, 177–178
hexagonal-field-effect-transistor (HEXFET),
20
hybrid topology, 107
hysteresis control, 271–279
for dc motor drive, 275–278
defining the state of the switches, 272
measured load current, 273
reference load current, 273
for regulating an ac variable, 278–279
startup transient for, 273
I
ideal switches, 11–15
characteristics, 11
dynamic controllability, 12–15
power electronics devices as, 11–15
static characteristics, 12
impedance-source inverters (ZSIs), 33
indirect ac–dc–ac conversion, 50–51
in-phase disposition (IPD), 167
insulated bipolar junction transistor (IGBT),
12
insulated-gate-bipolar transistor (IGBT), 4,
58
Integrated gate commutation thyristor
(IGCT), 22
interdisciplinary nature of power electronics,
2
L
linear control, ac variable, 288–289
linear control, dc variable, 279–288
proportional controller, 279–280
dc motor drive system, 280–283
RL load, 279–280
proportional-integral controller, 283–285
dc motor, 285–286
RL load, 283–285
proportional-integral-derivative controller,
286–288
dc motor, 286–288
linear regulators, 5
M
macro grid, 7
magnetic element at the output, topology
with, 205–211
five-level topology, 209
modular multilevel converter, 211
with PBs, 210
three-level configurations, 206
maximum peak nonrepetitive forward and
reverse voltage, 16
metal oxide semiconductor field-effect
transistors (MOSFETs), 4, 19, 20–21,
58
micro grid, 7–8
mixed NPC/FC converters, 215–216
using flying capacitor, 217
and first PB-ac, 217
first/second PB-ac, 217
modular multilevel converter (MMC), 199
MOS-controlled thyristor (MCT), 4, 22
motor drive, speed-current control, 290–293
350 INDEX
multilevel configurations, 79–81, 199–219,
See also active-neutral-point-clamped
(ANPC) converters; active switch
ANPC converters; mixed NPC/FC
converters; nested multilevel
configurations
N
nested multilevel configurations, 200–205
with block representation, 200
generalization of, 205
PWM approach for, 204
with switches representation, 201
three-phase four-level nested
configurations, 204
neutral-point-clamped (NPC) configuration,
88–124, 172
five-level configuration, 119–123
four-level NPC configuration, 112–115
full-bridge and other circuits (four-level
configuration), 118–119
nonconventional arrangements by using
three-level legs, 101–108
three-level configuration, 89–93
full-bridge topologies, 95–98
three-phase NPC converter, 98–101
unbalanced capacitor voltage, 108–112
neutral-point-clamped (NPC) inverter, 67
configuration, 68–72
NPC multilevel legs, construction, 69
nonconventional arrangements by using
three-level legs, 101–108
five-level single-phase converter, 103
four-level single-phase converter, 103
hybrid topology, 107
nonconventional FC converters with
three-level legs, 186–189
five-level FC topology, 188
four-level FC topology, 188
nonconventional topologies with CPWM,
252–261
open-end winding motor drive system,
257–261
split-wound coupled inductors, inverter
with, 252–254
Z-source converter, 254–257
O
on-state current, 16
on-state root mean square (RMS) current, 16
open-end winding motor drive system,
257–261
optimized PWM approach, 221–261, See
also space vector modulation
(SVPWM); two-leg converter
P
peak repetitive forward current, 16
peak surge forward current, 16
phase control, 45
phase opposite disposition (POD), 167
photovoltaic (PV) power system, 135–140
point of common coupling (PCC), 8
power blocks geometry (PBG), 56–86
application in multilevel configurations,
67–81
cascade configuration, 72–75
flying capacitor configuration, 75–79
multilevel configurations, 79–81
neutral-point-clamped configuration,
68–72
basic units used in, 61
concepts, 58
configurations employing four controlled
switches, 59
configurations employing six controlled
switches, 60
description of power blocks, 62–67
variables associated with, 63–65
principles of, 58–62
propositions, 58
power converters
applications of, 6–9
basic control principles, 265–271
ATLAB code, 266, 269
discretization method, 265
control strategies for, 264–293, See also
cascade control strategies; hysteresis
control; linear control, ac variable;
linear control, dc variable
history of, 4–6
processing ac voltage, 56–86, See also
power blocks geometry (PBG)
synthesize ac voltage, 57
power losses, 17
power semiconductor devices, 16–25
controlled conduction/controlled blocking
devices, 19–22, See also individual
entry
INDEX 351
controlled conduction/spontaneous
blocking devices, 18–19
forward and reverse voltage capability,
16
forward blocking voltage, 16
forward voltage drop, 16
maximum peak nonrepetitive forward and
reverse voltage, 16
nonideal device characteristics, 16
peak repetitive forward current, 16
peak surge forward current, 16
power losses, 17
reverse blocking voltage, 16
spontaneous conduction/controlled
blocking devices, 22–24
spontaneous conduction/spontaneous
blocking, 17–18
on-state current, 16
on-state root mean square (RMS) current,
16
turn-off time, 17
turn-on time, 16
power switches, 10–52, See also ideal
switches
history of, 4–6
powerblock geometry (PBG), 172
pulse width modulation (PWM), 10, 88, 172,
221–261, See also optimized PWM
approach
generation, 105
analog implementation, 105
waveforms, 105
implementation, 125
four-level configuration, 115–118
of single H-bridge converter, 129–140
of two cascade H-bridges, 146–149
half-bridge topology, 93–95, 177–178
PWM control, 47
pulsed voltage source, 57
pulse-width modulation (PWM) converters,
10
R
rectifier or inverter, 3
rectifier circuit, 289–290
voltage-current control, 289–290
reverse blocking IGCT (RBIGCT), 22
reverse blocking voltage, 16
reverse voltage capability, 16
S
Schottky diode, 18
Siemens-Power Metal Oxide Silicon
(SIPMOS), 20
silicon-controlled rectifier (SCR), 6, 18
single H-bridge converter, 126–128
one h-bridge converter per phase,
140–144
PWM implementation of, 129–140
two-level H-bridge converter, 131
single-ended primary-inductor converter
(SEPIC) converter, 33
single-phase full-bridge inverter, 36–37
single-phase rectifier, 46–47
single-phase to single-phase back-to-back
converter, 295–321, See also
full-bridge converter
component count reduction, topology
with, 307–310
topologies with increased number of
switches
converters in parallel, 310–318
converters in series, 318–321
single-phase to single-phase configurations,
85
sinusoidal pulse width modulation (SPWM),
34, 221
space vector modulation (SVPWM), 221,
243–247
graphical analysis for, 245
split-wound coupled inductors, inverter with,
252–254
spontaneous conduction/controlled blocking
devices, 22–24
static induction thyristor (SITH), 23–24
static induction transistor (SIT), 22–23
spontaneous conduction/spontaneous
blocking, 17–18
conventional diode, 17–18
Schottky diode, 18
static characteristics, ideal switches, 12
static induction thyristor (SITH), 23–24
static induction transistor (SIT), 22–23
switching power suppliers, 5
T
T flowing current metal oxide silicon
(TMOS), 20
three H-bridge converters, 164–169
analog control circuitries, 167, 168
352 INDEX
three H-bridge converters (Continued)
Δ connections for the outer converters,
165
level shift multicarrier modulation, 168
open-winding machine, 165
three-phase Y-connected, 165
three-phase Δ-connected, 165
three-leg converter, two-phase machine,
247–249
three-level configuration
flying capacitor (FC) converter, 173–176
three-level NPC configuration, 89–93
three-phase converter, 149–162
FC converter, 183–186
two cascade H-bridges per phase,
149–162
fault-tolerant converter with triacs,
155
fault-tolerant strategy, 160
motor drive system with open-end
winding topology, 157
open-circuit type of fault, 153
post-fault configuration, 159
pre-fault configuration, 158
short-circuit type of fault, 153
three-phase four-level nested configurations,
204
three-phase inverter, 38
line-to-line voltage, 40
load phase voltage, 40
modes of operation, 41
pole voltages, 40
zero-sequence voltage, 40
three-phase machine connection, 238–242
influence over inverter variables, 238–242
three-phase NPC converter, 98–101
three-phase switching matrix, 51
three-phase to three-phase converters,
324–344, See also full-bridge converter
block representation, 325
configurations, 82–85
switch representation, 325
topologies with increased number of
switches
converters in parallel, 332–340
converters in series, 340
topology with component count reduction,
330–332
topologies with increased number of
switches, 310–318, 332–340
control strategy, 316–318
converters in parallel, 332–340
control strategies, 339–340
half-bridge three-phase back-to-back
converter, 333
model, 333–338
PWM strategy, 338–339
three-phase back-to-back converter
with switches in parallel, 333
converters in series, 340
model, 311–314
topology with component count reduction,
330–332
dc-link voltage requirement, 332
half-bridge converter, 332
model, 330–331
PWM strategies, 331–332
total harmonic distortion (THD), 67
TRIode AC (TRIAC), 18–19
two cascade H-bridges, PWM
implementation of, 146–149
two H-bridge converters, 144–146,
162–164
seven- and nine-level topologies,
162–164
two-leg converter, 222–233
analog implementation, 228–231
digital implementation, 228–231
model, 222–223
PWM implementation, 223–228
𝜇 influence for, 231–233, 236–238
and three-phase load, 233–242
analog implementation, 236
digital implementation, 236
model, 233–235
PWM implementation, 235–236
U
unbalanced capacitor voltage, 108–112
uncontrolled rectifiers, 43
uninterrupted power supply (UPS), 303,
305
unipolar modulation, 38
Universal Power Quality Conditioner
(UPQC), 329
INDEX 353
V
voltage control, flying capacitor,
179–181
voltage-source inverters (VSIs),
33, 34
full-bridge, 36
half-bridge inverter, 34
W
weighted total harmonic distortion (WTHD),
236–237
Z
zeta converter, 33
Z-source converter, 254–257
ADVANCED POWER ELECTRONIC CONVERTERS AND APPLICATIONS
IEEE Press Series
on Power Engineering
Series Editor: M. E. El-Hawary, Dalhousie University, Halifax, Nova Scotia,
Canada
The mission of IEEE Press Series on Power Engineering is to publish leading-
edge books that cover the broad spectrum of current and forward-looking tech-
nologies in this fast-moving area. The series attracts highly acclaimed authors
from industry/academia to provide accessible coverage of current and emerging
topics in power engineering and allied fields. Our target audience includes the
power engineering professional who is interested in enhancing their knowledge
and perspective in their areas of interest.
1. Principles of Electric Machines with Power Electronic Applications, Second
Edition
M. E. El-Hawary
2. Pulse Width Modulation for Power Converters: Principles and Practice
D. Grahame Holmes and Thomas Lipo
3. Analysis of Electric Machinery and Drive Systems, Second Edition
Paul C. Krause, Oleg Wasynczuk, and Scott D. Sudhoff
4. Risk Assessment for Power Systems: Models, Methods, and Applications
Wenyuan Li
5. Optimization Principles: Practical Applications to the Operations of Markets
of the Electric Power Industry
Narayan S. Rau
6. Electric Economics: Regulation and Deregulation
Geoffrey Rothwell and Tomas Gomez
7. Electric Power Systems: Analysis and Control
Fabio Saccomanno
8. Electrical Insulation for Rotating Machines: Design, Evaluation, Aging,
Testing, and Repair, Second Edition
Greg Stone, Edward A. Boulter, Ian Culbert, and Hussein Dhirani
9. Signal Processing of Power Quality Disturbances
Math H. J. Bollen and Irene Y. H. Gu
10. Instantaneous Power Theory and Applications to Power Conditioning
Hirofumi Akagi, Edson H. Watanabe, and Mauricio Aredes
11. Maintaining Mission Critical Systems in a 24/7 Environment
Peter M. Curtis
12. Elements of Tidal-Electric Engineering
Robert H. Clark
13. Handbook of Large Turbo-Generator Operation and Maintenance, Second
Edition
Geoff Klempner and Isidor Kerszenbaum
14. Introduction to Electrical Power Systems
Mohamed E. El-Hawary
15. Modeling and Control of Fuel Cells: Distributed Generation Applications
M. Hashem Nehrir and Caisheng Wang
16. Power Distribution System Reliability: Practical Methods and Applications
Ali A. Chowdhury and Don O. Koval
17. Introduction to FACTS Controllers: Theory, Modeling, and Applications
Kalyan K. Sen and Mey Ling Sen
18. Economic Market Design and Planning for Electric Power Systems
James Momoh and Lamine Mili
19. Operation and Control of Electric Energy Processing Systems
James Momoh and Lamine Mili
20. Restructured Electric Power Systems: Analysis of Electricity Markets with
Equilibrium Models
Xiao-Ping Zhang
21. An Introduction to Wavelet Modulated Inverters
S.A. Saleh and M.A. Rahman
22. Control of Electric Machine Drive Systems
Seung-Ki Sul,
23. Probabilistic Transmission System Planning
Wenyuan Li
24. Electricity Power Generation: The Changing Dimensions
Digambar M. Tigare
25. Electric Distribution Systems
Abdelhay A. Sallam and Om P. Malik
26. Practical Lighting Design with LEDs
Ron Lenk and Carol Lenk
27. High Voltage and Electrical Insulation Engineering
Ravindra Arora and Wolfgang Mosch
28. Maintaining Mission Critical Systems in a 24/7 Environment, Second Edition
Peter Curtis
29. Power Conversion and Control of Wind Energy Systems
Bin Wu, Yongqiang Lang, Navid Zargari, and Samir Kouro
30. Integration of Distributed Generation in the Power System
Math H. Bollen and Fainan Hassan
31. Doubly Fed Induction Machine: Modeling and Control for Wind Energy
Generation Applications
Gonzalo Abad, Jesus Lopez, Miguel Rodrigues, Luis Marroyo, and Grzegorz
Iwanski
32. High Voltage Protection for Telecommunications
Steven W. Blume
33. Smart Grid: Fundamentals of Design and Analysis
James Momoh
34. Electromechanical Motion Devices, Second Edition
Paul C. Krause, Oleg Wasynczuk, and Steven D. Pekarek
35. Electrical Energy Conversion and Transport: An Interactive Computer-Based
Approach, Second Edition
George G. Karady and Keith E. Holbert
36. ARC Flash Hazard and Analysis and Mitigation
J. C. Das
37. Handbook of Electrical Power System Dynamics: Modeling, Stability, and
Control
Mircea Eremia and Mohammad Shahidehpour
38. Analysis of Electric Machinery and Drive Systems, Third Edition
Paul Krause, Oleg Wasynczuk, S. D. Sudhoff, and Steven D. Pekarek
39. Extruded Cables for High-Voltage Direct-Current Transmission: Advances in
Research and Development
Giovanni Mazzanti and Massimo Marzinotto
40. Power Magnetic Devices: A Multi-Objective Design Approach
S. D. Sudhoff
41. Risk Assessment of Power Systems: Models, Methods, and Applications,
Second Edition
Wenyuan Li
42. Practical Power System Operation
Ebrahim Vaahedi
43. The Selection Process of Biomass Materials for the Production of Bio-Fuels
and Co-Firing
Najib Altawell
44. Electrical Insulation for Rotating Machines: Design, Evaluation, Aging,
Testing, and Repair, Second Edition
Greg C. Stone, Ian Culbert, Edward A. Boulter, Hussein Dhirani
45. Principles of Electrical Safety
Peter E. Sutherland
46. Advanced Power Electronics Converters: PWM Converters Processing AC
Voltages
Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva
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ADVANCED POWER ELECTRONIC CONVERTERS AND APPLICATIONS

  • 4. IEEE Press 445 Hoes Lane Piscataway, NJ 08854 IEEE Press Editorial Board Tariq Samad, Editor in Chief George W. Arnold Mary Lanzerotti Linda Shafer Dmitry Goldgof Pui-In Mak MengChu Zhou Ekram Hossain Ray Perez George Zobrist Kenneth Moore, Director of IEEE Book and Information Services (BIS) Technical Reviewers Marcelo Godoy Simões, Colorado School of Mines Hamid A. Toliyat, Texas A&M University
  • 5. ADVANCED POWER ELECTRONICS CONVERTERS PWM Converters Processing AC Voltages EUZELI CIPRIANO DOS SANTOS JR. EDISON ROBERTO CABRAL DA SILVA
  • 6. Copyright © 2015 by The Institute of Electrical and Electronics Engineers, Inc. Published by John Wiley & Sons, Inc., Hoboken, New Jersey. All rights reserved Published simultaneously in Canada No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning, or otherwise, except as permitted under Section 107 or 108 of the 1976 United States Copyright Act, without either the prior written permission of the Publisher, or authorization through payment of the appropriate per-copy fee to the Copyright Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923, (978) 750-8400, fax (978) 750-4470, or on the web at www.copyright.com. Requests to the Publisher for permission should be addressed to the Permissions Department, John Wiley & Sons, Inc., 111 River Street, Hoboken, NJ 07030, (201) 748-6011, fax (201) 748-6008, or online at http://www.wiley.com/go/permission. Limit of Liability/Disclaimer of Warranty: While the publisher and author have used their best efforts in preparing this book, they make no representations or warranties with respect to the accuracy or completeness of the contents of this book and specifically disclaim any implied warranties of merchantability or fitness for a particular purpose. No warranty may be created or extended by sales representatives or written sales materials. The advice and strategies contained herein may not be suitable for your situation. You should consult with a professional where appropriate. Neither the publisher nor author shall be liable for any loss of profit or any other commercial damages, including but not limited to special, incidental, consequential, or other damages. For general information on our other products and services or for technical support, please contact our Customer Care Department within the United States at (800) 762-2974, outside the United States at (317) 572-3993 or fax (317) 572-4002. Wiley also publishes its books in a variety of electronic formats. Some content that appears in print may not be available in electronic formats. For more information about Wiley products, visit our web site at www.wiley.com. Library of Congress Cataloging-in-Publication Data is available. ISBN: 9781118880944 Printed in the United States of America 10 9 8 7 6 5 4 3 2 1
  • 7. CONTENTS PREFACE xi CHAPTER 1 INTRODUCTION 1 1.1 Introduction 1 1.2 Background 3 1.3 History of Power Switches and Power Converters 4 1.4 Applications of Power Electronics Converters 6 1.5 Summary 9 References 9 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS 10 2.1 Introduction 10 2.2 Power Electronics Devices as Ideal Switches 11 2.2.1 Static Characteristics 12 2.2.2 Dynamic Characteristics 12 2.3 Main Real Power Semiconductor Devices 16 2.3.1 Spontaneous Conduction/Spontaneous Blocking 17 2.3.2 Controlled Conduction/Spontaneous Blocking Devices 18 2.3.3 Controlled Conduction/Controlled Blocking Devices 19 2.3.4 Spontaneous Conduction/Controlled Blocking Devices 22 2.3.5 List of Inventors of the Major Power Switches 24 2.4 Basic Converters 25 2.4.1 dc–dc Conversion 28 2.4.2 dc–ac Conversion 33 2.4.3 ac–dc Conversion 43 2.4.4 ac–dc Conversion 49 2.5 Summary 50 References 52 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING ac VOLTAGE AND POWER BLOCKS GEOMETRY 56 3.1 Introduction 56 3.2 Principles of Power Blocks Geometry (PBG) 58 3.3 Description of Power Blocks 62 3.4 Application of PBG in Multilevel Configurations 67 3.4.1 Neutral-Point-Clamped Configuration 68 v
  • 8. vi CONTENTS 3.4.2 Cascade Configuration 72 3.4.3 Flying Capacitor Configuration 75 3.4.4 Other Multilevel Configurations 79 3.5 Application of PBG in ac–dc–ac Configurations 81 3.5.1 Three-Phase to Three-Phase Configurations 82 3.5.2 Single-Phase to Single-Phase Configurations 85 3.6 Summary 85 References 87 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION 88 4.1 Introduction 88 4.2 Three-Level Configuration 89 4.3 PWM Implementation (Half-Bridge Topology) 93 4.4 Full-Bridge Topologies 95 4.5 Three-Phase NPC Converter 98 4.6 Nonconventional Arrangements by Using Three-Level Legs 101 4.7 Unbalanced Capacitor Voltage 108 4.8 Four-Level Configuration 112 4.9 PWM Implementation (Four-Level Configuration) 115 4.10 Full-Bridge and Other Circuits (Four-Level Configuration) 118 4.11 Five-Level Configuration 119 4.12 Summary 124 References 124 CHAPTER 5 CASCADE CONFIGURATION 125 5.1 Introduction 125 5.2 Single H-Bridge Converter 126 5.3 PWM Implementation of A Single H-Bridge Converter 129 5.4 Three-Phase Converter—One H-Bridge Converter Per Phase 140 5.5 Two H-Bridge Converters 144 5.6 PWM Implementation of Two Cascade H-Bridges 146 5.7 Three-Phase Converter—Two Cascade H-Bridges Per Phase 149 5.8 Two H-Bridge Converters (Seven- and Nine-Level Topologies) 162 5.9 Three H-Bridge Converters 164 5.10 Four H-Bridge Converters and Generalization 169 5.11 Summary 169 References 170 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION 172 6.1 Introduction 172 6.2 Three-Level Configuration 173 6.3 PWM Implementation (Half-Bridge Topology) 177 6.4 Flying Capacitor Voltage Control 179 6.5 Full-Bridge Topology 181 6.6 Three-Phase FC Converter 183 6.7 Nonconventional FC Converters with Three-Level Legs 186
  • 9. CONTENTS vii 6.8 Four-Level Configuration 189 6.9 Generalization 196 6.10 Summary 197 References 198 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS 199 7.1 Introduction 199 7.2 Nested Configuration 200 7.3 Topology with Magnetic Element at the Output 205 7.4 Active-Neutral-Point-Clamped Converters 211 7.5 More Multilevel Converters 214 7.6 Summary 218 References 219 CHAPTER 8 OPTIMIZED PWM APPROACH 221 8.1 Introduction 221 8.2 Two-Leg Converter 222 8.2.1 Model 222 8.2.2 PWM Implementation 223 8.2.3 Analog and Digital Implementation 228 8.2.4 Influence of 𝜇 for PWM Implementation 231 8.3 Three-Leg Converter and Three-Phase Load 233 8.3.1 Model 233 8.3.2 PWM Implementation 235 8.3.3 Analog and Digital Implementation 236 8.3.4 Influence of 𝜇 for PWM Implementation in a Three-Leg Converter 236 8.3.5 Influence of the Three-Phase Machine Connection over Inverter Variables 238 8.4 Space Vector Modulation (SVPWM) 243 8.5 Other Configurations with CPWM 247 8.5.1 Three-Leg Converter—Two-Phase Machine 247 8.5.2 Four-Leg Converter 249 8.6 Nonconventional Topologies with CPWM 252 8.6.1 Inverter with Split-Wound Coupled Inductors 252 8.6.2 Z-Source Converter 254 8.6.3 Open-End Winding Motor Drive System 257 8.7 Summary 261 References 261 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS 264 9.1 Introduction 264 9.2 Basic Control Principles 265 9.3 Hysteresis Control 271 9.3.1 Application of the Hysteresis Control for dc Motor Drive 275 9.3.2 Hysteresis Control for Regulating an ac Variable 278
  • 10. viii CONTENTS 9.4 Linear Control—dc Variable 279 9.4.1 Proportional Controller: RL Load 279 9.4.2 Proportional Controller: dc Motor Drive System 280 9.4.3 Proportional-Integral Controller: RL Load 283 9.4.4 Proportional-Integral Controller: dc Motor 285 9.4.5 Proportional-Integral-Derivative Controller: dc Motor 286 9.5 Linear Control—ac Variable 288 9.6 Cascade Control Strategies 289 9.6.1 Rectifier Circuit: Voltage-Current Control 289 9.6.2 Motor Drive: Speed-Current Control 290 9.7 Summary 293 References 293 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER 295 10.1 Introduction 295 10.2 Full-Bridge Converter 296 10.2.1 Model 296 10.2.2 PWM Strategy 297 10.2.3 Control Approach 298 10.2.4 Power Analysis 299 10.2.5 dc-link Capacitor Voltage 301 10.2.6 Capacitor Bank Design 304 10.3 Topology with Component Count Reduction 307 10.3.1 Model 307 10.3.2 PWM Strategy 308 10.3.3 dc-link Voltage Requirement 309 10.3.4 Half-Bridge Converter 310 10.4 Topologies with Increased Number of Switches (Converters in Parallel) 310 10.4.1 Model 311 10.4.2 PWM Strategy 315 10.4.3 Control Strategy 316 10.5 Topologies with Increased Number of Switches (Converters in Series) 318 10.6 Summary 321 References 321 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS 324 11.1 Introduction 324 11.2 Full-Bridge Converter 325 11.2.1 Model 325 11.2.2 PWM Strategy 327 11.2.3 Control Approach 328 11.3 Topology with Component Count Reduction 330 11.3.1 Model 330 11.3.2 PWM Strategies 331 11.3.3 dc-link Voltage Requirement 332 11.3.4 Half-Bridge Converter 332
  • 11. CONTENTS ix 11.4 Topologies with Increased Number of Switches (Converters in Parallel) 332 11.4.1 Model 333 11.4.2 PWM 338 11.4.3 Control Strategies 339 11.5 Topologies with Increased Number of Switches (Converters in Series) 340 11.6 Other Back-To-Back Converters 340 11.7 Summary 344 References 344 INDEX 347
  • 13. PREFACE This book deals with a new methodology to present an important class of electri- cal devices, that is, power electronics converters. The common approach to teaching converters is to consider each type individually, in a separate and isolated fashion. The direct consequence is that the learning process becomes passive since the power electronics configurations are presented without consideration of their origin and development. Since the teaching process is based on the topology itself, students do not develop the ability to construct new topologies from the conventional ones. A systematic approach is taken to the presentation of multilevel and back-to-back converters, instead of showing them separately, which is normally done in a conventional presentation. Another special aspect of this book is that it covers only subjects related to the converters themselves. This will give more room for exploring the details of each topology and its concept. In this way, the method of con- ceptual construction of power electronics converters can be highlighted appropriately. While presenting the basics of power devices, as well as an overview of the main power converter topologies in Chapter 2, this book focuses primarily on con- figurations processing ac voltage through a dc-link stage. This text is ideally suited for students who have previously taken an introductory course on power electronics. It serves as a reference book to senior undergraduate and graduate students in elec- trical engineering courses. However, due to the content in Chapter 2, it is expected that even students who the lack knowledge of power devices and basic concepts of converters can understand the subject. Although the primary market for this text is heavily academic, electrical engi- neers working in the field of power electronics, motor drive systems, power systems, and renewable energy systems will also find this book useful. The organization of the book is as follows: Chapter 1 is the introductory chapter. Chapter 2 presents the basics of power devices as well as an overview of the main power converter topologies. Chapter 3 provides a brief review of the main power electronics converters that process ac voltage; additionally, it furnishes the introduction to the power blocks geometry (PBG), which will be used to describe the power converters described in this book. In fact, this chapter brings up a compilation of the topologies explained throughout this book. The fundamentals of PBG and its correlation to the development of power electronics converters are presented in a general way. Multilevel configurations are presented from Chapters 4–7. Neutral-point-clamped, cascade, flying capacitor, and other multilevel configura- tions are presented in Chapters 4–7, respectively. Chapter 8 deals with techniques for optimization of the pulse width modulation (PWM), considering the fact that the number of pole voltages is higher than the number of voltages demanded by the load. After describing many topologies throughout Chapters 2–7, highlighting the circuits xi
  • 14. xii PREFACE themselves, as well as PWM strategies in Chapter 8, Chapter 9 handles control actions needed to keep a specific variable of the converter under control. Chapter 9 is strategically placed before the presentation of the back-to-back converters (Chapters 10 and 11) due to their need for regulation of electrical variables. Single-phase to single-phase back-to-back converters are presented in Chapter 10, and the final chapter deals with three-phase to three-phase back-to-back converters. Euzeli Cipriano Dos Santos Jr. Edison Roberto Cabral Da Silva
  • 15. CHAPTER 1 INTRODUCTION 1.1 INTRODUCTION Power electronics may be considered a revolutionary field in electrical engineer- ing because of the new insights obtained during its development. This has actually been the case from the beginning, when mercury arc rectifiers and thyratrons were employed in grid-controlled circuits. After this first generation of power devices and converters, power electronics with silicon power diodes and thyristors was developed to overcome many of the problems of the first generation, such as the operation in low efficiency. As mentioned in Reference 1, the so-called power electronics, with gas tube and glass-bulb electronics, was known as industrial electronics, and the power electronics with silicon-controlled rectifiers began emerging in the market in the early 1960s. The different definitions of power electronics lead to the same concept or idea: that the control of power flow between an apparatus that furnishes electrical energy and another one that demands electrical energy. For instance, the definition given in References 2 and 3 say, respectively: “ … power electronics involves the study of electronic circuits intended to control the flow of electrical energy. These circuits can handle power flow at levels much higher than the individual devices ratings … ” and “ … power electronics deal with conversion and control of electrical power with the help of electronic switching devices.” Power electronics involves several academic disciplines creating a complex system, including semiconductor physics, control theory, electronics, power systems, and circuit principles. The comprehensive aspect of power electronics makes the pre- sentation of its contents difficult. The interdisciplinary nature of power electronics requires the integration of the practices and assumptions of all the academic dis- ciplines involved, as well as calling for significant prerequisites on the part of the students enrolled for the course. Figure 1.1 illustrates this by analogy, with the pre- requisite skills needed for a power electronics course being shown as the roots of a tree, the various power electronics devices as the trunk, and the resulting technologies and applications (power quality, renewable energy systems, etc.) as the branches. Since the dawn of solid-state power electronics, the use of semiconductor devices has been the major technology to drive power processors. A comparison Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 1
  • 16. 2 CHAPTER 1 INTRODUCTION Power quality Motor drive Renewable energies Computer Control Electronics Circuits Math Physics Hybrid electric vehicles Power systems Figure 1.1 Interdisciplinary nature and new insights obtained from power electronics. of the semiconductor devices formerly used in controlled rectifiers with new technologies underlines this dramatic development. In addition to the improvement of power switches, there has also been great activity in terms of circuit topology innovations. A power electronic converter is the centerpiece of many electrical systems. Common applications include, but are not limited to, motor drive systems, renew- able energies, robotics, electrical and hybrid vehicles, and circuits promoting power quality. These applications have required considerable research worldwide to develop semiconductor devices, configurations that process ac and dc variables, control and diagnosis, fault-tolerant systems, and the like. In addition to the technical side mentioned already, the educational aspects have considerable importance, as students usually consider power electronics courses to be particularly difficult, perhaps because of their interdisciplinary nature. Achieving student motivation is thus a fundamental task of educators involved in the field of power electronics. In this context, this book discusses a novel methodology for presenting an important set of power electronics converters, that is, topologies that process ac voltage. The common approach to teaching converters is to consider each type individually, in a separated and isolated manner. The direct consequence is that the learning process becomes passive as the power electronics configurations are pre- sented without any consideration of their origin and development. Since the teaching process is based on the topology itself, students develop no ability to construct new topologies, different from the conventional ones. Section 1.2 outlines this new methodology.
  • 17. 1.2 BACKGROUND 3 1.2 BACKGROUND Although presenting the basics of power devices as well as an overview of the main power converter topologies in Chapter 2, this book focuses primarily on configura- tions processing ac voltage through a dc-link stage. This book is ideally suited for students who have already taken an introductory course in power electronics. It also serves as a reference book to senior undergraduate and graduate students in electrical engineering courses. However, students can easily manage despite the lack of knowl- edge of power devices and basic concepts of converters, because they are explained in Chapter 2. Systems with power electronics conversion have been used to guarantee grid and load requirements in terms of controllability and efficiency of the electrical energy demanded, especially in industrial applications. Power electronics topologies convert energy from a primary source to a load (or to another source) requiring any level of processed energy. Classifications of the power electronics topologies can be done in terms of the type of variable under control (i.e., ac or dc), as well as the number of stages of power conversions used, as observed in Fig. 1.2. Figure 1.2(a) shows, in a general way, many of the possibilities related to energy conversion. Figure 1.2(b) highlights a direct ac–ac conversion, which converts an ac voltage (v1) with a specific frequency (f1) to another ac voltage with a different (or same) voltage (v2) and frequency (f2); this converter is normally called a cycle converter. Figure 1.2(c) depicts the ac–dc or dc–ac conversion, while Fig. 1.2(d) shows a dc–dc converter. Even admitting ac (ν1,f1) dc (V3) (a) (b) (c) (d) (e) (f) dc (V3) dc (V4) dc (V3) dc (V4) dc (V4) ac (ν2,f2) ac (ν1,f1) ac (ν2,f2) ac (ν1,f1) ac (ν2,f2) ac (ν1,f1) dc (V3) dc (V3) dc (V4) dc (V3) dc (V4) dc (V4) ac (ν2,f2) ac (ν1,f1) ac (ν2,f2) ac (ν1,f1) ac (ν2,f2) Figure 1.2 Power conversion: (a) all possibilities of conversion, (b) cycle converter, (c) rectifier or inverter, (d) chopper, (e) ac–dc–ac, and (f) dc–ac–dc.
  • 18. 4 CHAPTER 1 INTRODUCTION that Fig. 1.2(e) and 1.2(f) could be considered as extended versions of the previous cases, those conversion systems (ac–dc–ac and dc–ac–dc) are presented in Fig. 1.2 because of the large use in different applications. Special attention is given to the conversion systems presented in Fig. 1.2(c) and 1.2(e), dealing with configurations that process ac voltage (at input and/or output converter sides) with one dc stage. A systematic approach is taken for the presenta- tion of those configurations, instead of just showing them separately, as is normally done in a conventional presentation. Another aspect of this book is that only the sub- jects related to the converters themselves will be considered, which means that the contents dealing with either ac filters or transformers will be omitted. This will give more room for exploring the details of each topology and its concept. In this way, the method of conceptual construction of power electronics converters can be highlighted appropriately. 1.3 HISTORY OF POWER SWITCHES AND POWER CONVERTERS Configurations of power electronics converters have provided an attractive alterna- tive for the applications needing energy processing, considering the acceptable level of losses associated with the conversion process itself, as well as improvement in reliability. As previously mentioned, power electronics converters must control the power flow, which means that the development of the devices used in those convert- ers is crucial to guarantee the expected features. In this section, a historic view of the power electronics devices will be furnished, highlighting the main events that contributed to the current development. The history of power electronics predates the development of the semiconduc- tor devices employed nowadays. The first converters were conceived in the early 1900s, when the mercury arc rectifiers were introduced. Until the 1950s the devices used to build power electronics converters were grid-controlled vacuum tube recti- fier, ignitron, phanotron, and thyratron. There were two important events in the power electronics development: (i) in 1948, when Bell Telephone Laboratories invented the silicon transistor, with applications in very low power devices such as in portable radios and (ii) in 1958, when the General Electric Company developed the thyristors or SCR, first using germaniums and later silicon. It was the first semiconductor power device. Besides these two events, many developments have been achieved in terms of switching development. Between 1967 and 1977, the gate turnoff (GTO) (gate-controlled switch) and gate-assisted turnoff thyristor (GATT) (gate-assisted turnoff switch) were invented. Power transistors, MOSFETs (metal oxide semi- conductor field-effect-transistors), MCTs (MOS-controlled thyristor) and IGBTs (insulated-gate-bipolar transistors) have been invented since the end of 1970s. In addition, it is worth mentioning that the area of power electronics was deeply influenced by microelectronics development, and the history of power electronics is closely related to advances in integrated circuits to control switching power supplies.
  • 19. 1.3 HISTORY OF POWER SWITCHES AND POWER CONVERTERS 5 Power transistors, MOSFETs (metal oxide semiconductors Field-Effect-Transistors), MCTs (MOS controlled thyristor) and IGBTs (Insulated-gate-bipolar transistor) were invented since the end of 1970s 1977 1980 GTO (gate-controlled switch) and GATT (gate-assisted-turnoff switch) were invented First semiconductor power device. General Electric Company developed the thyristor or SCR 1967 Bell Telephone Laboratories invented the silicon transistor with former applications in very low power applications such as in portable radios 1958 1948 The first investigators to study controlled rectification in gas tubes The mercury arc rectifier was invented by Peter Cooper Hewitt. Before the advent of solid-state devices, mercury-arc rectifiers were one of the most efficient rectifiers 1914 1900 Figure 1.3 Timeline of historical events in the power electronics devices evolution. Figure 1.3 depicts the timeline showing the development of power electronics devices. An important chapter in the history of power electronics converters was the development of switching power suppliers. In 1958, the IBM 704 computer, which was developed for large-scale calculations, used as a switching power supplier the primitive vacuum tube-based switching regulator. But the revolution in power sup- plier concepts came in the late 1960s, when the switching power supplies replaced the linear ones. In a linear power supply, regulated dc voltages are obtained from the ac utility grid throughout the following sequence of steps: (i) 60 Hz power transformer, to converter 120 ac voltage at the primary transformer side to low voltage at secondary transformer side; (ii) such voltage is converted to dc with a simple diode rectifier; and (iii) a linear regulator drops the voltage to a desired value. Indeed, it is possible to identify many problems related to this technology, such as low efficiency (50–65% of the power is wasted as heat), and it was heavy and large (mainly due to the low frequency transformer, heatsink and fans to deal with the heat). The advantages are that it has a very stable output voltage and the conversion system is noise-free. To overcome the disadvantages of the linear regulators, General Electric pub- lished a design of an early stage switching power supply in 1959. The concept of switching power suppliers is very different from linear regula- tors. Instead of conducting power 100% of the time (i.e., turning excess power into heat), the switches and passive elements are connected to rapidly turn the power on and off. Unlike linear regulators, the ac utility voltage is converted directly to dc volt- age, and the gating signal controls the time of the switching, regulating the average voltage desired at the output converter end.
  • 20. 6 CHAPTER 1 INTRODUCTION Another important development in power electronics configurations was the controlled rectifiers, especially with the production of the silicon-controlled rectifier (SCR or thyristor). Such a device allowed the control of high power by just changing the signal applied to its gating circuit with higher efficiency rather than the older technology of employing a mercury arc rectifier. 1.4 APPLICATIONS OF POWER ELECTRONICS CONVERTERS The range of applications for power electronics converters is so large that it goes from low power residential applications to high power transmission lines. Many of those applications can be considered as traditional ones (e.g., rectification circuits and motor drive systems). On the other hand, a few emerging applications have generated wide interest (e.g., renewable energy systems). A brief discussion matching the power electronics converters with those applications will be introduced here, with the details of those applications being presented throughout the chapters. Figures 1.4 and 1.5 summarize some examples that demonstrate the presence of power electronics in a wide range of applications. Figure 1.4(a) shows schemati- cally the application of power electronics in hybrid/electric vehicles. From the power Power electronics apparatus Memory CPU Source Nano-grid house Energy-control- center PV PV Outlet ECC Single-phase utility grid Hard drive DC DC DC dc dc DC (a) (c) (b) (d) Figure 1.4 Applications of power electronics using converters that process ac voltage.
  • 21. 1.4 APPLICATIONS OF POWER ELECTRONICS CONVERTERS 7 Macro grid Micro grid Power converter C C ac motor Wind generation C C C dc motor PV generation C HEV Energy Control Center (ECC) Loads T T ac DC ac or Coal-fired generation Single-phase utility grid Long-distance transmission lines Hydroelectric generation Centralized generation Transformer Figure 1.5 Application of power electronics in a distributed generation system. C stands for converter. electronics point of view, the hybrid and fully electric automobiles differ one from another, mainly due to the power ratings of the inverters used. While a typical inverter rating is about 50 kW for the hybrid vehicle, the inverter rating for a fully electric vehicle is about 200 kW. The inverter motor drive system that furnishes energy to the power-train is by far the most important power electronics system used in this kind of
  • 22. 8 CHAPTER 1 INTRODUCTION application, but the battery charge and other peripheral systems are also crucial. The main features expected in this application are high efficiency performance, compact on-board energy storage, and low manufacturing cost for market competition with conventional thermal-engine vehicles. Desktop and laptop computers can be considered as systems with on-board distribution schemes where different dc bus voltages are required. Inside these equip- ment can be found many power electronics converters, as seen in Fig. 1.4(b). An ac–dc converter produces a dc voltage bus from an ac utility grid, which will be employed by different dc–dc converters to supply the microprocessor, disk drive, memory, and so on. In the case of laptops, a battery charger is added with a power management system to control sleep modes, which guarantees extension in battery life via power consumption reduction. Figure 1.4(c) shows the application of the power electronics converters in renewable energy systems, which nowadays is a hot topic in the political agenda of many industrialized countries, mainly due to environmental issues and as an alternative way to establish a decentralized generation system. It is worth mentioning that, besides the advantages of renewable energy, this kind of system presents a high price energy generation, especially when it is compared to conventional sources such as hydroelectric power and coal. In this sense, power electronics converters must deal with efficiency, reliability, and cost reduction, in order to make those alternative sources of energy more competitive. Figure 1.4(d) shows a trolley bus, which is an electric bus that receives electrical energy directly from overhead wires (generally suspended from roadside posts) by using spring-loaded trolley poles. A well-defined traditional power distribution system has a radial topology and unidirectional power flow to feed end-users. However, in the last few years, there has been research and development in replacing this paradigm by a new and complex multisource system with active functions and bidirectional power flow capability. In this new scenario, the utility grid is supposed to guarantee load management and demand side management, as well as using market price of electricity, and forecasting of energy (e.g., based on wind and solar renewable sources) in order to optimize the distribution system as a whole. A microgrid can be defined as a localized grouping of electricity generation, energy storage, and loads that are normally connected to a traditional centralized grid (macrogrid), as seen in Fig. 1.5. Figure 1.5 shows a microgrid with a dc bus, where the power converters (represented generically by the letter C) interface dis- tributed sources and loads with the dc bus. The point of common coupling (PCC) between micro- and macrogrid can be disconnected, which means that the microgrid can then operate autonomously. In this case, an island detection system is necessary, which safely disconnects the microgrid. The interface between micro- and macrogrid is possible due to advances made in the power electronics The important equipment in this scenario is the Energy-Control-Center (ECC), consisting of a bidirectional ac–dc (or dc–ac) power conversion converter used to interface the utility ac grid and dc bus. The multiple dispersed generation sources and the ability to isolate the microgrid from a larger network would provide highly reliable electric power.
  • 23. REFERENCES 9 Another important area in which power electronics is becoming more and more common is in aerospace industry. Many loads classically powered by hydraulic net- works were replaced by electrical power loads (e.g., pumps and braking). Besides facing the common challenges, the power electronics converters must deal with harsh environment constraints in terms of temperature, low pressure, humidity, and vibra- tions. 1.5 SUMMARY Following the introduction, this chapter presents in Section 1.2 the background of the book, highlighting the type of configurations that this book will deal with (i.e., dc–ac and ac–dc–ac converters). Section 1.3 gives a brief history of the power electronics devices and power electronics converters, focusing on the development of switch- ing power suppliers and SCR rectifiers. Finally, some applications are considered in Section 1.4 to show the wide range of applications of power electronics converters. Readers can find further discussion from References 4 to 13. REFERENCES [1] Liserre M. Dr. Bimal K. Bose: a reference for generations [editor’s column]. IEEE Ind Electron Mag 2009;3(2):2–5. [2] Rashid MH. Power Electronics Handbook: Devices, Circuits, and Applications. San Diego, CA: Elsevier; 2007. p 1–2. [3] Bose BK. Power Electronics and Motor Drives: Advances and Trends. San Diego, CA: Elsevier; 2006. p 1–3. [4] Blaabjerg F, Consoli A, Ferreira JA, van Wyk JD. The future of electronic power processing and conversion. IEEE Trans Ind Appl 2005;41(1):3–8. [5] Gutzwiller FW. Thyristors and rectifier diodes - the semiconductor workhorses. IEEE Spectr 1967;4:102–111. [6] Elasser A, Kheraluwala MH, Ghezzo M, Steigerwald RL, Evers NA, Kretchmer J, Chow TP. A comparative evaluation of new silicon carbide diodes and state-of-the-art silicon diodes for power electronic applications. IEEE Trans Ind Appl 2003;39(4):915–921. [7] dos Santos EC Jr, Jacobina CB, da Silva ERC, Rocha N. Single-phase to three-phase power convert- ers: state of the art. IEEE Trans Power Electron 2012;27(5):2437–2452. [8] Goldman A. Magnetic Components for Power Electronics. Kluwer Academic Publishers; 2002. [9] IBM Customer Engineering Reference Manual: 736 Power Supply, 741 Power Supply, 746 Power Distribution Unit; 1958. p 60–17. [10] Karcher EA. Silicon controlled rectifiers in monolithic integrated circuits. Electron Devices Meeting, 1965 International; vol. 11; 1965. p 6–17. [11] Mohan N, Undeland TM, Robbins WP. Power Electronics: Converters, Applications, and Design. 3rd ed. John Wiley & Sons; 2002. [12] Rashid MH. Power Electronics: Circuits, Devices, and Applications. Prentice Hall; 1993. [13] El-Hawary ME. Principles of Electric Machines with Power Electronic. Wiley: IEEE Press; 2002.
  • 24. CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS 2.1 INTRODUCTION The basic principles and characteristics of the main power switches are presented in this chapter. Furthermore, an overview of the principal power electronics converters is furnished, highlighting the main characteristics for each type of topology. Semiconductor power devices are the center piece of the power elec- tronics converters. While the knowledge about such devices is crucial to design a power converter with specific characteristics for a given application, the study of different topologies brings up new possibilities to improve the energy process system. Before dealing specifically with pulse-width modulation (PWM) converters processing ac voltage, which is the core of this book, this chapter considers a large variety of power conversion possibilities. The converters studied in this chapter include dc–dc, dc–ac, ac–dc, and ac–ac converters, as well as voltage-, and current-source converters. As the objective is to furnish an overview of the different types of switches and converters, a deep analysis of the converters described in this chapter is omit- ted. However, the following chapters present a systematic description of both power converters, called Power Block Geometry, and the advanced PWM converters pro- cessing ac voltage (e.g., multilevel converters and back-to-back converters) to the smallest detail. This chapter is organized as follows: Section 2.2 presents the ideal charac- teristics of the major power switches available in the market, highlighting their static and dynamic features; Section 2.3 shows the real characteristics of such semiconductor devices, sorted in terms of dynamic characteristics; Section 2.4 describes basic power electronics converters, and finally, Section 2.5 summarizes the chapter. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 10
  • 25. 2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES 11 2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES The design and construction of power semiconductor devices focus on how to improve their performance toward the hypothetical concept of an ideal switch. Figure 2.1 shows the power switches and the year of development of each switch. The performance of a given power switch is normally measured by its static and dynamic characteristics. An ideal switch must have the following characteristics: (i) infinite blocking voltage capability, (ii) no current while the switch is off, (iii) infinite current capability when on, (iv) drop voltage equal to zero while on, (v) no switching or conduction losses, and (vi) capability to operate at any switching frequency. There are different ways to classify a power switch. In this book, two differ- ent ways are considered: static characteristics and dynamic controllability. The main Ideal switch GalliumARsenide (GAAS) technology Silicon carbide (SiC) technology BCT - Bilateral conduction thyristor (1999) IGCT – Integrated gate- commutated thyristor (1996) SITH static induction thyristor, normally “on” (1983) MOSFET – metal-oxide field effect transistor (1975) TRIAC (1963) SCR – silicon-controlled rectifier, thyristor (1956) Magnetic amplifier (1947) Mercury arc rectifier (1902) Thyratron (1920) Ignitron (1930) BJT – bipolar junction transistor (1950) GTO (1960) RCT (1963) IGBT – insulated gate bipolar transistor (1983) MTO – MOS turn-off (1995) ETO – emitter turn-off (1998) Figure 2.1 Development of the power switches toward the concept of the ideal switch.
  • 26. 12 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS figures of merit for the static characteristics are the graphs describing the current versus voltage behaviors (I–V). On the other hand, for the dynamic features, the capability to change the states on and off through either an external signal (gat- ing command) or by the variables of the circuit in which the switch is connected is considered. For example, there is no gating signal to turn on and off a diode, its conduction or blocking depends upon the voltage and current imposed by the circuit. 2.2.1 Static Characteristics The static characteristics of the power semiconductor devices are related to their abil- ity to either conduct or block one or two polarities, as shown in Fig. 2.2. Figure 2.2(a) and 2.2(b) shows the ideal I–V characteristic for the blocking and conducting states, respectively. Figure 2.2(c)–2.2(g) depicts the voltage versus current (I–V) ideal characteristics for the main devices found in the market. The semiconductor devices can, therefore, operate with either unidirectional or bidirectional (UniC or BidC) current, and with either unidirectional or bidirectional voltage (UniV or BidV). For example: (i) diode, bipolar junction transistor (BJT), and insulated bipolar junction transistor (IGBT) are unidirectional voltage and cur- rent type of devices, (ii) SCR is an unidirectional current and bidirectional voltage device, (iii) TRIAC and bidirectional controlled thyristor (BCT) are bidirectional in current and voltage, and (iv) MOSFET is unidirectional in voltage and bidirectional in current. The characteristics presented in Fig. 2.2(c)–2.2(g) play an important role for the specification and design of the power electronics converters. These graphs are in fact approximations of the real I–V characteristics of the device. For example, Fig. 2.2(c) is an approximation of the real characteristics of a power diode, which is presented later in this chapter. 2.2.2 Dynamic Characteristics The dynamic characteristics of a specific device are related to the behavior of voltage and current when there is a change either from conduction to blocking state or from blocking to conduction. Such a change is known as commutation or switching. The commutation (or switching) from the blocking state to the conduction state is referred to as either turn-on or conduction. The commutation from the conduction state to the blocking state is referred to as either turn-off or blocking. For the I–V characteristic curves (shown in Fig. 2.2), the commutation process corresponds to going from the operating point on an axis to another one. For example, for a switch UniC/UniV with direct voltage as in Fig. 2.2(c), the blocking procedure makes the variables of the switch (voltage and current) go from the I-axis to the V-axis. In fact, the commutation process can be spontaneous or controlled, as shown in Fig. 2.3. Four cases are presented as follows: • Spontaneous conduction (SC)—see Fig. 2.3(a); • Spontaneous blocking (SB)—see Fig. 2.3(b);
  • 27. 2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES 13 Blocking state (a) Conducting state (b) Unidirectional current (UniC) Unidirectional (reverse) voltage (UniV-r) (c) Unidirectional current (UniC) Unidirectional voltage(UniV) (d) Unidirectional current (UniC) Bidirectional voltage (BidC) (e) Bidirectional current (BidC) Unidirectional voltage (UniV) (f) Bidirectional current (BidC) Bidirectional voltage (BidV) (g) i ν i ν i ν i ν i ν i ν i ν Figure 2.2 Ideal I–V characteristics for blocking and conduction states of the power switches available in the market. • Controlled conduction (CC)—see Fig. 2.3(c); • CB—see Fig. 2.3(d). In the case of spontaneous commutation (i.e., conduction and blocking), the change of state is defined by the variables of the power circuit, while for the controlled
  • 28. 14 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS SC ν i SB ν i CC ν i CB ν i (a) (c) (d) (b) Figure 2.3 Dynamic characteristics of an ideal device considering its commutation process. (a) Spontaneous turn on, (b) spontaneous turn off, (c) controlled turn on, and (d) controlled turn off. commutation, the change of state is guaranteed via a gating signal (command signal). Figure 2.4 shows the behavior of the voltage and current in time-domain (left side) and dynamic characteristics (right side) for SC, SB, CC, and CB. The points (P1, P2, and P3) along with the axes in Fig. 2.4 illustrate the behavior of the variables when the switching process occurs for both spontaneous and controlled commutation. For example, in Fig. 2.4(a) P1 indicates the operation point when the switch is blocked, which means that such a device is submitted to a negative voltage while its current is zero. The operation point P2 shows the device’s behavior while its voltage has been reduced. Finally, P3 shows the values of voltage and current when the switch is turned on. This commutation process occurs, for example, in a rectifier circuit with diodes where the circuit itself allows the state change from blocking to conduction. A similar analysis can be done for SB in Fig. 2.4(b). On the other hand, a controlled commutation device must have a control elec- trode, usually called a gate or base, in addition to the two main terminals. A control signal applied to the gate or base, while the voltage applied between the main termi- nals is positive, results in change of state in a desirable manner, that is, from one axis to another, as shown in Fig. 2.4(c) and 2.4(d). In terms of dynamic characteristics, the ideal power devices can be classified as follows: • SC/SB; • CC/SB; • CC/CB; • SC/CB.
  • 29. 2.2 POWER ELECTRONICS DEVICES AS IDEAL SWITCHES 15 (b) (a) (c) (d) P3 P3 P3 P2 P2 SC P2 P1 P1 P1 t t i i ν ν P3 P3 P3 P2 P2 SB P2 P1 P1 P1 t t i i ν ν P2 P2 CC P2 P1 P1 P1 t t i i ν ν P2 P2 CB P2 P1 P1 P1 t t i i ν ν Figure 2.4 Comparison on time-domain and dynamic characteristics during the commutation process. (a) SC, (b) SB, (c) CC, and (d) CB.
  • 30. 16 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS 2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES The most common power electronics devices are diodes, thyristors, and power tran- sistors. Usually they have two power terminals (anode/cathode, or collector/emitter or drain/source) and one or more command terminals ( gate/ base). Unlike the ideal char- acteristics presented earlier, real devices have practical limits for rated voltage and current, as well as for their operation frequency. Such limits are normally specified by the datasheet furnished by manufacturers. Therefore, the device characteristics and their specification are crucial to choose a particular power device instead of others. The most common nonideal device characteristics are (a) The Forward and Reverse Voltage Capability. The main limiting ratings are as follows: i. Forward Blocking Voltage. The maximum repetitive forward voltage that can be applied to the power terminals of the device (normally from anode to cathode, from collector to emitter, from drain to source) so that the device blocks the current flow (blocking state) in the direct sense, unless com- manded to turn on. ii. Reverse Blocking Voltage. The maximum repetitive reverse voltage that can be applied to the power terminals of the device (from cathode to anode, for instance) so that the device blocks the current flow in the reverse sense. iii. Maximum Peak Nonrepetitive Forward and Reverse Voltage. The maximum nonrepetitive forward and reverse voltages, respectively, under transient conditions. iv. Vdc and VR. Maximum continuous direct (forward) and reverse blocking voltages, respectively. This is the maximum dc voltage that the diode can withstand in reverse-bias mode on a continual basis. v. Forward Voltage Drop. This is the instantaneous value of the drop voltage, which is normally dependent on the temperature. (b) The current capability while the device is on (conducting) is junction temperature-dependent. The main limiting ratings are the following: i. On-State Current. It is the average value of the conduction current. ii. On-State Root Mean Square (RMS) Current. It is the RMS value of the conduction current. iii. Peak Repetitive Forward Current. It is the maximum repetitive current that can flow through the device. iv. Peak Surge Forward Current. It is the maximum nonrepetitive forward cur- rent that can flow through the device under transient conditions. It should be noted that when blocked, the device still conducts a leakage current that can be forward or reverse, depending on the device state. (c) The switching is not instantaneous, so there are limits in the switching fre- quency, as follows: i. Turn-On Time. It is the time required to complete the turn-on process.
  • 31. 2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 17 ii. Turn-Off Time or Recovery Time (trr). it is the minimum interval of time required from the instant the conduction current is decreased to zero so that the device is capable of withstanding the forward voltage without turning on. iii. d𝑣∕dt. It is the maximum variation rate of the forward voltage that can be applied to the device in the blocking state without starting a nonpro- grammed turn-on. iv. di∕dt. It is the maximum variation rate of the forward current during turn-on that can be applied to the device; higher di∕dt than the one specified by the manufacturer may destroy the component. (d) The maximum switching frequency depends on the recovery time of the device. (e) Power Losses. There are three main components of losses in a semiconductor device: (i) switching losses (turn-on and turn-off), (ii) conduction losses, and (iii) reverse conduction losses. The most used devices in industrial applications are considered in the following section. Such switches are sorted in terms of their dynamic characteristics. 2.3.1 Spontaneous Conduction/Spontaneous Blocking The conventional diode and the Schottky diode have the characteristic of SC and SB, as presented in the sequence. The Conventional Diode The conventional diode is a silicon p–n junction device with two terminals, anode (A) and cathode (K), that conducts current from A to K and blocks the reverse current. The rating of the voltage goes up to 9 kV with 4.8 kA and 5 kV with 13 kA. Its symbol is presented in Fig. 2.5(a) and its real I–V characteristic is given in Fig. 2.5(b). The diode conducts when 𝑣AK > 0, the current being limited by the external circuit, its typical direct voltage drop is 0.7 V. Generally speaking, it can be said that they recover their reverse blocking capability when the forward current iA goes to zero and a reverse voltage is applied across its terminals, for an interval of time longer than the reverse recovery time trr obtained in its technical data sheet. In reality, after reaching zero, the current reverses its direction, reaching a reverse peak called “peak reverse recovery current” that is comparable to the forward current. Snubber K νAK A iA iA (a) (b) Figure 2.5 The diode: (a) symbol and (b) I–V characteristic.
  • 32. 18 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS circuits are essential for the adequate protection of the diode. The snubber circuit will protect it from overvoltage spikes, mainly due to the junction capacitance and leakage inductance from terminals and circuit connections. The basic snubber circuit is com- posed of a capacitor in series with a resistor connected in parallel with the diode. The size of the snubber circuit is reduced for the fast (trr < 1 μs) and ultrafast recovery diode (trr < 100 ns), with ratings reaching: (i) 600 V, 30 A and trr = 50 ns, and (ii) 1200 V, 120 A, trr = 85 ns. Recent development in the silicon carbide material allows reducing the diode reverse recovery time up to 16 ns. The Schottky Diode Unlike the standard diode presented previously, the Schottky diode is formed by a metal–semiconductor junction (the p material is replaced by metal). It has a lower conduction drop voltage (typically 0.5 V) and faster switching time than the standard diode (less than 100 ps), which allows its operation in higher frequency. However, it has lower blocking voltage (typically up to 200 V) and higher leakage current. Its silicon carbide (SiC) version is promising and has been already tested to withstand 1.2 kV with 60 A. 2.3.2 Controlled Conduction/Spontaneous Blocking Devices The main devices in this group are the silicon-controlled rectifier (SCR) and the TRI- ode AC (TRIAC). The SCR The SCR is a silicon p–n–p–n device with three terminals: two power terminals, anode (A) and cathode (K) through which the current flows, and a control terminal, named the gate terminal (G). It is unidirectional in current and blocks in both forward and reverse directions (UniC/BidV). The device is triggered by a posi- tive gate current pulse. When the gate is not triggered the SCR blocks the current in the forward direction even with 𝑣AK > 0. If iGK > 0 while 𝑣AK > 0, the SCR conducts the current from anode to cathode imposed by the circuit in which the SCR is inserted. Its voltage drop in conduction is from 1 to 4 V. Once in conduction, the SCR behaves like a diode and it can only be turned off when the anode current becomes zero. After the current reaches zero, a reverse voltage should be applied across its terminals in order to accelerate the capability of forward blocking. Note that the gate loses con- trol over the SCR during its conduction. The symbol and real I–V characteristics are shown in Fig. 2.6(a) and 2.6(b), respectively. The direct and reverse voltages across its terminals are symmetrical in the conventional SCR (there are SCRs with asym- metrical voltage characteristics, the ASCR) and can reach 5 kV with 5 kA and 12 kV with 2.3 kA, or even 5 kV with 8 kA. Unexpected turn-on can occur due to a high d𝑣∕dt. For these reasons a snubber circuit with a capacitor can be used to avoid both triggering by d𝑣∕dt and overvoltage spikes, a resistor that limits the current peak, and an inductor that limits the di∕dt rate. The TRIAC The TRIAC is a thyristor that operates as two SCRs monolithically integrated connected in antiparallel. Such a device can conduct and block in both forward and reverse directions (BidC/BidV). It has two power terminals, T1 and T2, and one gate G. Its symbol and its I–V characteristic are presented in Fig. 2.7(a) and
  • 33. 2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 19 K G νAK A iA iA (a) (b) Figure 2.6 The SCR: (a) symbol and (b) I–V characteristic. 2.7(b), respectively. When 𝑣T = 𝑣T1 − 𝑣T2 is positive (quadrant I) and the TRIAC is turned on by a positive gate current pulse. But when the 𝑣T is negative (quadrant III) it is turned on by a negative gate current pulse. The operation in quadrants II and IV is also possible but the gate triggering is less sensitive in these cases. Also, the d𝑣∕dt is poorer than that of SCRs. Other CC/SB devices are the light-activated SCR (LASCR), the reverse con- ducting thyristor (RCT), which functions as an SCR with an inverse-parallel diode (BidC/UniV), and the BCT, in which two SCRs are also connected in antiparallel, but differently from the TRIAC, each one acting independently with its independent gate control (BidC/BidV). 2.3.3 Controlled Conduction/Controlled Blocking Devices The main CC and CB devices are (1) basic transistors, like the BJT and the metal oxide semiconductor field-effect transistor (MOSFET); (2) basic thyristors, like the gate turn-off (GTO); (3) mixed transistors, like the IGBT; and (4) mixed thyristors, like the MOS-controlled thyristor (MCT) and the Integrated gate commutation thyristor (IGCT). Bipolar Junction Transistor (BJT) Unidirectional in current, the BJT can be either n–p–n or p–n–p and it has asymmetric blocking, only withstanding some tens of reverse blocking voltage (UniC/UniV). Its symbol and static characteristics T2 T1 G νT iT iT (a) (b) Figure 2.7 The TRIAC: (a) symbol and (b) I–V characteristic.
  • 34. 20 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS B E C iB = 0 iC iB iC iB νCE (a) (b) Figure 2.8 The BJT: (a) symbol and (b) I–V characteristic. are shown in Fig. 2.8. It has three terminals, the collector (C) and emitter (E) through which the current (ic) flows and the base (B) that controls the amplitude of ic. Unlike lower power BJT devices, the power devices operate in the quasi-saturated region, which reduces the stored charge, avoiding the long recovery time obtained when operated in the saturated region. As its dc current gain (hfe) is much lower than its signal level counterpart (in general as low as 5), the Darlington connection is more common because its dc current gain is higher. A disadvantage of this arrangement is its drop voltage and leakage current. BJTs with forward blocking voltage up to 1 kV are available. The MOSFET Application of the metal oxide semiconductor (MOS) technology to the field-effect transistor resulted in the power MOSFET. It has three terminals, the drain (D), the source (S), and the gate (G). Its symbol and I–V characteristics are shown in Fig. 2.9. It is an n–p–n, or p–n–p, device in which its two p–n, or n–p, layers are connected through a metal, so that a capacitor is formed between G and D. The MOSFET is turned on by a voltage pulse. The MOSFET acts as a resistance while conducting and behaves like a transistor before being turned on. Similar devices have been developed under different names, depending on the manufacturer, such as the HEXFET (“hexagonal-field-effect-transistor”), SIPMOS (“Siemens-Power Metal Oxide Silicon”) and TMOS (“T flowing current metal oxide silicon”). Its forward blocking voltage is in the range of 1 kV and it can operate in high frequency. Since it has an intrinsic diode in antiparallel connection, it operates with forward and reverse current and can be classified as a BidC/UniV device. It has replaced the BJT in the range of low voltage and high frequency but its disadvantage comes from its high conduction resistance that increases with the voltage. G S D νGS = 0 iD iD νGS νDS (a) (b) Figure 2.9 The MOSFET: (a) symbol and (b) I–V characteristic.
  • 35. 2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 21 G E C iC iC νGE νCE (a) (b) Figure 2.10 The IGBT: (a) symbol and (b) I–V characteristic. However, it has been demonstrated that SiC MOSFET can have extremely low on-resistance, thus saving energy. It has been predicted that in some applications the SiC MOSFET will replace the Si-IGBT in the voltage range of more than 1 kV. The IGBT The IGBT promoted a great revolution in power electronics as it uses a mixed bipolar-MOSFET technology. It combines the advantages of the MOSFET and the BJT Darlington, with controlled turn-on and turn-off. Like the MOSFET it has a high input impedance and needs low energy to be switched on. Its symbol and I–V characteristics are given in Fig. 2.10. The IGBT conduction drop voltage is small (from 2 to 3 V in a device of 1 kV). The conventional device is unidirectional in cur- rent and only blocks forward voltage (UniI/UniV) with a voltage of 6.5 kV for 750 A, or 1.7 kV for 3.6 kA for d𝑣∕dt of order from 50, 000 V∕μs to 100, 000 V∕μs. The type NPT (“nonpunch-through”) can reach 3.5 kV and 2 kA. Its typical turn on and turn off time is from 200 ns to 1 μs. It is possible to design it to block the voltage in both directions, forward and reverse voltages. Such a device has been recently introduced in the market with the name of reverse blocking IGBT but for lower voltage (1.7 kV) and current (25 A), 1200 V∕40 A, 600 V∕200 A. As for the MOSFET, the SiC tech- nology is also designing SiC–IGBT, which has reached the high blocking voltage of 15 kV. The GTO The GTO did appear to give thyristors the option to control its turn-off. Its symbol and I–V characteristics are given in Fig. 2.11 and it is, normally, a UniC/UniV device. For turning on, it only needs a small pulse of positive current at the gate. However, its turn-off current gain of the negative current pulse is typically 3–5, which means that for turning off a 6 kV∕6 kA GTO, it needs a negative gate A K G iA iA νAK (a) (b) Figure 2.11 The GTO: (a) symbol and (b) I–V characteristic.
  • 36. 22 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS current pulse of 1.5 kA. The reverse blocking GTO can withstand reverse voltage of 4.5 kV with 3 kA. Also, the GTO needs snubbers when used with inductive load. The MCT The MCT is also called MOS-GTO and combines the characteristics of the FET integrated with the p–n–p–n structure of a thyristor. It is a UniC/UniV device. When designed, it was expected that it would be able to handle more than 200 kVA and more than 1 MVA in subsequent years. In conduction, it approximates to the SCR characteristics. Its blocking is obtained through the turn-off gate. How- ever, even though it reached values of 2 and 3 kV and hundreds of amperes, its acceptance by the market is still undefined at the moment. Its symbol is given in Fig. 2.12(a). The IGCT The IGCT was introduced in 1997 and it is a high voltage, high power, asymmetric blocking device, with a structure very similar to a GTO thyristor. As it is designed with a monolithically integrated antiparallel diode, it is a BidC/UniV type of device. Its symbol is given in Fig. 2.12(b). It is a device with unity turn-off current gain. This means that a 4.5 kV IGCT with a controllable anode current of 3000 A requires a turn-off negative gate current of 3 kA. So it needs a great amplification for turn off and, also, the gate driver must have an ultralow leakage inductance in order to have short duration and very large di∕dt. With this purpose, the gate drive circuit is built in and such integration between the command and the device results in high turn-off speed (1 μs) and basically eliminates the problem of d𝑣∕dt found in GTOs permitting snubberless operation. In IGCTs the cathode current is diverted to the gate before any distribution of current between gate and anode is observed so that the structure p–n–p–n can be converted to a p–n–p structure. As a result, the IGCT conducts as a GTO but turns off as an IGBT, combining the characteristics of these devices. Other parameters superior in the IGCT as compared to the GTO are the con- duction drop voltage and gate-driver loss. Its typical frequency is around 500 Hz it can reach 1 kHz. The device has been applied in power system installations of 100 MVA and medium power (up to 5 MW) industrial drives. Like the GTO and IGCT, the reverse blocking IGCT (RBIGCT), symmetric, has been recently developed, and can withstand 5 kV. 2.3.4 Spontaneous Conduction/Controlled Blocking Devices Two devices can be classified as SC/CB, that is, the static induction transistor (SIT) normally-on and the Static Induction Thyristor (SITH) normally-on. K K A G G A (a) (b) Figure 2.12 Symbol of the: (a) MCT and (b) IGCT.
  • 37. 2.3 MAIN REAL POWER SEMICONDUCTOR DEVICES 23 K S D G G A (a) (b) Figure 2.13 Symbol of: (a) SIT and (b) SITH. The SIT The SIT, also known as Junction Field-Effect Transistor (J-FET), is an n-type field-effect transistor, voltage driven. Its symbol is given in Fig. 2.13(a). It is a UniC/UniV device with ratings of 1.2 kV and 300 A and can operate up to 100 kHz. It conducts when 𝑣GS = 0 and its drain current can be controlled by the gate-source voltage, 𝑣GS. However, the gate-source voltage required for turning off the device is high and it is not uncommon that a voltage as high as 40 V (negative) is needed. This characteristic of normally turned on with controlled turn-off classifies the device as SC/CB (the SIT normally-off has been already developed, with limited performance). However, its high forward voltage makes it unsuitable for most power electronics applications, unless radio frequency operation is needed. Additionally, the difficulty in manufacturing it raises concerns about its mass production. This device has been shown to be more promising with the SiC technology reaching ratings of 1.2 kV∕17 A and 6.5 kV∕5 A. Its range of power operation is up to 50 kW. It has been shown that a SiC SIT of 125 V∕2.2 kW can operate in the ultrahigh frequency range up to 450 MHz. However, the gate-source voltage required for turning this device off is about VGS = −30 V. Although SiC SIT is a normally-on device, recently a SiC SIT normally-off has been developed with ratings of 1.2 kV and 35 A, with a turn-off VGS of only −2.5 V. The SITH The SITH, or SIThy, a device unidirectional in voltage, is a combination of an n-channel SIT and a p–n–p transistor. Its symbol is given in Fig. 2.13(b). It is a normally-on device with turn-off controlled by negative gate voltages and it does not have reverse blocking capability. It can handle currents in the range of 300 A to 2 kA with a recovery time from 2 to 4 μs and it is a device rated with 1.5 kV∕300 A and has a rated frequency of 10 kHz but it is expected to be applied to power sources up to 10 MHz. Although it can operate at higher frequencies compared to the GTO, its higher drop voltage and lower current gain are its main disadvantages. As for the SIT, the complexity of the manufacture process and the high negative gate voltage for turning it off are its major drawbacks. Exercise 2.1 The simple circuit presented below allows the power flow control between the voltage source (Vdc = 1 kV) and the resistive load (Ro), by turning-on and -off the switch S with switching frequency equal to fs. From the ratings of the
  • 38. 24 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS switches given in this chapter determine the appropriate power device to be employed as the switch S, considering the following conditions: (a) fs = 1 kHz and Ro = 0.6 (b) fs = 50 kHz and Ro = 2.5 (c) fs = 200 kHz and Ro = 10. Vdc S Ro 2.3.5 List of Inventors of the Major Power Switches The list of inventors of the major power devices available in today’s market is pre- sented here: • Diode pn. The first semiconductor diode, a germanium-made device, was cre- ated in 1952, 200 V/35 A, by R.N. Hall. Its counterpart in silicon was invented by Russell Ohl at Bell Laboratories, 500 V. • BJT. In 1947, W. Shockley, J. Bardeen, and W. Brattain built a germanium point-contact transistor. The BJT was created by W. Shockley from Bell Lab- oratory in 1948 and developed in 1950 for 500 V/20 A. The first commer- cially available silicon devices (grown junction) were manufactured in 1954 by Gordon Teal. • SCR (Thyristor). The SCR or thyristor was proposed by William Shockley in 1950. It was theoretically described in 1954 and 1955 by J.L. Moll from Bell Laboratory but it was not well accepted until GE manufactured a feasible device in 1957. Its commercial version was available in 1958 and was championed by G. E.’s Frank W. “Bill” Gutzwiller (300 V/16 A). • GTO. The GTO thyristor was created in 1962 by R. Aldrich and N. Holonyak from GE. It was used until the 1970s when it was replaced by the silicon power MOSFET and IGBT. This happened because the GTO was limited to low cur- rent. For instance, in 1967 its maximum rates were 500 V/10 A. However, an improved Hitachi GTO was developed in 1981 allowing for higher voltage and current (2500 V/1000 A). • TRIAC. The bidirectional triode thyristor was created by F. W. Gutzwiller, from GE, in 1963. It reached 40 A experimentally but the first commercial Triacs were the SC40 and SC45, rated 200 V, 6 A, and 10 A, in 1965 and 1966, respectively, following basic research steps developed by GE’s Aldrich and Nick Holonyak (1958), and Finis E. Gentry and Tuft (1963). • RCT. The RCT was created in 1970 by Kokosa and B. Tuft from GE.
  • 39. 2.4 BASIC CONVERTERS 25 • MOSFET. The first metal-oxide field-effect transistor was created in 1958 and reported in 1960 by D. Kahng and M.M. Atalla, from Bell Laboratory. How- ever, the first successfully commercialized power MOSFET was from Interna- tional Rectifier. • SITH or FCT (Field-Controlled Thyristor). The SITH was proposed by J. Nishizawa from Mitsubishi Electric Corporation in 1975 (700 V); in the same year a similar device that received the name of FCT was reported by D.E. Houston. • IGBT. The first IGBT with substantial current ratings was developed in 1982 by J. Baliga, from GE, with a symmetric blocking voltage of 600 V for 10 A (6 kVA). It was also reported by J.P. Russel in 1983 under the name of COM- FET, reaching 400 V and 30 A. • SIT (normally “on” or JFET) was introduced by J. Nishizawa in 1975, 300 V, 2 A, with an output power of 5 W at 1 GHz, 36W at 200 kHz and 40 W at 100 MHz. • BCT. The bilateral controlled thyristor was created by ABB in 1998, having voltage and current ratings of 6.5 kV and 1390 A. • IGCT. The IGCT was conceived in 1993 at ABB and reported in 1996 by P.K. Steimer, H. Gruning et al. from ABB for 4.5 kV and 3 kA. It was also reported in 1996 by J. Sakano et al. from Hitachi and was able to block 4 kV. • MTO. The MOS turn-off thyristor was invented in 1995 by D.E. Piccone et al. from Silicon Power Corporation, with rated values of 6000 V and 500 A. 2.4 BASIC CONVERTERS As mentioned earlier, a power electronics converter interfaces a source and a load (or another source). The source can be either of voltage type or current type. Also, the load can be of either voltage type (e.g., a capacitive load) or current type (e.g., an inductive load). The connection between a source and a load should obey the following sequences: (i) voltage (V)–current (I)–voltage (V)–current (I), or (ii) current (I)–voltage (V)–current (I)–voltage (V). Four connections between source and load are then possible, as shown in Fig. 2.14, which establishes the following connections, V –I, I–V, V − V and I–I. Notice that, for the V –V connection as in Fig. 2.14(c), the power converter interfacing load and source are expected Power converter Power converter Power converter Power converter (d) (c) (b) (a) + – + – + – + – Figure 2.14 Four possibilities of connection between source and load.
  • 40. 26 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS to have an inductor element inside that block. The same rationale applies for Fig. 2.14(d). Only sources and loads of different types can be directly connected, that is: (i) a voltage source can be directly connected to a current-type load and (ii) a current source can be directly connected to a voltage-type load. Such a restriction comes from the need to avoid, for example, a parallel connection between two voltage-type elements, and so preventing short-circuit between these two elements. Except for the case of resistive load, the minimal number of switches that allows interconnecting a source and a load is two, which is called basic commutation cell. In fact such a commutation cell can be obtained with two different arrange- ments, as seen in Figs 2.15 (Cell I) and 2.16 (Cell II). Cell I in Fig. 2.15(a), also known as leg when it is arranged as presented in Fig. 2.15(b), can be used to con- nect a voltage source to an inductive load. In Fig. 2.15(c), the source is connected between points M and N while the load is connected to the point A, named as pole. Instead, in Cell II in Fig. 2.16(a), or its leg representation [Fig. 2.16(b)], the cur- rent source connected to point A allows feeding a capacitive load connected between points M and N (voltage-type load), as shown in Fig. 2.16(c). It should be noticed that while one of the switches is conducting, the other one is turned off. Note that the pole (point A) can be connected to either point M or point N, so that it can only assume the potential of those points. For this reason, both cells are said to be two-level cells. S1 S1 S1 S2 S2 S2 A A A N N (a) (b) (c) M M N M Figure 2.15 Basic cell employed to connect voltage source to current-type load. S1 S1 S2 S2 A A N N (a) (b) M M S1 S2 A N (c) M Figure 2.16 Basic cell employed to connect current source to voltage-type load.
  • 41. 2.4 BASIC CONVERTERS 27 (a) (b) (c) (d) C S1 S2 + – S1 S2 + – + – S1 S2 L + – + – Figure 2.17 Principles for building power converters. Figure 2.17 shows how different types of sources and loads can be connected through the basic cells presented in Figs 2.15 and 2.16. As mentioned earlier, sources and loads of the same type can only be connected through an intermediate coupling circuit. For example, to connect a voltage source to a voltage-type load, it is necessary to employ a current-type element (inductor) between the source and load [see Fig. 2.17(c)]. For duality, the voltage-type element is a capacitor that is used to connect both current source and current-type load, as shown in Fig. 2.17(d). The basic cells permit the basic converters used to convert energy from dc-to-dc, dc-to-ac, ac-to-dc, and ac-to-ac (or simply dc–dc, dc–ac, ac–dc, and ac–ac) and also to extend them to more complex structures, in a more systematic way. This will be in fact the approach employed in this book. Depending of the application, it is possible to define two scenarios: (i) one load supplied by one or more sources and (ii) one source supplying one or more loads. Consider first the case in which there is only one load supplied from one or more sources. Each source can be connected to either a switch (corresponding to the point M in Fig. 2.15, for example), as shown in Fig. 2.18(a)–2.18(d), or to the pole (midpoint of the leg, i.e., point A), as shown in Fig. 2.18(e) and 2.18(f). Similarly, for the second scenario, when there is only one source and the load is constituted by one or more elements, each part of the load can be connected to either a switch (point M, for example), as shown in Fig. 2.19(g) or to the midpoint of the leg (A), as shown in Fig. 2.18(h) and 2.18(i). Notice from Figs 2.15–2.18 that the power switches, sources, and loads are represented generically. The procedure to choose first the appropriate power switch and the converter with desirable characteristics depends on the type of source and load that have been considered, as well as the requirements for a specific application.
  • 42. 28 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS (a) (b) (c) (d) (e) (f) (g) (h) (i) Figure 2.18 Different ways to connect source(s) to the load(s). The following technical characteristics are used for choosing the appropriate switch and converter: (i) UniC or BidC, (ii) UniV or BidV, (iii) SC or CC, and (iv) SB or CB. Other essential features are switching frequency, voltage and current ratings, and cost. 2.4.1 dc–dc Conversion Buck Converter The buck converter is presented in Fig. 2.19(a), which comprises (i) a dc voltage source (Vdc), (ii) a basic cell as in Fig. 2.15(a) with switches S1 and S2, (iii) energy storage component (L) due to the interface between two voltage-type elements, and (iv) a resistive load with voltage Vo. As demanded for this application, both switches S1 and S2 should be (a) UniC and UniV and (b) CC and CB. However, notice that S2 must be complementary to S1 to avoid a short circuit of the dc source (Vdc), which means that when S1 is on, S2 should be off, and when S2 is on, S1 should be off.
  • 43. 2.4 BASIC CONVERTERS 29 (a) (b) (c) (d) (e) S2 Vdc + – Vo + – S1 L C Vdc + – Vo + – C off on L iL Vdc νD Toff Ton t Vdc + – Vo + – C off on L iL Vdc + – Vo + – Q L iL C D Figure 2.19 Buck converter with: (a) basic cell and (b) real switches. (c) TS 1. (d) TS 2. (e) Diode voltage. This means that the circuit will have the same functionality if a SC/SB type of switch (i.e., diode) is employed for S2. Then, the circuit will be as shown in Fig. 2.19(b). There are two topological states (TSs) for the buck converter: TS 1—The switch Q is on and conducts the inductor current, while the diode is off, as shown in Fig. 2.19(c). TS 2—When Q is turned off, the diode conducts the inductor current, as shown in Fig. 2.19(d). Example 2.1 Explain why a buck converter such as the one presented in Fig. 2.19 requires two power switches with UniC and UniV characteristics. Solution As the output voltage is dc, the load current is also dc, which leads to a dc current for IL. During the TS 1, the switch Q will carry this unidirectional type of current (UniC) and during the TS 2 the diode will carry IL. When both
  • 44. 30 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS switches are turned off their current will be zero. In terms of the voltage applied to those devices, it is also UniV, as the voltage will be either zero or Vdc for Q and either zero or −Vdc for D. Figure 2.19(e) shows the diode voltage, which is the voltage applied to the LC filter. While the time domain representation—as in Fig. 2.19(e)—provides a good understanding of the topology itself, the frequency domain with the Fourier series allows identification of the frequency components. In general terms, the expansion of a periodical waveform f(t) in Fourier series is given by f(t) = Fo + ∞ ∑ n=1 fn(t) = 1 2 ao + ∞ ∑ n=1 {an cos(n𝜔t) + bn sin(n𝜔t)} (2.1) where Fo = 1∕2(ao) is the average value and an = 1 𝜋 ∫ 2𝜋 0 f(t) cos(n𝜔t)d(𝜔t) for n = 0, … , ∞ (2.2) bn = 1 𝜋 ∫ 2𝜋 0 f(t) sin(n𝜔t)d(𝜔t) for n = 1, … , ∞ (2.3) In the case of Fig. 2.19(e), the average value Fo in (2.1) is given by Vo = TonVdc Ts = dVdc with d = Ton∕Ts (2.4) where Ton is the interval of time with the switch S1 on, Ts is the switching period (Ton + Toff), and d is known as duty cycle. Notice that the input voltage of the LC filter has infinite components of fre- quency [see equation (2.1)], which must be filtered allowing, ideally, an output volt- age Vo with only the zero frequency component, as in equation (2.4). Example 2.2 Assume the inductor voltage waveform and the information that this energy storage component is in fact a passive element to deduce equation (2.4) without the expansion in Fourier series. Solution The graphs below show the inductor waveforms (voltage and current) assum- ing a continuous conduction mode (i.e., iL is always higher than zero). As the inductor is a passive component, the average power on this device is zero, lead- ing to an average voltage also equal to zero. It turns out that:(Vdc − Vo)Ton = VoToff and consequently: Vo∕Vdc = Ton∕T = d.
  • 45. 2.4 BASIC CONVERTERS 31 t t iL ILmax –Vo νL Ton Toff Vdc–Vo ILmin IL Exercise 2.2 By using equations (2.2) and (2.3) calculate the Fourier coefficients an and bn from 0 to the seventh harmonic for two waveforms of the diode voltage with buck converter operating with d = 0.5 and 0.75. Also, consider a switching frequency equal to 50 kHz. If the LC filter in Fig. 2.19 is designed with a cut frequency equal to 20 kHz (3dB), find out if this filter can cut the switching frequency of the buck converter for both cases: d = 0.5 and 0.75? Boost Converter The boost converter with the representation of the real semi- conductor devices is presented in Fig. 2.20(a). Its TSs are given in Fig. 2.20(b) and 2.20(c). TS 1—In this mode, the switch is on and the diode is off. The input voltage is then applied to the inductor with a consequent increase in its current iL. Since D is off, the load current is provided by the capacitor C. TS 2—This mode starts when the switch is turned off and consequently the diode is on. At this moment, the energy stored at the magnetic field of the inductor is released to the capacitor and load. The average output voltage of the boost converter is given by Vo = Vdc (1 − d) (2.5)
  • 46. 32 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS (a) (b) (c) Vdc + – Vo + – C Q L D iL Vdc + – Vo + – C on L off iL Vdc + – Vo + – C on L off iL Figure 2.20 Boost converter and its topological states. The characteristics of the boost converter are the following: 1. Its output average voltage value is greater than the input voltage source. 2. Its input current is continuous with a ripple that depends on the value of the input inductance and switching frequency. 3. The output voltage is positive. Exercise 2.3 A boost converter as in Fig. 2.20 aims to obtain a dc output voltage of 120 V from a voltage source with 24 V. The resistive load is 120 Ω, switching fre- quency is equal to 50 kHz and the converter operates at continuous conduction mode (iL > 0). Determine: (a) duty cycle d, (b) average load current, (c) aver- age source current, and (d) inductor value to guarantee a current ripple less than 5%. Other Basic dc–dc Converters In addition to the buck and boost converters pre- sented previously, there are four other basic nonisolated dc–dc converters that can control the output voltage, as shown in Fig. 2.21. The absolute value of their average output voltage is given by Vo = dVdc (1 − d) (2.6) For all of the topologies in Fig. 2.21, the average of the output voltage can be either smaller or greater than that of the voltage source, depending on the value of d. The main characteristics of the configurations presented in Fig. 2.21 are presented in the sequence.
  • 47. 2.4 BASIC CONVERTERS 33 (a) (b) (c) (d) Vdc + – Vo + – Vdc + – Vo + – Vdc + – Vo + – Vdc + – Vo + – Figure 2.21 Four basic dc–dc converters: (a) buck-boost, (b) cuk, (c) zeta, and (d) SEPIC. (i) Buck-Boost Converter. This converter is shown in Fig. 2.21(a) and can connect a voltage source to a voltage type load. The characteristics of the buck-boost converter are the following: 1. Both input current and the current iD are discontinuous. 2. The output voltage is negative. (ii) Cuk Converter. This converter is shown in Fig. 2.21(b) and can connect a cur- rent source to a current-type load. The characteristics of the Cuk converter are the following: 1. Both input current and output current are continuous. 2. The output voltage is negative. (iii) Zeta Converter. This converter is shown in Fig. 2.21(c) and can connect a volt- age source to a current-type load. The characteristics of the Zeta converter are the following. 1. The input current is discontinuous and the output current is continuous. 2. The output voltage is positive. (iv) Single-Ended Primary-Inductor Converter (SEPIC) Converter. The SEPIC converter is based on the scheme of Fig. 2.21(d) and can connect a current source to a voltage type load. The characteristics of the Zeta converter are the following: 1. The input current is continuous and the current iD is discontinuous; 2. The output voltage is positive. 2.4.2 dc–ac Conversion The circuits that permit a conversion from dc to ac are also known as inverters. They can be voltage-source inverters (VSIs), current-source inverters (CSIs) and impedance-source inverters (ZSIs). The fundamental concepts and main
  • 48. 34 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS νo io +Vdc/2 –Vdc/2 q1 q2 d1 d1 t d2 Vdc 2 R L a + – νo io Vdc 2 q2 q1 d1 d2 0 (a) (b) Figure 2.22 (a) Half-bridge inverter and (b) its output voltage and current waveforms for d = 0.5. characteristics of the VSI and CSI are given in the sequence, while the ZSI is considered in Chapter 8 (Section 8.6.2). Voltage Source Inverter (VSI) The simplest way to generate an ac voltage from a dc source is with the arrangement as in Fig. 2.18(b) with the load connected between the basic cell and two sources. Figure 2.22 shows the same converter with the repre- sentation of real switches. Half-Bridge When the switch q1 is on, the voltage source +Vdc∕2 is applied to the load. The load current then increases exponentially. When q1 is turned off (q2 is on), the current is obliged to decrease via diode d2, and a negative voltage is applied to the load. A similar operation but related to d1 and q1 starts when q2 is turned off. When d = Ton∕Ts = 0.5, a square wave is generated at the inverter output. The output voltage is depicted in Fig. 2.22(b) along with the load current. The expansion in Fourier series of the output voltage is given by 𝑣a0 = 4 𝜋 Vdc 2 [ sin (𝜔t) + 1 3 sin(3𝜔t) + 1 5 sin(5𝜔t) + 1 7 sin(7𝜔t) + … ] (2.7) Equation (2.7) allows calculating the amplitude of the output fundamental volt- age as well as the existing odd harmonics. The sinusoidal variation of the duty cycle d inside the switching interval Ts allows shifting the harmonics to the high frequency region. The order of the most significant ones is around the frequency modulation index, defined as mf = fs fm (2.8) where fs is the frequency of the carrier signal that defines the switching frequency (e.g., triangular waveform) and fm is the frequency of the modulating signal (e.g., sinusoidal signal). This technique is known as sinusoidal pulse-width modulation (SPWM). Its implementation is achieved by comparing a sinusoidal (modulating signal) with a
  • 49. 2.4 BASIC CONVERTERS 35 +Vt νt νa0 0 +Va0 * +Vdc/2 –Vdc/2 +Va0(1) Va0(1) fundamental of νa0 –Va0(1) Va0 * –Vt –Va0 * Figure 2.23 Sinusoidal modulation: reference (top) and pole voltage waveform (bottom). triangle waveform (carrier signal), the frequency of the modulating signal being the fundamental one and the carrier frequency defining the switching frequency. The main waveforms of the SPWM are presented in Fig. 2.23 (top), while Fig. 2.23 (bot- tom) shows the waveforms for the output voltage. The relationship between the amplitude of modulating signal, V∗ a0 , and that of the carrier signal, Vt, defines the amplitude modulation index, ma, that is ma = V∗ a0 Vt (2.9) For the sinusoidal modulation (SPWM), the amplitude of the fundamental volt- age is given by Va0(1) = V∗ a0 Vt Vdc 2 = ma Vdc 2 (2.10) This means that the amplitude of the fundamental is directly proportional to the amplitude modulation index (ma) for a given dc bus value (Vdc). Example 2.3 For a half-bridge inverter as presented in Fig. 2.22(a) supplying a resistive load of 5Ω, switching frequency of 10 kHz and Vdc = 100 V (duty cycle equal to 50%), calculate: (a) the RMS of the output voltage assuming all harmonic frequencies, (b) the RMS of the output voltage at the fundamental frequency, and (c) output power as well as voltage and current processed by each switch.
  • 50. 36 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS Solution (a) By definition, the RMS value of a periodic function f(t) with period T is given by fRMS = √ 1 T ∫ T 0 [f(t)]2dt Applying this equation for the waveform of the voltage presented in Fig. 2.22(b), gives an output RMS voltage equal to VoRMS = 50 V (b) As observed in equation (2.7), the fundamental component of the output voltage is given by𝑣ao1 = 2Vdc∕𝜋(sin(𝜔t)), consequently the RMS value of the fundamental voltage will be given by Vo1RMS = 2Vdc∕𝜋 √ 2 = 45.15 V. (c) The output power is given by Po = V2 oRMS ∕R = 500 W. The blocking volt- age and current processed by each switch is given by 100 V and 20 A, respectively. Exercise 2.4 Repeat the last example with a converter operating with a switching frequency equal to 20 kHz and a RL load with R = 5Ω and L = 15 mH. Full-Bridge The circuit of the single-phase full-bridge inverter is given in Fig. 2.24(a). The output voltage can be written as a function of the pole voltages, as 𝑣ab = 𝑣a0 − 𝑣b0 (2.11) The main waveforms of the converter are shown in Fig. 2.24(b). In this case the pole voltages 𝑣a0 and 𝑣b0 are phase-shifted by180 electrical degrees. As in the half-bridge with duty cycle equal to 50%, the output voltage includes odd harmonics components, that is, third, fifth, seventh, and so on, as d = 0.5. When the pole voltages are phase-shifted of 𝜃 degrees, as shown in Fig. 2.25(a), four of the eight modes of operation are given in Fig. 2.25(b)–2.25(e). In Mode 1, switches q1 and q2 conduct the increasing positive load current (t0 < t < t1), then q2 is turned off forcing q1 to conduct the load current along with d3 in a free-wheeling mode (Mode 2, t1 < t < t2) until q1 is turned off (t2). From this moment on, Mode 3 starts with d3 and d4 conducting together; the load voltage becomes negative and the load current is then forced to zero (t2 < t < t3). The zero crossing determines the beginning of Mode 4, in which the current increases in the negative direction.
  • 51. 2.4 BASIC CONVERTERS 37 io q1 q3 q2 d2 d3 d1 d4 q4 0 νo Vdc 2 R L a b Vdc 2 + – q1 d1 d1 q4 d4 q2 d2 d2 q3 d3 νa0 νb0 νo io +Vdc/2 +Vdc/2 +Vdc –Vdc t t t –Vdc/2 –Vdc/2 (a) (b) Figure 2.24 (a) Single-phase full-bridge inverter. (b) Main waveforms. (b) (c) (a) (d) (e) q1 q1 0 a b R L q3 q2 t0 t1 t2 t3 t4 t5 t6 t q2 d2 d2 d3 d1 d1 θ d4 q4 νo io +Vdc –Vdc νo io + – Vdc 2 q1 q2 Vdc 2 0 a b R L νo io + – Vdc 2 d3 d4 Vdc 2 0 a b R L νo io + – Vdc 2 q1 d3 Vdc 2 0 a b R L νo io + – Vdc 2 q3 q4 Vdc 2 Figure 2.25 Single-phase full-bridge inverter. (a) Gating signals and main waveforms. (b) Mode 1. (c) Mode 2. (d) Mode 3. (e) Mode 4. When q4 is turned off, q3 starts conducting with d1, and so on, until the cycle is completed. The strategy of adding the phase-shift angle 𝜃 modifies the amplitude of the fundamental and harmonics of the load voltage, which is given in equation (2.12)
  • 52. 38 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS 0.1 0 20 40 60 80 100 120 140 160 180 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0 νab(1,n) 4Vdc π νab(3,n) 4Vdc π νab(5,n) 4Vdc π νab(7,n) 4Vdc π Figure 2.26 Behavior of the fundamental and harmonics of the output voltage as a function of 𝛾. as a function of 𝛾 = 𝜋 − 𝜃. Figure 2.26 depicts the behavior of the fundamental and harmonics components of the load voltage as a function of 𝛾. It can be observed that for 𝛾 = 120∘ the amplitude of the third harmonic is zero, although the 5th, 7th, 11th, 13th harmonics are still present. Vo(n) = 4Vdc n𝜋 sin (n𝛾 2 ) (2.12) Another way to reduce the low frequency harmonic components for the out- put voltage is to apply a PWM strategy for the gating signals, as previously done for the half-bridge converter. There are different ways to generate the PWM signals for the full-bridge converter, such as: (i) bipolar modulation—when the sinusoidal references for pole 1 and pole 2 are in phase, (ii) unipolar modulation—when the sinusoidal reference voltages are phase-shifted by 180∘, and (iii) a third possibility is to operate one of the legs with PWM signal while the other one is operated at the fundamental frequency; this corresponds to the unipolar modulation with clamped voltage. Details about the PWM for the full-bridge converter are furnished in Chapters 5 and 8. Three-Phase Inverter A dc–ac three-phase converter is shown in Fig. 2.27. The gating signal generation for the power switches can be obtained as done pre- viously by either changing 𝛾 to eliminate specific harmonics components or with a PWM approach, which will push the harmonics to higher frequencies components. First, assuming the pole voltages with phase-shift equal to 120∘ from each other, the
  • 53. 2.4 BASIC CONVERTERS 39 Vdc Vdc 2 0 Vdc 2 a b c Figure 2.27 Three-phase inverter. line-to-line voltages can be calculated as 𝑣ab = 𝑣a0 − 𝑣b0 𝑣bc = 𝑣b0 − 𝑣c0 (2.13) 𝑣ca = 𝑣c0 − 𝑣a0 As the load is Y-connected, it turns out that 𝑣an = 1 3 (2𝑣a0 − 𝑣b0 − 𝑣c0) 𝑣bn = 1 3 (2𝑣b0 − 𝑣c0 − 𝑣a0) (2.14) 𝑣cn = 1 3 (2𝑣c0 − 𝑣a0 − 𝑣b0) Also, it can be shown that the relationship between the load neutral and the midpoint of the dc bus for a balanced three-phase system is given by 𝑣n0 = 1 3 (𝑣a0 + 𝑣b0 + 𝑣c0) (2.15) The corresponding waveforms for equations (2.13)–(2.15) are shown in Fig. 2.28. As the line-to-line voltage in Fig. 2.28(b) was obtained with 𝛾 = 120∘, then neither third harmonic nor its multiples are measured in these voltages. This is an important characteristic for three-phase systems, as the natural phase angle displace- ment among the phases (120∘) allows elimination of harmonics. It can be seen from Fig. 2.28 that there are six modes of operation. These modes are highlighted in Fig. 2.29(a)–2.29(f). In addition to these six modes of operation, there are two other modes of operation that apply zero voltage to the loads. These are the free-wheeling configurations presented in Fig. 2.29(g) and 2.29(h), where three bottom or upper switches conduct at the same time. Note that for simplifica- tion purposes the operation modes of the three-phase circuit are presented with ideal switch.
  • 54. 40 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS νa0 νab νan νb0 νc0 +Vdc/2 –Vdc/2 +Vdc/2 +2/3Vdc +1/3Vdc –1/3Vdc (c) (b) (a) (d) t t t t t t +1/6Vdc –1/6Vdc –2/3Vdc –Vdc/2 +Vdc/2 +Vdc –Vdc –Vdc/2 Figure 2.28 Waveforms of three-phase inverter. (a) Pole voltages; (b) line-to-line voltage; (c) load phase voltage; and (d) zero-sequence voltage. Another way to eliminate harmonics for the output voltage is to generate a SPWM signal for the gating of the switches, as presented in Fig. 2.30, which shows three reference signals phase-shifted by 120∘ compared to a carrier signal. This figure shows also the pole voltages as a result of the sine-triangular comparison. Example 2.4 Draw the waveforms of the pole voltages (𝑣a0, 𝑣b0, and 𝑣c0), line-to-line volt- age (𝑣ab), and load phase voltage (𝑣an) considering a SPWM strategy applied
  • 55. 2.4 BASIC CONVERTERS 41 to dc–ac three-phase converter with the switching frequency and modulating frequency equal to 10 kHz and 60 Hz, respectively. Also prove that ma → ∞. Solution As the amplitude modulation index (ma) is infinite, from equation (2.9) it means that the amplitude of the modulating signal is infinitely higher than the amplitude of the carrier signal, which leads to a pole voltage and load voltages as presented in Fig. 2.28. (a) (b) (c) (d) (e) (f) (g) (h) Vdc + – Vdc + – Vdc + – Vdc + – Vdc + – Vdc + – Vdc + – Vdc + – Figure 2.29 Modes of operation of the three-phase inverter.
  • 56. 42 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS νt νa0 ∗ νa0 νb0 νc0 νb0 ∗ νc0 ∗ Figure 2.30 Three-phase inverter waveforms with PWM approach. Exercise 2.5 The three-phase inverter in Fig. 2.27 (Vdc = 300 V) is operated with a sinu- soidal PWM approach with a modulation index ma = 0.9. The ratio between the frequency of the carrier and modulating signals (mf ) is high enough to guarantee sinusoidal load currents when the three-phase load is constituted by R = 5 Ω and L = 20 mH (per phase). The frequency of the modulating signal is 50 Hz. (a) What is the RMS value of the voltage 𝑣a0 at the fundamental frequency? (b) What is the RMS value of the voltage 𝑣ab at the fundamental frequency? (c) What is the RMS value of the current in each phase? (d) CSI The three-phase version of the CSI is shown in Fig. 2.31. As the current source is unidirectional, the switches are of UniC type. However, due to the bidirectional load voltage type, the switches must be of BidV type. In fact, the CSI is dual to the VSI. Because of this, the line-to-line output voltage waveform of a VSI is equiva- lent to the line output current waveform of a CSI. Using this knowledge, the CSI can be controlled by the same PWM techniques used to control the VSI. However, practical aspects such as dead-time generation follows different rules for both types of converters.
  • 57. 2.4 BASIC CONVERTERS 43 a b c Figure 2.31 Current source inverter (CSI). 2.4.3 ac–dc Conversion Ac–dc converters are also known as rectifiers. Such converters can be sorted as uncontrolled or controlled rectifiers. An overview about this type of converter is pre- sented here. Uncontrolled Rectifiers Notice that a sinusoidal waveform as those obtained on the utility grid has average voltage equal to zero. Some applications, such as dc motor drive systems, require a waveform with average voltage different from zero. If a resistive load is employed, the simplest way to satisfy the condition of non-null average voltage is to use a power converter able to cut, for instance, the negative part of the sinusoidal waveform, as presented schematically in Fig. 2.32(a). A power switch series connected between the source and load will implement this rectifier circuit with no need to use the basic cells as in Figs 2.15 and 2.16. It is evident that the output voltage and output current are unidirectional, which leads to a device with the following characteristics SC/SB/UniC/UniV-r, that is, diode. There are two TSs defined by the variables of the circuit as there is no gating signal control. The TSs are shown in Fig. 2.32(b). However, for an RL type of load [see Fig. 2.33(a)] the sinusoidal input volt- age obliges the current to become zero somewhere between 𝜔t = 𝜋 and 𝜔t = 3𝜋∕2 (a) (b) νac + – νo + + – – Figure 2.32 Single-phase half-bridge diode rectifier with resistive load: (a) circuit; (b) operation modes.
  • 58. 44 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS (a) (b) νac + – νo i + – Figure 2.33 Single-phase half-bridge diode rectifier with inductive load: (a) circuit; (b) operation modes. (depending of the load power factor), thus turning off the diode. During the diode con- duction after 𝜔t = 𝜋, the negative input voltage is applied to the load. Even dealing with negative voltage, the diode will turn off only when both conditions are satisfied: reverse voltage and zero current [see section “The Conventional Diode”]. In this case, the average of the output voltage will vary with the load power factor, which is some- times an undesirable condition. The output voltage varying with the power factor of the load can be avoided by using a diode in parallel with the load (free-wheeling diode), that, in fact, clamps the negative part of the load voltage at zero, as shown in Fig. 2.34. The arrangement of two diodes as presented in this figure is indeed a particular case of the basic cell shown in Fig. 2.15. In this case, the output voltage will be equal to Vo = Vm 𝜋 (2.16) where Vm is the amplitude of the sinusoidal waveform. Example 2.5 Deduce equation (2.16). Notice from Fig. 2.34 that due to the inductive load, the arrangement of diodes is in fact a basic cell (as in Fig. 2.16) constituted by diodes. While a single-phase full-bridge diode rectifier is presented in Fig. 2.35(a), the three-phase version is presented in Fig. 2.35(b). Both circuits are also one of the cases presented in Fig. 2.18 with higher output dc voltage than the half-bridge, as in Figs 2.32–2.34.
  • 59. 2.4 BASIC CONVERTERS 45 (a) (b) νac + – νo + – Figure 2.34 Single-phase half-bridge diode rectifier with inductive load and free-wheeling diode: (a) circuit; (b) operation modes. (a) (b) Figure 2.35 Diode rectifier: (a) single-phase and (b) three-phase circuits. Controlled Rectifiers The controlled rectifiers can also be either half-bridge or full-bridge topologies. Their control can be obtained either by phase control or by PWM control, depending on the type of switch employed in the circuit. Phase Control Considering a sinusoidal (bidirectional) voltage source feeding a unidirectional inductive load, as shown in Fig. 2.36(a), the type of switch for S1 and S2 can be given respectively by: CC/SB/UniC/BidV (SCR) and SC/SB/UniC/UniV-r (diode), as in Fig. 2.36(b). The SCR is turned on at a given angle 𝛼 in relation to the moment that the SCR voltage becomes positive on its terminals. Unlike the previous rectifiers, the angle control allowed by the gating circuit of the SCR permits varying the output average voltage by changing 𝛼. This technique is known as phase control.
  • 60. 46 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS (a) (b) νac + – νac + – νo + S2 D T S1 – νo + – Figure 2.36 (a) Controlled ac–dc converter using a switching cell. (b) Single-phase rectifier with SCR. The average of the output voltage (Vo𝛼), as a function of both 𝛼 and the ampli- tude of the sinusoidal voltage, is given by Vo𝛼 = Vm 2𝜋 (1 + cos 𝛼) (2.17) It can be seen from equation (2.17) that when 𝛼 = 0∘, the value of the output voltage is the same as in equation (2.16), as the SCR is equivalent to the diode when 𝛼 = 0. Exercise 2.6 Deduce the expression for the average of the output voltage as in equation (2.17) of the controlled rectifier as presented in Fig. 2.36. The single split-phase half-bridge rectifier is shown in Fig. 2.37(a), in which the sinusoidal voltage sources 𝑣ac1 and 𝑣ac2 are phase-shifted 180o to each other, as shown in Fig. 2.37(b). Suppose that the load current is continuous (i.e., always above zero) and that the SCR T1 is turned on at a given angle 𝛼 after 𝑣ac1 becomes positive. This voltage is then applied to the load. From 𝜔t = 𝜋, 𝑣ac1 becomes negative while 𝑣ac2 becomes positive allowing T2 to be turned on when 𝜔t = 𝜋 + 𝛼. Until this time the load current is furnished by 𝑣ac1, as shown in Fig. 2.37(c). From 𝜔t = 𝜋 + 𝛼 on, 𝑣ac2 feeds the load current, as shown in Fig. 2.37(d). Note that when a free-wheeling diode is added as in Fig. 2.38(a), the negative part of the output waveform is clamped to zero as in Fig. 2.38(b) and the output average voltage is calculated from equation (2.17). The three-phase and six-phase half-bridge rectifiers are shown in Figs 2.39 and 2.40, respectively. In the results presented in Figs 2.39(b) and 2.40(b) their output voltages are obtained for 𝛼 = 30∘. The general expression for the average output voltage for a n-phase half-bridge rectifier considering 𝛼 = 0∘ is given by (2.18).
  • 61. 2.4 BASIC CONVERTERS 47 (a) (b) (c) (d) νac + – νac + + + – – – νac + – νo io νo νg2 νg1 νac1,νac2 νac1 νac2 + + – – νac1 νac2 io + – νo + – νo + – T2 T1 T1 T2 Figure 2.37 Single split-phase rectifier: (a) power circuit, (b) waveforms, and (c) and (d) modes of operation. Vo = nVm 𝜋 sin ( 𝜋 n ) (2.18) Examples of the full-bridge rectifiers for single-phase and three-phase circuits are presented in Fig. 2.41(a) and 2.41(b), respectively. The output voltage wave- form of the full-bridge single-phase bridge is similar to that of the single split-phase half-bridge rectifier. The output voltage waveform of the three-phase bridge is similar to that of the six-phase half-bridge. PWM Control A three-phase PWM converter with bidirectional power flow capability, sinusoidal grid current, and power factor control is presented in Fig. 2.42. Each phase can employ the boost principle so that the output voltage is higher than the amplitude of the input voltage. This topology is discussed in detail in Chapter 9.
  • 62. 48 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS (a) (b) νac + – νo νo νac1,νac2 + – T1 D T2 Figure 2.38 Single split-phase rectifier with a free-wheeling diode: (a) power circuit and (b) main waveforms. (a) (b) νo νa νb νc + – νa νb νc – t Figure 2.39 (a) Three-phase half-bridge controlled rectifier and (b) output waveform. (a) (b) νo + – νa νb νc t Figure 2.40 (a) Six-phase half-bridge controlled rectifier and (b) output waveform.
  • 63. 2.4 BASIC CONVERTERS 49 (a) (b) Figure 2.41 Full-bridge controlled: (a) single-phase and (b) three-phase rectifiers. Figure 2.42 Three-phase controlled rectifier. 2.4.4 ac–dc Conversion An example of a simple ac–ac converter is presented in Fig. 2.43(a), where the switch is a TRIAC (or two SRCs in antiparallel), for a resistive load. By varying the switch turn-on angle 𝛼, the RMS value of the fundamental component of the output voltage is varied as well. During the positive semicycle of the input voltage, when turned on, the TRIAC conducts from M1 to M2 and during the negative semicycle of the input voltage, when turned on, it conducts from M2 to M1. The voltages are shown in Fig. 2.43(b). The need for a device of BidV type is confirmed from the waveform of the voltage across the device. The RMS of the output voltage is given by Vo𝛼 = Vm √ 2 √ 1 𝜋 ( 𝜋 − 𝛼 + sin 2𝛼 2 ) (2.19) The circuit shown in Fig. 2.44(a) is a single-phase ac–ac converter, referred to as a cycloconverter. The switches must be of the type CC/SB and BidV/UniC as in this figure. The positive (P) and negative (N) converters are controlled to achieve an output voltage with variable amplitude and a variable frequency, as in Fig. 2.44(b). Another ac–ac converter is the matrix converter, which consists of an array of bidirectional switches that directly connect the load to the source. The three-phase to three-phase conversion is given in Fig. 2.45(a) with ideal switches. The practical realization of the matrix converter is presented in Fig. 2.45(b).
  • 64. 50 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS (a) (b) νo νo νac νac M1 M2 Figure 2.43 Simple ac–ac converter: (a) circuit and (b) phase control. P N (a) (b) N N N N N N P P P P P P Figure 2.44 (a) Single-phase cycloconverter. (b) Waveforms of the circuit: (top) grid voltage and (bottom) load voltage with dashed line. The back-to-back converter is another way to generate a controlled ac voltage from the utility grid voltage. Such a converter is also known as indirect ac–dc–ac conversion, as there is a dc link between both ac stages, as in Fig. 2.46. This converter is described in detail in Chapters 10 and 11. The ac–dc–ac converter can also be implemented with a current source configuration. 2.5 SUMMARY This chapter first classified the static (unidirectional or bidirectional features in terms of current and voltage) and dynamic (spontaneous or controlled turn-on and/or turn-off) characteristics of the ideal power switches. Then a summary of the main
  • 65. 2.5 SUMMARY 51 (a) a b c a b c A B C A B C (b) Figure 2.45 (a) Three-phase switching matrix. (b) Practical implementation of the matrix converter. Figure 2.46 Indirect converter: ac–dc–ac conversion. real power semiconductor devices available in the market was given, taking into account the static and dynamic characteristics. It was outlined their limit values for current, voltage, and switching frequency. The bedrock for the following chapters was given by introducing the concept of basic switching cell, from which it is pos- sible to generate the basic converter topologies used in power electronics. By using these switching cells, a general discussion on the principles of power conversion
  • 66. 52 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS from dc sources (dc–dc and dc–ac conversion) and ac sources (ac–dc and ac–ac) is furnished. Also the principle of operation of the main converter topologies is explained. It is expected from this chapter to provide the reader a systematic way of deciding which type of power semiconductor is the most appropriate choice for a given application based on: (i) the static and dynamic characteristic, (ii) voltage and current ratings, and (iii) on the frequency of operation. In addition to the generation of conventional power electronics topologies, the concept of cell can be applied to conceive other topologies used by researchers and by related industry. These other topologies, named in this book as advanced power electronics converters, are introduced in the following chapters. Details on the topics can be found from References 1 to 77. As will be presented from Chapter 3 onwards, this text will focus on advanced power electronics converters that process AC voltage by using PWM strategies as the gating signal control of the power switches. REFERENCES [1] Gutzwiller FW. Silicon-Controlled Rectifier Manual. 5th ed. Auburn, NY: General Electric Co.; 1972. [2] Burns WB III, Kociecki J. Power electronics in the minicomputer industry. Proc IEEE 1988;76(4):311–324. [3] Hower PL. Power semiconductor devices: an overview. Proc IEEE 1988;76(4):335–342. [4] Baliga BJ. Evolution of MOS-bipolar power semiconductor technology. Proc IEEE 1988;76(4): 409–418. [5] Chen DY. Power semiconductors: fast, tough, and compact. IEEE Spect 1987;24. [6] Thomson-C.S.F. Le transistor de puissance dans son environement. Paris: Thomson-CSF-DSD, 1978. [7] Ferrieux JP, Forest F, Lienart P. The insulated gate bipolar transistor: switching modes. Proceedings of European Power Electronics Conference; 1969. p 171–175. [8] Heumann K, Papp G, Jung M. Comparative study on new power transistors with respect to high frequency inverter applications. Ibid; 1989. p 99–104. [9] Muraoka K, Kawamura Y, Ohtsubo Y, Sugawara S, Tamamushi T, Nishizawa J. Characteristics of the high-speed SI thyristor and its application to the 70-kHz 100-kW high efficiency inverter. IEEE Trans Power Electron 1989;4(1):92–100. [10] Akagi H, Sawae T, Nabae A. 130 kHz 7.5 kW current source inverters using static induction transis- tors for induction heating applications. IEEE Trans Power Electron 1988;3(3):303–309. [11] Escaud B, Marty P. Introduction à l’étude des structures des convertisseurs statiques. Electron Ind 1983;56:65–71. [12] Marty P, Escaud B, La commutation dans les convertisseurs statiques, Ibid., No. 60; 1983. p 69–73. [13] McMurray W. Power electronic circuit topology. Proc IEEE 1988;76(4):428–437. [14] Cheron Y. Analyse des contraintes subies par les interrupteurs pendant les commutations. Recherche des regles de leur utilisation optimale dans les convertisseurs. Proceedings de la Journée d’Etude S.E.E./GRECO; Toulouse; 1987. [15] Liu K, Lee F. Topological constraints on basic PWM converters; IEEE PESC’88 Record; 1988. p 164–172. [16] Wood P. Switching Power Converters. Malabar, Fl.: Robert E. Krieger Publishing Co.; 1984. [17] Mohan N, Undeland TM, Robbins WP. Power Electronics: Converters, Applications, and Design. New York: John Wiley and Sons; 1989. [18] Ledwich G. Current source inverter modulation. IEEE Trans Power Electron 2001;6(4):618–623. [19] Hsin-Hua PL Bidirectional lateral insulated gate bipolar transistor having increased voltage blocking capability US patent 5977569 A. 1999 Nov 02. [20] Dahono P, Kataoka T, Sato Y, Dual relationships between voltage-source and current-source three-phase inverters and its applications. Proceedings of PEDS; 1997. p 559–565.
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  • 68. 54 CHAPTER 2 POWER SWITCHES AND OVERVIEW OF BASIC POWER CONVERTERS [46] Lorenz L. Power semiconductor devices and smart power IC’s - the enabling technology for future high efficient power conversion systems. Proceedings of IPEMC; 2009. p 193–201. [47] Shigekane H, Fujihira T, Sasagawa K et al. Macro-trend and a future expectation of innovations in power electronics and power devices. Proceedings of IPEMC; 2009. p 35–39. [48] Klaka S, Frecker M, Grüning H. The Integrated Gate-Commutated Thyristor: A New High-Efficiency, High-Power Switch for Series or Snubberless Operation. Nürnberg: PCIM; 1997. [49] Arsov GL, Slobodan M. The sixth decade of the thyristor. Electronics 2010;14(1):3–7. [50] Riordan M, Hoddeson L. The origins of the p-n junction. IEEE Spect 1997;34(6):46. [51] Baliga BJ. How the super-transistor works. Scientific American Magazine, Special Issue on “The Solid State Century”, pp. 34–41, 1998. [52] Bedford BD, Hoft RG. “Principles of Inverter Circuits”. New York: John Wiley; 1964. [53] Gentry FE, Gutzwiller FW, Holonyak N, Von Zastrow EE. Semiconductor Controlled Rectifiers. Englewood Cliffs: Prentice Hall; 1964. [54] Łukasiak L, Jakubowski A. History of semiconductors. J Telecommun Inf Technol 2010;1:3–9. [55] Baliga J. Fundamentals of Power Electronics Devices. Springer Science; 2008. [56] Moll JL, Tanenbaum M, Goldey JM, Holonyak , N Jr.. p-n-p-n transistor switches. Proceedings of IRE; 1956; vol. 44. p 1174–1182. New way to change ac to dc, Business Work; 1957 Dec 28. p :114–:116. [57] Nishizawa J, Terasaki T, Shibata J. Field effect transistor versus analog transistor (static induction transistor). Res. Inst. Electrical Comm., Tohoku University, Tech. Rep. RIEC TR-36; 1973; also IEEE Trans Electron Devices 1975; ED-22(4):185–197. [58] Houston DE, Khrishna S, Piccone D, Finke RJ, Sun YS. Field controlled thyristor (FCT)—a new electronic component. IEDM Tech Digest 1975:379–382. [59] Burgess MPD. Semiconductor Research and Development at General Electric. US Semiconductor Manufactures; 2008 and 2011. [60] Kahng D, Atalla MM, DRC, Pittsburg (1960); US patent 3,102, 230. 1963. [61] Russell JP et al. The COMFET: a new high conductance MOS gated device. IEEE ED Lett 1983;EDL 4(3):63–65. [62] Temple VAK. MOS GTO—a new class of power devices. IEEE Trans Elect Devices 1986;33:1609–1618. [63] Stoisiek M, Strack H. Turn-off thyristor with MOS-controlled emitter shorts. IEEE IEDM Tech Digest 1885:158–161. [64] US patent 3,239,728. Semiconductor switch, Richard W. Aldrich and Nick Holonyak, assignors to General Electric Company, Filed July 17, 1962, Date of Patent: 1965 Nov 5. [65] US patent 3,303,360. Semiconductor switch. Finis E. Gentry, assignor to General Electric Company Original application. 1963 Sept 3, Ser. No. 306,147, now Patent no. 3,265,909. [66] (Insulated Gated Controlled Semiconductor) United States Patent 4,551,643 Power switching cir- cuitry. Inventors: John P. Russell, Pennmgton; Alvin M. Goodman, Filed 10/1983, Date of Patent: 1985 Nov 5. [67] Thomas KM, Backlund B, Toker O, Thorvaldsson B. The Bidirectional Control Thyristor. ABB; 1999. [68] Application Note 5SYA 2006-03, Bi-directionally controlled thyristors ABB, 2013. Storm, F. Herbert, Introduction to turn-off silicon-controlled rectifiers. [69] Baliga BJ, Adler MS, Love RP, Gray PV, Zommer ND. The insulated gate transistor: A new three-terminal MOS-controlled bipolar power device. IEEE Trans Electron Devices 1984;31(6):821–828. [70] Adler MS, Owyang KW, Jayant Baliga B, Kokosa RA. The evolution of power device technology. IEEE Trans Electron Devices 1984;11:1570–1591. [71] Kokosa RA, Tuft BR. A high-voltage, high-temperature reverse conducting thyristor. IEEE Trans Electron Devices 1970;17(9):667–672. [72] Shockley W. The theory of p-n junctions in semiconductor; and p-n junction transistors. Bell Syst Tech J 1949;28:435–489. [73] Teal GK. Some recent developments in silicon and germanium materials and devices. National IRE Conference; 1954.
  • 69. REFERENCES 55 [74] Piccone DE, De Doncker RW, Barrow JA, Tobin WH. The MTO thyristor—a new high power bipolar MOS thyristor. IEEE Industry Applications Society 31 Annual Meeting; 1996 Oct 6–10. p 1472–1473. [75] Gruning H, Odegbrd B, Rees J. High-power hard-driven GTO module for 4.5kV/3kA snubberless operation; 1996. . PCIM 96. [76] Jakubowski A, Lukasiak L. CMOS evolution. Development limits. Mater Sci-Pol 2008;26(1):5–20.
  • 70. CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING ac VOLTAGE AND POWER BLOCKS GEOMETRY 3.1 INTRODUCTION This chapter provides a brief review of the main power electronics converters that pro- cess ac voltage and an introduction to power blocks geometry (PBG), to understand the power converters described later in this book. In fact, this chapter has a compi- lation of the topologies studied throughout this book. The fundamentals of PBG and its correlation to the development of power electronics converters are presented in a general way; details regarding each converter are presented in the following chapters. This approach is called geometry because it deals with interconnection of geometric shapes following specifics axioms and conjectures. The main goal of the PBG is to provide an alternative and systematic approach for the presentation of the power converters used to process ac voltage. This strategy employs formal methods based on a simple geometrical representation with estab- lished rules. A universe with axioms and conjectures is defined in order to establish a formation law. Through this method, which is called PBG, power electronics con- figurations observed in the technical literature, especially the traditional ones, can be obtained by following the proposed rules with a high level of abstraction. The PBG method is a general approach that can be employed for the creation and develop- ment of dc–ac and ac–dc–ac converters from two levels to n levels. It is demon- strated that different types of converters processing ac voltage can be easily built by using PBG. The converters studied in this book have at least one stage that synthesizes ac voltage (𝑣o), as observed in Fig. 3.1(a). This kind of converter should be able to create ac waveforms from a dc voltage, with at least two levels, as in Fig. 3.1(b). Figure 3.1(c) shows a pulse width modulation (PWM) waveform for the output con- verter, also with two levels, but with reduced harmonic distortion compared to that in Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 56
  • 71. 3.1 INTRODUCTION 57 (a) (b) Pulsed- voltage source PWM PBG LEG Model Table of Variables (d) (c) t t Converter processing ac voltage νo νo νo Figure 3.1 (a) Power converter able to synthesize ac voltage. (b) ac Output voltage with two levels. (c) PWM ac output voltage with two levels. (d) Approach employed to determine the pulsed voltage source. Fig. 3.1(b). The focus of this book is topologies dealing with PWM voltages with two or more levels obtained from a dc stage. Indeed, the block in Fig. 3.1(a) that processes a PWM ac voltage can also be referred to as a pulsed voltage source. Figure 3.1(d), in turn, shows the approach employed throughout this book to obtain the pulsed voltage sources systematically. First, the PBG is considered to define what a single leg looks like (LEG in Fig. 3.1(d) – circuit constituted by a set of switches able to generate a waveform with two or more levels). Then the table of variables will be employed to define both the model of the converter and the PWM strategy. Such a leg can be defined from the PBG, considering different figures of merit, for example, number of levels, quantity of semiconductors and passive elements desired. This chapter is organized as follows: Section 3.2 introduces the concept of PBG with the concepts, axioms, and postulates defining a systematic way to present power electronics converters; Section 3.3 describes each power block (PB) used in the PBG; Sections 3.4 and 3.5 describe the application of the PBG for multilevel and
  • 72. 58 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING back-to-back configurations, respectively. Finally, Section 3.6 summarizes the entire chapter. 3.2 PRINCIPLES OF POWER BLOCKS GEOMETRY (PBG) By definition, engineering is the application of science to practical uses, and one of the most important approaches employed in engineering is the act of abstracting, that is, simplifying a complex system in a simple statement or simple equation. An example of abstraction is in analog and digital electronics where OpAmp and Inverter Logic symbols are considered abstract elements that describe the behavior of electrical variables. There is a high level of abstraction from the physical elements to the symbols. Such a level of abstraction is crucial to the development of important devices such as computers and satellites, as the designer can focus on the functionality of each element (high level consideration) instead of, for instance, either the interactions of atoms or operation of internal transistors (low level consideration). Also, the presentation of power electronics converters can involve some level of abstraction, with the power switches (e.g., insulated-gate-bipolar transistor (IGBT) and metal oxide semiconductor field-effect-transistors (MOSFETs)) being consid- ered as a simple and ideal (loss-free) two-state switch, on (1) or off (0). In this sense, the goal of the PBG is to bring a higher level of abstraction to the concept of convert- ers by furnishing a set of concepts, axioms, and postulates, as presented in the rest of this chapter. Propositions, as considered in general statements of geometry relationships, are basically divided into two types: (i) those assumed to be true, and (ii) those proven to be true. The former are called (in Euclid’s terminology) axioms if they deal with quantities and postulates if they deal with geometrical figures, while the latter are called theorems. In this way, to axiomatize a particular system is to show that its influences can be defined by a short set of sentences. Hence, it is possible to use some concepts, axioms, and postulates to define a formation law for many power electronics converters that process ac voltage as follows. Concepts Concept 1. PB is a basic unit of the power electronics configurations. There are six different PBs, which are able to represent a large number of topologies by just changing their arrangement. Concept 2. Shape is either a slot or tooth with triangular or square geome- try. Each block is constituted by either three or four shapes. Triangular and square shapes are used to represent specific types of variables, that is, dc or ac. On the other hand, slot and tooth are employed in the PBG to bring up the intuitive aspect of mechanical connection among blocks. Concept 3. PB–dc (PB which processes dc variables) is a PB with at least one triangular shape. If a PB presents one or more triangular shapes, it is considered a unit that processes dc voltage.
  • 73. 3.2 PRINCIPLES OF POWER BLOCKS GEOMETRY (PBG) 59 Concept 4. PB–ac (PB which processes ac variables) is a PB without any tri- angular shape. If a PB presents only square shapes, it is considered a unit that processes ac voltage. Axioms Axiom 1. Every PB is constituted of at least three shapes. Axiom 2. Every mechanical connection between PBs is an electrical connection. Axiom 3. A dashed line denotes ac variable and a solid line denotes dc variable. Postulates Postulate 1. A triangular shape connects only with another triangular shape. Postulate 2. A square shape connects only with another square shape. Postulate 3. The triangular shape is associated with dc variables. Postulate 4. The square shapes could be associated with either dc or ac variables. Regarding these concepts, the axioms and postulates described above, it is pos- sible to construct a large number of configurations proposed in the technical literature that process ac voltage. Normally, power switches are considered the basic elements or cells for construction of power electronics converters. Figure 3.2 shows different topologies conceived for different applications, but with the same number of controlled power switches (i.e., four power switches). While Fig. 3.2(a) depicts an H-bridge configuration, Fig. 3.2(b) and 3.2(c) show a leg for the three-level NPC and flying capacitor topologies, respectively; finally Fig. 3.2(d) shows an ac–dc–ac single-phase half-bridge (at both sides) configura- tion. It is worth mentioning that the configurations in Fig. 3.2 also process ac voltage (a) (b) (c) (d) Figure 3.2 Configurations employing four controlled switches: (a) H-bridge, (b) three-level NPC, (c) three-level flying capacitor, and (d) ac–dc–ac single-phase half-bridge.
  • 74. 60 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING (a) (b) (c) (d) (e) Figure 3.3 Configurations employing six controlled switches: (a) three-phase inverter, (b) four-level NPC, (c) four-level flying capacitor, (d) ac–dc–ac single-phase shared leg, and (e) nested configuration. through a dc stage and have the same number of switches. The conventional way to present power converters with the switches as basic cells assumes the configurations in Fig. 3.2 as distinct categories. As a consequence, students are unable to under- stand how those configurations were created. A similar situation can be observed in Fig. 3.3. Also, in this figure, an isolated presentation hides the understanding of creation of the topologies. In this case the configurations have six controlled power switches and Fig. 3.3(e) shows a different type of topology (as compared to those presented in Fig. 3.2) named nested converter. To overcome such a difficulty, the conception of topologies by using the prin- ciples of the PBG brings up a systematic presentation with a simple and familiar concept of connecting blocks. Such an approach guarantees a formal outline needed for a generalized and didactic presentation. It is worth emphasizing that with PBG it is possible to create a large number of topologies from two- to n-level, just following simple rules. The PBs used in the PBG is shown in Fig. 3.4. Figure 3.4(a) and 3.4(b) shows three PB-dc and three PB-ac, respectively. See Concepts 3 and 4. Each PB constitutes a set of power switches, which guarantees specific char- acteristics for the blocks. Figure 3.5 shows what is obtained inside each PB. Dur- ing the process of creation of the configurations the PBs are considered in their
  • 75. 3.2 PRINCIPLES OF POWER BLOCKS GEOMETRY (PBG) 61 (a) (b) Figure 3.4 Basic units (power blocks – PB) used in the power blocks geometry (PBG): (a) PB-dc and (b) PB-ac. (a) (b) (c) (d) (e) (f) Figure 3.5 Basic units (power blocks – PBs) used in the power blocks geometry (PBG): (a) first PB-dc, (b) second PB-dc, (c) third PB-dc, (d) first PB-ac, (e) second PB-ac, and (f) third PB-ac.
  • 76. 62 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING (a) (b) (c) (d) Figure 3.6 Configurations in Fig. 3.2 obtained from the PBs. higher level (i.e., with strong abstraction from the details inside the blocks). The connections among the PBs, considering the postulates mentioned previously, will be employed for construction of the classical and nonconventional configurations, as considered in the next sections. In fact, the topologies showed in Figs 3.2 and 3.3 are obtained from the PBs following the rules presented in Section 3.2, as observed in Fig. 3.6. 3.3 DESCRIPTION OF POWER BLOCKS The first PB-dc [see Fig. 3.5(a)] is constituted only by diodes, which means that there is no generation of gating signals. On the other hand, there is at least one controlled power switch inside all other PBs, which requires some understanding. Figure 3.7 shows the variables associated with the second PB-dc, as well as the table with their related variables, called Table of Variables. In this table, q is the state of the controlled switch (q = 1 means closed switch, while q = 0 means open switch), 𝑣o, Vp, and Vn are the output voltage,
  • 77. 3.3 DESCRIPTION OF POWER BLOCKS 63 q q Vp Vp Vn Vn νo io νo νo io (a) (b) row q 1 1 2 1 3 0 4 0 > 0 < 0 > 0 < 0 Vp Vp Vp Vn Figure 3.7 Variables associated with the second PB-dc and Table of Variables. positive terminal of the input voltage, and negative terminal of the input voltage, respectively. In principle, considering Postulate 4, it is possible to generate an ac output voltage, since a square tooth is observed at the output of this block. Since the desir- able scenario indicates that the output voltage could be defined by the switching state independent of the load current, there is no full control associated with the first PB-dc. Hence, taking into account the possibilities shown in the Table of Variables (see Fig. 3.7), some restrictions related to the controllability of the output voltage (𝑣o) are observed. When the output current is negative (rows 2 and 4) the output voltage is always Vp, independent of q, which means that there is no control of the output voltage in this case (i.e., io < 0). Then, considering the PB-dc operating alone, as depicted in Fig. 3.7, the full controlled cell is obtained only when io > 0. Equation (3.1) describes the behavior of the output voltage for the second PB-dc when io > 0. 𝑣o = qVp + (1 − q)Vn (3.1) A similar restriction is observed in the third PB-dc, when io > 0, which means that the full controlled output voltage is obtained when io < 0, as observed in Fig. 3.8. In this case it turns out that 𝑣o = qVn + (1 − q)Vp (3.2) Although such current restriction observed in Figs 3.7 and 3.8 can prohibit the application of those blocks to process ac voltage, their associations will guarantee the use of these blocks to generate multilevel circuits able to process ac voltage.
  • 78. 64 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING q q Vp Vp Vn Vn νo io νo νo io (a) (b) row q 1 1 2 1 3 0 4 0 > 0 < 0 > 0 < 0 Vn Vn Vp Vn Figure 3.8 Variables associated with the third PB-dc and Table of Variables. q q q Vp Vp Vn Vn νo io νo νo io (a) (b) row q 1 1 2 1 3 0 4 0 > 0 < 0 > 0 < 0 Vp Vp Vn Vn Figure 3.9 Variables associated with the first PB-ac and Table of Variables. On the other hand, the current restriction does not appear in the PBs that process ac voltage (PB-ac). Figure 3.9 shows the variables associated with the first PB-ac, as well as its Table of Variables. Since there are two controlled switches, there is no restriction in terms of the controllability of the output voltage, even in the case of
  • 79. 3.3 DESCRIPTION OF POWER BLOCKS 65 q2 q1 q1 q1 q2 Vp Vp Vn Vn νo io νo νo io (a) (b) row q1 1 0 2 0 3 0 4 5 6 7 8 0 1 1 1 1 q2 0 0 0 0 0 0 1 1 0 0 1 1 > 0 > 0 > 0 > 0 < 0 < 0 < 0 < 0 Vn – Vp Vn – Vp Vp – Vn Vp – Vn q2 Figure 3.10 Variables associated with the first PB-ac and Table of Variables. positive and negative currents. In this case, equation (3.1) is valid for any value of io, and q is complementary to q (i.e., q = 1 − q) to avoid a short-circuit between Vp and Vn. The second PB-ac [see Fig. 3.5(e)] is in fact a particular case of the first instance with the ability to control positive and negative currents due to the antiseries connection of the switches. The third PB-ac [see Fig. 3.5(f)] has four controlled switches q1 and q2 and their complementary switches q1 and q2. Like the first PB-ac, the output voltage is a function of only the state of switches (q1 and q2). But unlike the case in Fig. 3.9, Fig. 3.10 shows that the output voltage has three different values, or three levels (Vn − Vp, 0, Vp − Vn), and in this case the output voltage is given by 𝑣o = (q1 − q2)Vp + (q2 − q1)Vn (3.3) The process of building power electronics converters processing ac voltage by using the PBG does not take into account the switching states, just the geom- etry of the blocks and the connections among them, which make possible the process of topologies creation. The Table of Variables presented in Figs 3.7–3.10 and equations (3.1)–(3.3) will be employed for the generation of the PWM waveforms, discussed in the following chapters. The next section of this chapter will deal only with the creation of the configurations by using the axioms and postulates.
  • 80. 66 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING Example 3.1 Assume a dc motor drive system requires a converter with controlled voltage at the output converter side and demanding positive currents only. (a) Choose one of the PBs with minimum components able to deal with these requirements. (b) If the motor average current is given by Io = 50A and the dc-link voltage is given by Vpn = 200V (with Vpn = Vp − Vn) specify the switches employed in this converter in terms of voltage and current values. Solution (a) Since the output has a positive dc current and there is a need for a controlled output voltage, the PB with fewer components will be the first PB-dc [i.e., configuration constituted by a controlled switch q and a diode – see Fig. 3.7(a)]. (b) Considering the operation of this PB: (1) when q = 1 the output current (Io) will be going through the controlled switch, the diode current will be zero, the controlled switch voltage will be zero and the reserve diode voltage will be Vpn; (2) when q = 0 the output current (Io) will be going through the diode, the controlled switch current will be zero, the controlled switch voltage will be Vpn and the diode voltage will be zero. The specification of the voltage and current for both devices (controlled switch and diode) are 200 V and 50 A. Example 3.2 A battery formation apparatus is constituted by circuits that aim to generate a specific voltage waveform in order to guarantee the charge and discharge pro- cess until the battery is considered formed. Sometimes the discharge process is obtained by burning the stored energy with resistors (i.e., inefficient process). To overcome this problem, it is possible to employ power electronics solutions to charge and discharge the battery by sending energy back to the primary source of energy with higher efficiency, as observed below. Choose one of the PBs with minimum components that can deal with these requirements. Primary source of energy Power electronics converter Vp IBat IBat VBat Battery under formation Vpn Vo + – + – Vn
  • 81. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 67 Solution The power electronics converter for this particular application must generate controlled output voltage either for positive or negative current, which means that both PB-ac (half-bridge or H-bridge configurations) could be used. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS Multilevel converters were first conceived for high voltage and high power appli- cations, beginning with the neutral-point-clamped (NPC) inverter. Since that time, many configurations have been proposed to establish the highly desirable character- istics for high power applications such as low blocking voltage by switching devices and reduced waveform distortion. The number of levels can be increased as far as necessary, limited by both the complexity of the control and the price of the con- verter itself, due to the increased number of semiconductor devices. To figure out the advantages of waveforms with increased number of levels, Fig. 3.11 shows the total harmonic distortion (THD) versus modulation index (or amplitude-modulation ratio) for two-, three-, and four-level waveforms. As defined in the previous chapter, Two-level Three-level Four-level 1.0 0.9 0.8 0.7 m (modulation index) 0.6 0.5 0.4 0.3 0.2 THD (total harmonic distortion) Figure 3.11 THD versus modulation index for voltages with two, three, and four levels.
  • 82. 68 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING (a) (b) (c) Figure 3.12 Output converter voltage with two-, three-, and four-level. the modulation index (ma) is a relationship between the amplitude of the sinusoidal waveform (also called modulating or control voltage – Vm) and triangular waveform (also called carrier voltage – Vt), that is, ma = Vm∕Vt. It can be seen from Fig. 3.11 that the increase in the number of levels results in THD reduction for a given value of ma. Figure 3.12 depicts the waveforms produced by converters with two-, three- and four-levels, respectively. From this figure it is easy to understand the behavior shown in Fig. 3.11 with better THD for a higher number of levels – notice that the waveforms in Fig. 3.12 become closer to a sinusoidal voltage. The most employed multilevel configurations, with industry interest, are diode-clamped (or NPC), cascade, and flying capacitor multilevel inverters. Those multilevel configurations will be considered throughout this book as the conven- tional ones, while different multilevel topologies presented in the technical literature will be treated as nonconventional solutions. The nonconventional converters are important in power electronics basically because they may provide an alternative solution to improve a specific aspect of the conversion system. Furthermore, such nontraditional power electronics converters play an important role in teaching students due to the extra effort required in modeling and dealing with specific requirements. 3.4.1 Neutral-Point-Clamped Configuration Considering the PBG, the constructions of the NPC configurations can be presented in a systematic way, as described briefly in this subsection. Chapter 4, however, will provide details of this configuration. With two PBs-dc cells [see Fig. 3.5(b) and 3.5(c)] and the first PB-ac cell [see Fig. 3.5(d)], and connecting them following the Postulates 1 and 2 presented previously, it is possible to generate the three-level NPC configu- ration, as observed in Fig. 3.13(a). This is a three-level converter because the blocks (and consequently the switches) are connected in such a way that one of the three inputs can be selected to appear at the output converter side. Other levels can be obtained following the same strategy, that is, connecting a triangular slot (or tooth) with a triangular tooth (or slot) (i.e., following Postulate 1); and connecting a square slot (or tooth) to a square tooth (or slot) (i.e., following Postulate 2).
  • 83. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 69 (a) (b) (c) 1 2 3 1 2 3 4 5 1 2 6 7 3 4 5 Figure 3.13 Construction of NPC multilevel legs using PBs: (a) three-levels, (b) four-levels, and (c) five-levels. From the four-level NPC configuration onward there are always two or more possibilities of connections among the triangle slots and teeth. For instance, consid- ering the configuration in Fig. 3.13(b), the triangle slot of PB 1 is connected to the triangle tooth of PB 4, while the slot of PB 3 is connected to the tooth of PB 2. There are other ways to connect the blocks differently from that shown in Fig. 3.13. These different ways and the PWM approach are considered in Chapter 4.
  • 84. 70 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING Example 3.3 Write the Table of Variables for the three-level NPC configuration; see Fig. 3.13(a). Prove that the switching devices can be represented by a binary variable, with qj = 1 used when the switch is on and qj = 0 when the switch is off (with j = 1, 2, 3, and 4), as highlighted below. Vn Vp q1 = {0,1} q2 = {0,1} νo q3 = {0,1} q4 = {0,1} Solution Since there are four switches with two states each, there are sixteen (22 = 16) possibilities for the total switching states, as shown below: row q1 q2 q3 q4 𝑣o 1 0 0 0 0 Undefined 2 0 0 0 1 Undefined 3 0 0 1 0 Undefined 4 0 0 1 1 Vn 5 0 1 0 0 Undefined 6 0 1 0 1 Undefined 7 0 1 1 0 0 8 0 1 1 1 Short-circuit 9 1 0 0 0 Undefined 10 1 0 0 1 Undefined 11 1 0 1 0 Undefined 12 1 0 1 1 0 13 1 1 0 0 Vp 14 1 1 0 1 Vp 15 1 1 1 0 Short-circuit 16 1 1 1 1 Short-circuit
  • 85. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 71 Notice that many of the states obtained in this Table are prohibited since they are either undefined or short-circuit, and so must be avoided. In this context, undefined means that the output voltage is not defined exclusively by the switching states. Without taking into account the prohibited states, this converter can generate three different voltages at its output (i.e., Vn, 0, Vp) for either positive or negative currents. Example 3.4 Many of the switching states in Example 3.3 cannot be applied since they are prohibited states. Since there are only three inputs and those inputs should be selected to appear at the output converter side (𝑣o), determine: (a) the mini- mum number of independent switching states to select any input voltage at the output converter side (b) how those switching states can be associated with the converter in Fig. 3.13(a) with four switches to generate a three-level output voltage. Solution (a) As there are three inputs and the requirement is to use the switching states to select each of these inputs at the output, the minimum number of inde- pendent switching states is 2, since 22 = 4. (b) As observed in Fig. 3.13(a), the three-level NPC topology requires four switches to guarantee an output with three levels. On the other hand, with two independent switching states (as concluded previously) it is possible to select three inputs available (Vn, 0, Vp), defining the complementary switch- ing states as q1 and q2, where q1 = 1 − q1 and q2 = 1 − q2. Below is pre- sented the three-level NPC topology, using only two independent switches, as well as its Table of Variables. The converter as presented below is able to select any input by using two independent switches. Vp Vn q1 q2 νo q2 q1
  • 86. 72 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING State q1 q2 𝑣o 1 0 0 Vn 2 0 1 0 3 1 0 Undefined 4 1 1 Vp 3.4.2 Cascade Configuration As the number of levels increases, the practical control limits observed in the NPC multilevel converter restrict its use, due to capacitor voltage control issues. Such oper- ation limits are presented in Chapter 4. Another topology that deals with generation of multilevel voltages without dramatically increasing the control complexity is the cascade configuration, since it normally uses isolated dc sources. A high power motor drive system with high level reliability is one of the applications where this kind of converter is popular. The construction of the cascade multilevel configurations are observed in Fig. 3.14, with the direct use of the third PB-ac (see Fig. 3.5) following Postulate 2 with the connection of the teeth in a series arrangement. Dashed lines at the output of these converters mean that they will deal with ac variables, while solid lines at the input side of the converter mean dc variables. Details of the cascade configuration are furnished in Chapter 5. Example 3.5 For the converter presented below [as in Fig. 3.14(a)], write the Table of Vari- ables for the case in which the dc-link voltage of the converters are given by Vdc1 = Vdc and Vdc2 = 2Vdc and then determine how many levels will be gen- erated at the output converter side with qj = 1 − qj and j = 1, 2, 3, 4. Vdc1 Vdc2 q1 q2 q3 q4 νo q1 q2 q3 q4
  • 87. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 73 (a) (b) Figure 3.14 Construction of cascade multilevel legs using PBs with: (a) two power blocks and (b) three power blocks.
  • 88. 74 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING Solution The Table of Variables for this converter is presented below. The output voltage will have seven levels given by 0, ±Vdc, ±2Vdc and ±3Vdc. row q1 q2 q3 q4 𝑣o 1 0 0 0 0 0 2 0 0 0 1 2Vdc 3 0 0 1 0 −2Vdc 4 0 0 1 1 0 5 0 1 0 0 Vdc 6 0 1 0 1 3Vdc 7 0 1 1 0 −Vdc 8 0 1 1 1 Vdc 9 1 0 0 0 −Vdc 10 1 0 0 1 Vdc 11 1 0 1 0 −3Vdc 12 1 0 1 1 −Vdc 13 1 1 0 0 0 14 1 1 0 1 2Vdc 15 1 1 1 0 −2Vdc 16 1 1 1 1 0 Example 3.6 Considering two cells of the first PB-ac, as presented in Fig. 3.5(d) and Pos- tulates 2 and 4, draw a different configuration from the ones presented so far with three inputs and one output and write the possible output voltages. Solution The postulates applied for two cells of the first PB-ac as presented in Fig. 3.5(d) allow a possible solution as depicted below. V1 V2 V3 νo After the process of defining the topology, it is possible to write the out- put voltages, taking into account the switches inside each block, as shown below.
  • 89. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 75 V1 V2 V3 q1 q2 q3 νo q4 Here, the output voltages are given respectively by • 𝑣o = V1 when q1 = q3 = 1 and q2 = q4 = 0 • 𝑣o = V2 when q2 = q3 = 1 and q1 = q4 = 0 • 𝑣o = V3 when q4 = 1 and q1 = q2 = q3 = 0 3.4.3 Flying Capacitor Configuration There are some drawbacks associated with both multilevel topologies (NPC and cas- cade) presented earlier. One of the disadvantages of the NPC topology is the need to control dc-link capacitor voltages. On the other hand, an obvious drawback for a cascade topology is the high number of dc voltage sources required. The flying capacitor converter is another topology that can generate multilevel voltages. Although needing additional flying capacitors (FCs), the capacitance values are smaller than the dc-link capacitor and there are two switching states to control the charging and discharging of FC. Unlike the NPC topology, in which just one switching state is available to obtain zero voltage at the output converter side, the FC converter has two states to generate zero voltage at the output. In practical implementation of the NPC topology there is only one dc voltage available; so two dc-link capacitors are normally used to guarantee three voltages at the input converter side, as in Fig. 3.15(a). Figure 3.15(b) shows the Table of Variables when two capacitors are used to generate three levels. For a symmetrical three-level output voltage [as in Fig. 3.12(b)] each capacitor voltage should be the same, for example, VC1 = VC2 = Vpn∕2. A control scheme should be added to guarantee this requirement, but as shown in Fig. 3.15(b), there is a missing switching state (State 3) q1 = 1 and q2 = 0, which reduces the degree of freedom for controlling capacitor voltage. This problem is minimized for the capacitor flying topologies since there are two switching states to generate zero voltage at the output. The PBG approach can also be employed to systematically obtain the flying capacitor converters. For example, Fig. 3.16(a) brings up the three-level flying
  • 90. 76 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING (a) State 1 0 q1 q2 0 2 0 1 0 3 1 0 4 1 1 (b) q2 q1 Vpn νo νo –VC2 VC2 VC1 VC1 q2 q1 – – + + 0 Figure 3.15 (a) NPC topology with a single dc voltage source and two dc-link capacitors. (b) Table of Variables. capacitor topology under PBs representation. The converters with four and five levels are depicted in Fig. 3.16(b) and 3.16(c), respectively. Details about this circuit are given in Chapter 6. Example 3.7 Write the Table of Variables for the converter given below, which is based on the three-level flying capacitor topology, with a dc voltage source instead of flying capacitor. Prove also that the switching devices can be represented by a binary variable, that is, qj = 1 is used when the switch is on and qj = 0 when the switch is off (with j = 1, 2, 3, and 4). Vdc Vdc Vdc q1 = {0,1} q2 = {0,1} νo q3 = {0,1} 0 q4 = {0,1} Solution Since there are four switches with two states each, there exist sixteen possibil- ities for the total switching states, as shown below:
  • 91. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 77 1 2 C C 1 3 2 C C 4 1 2 3 C C C C C C C C (a) (b) (c) Figure 3.16 Construction of flying capacitor multilevel legs using PBs: (a) three-level, (b) four-level, and (c) five-level.
  • 92. 78 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING row q1 q2 q3 q4 𝑣o 1 0 0 0 0 Undefined 2 0 0 0 1 Undefined 3 0 0 1 0 Undefined 4 0 0 1 1 −Vdc 5 0 1 0 0 Undefined 6 0 1 0 1 0 7 0 1 1 0 Short-circuit 8 0 1 1 1 Short-circuit 9 1 0 0 0 Undefined 10 1 0 0 1 Undefined 11 1 0 1 0 0 12 1 0 1 1 −Vdc 13 1 1 0 0 Vdc 14 1 1 0 1 Vdc 15 1 1 1 0 Short-circuit 16 1 1 1 1 Short-circuit Notice that many of the states obtained in this table are prohibited, that is, either undefined or short-circuit, and so must be avoided. Without taking into account the prohibited states, this converter can generate three different voltages at its output (i.e., −Vdc, 0, Vdc) for either positive or negative currents. Example 3.8 (a) Considering Example 3.7, what is the minimum number of independent switching states that still allows three levels at the output converter side? b) Draw the power converter with this minimum number of independent switches to guarantee a three-level output voltage. Solution (a) If there are three input voltages and the requirement is to use the switching states to select each input, the minimum number of independent switching states is 2, since 22 = 4. (b) As observed in Fig. 3.16(a), the three-level flying capacitor topology requires four switches to guarantee an output with three levels. Moreover, as shown earlier, with two independent switching states (q1 and q2) it is possible to select the three inputs available (Vdc, 0, −Vdc), which ends up with the definition of the complementary switching states q1 and q2 (q1 = 1 − q1 and q2 = 1 − q2). Below is presented the three-level flying
  • 93. 3.4 APPLICATION OF PBG IN MULTILEVEL CONFIGURATIONS 79 capacitor configuration, using only two independent switching states and the complementary switching states, as well as the Table of Variables. Comparing this Table with that in Fig. 3.15, there is no prohibited state for this topology, and this degree of freedom is used to control the voltage of the flying capacitor. Vdc Vdc Vdc q1 q2 νo 0 q1 q2 State q1 q2 𝑣o 1 0 0 −Vdc 2 0 1 0 3 1 0 0 4 1 1 Vdc 3.4.4 Other Multilevel Configurations Although the configuration obtained in Example 3.6 can generate an output voltage with three levels, it is clearly a nonconventional topology, since it is not identified as NPC, cascade, or flying capacitor converter. This section presents briefly some nonconventional converters and Chapter 7 provides the necessary details. Figure 3.17(a) shows a possible four-level topology by using the first and second PBs-ac. Since this is a four-level converter, one of its counterparts is the four-level NPC configuration shown in Fig. 3.13(b). Considering just the number of semiconductor devices employed for both circuits, it favors the nonconventional one in Fig. 3.17(a) due to the elimination of four diodes. In addition to the drawbacks of the NPC converters mentioned earlier, such topologies present unequal loss distribution among the semiconductor power devices. The active NPC (ANPC) achieves a better loss distribution and wider semiconductor devices utilization. ANPC configurations can also be presented following the PBG approach (basically considering Postulates 2 and 4), as depicted in Fig. 3.17(b) for three-level and in Fig. 3.17(c) for four-level output voltage. Many of the nonconventional configurations proposed in the technical literature can be obtained by following the axioms and postulates of the principles of the PBG, as in Fig. 3.18.
  • 94. 80 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING V2 V1 V3 V4 V2 V1 V3 V4 νo νo V2 V1 V3 V2 V1 V3 νo νo V1 V1 V4 V4 V2 V2 V3 V3 V1 V4 V2 V3 νo νo νo (a) (b) (c) Figure 3.17 Construction of nonconventional converters. (a) Nested multilevel converter. (b) Three-level ANPC multilevel legs using PB. (c) Four-level ANPC multilevel legs using PB.
  • 95. 3.5 APPLICATION OF PBG IN ac–dc–ac CONFIGURATIONS 81 (a) (b) (c) Figure 3.18 Construction of multilevel legs using PBs. 3.5 APPLICATION OF PBG IN ac–dc–ac CONFIGURATIONS Another important class of configuration that processes ac voltage is the one with two conversion stages, that is, with both rectification (ac–dc conversion) and inversion (dc–ac conversion) stages connected through a dc-link capacitor link. Such topologies are normally called ac–dc–ac configurations (or back-to-back
  • 96. 82 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING configurations) and are usually described as three-phase to three-phase (3ph–3ph), single-phase to single-phase (1ph–1ph), and single-phase to three-phase (1ph–3ph) conversions. Although each power conversion system (3ph–3ph, 1ph–1ph or 1ph–3ph) presents many possibilities of implementation in terms of the topology structure employed, the ac–dc–ac configurations can be formulated considering the principles of the PBG. Many applications require this kind of converter: (i) three-phase motor drive system with active power factor correction [see Fig. 3.19(a)], (ii) universal active power filter with a combination of series and shunt active filters [see Fig. 3.19(b)], and (iii) wind generation system [see Fig. 3.19(c)]. 3.5.1 Three-Phase to Three-Phase Configurations A three-phase back-to-back converter feeds a three-phase load from a three-phase grid employing six legs (twelve switches) with one leg connected to each phase of the system, as shown in Fig. 3.20(a). Considering the PBs and the geometry involving them, the dashed line means that all input and output variables are of ac type, while the solid line represents the dc variables of the dc-link voltage. Some other topologies can be derived from the conventional one in Fig. 3.20(a), especially when it is necessary to reduce the number of semiconductor devices. In this way, both dc-link midpoint and shared-leg connections have been employed as an approach to reduce the power switches. It means that at least one of the legs, constituted by two power switches, is no longer used for the solutions presented in Three-phase utility grid Three-phase utility grid ac–dc–ac three-phase to three-phase converter ac–dc–ac three-phase to three-phase converter Three-phase ac motor Induction machine Wind turbine Gearbox (a) (c) Three-phase utility grid ac–dc–ac three-phase to three-phase converter Non-linear load (b) Figure 3.19 Applications of the ac–dc–ac three-phase to three-phase converter: (a) ac motor drive system, (b) active power filter, and (c) double-fed induction generation system used in wind turbines.
  • 97. 3.5 APPLICATION OF PBG IN ac–dc–ac CONFIGURATIONS 83 (a) (b) (c) (d) (e) Figure 3.20 Three-phase to three-phase ac–dc–ac power conversion topology: (a) Direct solution with six legs, (b) one shared leg, (c) one dc-link midpoint connection, (d) two dc-link midpoint connections, and (e) shared-leg and dc-link midpoint connections.
  • 98. 84 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING Fig. 3.20(b)–3.20(e). However, regarding cost reduction, this approach make sense if what is saved by the number of power semiconductor devices is not lost in higher device ratings and higher values of electrolytic capacitor. Figure 3.20(b) shows a solution with a shared leg between input-output con- verter sides. Figure 3.20(c) presents a full-bridge configuration at the input side (left side), and a half-bridge configuration at the output side (right side). Although using the same number of power switches, the configuration in Fig. 3.20(e) has advantages compared to that in Fig. 3.20(d). Notice from Fig. 3.20(e) that one of the converter sides presents full-bridge characteristics (no connection with the dc-link midpoint capacitors). On the other hand, in Fig. 3.20(d), both converter sides are half-bridge. The topologies presented in Fig. 3.20 are discussed in detail in Chapter 11. Exercise 3.1 The common principle behind the topologies proposed in Fig. 3.20 is the inher- ent redundancy of the three-phase systems. For a set of balanced three-phase voltages, the relationship among the voltages is given by 𝑣1 + 𝑣2 + 𝑣3 = 0, which means that if two voltages are defined, the third one will be indirectly defined (they are linearly dependent). Considering the three-phase load con- nected to a voltage source with only two phases [𝑣A = VAcos(𝜔t + ΦA) and 𝑣B = VBcos(𝜔t + ΦB)], as depicted below, define the amplitude of the volt- ages (VA and VB) and the values of phases (ΦA and ΦB) to guarantee a balanced three-phase load voltage given by 𝑣1 = V cos(𝜔t), 𝑣2 = V cos(𝜔t + 120), and 𝑣3 = V cos(𝜔t − 120). ν1 VA VB ν2 ν3 + – – – + – + + + – In addition to reducing the number of power switches to reduce costs, it is also possible to increase the number of semiconductor devices, as depicted in Fig. 3.21 paralleling back-to-back converters, to reduce the amount of power processed by each conversion stage and improve the quality of the waveform generated by converters.
  • 99. 3.6 SUMMARY 85 (a) (b) Figure 3.21 Paralleling back-to-back converters: (a) PB representation and (b) representation with switches. 3.5.2 Single-Phase to Single-Phase Configurations As in the three-phase to three-phase ac–dc–ac configurations, it is possible to establish a systematic presentation for generation of single-phase to single-phase ac–dc–ac configurations, as in Fig. 3.22. Note that the approach of using shared-leg and dc-link capacitor midpoint are still used to guarantee the component count reduction. The single-phase back-to-back converters, including their model, PWM strategy, and analysis are addressed in Chapter 10. 3.6 SUMMARY This chapter shows that the proposed PBG strategy could be used to establish a sys- tematic method for the presentation of many of the power electronics converters that process ac voltage through a dc stage. A compilation of the main configurations was done under the PBG point of view. Instead of considering power switches as the basic elements in the process of converter construction, the PBs are employed as a higher level component, with descriptions of the details inside the blocks. The connection among the PBs, using the postulates and axioms, furnishes a simple and familiar con- cept of geometrical blocks. Such a strategy was employed for construction of classical and nonconventional configurations. As a result of the PBG approach, different configurations are now presented as a part of the same set of converters (i.e., topologies dealing with ac voltage with at least one dc stage). Besides bringing a systematic presentation, the PBG technique will play an important role in the process of topology construction. Even in the case in which practical applications are not directly addressed for a specific configuration obtained with PBG, this configuration still will be considered in this book since it provides challenges in terms of converter understanding itself and creativity in devel- oping its model and control strategies. Each configuration presented in this chapter is deeply studied in the following chapters, with the development of comprehensive model and PWM strategies. Further details can be found in References from 1 to 21.
  • 100. 86 CHAPTER 3 POWER ELECTRONICS CONVERTERS PROCESSING (a) (b) (c) (d) (e) Figure 3.22 Single-phase to single-phase ac–dc–ac power conversion topology: (a) Direct solution with four legs, (b) one shared leg, (c) one dc-link midpoint connection, (d) two dc-link midpoint connections, and (e) shared-leg and dc-link midpoint connections.
  • 101. REFERENCES 87 REFERENCES [1] Escaud B, Marty P. Introduction à l’étude des structures des convertisseurs statiques. Electron Ind 1983;56:65–71. [2] Marty and Escaud B. La commutation dans les convertisseurs statiques, Ibid., No. 60; 1983. p 69–73. [3] M. V. Miranda, A. M. N. Lima, Formal verification and controller redesign of power electronic con- verters, Proc IEEE Int Symp Ind Electron, 2004. v. 1. p. 1–6. [4] E. C. dos Santos Jr, E. R. C. da Silva. Power block geometry applied to the building of power elec- tronics converters, IEEE Trans Educ, v. 2, pp. 191–198, 2013. [5] Babaei E, Hosseini SH. New multilevel converter topology with minimum number of gate driver circuits, SPEEDAM 08; 2008. p 792–797. [6] Baker RH. Bridge converter circuit. US patent 4270163. May 1981 (filed in Aug. 79). [7] Nabae A, Takahashi I, Akagi H. A new neutral-point-clamped PWM inverter. Trans Ind Appl 1981;IA-17(5):518–523. [8] Meynard TA, Foch H. Multilevel conversion: high voltage chopper and voltage source inverters. Proceedings of IEEE PESC’92; 1992. p 397–403. [9] Chen A, Hu L, He X. A novel type of combined multilevel converter topologies. IEEE Proceedings of IECON’04; 2004. p 2290–2294. [10] Andrejak JM Lescure M. High voltage converters promising technological developments. Proc. Rec. EPE Conf.; 1987. p 1.159–1.162. [11] Choi NS, Cho JG, Cho GH. A general circuit topology of multilevel inverter. Proc Rec IEEE PESC; 1991. p 96–103. [12] Carpita M, Tenconi S. A novel multilevel structure for voltage source inverter. Proc. Rec. EPE Conf.; 1991. p. 1.90–1.94. [13] Hammond PW. Medium voltage PWM drive and method. US patent 5,625,545. 1997. [14] Peng FZ. A generalized multilevel inverter topology with self voltage balancing. IEEE Trans Ind Appl 2001;37(2):611–618. [15] Brückner T, Bernet S, Güldner H. The active NPC converter and its loss-balancing control, IEEE Trans Ind Electron, 52, No. 3, 2005, pp. 855–868. [16] T. Bruckner, S. Bernet, P.K. Steimer, Feedforward loss control of three-level active NPC converters, IEEE Trans Ind Appl, 43, no.6, pp.1588–1596, 2007. [17] Lin B-R, Yang T-Y. Single-phase switching mode multilevel rectifier with a high power factor. IEE Proc-Electr Power Appl 2005;152(3):447–454. [18] Bhagwat PM, Stefanovic VR. Generalized structure of a multilevel PWM inverter. IEEE Trans Ind Appl 1983;IA-19(6):1057–1069. [19] dos Santos Jr EC, Muniz JH, da Silva ERC, Jacobina CB. Nested multilevel configurations. IEEE Energy Conversion Congress and Exposition, ECCE 2012; 2012. p 324–329. [20] Perantzakis GS, Xepapas FH, Manias SN, A new four-level PWM inverter topology for high power applications - effect of switching strategies on power losses distribution, PESC’04; 2004. p 4398–4404. [21] Tang T, Han J, Zhou L, Yao P, Tan X. Novel hybrid cascade asymmetrical converter based on asym- metrical converter. Proceedings of IEEE ISIE; 2007 Jun. p 1004–1008.
  • 102. CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION 4.1 INTRODUCTION In this chapter, the neutral-point-clamped (NPC) configuration, also known as diode-clamped configuration, is considered under the power blocks geometry (PBG) point of view. The introduction and fundamental concepts of NPC configurations from three-level to n-level, as well as a detailed description of these circuits, including its model, pulse width modulation (PWM), and control strategies, are addressed in this chapter. The three-level NPC configuration is one of the most common topologies for medium and high voltage applications, especially in motor drive systems, because of reduced dv/dt, reduced total harmonic distortion (THD), and especially its ability to deal with high voltage demand without connecting switches in series. However, it is also possible to employ this kind of topology in lower power applications, as in photovoltaic energy systems where other factors such as voltage with low distortion and reduced leakage current are important factors. This chapter is organized as follows: in Section 4.2 the three-level NPC topology is once again obtained from the PBs and also treated in the level of power switches. Its model is obtained by deducing an equation to describe the voltage behavior at the ac side. Such an equation is achieved from the Table of Variables, which also plays an important role in the PWM development. In Section 4.3 the simplest PWM approach is detailed for the half-bridge single-phase three-level con- verter. The concepts presented previously are expanded to full-bridge single-phase and three-phase converters in Sections 4.4 and 4.5, respectively. Section 4.6 brings up nonconventional converters demonstrating how those topologies can be easily constructed by using PBG. The inherent problem of the unbalanced capacitor voltages in NPC topologies is addressed in Section 4.7. NPC configurations with number of levels higher than three are presented from Section 4.8–4.11. Section 4.12 provides a summary of the chapter. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 88
  • 103. 4.2 THREE-LEVEL CONFIGURATION 89 (a) 2 1 3 V1 V2 vo V2 (b) 2 1 3 V1 vo (c) 2 1 3 V2 vo (d) 2 1 3 V3 vo Figure 4.1 (a) Three-level (V1, V2, V3) NPC configuration with PBs. Activation of the PBs to obtain the level: (b) 𝑣o = V1. (c) 𝑣o = V2. (d) 𝑣o = V3. 4.2 THREE-LEVEL CONFIGURATION As already seen, the power blocks (PBs), can be connected following a systematic approach to guarantee the creation of NPC multilevel configurations. The first and direct arrangement of the blocks is repeated in Fig. 4.1(a), with triangular shape connected to triangular shape and square shapes connected to each other. Figure 4.1(b)–4.1(d) show the ways used to obtain each specific level (V1, V2, V3) at the output converter side. Figure 4.1(b) illustrates that it is necessary to activate PBs 1 and 3 to obtain 𝑣o = V1, while 𝑣o = V3 is obtained when PBs 2 and 3 are activated [see Fig. 4.1(d)]. On the other hand, the voltage V2 appears at the output side (𝑣o), when just PB 3 is fully activated, as observed in Fig. 4.1(c). To generate an output waveform with three levels, it is necessary to activate the PBs in a sequence as observed in Fig. 4.2. Since 𝑣o can assume just one input voltage V1, V2, or V3 at any time, it is pos- sible to write an equation to describe the output voltage 𝑣o as a function of input voltages and two independent binary variables (q1 and q2). Since there are three inputs to be selected, the minimum number of binary variables employed to select those inputs is two. These three inputs must appear at the output converter side through the use of two binary variables, which means that one possible combination to achieve this goal is given in Table 4.1. Defining complementary variables (q1 and q2) as q1 = 1 − q1 and q2 = 1 − q2, the output voltage can be defined as follows: 𝑣o = q1q2V3 + q1q2V2 + q1q2V1 (4.1) Developing (4.1) we get 𝑣o = (1 − q1)(1 − q2)V3 + (1 − q1)q2V2 + q1q2V1 (4.2) 𝑣o = (1 − q2 − q1)V3 + q2V2 + q1q2(V3 − V2 + V1) (4.3)
  • 104. 90 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION 1 2 1 2 3 3 V1 V1 V2 V3 t V2 vo vo vo 1 2 3 V3 vo Figure 4.2 Generation of a three-level output voltage for generic values of V1, V2 and V3. TABLE 4.1 Table of Variables for the Converter in Fig. 4.1(a) State q1 q2 𝑣o 1 0 0 V3 2 0 1 V2 3 1 0 4 1 1 V1 Normally the waveform presented in Fig. 4.2 must be symmetrical, which means that V1 = Vdc, V2 = 0 and V3 = − Vdc, and then it turns out that 𝑣o = (q1 + q2 − 1)Vdc (4.4) It is worth mentioning that the binary variables considered in Table 4.1 are related to the switching states inside the blocks in Fig. 4.1. Figure 4.3 shows the same topology presented in Fig. 4.1 along with the binary variables describing the state of the switches for both positive and negative output currents (io). Notice that, unlike PB-dc operating alone (see Figs 3.7 and 3.8), the NPC topology is able to generate the desired output voltage for both positive and nega- tive currents, which means that each voltage value V1, V2, and V3 can be obtained at the output converter side independent of the current values. In other words any
  • 105. 4.2 THREE-LEVEL CONFIGURATION 91 (a) V1 V2 q1 q2 V3 io q1 q2 (b) V1 V2 q1 q2 V3 io q1 q2 (c) V1 V2 q1 q2 V3 io q1 q2 Figure 4.3 Generation of levels: (a) V1, (b) V2, and (c) V3 independent of the output current. desired output voltage is obtained for both cases io > 0 and io < 0, as observed in Fig. 4.3. Example 4.1 Considering the Tables of Variables presented below, place each switch (q1, q2, q1, and q2) in the correct position in the circuit below to guarantee the generation of the levels as demanded in the following tables. State q1 q2 𝑣o State q1 q2 𝑣o 1 0 0 1 0 0 2 0 1 2 0 1 3 1 0 3 1 0 4 1 1 4 1 1 V1 V2 V3 Position 1 Position 2 Position 3 Position 4 vo Solution To guarantee an output voltage 𝑣o as demanded in the first Table of Variables, the switches q1, q2, q1, and q2 should be placed, respectively, in the positions 3, 4, 1, and 2 as below. There is no possible combination for the second table.
  • 106. 92 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION State q1 q2 𝑣o State q1 q2 𝑣o 1 0 0 V1 1 0 0 V1 2 0 1 – 2 0 1 V2 3 1 0 V2 3 1 0 V3 4 1 1 V3 4 1 1 – Example 4.2 Build the Table of Variables for the circuits presented below, with respect to the position of each switch. V1 V2 V3 q1 q2 q1 q2 vo V1 V2 V3 q1 q2 q1 q2 vo Solution The Table of Variables for each circuit is given, respectively, by State q1 q2 𝑣o State q1 q2 𝑣o 1 0 0 V3 1 0 0 V2 2 0 1 undefined 2 0 1 undefined 3 1 0 undefined 3 1 0 undefined 4 1 1 V3 4 1 1 undefined Exercise 4.1 Considering the tables presented in Example 4.2, show through equivalent cir- cuits and assuming positive and negative currents, why some of the states are undefined.
  • 107. 4.3 PWM IMPLEMENTATION (HALF-BRIDGE TOPOLOGY) 93 Notice that for the two arrangements in Example 4.2 there are more than one undefined states, which means that there is no way to obtain three levels at the output converter side, as seen in Fig. 4.3. Such a characteristic is not desirable for a power converter processing ac voltage. 4.3 PWM IMPLEMENTATION (HALF-BRIDGE TOPOLOGY) If the aim is to generate an ac voltage at the output converter side with both ampli- tude and frequency controllable, a PWM strategy is applied to generate the switching gating signals. From a converter processing ac voltage, ideally an output sinusoidal voltage is expected. However, due to the characteristics of the NPC converter pre- sented in Fig. 4.2, the number of levels is limited to three. Hence, the aim of the PWM strategy is to guarantee that the three-level voltage at the output of the converter emulates the desirable sinusoidal voltage. The average value of the square output waveform must be equal to a sinusoidal reference (inside the switching period) as presented in the figure below. vl ∗ vl ∗ vl ∗ vl vl vl Switching frequency Normally, the switching frequency is kept high (compared to the modulating signal) to increase the accuracy of 𝑣l ≈ 𝑣∗ l . In fact many works in the technical lit- erature have proposed solutions in terms of modulation approaches applied for NPC converters to improve different aspects of the converter. In this chapter, the simplest way to generate the PWM waveforms is considered. However, an optimized PWM approach is derived in Chapter 8. Figure 4.4 shows a simple analog solution, in which the states of the four switches are determined by a comparison among a sinusoidal waveform (𝑣∗ sin ) and two high frequency triangular waveforms (𝑣∗ t1 and 𝑣∗ t2 ). Such PWM can be expanded for NPC converters with higher levels, which uses N − 1 (N is the number of levels) triangular carrier signals with just one modulating signal. The sinusoidal waveform is given by 𝑣∗ sin = Vl sin(𝜔lt), where Vl is the amplitude and 𝜔l is the angular fre- quency desired to the load. The block mentioned as driver must guarantee the levels of voltage and current in the switch’s gate circuit needed to operate the power devices adequately as well as guarantee galvanic isolation. Notice from Fig. 4.4(c) and 4.4(d) that when the switches q1 and q1 are chang- ing their states (during the positive half cycle of 𝑣∗ sin ), switch q2 is on and switch q2
  • 108. 94 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION driver + – driver q1 q2 q1 q2 vsin * vt1 * 1 0 1 0 1 0 0.2 0.225 0.25 –1 q1 q1 vsin * vt1 * 0.2 0.225 0.25 1 0 1 0 1 0 –1 q1 q2 vsin * vt2 * driver + – driver q1 q2 q1 q2 vsin * vt2 * (a) (b) (c) (d) Figure 4.4 (a) PWM generation circuit for switches: (a) q1 and q1; and (b) q2 and q2. (c) Variables associated with switches q1 and q1 (from top to bottom) – reference voltages, gating signal of switch q1 and gating signal of switch q1. (d) Variables associated with switches q2 and q2 (from top to bottom) reference voltages, gating signal of switch q2 and gating signal of switch q2. is consequently off for the entire half cycle, while in the negative half cycle of 𝑣∗ sin , when switches q2 and q2 are changing their states, switch q1 is off and switch q1 is on. The modulation presented in Fig. 4.4 describes the states in Table 4.1, when q2 is on and q1 can be either off (State 2 in Table 4.1) or on (State 4 in Table 4.1). In the same way, when q1 is off, q2 can be either off (State 4.1 in Table 4.1) or on (State 2 in Table 4.1). Also, this modulation approach avoids the undesired State 3. Figure 4.5(a) shows the half-bridge three-level configuration, in which the load is connected between the dc-link midpoint and the center point of the leg.
  • 109. 4.4 FULL-BRIDGE TOPOLOGIES 95 q2 q1 q1 q1 q2 Vdc Vdc R + – L q2 vo vo io io 0 0 1 –1 1 0 200 50 –200 –50 0.2 0.225 0.25 1 (a) (b) Figure 4.5 (a) Three-level NPC half-bridge converter. (b) (from top to bottom) 𝑣∗ sin , 𝑣∗ t1 , 𝑣∗ t2 ; gating signal of switch q1; gating signal of switch q2; load voltage and load current. Figure 4.5(b) depicts (from top to bottom) PWM reference waveforms, gat- ing signal of switches q1 and q2, load voltage, and load current, respectively. The parameters employed in these simulation tests were: Vdc = 200 V, R = 5Ω and L = 5mH, and switching frequency equal to 500Hz. For the sake of com- parison, the same parameters are used for the other simulation results in this chapter. Sometimes in practical applications just one dc source is available, which means that both dc sources shown in Fig. 4.5(a) are changed by capacitors connected to a single dc source. In this sense, it is necessary to guarantee the control voltage for both capacitors. This specific issue is considered later on in this chapter. 4.4 FULL-BRIDGE TOPOLOGIES The three-level NPC topology with two legs, that forms a full-bridge single-phase converter, can be obtained from PBG by connecting the PBs given in Fig. 4.1 appro- priately, as seen in Fig. 4.6(a). Following this approach it is also possible to build
  • 110. 96 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION a (a) b V2 V1 V3 1 2 3 a (b) b c V2 V1 V3 1 2 3 a (c) b c d V2 V1 V3 1 2 3 Figure 4.6 NPC three-level topology with: (a) two legs (full-bridge single-phase load), (b) three legs (three-phase load), and (c) four legs (three-phase four-wire load). configurations with n legs. Figure 4.6(b) shows a three-level NPC topology with three legs for applications demanding a three-phase system (e.g., three-phase motor drive systems or three-phase rectifier converter), while Fig. 4.6(c) shows a three-level NPC topology with four legs to be employed, for instance, in a three-phase four-wire system. These three configurations in Fig. 4.6 are described in the following sections. Figure 4.7(a) presents the full-bridge single-phase converter [as in Fig. 4.6(a)] highlighting the connections of the switches. It is worth mentioning that even though the full-bridge topology in Fig. 4.7(a) is constituted by three-level legs, the output voltage has five levels. Figure 4.7(b) shows (from top to bottom) pole voltage (voltage between the midpoint of the leg and the dc-link capacitor midpoint 𝑣a0) of the first leg with three levels, pole voltage of the second (𝑣b0) also with three levels, load voltage, and load current, respectively. Comparing Figs 4.5 and 4.7, it is evident that the increased number of levels observed on the load voltage of the full-bridge topology guarantees a ripple reduction on the load current for the full-bridge topology. In this case the output voltage is given by 𝑣o = (q1a + q2a − q1b − q2b)Vdc (4.5) The number of levels considered in this chapter for conventional topologies is defined by the pole voltages. For instance, both converters in Figs 4.5 and 4.7 are
  • 111. 4.4 FULL-BRIDGE TOPOLOGIES 97 q2a q1a q2b q1b q1a q2a a b 0 q1b q2b Vdc Vdc R + – L vo va0 vb0 vo io io 200 –200 200 500 –500 100 –100 0.2 0.225 0.25 –200 (a) (b) Figure 4.7 (a) Three-level NPC full-bridge converter. (b) (from top to bottom) pole voltage of the first leg (𝑣a0), pole voltage of the second (𝑣b0), load voltage and load current. considered as single-phase three-level NPC topologies, although they present differ- ent number of levels for the load voltages. Example 4.3 Considering the topology presented in Fig. 4.7(a), find a solution for the PWM generation circuit to guarantee the waveforms shown in Fig. 4.7(b). Solution A set with a reference sinusoidal and two triangular waveforms plus two OpAmps for each leg (as seen in Fig. 4.4 for the half-bridge topology) can be employed for the PWM signal generation for the full-bridge topology. Since the control of both legs is independent, those sinusoidal waveforms should have 180∘ of phase apart to guarantee a maximum output voltage.
  • 112. 98 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION Example 4.4 What happens if different phase displacements are employed for both reference sinusoidal waveforms? Solution The figure below shows a phase or diagram representation for the pole voltages 𝑣a0 and 𝑣b0 (just for the sinusoidal components) as well as for the load voltage 𝑣o = 𝑣a0 − 𝑣b0. The output voltage is a function of the phase displacement of the pole voltages, meaning that the maximum output voltages will be obtained when this phase displacement angle is equal to 180∘. 180° 90° 0° va0 va0 vb0 vl = va0 – vb0 vl = va0 – vb0 vl = 0 va0 = vb0 vb0 4.5 THREE-PHASE NPC CONVERTER A three-phase three-level full-bridge NPC configuration is depicted in Fig. 4.8(a) by employing switches. Notice that this circuit was easily obtained by just connecting the PBs as seen in Fig. 4.6(b). Figure 4.8(b), in turn, shows some variables associated with this converter, that is, (from top to bottom): pole voltage, voltage between the load neutral point (NP) (n) and dc-link midpoint connection (0), load phase voltage, and load current, respectively. The pole voltages can be written as follows: 𝑣a0 = (q1a + q2a − 1)Vdc (4.6) 𝑣b0 = (q1b + q2b − 1)Vdc (4.7) 𝑣c0 = (q1c + q2c − 1)Vdc (4.8) The load phase voltages are given by 𝑣a = 𝑣a0 − 𝑣n0 (4.9) 𝑣b = 𝑣b0 − 𝑣n0 (4.10) 𝑣c = 𝑣c0 − 𝑣n0 (4.11) Considering a balanced three-phase condition (𝑣a + 𝑣b + 𝑣c = 0), the voltage between the NP of the three-phase load (n) and the dc-link midpoint can be defined
  • 113. 4.5 THREE-PHASE NPC CONVERTER 99 q2a q1a q2b q1b q2c q1c q1a q2a a b c n 0 q1b q2b q1c q2c Vdc Vdc R L R L R L va0 vn0 van ia ia 500 0 0 0 0 –500 500 500 –500 100 –100 0.2 0.225 (b) (a) 0.25 –500 Figure 4.8 (a) Three-phase NPC converter. (b) (from top to bottom) pole voltage, voltage 𝑣n0, load voltage, and load current. analytically by 𝑣n0 = 1 3 (𝑣a0 + 𝑣b0 + 𝑣c0) (4.12) Substituting (4.10)–(4.12) into (4.13), we have 𝑣n0 = Vdc 3 (q1a + q2a + q1b + q2b + q1c + q2c) − Vdc (4.13) From (4.13), the voltage for each phase of the three-phase load can be written as follows: 𝑣a = ( 2 3 q1a + 2 3 q2a − 1 3 q1b − 1 3 q2b − 1 3 q1c − 1 3 q2c ) Vdc (4.14) 𝑣b = ( − 1 3 q1a − 1 3 q2a + 2 3 q1b + 2 3 q2b − 1 3 q1c − 1 3 q2c ) Vdc (4.15) 𝑣c = ( − 1 3 q1a − 1 3 q2a − 1 3 q1b − 1 3 q2b + 2 3 q1c + 2 3 q2c ) Vdc (4.16) In the case of a balanced three-phase load, the load voltages depend only of the state of the switches and of the dc-link voltage as considered in (4.15)–(4.17).
  • 114. 100 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION The control circuit for the three-phase converter can be obtained as seen in Fig. 4.4. The difference is the number of modulating signals needed; in this case there are three references: 𝑣∗ sin 1 = Vl sin(𝜔t), 𝑣∗ sin 2 = Vl sin(𝜔t + 120∘) and 𝑣∗ sin 3 = Vl sin(𝜔t + 240∘), where Vl and 𝜔l are the desired peak voltage and frequency for the load, respectively. Exercise 4.2 Create a table relating all states of the switches (64 possibilities) to find the number of levels for 𝑣n0 and the number of levels for the phase voltage 𝑣a for the converter shown in Fig. 4.8. Application (High Voltage Motor Drive System) The three-phase NPC multilevel configuration can be employed in medium voltage (MV) drives to reach a high voltage level without using switching devices in series connection. The switching frequency for MV high power application is normally low as compared to the two-level converter in order to reduce the power losses (it is usually limited to a few hundred hertz) without compromising the quality of the wave- forms generated due to the number of levels. Normally, special modulation tech- niques are needed to produce the minimum harmonic distortion for the motor cur- rent for a large range of speed and torque. The main applications are in pumps, fans/exhausts, compressors, mixers, agitators, conveyors, cement mills, steel mills, winders/unwinders, sugar mills, refiners, banburys, and extruders. The figure below shows a common scheme with an NPC topology employed in MV drives. Utility grid Switch gear Transformer Mv inverter MV induction motor M 3~ Y Δ Δ
  • 115. 4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 101 q2a q1a q2b q1b q2c q1c q1a q2a a b c 0 q1b q2b q1c q2c Vdc Vdc R L R L R L Figure 4.9 Three-level NPC converter supplying a three-phase load connected in Δ arrangement. Exercise 4.3 An MV three-phase motor has line-to-line and active power given, respectively, by 2.3 kV and 150 kW (with power factor 0.85). Assuming that this motor will be supplied by a three-leg NPC topology, determine the voltage and current ratings of the switches for this configuration. Figure 4.9 shows the NPC three-phase power converter topology supplying a Δ- connected three-phase load. The main difference between Figs 4.9 and 4.8(a) is related to the values of voltages and current demanded by the load, as well as the number of levels measured on the load voltages. In this case (Δ-connected) the load phase voltage has only five levels, as seen from the equations given below: 𝑣a = (q1a + q2a − q1b − q2b)Vdc (4.17) 𝑣b = (q1b + q2b − q1c − q2c)Vdc (4.18) 𝑣c = (q1c + q2c − q1a − q2a)Vdc (4.19) 4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS It is possible to combine the NPC leg with two-level legs already presented in this chapter to establish a nonconventional single-phase multilevel converter, as seen in Fig. 4.10. In this case, it is used four PBs with the output load connected between blocks 3 and 4. Since the output of block 3 has three levels (V1, V2, and V3) and the
  • 116. 102 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION V1 V2 V3 2 1 3 4 vo Figure 4.10 Five-level single-phase converter obtained by the combination of NPC and conventional legs – block representation. TABLE 4.2 Table of Variables for the Converter in Fig. 4.10 State q1a q2a q1b Output of PB 3 Output of PB 4 𝑣o 1 0 0 0 − Vdc − Vdc 0 2 0 0 1 − Vdc Vdc − 2Vdc 3 0 1 0 0 − Vdc Vdc 4 0 1 1 0 Vdc − Vdc 5 1 1 0 Vdc − Vdc 2Vdc 6 1 1 1 Vdc Vdc 0 output of block 4 has two levels (V1 and V3), it leads to an output voltage with five levels (0, V1 − V3, V2 − V1, V2 − V3, V3 − V1). For a symmetrical output voltage generation, the input voltages should have the following parameters: V1 = Vdc, V2 = 0, and V3 = − Vdc, meaning that the output volt- age will be with the following values 0, ± Vdc, ± 2Vdc. For the converter in Fig. 4.10 it is necessary for three independent binary signals (q1a, q2a, and q1b) to synthesize the desired output voltage since there are five levels. Table 4.2 shows the voltage 𝑣o as a function of q1a, q2a, and q1b. Equations to describe the pole voltages (𝑣a0 and 𝑣b0) and output voltage 𝑣o as a function of the input voltages and as a function of three independent binary variables (q1a, q2a, and q1b) are given below, respectively: 𝑣a0 = (q1a + q2a − 1)Vdc (4.20) 𝑣b0 = (2q1b − 1)Vdc (4.21) 𝑣o = (q1a + q2a − 2q1b)Vdc (4.22) The binary variables considered in both Table 4.2 and in equation (4.22) are in fact the switching states inside the blocks, which means that the topology presented in Fig. 4.10 can be considered in its lower level representation (switches instead of blocks), as in Fig. 4.11.
  • 117. 4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 103 q2a q1a q1b q1a q1b q2a a b 0 Vdc Vdc + – vo io Figure 4.11 Five-level single-phase converter obtained by the combination of NPC and conventional legs with switches. Exercise 4.4 Assuming all switching states given in Table 4.2, write a Table showing the blocking voltages and current through the switches for the six switches employed in Fig. 4.11. It is also possible to generate a four-level topology with the same PBs as in Fig. 4.10, but with a different arrangement as presented in Fig. 4.12. Notice that the capacitors in Fig. 4.12(a) are used to guarantee the NP needed by the NPC leg. Figure 4.12(b) shows the same configuration with the switches. In this case, it needs three dc sources with the advantage of using all switches with the same blocking voltage, as discussed in this section. q2a q1a q1b q1b q1a q2a a b V1 1 2 3 4 V2 V3 V1 V2 V3 + – vo vo io Figure 4.12 Four-level single-phase converter: (a) block representation and (b) circuit with switches.
  • 118. 104 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION TABLE 4.3 Table of Variables for the Converter in Fig. 4.12 State q1a q2a q1b 𝑣o 1 0 0 0 − V3 2 0 0 1 − V3 − V2 3 0 1 0 − V2/2 4 0 1 1 V2/2 5 1 1 0 V1 + V2 6 1 1 1 V1 The converter in Fig. 4.12 has six switches (q1a, q1a, q2a, q2a, q1b, and q1b), two clamping diodes, three dc sources, and two dc-link capacitors. Considering all possible switching states available and eliminating the prohibited ones, the output voltage is determined in Table 4.3. To guarantee that all power switches will oper- ate under the same blocking voltage as well as a symmetrical output voltage, it is necessary to establish V1 = V3 = Vdc/4 and V2 = Vdc/2. The modulation strategy for the converter shown in Fig. 4.12 can be determined assuming a combination of the two-level and three-level PWM approaches, which means that, for the two-level leg [PB 4 in Fig. 4.12(a)] only one triangular carrier signal will be employed, while for the three-level leg [PBs 1, 2, and 3 in Fig. 4.12(a)] two triangular carrier signals will be employed, as observed in Fig. 4.13(a). Since the triangular waveform is proportional to the dc-link voltage associated with each leg, the voltages 𝑣∗ t1 , 𝑣∗ t2 , and 𝑣∗ t3 can be obtained as shown in Fig. 4.13(b). In this sense, the two-level leg will deal with one-third of the output voltage while the three-level leg will deal with two-third of the desired output voltage. The pole voltage for the three-level, two-level legs and output voltage is given respectively by 𝑣a0 = (q1a + q2a − 1)2Vdc (4.23) 𝑣b0 = (2q1b − 1)Vdc (4.24) 𝑣o = (q1a + q2a − 2q1b − 1)Vdc (4.25) Figure 4.14(a) and 4.14(b) shows the output voltage and current for a switching frequency equal to 500 Hz and 1 kHz, respectively. Although the configuration shown in Fig. 4.12 can generate a four-level output voltage, it needs either three independent dc voltages or an auxiliary circuit to obtain three controlled voltages from a unique dc voltage source, as in Fig. 4.14(c) – top. Figure 4.14(c) – bottom shows the equivalent topological states when the switches in the auxiliary circuit are turned on and off simultaneously. A duty cycle of 50% should be generated to guarantee a desired capacitor voltage in the dc-link of the converters. Using the three-level NPC topologies and a three-phase load type, it is possible to create a three-phase NPC topology with both two- and three-level characteristics
  • 119. 4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 105 q2a qb qb q1a q1a q2a vsin * 2 3 + – vt1 * vsin * 2 3 + – + – – 2/3vsin –1/3vsin * * vt1 * vsin * 1 3 vt2 * vt2 * vt1 * vt3 * 1 –1 0 0.66 –0.66 0 0.2 0.225 0.25 Figure 4.13 PWM generation: (a) analog implementation and (b) waveforms. for the pole voltage. In this case, the dc-link of the three-phase converter is connected to two PB-dc blocks, as depicted in Fig. 4.15. Figure 4.15(a) shows such hybrid topol- ogy with the PBs perspective, while Fig. 4.15(b) depicts this topology by using power switches. For a symmetrical waveform generation, it is necessary to define the input voltages as follows: V1 = Vdc, V2 = 0, and V3 = − Vdc. The operation of this converter takes into account the fact that it is possible to obtain different levels per phase, depending on the values for the reference voltages. For instance, Fig. 4.16(a) – top shows the desired phase voltages (𝑣∗ a, 𝑣∗ b , and 𝑣∗ c ) divided by sectors. The first sector is defined by the interval of time in which 𝑣∗ a is
  • 120. 106 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION (a) (b) (c) –30 –150 150 0 30 0 0.2 0.225 0.25 vo io –30 –150 150 0 30 0 0.2 0.225 0.25 vo io q1a q2a q1a qb qb q2a a b Vdc Auxiliary circuit Equivalent circuit 1 Equivalent circuit 2 C1 C2 C3 C4 + – vo io Figure 4.14 Output voltage and current for the configuration in Fig. 4.12 with: (a) 500 Hz and (b) 1 kHz. (c) (top) Auxiliary circuit and (bottom) equivalent topological circuit.
  • 121. 4.6 NONCONVENTIONAL ARRANGEMENTS BY USING THREE-LEVEL LEGS 107 q2 q1a qb qa q1 qb qc qc qa a b c 0 Vdc Vdc V1 c b a V2 1 2 (a) (b) 3 V3 Figure 4.15 Hybrid topology: (a) power blocks and (b) switching representation. maximum, 𝑣∗ b is minimum, and 𝑣∗ c is in-between. It means that: (i) phase a can be modulated as a three-level leg (with pole voltage 𝑣a0 between Vdc and 0), since it is expected to generate the maximum voltage; (ii) phase b can be modulated as a three-level leg (with pole voltage 𝑣b0 between 0 and − Vdc); and finally (iii) phase c can be modulated as a two-level leg (with the pole voltage between Vdc and − Vdc). The modulation strategy for the leg dealing with the highest and smallest voltages (three levels) are obtained by comparing the desired waveforms with two triangular waveforms (with level-shift approach) as shown in Fig. 4.4, while the modulation for the leg dealing with middle voltages (two levels) is obtained through a comparison between the reference voltage and one triangular waveform. Still considering nonconventional configurations, a half-bridge three-phase NPC topology is shown in Fig. 4.17(a).
  • 122. 108 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION va * vb * vc * 1 –1 0 50 –50 0 50 –50 0 50 –50 –15 15 0 0 0.77 0.8 0.77 0.8 va0 vb0 vc0 ia ib ic (a) (b) Figure 4.16 (a) Desired reference voltage and pole voltages. (b) Load current. As in the case of previous nonconventional topologies, it is necessary to adapt the PWM strategy [see Fig. 4.17(b) and 4.17(c)] employed to guarantee the gener- ation of a balanced three-phase load voltage. The challenge in this case is that the three-phase currents of the load must be regulated in a balanced way, even though there are only two legs available to do it. Two load currents are directly controlled by these two legs, and the third one is indirectly controlled, since ia + ib + ic = 0. The maximum amplitude of the line-to-line reference voltages (𝑣∗ ac = 𝑣∗ a − 𝑣∗ c ) and (𝑣∗ bc = 𝑣∗ b − 𝑣∗ c) is limited by the amplitude of the triangular waveforms, as in Fig. 4.17(c). In these, the triangular waveforms have a frequency of 1 KHz. As this topology cannot be considered conventional, there are some restrictions in its practical application. However, it could be employed in fault-tolerant systems, as a backup configuration in the case of a fault of the three-leg conventional topology (Fig. 4.8). 4.7 UNBALANCED CAPACITOR VOLTAGE If there is only one dc voltage source available, the NP required for the NPC con- figuration can be obtained with two capacitors in a series connection, as seen in Fig. 4.18(a). When a leg of the converter is connected (or clamped) to the NP, as in
  • 123. 4.7 UNBALANCED CAPACITOR VOLTAGE 109 q2b q1a driver driver driver driver driver driver driver driver q1a q2a q2a q1b q1b q2b q2b q1b q1b q2b q2a q1a q1a q2a Vdc Vdc R R R L L L va * vac * vt1 * vt2 * vc * vb * Σ Σ + – + – + – – – + – vac * vac * vt1 * vt1 1 –1 0 1 –1 0 40 –40 0 0.2 0.225 0.25 * vt2 * vt2 * vbc * vt1 * ia ib ic vt2 * vb * (a) (b) (c) Figure 4.17 (a) Half-bridge three-level three-phase NPC converter. (b) PWM strategy. (c) (from top to bottom) reference waveforms for leg a (𝑣∗ a − 𝑣∗ c , 𝑣∗ t1 , and 𝑣∗ t2 ), reference waveforms for leg b (𝑣∗ b − 𝑣∗ c , 𝑣∗ t1 , and 𝑣∗ t2 ) and load currents.
  • 124. 110 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION a b c Three-phase load 215 200 185 0 0.5 1 Vdc Vdc C1 0 (NP) 0 (NP) + – + – C2 C1 C2 iC1 iC1 iNP vC1 vC2 iC2 vC2 vC1 iC2 ic ib ia iNP iNPa iNPb iNPc (a) (b) (c) Figure 4.18 (a) NPC three-level topology with one dc voltage source. (b) Circuit showing the currents in the capacitors. (c) Capacitor voltages. Fig. 4.18(b), its current is injected at this point. The NP current (iNP) can be expressed by the following equation iNP = q2aq1aia + q2bq1bib + q2cq1cic (4.26) Notice that the NP is a floating point. In an open-loop operation and without a specific PWM strategy, there is no guarantee that 𝑣C1 and 𝑣C2 will converge to the desired voltage, that is, Vdc/2. Considering the simple modulation strategy presented in this chapter, the capacitor voltages are unbalanced, as in Fig. 4.18(c), which brings up asymmetry at the output voltage of the converter. To explain this capacitor voltage behavior it is necessary to observe the vari- ables responsible for charging and discharging C1 and C2 highlighting the start-up transient. From equation (4.25) it is seen that each component of the NP current iNPx = q2xq1xix (with x = a, b, c) is a function of load current and switching states. For example, Fig. 4.19(a) shows two currents associated with phase a, (i.e., ia and iNPa). Notice that iNPa [the first portion of equation (4.26)] is actually the current ia multiplied by the state of the switches q2a and q1a. As expected, such a current has
  • 125. 4.7 UNBALANCED CAPACITOR VOLTAGE 111 (a) (b) (c) 0.2 100 –100 0 100 –100 0 100 –100 0 100 –100 0 100 –100 0 0.225 0.25 0.2 0.225 0.25 100 –100 0 100 –100 0 0.2 0.225 0.25 iC2 iC1 iNPa iNPa iNPb iNPc ia Figure 4.19 (a) ia and iNPa. (b) iNPa, iNPb, and iNPc. (c) iC1 and iC2. an average value equal to 0. The behavior of the currents iNPa, iNPb, and iNPc is shown in Fig. 4.19(b). The capacitor currents iC1 and iC2 are functions of iNPa, iNPb, and iNPc, as seen in Fig. 4.19(c). The reason why the capacitor voltage 𝑣C1 goes down and 𝑣C2 goes up in Fig. 4.18(c) is because iC1 starts with a negative value while iC2 starts with a positive value, that is, initially C1 is discharged and C2 is charged but always maintaining the 𝑣C1 + 𝑣C2 constant and equal to Vdc. There are different strategies to regulate 𝑣C1 and 𝑣C2 by either using feedback controllers or with specific PWM approaches.
  • 126. 112 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION (a) (b) (c) (d) (e) 2 1 4 5 3 V1 V2 vo 2 1 4 5 3 V1 vo 2 1 4 5 3 V2 vo 2 1 4 5 3 V3 vo 2 1 4 5 3 V4 vo V3 V4 Figure 4.20 (a) Four-level NPC configuration with PBs. (b) 𝑣o = V1. (c) 𝑣o = V2. (d) 𝑣o = V3. (e) 𝑣o = V4. 4.8 FOUR-LEVEL CONFIGURATION Following the axioms and postulates involving the PBs, presented in the previous chapter, the four-level (NPC) leg can be easily obtained as seen in Fig. 4.20(a). Figure 4.20(b)–4.20(e) shows the ways used to obtain each specific level (V1, V2, V3, and V4) at the output converter side. Figure 4.20(b) illustrates that it is necessary to activate the PBs 1, 3 and 5 to obtain 𝑣o = V1, while 𝑣o = V4 is obtained when PBs 2, 4, and 5 are activated [see Fig. 4.20(e)]. On the other hand, the intermediate voltages V2 and V3 are obtained at the output side when PBs 3 and 5, and PBs 4 and 5 are activated, respectively. In general terms, to generate an output waveform with four levels as in Fig. 4.21 (bottom), it is necessary to activate the PBs in a sequence as observed in Fig. 4.21 (top). Since 𝑣o is supposed to assume just one input voltage V1, V2, V3, or V4 at a time, an equation to describe the output voltage 𝑣o as a function of the input voltages can be obtained from the independent binary variables (q1, q2, and q3). As in the
  • 127. 4.8 FOUR-LEVEL CONFIGURATION 113 2 1 4 5 3 V1 V1 vo vo 2 1 4 5 3 V2 V2 vo 2 1 4 5 3 V3 V3 vo 2 1 4 5 3 V4 V4 t vo Figure 4.21 Generation of a general four-level output voltage. TABLE 4.4 Table of Variables for the Converter in Fig. 4.20(a) State q1 q2 q3 𝑣o 1 0 0 0 V4 2 0 0 1 V3 3 0 1 0 4 0 1 1 V2 5 1 0 0 6 1 0 1 7 1 1 0 8 1 1 1 V1 three-level NPC topology, the binary variables considered in Table 4.4 are related to the switching states inside the blocks in Fig. 4.20. In this case, the output pole voltage is given by 𝑣o = q1q2q3V4 + q1q2q3V3 + q1q2q3V2 + q1q2q3V1 (4.27) where q1 = 1 − q1, q2 = 1 − q2, and q3 = 1 − q3. Normally the waveform shown in Fig. 4.21 must be symmetrical, which means that V1 = Vdc, V2 = Vdc/3, V3 = − Vdc/3, and V4 = − Vdc, and 𝑣o = ( −q1q2q3 − q1q2q3 3 + q1q2q3 3 + q1q2q3 ) Vdc (4.28) If any other combination of output voltages associated with the switching states is considered, instead of the Table of Variables presented in Table 4.4, it will lead to undesired states, as presented shown in Example 4.2.
  • 128. 114 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION q1 V1 q2 (a) (b) (c) (d) q3 io q1 V3 q2 q3 io q1 V4 q2 q3 io q1 V2 q2 q3 io Figure 4.22 Generation of the level: (a) V1, (b) V2, (c) V3, and (d) V4 independent of the output current. The four-level NPC configuration has no restriction in terms of the generation of desired output voltage and the values of currents, which means that each desired voltage value V1, V2, V3, and V4 can be obtained at the output converter side for any values of current (io > 0 or io < 0) as in Fig. 4.22.
  • 129. 4.9 PWM IMPLEMENTATION (FOUR-LEVEL CONFIGURATION) 115 driver driver + – q1 q2 q3 q1 q1 q2 q3 vsin * vt1 * vt1 * driver driver + – q1 q2 q3 q1 q2 q3 vsin * vt2 * driver driver + – q1 q2 q3 q1 q2 q3 vsin * vt3 * 1 0 1 0 1 0 0.2 0.225 0.25 –1 q1 vsin * q2 vt2 * 1 0 1 0 1 0 0.2 0.225 0.25 –1 q2 vsin * q3 vt3 * 1 0 1 0 1 0 0.2 0.225 0.25 –1 q3 vsin * (a) (b) (c) (d) (e) (f) Figure 4.23 Four-level NPC topology – control circuit and signals for the switches. 4.9 PWM IMPLEMENTATION (FOUR-LEVEL CONFIGURATION) Figure 4.23 shows the analog solution for the PWM generation of one leg. The states of the six switches are determined by a comparison among three high frequency tri- angular waveforms (𝑣∗ t1 , 𝑣∗ t2 , and 𝑣∗ t3 ) and a sinusoidal waveform (𝑣∗ sin ).
  • 130. 116 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION It can be seen from Fig. 4.23 that these three triangular waveforms (𝑣∗ t1 , 𝑣∗ t2 , and 𝑣∗ t3 ) are intentionally level-shifted to guarantee four levels at the output converter side. During the interval of time in which q1 and q1 are in operation (i.e., turning on and off) q2 and q3 are always on and consequently q2 and q3 are always off. This is exactly what is expected from Table 4.4, rows 8 and 4, that is, when the switching sequence is changed from (q1,q2,q3) = (1,1,1) to (q1,q2,q3) = (0,1,1) the output voltage will change from V1 to V2. On the other hand, during the interval of time in which q2 and q2 are in operation (turning on and off) q1 is always off and q3 is always on, which is expected from Table 4.4, rows 2 and 4. In this case, when the switching sequence is changed from (q1,q2,q3) = (0,0,1) to (q1,q2,q3) = (0,1,1) the output voltage will change from V3 to V2. Finally, for the interval of time in which q3 and q3 are in operation (turning on and off) q1 and q2 are always off, which is also expected from Table 4.4, rows 1 and 2. When the switching sequence is changed from (q1,q2,q3) = (0,0,0) to (q1,q2,q3) = (0,0,1) the output voltage will change from V4 to V3. Figure 4.24 shows the power converter and waveforms for a half-bridge four-level configuration. If only one dc source is available, as in Fig. 4.18, additional R L q1 Vdc1 Vdc2 Vdc3 Vdc4 q2 q3 q1 q2 q3 (a) 1 1 0 1 0 1 0 200 –200 50 –50 0.2 0.225 0.25 –1 q1 q2 q3 vo io (b) Figure 4.24 (a) Four-level NPC half-bridge converter. (b) (from top to bottom) 𝑣∗ sin , 𝑣∗ t1 , 𝑣∗ t2 , 𝑣∗ t3 ; gating signal of switch q1; gating signal of switch q2; gating signal of switch q3; load voltage and load current.
  • 131. 4.9 PWM IMPLEMENTATION (FOUR-LEVEL CONFIGURATION) 117 capacitors can be employed to obtain four voltage levels. However, the challenge to control the capacitor voltages from a single dc source increases with the number of levels of the converters. From four levels onwards, an auxiliary circuit is normally needed to guarantee the control of such capacitors for a large range of load power factor. It is worth mentioning that the number of triangular waveforms increases pro- portionally to the number of levels. For a converter with n levels n − 1 triangular waveforms are needed at the output of the converter. As a consequence of the high number of triangular waveforms, such converters must be designed to operate at high modulation index to guarantee the desired amount of levels at the output converter side. Figure 4.25 shows the influence of the modulation index (ma) in the converter waveforms. Such a figure highlights the control (top) and output converter (middle and bottom) waveforms for three different values of ma. When ma is decreased, the (a) (b) 1 0 –1 200 0 –200 40 0 0 0.02 0.04 0 0.02 0.04 –40 1 0 –1 200 0 –200 40 0 –40 Figure 4.25 (top) Sinusoidal and triangular waveforms, (middle) load voltage and (bottom) load current: (a) ma = 0.8, (b) ma = 0.45, and ma = 0.2.
  • 132. 118 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION (c) 0 0.02 0.04 1 0 –1 200 0 –200 40 0 –40 Figure 4.25 (Continued) number of levels reduces as well, as observed in the sequence of Fig. 4.25(a), 4.25(b), and 4.25(c), respectively. The output voltage is reduced to a two-level waveform when the modulation index is equal to 0.2. 4.10 FULL-BRIDGE AND OTHER CIRCUITS (FOUR-LEVEL CONFIGURATION) The full-bridge single-phase converter using four-level NPC legs is shown in Fig. 4.26(a). This topology could be of interest in single-phase applications when the quality of the output voltage is an important aspect of the design since the load voltage (𝑣o = 𝑣a0 − 𝑣b0) has almost sinusoidal behavior. Figure 4.26(b) shows (from top to bottom) pole voltage 𝑣a0, pole voltage 𝑣b0, load voltage, and load current, respectively. A three-phase three-level full-bridge NPC configuration is depicted in Fig. 4.27(a), while Fig. 4.27(b) shows some variables associated with this converter, that is, (from top to bottom) pole voltage (𝑣a0), voltage between load NP and dc-link midpoint connection (𝑣n0), load phase voltage (𝑣an), and load current (ia), respectively. Figure 4.28 shows a half-bridge three-phase four-level NPC topology. In this case, a similar approach employed for the three-level topology, in terms of the PWM circuit, is also considered for this configuration. A four-level topology can be obtained for a three-phase machine with open-end windings following the pattern of the circuit given in Fig. 4.12, and shown in Fig. 4.29. This is an open-end winding motor drive system, which requires access to six terminals of the machine. A four-level voltage appears in each phase of the machine.
  • 133. 4.11 FIVE-LEVEL CONFIGURATION 119 R L q1a Vdc1 Vdc2 a 0 b Vdc3 Vdc4 q2a q3a q1a q2a q3a q1b q2b q3b q1b q2b q3b (a) 200 0 0.2 0.225 0.25 –200 200 0 –200 500 0 –500 100 0 –100 vo vb0 va0 io (b) Figure 4.26 (a) Four-level NPC full-bridge converter. (b) (from top to bottom) pole voltage 𝑣a0, pole voltage 𝑣b0, load voltage, and load current. 4.11 FIVE-LEVEL CONFIGURATION Following the same approach presented before for the three- and four-level configura- tions, the five-level converter is shown in Fig. 4.30(a). As done for the previous NPC topologies. Notice that just two types of PBs are employed. Figure 4.30(b) shows the five-level configuration with the traditional representation, using switches. In addition to the capacitor voltage balancing problem, another challenge appears when the number of levels increases for an NPC topology. The blocking voltage for each clamping diode changes and it depends on its position in the circuit. The diode voltage can be written as 𝑣D = (N − 1 − x)(N − 1)−1 Vdc (4.29)
  • 134. 120 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION R L R L R + – L n q1a Vdc1 Vdc2 a 0 b Vdc3 Vdc4 q2a q3a q1a q2a q3a q1b q2b q3b q1b q2b q3b q1c q2c q3c q1c q2c q3c (a) 500 0 0.2 0.225 0.25 –500 500 0 –500 500 0 –500 100 0 –100 van vn0 va0 van ia ia (b) Figure 4.27 (a) Four-level three-phase NPC converter. (b) (from top to bottom) pole voltage, voltage between load NP and dc-link midpoint connection, load voltage, and load current. R L R L R L b c q1b q2b q3b q1b q2b q3b q1c q2c q3c q1c q2c q3c Vdc1 Vdc2 0 Vdc3 Vdc4 Figure 4.28 Half-bridge four-level three-phase NPC converter.
  • 135. 4.11 FIVE-LEVEL CONFIGURATION 121 q1a C1 C2 C3 C4 qc c b a a+ q2a q1a q2a q1b b+ q2b q1b q2b q1c c+ q2c q1c q2c qc qb qb qa Phase 1 Phase 2 Phase 3 Three-phase machine qa Figure 4.29 Four-level open-end motor drive system. (a) (b) 2 1 4 5 7 6 3 V1 V2 vo V3 V4 V5 q1 q2 q3 q4 q1 q2 q3 q4 Vdc1 Vdc2 Vdc3 0 Vdc4 Figure 4.30 Five-level NPC converter: (a) PB representation and (b) representation with switches.
  • 136. 122 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION (a) (b) V1 V2 vo V3 V4 V5 q1 q2 q3 q4 q1 q2 q3 q4 Vdc1 Vdc2 Vdc3 0 Vdc4 Figure 4.31 Five-level NPC converter with pyramid structure: (a) PB representation and (b) representation with switches. where N is the number of levels, x changes from 1 to N − 2 and Vdc is the dc-link voltage of the whole dc source. For high voltage applications, such different blocking voltage characteristics could bring up operational limits for the converter. To solve this problem and guarantee the same blocking voltages for all diodes, it is necessary to add more clamping diodes in series. By adding the first PB-dc shown in Fig. 4.31(a), it is possible to find a topology with the same blocking voltages for all diodes with a pyramid structure as proposed by Yuan and Barbi [14] and depicted in Fig. 4.31(b). Theoretically, the number of levels in an NPC topology can be increased as necessary, and to do so the PB-cc blocks must be stacked as in Fig. 4.32.
  • 137. 4.11 FIVE-LEVEL CONFIGURATION 123 3 1 2 1 3 5 4 2 1 3 5 7 6 4 2 (a) (b) (c) (d) Figure 4.32 Generation of the n-level NPC topologies: (a) three-level, (b) four-level, (c) five-level, and (d) n-level.
  • 138. 124 CHAPTER 4 NEUTRAL-POINT-CLAMPED CONFIGURATION 4.12 SUMMARY This chapter is dedicated to NPC configurations. Further details about NPC topolo- gies can be found in References from 1 to 14. The topologies are presented in a systematic way in the following sequence: (i) PBs connections obtained from the rules presented in Chapter 3; (ii) once the topology is established, the Table of Vari- ables is obtained; (iii) the next step is modeling the converter by writing the output voltage to describe what was obtained in the Table of Variables; and (iv) and finally the PWM approach is developed from the Table of Variables. The same systematic approach has been applied for both conventional and nonconventional topologies. More than bringing new possibilities for power electronics converters in differ- ent applications, nonconventional converters play an important role in the learning process and ensure a deep understanding of the subject. REFERENCES [1] Baker RH. Bridge converter circuit. US patent 4270163. 1981 May (filed in Aug. 79). [2] Nabae A, Takahashi I, Akagi H. A new neutral-point-clamped PWM inverter. IEEE Trans Ind Appl 1981;IA-17(5):518–523. [3] Steinke JK. Control of a neutral-point-clamped PWM inverter for high power AC traction drives. Int’l Conf on Power Electron and Variable-Speed Drives on; 1988 Jul 13–15. p 214–217. [4] Holtz J. Self-commutated inverters with a stepped output-voltage waveform suitable for high powers and frequencies. Siemens Forsch-U Entwick1-Ber 1977;6(3):164–171. [5] Carrara G, Gardella S, Marchesoni M, Salutari R, Sciutto G. A new multilevel PWM method: a theoretical analysis. IEEE Trans Power Electron 1992;7:497–505. [6] Lin B-R, Wei T-C. Space vector modulation strategy for an eight-switch three-phase NPC converter. IEEE Trans Aerosp Electron Syst 2004;40(2):553–566. [7] Holmes DG, Lipo TA. Pulse Width Modulation for Power Converters. Piscataway: IEEE/Wiley Inter- science; 2003. [8] E. C. dos Santos Jr., Muniz JHG, and da Silva ERC. 2L3L inverter. Proc of Brazilian Power Electron Conf (COBEP); 2011, p 924–929 [9] Mihalache L. A hybrid 2/3 level converter with the minimum switch count. Industry Applications Conference. 41st IAS Annual Meeting. Conference Record of the 2006 IEEE; 2006; vol. 2. p 611–618. [10] da Silva ER, Muniz JG, da Nobrega RB, dos Santos Jr. EC. An improved pulse-width-modulation for the modified hybrid 2/3-level converter. Proc of Brazilian Power Electron Conf (COBEP); 2013, p 248–253. [11] Choi NS, Cho JG, Cho GH. A general circuit topology of multilevel inverter. Proc. Rec. IEEE PESC; 1991. p 96–103. [12] Carpita M, Tenconi S. A novel multilevel structure for voltage source inverter. Proc. Rec. EPE Conf.; 1991. p 1.90–1.94. [13] Hammond PW. Medium voltage PWM drive and method. US patent 5,625,545. 1997. [14] Yuan X, Barbi I. A new diode clamping multilevel inverter. Proceedings of APEC99; 1999. p 495–501.
  • 139. CHAPTER 5 CASCADE CONFIGURATION 5.1 INTRODUCTION The PBG is employed in this chapter to describe the cascade multilevel configura- tions, also known as H-bridge series connected configurations. The introduction and fundamental concepts are furnished for a single H-bridge topology, followed by the connection of other H-bridge converters for generation of topologies with more lev- els. Such configurations deal with attractive characteristics common for multilevel circuits, such as low electromagnetic interference (EMI), reduced total harmonic dis- tortion and high relationship between the number of levels per number of switches. Comparing this multilevel configuration with the neutral point clamped (NPC) topol- ogy described earlier, it is possible to sort some advantages such as (i) simple pack- aging and physical structure with no neutral point clamping circuits, (ii) modular structure (more or fewer H-bridge cells can be cascaded depending on the desired power quality), and (iii) possibility to operate even with partial failure. On the other hand, the main disadvantages are associated with (i) greater number of dc sources and (ii) control complexity. The previous chapter was organized with the sections divided in terms of the number of levels of the converter, that is, three levels, four levels, and so on. In this chapter, on the other hand, the organization (labeling scheme) of the sections considers the number of H-bridge converters instead of number of levels. The main reason for that is, depending on the values of the dc voltage sources and modulation approach, the same topology can generate different number of levels. Accordingly, Section 5.2 presents the description of a single H-bridge converter along with its Table of Variables. The pulse width modulation (PWM) implementa- tion is derived from the Table of Variables, as highlighted in Section 5.3. The fol- lowing section presents the three-phase version with a single H-bridge converter per phase. Sections 5.5, 5.6, and 5.7 deal with two H-bridge converters in series, with the sequence given respectively by power converter construction, PWM approach, and three-phase version. After showing how it is possible to guarantee post-fault oper- ation with this type of converter in Section 5.7, Section 5.8 demonstrates that two H-bridge converters can be employed to generate an output voltage with either seven or nine levels, by employing the correct relationship between the dc-link voltages. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 125
  • 140. 126 CHAPTER 5 CASCADE CONFIGURATION V1 V2 (a) (b) (c) (d) vo V1 V2 vo V1 V2 vo V1 V2 vo Figure 5.1 (a) One H-bridge configuration with PBs. (b) 𝑣o = V1 − V2. (c) 𝑣o = V2 − V1. (d) 𝑣o = 0. Section 5.9 presents different arrangements and PWM solutions for three H-bridge converters connected in series. Finally, Section 5.10 introduces the generalization and other possible converters characterized by series arrangements of H-bridge circuits. This chapter has been written with the help of References from 1 to 14. 5.2 SINGLE H-BRIDGE CONVERTER Considering the power blocks (PBs), no connection is needed among PBs to obtain an H-bridge topology, since there is a block that represents this converter directly, as observed in Fig. 5.1(a). Figure 5.1(b), 5.1(c) and 5.1(d) illustrates the methods used to obtain three levels at the output converter side (V1 − V2, V2 − V1, 0). In general terms, to generate an output waveform with three levels as in Fig. 5.2 (bot- tom), it is necessary to activate the PBs in a sequence as observed in this figure (top). Notice that instead of selecting one of the input voltages V1, V2, and V3 as done for the NPC topology considered in the previous chapter, the three-level output voltage in Fig. 5.2 is a combination of two voltages V1 and V2 available at the input converter side. Despite the three-level voltage in Fig. 5.2, it is convenient to start the analysis of the cascade multilevel topologies by assuming just two levels (V1 − V2, V2 − V1) at the output converter side, as in Fig. 5.1(b) and 5.1(c). Since 𝑣o can assume just one combination of the input voltages each time, it is reasonable to write an equation to describe the output voltage 𝑣o as a function of both input voltages and an independent binary variable. As the number of input voltages to be selected is two, the minimum number of binary control variable is one. This binary variable should be used to select one combination of the inputs to appear at the output converter side, which means that one possible solution to achieve this goal is given in Table 5.1. From q1 and its complementary signal q1 = 1 − q1, the output voltage can be obtained as follows: 𝑣o = q1(V1 − V2) + q1(V2 − V1) (5.1)
  • 141. 5.2 SINGLE H-BRIDGE CONVERTER 127 V1 V1 – V2 V2 – V1 t 0 V2 vo vo V1 V2 vo V1 V2 vo Figure 5.2 General three-level output voltage. TABLE 5.1 Converter in Fig. 5.1(a) Operating as a Two-Level Converter State q1 𝑣o 1 1 V1 − V2 2 0 V2 − V1 If V1 − V2 = Vdc, then (5.1) can be written as follows: 𝑣o = (2q1 − 1)Vdc (5.2) As seen in the previous chapter, these control variables (q1 and q1) are in fact the states of the switches inside the blocks. Comparing Table 5.1 with Fig. 5.2 (bottom) it is evident that just one binary control variable (q1) and its complementary signal (q1) are not enough to select three levels at the output converter side. If the number of levels for the output voltage is expected to be three (±Vdc,0), the minimum number of binary variables in this case should be two, which are used to select a desired output voltage, meaning that one possible combination to achieve this goal is given in Table 5.2. The output voltage can be written as 𝑣o = −q1q2Vdc + q2q1Vdc (5.3) where q2 = 1 − q2. Substituting the complementary variables, the previous equation becomes 𝑣o = −(1 − q1)q2Vdc + (1 − q2)q1Vdc (5.4) 𝑣o = (q1 − q2)Vdc (5.5)
  • 142. 128 CHAPTER 5 CASCADE CONFIGURATION TABLE 5.2 Converter in Fig. 5.1(a) Operating as a Three-Level Converter State q1 q2 𝑣o 1 0 0 0 2 0 1 −Vdc 3 1 0 Vdc 4 1 1 0 Figure 3.10 shows the same configuration presented in Fig. 5.1, along with binary variables describing the state of the switches for positive and negative output currents (io). Notice that there is no restriction in terms of state of the switches and the values of currents, which means that each voltage value can be obtained at the output converter independent of the current values (io > 0 and io < 0). Example 5.1 Considering the previous analysis, place each switch (q1, q1, q2, and q2) in the correct position in the following circuit to guarantee the generation of the levels as shown in Table 5.2. Vdc Position 1 + – Position 3 Position 2 Position 4 vo Solution For the generation of a voltage 𝑣o with three levels, as in Table 5.2, q1 should be placed, for example, in position 2, while q2 should be placed in position 1. Consequently q1 and q2 should be placed in positions 4 and 3, respectively.
  • 143. 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 129 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER If a single H-bridge converter is operating with two or three levels independently, the ultimate control goal is to guarantee a regulated voltage at its output side. The output voltage is regulated in terms of amplitude and frequency, obtained through PWM strategies. Many works in the technical literature have proposed solutions in terms of modulation approach applied to cascade converters. A simple sinusoidal carrier-based PWM strategy is considered in this chapter. Figure 5.3 shows an analog solution for implementation of PWM, in which the states of the four switches are determined by a comparison between one high frequency triangular waveform (𝑣∗ t ) and a sinusoidal waveform (𝑣∗ sin ). Note that this modulation strategy generates the waveforms with two levels as seen in Table 5.1. In Fig. 5.3(a) (top) the same gating signals are sent to q1 and q2, while the same complementary signals are sent to q2 and q1, which implies that the pair of switches q1 − q2 and q2 − q1 are always turned on and off simultaneously. Figure 5.3(a) (bot- tom) shows the power part of the converter, and Fig. 5.3(b) shows the waveforms of the PWM and gating signals. While Fig. 5.4(a) shows an H-bridge converter supplying a single-phase RL load, Fig. 5.4(b) shows (from top to bottom) PWM reference waveforms (𝑣∗ sin and 𝑣∗ t ), gating signal of switch q1, gating signal of switch q2, load voltage and load current, respectively. The parameters employed in these simulation results were Vdc = 200V, R = 5Ω, and L = 5mH, and switching frequency was equal to 1000Hz. These same parameters have been used for other simulation outcomes in this chapter. The modulation strategy presented in Figs 5.3 and 5.4 seems to have low prac- tical interest due to a two-level voltage generation, which means reduced THD as compared to the three-level option. However, it permits applicability in photovoltaic systems due to common mode voltage and current reduction. As indicated by Fig. 5.2 and Table 5.2, an H-bridge converter is also able to generate a three-level voltage by just changing the PWM control signals. Figure 5.5 shows two PWM approaches used to control the H-bridge converter. A direct comparison between the results obtained in Fig. 5.5 highlights some advan- tages and drawbacks for each method used to generate three levels at the output converter side. For instance, with two high frequency waveforms (𝑣∗ t1 and 𝑣∗ t2 ) [see Fig. 5.5(a) and 5.5(c) – Method 1] it is possible to operate the converter with reduced power converter losses, since one leg will modulate (turning the switches on and off) while the other one will be clamped. Method 1 is also known as level-shift PWM strat- egy. On the other hand, the operation with one high frequency waveform (𝑣∗ t ) and two modulating signals (𝑣∗ sin 1 and 𝑣∗ sin 2 ) [see Fig. 5.5(b) and 5.5(d) – Method 2] guaran- tees lower harmonic distortion, which can be verified by the reduced current ripple. In this case, both legs modulate during the whole period of the sinusoidal waveforms; as a consequence, the harmonic content of the high frequency components is twice that of the switching frequency. In Method 1 [Fig. 5.5(a) and 5.5(c)] just two states in Table 5.2 are employed per half of the sinusoidal period, that is, states 1 and 3 for the positive half of the
  • 144. 130 CHAPTER 5 CASCADE CONFIGURATION driver driver + – q1 q2 q1 q2 q1 q2 q2 q1 q1 q2 vsin * vt2 * vsin * vt * (a) 1 1 –1 0 0 1 1 1.025 1.05 0 (b) Figure 5.3 (a) PWM generation for switches q1, q2, q1, and q2. (b). (from top to bottom) – reference voltages, gating signal of switch q1, and gating signal of switch q2. sine, and states 1 and 2 for the negative half of the sine. In this method, state 4 with both switches on is never employed. On the other hand, in Method 2 all states are employed. Figures 5.4 and 5.5 highlight that the same average voltage and consequently the same amplitude (in terms of average values) of the load current is obtained at the output converter side, independent of the modulation strategies employed. The frequency-domain representation, using the Fourier transformation of the output voltage, is an important tool to understand the differences between the PWM strategies in Fig. 5.5. Figure 5.6(a) and 5.6(b) shows the waveforms presented in Fig. 5.5, with both time- and frequency-domain for Methods 2 and 1, respectively. Notice that the pole
  • 145. 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 131 (a) q1 q2 vsin * vo io vt * 1 1 –1 0 0 1 1 1.025 1.05 0 200 –200 50 –50 (b) q1 q2 R + – L q2 2 1 0 q1 io vo Vdc 2 Vdc 2 Figure 5.4 (a) Two-level H-bridge converter. (b) (from top to bottom) 𝑣∗ sin , 𝑣∗ t ; gating signal of switch q1; gating signal of switch q2; load voltage and load current. voltages for Method 2 have two main frequency components, that is, one related to the sinusoidal and another related to the triangular waveform. Since 𝑣o = 𝑣10 − 𝑣20 and there is just one triangular waveform, such a frequency component is cancelled for 𝑣o. Although not shown in this figure, there are higher frequency components. On the other hand, there are two sinusoidal waveforms with phase shift equal to 180∘ for Method 2, which explains why the amplitude of the sine frequency component for 𝑣o is twice that for 𝑣10 and 𝑣20. Such a characteristic also explains the higher switching frequency observed for 𝑣o in the time domain. For Method 1 [Fig. 5.6(b)], each pole voltage has dc components that are cancelled for 𝑣o, but the triangular frequency com- ponents are not cancelled. Since this waveform was obtained by employing different carrier signals, it is clear why the switching frequency components for 𝑣o in Method 1 are equal to the switching frequency component observed in the pole voltages. Exercise 5.1 Determine all topological states (equivalent circuits) for the switching states in both strategies presented in Fig. 5.5. Assume both positive and negative currents.
  • 146. 132 CHAPTER 5 CASCADE CONFIGURATION driver driver driver driver + – + – q1 q1 q2 q2 q1 q1 q2 q2 vsin * vt1 * vt1 * v10 v20 vo io vt2 * vt2 * driver driver driver driver + – + – q1 q1 q2 q2 q1 q1 q2 q2 vsin1 * vsin * vsin2 * vt * (a) (b) 1 –1 100 –100 100 –100 200 –200 50 –50 1 1.025 1.05 0 vt * v10 v20 vo io vsin1 * vsin2 * 1 –1 100 –100 100 –100 200 –200 50 –50 1 1.025 1.05 0 (c) (d) Figure 5.5 PWM strategy: (a) Method 1 and (b) Method 2. (c) Waveforms for method 1: (from top to bottom) 𝑣∗ sin , 𝑣∗ t1 , and 𝑣∗ t2 ; pole voltage 𝑣10; pole voltage 𝑣20, load voltage 𝑣o; and load current io. (d) Waveforms for method 2: (from top to bottom) 𝑣∗ sin 1 , 𝑣∗ sin 2 , and 𝑣∗ t ; pole voltage 𝑣10; pole voltage 𝑣20, load voltage 𝑣o; and load current io.
  • 147. 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 133 (a) (b) v10 Time domain v20 Time domain v10 Frequency domain Sine freq. Triangular freq. Sine frequency Sine frequency Triangular frequency Frequency domain Time domain Frequency domain v20 vo v10 Time domain v20 Time domain v10 Frequency domain Sine frequency Triangular frequency Sine frequency Sine frequency Triangular frequency Triangular frequency Frequency domain Time domain Frequency domain v20 vo vo vo Figure 5.6 Waveforms for time and frequency domains for: (a) Method 2 and (b) Method 1. In general terms, for a PWM strategy obtained from a comparison between sinusoidal and triangular waveforms as presented in Figs 5.3 and 5.5(b), the peak amplitude of the fundamental component for the pole voltage V10(1) [see equation (2.10)] is given by V10(1) = V∗ sin Vt Vdc 2 = ma Vdc 2 (5.6)
  • 148. 134 CHAPTER 5 CASCADE CONFIGURATION It turns out that the fundamental component can be written by 𝑣10(1)(t) = ma(Vdc∕2) sin(𝜔t) with ma ≤ 1. The harmonic components can be calculated using the Fourier series as follows: 𝑣10(t) = V10(0) + ∞ ∑ h=1 𝑣10(h)(t) (5.7) with ∞ ∑ h=1 𝑣10(h)(t) = ∞ ∑ h=1 {ah cos(h𝜔t) + bh sin(h𝜔t)}. Note that ah are the cosine components in the Fourier series, while bh are the sine components, see equations (2.1)–(2.3). Indeed the harmonic for the pole voltage comes out as side-bands centered on the switching frequency and its multiples. The figure below shows the amplitude of the normalized harmonic component V10(h)∕(Vdc∕2) versus the harmonics, obtained from equation (5.6) for three values of modulation indexes: ma = 1, 0.6, and 0.4, and with mf > 21 for all cases. 1 1 0.02 0.03 0.03 0.13 1.00 0.13 0.07 0.37 0.37 0.07 0.04 0.04 0.08 0.20 0.20 0 0 0.06 0.06 0.02 0.02 0.01 0.01 0.12 0.13 0.13 0.32 0.32 1.15 0.40 0 0 0 0 0 0 0 0 0 0 0.04 0.15 0.11 0.15 0.06 0.06 0.04 Harmonic mf–4 2mf–5 2mf+5 2mf+3 2mf–3 2mf+1 3mf+4 3mf–4 3mf–6 3mf+6 3mf–2 3mf+2 3mf 2mf–1 mf+4 mf–2 mf+2 ma=1.0 mf>21 ma=0.6 mf>21 ma=0.4 mf>21 mf 1 Harmonic mf–4 2mf–5 2mf+5 2mf+3 2mf–3 2mf+1 3mf+4 3mf–4 3mf–6 3mf+6 3mf–2 3mf+2 3mf 2mf–1 mf+4 mf–2 mf+2 mf 1 Harmonic mf–4 2mf–5 2mf+5 2mf+3 2mf–3 2mf+1 3mf+4 3mf–4 3mf–6 3mf+6 3mf–2 3mf+2 3mf 2mf–1 mf+4 mf–2 mf+2 mf 0.02 0.32 0.32 0.21 0.21 0.18 0.18 0.60 0.60 v10 v10 v10 It can be seen from this figure that the pole voltage has an interesting charac- teristic, that is, there is only odd harmonics. The even harmonics disappear if mf is an odd integer bigger than 9. This is due to odd symmetry with 𝑣10(−t) = −𝑣10(t). Also, the ah (cosine elements in the Fourier series) are equal to zero, while the terms bh (sine elements) can be different from zero.
  • 149. 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 135 The pole voltage is plotted below to demonstrate the effect of an even value for mf as compared to an odd one. Note that when mf = 8, an asymmetric waveform is obtained at the pole voltage, since the comparison of the peaks and valleys of the sinusoidal voltage along with the triangular one is different. On the other hand, when mf = 9 (an odd number for mf ) a symmetric waveform is obtained since the comparison is symmetric for all periods, as highlighted in the peaks and valleys. • ma = 0.9 and mf = 8 vsin * vt v10 Asymmetrical waveform ma = 0.9 and mf = 8 • ma = 0.9 and mf = 9 vsin * vt v10 Symmetrical waveform ma = 0.9 and mf = 9 Other harmonic component elimination can be obtained when both sinusoidal (𝑣∗ sin ) and triangular (𝑣t) waveforms are synchronized for mf < 21. If mf > 21, no synchronization is needed due to low gain. Application (Photovoltaic Systems) A typical photovoltaic (PV) power system is composed of a set of PV arrays with one central inverter, which can be implemented transformerless or with an isolated trans- former as shown below. The last solution is sometimes avoided due to size, weight, and price of the low frequency transformer.
  • 150. 136 CHAPTER 5 CASCADE CONFIGURATION Inverter 1 2 PV arrays Transformerless Utility grid Due to high frequency on the inverter, a common mode voltage (𝑣CM ) is gener- ated with respect to the ground, which will induce a circulating current between the PV panels and the grid through the inverter. Notice that such a current does not exist when a transformer is used. Due to safety requirements the PV module frame is connected to the ground, as represented in figure below (left side). Since the panels have a planar structure and module glass, it results in capacitance to the ground. In fact, the individual PV cells have distributed stray capacitance to the ground, as depicted in the middle of the figure below. The distributed capacitance throughout the module can be characterized by an equivalent lumped capacitance highlighted in the right figure below. PV panel Individual PV cell CPV CPV PV Panel PV panel Distributed stray capacitance Lumped stray capacitance P(+) P(+) P(+) N(–) N(–) N(–) Assuming this equivalent circuit for the PV along with the stray capacitances, it is possible to obtain the circuit below (top). Without an isolated transformer there is a galvanic connection between the grid and PV arrays represented in this figure by the circulating current iLeakage. The bottom-left-side figure below shows a simplification of this circuit with a block representing the panels and the inverter. In this case,
  • 151. 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 137 for simplification purposes, just one CPV is considered between the point N and the ground. If an H-bridge topology (bottom-right-side figure below) is chosen to implement the grid-tie inverter, it is possible to define two voltages as function of 𝑣1N = q1VPN and 𝑣2N = q2VPN as follows: • Differential voltage: 𝑣DM = 𝑣1N − 𝑣2N; • Common mode voltage: 𝑣CM = (𝑣1N + 𝑣2N)∕2. Dc-link capacitances P P q1 q2 L1 L2 L1 L2 1 1 2 2 1 2 Grid-tie Inverter PV array + inverter CPV CPV CPV N N N Stray capacitance iLeakage iLeakage Using both voltages 𝑣DM and 𝑣CM it is possible to model the block describing PV array + Inverter above with the circuit presented below. PV array + inverter L1 L2 1 2 CPV vCM –vDM/2 vDM/2 N iLeakage
  • 152. 138 CHAPTER 5 CASCADE CONFIGURATION As observed in the figures above, the leakage current varies particularly with 𝑣CM, or by using other words, iLeakage is a function of the common mode voltage given by 𝑣CM = (q1 + q2)VPN∕2. From the Table presented in the sequence, it is quite clear that if the modulation strategy selects only states 2 and 3, 𝑣CM is always equal to VPN∕2, which means constant voltage applied to the capacitor CPV and consequently null circulating current (i.e., iLeakage = 0). The direct consequence of cancelling iCM is that the number of levels at the output converter side will be two, instead of three. See Table 5.1 as well as Fig. 5.3. State q1 q2 𝑣CM 1 0 0 0 2 0 1 VPN∕2 3 1 0 VPN∕2 4 1 1 VPN Example 5.2 For the H-bridge topology shown in Fig. 5.4(a) with Vdc = 600V, ma = 0.6, switching frequency: 1950 Hz and 𝑣∗ sin = 180 sin(2𝜋50t), calculate the root mean square (RMS) values of the fundamental and most important harmonics (with at least 10% of the amplitude of the biggest harmonic) for the pole voltage 𝑣10 assuming Method 2 in Fig. 5.5. Solution The amplitude of the fundamental and harmonics can be obtained from the figure below that shows the relationship between V10(h)∕(Vdc∕2) and the har- monics. 0.13 1.00 0.13 0.07 0.37 0.37 0.07 0.04 0.04 0.08 0.20 0.20 0 0 0 0 0 0 ma=0.6 mf>21 1 Harmonic mf–4 2mf–5 2mf+5 2mf+3 2mf–3 2mf+1 3mf+4 3mf–4 3mf–6 3mf+6 3mf–2 3mf+2 3mf 2mf–1 mf+4 mf–2 mf+2 mf 0.60 v10 So, the amplitude of the harmonic hV10(h) is given by V10(h) = ( V10(h) Vdc∕2 ) Vdc 2 The RMS value can be obtained directly as follows: V10(h)RMS = 1 √ 2 ( V10(h) Vdc∕2 ) Vdc 2
  • 153. 5.3 PWM IMPLEMENTATION OF A SINGLE H-BRIDGE CONVERTER 139 Since ma = 0.6 and mf = ft∕fsin = 1950∕50 = 39, it is possible to write: h = 1 → V10(1)RMS = 1 √ 2 ⋅ 0.6 ⋅ 600 2 = 127V h = 39 → V10(39)RMS = 1 √ 2 ⋅ 1 ⋅ 600 2 = 212V h = 37, 41 → V10(37,41)RMS = 1 √ 2 ⋅ 0.13 ⋅ 600 2 = 27V h = 77, 79 → V10(77,79)RMS = 1 √ 2 ⋅ 0.37 ⋅ 600 2 = 78V h = 115, 119 → V10(115,119)RMS = 1 √ 2 ⋅ 0.2 ⋅ 600 2 = 42V All the other harmonics will not be considered since their amplitude is less than 10%. Example 5.3 Determine the RMS voltage value for the fundamental and for the harmonic number 39 of the output voltage assuming the conditions of the last example; assume both PWM strategies shown in Figs 5.4 and 5.5(b). Solution Since the output voltage of the PWM approach shown in Fig. 5.4 has the same shape of the pole voltage [see Fig. 5.4(b)] it is possible to keep using the tem- plate furnished in the figure V10(h) Vdc∕2 versus harmonics. However, the RMS values are given by Vo(h) = ( V10(h) Vdc∕2 ) Vdc h = 1 → Vo(1)RMS = 1 √ 2 ⋅ 0.6 ⋅ 600 = 254V h = 39 → Vo(39)RMS = 1 √ 2 ⋅ 1 ⋅ 600 = 424V On the other hand, for the PWM technique given in Fig. 5.5(b) the out- put voltage presents a different shape from the pole voltage, which means that it is possible to use the template in figure V10(h)∕(Vdc∕2) versus harmon- ics. Although 𝑣o has three levels instead of two, the fundamental component (h = 1) should be the same as for the PWM in Fig. 5.3 since in both cases the converter is operating under the same conditions in terms of Vdc, ma, and mf . Then: h = 1 → Vo(1)RMS = 254V. For the harmonic 39, it turns out that Vo(39)RMS = 0, [see Fig. 5.6(a)].
  • 154. 140 CHAPTER 5 CASCADE CONFIGURATION Exercise 5.2 Repeat Examples 5.1 and 5. with ma = 1.0 instead of 0.6. The other operation conditions are the same as in the previous examples. 5.4 THREE-PHASE CONVERTER—ONE H-BRIDGE CONVERTER PER PHASE A three-phase configuration by using one H-bridge converter per phase is depicted in Fig. 5.7(a). It is worth mentioning that both converter and three-phase load are con- nected in a Y arrangement. The converter pole voltages can be written as a function of the states of switches, as follows: 𝑣a0 = (q1a − q2a)Vdc (5.8) 𝑣b0 = (q1b − q2b)Vdc (5.9) 𝑣c0 = (q1c − q2c)Vdc (5.10) Considering a balanced three-phase system, it turns out that the voltage between the neutral of the load and the point “0” is given by 𝑣n0 = Vdc 3 (q1a − q2a + q1b − q2b + q1c − q2c) (5.11) Compiling equations (5.8)–(5.11), it is possible to write the load voltages 𝑣an, 𝑣bn, and 𝑣cn in a matrix representation, as shown below: ⎡ ⎢ ⎢ ⎣ 𝑣an 𝑣bn 𝑣cn ⎤ ⎥ ⎥ ⎦ = Vdc ⎡ ⎢ ⎢ ⎢ ⎢ ⎢ ⎢ ⎣ 2 3 −2 3 −1 3 −1 3 1 3 2 3 −1 3 1 3 −1 3 1 3 −1 3 1 3 −2 3 −1 3 1 3 1 3 2 3 −2 3 ⎤ ⎥ ⎥ ⎥ ⎥ ⎥ ⎥ ⎦ ⎡ ⎢ ⎢ ⎢ ⎢ ⎢ ⎢ ⎣ q1a q2a q1b q2b q1c q2c ⎤ ⎥ ⎥ ⎥ ⎥ ⎥ ⎥ ⎦ (5.12) The power converter constituted by the arrangement of H-bridges topologies, as in Fig. 5.7(a) allows different connections for the H-bridge converters. Such a characteristic is not observed for the converters shown in the previous chapter. In fact, for a given three-level NPC topology, different arrangements can be addressed for the load side with either Y or Δ connections of the three-phase load, but the connections of the converter itself cannot be changed, since all legs are connected to the same dc-link source. On the other hand, due to its modular feature, H-bridge converters can be changed in order to deal with specific requirements. In this sense, Fig. 5.7(b)
  • 155. 5.4 THREE-PHASE CONVERTER—ONE H-BRIDGE CONVERTER PER PHASE 141 q1a a b n L R L 0 (a) (b) R Vdc va0 vb0 vc0 van vbn c L R vcn vab q1a q2a q2a q1b q1b q2b q2b q1c q1c q2c q2c q1a n L R L R Vdc Vdc Vdc van vbn L R vcn q1a q2a q2a q1b q1b q2b q2b q1c q1c q2c q2c Figure 5.7 (a) Three-phase H-bridge configuration connected in a Y arrangement. (b) Three-phase H-bridge configuration connected in a Δ arrangement. shows a solution in which the converters are arranged in a Δ connection. There is also a possibility to connect a three-phase load in Δ for the converters depicted in Fig. 5.7(a) and 5.7(b). Exercise 5.3 Fill a table to show the number of levels of the load phase voltage 𝑣an for both topologies given in Fig. 5.7 as a function of the switching states. To highlight the influence of the PWM strategies presented in Fig. 5.5 (Methods 1 and 2) for the three-phase configuration as in Figs 5.7(a), 5.8(a), 5.8(b) show the waveforms related to Methods 1 and 2, respectively. In the three-phase case, the waveforms for the line-to-line voltage obtained through Method 1 have an interesting characteristic with the same d𝑣∕dt, while Method 2 presents a line-to-line voltage with the levels not well defined as in Fig. 5.8(a). As a conse- quence 𝑣an in Fig. 5.8(a) is closer to a sine waveform than in Fig. 5.8(b). Note that Fig. 5.8(c) highlights the advantages of Method 1 with a voltage presenting the same d𝑣∕dt.
  • 156. 142 CHAPTER 5 CASCADE CONFIGURATION va0 va0 vab vab van van ia ib ic vab vab ib ic –200 0 200 –200 0 200 –50 1 1.025 (a) (b) (c) 1.05 1 1.025 Method 1 Method 2 Same dv/dt Different dv/dt 1.05 0 50 –400 0 400 –200 0 200 –200 0 200 –50 0 50 –400 0 400 Figure 5.8 (from top to bottom) Voltages: 𝑣a0, 𝑣ab, and 𝑣an and load currents for (a) Method 1, (b) Method 2, and (c) levels of line-to-line voltage.
  • 157. 5.4 THREE-PHASE CONVERTER—ONE H-BRIDGE CONVERTER PER PHASE 143 As described in the previous chapter, there is a possibility to supply a three-phase load by using a converter able to supply only two phases, since the third phase will be indirectly controlled, due to the redundancy inherent in the balanced three-phase systems (ia + ib + ic = 0 and 𝑣a + 𝑣b + 𝑣c = 0). Exercise 5.4 Assuming all possibilities in terms of converter and three-phase load connec- tions as given in the table below, specify the switches of the converters in terms of voltage and current requirement, assuming the same RL load and dc-link voltage for all connections below. Also, disregard any safety margin while specifying the components. Converter Load Connection Connection Figure Y Y 5.7(a) Δ Y 5.7(b) Y Δ – Δ Δ – Figure 5.9(a) shows the configuration with only two H-bridges connected to phases a and b, while Fig. 5.9(b) shows the waveforms related to this configuration. This kind of topology seems to have low practical interest, but in a fault-tolerant system it could be interesting due to its ability to maintain the three-phase voltage applied to the load on the post-fault operation. In this scenario, the “healthy” config- uration is changed to the post-fault one after fault identification in the third phase of the converter. The PWM control of the configuration presented in Fig. 5.9(a) needs to be adapted. The amplitude of voltage applied to the load is reduced by √ 3 and its dis- tortion harmonic increased. However, the converter is still able to supply a three-phase load with balanced currents as in Fig. 5.9(b) with ia, ib, and ic having the same ampli- tude and a phase shift equal to 120∘. Exercise 5.5 Does the connection shown in Fig. 5.9 affect the number of levels of the load phase voltage? To answer this question, write a table to show the load voltages as a function of the switching states and compare with the results obtained in Exercise 5.3.
  • 158. 144 CHAPTER 5 CASCADE CONFIGURATION ia ib ic vcn vbn van 1 1.025 1.05 0 200 –200 0 200 –200 0 200 –200 50 0 –50 q1a R a b c L R L R L van vbn vcn Vdc q1a q2a q2a q1b q1b q2b q2b (a) (b) Figure 5.9 (a) Configuration supplying only two phases of the three-phase load. (b) (from top to bottom) 𝑣an, 𝑣bn, 𝑣cn, and load currents. 5.5 TWO H-BRIDGE CONVERTERS Connecting H-bridge converters in series, as in Fig. 5.10(a), allows the generation of voltage with a higher number of levels. Such a cascade converter is in fact a very popular topology in high voltage motor drive applications, especially due to its mod- ular characteristic. As discussed previously, each H-bridge converter can generate a maximum of three levels at its output, which means a maximum of nine levels at the output of two connected H-bridges series. All levels are considered in Table 5.3 for each switch- ing state. The levels are: {0, ±Va, ±Vb, −Va − Vb, −Va + Vb, Va − Vb, Va + Vb}. Figure 5.10(b)–5.10(j) show the combination used to obtain each specific level at the output converter side.
  • 159. 5.5 TWO H-BRIDGE CONVERTERS 145 va vb vo (a) va vb vo (b) va vb vo (c) va vb vo (d) va vb vo (e) va vb vo (f) va vb vo (g) va vb vo (h) va vb vo (i) va vb vo (j) Figure 5.10 (a) Two H-bridges configuration with PBs. (b) 𝑣o = Va + Vb. (c) 𝑣o = −Va − Vb. (d) 𝑣o = Va − Vb. (e) 𝑣o = −Va + Vb. (f) 𝑣o = Va. (g) 𝑣o = −Va. (h) 𝑣o = Vb. (i) 𝑣o = −Vb. (j) 𝑣o = 0. From the expression for the output voltage of one H-bridge converter given in (5.5), the output voltage 𝑣o of the converter presented in Fig. 5.10(a) can be written as a function of the binary variables presented in Table 5.3, as follows: 𝑣o = (q1a − q2a)Va + (q1b − q2b)Vb (5.13)
  • 160. 146 CHAPTER 5 CASCADE CONFIGURATION TABLE 5.3 Table of Variables for the Converter in Fig. 5.10 State q1a q2a q1b q2b 𝑣o 1 0 0 0 0 0 2 0 0 0 1 −Vb 3 0 0 1 0 Vb 4 0 0 1 1 0 5 0 1 0 0 −Va 6 0 1 0 1 −Va − Vb 7 0 1 1 0 −Va + Vb 8 0 1 1 1 −Va 9 1 0 0 0 Va 10 1 0 0 1 Va − Vb 11 1 0 1 0 Va + Vb 12 1 0 1 1 Va 13 1 1 0 0 0 14 1 1 0 1 −Vb 15 1 1 1 0 Vb 16 1 1 1 1 0 Although it is possible to generate nine levels at the output of the converter in Fig. 5.10, this section will start with the analysis to obtain five levels followed by seven and nine. Example 5.4 What should be the relationship between Va and Vb to reach the maximum nine levels (the maximum number of levels) at the output converter side? Solution To generate the maximum number of levels at the output converter side it is nec- essary to guarantee either V1 = 3V2 or V2 = 3V1. Other numbers of levels can be obtained with other relationships of the input voltages. For instance, seven levels is obtained with V1 = 2V2 or V2 = 2V1, while five levels is obtained with V1 = V2. 5.6 PWM IMPLEMENTATION OF TWO CASCADE H-BRIDGES PWM control strategies are also employed for a converter with two cascade H-bridge topology to guarantee controlled voltage and frequency at its output. Since there
  • 161. 5.6 PWM IMPLEMENTATION OF TWO CASCADE H-BRIDGES 147 are more switches to generate the desired output voltage as compared to the single H-bridge topology, it is also expected to have ways to implement the PWM strategies. This section explores some of these PWM approaches. Figure 5.11 shows the analog solution with phase shift multicarrier modulation technique, in which the states of the eight switches are determined by a comparison between two high frequency triangular waveforms (𝑣∗ t1 and 𝑣∗ t2 , carrier signals) and two sinusoidal waveforms (𝑣∗ sin and −𝑣∗ sin , control signals) for the case where Va = Vb = Vdc. The voltages 𝑣∗ t1 and 𝑣∗ t2 are shifted by 90∘. In this case the converter is able to generate a five-level waveform at its output. As mentioned previously, the (a) (b) driver driver driver driver 90° Phase shift driver driver driver driver + – + + + 1 0 –1 200 0 –200 – – – q1a q1a q2a q2a q1a q1a q2a q2a q1b q1b q2b q2b q1b q1b q2b q2b vsin * vsin * vsin * –vsin * –vsin * vo vt1 * vt1 * vt2 * vt2 * (a) Figure 5.11 (a) PWM strategy with phase-shift method. (b) (top) PWM waveforms and (bottom) output converter voltage.
  • 162. 148 CHAPTER 5 CASCADE CONFIGURATION block named driver must guarantee the levels of voltage and current needed to operate (turning on and off) the power switches adequately, as well as isolate the control (signal) and the power circuits. It is evident that the phase shift between 𝑣∗ t1 and 𝑣∗ t2 plays an important role in the PWM approach as in Fig. 5.11. In fact, the influence of this parameter is depicted in Fig. 5.12, which shows triangular (𝑣∗ t1 and 𝑣∗ t2 ) and sinusoidal (𝑣∗ sin ) voltages (top); load voltage (middle); and load current (bottom). The parameters employed in these simulation results were: input voltage – Va = 100V and Vb = 100V; load – R = 5Ω and L = 5mH; and switching frequency – 1kHz. Figure 5.12(a) shows those vari- ables with phase shift between 𝑣∗ t1 and 𝑣∗ t2 equal to 0∘. Other phase shifts are consid- ered, that is, 45∘, 90∘, and 180∘, as in Fig. 5.12(b), 5.12(c) and 5.12(d), respectively. Considering the waveforms of the load voltage and load current, it is evident that 90∘ reduces the harmonic distortion for both voltage and current. Although changing the high frequency components and consequently the THD of the variables, the phase shift does not influence the value of voltage applied to the load. In fact, the phase angle displacement of 90∘ between 𝑣∗ t1 and 𝑣∗ t2 guarantees an optimum output voltage because it generates a sequence of switching states with the (a) (b) (c) (d) 1 –1 200 0 –200 50 0 –50 0 1 –1 200 0 –200 50 0 –50 0 1 –1 200 0 –200 50 0 –50 0 1 –1 200 0 –200 50 0 –50 0 Figure 5.12 Triangular (𝑣∗ t1 , 𝑣∗ t2 ) and sinusoidal (𝑣∗ sin ) waveforms (top); load voltage (middle); and load current (bottom): with phase shift of (a) 0∘, (b) 45∘, (c) 90∘, and (d) 180∘.
  • 163. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 149 vsin * –vsin * vt2 * vt1 * 2Vdc State 11 State 11 State 3 State 9 State 15 State 12 State 11 State 11 State 11 Vdc Figure 5.13 Switching states when 𝑣∗ sin is in its peak with 90∘of the phase displacement between 𝑣∗ t1 and 𝑣∗ t2 . levels well defined as in Fig. 5.8. For instance, during the peaks it is expected that the output voltages change from Vdc to 2Vdc, while during the valleys the voltages should change from −2Vdc to −Vdc. Figure 5.13 shows the sequence of the switching states when 𝑣∗ sin is around its peak. Since Va = Vb = Vdc, States 3, 9, 15, and 12 in Table 5.3 generate the same output voltage equal to Vdc. On the other hand, there is only one way to generate 2Vdc, which is through State 11. Note that any other phase shift will generate a sequence different from the one in Fig. 5.13. Another way to implement the PWM strategy for the converter employing two H-bridge cells in series is presented in Fig. 5.14. Such a technique is called level-shift (or level dispositions), where all carrier signals are in phase but with different offsets. For a symmetrical (same dc-link voltages) cascade multilevel converter, the quantity of the carrier signals is defined by the number of levels desired at the output converter side, that is, for N levels (N − 1) triangular carriers are required. Figure 5.15 shows a comparison between two-level shift PWM approaches. Note that other outcomes are obtained when all triangular carriers have the same peak-to-peak voltage, but there is a phase shift of 180∘ between any two adjacent carrier waves. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE A three-phase configuration employing two H-bridge converters per phase is depicted in Fig. 5.16(a), with both converter and load connected in a Y arrangement. The waveforms associated with this configuration are depicted in Fig. 5.16(b). These load voltages present high quality with reduced THD due to the high number of levels. The PWM strategy employed in the results of Fig. 5.16 were obtained with the level shift approach, as in Fig. 5.14. The converter voltages can be written as a function of the states of switches, as follows: 𝑣a0 = (q1a − q2a + q3a − q4a)Vdc (5.14) 𝑣b0 = (q1b − q2b + q3b − q4b)Vdc (5.15)
  • 164. 150 CHAPTER 5 CASCADE CONFIGURATION driver driver driver driver + – + – q1a q1a q1a q1a q2a q2a q2a q2a driver driver driver driver q1b q1b q1b q1b q2b q2b q2b q2b vsin * vt1 * vsin * vo vt2 * vt3 * vt4 * + – + – (a) (b) 1 –1 100 0 –200 0 Figure 5.14 (a) PWM strategy with phase disposition (PD) method. (b) (top) PWM waveforms and (bottom) output converter voltage. 𝑣c0 = (q1c − q2c + q3c − q4c)Vdc (5.16) Considering a balanced three-phase system, the voltage between the neutral of the load “n” and the point “0” is given by 𝑣n0 = Vdc 3 c ∑ x=a (q1x − q2x + q3x − q4x) (5.17)
  • 165. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 151 (a) (b) 50 0 1 1.016 0 200 –200 0 1 –1 –50 50 0 1 1.016 0 200 –200 0 1 –1 –50 Figure 5.15 Comparison between two-level shift PWM techniques. Compiling equations (5.14)–(5.17), and assuming a balanced scenario, it is possible to write the load voltages 𝑣an, 𝑣bn, and 𝑣cn as a function of both switching states and dc-link voltages. As mentioned previously, one of the main advantages of the cascade configura- tions is their modularity, which brings benefits in terms of fault tolerance capability. The fault compensation is achieved by reconfiguring the power converter topology to keep the system in operation, even with a different number of H-bridges per phase. Figure 5.17(a) shows one phase of the three-phase converter as in Fig. 5.16(a) under “healthy” operation and generating a five-level voltage at the output. For the sake of illustration, let us assume that a fault occurs in the switch q1a, as highlighted in Fig. 5.17(b). Such a fault can be characterized as either a permanent short-circuit [see Fig. 5.17(c)] or a permanent open-circuit [see Fig. 5.17(d)]. The fault detection sys- tem must be able to identify where the fault has occurred (determining which switch is at fault), and also the type of fault (short- or open-circuit). Sometimes it is necessary to use fuses to deal with the reconfiguration of the power converter, which will help to isolate part of converter under fault. For simplification purposes, the fuse devices are not presented in Fig. 5.17. The first action to be taken for a short-circuit failure [Fig. 5.17(c)] in the switch q1a is to keep the complementary switch q1a open. As a consequence, the voltage generated at the output of this H-bridge converter 𝑣1a2a = 𝑣1a − 𝑣2a can assume only two values 0 or Vdc, that is, 𝑣1a2a = {0, Vdc}. Another scenario is with an open-circuit failure as shown in Fig. 5.17(d). In this case, the complementary switch q1a must be on to avoid current discontinuity. Consequently, the voltage generated at the output of this H-bridge converter can also assume only two values, that is, 𝑣1a2a = {0, −Vdc}. Both cases of failure lead to a voltage generation at the output of the H-bridge under fault with just one polarity: positive polarity {0, Vdc} for short-circuit failure and neg- ative polarity {0, −Vdc} for open-circuit failure. This represents a restriction for the amount of voltage generated by the phase under fault. However, a sinusoidal voltage with smaller amplitude and only three levels {0, ±Vdc} can still be generated by these two H-bridge converters in series. Although the faults presented in Fig. 5.17, there are some failures that damage the whole H-bridge converter. For example, it is quite common to have
  • 166. 152 CHAPTER 5 CASCADE CONFIGURATION (a) q1a q1a Vdc Vdc q2a q2a q3a q3a q4a q4a q1b q1b Vdc Vdc a b c L R L n R L R q2b q2b q3b q3b q4b q4b q1c q1c Vdc Vdc q2c q2c q3c q3c q4c q4c van vbn vcn (b) 200 –200 0 200 –200 0 200 –200 0 50 –50 0 1 1.025 1.05 van vbn vcn ia ib ic Figure 5.16 (a) Three-phase H-bridge configuration connected in a Y arrangement (b) Voltages and currents.
  • 167. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 153 (a) (b) (c) (d) q1a q1a 2a 1a a 0 Vdc Vdc q2a q2a q3a q3a q4a q4a q1a q1a 2a 1a a Permanent short-circuit Permanent short-circuit 0 Vdc Vdc q2a q2a q3a q3a q4a q4a q1a q1a 2a 1a a 0 + – Vdc Vdc q2a q2a q3a q3a q4a q4a v1a2a q1a q1a 2a 1a a 0 + – Vdc Vdc q2a q2a q3a q3a q4a q4a v1a2a Figure 5.17 (a) “Healthy” operation for the leg of the cascade topology. (b) Fault occurring in the switch q1a. (c) Short-circuit type of fault. (d) Open-circuit type of fault.
  • 168. 154 CHAPTER 5 CASCADE CONFIGURATION two switches inserted in the same package constituting a leg, and likely one switch will be affected if a malfunction has happened to another switch in the same leg. Another example of malfunction that deteriorates the whole H-bridge cell (in terms of capacity to generate any voltage) is when a fault occurs in the dc-link. There is no way to generate any desired voltage at the output of any H-bridge without dc-link voltage. The fault compensation when the entire H-bridge is suffering from a fault is achieved by reconfiguring the power converter topology along with additional devices, such as triacs, as shown in Fig. 5.18(a). The triacs t1 and t2 are open under “healthy” operation and must be turned on if a fault is detected, to isolate the whole H-bridge under fault. Figure 5.18(b) shows the post-fault topology with the H-bridge converter isolated by using the triac t1. The post-fault operation requires a new PWM approach to keep a set of bal- anced three-phase voltages applied to the load. There exist different ways to generate the PWM signals for the post-fault topology as in Fig. 5.18(b), since there are two converters per phase (in phases b and c) and just one converter in the phase a to synthe- size the desire three-phase load voltage. One possibility to maintain the three-phase balanced voltage is to turn on the triacs t3 and t5 to make this topology equal to that presented in Fig. 5.7(a). This means that the two H-bridge per phase configuration will be changed to a single H-bridge per phase. Also the rated voltage is reduced to half of the pre-fault operation. Another possibility is to keep the post-fault topology as presented in Fig. 5.18(b), that is, phase a with one H-bridge and phases b and c with two H-bridges. To guarantee a balanced three-phase voltage among the phases, the modulation index for phases b and c should be reduced to 50% of the modulation index employed for phase a. Exercise 5.6 Determine the number of levels of the post-fault topology in Fig. 5.18(b) con- sidering the case in which the modulation index for phases b and c is reduced by 50%. As done before, the connection of the converters can be changed in order to deal with specific requirements of the load. For instance, Fig. 5.19 shows a solution in which the converters are arranged in a Δ connection. There is also a possibility to connect a three-phase load in the Δ connection. If the three-phase load is an electrical machine, it is also possible to connect this machine with an open-end winding arrangement as seen in Fig. 5.20. Open-end winding motor structure is obtained by opening the neutral point of the conventional induction or synchronous machine and does not require any design change for the machine itself. In fact, a three-phase machine with six terminals available is needed. In this case the model of the converter is given by 𝑣a1n1 = (q1a − q2a)Vdc (5.18)
  • 169. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 155 (a) q1a q1a 2a 1a a 0 Vdc Vdc q2a q2a t1 t2 q3a q3a q4a q4a (b) q1b q1b b L R L R n 0 Vdc Vdc q2b q2b t3 t4 q3b q3b q4b q4b a Vdc t2 q3a q3a q4a q4a q1c q1c c Vdc Vdc q2c q2c t5 t6 q3c q3c q4c q4c van vbn L R vcn Figure 5.18 (a) Fault-tolerant converter with triacs. (b) Post-fault topology.
  • 170. 156 CHAPTER 5 CASCADE CONFIGURATION a L R n Vdc q1a q1a q2a q2a Vdc q3a q3a q4a q4a van b L R Vdc q1b q1b q2b q2b Vdc q3b q3b q4b q4b vbn c L R Vdc q1c q1c q2c q2c Vdc q3c q3c q4c q4c vcn Figure 5.19 (a) Three-phase with two H-bridges connected in Δ. 𝑣b1n1 = (q1b − q2b)Vdc (5.19) 𝑣c1n1 = (q1c − q2c)Vdc (5.20) and 𝑣a2n2 = (q3a − q4a)Vdc (5.21) 𝑣b2n2 = (q3b − q4b)Vdc (5.22) 𝑣c2n2 = (q3c − q4c)Vdc (5.23) Then the voltage applied to the machine’s phases are given by 𝑣a1a2 = 𝑣a1n1 − 𝑣a2n2 + 𝑣n1n2 (5.24) 𝑣b1b2 = 𝑣b1n1 − 𝑣b2n2 + 𝑣n1n2 (5.25) 𝑣c1c2 = 𝑣c1n1 − 𝑣c2n2 + 𝑣n1n2 (5.26)
  • 171. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 157 (a) (b) a2 a1 b2 n2 n1 b1 c2 c1 200 0 –200 200 0 –200 200 0 –200 50 0 1 1.01 1.02 1.03 1.04 1.05 –50 Three-phase machine Vdc q1a q1a q2a q2a Vdc q3a q3a q4a q4a Vdc q1b q1b q2b q2b Vdc q3b q3b Phase 1 Phase 2 Phase 3 q4b q4b Vdc q1c q1c q2c q2c Vdc q3c q3c q4c q4c Figure 5.20 (a) Motor drive system with open-end winding topology. (b) Voltages and currents.
  • 172. 158 CHAPTER 5 CASCADE CONFIGURATION with 𝑣n1n2 given by 𝑣n1n2 = 𝑣a1n1 + 𝑣b1n1 + 𝑣c1n1 − 𝑣a2n2 − 𝑣b2n2 − 𝑣c2n2 (5.27) The open-end winding arrangement of the three-phase machine allows another series connection of the converter, as presented in Fig. 5.21(a). This is a three-phase motor drive system employing two three-leg inverters. Since the three-phase machine is in series with both converters, this is also considered a series connection arrange- ment among converters and machine. One of the advantages of the system presented in Fig. 5.21(a) is its fault tolerance capability. Two cases can be considered: Case I. The fault compensation is achieved by reconfiguring the power con- verter topology without any additional devices such as triacs. The post-fault configuration guarantees a Y connection of the motor. Case II. The fault compensation is achieved by reconfiguring the power con- verter topology with devices such as triacs. The post-fault configuration guarantees a delta connection of the motor. Both fault-tolerant strategies (Cases I and II) are based on the open-end winding machine and can be compensated for (i) dc-link capacitor failure; (ii) short-circuit failure; and (iii) open-circuit failure of the power switches. As previously presented, fault compensation is achieved by reconfiguring the power converter topology when a failure is detected. Vdc q1a Fuse Inverter 1 01 q1b 1b 1a 1c q1c q1a q1b q1c ia ib ic va vb vc Vdc q2a Fuse Inverter 2 (a) (b) 02 q2b 2b 2a 2c q2c + + + – – – q2a q2b q2c va * vt1 * va vt2 * Figure 5.21 (a) Pre-fault configuration—open-end winding motor drive system. (b) PWM waveforms (top) and motor phase voltage (bottom).
  • 173. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 159 A modulator with two carriers can be used for the PWM generation of the “healthy” open-end winding motor drive system [Fig. 5.21(a)], as observed in Fig. 5.21(b). The comparison between 𝑣∗ a and 𝑣∗ t1 defines the state of the switch q1a, while the comparison between 𝑣∗ a and 𝑣∗ t2 defines the state of the switch q2a. Each inverter also has a fuse for isolation purposes. As seen in Fig. 5.21(b) the motor phase voltage (𝑣a) has also multilevel characteristics. For Case I, the reconfiguration approach is obtained by using the other power switches not affected by the fault to create a neutral for the machine. Figure 5.22(a), 5.22(b), and 5.22(c) show the procedure to create a post-fault configuration in the case of open-circuit failure, short- circuit failure, and dc-link failure, respectively. Note that, in the case of dc-link failure, the creation of the neutral of the machine can be accomplished by either upper or lower switches of the converter under fault. In this strategy (Case I) the motor voltage value after the fault is reduced by 50%. Open-circuit failure Short-circuit failure Fuse Fuse Fuse Fuse Y connection Y connection Fuse Fuse Fuse (a) (b) Figure 5.22 Post-fault configuration for: (a) open-circuit failure, (b) short-circuit failure, and (c) dc-link failure.
  • 174. 160 CHAPTER 5 CASCADE CONFIGURATION DC-link failure Fuse Fuse Fuse Fuse Y connection (c) Figure 5.22 (Continued). On the other hand, for Case II, the fault compensation is achieved by reconfig- uring the power converter topology along with reconfiguration devices (triacs). The pre-fault configuration is depicted in Fig. 5.23(a). In order to increase the voltage applied to the machine, the reconfiguration approach aims to guarantee a delta con- nection of the motor after the fault. Two actions must be managed by the control system: isolate the source of the converter under fault and turn on all triacs, as depicted in Fig. 5.23(b). Despite using more devices (three triacs – ta, tb, and tc) than the solu- tion presented in Case I, the values for the motor phase voltage after the fault are reduced by just 13.4%, due to the Δ connection. Fuse q1a 1a 1b 1c Vdc 01 q1b q1c q1a q1b q1c Inverter 1 Inverter 2 (a) Fuse q2a 2a 2b 2c Vdc 02 q2b q2c q2a q2b q2c ia ib ic ta tb tc va vb vc + + + – – – Figure 5.23 Fault-tolerant strategy—Case II. (a) Pre-fault configuration. (b) Fault reconfiguration procedure to make a delta connection of the machine considering a short-circuit failure.
  • 175. 5.7 THREE-PHASE CONVERTER—TWO CASCADE H-BRIDGES PER PHASE 161 Delta connection Source isolation Fuse Fuse Fuse (b) Figure 5.23 (Continued). (a) (b) vb * va * PWM Inverter 1 Three-phase open-end winding machine Inverter 2 vc * Fault detection vb * va * PWM Inverter 1 Three-phase open-end winding machine Inverter 2 vc * Fault detection Figure 5.24 Control block diagram. (a) Case I. (b) Case II.
  • 176. 162 CHAPTER 5 CASCADE CONFIGURATION (a) (b) v a (V) 50 –50 0.05 0.06 0.07 0.08 Fault Reconfiguration 0.09 0.1 0.11 0.12 0.13 0.14 0.15 0 i a, i b, i c (A) 50 –50 0.05 0.06 0.07 0.08 Fault t (s) Reconfiguration 0.09 0.1 0.11 0.12 0.13 0.14 0.15 0 v a (V) 50 –50 0.05 0.06 0.07 0.08 Fault Reconfiguration 0.09 0.1 0.11 0.12 0.13 0.14 0.15 0 i a, i b, i c (A) 50 –50 0.05 0.06 0.07 0.08 Fault t (s) Reconfiguration 0.09 0.1 0.11 0.12 0.13 0.14 0.15 0 Figure 5.25 Motor phase voltage (top) and current (bottom) with a fault occurring at t = 0.1 s. (a) Case I and (b) Case II. Figure 5.24 shows a simplified schematic of the control strategy for Cases I and II. The fault can be identified by comparing the reference voltage with the measured ones. After the fault occurrence, the reconfiguration procedure changes from the open-end winding motor (“healthy” configuration) to a post-fault converter. Figure 5.25 shows simulated results with a fault (open-circuit failure) occurring in switch q2b at t = 0.1s. The variables in this figure are motor phase voltage (𝑣a) and motor currents (ia, ib, and ic). Figure 5.25(a) shows the results for Case I, while Fig. 5.25(b) shows the results for Case II. In this case, the switching frequency was 2 kHz and the dc-link voltage of each dc source was 50 V. 5.8 TWO H-BRIDGE CONVERTERS (SEVEN- AND NINE-LEVEL TOPOLOGIES) The PWM approach previously presented for two H-bridge converters connected in series generates the gating signals to guarantee a five-level voltage at the output of the converter. Such a converter structure is also known as symmetric cascade multilevel
  • 177. 5.8 TWO H-BRIDGE CONVERTERS (SEVEN- AND NINE-LEVEL TOPOLOGIES) 163 TABLE 5.4 Table of Variables for the Cascade Converter Operating with Seven Levels State q1a q2a q1b q2b 𝑣o 1 0 0 0 0 0 2 0 0 0 1 −Vb 3 0 0 1 0 Vb 4 0 0 1 1 0 5 0 1 0 0 −2Vb 6 0 1 0 1 −3Vb 7 0 1 1 0 −Vb 8 0 1 1 1 −2Vb 9 1 0 0 0 2Vb 10 1 0 0 1 Vb 11 1 0 1 0 3Vb 12 1 0 1 1 2Vb 13 1 1 0 0 0 14 1 1 0 1 −Vb 15 1 1 1 0 Vb 16 1 1 1 1 0 inverter, since it uses the same dc-link voltages. An asymmetric cascade multilevel inverter using unequal dc sources in each phase can be employed to generate either a seven-level or a nine-level waveform. From Table 5.3 and considering Va = 2Vb, it turns out that the number of lev- els for 𝑣o will be seven: {0,±Vb,±2Vb,±3Vb}, as presented in Table 5.4. Note that equation (5.28) describes the voltage at the output converter side as a function of the switching states. 𝑣o = (2q1a − 2q2a + q1b − q2b)Vb (5.28) Although increasing the number of levels, asymmetric cascade multilevel inverters operate with switches dealing with different blocking voltages and also require different dc-link voltages, which could restrict their applications. A higher number of levels can be obtained when Va = 3Vb. Table 5.5 shows nine levels for the output voltage as a function of the state of the switches. In this case the nine levels are {0,±Vb,±2Vb,±3Vb,±4Vb}. Another possible restriction of the unsymmetrical cascade multilevel topology is related to the lack of redundancy for generation of each level. Such a redundancy brings a degree of freedom to optimize the converter’s operation. A comparison between Tables 5.4 and 5.5 shows the generation of the level 2Vb is obtained with two switching states (States 9 and 12 in Table 5.4) for the seven-level configuration, while the generation of the same level for a nine-level configuration is done with just one switching state (State 10 in Table 5.5).
  • 178. 164 CHAPTER 5 CASCADE CONFIGURATION TABLE 5.5 Table of Variables for the Cascade Converter Operating with Nine Levels State q1a q2a q1b q2b 𝑣o 1 0 0 0 0 0 2 0 0 0 1 −Vb 3 0 0 1 0 Vb 4 0 0 1 1 0 5 0 1 0 0 −3Vb 6 0 1 0 1 −4Vb 7 0 1 1 0 −2Vb 8 0 1 1 1 −3Vb 9 1 0 0 0 3Vb 10 1 0 0 1 2Vb 11 1 0 1 0 4Vb 12 1 0 1 1 3Vb 13 1 1 0 0 0 14 1 1 0 1 −Vb 15 1 1 1 0 Vb 16 1 1 1 1 0 TABLE 5.6 Different Switching States to Generate the Same Output Level 2Vdc State q1a q2a q1b q2b q1c q2c 𝑣o 1 1 0 1 0 0 0 2Vdc 2 1 0 1 0 1 1 2Vdc 3 1 0 1 1 1 0 2Vdc 4 1 0 0 0 1 0 2Vdc 5 0 0 1 0 1 0 2Vdc 6 1 1 1 0 1 0 2Vdc 5.9 THREE H-BRIDGE CONVERTERS Multilevel configurations with three H-bridges can be obtained easily just following the axioms and postulates of the power blocks geometry (PBG). Figure 5.26(a) shows a single-phase topology with three H-bridges series connected. Figure 5.26(b), 5.26(c), and 5.26(d) present three-phase solutions with H-bridges Y-connected, Δ-connected, and with open-winding machine arrangement, respec- tively. Figure 5.26(e) shows another possibility of connections with Δ arrangements for the outer converters. With the increase of the number of H-bridge cells, the number of switching states and levels increases. For example, assuming that Va, Vb, and Vc have the same value Vdc, there are six ways to generate the level 2Vdc, as presented in Table 5.6.
  • 179. 5.9 THREE H-BRIDGE CONVERTERS 165 (a) (b) (c) (d) (e) Va Vb Vc Va1 Vb1 Vc1 Va2 Vb2 Vc2 Va3 Vb3 Vc3 n vo 1 2 3 Va1 Vb1 Vc1 Va2 Vb2 Vc2 Va3 Va1 Va2 Va3 Vb1 Three-phase machine Phase 1 Phase 2 Phase 3 Vb2 Vb3 Vc1 Vc2 Vc3 Va1 Va2 Va3 Vb1 Three-phase machine Phase 1 Phase 2 Phase 3 Vb2 Vb3 Vc1 Vc2 Vc3 Vb3 Vc3 1 2 3 Figure 5.26 Three H-bridge configuration: (a) single-phase, (b) three-phase Y-connected, (c) three-phase Δ-connected, and (d) open-winding machine. (e) Δ connections for the outer converters.
  • 180. 166 CHAPTER 5 CASCADE CONFIGURATION (a) (b) 200 0 –200 50 0 –50 300 0 –300 1 0 –1 0.03 0.05 0.07 0.055 0.06 200 0 –200 vo vo vsin * vt1 * vt6 * vt3 * vt2 * vt5 * vt4 * io vsin * Figure 5.27 (a) Phase-shift modulation with (top) PWM signals, (middle) output voltage and (bottom) output current. (b) Zoom of the PWM and output voltages. In a general way, the output voltage of the three symmetrical H-bridge config- uration can be written as 𝑣o = (q1a − q2a)Va + (q1b − q2b)Vb + (q1c − q2c)Vc (5.29) Figure 5.27 shows the waveforms for the configuration in Fig. 5.26(a) supplying a single-phase RL load. Figure 5.27(a) top presents the PWM signals with phase-shift multicarrier modulation. Six triangular carrier signals (𝑣∗ t1 , 𝑣∗ t2 , 𝑣∗ t3 , 𝑣∗ t4 , 𝑣∗ t5 , and 𝑣∗ t6 ) are required since 7 levels are expected at the output. There is a phase shift between any two adjacent carrier waveforms given by 360∘/(N – 1), where N is the number of levels. Figure 5.27(b) shows details (zoom) for the voltages presented in Fig. 5.27(a). The control circuitries as well as the power part of the converter (with the power switches) are presented in Fig. 5.28. Note that the control waveforms (𝑣∗ sin and 𝑣∗ t1 , 𝑣∗ t6 , 𝑣∗ t3 , 𝑣∗ t2 , 𝑣∗ t5 , 𝑣∗ t4 ) and the ana- log circuit as presented in Fig. 5.28 generate a desired sequence of pulses at the output
  • 181. 5.9 THREE H-BRIDGE CONVERTERS 167 driver driver driver driver driver driver driver driver driver driver driver driver + + – – + – + – q1a q1a q2c q1b q1a q1a q2a q2a q1b q1b q2b q2b q1c q1c q2c q2c q2c q1b q2a q1c q2b q2a q1c q2b vsin * vt1 * vt6 * vt3 * vt2 * + – + – vt5 * vt4 * Figure 5.28 Analog control circuitries (left side) and the power part of the converter (right side). voltage with seven levels, all of them with the same d𝑣∕dt. If another PWM signal is employed (different from that presented in Fig. 5.27), changes are also expected in the analog circuit solution. For example, Fig. 5.29 shows the level-shift multicarrier PWM modulation for the three H-bridge converter with six triangular carrier signals vertically disposed. In this case, all carrier signals are in phase with each other. Such a technique is also known as in-phase disposition (IPD). In addition to the approach pre- sented in Fig. 5.29 there are other possibilities: alternate phase opposite disposition (APOD) and phase opposite disposition (POD). In the APOD approach all carriers are alternately in opposite disposition, while for the POD all carriers below zero are in phase, but in phase opposition with those above the zero axis. Figure 5.30 shows the control and power part of the converter to generate a seven-level output voltage as presented in Fig. 5.29. A direct comparison between phase shift and level shift strategies (presented in Figs 5.27 and 5.29, respectively) reveals that the phase shift approach has advantages in terms of reduced harmonic distortions. It is also possible to combine the solutions presented in Figs 5.27 and 5.29, as presented in Fig. 5.31. Such a combination results in a phase shift and level shift multicarrier approach.
  • 182. 168 CHAPTER 5 CASCADE CONFIGURATION 200 0 –200 50 0 –50 0.03 0.05 0.07 1 0 –1 vo io vsin * Figure 5.29 Level shift multicarrier modulation: (top) PWM signals (from top to bottom): 𝑣t1, 𝑣t3, 𝑣t5, 𝑣t6, 𝑣t4, and 𝑣t2. (middle) output voltage 𝑣o, and (bottom) output current io. driver driver driver driver driver driver driver driver driver driver driver driver + + – – + – + – q1a q1a q1b q1c q1a q1a q2a q2a q1b q1b q2b q2b q1c q1c q2c q2c q1b q1c q2c q2b q2a q2c q2b q2a vsin * vt1 * vt3 * vt5 * vt6 * + – + – vt4 * vt2 * Figure 5.30 Analog control circuitries (left side) and the power part of the converter (right side) for the level-shift modulation.
  • 183. 5.11 SUMMARY 169 200 0 –200 50 0 –50 0.03 0.05 0.07 1 0 –1 vo io vsin * Figure 5.31 Phase shift/level shift multicarrier modulation: (top) PWM signals: 𝑣t1, 𝑣t3, 𝑣t5, 𝑣t6, 𝑣t4, and 𝑣t2. (b) Output voltage 𝑣o, and (c) output current io. 5.10 FOUR H-BRIDGE CONVERTERS AND GENERALIZATION A converter with four H-bridges and also the generalization of the cascade converters are presented in Fig. 5.32(a). Figure 5.32(b) shows another type of series connection converter with a combination of the conventional three-phase converter and H-bridges topologies. 5.11 SUMMARY This chapter dealt with configurations and PWM techniques for connected H-bridge converters series. After discussing the single-phase converter, the three-phase version was presented using a single H-bridge converter per phase. Also, it was shown how to increase the number of levels with two H-bridge converters connected in series, bring- ing up the sequence given respectively by power converter construction, model, PWM approach, and three-phase version. Different multicarrier based schemes were pre- sented and various associated aspects discussed. For instance, the direct comparison between phase shift and level shift strategies revealed that the phase shift approach has advantages in terms of reduced harmonic distortions. One special issue treated in this chapter was the possibility of guaranteeing post-fault operation with cascaded H-bridge converters. In addition, it was shown that two H-bridge converters can be employed to generate an output voltage with seven and nine levels, employing the correct relationship between the dc-link voltages. Finally, different arrangements and PWM solutions for three connected H-bridge converter series were introduced based on the PBG approach. The chapter is enriched with Table of Variables and analog control circuitries for most cases.
  • 184. 170 CHAPTER 5 CASCADE CONFIGURATION a L R van b n L R vbn c L R vcn (b) (a) Figure 5.32 Four H-bridges and generalization. (b) Hybrid topology combining H-bridge and conventional three-phase inverter. REFERENCES [1] L. M. Tolbert, F. Z. Peng, and T. G. Habetler, Multilevel converters for large electric drives, IEEE Trans Ind Appl, vol. 35, no. 1, pp. 36–44, 1999. [2] R. Rabinovici, D. Baimel, J. Tomasik, A. Zuckerberger, Series space vector modulation for multi-level cascaded H-bridge inverters, IEE Proc IET, vol. 3, no. 10, pp. 843–857, 2010.
  • 185. REFERENCES 171 [3] Rodriguez J, Hammond PW, Pontt JO, Musalem R, Escobar Mj. Operation of a medium-voltage drive under faulty conditions. IEEE Trans Ind Electron 2005;52(4):1080–1085. [4] Wu B. High Power Converters and AC Drives. New Jersey: John Wiley and Sons; 2006. [5] J. Rodriguez, J. Lai and F. Z. Peng, Multilevel inverters: a survey of topologies, controls, and appli- cations, IEEE Trans Ind Electron, 49, No. 4, 2002, 724–738. [6] J Rodriguez, S. Bernet, Bin Wu, J. O. Pontt, S. Kouro, Multilevel voltage-source-converter topologies for industrial medium-voltage drives, IEEE Trans Ind Electron, vol. 54, no. 6, pp. 2930–2945, 2007. [7] Rashid MH. Power Electronics Handbook. New York: Academic; 2001. [8] Peng FZ, Lai J-S. Multilevel cascade voltage source inverter with separate DC sources. US patent 5,642,275. Jun 1997. [9] Hammond PW. Medium voltage PWM drive and method. US patent 5,625,545. Apr 1997. [10] Corzine Keith, Familiant Yakov. A new cascaded multilevel H-bridge drive. IEEE Trans Power Elec- tron, 2002, Vol. 17, No. 1, pp.125–131. [11] Manjrekar MD, Lipo TA. Hybrid multilevel power conversion system: a competitive solution for high-power applications. IEEE Trans Ind Appl 2000;36(3):834–841. [12] Lund R, Manjrekar MD, Steimer P, Lipo TA. Control strategies for a hybrid seven-level Inverter, Conference Record of EPE, pp. 1–10, 1999. [13] Manjrekar MD, Lipo TA. A hybrid multilevel inverter topology for drive applications. IEEE APEC; 1998, 523–529. [14] Carrara G, Gardella S, Marchenosi M, Salutari R, Sciutto G. A new multilevel PWM method: a theoretical analysis. IEEE Trans Power Electron, July 1992;7:497–505.
  • 186. CHAPTER 6 FLYING-CAPACITOR CONFIGURATION 6.1 INTRODUCTION A type of multilevel configuration known as flying capacitor (FC) converter is presented in this chapter under powerblock geometry (PBG) point of view. The introduction and fundamental concepts of configurations with three and more levels employing a FC approach, as well as a detailed description of these circuits, are addressed in this chapter. FC converters present higher degrees of freedom (redundant states) to synthesize a specific output voltage and employ a lesser number of semiconductor power devices than the neutral point clamped (NPC) topology. Such redundant states are used to regulate the FC voltage. Unlike the cascade configuration presented in Chapter 5, there is no need for isolated dc sources. The main challenge of the FC configuration is to keep the FC voltage under a desired level, avoiding distortion at the ac part of the converter. Part of this chapter will be dedicated to discussing strategies to balance the FC voltage. For the sake of illustra- tion, the analysis starts with the FC being substituted by a dc voltage source. A simple pulse width modulation (PWM) approach is employed to generate a three-level out- put voltage. It is demonstrated that the PWM approach affects the voltage ripple of the FC voltage. In fact, there are different strategies to regulate the capacitor voltage, which can be sorted into two main types: natural-balancing and active schemes. The natural-balancing approach employs solutions in terms of PWM strategies without any voltage and current sensors, while the active method employs feedback regula- tion and control algorithms to maintain the voltage constant. It is worth mentioning that different aspects affect the capacitor voltage balancing, for example, the type of load (linear or nonlinear). This chapter is organized considering the number of levels generated by each circuit, as done in Chapter 4 for NPC circuits. Subsequent to this introduction, Section 6.2 presents the power blocks (PBs) and the circuit with switches for the FC three-level topology, as also the model and Table of Variables. Section 6.3 deals with a simple PWM strategy applied for the three-level circuit. The FC voltage regulation is presented in Section 6.4. Sections 6.5 and 6.6 show the FC topologies for single-phase (full-bridge) and three-phase appli- cations, respectively. Other circuits of three-phase converters appear in Section 6.7. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 172
  • 187. 6.2 THREE-LEVEL CONFIGURATION 173 Four-level topologies are considered in Section 6.8. Finally, Section 6.9 presents the generalization and Section 6.10 summarizes this chapter. 6.2 THREE-LEVEL CONFIGURATION The PBs, as described in the Chapter 3, can be connected in a systematic appro- ach to guarantee the creation of FC multilevel configurations. An arrangement using two PB-ac blocks is depicted in Fig. 6.1(a), which follows Postulate 2. Figure 6.1(b)–6.1(e) shows the ways used to obtain each specific level at the output converter side 𝑣o referred to as the point “0”, that is, V1, (V1 − V2), (V2 − V3), −V3, respectively. Figure 6.1(c) and 6.1(d) illustrates that it is necessary to activate two PBs to obtain 𝑣o = (V1 − V2) and 𝑣o = (V2 − V3), while 𝑣o = V1 and 𝑣o = −V3 are obtained activating only one PB as in Fig. 6.1(b) and 6.1(e), respectively. (a) 0 2 1 V1 V3 vo V2 (b) 0 2 1 V1 vo (c) 0 2 1 V1 V2 vo (d) 0 2 1 V3 V2 vo (e) 0 2 1 V3 vo Figure 6.1 (a) Three levels FC configuration with PBs. Arrangement to obtain: (b) 𝑣o = V1. (c) 𝑣o = V1 − V2. (d) 𝑣o = V2 − V3. (e) 𝑣o = −V3.
  • 188. 174 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION or 0 2 1 V1 vo V2 0 2 1 V1 V1 –V3 t vo vo 0 2 1 V3 V2 vo 0 2 1 V3 vo V1 – V3 2 Figure 6.2 Generation of a general three-level output voltage. In general terms, to generate an output waveform with three levels it is nec- essary to activate the PBs in a sequence as observed from the waveform of 𝑣o in Fig. 6.2 (bottom). Since this is a three-level converter, V1 − V2 = V2 − V3, which means V2 = (V1 + V3)∕2. It is worth emphasizing that with FC topology it is possi- ble to generate the V2 level with two different circuit arrangements (i.e., topological states), as observed in Fig. 6.2 (top). This is an important characteristic of the FC topologies, which will be explored later in this chapter. Since 𝑣o can assume just one voltage value V1, (V1 − V3)∕2 or −V3 at each instant of time, it is possible to establish an equation to describe the output voltage 𝑣o as a function of the input voltages V′ 1 , V′ 2 , V′ 3 [where V′ 1 = V1, V′ 2 = (V1 − V3)∕2, and V′ 3 = −V3] as well as a function of two independent binary variables (q1 and q2). Following the same approach employed previously in this book, these binary vari- ables define the states of the switches inside the blocks. In this sense, since there are three inputs to be selected (V′ 1 , V′ 2 , and V′ 3 ), the minimum number of binary variables employed to select those inputs is two. Considering that there are three input voltages to be selected by using these binary variables, the output voltage can be obtained as presented in Table 6.1.
  • 189. 6.2 THREE-LEVEL CONFIGURATION 175 TABLE 6.1 Table of Variables for the Converter in Fig. 6.1(a) State q1 q2 𝑣o 𝑣o 1 0 0 −V3 V′ 3 2 0 1 V1 − V3 2 V′ 2 3 1 0 V1 − V3 2 V′ 2 4 1 1 V1 V′ 1 An equation used to describe the behavior presented in this table is given below: 𝑣o = q1q2V′ 3 + q1q2V′ 2 + q1q2V′ 2 + q1q2V′ 1 (6.1) where q1 = 1 − q1 and q2 = 1 − q2. In this case, (6.1) becomes 𝑣o = (1 − q1)(1 − q2)V′ 3 + (1 − q1)q2V′ 2 + q1(1 − q2)V′ 2 + q1q2V′ 1 (6.2) Normally, there are some requirements associated with total harmonic distortion (THD) minimization for the output voltage, which ends up with a sym- metrical waveform at the converter output, and consequently V′ 1 = Vdc, V′ 2 = 0, and V′ 3 = −Vdc. In this case it is possible to write equation (6.2) as follows: 𝑣o = (q1 + q2 − 1)Vdc (6.3) The binary variables considered in Table 6.1 are in fact the switching states inside the blocks, which means that the topology presented in Fig. 6.1 can be treated at its lower level presentation (switches instead of blocks), as in Fig. 6.3. Note that the FC configuration is bidirectional, which means that each voltage value V′ 1 , V′ 2 , V′ 3 can be obtained at the output converter side independent of the cur- rent, that is, any desired output value is obtained for both cases io > 0 and io < 0, as observed in Fig. 6.3. (a) (b) (c) (d) Vdc Vdc Vdc q1 q2 io q1 q2 Vdc Vdc Vdc q1 q2 io q1 q2 Vdc Vdc Vdc q1 q2 io q1 q2 Vdc Vdc Vdc q1 q2 io q1 q2 Figure 6.3 Generation of levels: (a) V′ 1 , (b) and (c) V′ 2 , and (d) V′ 3 independent of the output current.
  • 190. 176 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION Exercise 6.1 (a) Assuming the FC configuration with four independent switches (q1, q2, q3, and q4) as presented below, fill the table below eliminating the prohibited states caused by either undefined states (e.g., all switches off) or short-circuit of the dc-link source (or FC). (b) Eliminate all undefined states in this table and find a logic relationship among q1, q2, q3, and q4. vo Vdc Vdc Vdc q1 q2 q3 q4 State q1 q2 q3 q4 𝑣o 1 0 0 0 0 2 0 0 0 1 3 0 0 1 0 4 0 0 1 1 5 0 1 0 0 6 0 1 0 1 7 0 1 1 0 8 0 1 1 1 9 1 0 0 0 10 1 0 0 1 11 1 0 1 0 12 1 0 1 1 13 1 1 0 0 14 1 1 0 1 15 1 1 1 0 16 1 1 1 1
  • 191. 6.3 PWM IMPLEMENTATION (HALF-BRIDGE TOPOLOGY) 177 6.3 PWM IMPLEMENTATION (HALF-BRIDGE TOPOLOGY) A desired output voltage with regulation of both voltage and frequency can be obtained for the FC converter with PWM strategies. As considered for the other topologies, such a strategy is able to synthesize a square waveform with an average value (at the switching frequency) equal to a sinusoidal waveform. Figure 6.4 shows one possible analog solution for the PWM implementation known as level-shift, in which the states of the four power switches are determined by a comparison among two high frequency triangular waveforms (𝑣∗ t1 and 𝑣∗ t2 ) and a sinusoidal waveform (𝑣∗ sin ). The block marked “driver” must guarantee the (a) (b) (c) (d) driver driver 1 0 1 0 1 0 0.2 0.225 0.25 –1 + – q1 q1 q2 q1 q1 q2 vsin * vt1 * vt1 * driver driver + – q1 q2 q1 q2 vsin * vsin * 1 0 1 0 1 0 0.2 0.225 0.25 –1 q2 q2 vt2 * vsin * vt2 * Figure 6.4 (a) PWM generation for switches q1 and q1. (b) PWM generation for switches q2 and q2. (c) Variables associated with switches q1 and q1 (from top to bottom) – reference voltages, gating signals of switches q1 and q1. (d) Variables associated with switches q2 and q2 (from top to bottom) – reference voltages, gating signals of switches q2 and q2.
  • 192. 178 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION levels of voltage and current at the gate circuit needed to operate the power switches adequately. Note that when the switches q1 and q1 are in operation (on and off during the positive half cycle of 𝑣∗ sin ) the switch q2 is on and consequently the switch q2 is off for the whole half period. This is equivalent to states 2 and 4 in Table 6.1, which generates the levels V′ 2 and V′ 1 , respectively. On the other hand, on the negative half cycle of 𝑣∗ sin , when the switches q2 and q2 are in operation (alternating on and off) the switch q1 is off and consequently the switch q1 is on. This is equivalent to states 1 and 2 in Table 6.1, which generates the levels V′ 3 and V′ 2 , respectively. The PWM presented in Fig. 6.4(a) is able to generate the output voltage with the desired number of levels (V′ 1 , V′ 2 , and V′ 3 ) using such a simple implementation. However, State 3 in Table 6.1 has not been used in this simple strategy, which means that there is still a degree of freedom to be explored, as seen in the following sections. Figure 6.5(a) shows the half-bridge three-level configuration, in which the load is connected between the dc-link mid-point and the center point of the leg. Figure 6.5(b) depicts (from top to bottom) PWM reference waveforms, gating signals of switches q1 and q2, load voltage, and load current, respectively. The parameters employed in these simulation tests were: Vdc = 200 V, R = 5 Ω, and L = 5 mH, and switching frequency equal to 500 Hz. (a) (b) vo io vt1 * vt2 * vsin * 0.2 0.225 0.25 0 200 –200 0 0 0 1 1 –1 1 50 0 –50 q1 q2 q1 L R + – vo io Vdc Vdc Vdc q2 q2 q1 Figure 6.5 (a) Three-level FC half-bridge converter. (b) (from top to bottom) 𝑣∗ sin , 𝑣∗ t1 , 𝑣∗ t2 ; gating signal of switch q1; gating signal of switch q2; load voltage and load current.
  • 193. 6.4 FLYING CAPACITOR VOLTAGE CONTROL 179 6.4 FLYING CAPACITOR VOLTAGE CONTROL In order to simplify the analysis of an FC converter, the FC was substituted by a dc voltage source, as in Fig. 6.5(a). However, in practical circuits the center dc voltage source in Fig. 6.5(a) is replaced by a capacitor, as in Fig. 6.6(a). In this case, it is necessary to guarantee the control voltage of this capacitor. For example, if the level-shift PWM approach presented in Fig. 6.4 is applied to the half-bridge converter presented in Fig. 6.6(a), the results for the capacitor vari- ables (𝑣C and iC) are as presented in Fig. 6.6(b). Even with the average value of 𝑣C equal to 200 V (as desired), there are variations for the voltage 𝑣C which will bring up low frequency distortion at the output converter side. From the node between the switches q1 and q2 in Fig. 6.6(a) it is possible to determine the capacitor current as follows: iC = iq1 − iq2, and assuming the level-shift modulation approach, it can be seen that: When 𝑣∗ sin > 0: q2 = 1 iq2 = io iq1 = q1io ∴iC = (q1 − 1)io (a) (b) vC vC iC io vt1 * vt2 * vsin * vsin * 1.01 1 1.02 0 200 150 250 50 0 0 1 1 –1 1 –50 q1 q2 q1 L R + – vo io Vdc Vdc q2 q2 q1 Figure 6.6 (a) Half-bridge converter with flying capacitor. (b) Control and power variables for the half-bridge circuit with level-shift PWM.
  • 194. 180 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION When 𝑣∗ sin < 0: q1 = 0 iq1 = 0 iq2 = q2io ∴iC = −q2io From the current iC obtained previously, it is possible to determine directly the capacitor voltage, since: 𝑣C = 1 C ∫ iCdt. Exercise 6.2 In order to deeply understand the mechanism behind the FC voltage control, draw the topological states considering the switching signals and capacitor waveforms in steady-state operation for the circuit in Fig. 6.6(a), as highlighted below. Consider each of the intervals of time below (from 1 to 17). vC iC q1 q2 1 2 3 5 7 11 4 6 8 9 13 15 10 12 14 16 17 To guarantee the capacitor voltage control with reduced variation, another PWM strategy can be considered, as seen in Fig. 6.7. A phase-shift has been considered in this case, which leads to a capacitor charging and discharging at the switching frequency. This plays an important role in keeping 𝑣C with reduced ripple. The polarity of the capacitor current in Fig. 6.6(b) has changed with the sinusoidal frequency, which increases the ripple for 𝑣C. Note from Fig. 6.6(b) that the FC is discharged during the entire positive half of the sinusoidal voltage (𝑣∗ sin ) since iC is either zero or negative. On the other hand, the FC during the negative half of the sinusoidal voltage is charged because iC is either zero or positive.
  • 195. 6.5 FULL-BRIDGE TOPOLOGY 181 vC iC io vt1 * vt2 * vsin * vsin * 1.01 1 1.02 0 200 150 250 50 0 0 –1 1 –1 1 –50 q1 q2 Figure 6.7 Control and power waveforms for the half-bridge circuit with level-shift PWM. On the other hand, in the PWM technique shown in Fig. 6.7, the charging/ discharging occurs on the switching frequency; this keeps the capacitor voltage ripple smaller. The PWM techniques able to reduce the ripple on the FC are fundamental for reducing the distortion of the output voltages. Figure 6.8(a) and 6.8(b) shows the load voltage for the level-shift and phase-shift approaches, respectively. Figure 6.9 in turn shows the start-up transient for the FC voltage. 6.5 FULL-BRIDGE TOPOLOGY Full-bridge three-level FC converters for both single-phase and three-phase loads are obtained by connecting the blocks in Fig. 6.1 as observed in Figs 6.10(a) and 6.10(b), respectively. Figure 6.10(c) shows the option in which the three-phase four-wire sys- tem is required. The full-bridge single-phase three-level FC converter is presented in Fig. 6.11(a) by using switches instead of blocks (lower level representation). Figure 6.11(b) shows (from top to bottom) pole voltage of the first leg (with switches q1a and q2a), pole voltage of the second (with switches q1b and q2b), load voltage, and load current, respectively. Comparing the load voltage in Figs 6.5(b) and 6.11(b), it is quite clear that the increased number of levels observed in the load voltage of the full-bridge topology guarantees the ripple reduction of the current and consequently a better quality of the voltage delivered by the converter. In this case the output voltage is given by 𝑣o = (q1a + q2a − q1b − q2b)Vdc (6.4)
  • 196. 182 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION (a) (b) vo 250 0 –250 1 1.025 1.05 vo 250 0 –250 1 1.025 1.05 Figure 6.8 Influence of the PWM technique for distortion reduction at the output voltage. vC 200 100 0 0 3 6 Figure 6.9 Start-up transient for the flying capacitor voltage (𝑣C). As mentioned previously, the number of levels considered in this chapter is defined by the voltage between the midpoint of the leg and the dc-link midpoint, that is, through the pole voltage. For instance, both converters in Figs 6.6 and 6.11 are considered as single-phase three-level FC configurations, even though the load voltage in the full-bridge topology presents five levels.
  • 197. 6.6 THREE-PHASE FC CONVERTER 183 (a) 0 1 2 Vdc a b Vdc (b) 0 1 2 Vdc a b c Vdc (c) 0 1 2 Vdc a b c d Vdc Figure 6.10 (a) Single-phase full-bridge three-level FC converter. (b) Three-phase full-bridge three-level FC converter. (c) Three-phase four-wire three-level FC converter. 6.6 THREE-PHASE FC CONVERTER A three-phase three-level FC configuration is depicted in Fig. 6.12(a), while Fig. 6.12(b) shows some variables associated with this converter, that is, (from top to bottom) pole voltage, voltage between the load neutral point and dc-link mid-point connection, load phase voltage, and load current, respectively. The pole voltages for the three-phase converter can be written as follows: 𝑣a0 = (q1a + q2a − 1)Vdc (6.5) 𝑣b0 = (q1b + q2b − 1)Vdc (6.6) 𝑣c0 = (q1c + q2c − 1)Vdc (6.7) Considering a balanced three-phase load, the voltage 𝑣n0 can be defined ana- lytically by 𝑣n0 = Vdc 3 (q1a + q2a + q1b + q2b + q1c + q2c) − Vdc (6.8) From (6.8), and considering all 64 switching states, the voltage 𝑣n0 depicted in Fig. 6.12(b) is responsible for increasing the number of levels in 𝑣an. The phase
  • 198. 184 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION io vo vb0 va0 0.225 0.2 0.25 200 –200 200 –200 500 –500 100 –100 q1a L R a b 0 + – vo io Vdc Vdc q2a q2a q1a q1b q2b q2b q1b (a) (b) Figure 6.11 (a) Three-level NPC full-bridge converter. (b) (from top to bottom) pole voltage of the first leg (q1a and q2a), pole voltage of the second (q1b and q2b), load voltage, and load current. voltage for each phase of a balanced three-phase load is given by 𝑣a = ( 2 3 q1a + 2 3 q2a − 1 3 q1b − 1 3 q2b − 1 3 q1c − 1 3 q2c ) Vdc (6.9) 𝑣b = ( − 1 3 q1a − 1 3 q2a + 2 3 q1b + 2 3 q2b − 1 3 q1c − 1 3 q2c ) Vdc (6.10) 𝑣c = ( − 1 3 q1a − 1 3 q2a − 1 3 q1b − 1 3 q2b + 2 3 q1c + 2 3 q2c ) Vdc (6.11) In this case (balanced three-phase load) the load voltages depend only on state of the switches and dc-link voltage. Notice that the control circuit is obtained as seen in Fig. 6.4, replicating the PWM control for the other two phases with the following sinusoidal references: 𝑣∗ sin 1 = Vp sin(𝑤t), 𝑣∗ sin 2 = Vp sin(𝑤t + 120∘), and 𝑣∗ sin 3 = Vp sin(𝑤t + 240∘), where Vp is the peak voltage desired for the load.
  • 199. 6.6 THREE-PHASE FC CONVERTER 185 ia van vn0 va0 0.225 (a) (b) 0.2 0.25 500 –500 0 500 –500 0 500 –500 0 100 –100 0 q1a n a b c 0 + – vc ic + – vb ib + – va ia Vdc Vdc q2a q2a q1a q1b q2b q2b q1b q1c q2c q2c q1c Figure 6.12 (a) Three-level NPC converter. (b) (from top to bottom) pole voltage, voltage 𝑣n0, load voltage and load current. Figure 6.13(a) shows the same power converter topology supplying a three-phase load connected in Δ arrangement. The way the load is connected to the FC topology plays an important role for the converter’s design and specification. Figure 6.13(b) shows the impact of the load’s connection (i.e., Δ or Y) on the FC voltage ripple of the phase a (𝑣Ca) with Fig. 6.13(b) – top showing the result for Y connection and Fig. 6.13(b) – bottom showing the same result under the same conditions for Δ connection. A FC of 100 μF was considered for both cases in Fig. 6.13. Since the Δ connection implies higher load currents, it also leads to higher FC voltage fluctuation, as highlighted in Fig. 6.13(b) – bottom. Another significant difference expected with the type of load connection (Y or Δ) is in terms of the number of levels obtained on the load phase as follows: 𝑣a = (q1a + q2a − q1b − q2b)Vdc (6.12) 𝑣b = (q1b + q2b − q1c − q2c)Vdc (6.13) 𝑣c = (q1c + q2c − q1a − q2a)Vdc (6.14)
  • 200. 186 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION 0 0.1 0.2 0.3 t (s) v Ca (V ) 0.4 0.5 240 220 200 180 160 0 0.1 0.2 0.3 t (s) v Ca (V) 0.4 0.5 240 220 200 180 160 q1a a b c 0 + – vc + – vb + – va Vdc Vdc q2a q2a q1a q1b q2b q2b q1b q1c q2c q2c q1c Figure 6.13 (a) Three-level FC converter supplying a three-phase load connected in Δ arrangement (b) FC voltage with (top) wye and (bottom) delta load connection. 6.7 NONCONVENTIONAL FC CONVERTERS WITH THREE-LEVEL LEGS The goal in this section, as in other chapters in this book, is to present different power circuits obtained by changing the way the switches are arranged. Even assuming that those configurations may not be considered as traditional ones, they are useful in pro- viding a learning intervention. In this sense, following the possibilities regarding the
  • 201. 6.7 NONCONVENTIONAL FC CONVERTERS WITH THREE-LEVEL LEGS 187 connection between the blocks that define a conventional two-level leg and those for FC three-level leg, it is possible that five- and four-level topologies can be obtained, as in Fig. 6.14(a) and 6.14(b), respectively. In fact, despite using three dc voltage sources and having lesser levels at the out- put converter side, the converter in Fig. 6.14(b) has the advantage of operating with switches under the same blocking voltage. To guarantee that all power switches oper- ate under the same blocking voltage and to guarantee a symmetrical output voltage, it is necessary to make V1 = V3 = Vdc and V2 = 2Vdc. Considering all possibilities of switching states available (that is, eliminating the prohibited states), the output voltage is determined by Table 6.2. From this table and avoiding the undesired states, there are four levels for 𝑣o. It is evident that Fig. 6.14(a) is a particular case of the converter with four levels with V1 = V3 = 0, which will lead necessarily to a converter with irregular blocking voltage among the switches. As can be observed in Fig. 6.14(b), the single-phase load is connected between the points a and b of the converter, which leads to an output voltage given by 𝑣o = (2q1a + 2q2a − 2qb − 1)Vdc (6.15) The modulation strategy for this converter can be decided, assuming a com- bination of the two-level and three-level PWM approaches, which means that one triangular carrier signal (𝑣∗ t2 ) is employed for the two-level leg, and two triangular carrier signals (𝑣∗ t1 and 𝑣∗ t3 ) are used for a three- level leg. Since each leg is capable of synthesizing different values of voltages, that is, 2Vdc for the two-level leg and 4Vdc for the three-level leg, the sinusoidal waveforms employed to define PWM signals should follow the same ratio. Indeed, there are two requirements: the reference volt- age for the three-level leg must be twice as big as the two-level leg and their difference must be the desired voltage (𝑣∗ sin ), which leads to 𝑣∗ a = ( 2 3 ) 𝑣∗ sin (6.16) 𝑣∗ b = − ( 1 3 ) 𝑣∗ sin (6.17) Figure 6.14(c) shows the analog implementation of the PWM approach for the proposed converter. Note that the level-shift technique has been applied to the FC three-level leg. Figure 6.14(d) shows the PWM signals with three triangular waveforms (𝑣∗ t1 and 𝑣∗ t3 employed for the three-level leg and 𝑣∗ t2 used for the two-level leg) and two sinusoidal waveforms, as in equations (6.16) and (6.17). Figure 6.15(a) shows the three-phase version of the FC four-level converter presented in Fig. 6.14(b) by using an open-end motor drive system. Again, this configuration presents all switches processing the voltage with the same blocking voltage. The model and PWM strategy for this topology can be adapted directly from Fig. 6.14(c). Figure 6.15(b) presents the machine phase voltage for phase 1 (𝑣a). The three-phase two-leg FC topology is depicted in Fig. 6.16.
  • 202. 188 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION b a vo vC + + + – – – + – + – io Vdc q2a q2a q1a qb qa qb b a vo vC + + – – io V2 V1 V3 q2a q2a q1a qb q1a q2a q2a q1a qb qb q1a qb va * vsin * 2 3 = vt1 * va * vsin * 2 3 = vt3 * vb * vsin * 1 3 = 1 0 –1 1 0 –1 0.2 0.225 (d) 0.25 vt2 * vt2 * vt3 * vb * va * vt1 * (a) (b) (c) Figure 6.14 (a) Five-level FC topology. (b) Four-level FC topology. (c) PWM strategy for the four-level circuit and (d) its waveforms.
  • 203. 6.8 FOUR-LEVEL CONFIGURATION 189 TABLE 6.2 Output Voltage Considering All Switching States Available State {q1aq2aqb} 𝑣o 1 {0 0 0} −Vdc 2 {0 0 1} −3Vdc 3 {0 1 0} −Vdc 4 {0 1 1} Vdc 5 {1 0 0} 6 {1 0 1} 7 {1 1 0} 3Vdc 8 {1 1 1} Vdc q1a V1 V2 V3 200 (a) (b) –200 0 qc c b a a+ q2a q1a q2a q1b b+ q2b q1b q2b q1c c+ q2c q1c q2c qc qb qb qa Phase 1 Phase 2 Phase 3 Three-phase machine qa v a (V) Figure 6.15 (a) Three-phase version of the four-level FC converter with open-end winding three-phase motor. (b) Machine phase voltage. 6.8 FOUR-LEVEL CONFIGURATION Following the axioms and postulates involving the PBs, presented in the Chapter 3, the four-level FC leg can be obtained as seen in Fig. 6.17(a). Figure 6.17(b)–6.17(i) shows the methods used to obtain the levels at the output converter side, specified in Table 6.3. Figure 6.17(b) illustrates that it is necessary to activate the PBs 2 and 3 to obtain 𝑣o = −V4, while 𝑣o = V1 is obtained when PBs 1 and 2 are activated.
  • 204. 190 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION b c 0 vc ic + – vb ib + – va ia + – Vdc Vdc q1b q2b q2b q1b q1c q2c q2c q1c Figure 6.16 Three-phase two-leg FC converter. TABLE 6.3 Table of Variables for the Converter in Fig. 6.17(a) State q1 q2 q3 𝑣o 1 0 0 0 −V4 2 0 0 1 V3 − V4 3 0 1 0 −V3 + V2 − V4 4 0 1 1 V2 − V4 5 1 0 0 −V2 + V1 6 1 0 1 V3 − V2 + V1 7 1 1 0 −V3 + V1 8 1 1 1 V1 The other levels are: 𝑣o = V3 − V4 [Fig. 6.17(c)], 𝑣o = −V3 + V2 − V4 [Fig. 6.17(d)], 𝑣o = V2 − V4 [Fig. 6.17(e)], 𝑣o = −V2 + V1 [Fig. 6.17(f)], 𝑣o = V3 − V2 + V1 [Fig. 6.17(g)], 𝑣o = −V3 + V1 [Fig. 6.17(h)], and 𝑣o = V1 [Fig. 6.17(i)]. In general terms, to generate an output waveform with four symmetrical levels as in Fig. 6.18, it is necessary to activate the PBs in a sequence as observed in the same figure, with V1 = 1.5Vdc, V2 = 2Vdc, V3 = 1Vdc, and V4 = 1.5Vdc. Table 6.4 shows the symmetrical levels as a function of the switching states. The interme- diate levels (−0.5Vdc and 0.5Vdc) can be obtained with three different circuits; such a characteristic can be employed to guarantee the FC voltage with reduced ripple. The equation employed to describe the output voltage 𝑣o as a function of both the input voltages and the binary variables (q1, q2, and q3) is presented below. The- oretically, it is possible to guarantee each input voltage at 𝑣o using only two binary variables, since 22 = 4. However, it is necessary to associate each binary variable to a switching state of the four-level configuration, which means a minimum of three binary variables (q1, q2, and q3).
  • 205. 6.8 FOUR-LEVEL CONFIGURATION 191 0 1 3 (a) (b) 2 vo V1 V4 V2 V3 1 3 2 vo V4 (c) 1 3 2 vo V4 V3 (d) 1 3 2 vo V4 V3 V2 (e) 1 3 2 vo V4 V2 (h) 1 3 2 vo V1 V3 (i) 1 3 2 0 vo V1 (f) 1 3 2 vo V1 V2 (g) 1 3 2 vo V1 V3 V2 Figure 6.17 (a) Four-level FC configuration with PBs. (b) 𝑣o = −V4. (c) 𝑣o = V3 − V4. (d) 𝑣o = −V3 + V2 − V4. (e) 𝑣o = V2 − V4. (f) 𝑣o = −V2 + V1. (g) 𝑣o = V3 − V2 + V1. (h) 𝑣o = −V3 + V1. (i) 𝑣o = V1. In this sense, the output pole voltage is given by 𝑣o = q1q2q3(−1.5Vdc) + q1q2q3(−0.5Vdc) + q1q2q3(−0.5Vdc) + q1q2q3(0.5Vdc) + q1q2q3(−0.5Vdc) + q1qq3(0.5Vdc) + q1q2q3(0.5Vdc) + q1q2q3(1.5Vdc) (6.18) where q1 = 1 − q1, q2 = 1 − q2, and q3 = 1 − q3.
  • 206. 192 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION 1 3 2 vo V1 V3 1 3 2 vo V1 V3 V2 1 3 2 0 vo V1 1 3 2 vo vo vo V2 V4 1.5Vdc 0.5Vdc –0.5Vdc –1.5Vdc 1 3 2 V4 t V3 vo 1 3 2 V4 1 3 2 vo V4 V3 V2 1 3 2 vo V1 V2 Figure 6.18 Generation of a general four-level output voltage. TABLE 6.4 Table of Variables for the Converter in Fig. 6.18(a) with 1.5Vdc, 0.5Vdc, −0.5Vdc, or −1.5Vdc State q1 q2 q3 𝑣o 1 0 0 0 −1.5Vdc 2 0 0 1 −0.5Vdc 3 0 1 0 −0.5Vdc 4 0 1 1 0.5Vdc 5 1 0 0 −0.5Vdc 6 1 0 1 0.5Vdc 7 1 1 0 0.5Vdc 8 1 1 1 1.5Vdc Developing (6.18) it is possible to write 𝑣o as follows: 𝑣o = (q1 + q2 + q3)Vdc − 1.5Vdc (6.19) As in the three-level FC configuration, the four-level one is able to generate the desired output voltage either for positive or negative voltage.
  • 207. 6.8 FOUR-LEVEL CONFIGURATION 193 (a) (b) (c) driver driver + – q1 q2 q3 vsin * vt1 * + – vsin * vt1 * q1 q2 q3 driver driver q1 q2 q3 q1 q2 q3 + – vsin * vt1 * driver driver q1 q2 q3 q1 q2 q3 Figure 6.19 Modulation strategy for gating signal generation. Considering the need for generation of an output waveform with reduced har- monic distortion, Fig. 6.19 shows the analog solution for the PWM signal gener- ation. The states of the six switches are determined by a comparison among three high frequency triangular waveforms (𝑣∗ t1 , 𝑣∗ t2 , and 𝑣∗ t3 ) and a sinusoidal waveform (𝑣∗ sin ). Such a comparison will allow the generation of the levels as in Table 6.4. Figure 6.20 shows the power converter and waveforms for a half-bridge four-level configuration. Although the topologies in Figs 6.17–6.20 present the conventional way to obtain a four-level voltage by using FC configuration, it is also possible to obtain a four-level output voltage with only two PBs, that is, with four switches per leg, as seen in Fig. 6.21(a). In this case, it is necessary to guarantee the following relation- ship among the input voltage sources: V1 = V3 = 2Vdc and V2 = Vdc and adapt the PWM generation to assure an output voltage with four levels. The pole voltage is given by 𝑣o = (3q1 + q2 − 2)Vdc (6.20) Figure 6.21(b) shows the desired sinusoidal voltage that must be synthesized by the studied converter. This waveform is intentionally separated into four sectors. To synthesize the desired voltage in each sector it is necessary to activate the switches q1 and q2 as described in Fig. 6.21(b) – bottom. While Fig. 6.22(a) shows the analog
  • 208. 194 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION (a) (b) R L io io vo vo + – 1.5Vdc 1.5Vdc 1 1 1 0 0 1 0 200 –200 0.2 0.225 0.25 50 –50 –1 2Vdc Vdc q1 q1 q1 q2 q2 q3 q3 q2 q3 Figure 6.20 (a) Four-level FC half-bridge converter. (b) (from top to bottom) 𝑣∗ sin , 𝑣∗ t1 , 𝑣∗ t2 , 𝑣∗ t3 ; gating signal of switches q1, q2, and q3; load voltage and load current. (a) va0 2Vdc –2Vdc –Vdc Vdc 2Vdc 0 2Vdc Vdc a 0 0 0 1 1 0 1 1 q1 q2 q2 q1 q1 q2 Figure 6.21 (a) Four-level FC converter with four switches (b) Desired waveform divided in sectors.
  • 209. 6.8 FOUR-LEVEL CONFIGURATION 195 (b) va0 = {Vdc, –Vdc} va0 = {Vdc, –Vdc} va0 = {Vdc, 2Vdc} va0 = {Vdc, –2Vdc} q1 = 1 Desired sinusoidal voltage q2 = {0,1} q1 = {0,1} q2 = {0,1} q1 = 0 q2 = {0,1} q1 = {0,1} q2 = {0,1} Sector 1 Sector 2 Sector 3 Sector 4 Figure 6.21 (Continued) (a) (b) + – q1 q2 vsin1 * vsin1 * vcarrier1 * vcarrier1 vsin2 * vcarrier2 + – vsin2 * vcarrier2 * q1 q2 Figure 6.22 (a) Four-level FC converter with four switches (b) Desired waveform divided in sectors.
  • 210. 196 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION (a) 0 1 2 3 V1 V4 V2 V3 a b (b) 0 1 2 3 V1 V4 V2 V3 a b c (c) 0 1 2 3 V1 V4 V2 V3 a b c d Figure 6.23 (a) Single-phase full-bridge four-level FC converter. (b) Three-phase four-level FC converter. (c) Three-phase four-wire four-level FC converter. circuit for the four-level topology in Fig. 6.21(a), Fig. 6.22(b) shows its PWM signals. Notice that the voltages 𝑣∗ sin 1 , 𝑣∗ sin 2 , 𝑣carrier1, and 𝑣carrier2 furnish the switching states necessary for a symmetrical output voltage with four levels. Full-bridge four-level FC converters for both single-phase and three-phase loads are obtained by connecting the PBs as in Fig. 6.23(a) and 6.23(b), respectively. Figure 6.23(c) shows the option in which a three-phase four-wire system is required. 6.9 GENERALIZATION Following the same approach as for the three- and four-level configurations, the N-level converter can be obtained as in Fig. 6.24(e) for an odd value for N, and in Fig. 6.24(f) for an even value for N. Theoretically, the number of levels in an FC topology can be increased as far as necessary, although practical limitations do appear when the number of levels is higher than five. Note that the evolution from three to N levels is presented in Fig. 6.24(a) to Fig. 6.24(f). It is worth mentioning that the PBG brings a simple and intuitive aspect of connecting blocks for creation of FC topologies from three to N levels. The model and PWM strategy applied for
  • 211. 6.10 SUMMARY 197 (a) 0 1 2 V1 V3 V2 (b) 0 1 2 3 V1 V4 V2 V3 (c) 0 0 0 1 4 2 3 V1 V5 V4 V2 V3 (d) (e) (f) 0 1 4 5 2 3 V1 V6 V4 V5 V2 V3 Figure 6.24 Generation of the n-level FC topologies: (a) three-level, (b) four-level, (c) five-level, (d) six-level, (e) N-level (with N odd), and (f) N-level (with N even). the configurations with number of levels higher than four can be easily adapted from the previous discussion in this chapter. 6.10 SUMMARY This chapter was dedicated to the multilevel topologies that are characterized by the presence of the FC employed to generate different levels. For the sake of simplifica- tion, first the FC was substituted by a DC source and then the circuit with capacitor was presented along with the analysis to keep 𝑣c with minimum ripple. As in the case of other configurations in this book, such as neutral-point-clamped and cas- cade arrangements, FC topologies were presented in a systematic way following this sequence: (i) PB connections obtained from the rules presented in Chapter 3, (ii) once the topology was established the Table of Variables was obtained, (iii) model- ing the converter by writing the output voltage to describe what was obtained in the Table of Variables, and (iv) developing the PWM approach from the Table of Vari- ables. As a learning intervention, nonconventional converters were also employed in
  • 212. 198 CHAPTER 6 FLYING-CAPACITOR CONFIGURATION this chapter. There is an extensive technical literature on this topic some of which is given as References from 1 to 9. REFERENCES [1] Meynard TA, Foch H. Multilevel conversion: high voltage chopper and voltage source inverters. Pro- ceedings of IEEE PESC’92; 1992. p 397–403. [2] Meynard TA, Foch H, Thomas P, Courault J, Jakob R, Nahrstaedt M. Multicell converters: basic con- cepts and industry applications. IEEE Trans Ind Electron 2002;49(5):955–964. [3] Jeon J-H, Kim T-J, Kang D-W, Hyun D-S. A symmetric carrier technique of CRPWM for voltage balance method of flying capacitor multi-level inverter. IEEE Trans Ind Electron 2005;52(3):879–888. [4] Lin B-R, Hung T-L, Huang C-H. “Single-phase AC/AC converter with capacitor-clamped scheme”. IEE Proc-Electr Power Appl 2003;150(4):464–470. [5] Lin BR, Huang CH. Single-phase switching-mode rectifier with capacitor-clamped topology. IEE Proc-Electr Power Appl 2005;152(1):9–16. [6] Lin B-R, Huang C-H. Three-phase capacitor-clamped converter with fewer switches for use in power factor correction. IEE Proc-Electr Power Appl 2005;152(3):596–604. [7] Kou X, Corzine KA, Familiant Y. Full binary combination schema for floating voltage source multi-level inverters. IEEE Trans Power Electron 2002;17(6):891–897. [8] Jing Huang, Keith Corzine. Extended operation of flying capacitor multilevel inverters. Proceedings of IEEE IAS’ 04; 2004. p 813–819. [9] Radermacher H, Schmidt B, De Doncker R. Determination and comparison of losses of single phase multi-level inverters with symmetric supply. Proceedings of IEEE PESC’04; vol. 6; 2004. p 4428–4433.
  • 213. CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS 7.1 INTRODUCTION After dealing with either conventional power circuits for multilevel topologies or non- traditional configurations based on the three most used circuits (neutral point clamped (NPC), cascade, and flying capacitor (FC)), this chapter presents some other topolo- gies obtained independently. Such power circuits are also easily obtained from the axioms and postulates of the power blocks geometry (PBG) presented in Chapter 3. Although many of the circuits presented in this chapter have not been con- sidered in industrial applications, such converters have characteristics that bring up specific advantages as compared to the traditional circuits. Furthermore, the noncon- ventional multilevel configurations presented in this chapter have an important role in helping to understand how new topologies have been conceived in the literature. Such NPCs are presented, following the same procedure as before, with the following steps: (i) consider the PBs and the rules to determine the connection of blocks and consequently the connection of the power switches, (ii) determine a Table of Variables to associate the output voltage with binary variables (switching states), (iii) find an equation to describe the Table of Variables and consequently model the converter, and (iv) determine a simple pulse width modulation (PWM) approach to obtain the gating signals of the switches. The sections in this chapter deal with different types of nontraditional con- verters and are organized as follows: Section 7.2 presents the nested configuration achieved by connecting only the first and second PB-ac in an appropriate way. Section 7.3 shows an alternate way to obtain a multilevel output voltage with a coupled inductor placed at the output of the converter, as well as a topology known as mod- ular multilevel converter (MMC). Section 7.4 presents the ANPC topology, high- lighting its thermal stress reduction among the power switches. A series of other topologies are included in Section 7.5, which brings up a review stressing how the multilevel circuits proposed in the technical literature can be in fact obtained eas- ily from the Power Block Geometry approach. Finally, Section 7.6 summarizes this chapter. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 199
  • 214. 200 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS (a) (b) (c) (d) V1 V2 V3 V1 V2 V4 V3 V1 V2 V4 V3 V5 V1 V2 V4 V3 V6 V5 vo vo vo vo Figure 7.1 Nested multilevel configurations with the block representation: (a) three-level, (b) four-level, (c) five-level, and (d) six-level. 7.2 NESTED CONFIGURATION This section presents multilevel topologies based on the concept of nested arrange- ment. Such topologies are called nested multilevel converters because the external connections of the blocks involve the internal ones. Figure 7.1(a) shows a three-level circuit obtained with the first PB-ac and second PB-ac. Figure 7.1(b), 7.1(c), and 7.1(d) depict a four-, five-, and six-level converters, respectively. Once the topolo- gies are obtained via the power blocks, the circuits can be considered in their lower level (representation with switches), as presented in Fig. 7.2. Figure 7.2(a) and 7.2(b) show three- and four-level converters, respectively. The converters presented in this figure show both single-leg and three-phase versions of the nested configuration. Figure 7.2(c) shows the evolution from five to seven levels. When compared to the NPC topologies, the nested configurations can be con- sidered as an interesting option due to the reduced number of power diodes. A draw- back would be different blocking voltage per switch. Although Figs 7.1 and 7.2 present topologies able to generate a number of lev- els between 3 and 7, the analysis in this section will be focused on the four-level converter, which is enough to give the reader a comprehensive idea of how to deal with this family of multilevel converters. The converter leg in Fig. 7.2(b) (left side) is constituted by two controlled switches (q1 and q4) and two bidirectional controlled switches (q2 and q3). For the version of the converter with three legs, required in three-phase systems, there are six controlled switches (q1x and q4x – x = a, b, and c) and six bidirectional controlled
  • 215. 7.2 NESTED CONFIGURATION 201 (a) (b) (c) V1 V1 V1 V1 V1 V1 V4 V4 V4 V4 V4 V5 V5 V5 V6 V6 V7 V2 V2 V2 V2 V2 V3 V3 V3 V3 V3 V2 V3 V1 V2 V3 q2 q1 q1 q1 q5 q2 q2 q3 q4 q4 q4 q1a q1b q1c q2a q2b q2c q3a q3a q3 q3 q2 q2 q1 q1 q3b q3b q3c q3c q4a q4 q4 q5 q5 q6 q6 q7 q4b q4c q2a q2b q2c q1a q1b q1c q3 vo vo vo vo vo vc vb va vc vb va Figure 7.2 Nested multilevel configurations with the switches representation: (a) three-level, (b) four-level, and (c) evolution from five- to seven-level. switches (q2x and q3x). The Table of Variables for the leg of the nested topology with four levels is presented in Table 7.1. Such a table can be described by the following equation: 𝑣o = q1q2q3q4V1 + q1q2q3q4V2 + q1q2q3q4V3 + q1q2q3q4V4 (7.1) with qy = 1 − qy for y = 1, 2, 3, and 4.
  • 216. 202 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS TABLE 7.1 Table of Variables for the Four-Level Nested Converter State q1 q2 q3 q4 𝑣o 1 1 0 0 0 V1 2 0 1 0 0 V2 3 0 0 1 0 V3 4 0 0 0 1 V4 For the generation of a symmetrical waveform with the maximum output volt- age given by Vdc, the input voltage can be obtained as follows: V1 = 3Vdc∕4, V2 = Vdc∕4, V3 = −Vdc∕4, and V4 = −3Vdc∕4. In this case, it turns out that equation (7.1) becomes 𝑣o = (3q1q2q3q4 + q1q2q3q4 − q1q2q3q4 − 3q1q2q3q4)Vdc 4 (7.2) Figure 7.3(a)–7.3(d) shows the positive and negative currents through the switches q1, q2, q3, and q4 when these switches are turned on, respectively. Notice that the bidirectional controlled switches (q2 and q3) have been employed on the inner leg, while the switches (q1 and q4) have been used on the outer leg. Exercise 7.1 Explain what would happen if the positions of the switches placed on the inner and outer legs are switched, for example, if the figure below is used instead of Fig. 7.1(b). Justify your answer by using equivalent circuits such as in Fig. 7.3. V1 V2 V3 vo From the Table of Variables (Table 7.1), it is possible to determine a PWM solution as shown in Fig. 7.4. Notice that the PWM approach for the nested topology can be obtained with only one modulating signal and three carrier signals with a level shift technique. Figure 7.5 shows the simulated results for the nested configuration with four levels for a three-phase application. The waveforms presented in Fig. 7.5(a) and 7.5(b)
  • 217. 7.2 NESTED CONFIGURATION 203 (a) (b) (c) (d) q1 Vdc 3 4 + – Vdc 1 4 Vdc 1 4 + + 0 – – Vdc 3 4 + – q2 Vdc 3 4 + – Vdc 1 4 Vdc 1 4 + + 0 – – Vdc 3 4 + – q3 Vdc 3 4 + – Vdc 1 4 Vdc 1 4 + + 0 – – Vdc 3 4 + – q4 Vdc 3 4 + – Vdc 1 4 Vdc 1 4 + + 0 – – Vdc 3 4 + – Figure 7.3 Current flows through the switches when (a) q1 = 1, (b) q2 = 1, (c) q3 = 1, and (d) q4 = 1. are: (a) pole voltages; (b) from top to bottom: output line voltage, pole voltage, and phase current. Exercise 7.2 Compare the nested and the NPC topologies in terms of the blocking voltage for the switches employed in one leg. Assume that both topologies have four levels and are generating the same output voltage. Disregard any safety margin while specifying the voltages for each power switch.
  • 218. 204 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS driver driver driver driver + – + – + – q1 V1 V4 V2 V3 q1 q2 q2 q3 q3 q4 q4 vsin * vt1 * vt2 * vo vt3 * Figure 7.4 PWM approach for the nested configuration. (a) (b) 0.1 0.15 0 100 –100 0 100 –100 0 100 –100 v c0 (V) t(s) v b0 (V) v a0 (V) 0.1 0.15 0 0.105 0.11 0.12 0.13 0.14 0.15 0.115 0.125 0.135 0.145 0.105 0.11 0.12 0.13 0.14 0.15 0.115 0.125 0.135 0.145 100 –100 0 100 –100 0 1 –1 i b (A) t(s) v b0 (V) v ac (V) Figure 7.5 Three-phase four-level nested configurations: (a) pole voltages and (b) line-to-line voltage (top), pole voltage (middle), and load current (bottom). Although sometimes there are practical limits for the converters with a higher number of levels, the nested topology allows its generation with N levels for both cases, N being an odd and an even number. Figure 7.6 presents a generalization of the nested multilevel converters for an odd [see Fig. 7.6(a)] and even [see Fig. 7.6(b)] number of levels.
  • 219. 7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT 205 (a) (b) vo vo Figure 7.6 Generalization of nested multilevel converter with (a) odd and (b) even number of levels. 7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT A three-level voltage can be obtained either by using the nested topology (as described in Section 7.2) or by employing any of the conventional circuits (described in previous chapters). All circuits considered so far for generation of a three-level voltage at the output of the converter have been achieved by placing switches, sources, and/or capacitors appropriately, as seen in Fig. 7.7(a)–7.7(c). The figures of the NPC, H-bridge, and FC configurations are repeated here in order to compare their principles with an alternate way to generate a three-level voltage. Observing such topologies, it is possible to use different strategies to generate the same number of levels at the output converter side. For instance, Fig. 7.7(a) shows an NPC topology that creates three different paths to connect the input voltages V1, V2, and V3 to the output (𝑣o). The H-bridge circuit shown in Fig. 7.7(b) combines both inputs to obtain the desirable three-level output voltage, that is, V1 − V2, 0, V2 − V1. On the other hand, the FC topology in Fig. 7.7(c) associates sources (or sources and capacitors) in series to obtain the desirable levels at the output. By employing a different approach, Fig. 7.7(d) shows another way to imple- ment a three-level power converter. Such an arrangement, using a split-wound cou- pled inductor at the output converter side, guarantees a three-level output voltage with only two PBs-dc. The lower level representation of this converter is furnished
  • 220. 206 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS (a) (c) (b) (d) (e) 2 2 1 1 0 + – q1 q2 0 V1 V1 V3 V2 V1 V1 V2 V2 V2 V3 vo vo vo vo io iCM vo 2 Vdc + – 2 Vdc Figure 7.7 Three-level configurations: (a) NPC, (b) cascade, (c) flying capacitor, (d) configuration with two PB-dc and split-wound coupled inductors, and (e) representation of the converter in Fig. 7.7(d) with switches. in Fig. 7.7(e), which highlights the connections of the power switches and coupled inductor. It is assumed that the currents through the coupled inductor are in continuous conduction mode, that is, the current is always higher than zero. Figure 7.8(a), 7.8(b), 7.8(c), and 7.8(d) shows the equivalent circuit for the leg when (q1,q2) are given by (0,0), (0,1), (1,0), and (1,1), respectively. Table 7.2 shows the Table of Variables for this converter. Notice that the output voltage has three levels, as explained later. The voltages 𝑣10 and 𝑣20 [voltages from the points 1 and 2 to the dc-link capac- itor midpoint – “0” in Fig. 7.7(e)] can be expressed as a function of the state of the switches q1 and q2, as follows: 𝑣10 = (2q1 − 1) Vdc 2 (7.3) 𝑣20 = (2q2 − 1) −Vdc 2 (7.4) The pole voltages as in equations (7.3) and (7.4) lead to the model presented in Fig. 7.9(a). Then the output voltage 𝑣o with respect to “0” can be in turn written as 𝑣o = 1 2 (𝑣10 + 𝑣20) (7.5) Substituting (7.3) and (7.4) in (7.5) it is possible to write 𝑣o as a function only of the state of the switches and dc-link voltage 𝑣o = (q1 − q2) Vdc 2 (7.6)
  • 221. 7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT 207 (a) 1 2 0 + – off off vo io 2 Vdc + – 2 Vdc (b) 1 x2 0 + – off off vo io 2 Vdc + – 2 Vdc (c) 1 2 0 + – off on vo io 2 Vdc + – 2 Vdc (d) 1 2 0 + – on on vo io 2 Vdc + – 2 Vdc Figure 7.8 Equivalent circuits for the topology presented in Fig. 7.7(d): (a) q1 = q2 = 0, (b) q1 = 0 and q2 = 1, (c) q1 = 1 and q2 = 0, and (d) q1 = q2 = 1. TABLE 7.2 Pole Voltage as a Function of the Switching States q1 q2 𝑣10 𝑣20 𝑣o 0 0 −Vdc∕2 Vdc∕2 0 0 1 −Vdc∕2 −Vdc∕2 −Vdc∕2 1 0 Vdc∕2 Vdc∕2 Vdc∕2 1 1 Vdc∕2 −Vdc∕2 0 From the Table of Variables presented in Table 7.2 it is possible to define the PWM strategies as in Fig. 7.9(b). Figure 7.9(c) shows the main waveforms associated with this circuit.
  • 222. 208 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS driver driver + + – – q1 q2 q2 qx1 q1 vsin * vsin * vt1 * vt1 * + – vsin * vt2 * vt2 * vo vo vo v10 + – v20 0 (a) (b) (c) 1 2 q2 qx2 qx2 Figure 7.9 (a) Model of converter in Fig. 7.7(e). (b) PWM circuit. (c) Waveforms for generation of a three-level voltage. Example 7.1 Deduce equation (7.5) for the three-level topology presented in Fig. 7.7(e). Solution The output voltage 𝑣o can be written with respect to the point “0” in two differ- ent ways, 𝑣o = −𝑣x1 + 𝑣10 and 𝑣o = 𝑣x2 + 𝑣20, where 𝑣x1 and 𝑣x2 are the drop voltages on the coupled inductor for the upper and lower parts of the inductor, respectively. Adding both equations 𝑣o is easily obtained as (𝑣10 + 𝑣20)∕2 for the symmetrical case (𝑣x1 = 𝑣x2).
  • 223. 7.3 TOPOLOGY WITH MAGNETIC ELEMENT AT THE OUTPUT 209 (a) (c) (b) Vp Vn 0 0 0 0 vo vo1 vo2 vo3 vo Figure 7.10 Five-level topology with coupled inductor placed at the output converter side: (a) PBG representation, (b) representation with switches, and (c) three-phase version. More levels can be obtained by combining the solution with coupled inductor and NPC converter. The circuit depicted in Fig. 7.10 is a five-level topology with a PBG representation [see Fig. 7.10(a)] and with a representation using switches [see Fig. 7.10(b)]. Its three-phase version is presented in Fig. 7.10(c). Notice that in this converter the number of levels is higher than the input voltages available (Vp, 0, Vn), which follows the same characteristics of the three-level version in Fig. 7.7(e) – in the three-level case there are three levels obtained from only two voltages. Although many of the converters presented so far in this and previous chapters are suitable for high voltage high power applications, the MMC combines excellent
  • 224. 210 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS V1 V2 vc vb va Figure 7.11 Modular multilevel converter with PBs. output voltage waveforms, very high efficiencies and an overall high blocking voltage capability with reduced stress on the switching devices of each submodule. Those characteristics are desirable in applications such as high power motor drives. Figures 7.11 and 7.12 show this configuration with power blocks and switches, respectively. There are some challenges related to the operation point of view of this converter. They are capacitor voltage ripple control for each module as well as circulating current regulation. Each phase of the converter shown in Figs. 7.11 and 7.12 constitutes two branches of half-bridge converters (also known as submodules), series connected to dc terminals V1 and V2. Those branches are connected through inductors. The ac terminals (𝑣a, 𝑣b, and 𝑣c) are connected to the middle point of the inductors. In general terms, the ac voltage is controlled by changing the number of half-bridge converters connected to each leg. From Fig. 7.12 ia and the circulating current (icc) can be written, respectively, by ia = ia1 − ia2 (7.7) icc = ia1 + ia2 2 (7.8) Consequently the currents ia1 and ia2 can be expressed as a function of both circulating current and output ac current as follows: ia1 = icc + ia 2 (7.9) ia2 = icc − ia 2 (7.10) The circulating current is associated to the energy exchange between the phase leg and the dc-link source. In fact, the control strategy applied for this converter should guarantee the capacitor voltage control for each submodule as well as desired output voltages 𝑣a, 𝑣b, and 𝑣c.
  • 225. 7.4 ACTIVE-NEUTRAL-POINT-CLAMPED CONVERTERS 211 V1 V2 vc vb ia1 ia ia2 va Figure 7.12 Modular multilevel converter – representation with switches. 7.4 ACTIVE-NEUTRAL-POINT-CLAMPED CONVERTERS The converter presented in Fig. 7.13 shows another arrangement using only the first PB-ac, which is called ANPC configuration. Figure 7.13(a) shows the three-level topology, while Fig. 7.13(b) presents the four-level version of the ANPC circuit. Yet more levels can be reached by adding more blocks as done in Chapter 4 for the NPC converter. Notice that for this family of multilevel converters controlled switches are employed instead of power diodes (as in NPC configurations) to obtain zero voltage
  • 226. 212 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS (a) (b) (c) (d) (e) q1 d1 d2 q2 d io io io Figure 7.13 ANPC configuration: (a) three-level circuit, (b) four-level circuit, (c) zero output voltage with positive current, (d) second path for zero output voltage with positive current, and (e) zero output voltage with positive current for NPC converter.
  • 227. 7.4 ACTIVE-NEUTRAL-POINT-CLAMPED CONVERTERS 213 at the output of the converter. The main advantages as compared to the conventional NPC topology [see Fig. 7.7(a)] is a better balance distribution of losses, which allows an increase in the maximum output power. In general terms, the design of a multilevel power electronics converter can be established by limiting the switching frequency in order to meet the maximum allow- able losses. In this sense and assuming a high power density scenario, a topology such as NPC, with irregular power losses distribution, presents unequal junction tempera- ture distribution on the power converter circuit. As a direct consequence, some power devices become hotter than others, restricting the switching frequency even more. On the other hand, due to the presence of controlled power switches, the ANPC topology can allow alternative paths to obtain the same zero voltage at the output converter side. It turns out that it is possible to manage the losses distribution of the switches by changing these paths. For example, Fig. 7.13(c) depicts the ANPC topology for the case in which a zero voltage is obtained for positive output current. On the other hand, Fig. 7.13(d) shows the same case as before (zero voltage obtained at the output with positive current) reached by using an alternative circuit. Finally, Fig. 7.13(e) shows that for the NPC converter there is only one path to obtain zero level voltage at the output of the converter with a positive current. Since the heat sink is essential for the thermal stability and lifetime of the semiconductor devices and for operation of the power converter as a whole, its specifi- cation must guarantee heat transfer capability for the switches, especially those under the highest thermal stress. Indeed, such a characteristic of the ANPC topology pre- sented in Fig. 7.13(c) and 7.13(d) plays an important role in the thermal design of this converter. The irregular junction temperature among diodes and power switches of the NPC topology is presented in Fig. 7.14(a). The components d, q1, q2, d1, and d2 are the semiconductor devices in Fig. 7.13(e). To avoid such irregular junction tempera- ture among the power switches while synthesizing the desired voltage, Fig. 7.14(b) shows one leg of the ANPC topology with a PWM defined by the temperature of the devices, which means that the hot points can be avoided by using alternative paths highlighted in Fig. 7.13(c) and 7.13(d). (a) (b) q1 q1 q1 T2,T4 T3,T6 d1 d Junction temperature PWM Approach d2 q2 q2 q2 q3 q3 q4 q4 q5 q5 q6 q6 vsin * Figure 7.14 (a) Junction temperature among the semiconductor devices. (b) PWM strategy for the ANPC topology.
  • 228. 214 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS TABLE 7.3 Table of Variables for the ANPC Topology q1 q2 q3 q4 q5 q6 𝑣o 1 1 0 0 0 0 Vdc 0 1 0 0 1 0 0 0 0 1 0 0 1 0 0 0 0 1 0 1 −Vdc As mentioned previously, such irregular losses distribution can be avoided with the ANPC topology and a regulated loss-balancing system. This loss control strategy can be achieved by either measuring or estimating the junction temperature. From Table 7.3 it is possible to establish a PWM strategy, depending on the temperature either measured or estimated from each semiconductor device. 7.5 MORE MULTILEVEL CONVERTERS Since the goal of this section is to demonstrate that many topologies can be repre- sented by PBG, their presentation is limited to the description of the circuits with both blocks and switches. All analysis in terms of Table of Variables, model, and PWM can be obtained by the reader following a similar approach as in the previous chapters. Also, this section aims to reiterate that the power blocks and the rules and postulates presented in Chapter 3 are an interesting way to understand how the mul- tilevel configurations have been presented in the technical literature. By following the rules and using specific blocks, it is possible to, for example, obtain the config- uration depicted in Fig. 7.15, which has been named by the authors as active switch NPC (ASNPC). Figure 7.15(a) shows this converter under PBG representation, which employs four PBs-ac. The equivalent lower-level representation using power switches is presented in Fig. 7.15(b). The improvement brought up by this converter lies on the reduction of the average switching frequency for all power devices. The three-level configuration obtained using just the second PB-ac comes up with two different implementations as presented in Fig. 7.16(a) and 7.16(c). (a) (b) V1 V2 V3 V1 V2 V3 vo vo Figure 7.15 Three-level configuration ASNPC (a) blocks and (b) switches.
  • 229. 7.5 MORE MULTILEVEL CONVERTERS 215 (a) (c) (d) (e) (b) V1 V3 V1 V2 V2 V1 V3 V3 V3 V2 V1 V2 V2 V3 V1 vo vo vo vo vo Figure 7.16 Three-level topologies using the second PB-ac only. Figure 7.16(b) shows the same topology with switches. Considering the representa- tion with the power switches as in Fig. 7.16(d), it is evident that the four switches between the 𝑣o and V2 can be simplified by only two antiseries switches as in Fig. 7.16(e). Indeed, Fig. 7.16(a) and 7.16(c) end up with the same topology, as presented in Fig. 7.16(b) and 7.16(e). Figure 7.17 shows a family of multilevel topologies known as mixed NPC/FC converters. Figure 7.17(a) depicts such a mixed three-level converter using both PB-dc and PB-ac, while Fig. 7.17(b) shows it with only PBs-ac. The representa- tion with switches for those converters is presented in Fig. 7.17(c) and 7.17(d), respectively. Higher levels can be easily obtained by stacking more elements as in Fig. 7.17(e)–7.17(h). Another way to merge a FC with the first PB-ac is presented in Fig. 7.18. Figure 7.19 depicts a similar configuration using a second PB-ac instead of the first one. Finally, Fig. 7.20(a) shows that two PBs-ac can be vertically stacked, which creates a differential converter, and Fig. 7.20(b) and 7.20(c) present different ways to generate a four-level converter.
  • 230. 216 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS (a) (b) (c) (d) (e) (f) (g) (h) V1 V1 V1 V1 V1 V2 V3 V4 V2 V3 V4 V2 V3 V4 V2 V3 V1 V2 V3 V2 V3 vo vo vo vo vo V1 V2 V3 V4 vo vo V1 V2 V3 vo Figure 7.17 Mixed NPC/FC converter.
  • 231. 7.5 MORE MULTILEVEL CONVERTERS 217 (a) (b) V1 V2 V3 V3 V2 V1 vo vo Figure 7.18 Mixed NPC/FC converter using flying capacitor and first PB-ac. (a) (b) V2 V3 V3 V2 V1 V1 vo vo Figure 7.19 Mixed NPC/FC converter using flying capacitor and first/second PB-ac.
  • 232. 218 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS (a) (b) (c) Figure 7.20 (a) Differential converter. (b) Four-level converter obtained with the first PB-ac. (c) Asymmetrical four-level topology. 7.6 SUMMARY This chapter dealt with of nontraditional multilevel converters. The approach used, with the PBG, shows that there is a high number of possibilities for generation of multilevel topologies and such an approach helps to understand how many of these topologies have been desscribed in the technical literature. Although not
  • 233. REFERENCES 219 all possibilities have been deeply examined, three of them have been analyzed, considering the PBs and the rules to determine the connection of blocks, Table of Variables and model of the converter. There is an extensive number of possibilities of multilevel topologies to which this technique can be used. Some of them, indicated in References from 1 to 26 have been used in this chapter. REFERENCES [1] Bhagwat PM, Stefanovic VR. Generalized structure of a multilevel PWM inverter. IEEE Trans Ind Appl 1983;IA-19(6):1057–1069. [2] Holmes D, Lipo T. Pulse Width Modulation for Power Converters: Principles and Practice. Wiley-IEEE Press; 2003. [3] dos Santos Jr. EC, Muniz JHG, da Silva ERC. 2L3L inverter. Proceedings of COBEP; 2011. p 924–929. [4] dos Santos Junior EC, Muniz JHG, da Silva ERC, Jacobina CB. Nested multilevel configurations. IEEE Energy Conversion Congress and Exposition (ECCE); 2012. p 324–329. [5] Matsui K, Murai Y, Watanabe M, Kaneko M, Ueda F. A pulsewidth modulated inverter with parallel-connected transistors by using current sharing reactors. IAS Annual Meeting Conference 1985; 1985. p 1015–1019. [6] Fratta A, Griffero G, Nieddu S, Pellegrino G Villata F. Inductive three-level V.-supplied conversion cell by new hybrid coupling reactor family. Proceedings of IAS’02; 2002. p 2378–2385. [7] Salmon J, Ewanchuk J, Knight AM. PWM inverters using split-wound coupled inductors. IEEE Trans Ind Appl 2009;45(6):2001–2009. [8] Teixeira CA, McGrath BP, Holmes DG, Topologically reduced multilevel converters using comple- mentary unidirectional phase-legs. IEEE International Symposium on Industrial Electronics (ISIE); 2012. p 2007–2012. [9] Brückner T, Bernet S, Güldner H. The active NPC converter and its loss-balancing control. IEEE Trans Ind Electron 2005;52(3):855–868. [10] Bruckner T, Bernet S, Steimer PK. Feedforward loss control of three-level active NPC converters. IEEE Trans on Ind Appl 2007;43(6):1588–1596. [11] Andrejak JM, Lescure M. High voltage converters promising technological developments. Proc. Rec. EPE Conf.; 1987. p 1.159–1.162. [12] Choi NS, Cho JG, Cho GH. A general circuit topology of multilevel inverter. Proc. Rec. IEEE PESC; 1991. p 96–103. [13] Carpita M, S Tenconi. A novel multilevel structure for voltage source inverter. Proc. Rec. EPE Conf.; 1991. p 1.90–1.94. [14] Floricau D, Gateau G, Leredde A. New active stacked NPC multilevel converter: operation and fea- tures. IEEE Trans Ind Electron 2010;57(7):2272–2278. [15] Gateau G, Meynard TA, Foch H. Stacked multicell converter (SMC): properties and design. IEEE 32nd Annual Power Electronics Specialists Conference, PESC 2001; 2001 Jun 17–22; Vancouver, Canada; 2001. [16] Suh B-S, Hyun D-S. A new n-level high voltage inversion system. IEEE Trans Ind Electron 1997;44(1):107–115. [17] Peng F. A generalized multilevel inverter topology with self voltage balancing. IEEE Trans Ind Appl 2001;37(2). [18] Barbosa P, Steimer P, Steinke J, Winkelnkemper M, Celanovic N. Active-neutral-point-clamped mul- tilevel converters. Proc. IEEE Power Electron. Spec. Conf.; 2005. p 2296–2301. [19] da Silva ERC, Muniz JHG, dos Santos EC, Silva RNA, Barreto LH. Capacitor balance in a five-level based halfbridge converter by use of a mixed active-cell. IEEE Energy Conversion Congress and Exposition (ECCE); 2013. p 414–419. [20] Meilil J, Ponnaluri S, Serpa L, Steimer PK, Kolar JW. Optimized pulse patterns for the 5-level ANPC converter for high speed high power applications. IEEE IECON 06; 2006. p 2597–2592.
  • 234. 220 CHAPTER 7 OTHER MULTILEVEL CONFIGURATIONS [21] Meynard T, Lienhardt AM, Gateau G, Haederli Ch, Barbosa P. Flying capacitor multiCell converters with reduced stored energy. Proceedings of IEEE ISIE; 2006. p 914–918. [22] Ramos RR, Ruiz-Caballero D, Ortmann MS, Mussa SA. New symmetrical hybrid multilevel dc-ac converters. Proceedings of Power Electronics Specialists Conference (PESC2008); 2008. p 1916–1922. [23] Ratnayake KR, Ishikawa H, Wang D, Yoshida M, Watanabe T. Novel hybrid five level inverter. IPEC; 2000. p 2025–2028. [24] Chen A, Hu L, and He X. A novel type of combined multilevel converter topologies. The 30th Annual Conference of the IEEE Industrial Electronics Society; 2004. p 2290–2294. [25] Haque MT. Series sub-multilevel voltage source inverters (MLVSIs) as a high quality MLVSI. Pro- ceedings of SPEEDAM; 2004. p F1B-1–F1B-4. [26] Babaei E. A cascade multilevel converter topology with reduced number of switches. IEEE Trans Power Electron 2008;23(6):2657–2664.
  • 235. CHAPTER 8 OPTIMIZED PWM APPROACH 8.1 INTRODUCTION Many pulse width modulation (PWM) approaches have been proposed by authors throughout the years for the systems studied in this book, that is, dc–ac and ac–dc–ac power conversions. In general terms, it is possible to sort the PWM strategies into two main categories: (i) sinusoidal pulse width modulation (SPWM) and (ii) space vector modulation (SVPWM). In SPWM, introduced by Schonnung in 1964 [1], to produce the output voltage waveform, a sinusoidal control signal (modulating signal) is compared to a triangular signal (carrier signal). SVPWM uses a complex voltage vector to define the pulse widths. Although one of the first suggestions for employing complex voltage vectors in a PWM control was made by Jardan [2], the SVPWM technique was first published by Busse and Holtz [3] followed by Pfaff et al. [4], in the same year. The majority of the PWM approaches presented in the previous chapters of this book can be classified as SPWM. For each of the configurations studied so far, inten- sive research has developed PWM strategies, bringing different levels of optimization in terms of the THD of the waveforms generated and also in terms of the efficiency of the converter. As a direct consequence of the high volume of research devoted to this topic, several improvements have been observed since the first studies. For instance, modification of the modulating signal has introduced many improvements to the SPWM technique, resulting in nonsinusoidal carrier-based PWM (CPWM) techniques [5–8]. After the reports by Buja and Indri [9] it has been gradually rec- ognized that the addition of an adequate third-harmonic zero-sequence component to each of the reference pole voltage increases 15.5% of the fundamental component of the output voltages in a three-phase converter. As concluded by Depenbrock [10], more than introducing the benefit of 15.5%, the zero sequence component can be used to reduce the number of times the switches are turned on and off, by clamping each pole voltage during 60∘ of the sinusoidal waveform. This chapter presents some techniques for optimization of the PWM approach considering the fact that the number of pole voltages is higher than the number of voltages demanded by the load, and then there is a degree of freedom to be explored. For instance, in Fig. 8.1 there is one degree of freedom for the H-bridge converter supplying a single-phase load. There are two pole voltages available (𝑣10 and 𝑣20) Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 221
  • 236. 222 CHAPTER 8 OPTIMIZED PWM APPROACH Vdc 0 1 2 iq1 iq2 + – + vo io – q1 q2 q1 q2 Figure 8.1 Converter with two legs supplying a single-phase load. at the converter side and just one voltage (𝑣o) must be controlled. Following this introduction, this chapter is organized in seven sections. Sections 8.2 and 8.3 show an optimized PWM strategy for converters with two and three legs, respectively. For both sections, a PWM approach is presented with both analog and digital implemen- tations, and finally the influence of the parameter 𝜇 is addressed for the quality of the waveform generated as well as for the losses of the converter. Section 8.4 deals with space vector modulation for a three-phase converter, while Section 8.5 presents the CPWM for both a three-leg converter feeding a two-phase symmetrical machine and a four-leg converter supplying a three-phase four-wire load. The CPWM is also employed in non-conventional converters (Section 8.6), such as split-wound coupled inductors, Z-source converter, and open-end winding motor. 8.2 TWO-LEG CONVERTER 8.2.1 Model A two-leg converter, as seen in Fig. 8.1, consists of four power switches q1, q1, q2, and q2. Note that the circuitry necessary to generate the gating signals is not presented in this figure. The upper (q1 and q2) and bottom (q1 and q2) switches are complemen- tary, which means that q1 = 1 − q1 and q2 = 1 − q2. As considered in the previous chapters, the conduction state of all switches can be represented by the binary vari- able with qx = 1 indicating a closed switch and qx = 0 indicating an open one (with x = 1 and 2). The pole voltages 𝑣10 and 𝑣20 can be defined as a function of the switching states, as follows: 𝑣10 = (2q1 − 1) Vdc 2 (8.1) 𝑣20 = (2q2 − 1) Vdc 2 (8.2)
  • 237. 8.2 TWO-LEG CONVERTER 223 TABLE 8.1 Voltages and Currents of the Switches as a Function of the Switching States Switching Voltages Across the Currents through the States Switches Switches q1 q2 𝑣q1 𝑣q1 𝑣q2 𝑣q2 iq1 iq1 iq2 iq2 0 0 Vdc 0 Vdc 0 0 io 0 io 0 1 Vdc 0 0 Vdc 0 io io 0 1 0 0 Vdc Vdc 0 io 0 0 io 1 1 0 Vdc 0 Vdc io 0 io 0 The output voltage is given by 𝑣o = 𝑣10 − 𝑣20 (8.3) 𝑣o = (q1 − q2)Vdc (8.4) Note that there are two control variables (switching states q1 and q2) to define just one output voltage (𝑣o). While the load voltage is generated by the converter, the load current (io) depends on the load connected to the converter (io = 𝑣o∕Z, where Z is the impedance for a linear load). The voltages across the switches and currents through the switches are presented in Table 8.1. From Table 8.1, the following equations can be used to define the voltage and currents of the switches: 𝑣qx = (1 − qx)Vdc (8.5) 𝑣qx = qxVdc (8.6) iqx = qxio (8.7) iqx = (1 − qx)io (8.8) with x = 1, 2. 8.2.2 PWM Implementation From equation (8.3) it is possible to define the desired output voltage as a function of the reference pole voltages, as follows: 𝑣∗ o = 𝑣∗ 10 − 𝑣∗ 20 (8.9) A reference voltage [𝑣∗ o = V∗ o cos(𝜔ot)] must be synthesized through two refer- ence pole voltages (𝑣∗ 10 and 𝑣∗ 20 ), which means one degree of freedom to be explored. Then, an auxiliary variable (𝑣∗ h ) can be defined to allow some level of improvement. In this case it is possible to write: 𝑣∗ 10 = 𝑣∗ o + 𝑣∗ h (8.10) 𝑣∗ 20 = 𝑣∗ h (8.11)
  • 238. 224 CHAPTER 8 OPTIMIZED PWM APPROACH Equation (8.9), in principle, is satisfied for any value of 𝑣∗ h . However, the aux- iliary voltage must be obtained in order to guarantee that the reference pole voltages are limited as follows: −Vdc 2 ≤ 𝑣∗ 10 ≤ Vdc 2 (8.12) −Vdc 2 ≤ 𝑣∗ 20 ≤ Vdc 2 (8.13) When equations (8.12)–(8.13) are satisfied, it is said that the converter is oper- ating in its linear region. The following development in this subsection aims to deter- mine an analytical expression for 𝑣∗ h , and consequently defining 𝑣∗ 10 and 𝑣∗ 20 for PWM implementation. Substituting (8.10) and (8.11) into (8.12) and (8.13), it is possible to write: (a) Inequality 1. 𝑣∗ h ≥ −Vdc 2 − 𝑣∗ o; (b) Inequality 2. 𝑣∗ h ≥ −Vdc 2 ; (c) Inequality 3. 𝑣∗ h ≤ Vdc 2 − 𝑣∗ o; (d) Inequality 4. 𝑣∗ h ≤ Vdc 2 . As long as 𝑣∗ o is a sinusoidal waveform, it can assume either positive or neg- ative values; then we have two cases, Case 1: when 𝑣∗ o > 0 and Case 2: for 𝑣∗ o < 0. Figure 8.2 shows the hatched area (feasible region) relative to inequalities 1 and 2 for Case 1, while Fig. 8.3 shows the same inequalities for Case 2. Even with 𝑣∗ o being a sinusoidal waveform, it appears in the following analysis (Figs 8.2–8.5) as a constant due to the short interval of time considered. Note that in Case 1 (Fig. 8.2) the inequality 1 is predominant over inequality 2 (since satisfying inequality 1, the inequality 2 will be necessarily satisfied), while in Case 2 inequality 2 is predominant. Then, equation (8.14) is enough to succinctly describe both scenarios presented in Figs 8.2 and 8.3: 𝑣∗ h ≥ −Vdc 2 − MAX{𝑣∗ o, 0} (8.14) Equation (8.14) is a generic way to present inequalities 1 and 2, and it is equiv- alent to the graphical analysis depicted in Figs 8.2 and 8.3. A similar approach can be used for inequalities 3 and 4. Figure 8.4 shows the hatched area (feasible region) related to inequalities 3 and 4 for Case 1, while Fig. 8.5 shows the same inequalities for Case 2. Note that in Case 1 inequality 4 is predomi- nant, while in Case 2 inequality 3 must be satisfied. Then, it is possible to write 𝑣∗ h in a short way as presented in 𝑣∗ h ≤ Vdc 2 − MIN{𝑣∗ o, 0} (8.15)
  • 239. 8.2 TWO-LEG CONVERTER 225 (a) (b) vo * t t t * (Case 1: vo >0) –Vdc 2 Inequality 1: Feasible region Inequality 2: Feasible region 0 Vdc 2 –Vdc 2 0 Vdc 2 0 –Vdc 2 Vdc 2 vo * – – Vdc 2 Figure 8.2 (a) Limits of 𝑣∗ h when 𝑣∗ o > 0 (Case 1). (b) Feasible region for inequality 1 (left) and inequality 2 (right). (a) (b) vo * t t t * (Case 2: vo <0) –Vdc 2 Inequality 1: Feasible region Inequality 2: Feasible region 0 Vdc 2 –Vdc 2 0 Vdc 2 0 –Vdc 2 Vdc 2 vo * + – Vdc 2 Figure 8.3 (a) Limits of 𝑣∗ h when 𝑣∗ o < 0 (Case 2). (b) Feasible region for inequality 1 (left) and inequality 2 (right).
  • 240. 226 CHAPTER 8 OPTIMIZED PWM APPROACH (a) (b) vo * t t t * (Case 1: vo >0) –Vdc 2 Inequality 3: Feasible region Inequality 4: Feasible region 0 Vdc 2 –Vdc 2 0 Vdc 2 –Vdc 2 0 Vdc 2 vo * – Vdc 2 Figure 8.4 (a) Limits of 𝑣∗ h when 𝑣∗ o < 0. (b) Feasible region for inequality 3 (left) and inequality 4 (right). (a) (b) vo * t t t * (Case 2: vo <0) –Vdc 2 Inequality 3: Feasible region Inequality 4: Feasible region 0 Vdc 2 –Vdc 2 0 Vdc 2 –Vdc 2 0 Vdc 2 vo * + Vdc 2 Figure 8.5 (a) Limits of 𝑣∗ h when 𝑣∗ o < 0. (b) Feasible region for inequality 3 (left) and inequality 4 (right).
  • 241. 8.2 TWO-LEG CONVERTER 227 As in equation (8.14), equation (8.15) can be used instead of employing the graphical analysis depicted in Figs 8.4 and 8.5. Hence, it is possible to write equations (8.14) and (8.15) together, as: −Vdc 2 − MAX{𝑣∗ o, 0} ≤ 𝑣∗ h ≤ Vdc 2 − MIN{𝑣∗ o, 0} (8.16) or −Vdc 2 − Vmax ≤ 𝑣∗ h ≤ Vdc 2 − Vmin (8.17) where Vmax = MAX{𝑣∗ o, 0} and Vmin = MIN{𝑣∗ o, 0}. For the operation inside a linear region [see equations (8.12) and (8.13)] 𝑣∗ h must be considered between the limits presented in equation (8.17) and observed in Fig. 8.6(a). Note from this figure that the lower and upper values for 𝑣∗ h are V1 and V2, respectively. These voltages are defined as follows: V1 = (−Vdc∕2) − Vmax and V2 = (Vdc∕2) − Vmin. It is possible to create an index 𝜇 (distribution factor) in such a way that the voltage 𝑣∗ h can be changed proportionally as a function of 𝜇, as observed in Fig. 8.6(b), with 0 ≤ 𝜇 ≤ 1. Therefore, the equation of the line in Fig. 8.6(b) can be defined as follows: 𝑣∗ h(𝜇) = V1 + (V2 − V1)𝜇 (8.18) By developing equation (8.18), 𝑣∗ h = Vdc ( 𝜇 − 1 2 ) + (𝜇 − 1)Vmax − 𝜇Vmin (8.19) 0 0 (a) (b) 0.5 1 vh * vh * μ V2 V1 t –Vdc 2 – Vmax V1 = –Vdc 2 – Vmin V2 = Figure 8.6 (a) Limits of 𝑣∗ h . (b) 𝑣∗ h as a function of the distribution factor.
  • 242. 228 CHAPTER 8 OPTIMIZED PWM APPROACH With 𝑣∗ h defined as in (8.19), the reference pole voltages (𝑣∗ 10 and 𝑣∗ 20 ) presented in (8.10), (8.11) are used either to compare with a high frequency triangular waveform (in the analog solution) or to generate timer counters (in the digital solution). Example 8.1 Determine the waveforms for 𝑣∗ 10 and 𝑣∗ 20 when 𝜇 = 0.5 (distribution factor) and assuming 𝑣∗ o = V∗ o cos(𝜔ot). Solution To determine the waveforms for 𝑣∗ 10 and 𝑣∗ 20 , from (8.10) and (8.11), it is nec- essary to find 𝑣∗ h , as in equation (8.19). Equation (8.19) with 𝜇 = 0.5 becomes 𝑣∗ h = −1∕2(V∗ min + V∗ max). As defined earlier, Vmax = MAX{𝑣∗ o, 0} and Vmin = MIN{𝑣∗ o, 0}, which means that: (a) When 𝑣∗ o > 0, Vmax = 𝑣∗ o and Vmin = 0 (b) When 𝑣∗ o ≤ 0, Vmax = 0 and Vmin = 𝑣∗ o. Hence, 𝑣∗ h is equal to −1∕2(𝑣∗ o) for both cases 𝑣∗ o > 0 and 𝑣∗ o ≤ 0. Therefore, 𝑣∗ 10 = 1 2 𝑣∗ o and 𝑣∗ 20 = −1 2 𝑣∗ o. The waveforms for 𝑣∗ 10 and 𝑣∗ 20 are two sinusoidal waves with the same amplitude but 180∘ apart. 8.2.3 Analog and Digital Implementation Figure 8.7 shows the analog implementation of the PWM solution for the two-leg converter as depicted in Fig. 8.1. Note that the reference pole voltages, obtained from equations (8.10)–(8.11) are compared to the carrier signal 𝑣∗ t with amplitude equal to Vt. The relationship between the amplitude of the modified voltages 𝑣∗ j0 (i.e., V∗ j0 –with j = 1, 2) and Vt defines the amplitude modulation ratio (ma = V∗ j0 ∕Vt). On the other hand, the relationship between the switching frequency (fs – frequency of the carrier signal) and the frequency of the sinusoidal waveform (fo) defines the frequency modulation ratio (mf = fs∕fo). v10 * v20 * 0 vo * vh * vt * μ q1 Equation (8.19) – + – + Vdc * VMAX MAX MIN * VMIN q1 q2 q2 Figure 8.7 Analog PWM implementation.
  • 243. 8.2 TWO-LEG CONVERTER 229 Example 8.2 Considering 𝜇 = 0.5, determine the load voltage 𝑣o assuming the amplitude modulation ratio (ma) equal to infinite. Solution By definition ma is given by V∗ j0 ∕Vt, which means that for a modulation ratio equal to infinite the amplitude of the sinusoidal waveform is always higher than the carrier signal amplitude. Then, qj = 1 if 𝑣∗ j0 > 0 and qj = 0 if 𝑣∗ j0 < 0 with j = 1, 2. Then the load voltage will be a square waveform with the same frequency of 𝑣∗ o and with amplitude equal to Vdc. The equivalent digital solution can be obtained as an alternative for the analog PWM implementation by defining the time in which the switches (q1 and q2) are on. For determination of the pulse widths, used to define when the switches are either on or off (i.e., emulating the OpAmp operation in Fig. 8.7), it is assumed that the modified reference voltages 𝑣∗ 10 and 𝑣∗ 20 are constants over the switching period Ts. From Fig. 8.8, this hypothesis (i.e., 𝑣∗ 10 and 𝑣∗ 20 constants over Ts) becomes more accurate as the switching frequency becomes much higher than the frequency of the modulating signal (i.e., fs ≫ fo). Then, assuming that the triangular frequency is high enough to guarantee the condition in Fig. 8.8(b), the average values of 𝑣10 and 𝑣20 over Ts should be equal to the medium values of 𝑣∗ 10 and 𝑣∗ 20 , respectively. Figure 8.9 shows the waveforms for the first leg highlighting that the medium values of 𝑣∗ 10 and 𝑣10 must be equal. Hence, it is possible to write 1 Ts ∫ t+Ts t 𝑣∗ 10(t)dt = 1 Ts ∫ t+Ts t 𝑣10(t)dt (8.20) 1 Ts ∫ t+Ts t 𝑣∗ 20(t)dt = 1 Ts ∫ t+Ts t 𝑣20(t)dt (8.21) Since 𝑣∗ 10 and 𝑣∗ 20 are assumed to be constant over Ts, 𝑣∗ 10 = [ Vdc 2 𝜏1 − Vdc 2 ( Ts − 𝜏1 ) ] 1 Ts (8.22) 𝑣∗ 20 = [ Vdc 2 𝜏2 − Vdc 2 ( Ts − 𝜏2 ) ] 1 Ts (8.23) where 𝜏1 and 𝜏2 are the time in which the switches q1 and q2 are on.
  • 244. 230 CHAPTER 8 OPTIMIZED PWM APPROACH zoom zoom vt * vt * vt * v10 * v10 * v10 * vt * v10 * (a) (b) Figure 8.8 Comparison of high frequency triangular and sinusoidal waveforms: (a) low frequency modulation ratio and (b) high frequency modulation ratio. v10 Ts A1 A2 A3 vt * avg {v10} = A2–A1–A3 * v10 * τ1 Figure 8.9 Average value of 𝑣∗ 10 equal to the average value 𝑣10. From expressions (8.22)–(8.23) it is possible to calculate the time intervals in which the switches q1 and q2 are on, that is 𝜏1 = ( 𝑣∗ 10 Vdc + 1 2 ) Ts (8.24) 𝜏2 = ( 𝑣∗ 20 Vdc + 1 2 ) Ts (8.25) After the definition of the pulse widths (𝜏1 and 𝜏2), it is necessary to pro- gram timers for implementation with either a digital signal processing (DSP) or a field-programmable gate array (FPGA) device, for instance.
  • 245. 8.2 TWO-LEG CONVERTER 231 Exercise 8.1 Assume a single-phase dc–ac converter as in Fig. 8.1 with Vdc = 100V. Also consider two ways to generate the PWM signals: (i) analog implementation with OpAmps with maximum voltage allowed equal to 15V (due to operation restrictions of the OpAmps), that is, maximum voltage for 𝑣∗ 10 , 𝑣∗ 20 , and 𝑣∗ t , must be equal to 15V; and (ii) digital implementation with the code written in C++ for a DSP, with 𝑣∗ 10 = 50 sin(𝜔t) and 𝑣∗ 20 = 50 sin(𝜔t + 180∘). Question: Is it possible to generate a desirable ac output voltage with amplitude equal to 100V for both analog and digital implementations as described before? 8.2.4 Influence of 𝝁 for PWM Implementation The parameter 𝜇 and consequently 𝑣∗ h play an important role in the PWM imple- mentation described already. As mentioned earlier, the distribution factor (𝜇) can be employed to optimize the converter operation. For instance, to emphasize such an vt * vh * vo * v10 * v10 –1 0.1 0.11 0.12 0 1 –1 0 1 io vo v20 * v20 –1 0.1 0.11 0.12 0 1 –1 0 1 Figure 8.10 Waveforms obtained with 𝜇 = 0.5. vt * vh * vo * v10 * v10 –1 0.1 0.11 0.12 0 1 –1 0 1 io vo v20 * v20 –1 0.1 0.11 0.12 0 1 –1 0 1 Figure 8.11 Waveforms obtained with 𝜇 = 0.0.
  • 246. 232 CHAPTER 8 OPTIMIZED PWM APPROACH vt * vh * vo * v10 * v10 –1 0.1 0.11 0.12 0 1 –1 0 1 io vo v20 * v20 –1 0.1 0.11 0.12 0 1 –1 0 1 Figure 8.12 Waveforms obtained with 𝜇 = 1.0. optimization, a set of the main converter’s variables are shown in Figs 8.10, 8.11, and 8.12 for 𝜇 equal to 0.5, 0.0, and 1.0, respectively. Notice that those results are normal- ized and the maximum value is always one for both power and control waveforms. Figure 8.10 shows the case with symmetrical waveforms (𝑣∗ 10 and 𝑣∗ 20 ) obtained with 𝜇 = 0.5, which represents the best option in terms of the total harmonic distortion (THD). Note that the ripple of the current in this result is lower than that shown in Figs 8.11 and 8.12. On the other hand, 𝜇 = 0 and 𝜇 = 1 generate asymmetrical waveforms (see Figs 8.11 and 8.12) with the main advantage related to the switching losses reduc- tion. There is a large period of time (180∘ of the modulating signal) in which there is no switching for either 𝑣10 or 𝑣20. It is important to highlight that although 𝜇 plays an important role creating waveforms with distortions to deal with either THD improvement or loss reduction, these parameters (𝜇 and consequently 𝑣∗ h ) will not change the lengths of the active states, as observed in Fig. 8.13. Example 8.3 Why does the load current (io) for all values of 𝜇 have the same average value? Does it change if another value for 𝜇 is chosen rather than 0.5, 0.0, or 1.0, for example 𝜇 = 0.3? Solution Even with different instantaneous load voltages due to different values of 𝑣∗ h , as observed in Figs 8.10–8.12, the average values of 𝑣o should be the same since the common term 𝑣∗ h is cancelled [see equation (8.9)]. That is why the amplitude value of the load current is kept constant. Another explanation can be obtained from Fig. 8.13, which shows the unchanged active vector length by either using 𝑣∗ h or not, that is, if the same active vectors are applied, the same amplitude for the currents is expected.
  • 247. 8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 233 v10 vh * vh * vt v10 * v20 * v20 Active states Ts Figure 8.13 Influence of 𝑣∗ h on the active states generation. Vdc n 0 1 2 3 iq1 iq2 iq3 – + + v1 i1 i2 i3 – + v2 – + v3 – q1 q2 q3 q1 q2 q3 Figure 8.14 Three-leg converter supplying a three-phase load. 8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 8.3.1 Model A three-leg converter, as seen in Fig. 8.14, is constituted by six power switches q1, q1, q2, q2, q3, and q3. For simplification purposes, the circuitry necessary to generate the gating signals is not presented in this figure; instead just the power part of the circuit has been presented. The upper (q1, q2, and q3) and bottom (q1, q2, and q3) switches are complementary, which means that qx = 1 − qx (with x = 1, 2, 3). The conduction state of all switches can also be represented by a binary variable with qx = 1 indicating a closed switch and qx = 0 indicating an open one.
  • 248. 234 CHAPTER 8 OPTIMIZED PWM APPROACH The pole voltages 𝑣10, 𝑣20, and 𝑣30 can be defined as a function of the switching states, as follows: 𝑣10 = (2q1 − 1) Vdc 2 (8.26) 𝑣20 = (2q2 − 1) Vdc 2 (8.27) 𝑣30 = (2q3 − 1) Vdc 2 (8.28) The output voltages (𝑣1, 𝑣2, and 𝑣3) are given by 𝑣1 = 𝑣10 − 𝑣n0 (8.29) 𝑣2 = 𝑣20 − 𝑣n0 (8.30) 𝑣3 = 𝑣30 − 𝑣n0 (8.31) Considering a balanced three-phase system (i.e., 𝑣1 + 𝑣2 + 𝑣3 = 0) and from (8.29)–(8.31), it is possible to define 𝑣n0 as in equation (8.32): 𝑣n0 = 1 3 (𝑣10 + 𝑣20 + 𝑣30) (8.32) Substituting (8.32) into (8.29)–(8.31), we get 𝑣1 = 2 3 𝑣10 − 1 3 𝑣20 − 1 3 𝑣30 (8.33) 𝑣2 = − 1 3 𝑣10 + 2 3 𝑣20 − 1 3 𝑣30 (8.34) 𝑣3 = − 1 3 𝑣10 − 1 3 𝑣20 + 2 3 𝑣30 (8.35) Note that it is possible to explore the redundancy inherent in a three-phase sys- tem. When two voltages are controlled, the third is indirectly controlled, such as: 𝑣3 = −(𝑣1 + 𝑣2). Substituting (8.26)–(8.28) into (8.33)–(8.35), it is possible to write the output voltages only as a function of the state of the switches: 𝑣1 = [ 2 3 q1 − 1 3 q2 − 1 3 q3 ] Vdc (8.36) 𝑣2 = [ − 1 3 q1 + 2 3 q2 − 1 3 q3 ] Vdc (8.37) 𝑣3 = −𝑣1 − 𝑣2 (8.38) The three-leg converter supplying a three-phase load (Fig. 8.14) also presents a degree of freedom. Note that there are only two output voltages to be controlled (𝑣1 and 𝑣2 – or any other combination of two voltages among 𝑣1, 𝑣2, and 𝑣3) throughout three controlled variables q1, q2, and q3. While the load voltages are generated by the converter, the load currents (i1, i2, and i3) depend on the load connected to the converter. In the case of a linear load, it can be written as ix = 𝑣x∕Zx, where Zx is the load impedance for phase x; with x = 1, 2, 3. The voltages and currents through the switches are presented in Table 8.2.
  • 249. 8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 235 TABLE 8.2 Voltages and Currents of the Switches as a Function of the Switching States Switching Voltages of the Currents of the States Switches Switches qx 𝑣qx 𝑣qx iqx iqx 0 Vdc 0 0 il 1 Vdc 0 il 0 From Table 8.2, the following equations can be used to define the voltage and currents of the switches, respectively. 𝑣qx = (1 − qx)Vdc (8.39) 𝑣qx = qxVdc (8.40) iqx = qxix (8.41) iqx = (1 − qx)ix (8.42) with x = 1, 2, 3. 8.3.2 PWM Implementation From equations (8.29)–(8.31) it is possible to define the desired output voltages as a function of both reference pole voltages and voltage 𝑣∗ n0 , as follows: 𝑣∗ 1 = 𝑣∗ 10 − 𝑣∗ n0 (8.43) 𝑣∗ 2 = 𝑣∗ 20 − 𝑣∗ n0 (8.44) 𝑣∗ 3 = 𝑣∗ 30 − 𝑣∗ n0 (8.45) The voltage 𝑣∗ n0 can be considered as an auxiliary variable (𝑣∗ h ) which is expected to bring a level of optimization for the converter, as for the single-phase converter presented previously. If the desired balanced three-phase voltages are given by 𝑣∗ 1 = V∗ o cos(𝜔ot), 𝑣∗ 2 = V∗ o cos(𝜔ot + 120∘), and 𝑣∗ 3 = V∗ o cos(𝜔ot − 120∘), the reference pole voltages can be defined by: 𝑣∗ 10 = 𝑣∗ 1 + 𝑣∗ h (8.46) 𝑣∗ 20 = 𝑣∗ 2 + 𝑣∗ h (8.47) 𝑣∗ 30 = 𝑣∗ 3 + 𝑣∗ h (8.48) with 𝑣∗ h = Vdc ( 𝜇 − 1 2 ) + (𝜇 − 1)Vmax − 𝜇Vmin (8.49) where Vmax = MAX{𝑣∗ 1 , 𝑣∗ 2 , 𝑣∗ 3 } and Vmin = MIN{𝑣∗ 1 , 𝑣∗ 2 , 𝑣∗ 3 }; 𝜇 is the distribution factor and determines how the free-wheeling time interval can be distributed through- out the switching period.
  • 250. 236 CHAPTER 8 OPTIMIZED PWM APPROACH Equations (8.19) and (8.49) are identical equations, just changing the terms Vmax and Vmin. In fact, 𝑣∗ h is a generalized expression that can be employed in different power converters processing ac voltage, as discussed later in this chapter. 8.3.3 Analog and Digital Implementation Figure 8.15 shows the analog implementation of the PWM solution for the three-leg converter depicted in Fig. 8.14. The reference pole voltages are obtained as in equations (8.46)–(8.48) and compared to the carrier signal 𝑣∗ t . Following the same approach employed for the single-phase converter, it is possible to calculate the time intervals in which the switches q1, q2, and q3 are on, that is 𝜏1 = ( 𝑣∗ 10 Vdc + 1 2 ) Ts (8.50) 𝜏2 = ( 𝑣∗ 20 Vdc + 1 2 ) Ts (8.51) 𝜏3 = ( 𝑣∗ 20 Vdc + 1 2 ) Ts (8.52) After defining the pulse widths (𝜏1, 𝜏2, and 𝜏3), it is necessary to program three timers associated with each leg. 8.3.4 Influence of 𝝁 for PWM Implementation in a Three-Leg Converter As considered for the two-leg converter, the voltage 𝑣∗ h can be used to optimize spe- cific parameters such as weighted total harmonic distortion (WTHD) and losses. v1 * v10 * v20 * v30 * v2 * v3 * vh * vt * μ q1 Equation (8.49) – + – + – + Vdc * VMAX MAX MIN * VMIN q1 q2 q2 q3 q3 Figure 8.15 Analog PWM implementation for the three-leg converter.
  • 251. 8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 237 vt * v1 * v10 i3 0.09 –1 0 1 –1 0 0 1 –1 1 0.105 (a) (b) 0.12 i2 i1 vt * v1 * v10 i3 0.09 –1 0 1 –1 0 0 1 –1 1 0.105 0.12 i2 i1 Figure 8.16 Waveforms obtained with: (a) 𝜇 = 0.5 and (b) 𝜇 = 1.0. 0 WTHD 0.5 1 μ Figure 8.17 WTHD versus 𝜇. Figure 8.16(a) and 8.16(b) shows the main waveforms for 𝜇 equal to 0.5 and 0, respec- tively. While Fig. 8.17 shows the WTHD of the load phase voltage as a function of 𝜇, Fig. 8.18 shows the same waveforms as in Fig. 8.16 with 𝜇 changing from 0 to 1 six times per period. Note that 𝜇 = 0.5 generates symmetrical waveforms with the benefit of better WTHD. On the other hand, 𝜇 = 0 leads to benefits in terms of loss reduction due to the clamped pole voltages. One way to bring up the benefits of both 𝜇 = 0.5 and 𝜇 = 1.0 is to change the parameter 𝜇 from 0 to 1 many times inside the sine period. This will guarantee an average value of 0.5 while keeping the pole voltages clamped.
  • 252. 238 CHAPTER 8 OPTIMIZED PWM APPROACH vt * vl1 * v10 i3 0.09 –1 0 1 –1 0 1 –1 1 0.105 0.12 i2 i1 Figure 8.18 Waveforms with 𝜇 changing from 0 to 1. 8.3.5 Influence of the Three-Phase Machine Connection over Inverter Variables Traditionally, a three-phase machine is designed to be connected in a wye (Y) or delta (Δ) arrangement depending on the voltage level available from the utility grid. In a motor drive system, the connections of the three-phase machine can still be defined as a function of the voltage level available on the dc-link capacitor. If the dc-link voltage for a given application is not restrictive, the choice between both possibil- ities of machine connections [Y – see Fig. 8.19(a) or Δ – see Fig. 8.19(b)] favors the Y connection, as shown. The following analysis is obtained with the assumption that the same power switches and dc-link capacitors are employed for both motor Vdc C C 0 1 2 3 i1 i2 i3 v1 v2 + + + v3 q1 q2 q3 q1 q2 q3 Vdc C C 0 1 2 3 i1 i2 i3 v1 v2 + + + v3 q1 q2 q3 q1 q2 q3 (a) (b) Figure 8.19 Ac motor drive system with a three-phase machine in a: (a) Y connection and (b) Δ connection.
  • 253. 8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 239 drive systems (Y and Δ), which is reasonable due to the range of IGBTs available in the market. For instance, there is a class of IGBTs that operates at 600 V, the fol- lowing IGBT available deals with 1200 V. As a consequence, the same IGBT can be employed for a three-phase system with 220Vrms (phase voltage) for both Y and Δ, since a Y arrangement would require power switches with 539 V (peak), while a Δ arrangement 311 V (peak). This section aims to show the advantages and disadvantages of the Y and Δ connections of the three-phase machine in a motor drive system, highlighting the influence of these connections on the converter variables. Some parameters of the inverter will be considered in this analysis, that is, (i) dc-link voltage requirement, (ii) RMS current of the dc-link capacitor, (iii) WTHD of the motor voltages, (iv) converter losses, and (v) fault tolerance capability. The dc-link voltage of a voltage source inverter (VSI) can be defined as a func- tion of the rated voltage demanded by the motor, as given in (8.53) and (8.54) for wye and delta connection, respectively Vdc = √ 3Vph (8.53) Vdc = Vph (8.54) where Vph is the amplitude of the motor phase voltage. The dc-link voltage requirement of the motor drive system in Fig. 8.19(a) is √ 3 times higher than that in the Fig 8.19(b), considering the motor phase voltage is the same. On the other hand, the dc-link capacitor current of the system with Y and Δ connections are given by (8.55) and (8.56), respectively: ic = q1i1 + q2i2 + q3i3 (8.55) ic = q1(i3 − i1) + q2(i1 − i2) + q3(i2 − i3) (8.56) 0 0 0.5 1 i c (mA) 1.5 2 20 40 60 80 100 Fig. 8.19(a) 0 0 0.5 1 i c (mA) Frequency (kHz) 1.5 2 20 40 60 80 100 Fig. 8.19(b) Figure 8.20 Capacitor current spectrum: (a) Y connection and (b) Δ connection.
  • 254. 240 CHAPTER 8 OPTIMIZED PWM APPROACH Figure 8.20 shows the spectra of the dc-link capacitor current. As expected in (8.55) and (8.56), the amplitude of the harmonic components is higher in Δ, which means that the dc-link capacitor losses will be also higher and consequently the lifes- pan is expected to be lower for a Δ connection. The quality of the waveform generated at the output converter side can be mea- sured by WTHD, which can be calculated by WTHD = 100 a1 √ √ √ √ p ∑ i=2 (ai i )2 (8.57) (a) (b) –400 0.01 0.1 0.2 0.4 0.6 0.8 1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 0.015 0.02 0 1 2 4 3 + + + + – – – – t (s) v 1 (V) WTHD − v 1 0.03 0.025 –200 0 200 400 –400 0.01 0.015 0.02 t (s) ma v 1 (V) 0.03 0.025 –200 0 200 400 Fig. 8.19(b) Fig. 8.19(b) Fig. 8.19(a) Fig. 8.19(a) q1 q2 q3 n q1 q2 q3 q4 q4 Three-phase Machine v2 vC2 + – vC1 v3 v1 i1 i2 i3 Figure 8.21 (a) (top) WTHD of the phase voltage (𝑣1) as a function modulation index. (bottom) Phase voltages with ma = 0.5. (b) Solution with two dc voltages available. (c) THD of the motor current as a function of the modulation index.
  • 255. 8.3 THREE-LEG CONVERTER AND THREE-PHASE LOAD 241 –2 –1 0 1 2 –2 4 10 20 30 40 50 Percent of the voltage (%) 60 70 80 90 100 6 8 10 THD (%) 12 14 16 –1 0 1 2 –2 –1 0 1 2 –2 –1 0 1 2 –2 –1 0 1 2 Figure 8.21 (Continued) where a1 is the amplitude of the fundamental voltage component, ai is the amplitude of the ith harmonic, and p is the highest harmonic taken into consideration. An interesting result is shown in Fig. 8.21(a) (top). This figure shows the WTHD of the phase voltage (𝑣1) as a function of the modulation index (ma) for both systems shown in Fig. 8.19. Note that independent of the three-phase motor connections (wye or delta) the WTHD of the phase voltages are exactly the same, although the waveforms of the motor phase voltages are different, as seen in Fig. 8.21(b) (bottom). Even with the phase voltage of a three-phase machine, Y connection presents five levels instead of three in a Δ connection; such levels have higher d𝑣∕dt in their peaks and valleys as compared to the three-level voltage, which reduces the WTHD. Therefore, even with higher levels, both voltages are
  • 256. 242 CHAPTER 8 OPTIMIZED PWM APPROACH equal under the WTHD point of view. A VSI able to drive a three-phase induction motor with reduced THD for a wide range of ma is shown in Fig. 8.21(b). When the range of the motor voltage is from 100% to 50%, the switch q4 must be turned on to guarantee the dc-link voltage equal to 𝑣C1 + 𝑣C2 and the modulation index goes from 1 to 0.5 (1 ≤ ma ≤ 0.5). On the other hand, when the range of the motor voltage is from 50% to 0%, the switch q4 must be turned off to guarantee the dc-link voltage equal to 𝑣c2 and the modulation index range goes back to 1 ≤ ma ≤ 0.5. It is worth mentioning that, even considering the operation at reduced output voltage range, the power converter in Fig. 8.21(b) operates with a high modulation index, which means reduced THD. Figure 8.21(c), in turn, shows the THD behavior of the motor current from 10% to 100% of rated voltage applied to the machine. Another important feature affected by the connection of the machine is the con- verter’s losses. Figure 8.22 shows the comparison of conduction, switching, and total (conduction + switching) losses of the VSI. In this figure the switching frequency of the converter is 10 kHz. The converter power losses are higher when the machine is connected in a Δ arrangement, due to the higher level of currents. Figures 8.20 and 8.22 indicate why a Y connection is the primary option for a three-phase machine connection in a motor drive system. Exercise 8.2 When the machine is Δ connected, the reference pole voltages for the PWM generation can be defined as follows: 𝑣∗ 10 = −𝑣∗ 1 + 𝑣∗ h 𝑣∗ 20 = 𝑣∗ h 𝑣∗ 30 = 𝑣∗ 2 + 𝑣∗ h with 𝑣∗ 1 = V∗ o cos(𝜔ot) and 𝑣∗ 2 = V∗ o cos(𝜔ot + 120∘) and 𝑣∗ h given by equation (8.49) with VMAX = {−𝑣∗ 1 , 0, 𝑣∗ 2 } and VMIN = {−𝑣∗ 1 , 0, 𝑣∗ 2 }. Explain why these equations guarantee a balanced three-phase voltage applied to the machine. What would happen if equations (8.46)–(8.48) are applied for the three-leg converter with a three-phase machine in a Δ arrangement? Y connection Conduction losses Switching losses Total losses Conduction losses Switching losses Total losses Δ connection 10 kHz 10 kHz 0 100 Losses (W) 200 0 100 Losses (W) 200 Figure 8.22 Converter losses of the ac motor drive system with a switching frequency equal to 10 kHz.
  • 257. 8.4 SPACE VECTOR MODULATION (SVPWM) 243 8.4 SPACE VECTOR MODULATION (SVPWM) The nonsinusoidal CPWM techniques described earlier in this chapter could be implemented in either an analog or a digital way. On the other hand, the space vector modulation is an inherent digital way to generate the gating signals for q1, q2, and q3. These three independent gating signals lead to eight possible switching combinations for a three-phase inverter. From the electrical machine and reference-frame theory analyses, it is possible to define a transformation to represent the original three-phase variables in a sim- ple system with variables in quadrature. Such a transformation changes the variables with no physical connotation. Hence, a three-phase system can be considered to form stationary vectors in the dq complex plane. The transformation of variables can be defined as 𝑣 s odq = P𝑣 s 123 (8.58) where 𝑣 s 123 are the voltages in the original three-phase system, 𝑣 s odq are the voltages in the dq complex plane plus zero sequence component represented by “o”; the super- script “s” stands for stationary reference-frame, as the stator variables in a three-phase ac machine. P is the transformation of variables with 𝑣 s odq = ⎡ ⎢ ⎢ ⎢ ⎣ 𝑣s o 𝑣s d 𝑣s q ⎤ ⎥ ⎥ ⎥ ⎦ , 𝑣 s 123 = ⎡ ⎢ ⎢ ⎢ ⎣ 𝑣s 1 𝑣s 2 𝑣s 3 ⎤ ⎥ ⎥ ⎥ ⎦ , and P = √ 2 3 ⎡ ⎢ ⎢ ⎢ ⎢ ⎣ 1 √ 2 1 √ 2 1 √ 2 1 −1 2 −1 2 0 √ 3 2 − √ 3 2 ⎤ ⎥ ⎥ ⎥ ⎥ ⎦ . The dq voltages in the stationary reference-frame can be obtained from 𝑣s 1 , 𝑣s 2 and 𝑣s 3 , by using the matrix P, as follows: 𝑣s d = √ 2 3 ( 𝑣s 1 − 1 2 𝑣s 2 − 1 2 𝑣s 3 ) (8.59) 𝑣s q = 1 √ 2 (𝑣s 2 − 𝑣s 3 ) (8.60) Since it is assumed a balanced case (𝑣s 1 + 𝑣s 2 + 𝑣s 3 = 0) the term 𝑣s o is null. Equations (8.59)–(8.60) can be written as functions of the states of the switches [see equations (8.36)–(8.38)], as follows: 𝑣s d = √ 2 3 ( q1 − 1 2 q2 − 1 2 q3 ) Vdc (8.61) 𝑣s q = 1 √ 2 (q2 − q3)Vdc (8.62) Table 8.3 shows the vectors in the dq plane Vs x = Vs d + jVs q (x = 1, 2, … , 8) associated with each switching state. Each vector means a topological circuit for the converter, as shown in Fig. 8.23. Note from Table 8.3 that there are two null (0 and 7) and six non-null (1, 2, 3, 4, 5, and 6) vectors – active vectors, which will be used to synthesize the desired
  • 258. 244 CHAPTER 8 OPTIMIZED PWM APPROACH TABLE 8.3 PWM Vectors as a Function of the Switching States Vector q1 q2 q3 Vs x 0 0 0 0 0 1 1 0 0 √ 2∕3Vdc 2 1 1 0 Vdc∕ √ 6 + jVdc∕ √ 2 3 0 1 0 −Vdc∕ √ 6 + jVdc∕ √ 2 4 0 1 1 − √ 2∕3Vdc 5 0 0 1 −Vdc∕ √ 6 − jVdc∕ √ 2 6 1 0 1 Vdc∕ √ 6 − jVdc∕ √ 2 7 1 1 1 0 (a) (b) (c) (d) (e) (f) (g) (h) V1 V2 V3 V1 q1 V2 V3 V1 q2 V2 V3 V1 q1 q1 q2 q3 q3 V2 V3 V1 V2 V3 V1 q2 q3 V2 V3 V1 q3 V2 V3 V1 q1 q2 V2 V3 Figure 8.23 Topological circuits as a function of the switching states: (a) Vector 0, (b) Vector 1, (c) Vector 2, (d) Vector 3, (e) Vector 4, (f) Vector 5, (g) Vector 6, (h) Vector 7.
  • 259. 8.4 SPACE VECTOR MODULATION (SVPWM) 245 (a) (c) (d) (e) (b) V3 s V2 s V1 s V0 s V6 s V5 s V2 s t2/T V2 s t2/T V3 s t3/T V1 s t1/T V4 s V7 s Vector 2 Vector 1 Vector 0 vswitch vswitch iswitch vdq s* vdq s* Pcond Pblock iswitch Sector 3 Sector 1 Sector 1 Sector 4 Sector 6 Sector 2 Sector 2 Sector 5 θ θ Figure 8.24 Graphical analysis for the space vector PWM showing the (a) vectors and (b) sectors (c) Losses associated to the switching states change A reference voltage in (d) Sector 1, and (e) Sector 2. load voltage. All vectors Vs x (x = 0, 2, … , 7) are shown in Fig. 8.24(a) as a graphical representation of Table 8.3. The area between two adjacent non-null vectors defines a sector as depicted in Fig. 8.24(b), which leads to six vectors. It is possible to go from one vector to its adjacent one with just a single change for the switching state. For instance, from Vector 1 to Vector 2, q2 is changed from 0 to 1, while q1 and q3 are kept constant. In the same way, from Vector 2 to Vector 3, q1 is changed from 1 to 0, while q2 and q3 are kept constant. It means that it is possible to reduce the number of changes in the switching states by using adjacent
  • 260. 246 CHAPTER 8 OPTIMIZED PWM APPROACH vectors to synthesize a specific value of the desired voltage. The strategy of applying adjacent vectors plays an important role for converter losses reduction, since losses appear each time it is necessary to change the switching states, as seen in Fig. 8.24(c). To reduce the switching losses, if the desired voltage is inside Sector 1, the Vectors 1 and 2 should be chosen [see Fig. 8.24(d)]. In the same way, if the desired voltage is inside Sector 2, Vectors 2 and 3 should be chosen [see Fig. 8.24(e)], and so on. All pairs of adjacent vectors available in a three-leg converter are: (Vs 1 and Vs 2 ), (Vs 2 and Vs 3 ), (Vs 3 and Vs 4 ), (Vs 4 and Vs 5 ), (Vs 5 and Vs 6 ), and (Vs 6 and Vs 1 ). Notice that it is possible to define such a set of adjacent vectors in a generic way by using (Vs k and Vs l ), with k = 1, … , 6, and l = k + 1 if k ≤ 5; and l = 1 if k = 6. The vectors Vs k and Vs l have their dq components (see Table 8.3), that is, Vs k = Vs dk + jVs qk and Vs l = Vs dl + jVs ql . The reference voltage 𝑣s∗ dq can be obtained from a set of three-phase reference voltages (𝑣s∗ 123 ) by using the transformation P given in (8.58). As mentioned earlier, a switching sequence for q1, q2, and q3 should be chosen to allow the converter to synthesize a given reference voltage 𝑣s∗ dq , which is constant in the switching period (Ts). In terms of average values, it is possible to write 1 Ts ∫ Ts 0 𝑣s∗ dqdt = 1 Ts ∫ tk 0 Vs kdt + 1 Ts ∫ tl 0 Vs l dt (8.63) 𝑣s∗ dq = tk Ts Vs k + tl Ts Vs l (8.64) where tk and tl are intervals of time for application of the vectors Vs k and Vs l , respec- tively. Rewriting (8.64) in terms of dq components, we get 𝑣s∗ d = tk Ts Vs kd + tl Ts Vs ld (8.65) 𝑣s∗ q = tk Ts Vs kq + tl Ts Vs lq (8.66) Equations (8.65) and (8.66) show that the reference voltages can be obtained from the interval of time for application of two adjacent vectors. From (8.65) and (8.66) it is possible to write tk = 𝑣s∗ d Vs lq − 𝑣s∗ q Vs ld Vs kd Vs lq − Vs ld Vs qk Ts (8.67) tl = 𝑣s∗ q Vs kd − 𝑣s∗ d Vs kq Vs kd Vs lq − Vs ld Vs qk Ts (8.68) To keep the switching frequency of the converter constant, it is necessary to guarantee that the sum of the time for the application of the vectors is equal to Ts. Then, the null vectors (Vectors 0 and 7 in Table 8.3) can be used to keep the switch- ing frequency constant, that is, tk + tl + to = Ts, and then to = Ts − tk − tl. Note that
  • 261. 8.5 OTHER CONFIGURATIONS WITH CPWM 247 V0 s V1 s V1 s V0 s V2 s V2 s V7 s V7 s v10 Vdc/2 –Vdc/2 toi tof Ts v20 Vdc/2 –Vdc/2 v30 Vdc/2 –Vdc/2 Figure 8.25 Pulses defining how the null vectors are divided at the beginning and end of the switching period. there is a degree of freedom for to, meaning that this time could be divided between the beginning (toi = 𝜇to) and the end [tof = (1 − 𝜇)to, 0 ≤ 𝜇 ≤ 1] of the sampling interval, as presented in Fig. 8.25. Note that this approach brings benefits in terms of THD reduction, since the pulse can be centered inside the sampling period. A summary of the SPWM is presented in Fig. 8.26, which also shows the algorithm for the implementation of the space vector modulation by using a MAT- LAB code. 8.5 OTHER CONFIGURATIONS WITH CPWM Although the SPWM approach represents one of the most popular options in indus- trial applications, the CPWM is able to generate PWM signals with the same benefits as in the SPWM. Furthermore, the expression derived in (8.19) is a generic way to represent the auxiliary voltage 𝑣∗ h . Such expressions can be employed in different con- verters with at least one degree of freedom, that is, the number of voltages available at the converter side higher than the number of voltage(s) demanded by the load. In the following sections, a symmetrical two-phase motor drive system and a converter for application in three-phase four-wire systems are employed as examples of the comprehensiveness of the CPWM. 8.5.1 Three-Leg Converter—Two-Phase Machine Two-phase motors can be found in home appliances, industrial tools, or small power applications. Such a motor is often used in fixed speed drives. However, a dc–ac power converter can be used when a variable motor speed operation is required. The
  • 262. 248 CHAPTER 8 OPTIMIZED PWM APPROACH v123 s* vdq s* Transformation of variables Definition of sectors and obtaining k and l Calculate Calculate Table 8.3 Equations (8.67) and (8.68) Vdk,Vqk,Vdl and Vql s s s s tk and tl Figure 8.26 Algorithm for implementation of the SVPWM. symmetrical two-phase motor can be considered as an interesting alternative for frac- tional horsepower variable-speed drive, due to its characteristic of no pulsating torque produced as observed in single-phase motors. Since a symmetrical two-phase motor is a three-terminal electrical apparatus, a three-leg converter can be used to supply it. Figure 8.27 shows a three-leg converter supplying a two-phase symmetrical machine. Since this type of machine demands two voltages in quadrature (𝑣∗ 𝛼 and 𝑣∗ 𝛽 ), the reference pole voltages are as follows: 𝑣∗ 10 = 𝑣∗ 𝛼 + 𝑣∗ h (8.69) 𝑣∗ 20 = 𝑣∗ 𝛽 + 𝑣∗ h (8.70) 𝑣∗ 30 = 𝑣∗ h (8.71) where 𝑣∗ h can be obtained directly from equation (8.49) with Vmax = MAX{𝑣∗ 𝛼, 𝑣∗ 𝛽 , 0} and Vmin = MIN{𝑣∗ 𝛼, 𝑣∗ 𝛽 , 0}.
  • 263. 8.5 OTHER CONFIGURATIONS WITH CPWM 249 Vdc 0 1 2 3 iq1 iq2 iq3 – + + vα iα iβ in – + vβ – q1 q2 q3 q1 q2 q3 n Figure 8.27 Three-leg converter supplying a symmetrical two-phase machine. Exercise 8.3 Comparing the three-leg converter supplying a three-phase load (as in Fig. 8.14) with the same converter supplying a two-phase load (as in Fig. 8.27), determine the changes in the specification of the power switches assuming that both machines have the same phase voltage, active power, and power factor. Disregard any safety margin while specifying the power switches. 8.5.2 Four-Leg Converter Note that the three-phase and two-phase motor drive systems require the same topol- ogy in terms of the number of switches employed. The difference is related to the load (e.g., type of machine) connected to the converter and also in terms of control considered for PWM and feedback strategies (if needed). Similarly, the same CPWM approach can be employed for dc-ac converters with four legs considered in different applications. Figure 8.28 shows a four-leg converter feeding a three-phase four-wire system. In this type of application, there Vdc 0 1 2 3 4 iq1 iq2 iq3 iq4 – + + v1 i1 i2 i3 iN – +v2 – +v3 – q1 q2 q3 q4 q1 q2 q3 q4 Figure 8.28 Four-leg converter supplying a three-phase four-wire load.
  • 264. 250 CHAPTER 8 OPTIMIZED PWM APPROACH Load Source υ1 Three-phase load – + υ2 – + υ3 – + υ1 – + υ2 – + υ3 – + 1 2 3 4 1 2 3 4 Figure 8.29 Three-phase four-wire systems with: (left) balanced and (right) unbalanced waveforms. Vdc 0 1 2 3 4 iq1 iq2 iq3 iq4 – + + v1 i1 i2 i3 i4 – +v2 – +v3 – +v4 – q1 q2 q3 q4 q1 q2 q3 q4 Figure 8.30 Four-leg converter supplying four-phase machine. are two different scenarios: balanced three-phase voltages, as in Fig. 8.29 (left-hand side), and unbalanced three-phase voltages, as in Fig. 8.29 (right-hand side). The latter case is employed for applications such as dynamic-voltage-restorer and series-active-power-filter. On the other hand, Fig. 8.30 shows the same four-leg converter supplying a four-phase machine. The PWM strategy with the inclusion of the voltage 𝑣∗ h is still valid for the converter with four legs, even considering the different applications highlighted previously. The use of a four-phase machine drive system brings some advantages such as eliminating the common mode, reducing the ratings of the power switches, and providing fault tolerance characteristics for the drive system.
  • 265. 8.5 OTHER CONFIGURATIONS WITH CPWM 251 Exercise 8.4 (a) Write the PWM equations (reference pole voltages) for the four-leg con- verter presented in Fig. 8.28 assuming both cases with balanced and unbal- anced requirement. (b) Write the PWM equations for the four-leg converter supplying a four-phase machine with balanced voltages. (c) Also, draw a block diagram as in Fig. 8.15 for the (a) and (b) questions. Application (Dynamic Voltage Restorer) Dynamic voltage restorer (DVR) can be used to minimize the effect of operational malfunction of the electric power grid, which can lead to sags or swells. The DVR’s benefits of sustaining and restoring the voltage supply are especially important in applications with critical loads requiring a regulated voltage. The operation principle of this electrical apparatus is as follows: during the normal operation of the grid, the static switch Q3 is turned on, while during sags or swells the switches Q1 and Q2 are turned on to either add or subtract the grid voltage, as compensation voltage from the DVR. 0 25% 35% 45% 55% 65% 100 200 ms Sags 300 400 500 The figure below shows the compensation requirement for a typical situation that shows a trend of deeper voltage sags with shorter duration, while moderate sags Q3 Q1 Distribution bus Control Charger Load Bus Q2 LPF
  • 266. 252 CHAPTER 8 OPTIMIZED PWM APPROACH occur for a longer period of time. The information provided in the graph below plays an important role for designing the charger of the DVR. The figure below presents the dynamic operation of the DVR highlighting the grid voltage with a 100 ms sag duration. Note that this figure shows a sag with bal- anced voltages, but it is quite common to have an unsymmetrical sag, which requires a DVR implemented by a three-phase four-wire dc-ac converter. Load voltage DVR voltage Grid voltage 100 ms 8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 8.6.1 Inverter with Split-Wound Coupled Inductors A converter having the same number of controlled power devices (six IGBTs) as in the conventional three-leg converter (Fig. 8.14) but with higher number of levels is presented in Fig. 8.31. Such a converter was presented in Section 7.3 with another PWM approach, consisting of two carrier and one modulating signal per phase. The Vdc a1 c1 b1 a2 c2 b2 a c b 0 qa1 da1 db1 dc1 a da2 db2 dc2 qb1 qc1 qa2 qb2 qc2 – +va – +vb – +vc Figure 8.31 Three-phase PWM inverter with split-wound coupled inductors.
  • 267. 8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 253 CPWM is presented in this section for the converter in Fig. 8.31 as an alternative option. The main advantages of this converter when compared to the solutions pre- sented in the technical literature are higher number of levels for the pole voltages and no dead-time requirement for the converter’s operation. Such a PWM inverter with split-wound coupled inductors is constituted by switching power devices (qx1 − qx2, with x = a, b, c), six diodes (dx1 − dx2), and three split-wound coupled inductors. The characteristics and the operation modes of this converter are presented in Section 7.3. The voltages 𝑣x10 and 𝑣x20 (voltages from the points x1 and x2 to the dc-link capacitor midpoint) can be expressed as a function of the state of the switches qx1 and qx2, respectively as follows: 𝑣x10 = (2qx1 − 1) Vdc 2 (8.72) 𝑣x20 = (2qx2 − 1) −Vdc 2 (8.73) It means that each leg can be modeled as in Fig. 8.32(a). Then the pole voltages 𝑣x0 will be given by 𝑣x0 = 1 2 (𝑣x10 − 𝑣x20) (8.74) Hence from (8.72)–(8.74) it is possible to write 𝑣x0 as a function only of the state of the switches and dc-link voltage, as follows: 𝑣x0 = (qx1 − qx2) Vdc 2 (8.75) or 𝑣x0 = 𝑣x1 − 𝑣x2 (8.76) where 𝑣x1 = qx1Vdc∕2 and 𝑣x2 = qx2Vdc∕2. From (8.76) it is possible to model the three-phase converter as depicted in Fig. 8.32(b). If the desired voltage in the three-phase load is given by 𝑣∗ a, 𝑣∗ b , and 𝑣∗ c , then the reference pole voltage can be written as 𝑣∗ a0 = 𝑣∗ a + 𝑣∗ h (8.77) 𝑣∗ b0 = 𝑣∗ b + 𝑣∗ h (8.78) 𝑣∗ c0 = 𝑣∗ c + 𝑣∗ h (8.79) where 𝑣∗ h can be obtained directly from equation (8.49). Once the reference pole volt- ages 𝑣∗ a0 , 𝑣∗ b0 , and 𝑣∗ c0 are defined from (8.77)–(8.79), the voltages from the points x1 and x2 (with x = a, b, c) with respect to 0 are given by 𝑣∗ x1 = 𝑣∗ x0 2 (8.80) 𝑣∗ x2 = − 𝑣∗ x0 2 (8.81) The PWM signals generation from equations (8.80) and (8.81) can be done as presented in Fig. 8.32(c).
  • 268. 254 CHAPTER 8 OPTIMIZED PWM APPROACH (a) (b) (c) 0 0 – – + + vx10 vb1 – + vc1 – – – – + + + + va1 vb2 vc2 va2 – + va – + vb – + vc ix x a b n c – + vx20 va * va0 * va1 * va2 * vb0 * vc0 * vb * vc * vh * μ vb1 * vb2 * vc1 * vc2 * vt * qa1 qa2 qb1 qb2 qc1 qc2 1/2 –1/2 1/2 –1/2 1/2 –1/2 Equations (8.49) – + – + – + – + – + – + Vdc * VMAX MAX MIN * VMIN Figure 8.32 (a) Leg model. (b) Model of the three-phase PWM inverter with split-wound coupled inductors. (c) Analog PWM implementation. 8.6.2 Z-Source Converter The PWM dc–ac power converters presented in this book are predominantly char- acterized as a voltage-source converter. However, in general terms, dc–ac power converters can be divided into two main groups: voltage-source and current-source converters, each one with its particular characteristics. The impedance-source con- verter is an alternative type of power converter, which provides the unique feature of buck and boost operation capability with the same number and same arrangement of the semiconductor devices. Such a converter employs an impedance circuit to con- nect the converter to the primary energy source, as seen in Fig. 8.33, and it is also known as Z-source inverter. Unlike the conventional dc–ac converter in which there is a need for dead time to avoid short-circuit of the dc-link source, in the Z-source converter such short-circuit (named as shoot-through zero state) is required to guarantee the boost operation of the converter. In fact the Z-source converter is a buck-boost dc-ac converter with the operation mode (buck or boost) defined by the PWM strategy.
  • 269. 8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 255 Vdc L2 L1 C1 C2 a b c Z-source 3 ~ motor – + – + vi vd qa1 qb1 qc1 qa2 qb2 qc2 Figure 8.33 Z-source converter. The circuit operates, boosting the input voltage (Vdc) if there is a short-circuit time between two switches of the same leg for one, two, or three legs. On the other hand, if there is no short-circuit time (as in a conventional converter) the circuit will operate as a buck converter. Figure 8.34(a) and 8.34(b) show the equivalent circuits considering the dc source (Vdc) point of view when the inverter is creating a short-circuit and without a short-circuit, respectively. Note that when there is no short-circuit, the inverter is represented by a current source ii, since it is assumed that the load has inductive characteristics. Considering an ideal and symmetrical circuit with L1 = L2 = L and C1 = C2 = C, it leads to VC1 = VC2 = VC (8.82) 𝑣L1 = 𝑣L2 = 𝑣L (8.83) From Fig. 8.34(a), that is, during the short-circuit time (𝜏o), it is seen that 𝑣L = VC (8.84) 𝑣d = 2VC (8.85) 𝑣i = 0 (8.86) On the other hand, from Fig. 8.34(b), during the conventional operation (𝜏N), it yields 𝑣L = Vdc − VC (8.87) 𝑣d = Vdc (8.88) 𝑣i = 2VC − Vdc (8.89) From equations (8.84)–(8.86) and (8.87)–(8.89) and since the average value of the inductor voltage into one switching period (Ts) should be zero, it leads to VL = 1 Ts ∫ t+Ts t 𝑣Ldt = 𝜏oVC + 𝜏N(Vdc − VC) Ts = 0 (8.90) where Ts = 𝜏N + 𝜏o.
  • 270. 256 CHAPTER 8 OPTIMIZED PWM APPROACH (a) (b) Vdc Vdc L1 iL1 iL2 vC1 vC2 L2 C1 C2 Diode open – – – + + + – + v i = 0 vd Vdc L1 L2 C1 C2 Diode close – + – + vd vi ii Figure 8.34 (a) Equivalent circuit during the short-circuit. (b) Equivalent circuit during the conventional operation. Working on equation (8.90) it becomes VC Vdc = 𝜏N 𝜏N − 𝜏o (8.91) The average voltage of the input converter side is given by Vi = 𝜏N 𝜏N − 𝜏o Vdc (8.92) Finally, the peak dc-link voltage can be obtained as follows: 𝑣i = VC − 𝑣L (8.93) 𝑣i = 2VC − Vdc (8.94) 𝑣i = 1 1 − 2𝜏o∕Ts Vdc = B ⋅ Vdc (8.95) where B is the boost factor of the Z-source converter. Equation (8.95) means that for any 𝜏o different from 0 the voltage value of the input side of the converter will be higher than the voltage at the source side (Vdc), that is, boost operation. The capacitor
  • 271. 8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 257 voltages can also be obtained as a function of the shoot-through time (𝜏o): VC1 = VC2 = 1 − 𝜏o∕Ts 1 − 2𝜏o∕Ts Vdc (8.96) To generate the PWM signals for the Z-source converter allowing the boost operation it is necessary to include the short-circuit time (shoot-through). The CPWM technique presented throughout this chapter can be applied to this type of converter as well. In this case, in order to facilitate the demonstration of the PWM signal genera- tion, the voltage of the input converter side (𝑣i) is divided into two parts, thus creating a virtual zero point (“0”), as observed in Fig. 8.35(a). Then, the pole voltages are defined as the voltage from the central point of the leg to the point “0”. The pole voltages are: 𝑣a0, 𝑣b0, and 𝑣c0. Figure 8.35(b) shows the generation of pole voltages through the comparison between the triangular and sinu- soidal waveforms for the conventional (left-side) and Z-source (right-side) inverters. The shoot-through zero states can be evenly distributed among the three-phase legs, while the equivalent active vectors are unchanged. It can be seen from Fig. 8.35(b) that 𝜏1 and 𝜏2 (time intervals of active vectors) have the same values for the conven- tional and Z-source converters. During the shoot-through zero state intervals of time the pole voltages are equal to zero, since 𝑣i = 0. Exercise 8.5 Assuming that the circuit in Fig. 8.33 (Z-source topology) should be designed to operate boosting this input voltage from 100V to 150V, what is the maxi- mum modulation index (ma) obtained in this scenario? 8.6.3 Open-End Winding Motor Drive System As mentioned in previous chapters of this book, besides the Δ and Y connections there is another way to connect a three-phase machine in motor drive systems, which is called open-end winding connection. Such a connection consists of a series arrange- ment of two conventional two-level converters (inverters 1 and 2 in Fig. 8.36) through the open-end windings of a three-phase machine. Note that in this case it is necessary to have access to six terminals of the machine. The converter pole voltages depend on the conduction states of the power switches, that is 𝑣al0l = (2qal − 1) Vdcl 2 (8.97) 𝑣bl0l = (2qbl − 1) Vdcl 2 (8.98) 𝑣cl0l = (2qcl − 1) Vdcl 2 (8.99) where l = 1 and 2.
  • 272. 258 CHAPTER 8 OPTIMIZED PWM APPROACH (a) (b) Vdc1 Ts Ts t t t t t t + + + – – – “Virtual” zero point vi = E vt * va * vb * vc * vt * va * vb * vc * τa τo τb τ1 τ2 τ1 τ2 τc τa τb τc E 2 E 2 0 – vb0 vc0 va0 E 2 3 τo 3 τo 6 τo 6 E 2 0 – E 2 E 2 0 – E 2 E 2 0 – vb0 vc0 va0 E 2 E 2 0 – E 2 E 2 0 – E 2 E 2 0 qa1 a b c qb1 qc1 qa2 qb2 qc2 Figure 8.35 (a) Inverter highlighting the virtual zero point “0”. (b) Generation of pole voltages through sine-triangle modulation for conventional (left-side) and Z-source (right-side) inverters.
  • 273. 8.6 NONCONVENTIONAL TOPOLOGIES WITH CPWM 259 Vdc1 Vdc2 Inverter 1 Inverter 2 Three-phase machine a1 a2 c1 c2 b1 b2 01 02 qa1 qb1 qc1 qa1 qb1 qc1 qc2 – + qb2 qa2 qc2 qb2 qa2 va – +vb – +vc Figure 8.36 Open-end winding machine supplied by two inverter series connected. The motor phase voltages can be written as a function of the pole voltages and as a function of the difference between the dc-link capacitor midpoints: 𝑣a = 𝑣a101 − 𝑣a202 + 𝑣0102 (8.100) 𝑣b = 𝑣b101 − 𝑣b202 + 𝑣0102 (8.101) 𝑣c = 𝑣c101 − 𝑣c202 + 𝑣0102 (8.102) where, for a balanced case it becomes 𝑣0102 = − 1 3 ( c ∑ j=a 𝑣j101 − c ∑ j=a 𝑣j202 ) (8.103) Both power converters must generate appropriate reference voltages (𝑣∗ a, 𝑣∗ b , and 𝑣∗ c) for the three-phase machine. Due to the inherent redundancy of the voltages demanded by a three-phase machine, the converters actually need to generate inde- pendently two line-to-line voltages (e.g., 𝑣ab = 𝑣a − 𝑣b and 𝑣ca = 𝑣c − 𝑣a). For the system presented in Fig. 8.36 there are four degrees of freedom in terms of the PWM generation, since the converter has six legs and it needs to generate just two voltages. Considering that the voltages 𝑣∗ ab and 𝑣∗ ca should be imposed by the converter, four auxiliary variables are introduced as presented in equations (8.104)–(8.109) 𝑣∗ ab = 𝑣∗ a101 − 𝑣∗ b101 − 𝑣∗ a202 + 𝑣∗ b202 (8.104) 𝑣∗ ca = −𝑣∗ a101 + 𝑣∗ c101 + 𝑣∗ a202 − 𝑣∗ c202 (8.105) 𝑣∗ h0 = 𝑣∗ a101 − 𝑣∗ a202 (8.106) 𝑣∗ h1 = 𝑣∗ a202 (8.107) 𝑣∗ h2 = 𝑣∗ b202 (8.108) 𝑣∗ h3 = 𝑣∗ c202 (8.109) It can be seen from these equations that both desired and auxiliary voltages have been written as a function of the reference pole voltages. However, for the PWM generation purposes, it is necessary to define the reference pole voltages as a function
  • 274. 260 CHAPTER 8 OPTIMIZED PWM APPROACH of the desired and auxiliary voltages as follows: 𝑣∗ a101 = 𝑣∗ h0 + 𝑣∗ h1 (8.110) 𝑣∗ b101 = −𝑣∗ ab + 𝑣∗ h0 + 𝑣∗ h2 (8.111) 𝑣∗ c101 = 𝑣∗ ca + 𝑣∗ h0 + 𝑣∗ h3 (8.112) 𝑣∗ a202 = 𝑣∗ h1 (8.113) 𝑣∗ b202 = 𝑣∗ h2 (8.114) 𝑣∗ c202 = 𝑣∗ h3 (8.115) It is also possible to define effective reference pole voltages since 𝑣∗ a120 = 𝑣∗ a101 − 𝑣∗ a202 (8.116) 𝑣∗ b120 = 𝑣∗ b101 − 𝑣∗ b202 (8.117) 𝑣∗ c120 = 𝑣∗ c101 − 𝑣∗ c202 (8.118) Another convenient way to write the effective reference pole voltages is as follows: 𝑣∗ a120 = 𝑣∗ h0 (8.119) 𝑣∗ b120 = −𝑣∗ ab + 𝑣∗ h0 (8.120) 𝑣∗ c120 = 𝑣∗ ca + 𝑣∗ h0 (8.121) Equations (8.122)–(8.124) lead to a straightforward way to write the PWM equations: 𝑣∗ a101 = 𝑣∗ a120 + 𝑣∗ h1 (8.122) 𝑣∗ b101 = 𝑣∗ b120 + 𝑣∗ h2 (8.123) 𝑣∗ c101 = 𝑣∗ c120 + 𝑣∗ h3 (8.124) 𝑣∗ a202 = 𝑣∗ h1 (8.125) 𝑣∗ b202 = 𝑣∗ h2 (8.126) 𝑣∗ c202 = 𝑣∗ h3 (8.127) To finally define the reference pole voltages, it remains to determine the auxil- iary voltages 𝑣∗ h0 , 𝑣∗ h1 , 𝑣∗ h2 , and 𝑣∗ h3 , as presented in the sequence: The auxiliary voltage (𝑣∗ h0 ) involves the desired line-to-line and effective pole voltages. It is possible to define 𝑣∗ h0 respecting the following restriction V0MIN ≤ 𝑣∗ h0 ≤ V0MAX (8.128) with V0MIN = MIN { − Vdc1 + Vdc2 2 , − Vdc1 + Vdc2 2 − 𝑣∗ ab, − Vdc1 + Vdc2 2 + 𝑣∗ ca } V0MAX = MAX { Vdc1 + Vdc2 2 , Vdc1 + Vdc2 2 − 𝑣∗ ab, Vdc1 + Vdc2 2 + 𝑣∗ ca }
  • 275. REFERENCES 261 The voltages 𝑣∗ h0 can be defined as a function of 𝜇0 as in equation (8.129), which is an adaption from equation (8.49): 𝑣∗ h0 = (1 − 𝜇0)V0MIN + 𝜇0V0MAX (8.129) Using the auxiliary voltage 𝑣∗ h0 and the desired line-to-line voltage it is possible to define the effective reference pole voltages. Finally to define the reference pole voltages (8.122)–(8.127) it is necessary to find 𝑣∗ h1 , 𝑣∗ h2 , and 𝑣∗ h3 as in the sequence: The auxiliary voltages (𝑣∗ h1 , 𝑣∗ h2 , and 𝑣∗ h3 ) can be considered as three single-phase auxiliary voltages, which are also restricted by VkMIN ≤ 𝑣∗ hk ≤ VkMAX (8.130) with k = 1, 2, 3; where the minimum and maximum values are given respectively by 𝑣∗ kMIN = MIN { − Vdc1 2 − 𝑣∗ l120, − Vdc2 2 } 𝑣∗ kMAX = MAX { Vdc1 2 − 𝑣∗ l120, Vdc2 2 } when k = 1 → l = a, k = 2 → l = b, and k = 3 → l = c. The remaining auxiliary voltages (𝑣∗ hk ) can be calculated as presented below: 𝑣∗ hk = (1 − 𝜇k)VkMIN + 𝜇kVkMAX (8.131) Equation (8.131) was obtained by following the same strategy as in equation (8.19). 8.7 SUMMARY This chapter presented a systematic way to implement an optimized PWM applied to dc–ac converters [1–23]. It has been demonstrated that if the converter presents a number of pole voltages higher than the number of desired output voltages, a parameter 𝑣∗ h can be added to improve either THD or efficiency of the converter. Section 8.2 introduced such an optimization for the H-bridge converter along with its model. Sections 8.3, 8.5, and 8.6 showed the same PWM technique for other converters [24–32], that is: (i) three-leg converter feeding a two-phase load, (ii) four-leg converter supplying a three-phase four-wire load, (iii) split-wound coupled inductor converters, (iv) Z-source converter, and (v) open-end winding motor drive system. Section 8.4 described the space vector modulation applied to the conventional three-phase dc–ac converter. REFERENCES [1] Schönung A, Stemmler H. Static frequency changers with subharmonic control in conjunction with reversible variable speed a.c. drives. Brown Boweri Rev 1964;51:555–577. [2] Jardan KR, Dewan SB, Slemon G. General analysis of three-phase inverters. IEEE Trans Ind Appl 1969;5(6):672–679.
  • 276. 262 CHAPTER 8 OPTIMIZED PWM APPROACH [3] Jardan KR. Modes of operation of three-phase inverters. IEEE Trans Ind Appl 1969;5(6):680–685. [4] Busse A, Holtz J. Multiloop control of a unity power factor fast-switching AC to DC Converter. Conference Record of IEEE Power Electronics Specialists Conference (PESC’82); 1982. p 171–179. [5] Pffaf G, Weschta A, Wick A. Design and experimental results of a brushless AC servo drive. Con- ference Record of IEEE/IAS Annual Meeting; 1982. p 692–697. [6] Zubek J, Abbondanti A, Nordby CJ. Pulsewidth modulated inverter motor drives with improved mod- ulation. IEEE Trans Ind Appl 1975;IA-11(6):1224–1228. [7] Bowes SR, Mount MJ. Microprocessor control of PWM inverters. IEE Proc B 1981:293–305. [8] Holtz J. Pulsewidth modulation for electronic power conversion. Proc IEEE 1994;82:1194–1214. [9] Buja G, Indri G. Improvement of pulse width modulation techniques. Arch Elektrotech 1977;57:281–289. [10] Depenbrock M. Pulse width control of a 3-phase inverter with non-sinusoidal phase voltages. Pro- ceedings of the IEEE International Semiconductor Power Converter Conference, ISPCC’07; 1977. p 399–403. [11] Houldsworth JA, Grant DA. The use of harmonic distortion to increase the output voltage of a three-phase PWM inverter. IEEE Trans Ind Appl 1984;IA-20(5):1224–1228. [12] Agelidis VG, Ziogas PD, Joos G. Dead-band PWM switching patterns. IEEE Trans Power Electron 1996;11:523–531. [13] Boost MA, Ziogas PD. State-of-the-art carrier PWM techniques: a critical evaluation. IEEE Trans Ind Appl 1988;24:271–280. [14] Ziogas PD, Moran L, Joos G, Vincenti D. A refined PWM scheme for voltage and current source converter. Proceedings IEEE PESC’90; 1990. p 977–983. [15] Seixas P. Commande numérique d’une machine synchrone autopilotée [D.Sc. Thesis]. L’Intitut Nationale Polytechnique de Toulouse, INPT; 1988. [16] Hava AM, Kerkman R, Lipo TA. A high-performance generalized discontinuous PWM algorithm. IEEE Trans Ind Appl 1998;34:1059–1071. [17] Holmes DG. The significance of zero space vector placement for carrier-based PWM schemes. IEEE Trans Ind Appl 1996;32:1122–1129. [18] Taniguchi K, Ogino Y, Irie H. PWM technique for power MOSFET inverter. IEEE Trans Power Elect 1988;3(3):328–334. [19] Jacobina CB, Lima AMN, da Silva ERC, Alves RNC, Seixas PF. Digital scalar pulse-width mod- ulation: a simple approach to introduce non-sinusoidal modulating waveforms. IEEE Trans Power Electron 2001;16:351–359. [20] Blasko V. A hybrid PWM strategy combining modified space vector and triangle comparison meth- ods. Proc Conf. Rec. PESC; 1996. p 1872–1878. [21] Trzynadlowski A, Legowski S. Minimum-loss vector PWM strategy for three-phase inverter. IEEE Trans Power Electron 1994;9:26–34. [22] van der Broeck HW, Skudelny HC, Stanke GV. Analysis and realization of a pulsewidth modulator based on voltage space vector. IEEE Trans Ind Appl 1988;24(1):142–150. [23] Holmes DG. The general relationship between regular-sampled pulse-width-modulation and space vector modulation for hard switched converters. Conf. Rec. IEEE-IAS Annual Meeting; 1992. p 1002–1009. [24] Matsui K, Murai Y, Watanabe M, Kaneko M, Ueda F. A pulsewidth modulated inverter with parallel-connected transistors by using current sharing reactors. IEEE Trans Ind Appl 1993;8(2):186–191. [25] Salmon J, Ewanchuk J, Knight AM. PWM inverters using split-wound coupled inductors. IEEE Trans Ind Appl 2009;45(6):2001–2009. [26] Teixeira, CA, McGrath BP, Holmes DG. Topologically reduced multilevel converters using complementary unidirectional phase-legs. Proc. of IEEE Int’l Symp on Industrial Electron; 2012. p 2007–2012. [27] F. Z. Peng, Z-source inverter, IEEE Trans Ind Appl, vol. 39, pp. 504–510, 2003. [28] dos Santos EC, Bradaschia F, Cavalcanti MC, da Silva ERC. Z-source converter applied for single-phase to three-phase conversion system. Proceedings of Applied Power Electron Conference and Exposition, APEC; 2011. p 216–223.
  • 277. REFERENCES 263 [29] Muniz JHG, da Silva ERC, dos Santos, EC. A hybrid PWM strategy for Z-source neutral-point- clamped inverter. Proceedings of Applied Power Electron Conference and Exposition, APEC; 2011. p 450–456. [30] dos Santos EC, Pimentel Filho EPX, Oliveira AC, da Silva ERC. Hybrid pulse width modulation for Z-source inverters. Proceedings of Energy Conversion Congress and Exposition (ECCE); 2010. p 2888–2892. [31] Shiny G, Baiju MR. Space vector PWM scheme without sector identification for an open-end wind- ing induction motor based 3-level inverter. Proceedings of IEEE Industrial Electronic Conference, IECON; 2009. p 1310–1315. [32] Park RM. Two-reaction theory of synchronous machines. AIEE Trans 1929;48:716–730.
  • 278. CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS 9.1 INTRODUCTION After describing many topologies in Chapters 2–7, highlighting the circuits them- selves, as well as optimized pulse width modulation (PWM) strategies in Chapter 8, this chapter deals with the control actions needed to keep a specific variable of the converter under control, for instance, in a motor drive system where the speed must be controlled electronically through a power converter, or in a circuit designed to correct the power factor actively. This chapter is strategically placed before the description of back-to-back converters, due to the need for regulation of some variables, such as grid current and dc-link capacitor voltage. It is worth mentioning that all power converters previously presented were without any feedback control. The types of controllers employed in applications with power converters as controlled source can be basically classified into two main groups: lin- ear and nonlinear controllers. Hysteresis and sliding-modes are examples of nonlinear controllers, while proportional (P), proportional–integral (PI), and proportional–integral–derivative (PID) regulators are examples of linear controllers. The principle and characteristics of both types of controllers are introduced here. Rather than providing deep analysis for each controller, this chapter aims to prepare the reader for the next chapters, where the converters demand feedback control. A dynamic simulation is an important aspect to test and validate control strate- gies, since the behavior of the variables can be verified to predict the dynamics of the system. MATLAB codes are presented for the control strategies developed in this chapter as an effective way to verify the actions of the studied controllers. Also, Euler’s integration method is employed to simulate the behavior of the state space variables, due to its simplicity. Following this introduction, Section 9.2 presents some principles of the con- trollers for systems using power converters as actuators. Section 9.3 deals with a nonlinear control technique called hysteresis control, highlighting some advantages and disadvantages of this technique. Two applications are also considered in this section: dc motor drive system and regulation of an ac variable. Although this book deals with PWM converters processing ac voltage, the dc motor drive system plays an Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 264
  • 279. 9.2 BASIC CONTROL PRINCIPLES 265 important role in understanding a critical feature of the hysteresis control, switching frequency changing with the load. The classic linear controllers (P, PI, and PID) are presented in Section 9.4 for dc variables, while Section 9.5 presents a linear type of controller for ac variables. A more complex control technique is presented in Section 9.6 with a cascade strategy for systems dealing with control of two variables with different dynamic responses. The cascade control strategy is applied to regulate both power factor and dc-link voltage in back-to-back converters for the next chapters. Finally, Section 9.7 summarizes this chapter. 9.2 BASIC CONTROL PRINCIPLES The system presented in Fig. 9.1(a) shows a Controlled Voltage Source supplying an RL load. Let us assume that the control objective in this system is to guarantee the load current regulation, that is, the measured output current (io) must follow a specific reference value (i∗ o). Since the output voltage (𝑣o) has been employed to reach this goal, a simple control block diagram can be obtained, as in Fig. 9.1(b). In this figure, C(s) and H(s) are the controller and the RL load in the s-domain, respectively. The transfer function of the H(s) is given by 1 Ls + R . A discretization method can be employed in order to simulate this system in a digital way (e.g., by using a MATLAB code). One of the simplest ways to discretize a specific process or system is to use the Euler discretization method. This is equivalent of approximating the integrals by using the left-point rule. Hence, the first integral is approximated as the product of the integrand at time t and the integration range dt, which is called step size (h) for the digital implementation. In the system of Fig. 9.1(a), for a given 𝑣o and considering a specific RL load, the following equations can be obtained: 𝑣o = Rio + L dio dt (9.1) dio dt = 𝑣o − Rio L (9.2) Considering the left-point rule, the discrete version of equation (9.2) can be written as io(t + h) = io(t) + 𝑣o − Rio L h (9.3) C(s) R L (a) Controlled voltage source (b) – – + H(s) Σ vo vo io * io io ei Figure 9.1 (a) Controlled voltage source feeding an RL load. (b) Control block diagram.
  • 280. 266 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS %Simulation of a RL load connected to a Controlled- Voltage-Source R=5; %Resistance of the RL load L=0.05; %Inductance of the RL load io=0; %state variable (load current) vo=100; %input variable (load voltage) h=1e-4; %step size j=0; %variable used to storage the outcomes t=0; %initial value of the digital time tmax=1; %maximum simulation time while t<=tmax, %begining of the simulation loop t = t + h; %time incrementation io = io + (vo-R*io)*h/L; %state space variable 1 % storage of the variables j = j + 1; time(j)=t; current(j)=io; voltage(j)=vo; end figure(1),plot(time,voltage) figure(2),plot(time,current) Figure 9.2 MATLAB code for the system presented in Fig. 9.1(a) for open loop operation. Figure 9.2 shows the MATLAB code for the system presented in Fig. 9.1(a), which simulates the behavior of the variables dynamically as well as plots their vari- ables in the time domain. The output current for the open-loop operation has the expected exponential behavior for a step voltage response, as observed in Fig. 9.3. Note that the load current (io) is a function of both the load itself (which is normally not controllable) and the output voltage 𝑣o, which is a variable used to control the load current. To implement the control block diagram presented in Fig. 9.1(b), and con- sidering the digital implementation as done in the MATLAB code of Fig. 9.2, it is necessary to add the code lines related to the controller C(s). For the sake of illustra- tion let us consider a simple proportional controller for C(s), which means that the output of this controller will define the voltage 𝑣o as follows: 𝑣o = Kei (9.4) where K is the gain of the controller and ei is the current error. Assuming a reference current as depicted in Fig. 9.4(a) with a desired step tran- sient, the control system allows that the measured current io will follow its reference, as observed in Fig. 9.4(b). Those waveforms were obtained with K = 200. Due to the inductive characteristics of the load, the value of voltage to allow this step transient of current is expected to be huge at the moment of the step transient (theoretically an infinite voltage is needed to allow such a variation of current). Figure 9.5(a) shows the output voltage of the controller, while Fig. 9.5(b) highlights the instant of the step transient [zoom of Fig. 9.5(a) between t = 0.49 s and t = 0.51 s]. Note that to guarantee a current step transient from 5 to −5 A as in Fig. 9.4, the value of voltage almost reaches −2000 V.
  • 281. 9.2 BASIC CONTROL PRINCIPLES 267 100 0 0.05 0.1 0.15 50 0 v o (V) t (s) (a) 10 0 0.05 0.1 0.15 5 15 20 25 0 i o (A) t (s) (b) Figure 9.3 (a) Output voltage. (b) Output current. 5 0 0.2 0.4 0.6 0.8 1 0 –5 i o (A) * t (s) (a) 5 0 0.2 0.4 0.6 0.8 1 0 –5 i o (A) t (s) (b) Figure 9.4 (a) Reference load current (b) Measured load current.
  • 282. 268 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS 0 0 0.2 0.4 0.6 0.8 1 1000 –1000 –2000 v o (V) * t (s) (a) 0 0.49 0.495 0.5 0.505 0.51 –1000 –2000 v o (V) t (s) (b) Figure 9.5 (a) Load voltage needed for a current step transient in Fig. 9.4. (b) Zoom of the voltage shown in Fig. 9.5(a). Exercise 9.1 Write a MATLAB code to implement the control strategy shown in Fig. 9.1(b) for an RL load (the reader is encouraged to use the code furnished in Fig. 9.2). Plot the waveforms as in Figs 9.4 and 9.5. Additionally, explain the behavior of the output voltage shown in Fig. 9.5 through the equations of the inductor voltage. In a real system, with the controlled voltage source having the maximum limit well defined in terms of voltage and power deliverable to the load, the situation observed in Fig. 9.5 is likely not possible. Even if a controller requires that amount of voltage to guarantee a small current error (ideally zero) during the step transient, there are practical limits for the voltage source, which will not allow such a condition. Indeed, the control scheme presented in Fig. 9.1(b) does not show the controlled voltage source (actuator) needed to implement this control scheme in a real-world scenario. Note from Fig. 9.1(b) that the controller’s output defines the load voltage directly. A more realistic system is considered in Fig. 9.6, in which the controlled voltage source is added for the system through block G(s). C(s) G(s) H(s) Σ * vo vo io * io ei – Figure 9.6 Control block diagram with inclusion of the controlled voltage source.
  • 283. 9.2 BASIC CONTROL PRINCIPLES 269 if t>tpwm, % begin of the pwm loop simulation tpwm=tpwm+hpwm; %definition of discrete time cont=0; %auxiliar variable v10r = vor/2; %pole voltage - leg 1 v20r = -vor/2; %pole voltage - leg 2 tal1 = (v10r/Vdc + 1/2)*hpwm; %Eq. (24) – Chapter 8 tal2 = (v20r/Vdc + 1/2)*hpwm; %Eq. (25) – Chapter 8 end% end of the pwm loop cont=cont+h; % updating auxiliary variable %Definition of the state of the switches if(cont<tal1) q1=1; else q1=0; end if(cont<tal2) q2=1; else q2=0; end v10=(2*q1-1)*(Vdc/2); %Expression for the pole volt. 1 v20=(2*q2-1)*(Vdc/2); %Expression for the pole volt. 2 vo = v10 - v20; %Load voltage Figure 9.7 MATLAB code for implementation of the digital PWM. Block G(s) could be implemented with one of the PWM converters described previously, but an H-bridge topology has been chosen and it will be used through- out this chapter. Applications in a dc motor drive system and in a controlled rectifier circuit will be considered later on in this chapter with the H-bridge converter imple- menting G(s). Under the control point of view, the H-bridge converter must generate a voltage at the load side (𝑣o) that represents accurately the voltage required by the controller 𝑣∗ o. For an ideal controlled voltage source, it turns out that 𝑣o = 𝑣∗ o with G(s) = 1. However, in terms of average value, the H-bridge topology G(s) can be represented more realistically by a first order transfer function, with its time con- stant equal to the switching period, G(s) = 1 Tss + 1 , where Ts = 1∕fs, and fs being the switching frequency of the H-bridge topology. A MATLAB code for an H-bridge converter can be written as in Fig. 9.7. The expressions (9.24), (9.25) deduced in Chapter 8 have been considered in this code for the digital implementation of the pulse widths (𝜏1 and 𝜏2). Note from this code that there is a digital loop to emulate the interrupt in systems like Digital Signal Processors (DSP). In order to implement a control system as seen in Fig. 9.6, the code lines for the converter (Fig. 9.7) should be added in the program presented in Fig. 9.2. Exercise 9.2 (a) Make a step transient for the reference voltage (𝑣∗ o) applied to the H-bridge converter, that is, 𝑣∗ o = −80 V for t < 0.1 s and 𝑣∗ o = 80 V for t ≥ 0.1 s.
  • 284. 270 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS Compare this reference with the average of the output voltage to demonstrate that this kind of converter can be represented approximately by a transfer function given by G(s) = 1 Tss+1 . (b) Combine the code lines presented in Figs 9.2 and 9.7 to implement the closed-loop system as in Fig. 9.6, that is, with the controlled voltage source as actuator; assume Vdc = 100 V. The results of the closed-loop transfer function considering the H-bridge topol- ogy as the controlled voltage source [G(s)] in Fig. 9.6 is presented in Fig. 9.8. When the controller requires a voltage higher than the maximum voltage available through the converter, the controlled voltage source (H-bridge topology) cannot follow this requirement due to physical limitations/restrictions. In this particular case, the maxi- mum and minimum voltages available on the H-bridge topology are 100 and −100 V, respectively. As a consequence of using a non-ideal controlled voltage source, the 0 0 0.2 0.4 0.6 0.8 1 1000 –1000 –2000 –100 –5 0 5 0 100 v o (V) i o (A) v o (V) * t (s) (a) (b) 0 0.2 0.4 0.6 0.8 1 t (s) (c) 0 0.2 0.4 0.6 0.8 1 t (s) Figure 9.8 (a) Controller’s output voltage (b) Converter’s output voltage (c) Load current.
  • 285. 9.3 HYSTERESIS CONTROL 271 0 0.49 0.495 0.5 0.505 0.51 1000 –1000 –2000 –100 –5 0 5 0 100 v o (V) v o (V) i o (A) * t (s) (a) (b) (c) 0.49 0.495 0.5 0.505 0.51 t (s) 0.49 0.495 0.5 0.505 0.51 t (s) Figure 9.9 Zoom of the waveforms presented in Fig. 9.8 around the transient time (t = 0.5 s). control actions will be delayed since instead of applying the necessary voltage to guarantee that transient for the current, that is, 𝑣o ≅ −2000 V, the converter will employ its minimum voltage of −100 V. The time transient will be affected, but the control action is still active, as observed in Fig. 9.9, which shows a zoom of the waveforms presented in Fig. 9.8 around the transient instant. The proportional controller along with other linear regulators will be presented with more details later on in this chapter. However, prior to analyzing deeply the linear controllers, in the following section a hysteresis control strategy will be considered, due to its simplicity. 9.3 HYSTERESIS CONTROL The hysteresis control is one of the simplest ways to guarantee a current control in systems as shown in Fig. 9.1(a). Unlike the linear controllers, such as the proportional
  • 286. 272 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS one considered in Section 9.2 in which the gains should be designed to obtain specific characteristics, the hysteresis control will define directly the state of the switches of the H-bridge topology to make the current follow its reference with a fixed value for the maximum error given by Δi. Notice that the dynamics of the results (and consequently the error) obtained in Figs 9.8 and 9.9 can be changed if another gain for K is employed. Details of how to design the gains of linear controllers are furnished in Section 9.4. Figure 9.10 shows the implementation of the hysteresis-type current controller, highlighting (i) the power and control parts of the circuit [Fig. 9.10(a)], (ii) the wave- form of the variable under control (io) [Fig. 9.10(b) - top], and (iii) the switching states q1 and q2 [Fig. 9.10(b) - middle and bottom]. In this case, the states of the switches are defined as follows: If io > i∗ o + Δi, the load current must be reduced, hence q2 = on (a) (b) 0 0 5 0.01 0.02 0.03 0.04 0.05 Vdc Hysteresis loop L R – – + io * io ei vo io q1 q2 q1 q2 q1 q2 i o , i o (A) * 0 0 1 0.5 0.01 0.02 0.03 0.04 0.05 q 1 0 0 1 0.5 0.01 0.02 0.03 0.04 0.05 q 2 t (s) Figure 9.10 (a) Hysteresis controller defining the state of the switches. (b) Reference and measured currents (top), and the state of the switches q1 and q2 (middle and bottom).
  • 287. 9.3 HYSTERESIS CONTROL 273 and q1 = off If io < i∗ o − Δi, the load current must be increase, hence q1 = on and q2 = off where Δi defines the hysteresis width below and above i∗ o. In steady state opera- tion conditions, the load current ripple is constant. The results of the hysteresis control for the same current transient presented before are shown in Fig. 9.11. The startup condition for the hysteresis control is highlighted in Fig. 9.12 where tr – interval of time in which io changes from 0 to i∗ o; (a) –5 5 0 0 0.5 1 t (s) i o (A) * (b) –5 5 0 0 0.5 1 t (s) i o (A) Figure 9.11 Hysteresis control: reference load current and (b) measured load current. io io * Δi Δi q1 tr Ts tα tβ Figure 9.12 Startup transient for the hysteresis control.
  • 288. 274 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS t𝛼 – time in steady state operation in which q1 is on; t𝛽 – time in steady state operation in which q2 is on; Ts – switching period. During tr the behavior of the load current can be described as in equation (9.5) io(t) = Vdc R ( 1 − e −R L t ) (9.5) when t = tr the load current will be io = i∗ o, then i∗ o = Vdc R ( 1 − e −R L tr ) (9.6) tr = − L R ln ( 1 − Ri∗ o Vdc ) (9.7) The rising time (tr) as well as the switching period (Ts = t𝛼 + t𝛽; in steady state operation) are functions of the load parameters (R and L). Ts is also a function of the hysteresis width (Δi). Exercise 9.3 (a) Write a code in MATLAB to implement the hysteresis control as in Fig. 9.10(a). (b) Validate the expression given in equation (9.7) for two differ- ent RL loads. (c) By using the same simulation code show that the switching frequency of the hysteresis control is dependent of the RL parameters by filling the Table below. R 5 Ω 10 Ω 50 Ω L 5 mH 5 mH 5 mH fs SKSHS Such a dependency of the switching period with the load can restrict the appli- cation of this type of controller. For instance, in dc motor drive applications, in addi- tion to the static components as in the RL load presented in Fig. 9.1(a), the load (dc motor) has also a dynamic component, back electromotive force (emf), which is a function of the rotor speed. This type of load affects directly the performance of the hysteresis controller. This topic is addressed in Section 9.3.1. Another characteristic of the hysteresis control is the constant ripple for the load current, which is defined by 2Δi, that is, the instantaneous error is not zero in the steady state operation. Ideally, to reach null error, Δi should be zero, which implies a hypothetical scenario with infinite switching frequency.
  • 289. 9.3 HYSTERESIS CONTROL 275 Despite this disadvantage, it is possible to see some advantages of the hysteresis control, such as simple implementation and there is no need to define the gains of the controller as done for linear control approaches. 9.3.1 Application of the Hysteresis Control for dc Motor Drive The model of the dc motor is presented in this section in order to understand the influence of a dynamic load in the switching frequency in a hysteresis control approach. A dc motor is constituted by two main magnetic circuits: (i) field circuit located at the stator and (ii) armature circuit placed at the rotor. A sketch of this motor is presented in Fig. 9.13(a), while Fig. 9.13(b) shows the electrical model for the motor, which can be obtained as in equations (9.8) and (9.9): 𝑣f = Rf if + Lf dif dt (9.8) 𝑣a = Raia + La dia dt + ea (9.9) (a) (b) λf λa if if ia υf υf υa υa ea Te Tm ωr Tl Field circuit R L ia R L M e c h a n i c a l l o a d Armature circuit + + – + – + – + – – Figure 9.13 (a) Representation of a dc motor. (b) Equivalent circuit of the field (top) and armature (bottom) circuits.
  • 290. 276 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS where ea = kc𝜆f 𝜔m is the back emf (electromotive force); kc is the coupling constant, 𝜆f is the field flux and 𝜔m is the mechanical speed. The electromagnetic torque is produced due to the trend of the armature flux to align with the field flux, and then the magnitude of this torque is obtained as follows: Te = k′ c𝜆a𝜆f (9.10) or Te = kc𝜆f ia (9.11) Applying Newton’s second law for rotation, that is, the net external torque is equal to the moment of inertia times angular acceleration, then: Te − Tl = Bm𝜔m + Jm d𝜔m dt (9.12) where Tl is the load torque, Bm is the damping coefficient and Jm is the moment of inertia. From equations (9.8), (9.9), and (9.12) it is possible to write the state space representation for this type of machine, as in the following equations: d dt [ ia 𝜔m ] = [ −Ra∕La − kc𝜆f ∕La kc𝜆f ∕Jm −Bm∕Jm ] [ ia 𝜔m ] + [ 1∕La 0 0 −1∕Jm ] [ 𝑣a Tl ] (9.13) 𝜔m = [ 0 1 ] [ ia 𝜔m ] + [0] [ 𝑣a Tl ] (9.14) where ia and 𝜔m are the state space variables. Figure 9.14 shows the MATLAB code for the motor equations presented in (9.13) and (9.14) with the Euler’s integration method. Figure 9.15, in turn, shows the simulation results highlighting the state space variables, that is, armature current and rotor angular speed. Besides the simplification brought up by this model, it describes the dynamics of the system reasonably well. Considering the hysteresis control described in this chapter, let us observe the influence of the motor speed in the switching frequency for a constant hysteresis width (2Δi). For low speed, when the amplitude of the back emf is small (ea = kc𝜆f 𝜔m), the switching frequency of the converter is high. On the other hand, for high speed, when the amplitude of the back emf is high, the switching frequency is low. To explain this behavior, a simulation has been performed with a dc motor connected to a mechani- cal load, which presents a variable characteristic, that is, the torque demand increases with speed squared. Examples of loads that exhibit this variable load torque charac- teristic are centrifugal fans, pumps, and blowers. Also, to illustrate how the switching frequency of the H-bridge converter can be influenced by the motor speed with hysteresis control, a reference armature current is set equal to 10 A for operation in high speed, and set up equal to 2.5 A for low speed operation. The outcomes for the measured and reference currents are presented in
  • 291. 9.3 HYSTERESIS CONTROL 277 %constants ra=0.06; Laa=0.0018; kf=0.1; Bm=0.01; Jm=0.001; lambdaf=1; %state variables wm=0; ia=0; %input variables va=1; %Armature voltage Tl=.1; %Load torque h=1e-4;%step size j=0; t=0; tmax=2; while t<=tmax, t = t + h; % simulation time ia=ia+(va/Laa-ra*ia/Laa-kf*lambdaf*wm/Laa)*h;%state space 1 wm = wm + (kf*lambdaf*ia/Jm-Tl/Jm-Bm*wm/Jm)*h;%state space 2 % storage the variables j = j + 1; time(j)=t; armature_current(j)=ia; rotor_speed(j)=wm; end figure(1),subplot(2,1,1),plot(time,armature_current) subplot(2,1,2),plot(time,rotor_speed) Figure 9.14 MATLAB code for implementation of the dc motor. 0.5 1 0 –2 0 2 4 6 8 10 t (s) i a (A) 0.5 1 0 0 2 4 6 8 10 12 t (s) (a) (b) ω m (rad/s) Figure 9.15 Dynamics of the dc motor showing (a) armature current and (b) rotor speed. Fig. 9.16. As expected, the switching frequency is higher in low speed operation, since T′′ s < T′ s then f′′ s > f′ s . It is worth mentioning that the emphasis that has been given to show the vari- ation of switching frequency in the hysteresis control approach is because it could
  • 292. 278 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS 2.3 0 2 4 6 8 10 12 2.35 2.4 2.45 2.5 2.55 2.6 2.65 2.7 t (s) Ts ' Ts '' High speed operation Low speed operation i a , i a (A) Figure 9.16 Waveforms for reference and measured motor current for operation in high and low speeds. represent a problem in terms of the power electronics converter design. The specifica- tions for the power switch normally consider current, blocking voltage, and switching frequency. Such a power switch may not operate adequately if it is outside the fre- quency range furnished by the manufacturer. 9.3.2 Hysteresis Control for Regulating an ac Variable The previous discussions dealt with the hysteresis approach applied to control a dc variable, that is, a dc current for both RL load and dc machine. The hysteresis control is also useful for controlling ac variables with sinusoidal or non-sinusoidal wave- forms. Examples of control systems requiring sinusoidal and non-sinusoidal wave- forms are ac motor control systems (induction and synchronous motors) and active power filters, respectively. Figure 9.17 shows the implementation of the hysteresis-type current controller, illustrating the circuit itself in Fig. 9.17(a) and the waveforms of the reference (i∗ o) and measured (io) variables in Fig. 9.17(b) and 9.17(c), respectively. Figure 9.17(a) is repeated here for convenience. Note in Fig. 9.17(a) that the definition of the states of the switches is exactly the same as seen previously for the dc control. In Fig. 9.17(b) there is an intentional transient in the current amplitude at t = 0.5 s to show the effec- tiveness of this control strategy. Exercise 9.4 With the approach established earlier to control the dc load current (see the def- inition of the switching states in Section 9.3), the output voltage had only two levels. Determine and simulate a hysteresis method to guarantee the current control as well as to generate an output voltage with three levels.
  • 293. 9.4 LINEAR CONTROL—dc VARIABLE 279 (a) (b) 0 –5 0 5 0.5 1 Vdc Hysteresis loop L R – – + io * io ei vo io q1 q2 t (s) q1 q2 q1 q2 i o (A) (c) 0 –5 0 5 0.5 1 t (s) i o (A) Figure 9.17 (a) Hysteresis controller defining the state of the switches (b) Reference current (c) Measured current. 9.4 LINEAR CONTROL—dc VARIABLE 9.4.1 Proportional Controller: RL Load In Section 9.2 (Basic Control Principles) was presented a simple control approach with a proportional controller, which is the simplest example of linear control. As pre- viously presented in Fig. 9.4, for an ideal, controlled voltage source, and in Fig. 9.8, for a nonideal controlled voltage source, it seems that the proportional controller is able to guarantee error equal to zero. However, this type of controller cannot reach
  • 294. 280 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS null error for a system with a first order transfer function, like an RL load. Indeed, analyzing in detail the waveforms in Figs 9.4 and 9.8 it is possible to realize that those errors are not zero even for an ideal, controlled voltage source. The reader is encouraged to plot those results by using his/her own simulation codes and observe the error between the measured and reference currents. Assuming an ideal controlled voltage source, as in Fig. 9.1(b), the open-loop transfer function [F(s)] and closed-loop transfer function [M(s)] are given respec- tively by F(s) = kp R + sL (9.15) M(s) = kp (R + kp) + sL (9.16) Equation (9.16) shows that in the steady state operation M(s) is not equal to one. When t → ∞ (steady state), s = jω → 0 – meaning that M(s) is equal to kp∕(R + kp). It is evident that null error will be obtained when M(s) = 1, which is only possible if kp → ∞. Also, for the case of using a non-ideal controlled voltage source (H-bridge topology) represented by G(s) = 1 Tss+1 , null error will be obtained only when kp → ∞. Unlike the hysteresis control, for which there is no need to specify gains, for the linear approach, the gains of the controller must be obtained to guarantee specific dynamic characteristics. A graphical analysis known as root locus can be used to determine stability of the system, as well as to visualize the poles and zeros behavior of the closed loop transfer function as a function of the proportional gain parameter, as in Fig. 9.18. These graphs are helpful to determine the design of the proportional controller (kp). For this simple example presented in Fig. 9.18 (i.e., proportional con- troller plus a first order transfer function), the gain should be selected as large as possible to minimize the error. Higher values of proportional gains (kp) guarantee smaller steady-state error and faster response as well, see Fig. 9.18 for kp equal to 1, 5, and 20. 9.4.2 Proportional Controller: dc Motor Drive System To analyze the proportional controller acting as a speed regulator in a dc motor drive system, it is useful to find the transfer function for the motor, as it was done for the RL load. Additionally, a detailed control block diagram will provide important information about how the motor variables and control actions interact among themselves. From the state-space representation in equations (9.13) and (9.14), the transfer function can be obtained as follows: (s) U(s) = C(sI − A)−1 B + D (9.17) where (s) and U(s) are the Laplace transformation for 𝜔m and input variables (𝑣a and Tl), respectively. The matrices for the state-space representation are given by:
  • 295. 9.4 LINEAR CONTROL—dc VARIABLE 281 0 0 2 4 i o , i o (A) i o , i o (A) * 6 1 2 t (ms) 3 4 5 0 0 2 4 i o , i o (A) * 6 1 2 t (ms) 3 4 5 0 0 2 4 6 1 2 t (ms) 3 4 5 kp = 1 Re Im kp = 5 kp = 20 Figure 9.18 Root locus of the system in Fig. 9.1(b). A = [ −Ra ∕La − kc 𝜆f ∕La kc 𝜆f ∕Jm −Bm ∕Jm ] , B = [ 1∕La 0 0 −1∕Jm ] , C = [ 0 1 ] and D = 0. The matrix I is a 2 × 2 identity matrix. Developing equation (9.17) (s) = Ga(s)Va(s) + Gm(s)Tl(s) (9.18) where Ga(s) = ka s2 + (sa + sm)s + k = ka (s + s1)(s + s2) with ka = kc𝜆f JmLa . The poles of the system can be written as follows: s1 = [ − ( sa + sm ) + √ (sa + sm)2 − 4k ] ∕2 s2 = [ − ( sa + sm ) − √ (sa + sm)2 − 4k ] ∕2 with sa = ra∕La, sm = Bm∕Jm, and k = (raBm + k2 c𝜆2 f )∕(JmLa). Considering the model for a dc machine developed in equations (9.13) and (9.14) it is possible to determine its block diagram, as presented in Fig. 9.19, where kc is the coupling constant. This block diagram helps to understand how the variables interact with each other. A simplified block diagram representation for this system
  • 296. 282 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS kc kc If Ia Ia Te Ea + + – – Lf Vf Va Tl Ω Ω Λf + 1 Rf + sLf 1 Ra + sLa 1 Bm + sJm × Figure 9.19 Detailed block diagram representation for a dc-motor. with one output (Ω) and two inputs (Va and Tl) is shown in Fig. 9.20(a). From the speed controller perspective, the term Gm(s)Tl(s) can be considered as a disturbance which must be compensated by the feedback control system. Figure 9.20(b) shows the speed closed-loop control block diagram, while Fig. 9.20(c) shows the same loop control without the disturbance term. The simplifi- cation brought up by Fig. 9.20(c) means that it has been assumed that the controller will be designed in such way that the disturbance term will be compensated by the controller itself, then for simplification purposes, the disturbance can be neglected. For a proportional controller [C(s) = kp] and assuming an ideal controlled volt- age source, the open-loop transfer function [F(s)] and closed-loop transfer function [M(s)] for the system presented in Fig. 9.20(c) are given respectively by F(s) = kpka (T1s + 1)(T2s + 1) (9.19) M(s) = kpka (T1s + 1)(T2s + 1) + kpka (9.20) where T1 = 1∕s1 and T2 = 1∕s2. Considering the steady state analysis (t → ∞ ⇒ s = jω → 0) for equation (9.20), it turns out that M(s) = kpka∕(1 + kpka), which is different from a desirable M(s) = 1 (i.e., null error). The error is not null, unless when kp → ∞, which goes to an unrealistic scenario of infinite voltage needed to keep error equal to zero. As observed in the root locus analysis presented in Fig 9.20(d), the consequence of increasing kp (to reduce the steady state error) is that the imaginary parts of poles will be much higher than the real part of the poles, bringing oscillation issues for response.
  • 297. 9.4 LINEAR CONTROL—dc VARIABLE 283 (a) (b) (c) (d) Va Tl Va Tl – – Ω Ω Ω* EΩ Ga(s) Ga(s) C(s) Va Im Ω Ω* EΩ Ga(s) C(s) Gm(s) Gm(s) + + + + –S2 –S1 Re Increasing kp Increasing kp Figure 9.20 (a) Simple block diagram representation for a dc machine drive system (b) Speed closed-loop control (c) Speed closed-loop control without the disturbance term. (d) Root locus of the dc motor drive system with proportional controller. 9.4.3 Proportional-Integral Controller: RL Load For a system with a first order transfer function (e.g., RL), the simplest linear con- troller to guarantee null error is the proportional-integral one. For this type of con- troller, the F(s) is given by F(s) = ( kp + ki s ) ( 1 R + sL ) (9.21) Equation (9.21) can be conveniently rewritten as below: F(s) = ki s ( kp ki s + 1 ) ( 1∕R L R s + 1 ) (9.22) From equation (9.22) it is evident that the open-loop transfer function has a pole placed at the origin of the complex plane, due to the ki∕s term, which means null
  • 298. 284 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS error at steady state operation. It also suggests that it is possible to cancel the zero of the controller with the pole of the system (RL load), making ki kp = R L (9.23) The zero-pole cancellation furnishes one possible design criterion for determin- ing the gains of the proportional-integral controller. Then, considering equation (9.22) and the zero-pole cancellation, the F(s) and M(s) are given respectively by ki sR and ki sR+ki . The root locus of the system is given in Fig. 9.21, which highlights three-step responses for ki equal to 0.5, 1.5, and 2.5. Once one of the characteristics is picked up from Fig. 9.21 for a specific value of ki, the gain kp will be defined from (9.23). If the zero-pole cancellation is not employed to determine the gains of the controller, the root locus will be clearly different, which could bring up an unde- sired complex situation. Also, the determination of the gains of the controller is not straightforward. Without zero-pole cancellation M(s) will be clearly a more complex 0 0 2 4 i o , i o (A) i o , i o (A) * 6 0.2 0.4 t (s) 0.6 0.8 1 0 0 2 4 6 0.2 0.4 t (s) 0.6 0.8 1 0 0 2 4 i o , i o (A) * ki = 0.5 Re Im ki = 1.5 ki = 2.5 6 0.2 0.4 t (s) 0.6 0.8 1 Figure 9.21 Root locus for a PI controller and RL load.
  • 299. 9.4 LINEAR CONTROL—dc VARIABLE 285 system, as below: M(s) = skp + ki s2L + s(R + kp) + ki (9.24) To test the proportional-integral controller by using the dynamic simulation (as done previously with the MATLAB code), it is necessary to discretize the controller itself. A discretization method using the Euler approach can also be used for simu- lation of the controller. The block diagram model for the PI controller is shown in Fig. 9.22, from which it is possible to determine the state space representation, as below: ̇ x = kie (9.25) y = x + kpe (9.26) Exercise 9.5 Write a MATLAB code to implement a PI controller. Test this code by control- ling an RL load current with both an ideal voltage source and with an H-bridge topology as actuator. For the case where a non-ideal controlled voltage source is considered, the F(s) obtained in (9.22) is now given by: ki s (kp ki s + 1 ) ( 1 Tss+1 ) ( 1∕R L R s+1 ) . In this case, the zero of the controller can be used to cancel one of the two poles, that is, s = −1∕Ts and s = −R∕L. Normally, due to the high switching frequency of the power converters, the dominant pole is s = −R∕L, which must be cancelled if a faster response is desired. 9.4.4 Proportional-Integral Controller: dc Motor As in the case of the RL type of load, a proportional-integral controller is employed to guarantee null error for a dc motor fed by an H-bridge converter. The control block diagram presented in Fig. 9.20(c) and the transfer function of the motor given by Output of the controller e(t) y(t) x(t) x(t) 1 s State space variable Error kp ki Figure 9.22 Block diagram representation for a PI controller.
  • 300. 286 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS Ga(s) = ka (T1s+1)(T2s+1) are considered in this analysis. In this case, unlike the RL load, the system has two poles; one of these poles can be cancelled to obtain specific char- acteristics, such as guarantee of faster dynamic response in a closed loop operation. The open-loop transfer function F(s) after the zero-pole cancelation kp∕ki = T2 is obtained as follows: F(s) = kika s(T1s + 1) (9.27) With the dominant pole cancelled (s = −1∕T2), the M(s) is obtained as M(s) = kika s(T1s + 1) + kika (9.28) Figure 9.23(a) and 9.23(b) shows the speed response for two cases, when the slowest (dominant) pole is cancelled [Fig. 9.23(a)] and when fastest pole is can- celled [Fig. 9.23(b)]. These results were obtained considering the parameters of the dc machine in Fig. 9.14 assuming the same ki gain for both results, that is, ki = 2 and kp = T1ki for Fig. 9.23(a); and with ki = 2 and kp = T2ki for Fig. 9.23(b). Although the waveforms presented in Fig. 9.23(a) and 9.23(b) were obtained with the same number for the integral gain ki = 2, it is also possible to determine the gains of the controllers analytically by using a specific design criterion. For example, Fig. 9.23(c) depicts the root locus of the dc motor with a PI controller after the cancel- lation of the dominant pole. Despite the fact that this controller guarantees null error, its limitation lies in the dynamics of the close-loop transfer function that is limited by −1∕2T1 regardless of the rise of the gain ki. One possible analytical solution for designing the gains of the PI controller can be identical poles for close-loop transfer function, as in ki = 1 4kaT1 (9.29) kp = T2ki (9.30) 9.4.5 Proportional-Integral-Derivative Controller: dc Motor As presented in the last section, the dc motor drive system with a PI controller has one of its poles placed at the origin of the complex plane (i.e., s = 0), which assures null error in steady state operation. From Fig. 9.23(c), however, it is evident that the fastest response obtained with this controller is reached when it leads to the real part of the dominant pole equal to −1∕(2T1). If a faster response is needed, another controller must be employed. Note that for the PI controller applied in this system, the dominant pole is always located on the right side of the pole −1∕T1. A PID controller is able to obtain faster response for a dc motor drive system than a PI type of controller, which has the following transfer function: C(s) = kp + ki s + kds (9.31)
  • 301. 9.4 LINEAR CONTROL—dc VARIABLE 287 (a) (b) (c) 0 0 2 4 6 8 0.2 0.4 t (s) Rotor speed 0.6 0.8 1 0 –1/2T1 –1/T1 0 2 4 6 8 0.2 0.4 t (s) Rotor speed Im Re Increasing ki Increasing ki 0.6 0.8 1 Figure 9.23 Speed dynamic response for cancellation of (a) slowest and (b) fastest pole (c) Root locus of the dc motor with a PI controller. In fact, the derivative term of the controller cannot be implemented as it appears in (9.31), as the transfer function of the PID controller will be: C(s) = kp + ki s + kds sTd + 1 (9.32) or C(s) = (Tdkp + kd)s2 + (Tdki + kp)s + ki s(Tds + 1) (9.33) where Td indicates the quality of the derivative part. Ideally Td must be equal to zero, but its real value depends on the physical limitation of both actuator and system as a whole. The expression (9.33) shows that C(s) presents two poles: s = 0 and s = −1∕Td, and two zeros. The zeros can be used to cancel both poles of the dc motor (as done
  • 302. 288 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS with the PI for cancellation of one pole). Moreover, the parameters kp and kd can be employed to allocate the closed loop poles anywhere in the complex plane. The following design of the controllers can be obtained for the condition of two real identical poles: ki = 1 Ti = 1∕ka 4Td (9.34) kp = T1 + T2 − Td Ti (9.35) kd = T1T2 − (T1 + T2 − Td)Td Ti (9.36) 9.5 LINEAR CONTROL—ac VARIABLE Note that the linear regulators considered so far in this chapter have been employed to control dc variables whether it is RL load or dc machine, current or speed. Two of these controllers were able to guarantee null steady state error (i.e., PI and PID), while the proportional one was not. Indeed, the integral part of the PI and PID con- trollers goes to infinite for dc variables; since the operation frequency is zero, s = 0 and consequently ki∕s → ∞. Such a characteristic leads to a desirable zero error char- acteristic. However, for ac variables, which means s ≠ 0, there is no term in the controller that tends to infinite, which leads to an error different from zero. For the case of ac variables, it is necessary to use another PI type of controller, such as presented below: C(s) = kas2 + kbs + kc (s2 + 𝜔2) (9.37) where ka, kb and kc are the gains of the controller. In this case, the controller presents an infinite value for the rated frequency 𝜔. The state space representation of this controller can be obtained as in equations (9.38)–(9.40) ̇ x1 = x2 + kbe (9.38) ̇ x2 = −𝜔2 x1 + kde (9.39) y = x1 + kae (9.40) where x1 and x2 are state variables and kd = kc − 𝜔2ka. After presenting controllers able to deal with dc and ac variables, it is important to present other control approaches for systems that have more than one variable to be regulated. For instance, a controlled rectifier circuit aims to guarantee power factor correction with sinusoidal current as well as keep the output voltage constant. The following section presents a control strategy regulating two variables known as cascade control.
  • 303. 9.6 CASCADE CONTROL STRATEGIES 289 9.6 CASCADE CONTROL STRATEGIES The control strategies described in this chapter have considered a schematic as pre- sented in Fig. 9.1(b). This leads to a controlled voltage source implemented by a dc–ac converter. For both types of loads (RL and dc motor) considered previously, there is just one variable to be regulated, either current or speed. However, in some applications there is a need to control two variables to reach specific requirements. In this section a control approach called cascade control is presented for two appli- cations, that is, power factor rectifier and dc motor drive system. 9.6.1 Rectifier Circuit: Voltage-Current Control Figure 9.24(a) shows the circuit for a single-phase controlled rectifier, which has two control objectives. They are: guarantee a regulated dc voltage (𝑣o) at the output and a sinusoidal grid current (ig) with power factor close to one at input converter side. Both control objectives are obtained simultaneously through the H-bridge power converter. Before showing details about the control operation of the rectifier circuit pre- sented in Fig. 9.24(a), it is convenient and simple to show the operation of a similar (a) (b) L C R – – – + + + iq1 iq2 ig eg vg iC vo L C R – – – + + + iq1 iq2 Ig Eg Vg iC vo Figure 9.24 (a) Rectifier circuit. (b) Dc–dc converter.
  • 304. 290 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS circuit in terms of the control strategy, as in Fig. 9.24(b). This topology deals with a dc to dc conversion [instead of ac to dc, as in Fig. 9.24(a)] and the principal goal is to control the output voltage. Besides, there is no need to control the power fac- tor; since the primary source of energy is dc, the control strategies for both circuits in Fig. 9.24 can be established following the same principle, that is, using control cascade scheme. Equations (9.41) and (9.42) show that the capacitor current, and consequently the capacitor voltage, can be regulated through Ig. iC = −iq1 − iq2 − 𝑣o R (9.41) iC = Ig(q1 − q2) − 𝑣o R (9.42) Figure 9.25(a) depicts a control block diagram for the converter in Fig. 9.24(b). The control structure for the controlled power factor rectifier in Fig. 9.24(a) is pre- sented in Fig. 9.25(b). The difference between both control approaches for the con- verters in Fig. 9.24(a) and 9.24(b) is the synchronization method for the power factor correction. 9.6.2 Motor Drive: Speed-Current Control The speed control of a dc motor, as presented in Fig. 9.20(c), was obtained directly by defining the armature voltage (Va) as the output of the speed controller. Indeed, (a) (b) – – Ig * Vg * Vg Ig eg iC vo Ig Vo * Vo Voltage controller Voltage controller Current controller Current controller TF of the inductor TF of the inductor Controlled voltage source Controlled voltage source 1 Cv(s) G(s) PLL H(s) sC Eq. (9.42) Ci(s) ev Σ Σ Σ ei – – – Ig * vg θ * vg iC ig vo vo * vo 1 Cv(s) G(s) sin(θ) H(s) sC Eq. (9.42) Ci(s) ev ei eg Eg Σ Σ Σ X * ig ig Figure 9.25 Control block diagrams: (a) for the converter in Fig. 9.24(b). (b) for the converter in Fig. 9.24(a).
  • 305. 9.6 CASCADE CONTROL STRATEGIES 291 + – + – – – Ia * Va * Va Vf Tl If 1 Ω* Ω Ω Ea Te Λf × × Cω(s) Ci(s) Gv(s) Ra + sLa + + kc kc Lf Ia Ia 1 Bm + sJm 1 Rf + sLf Figure 9.26 Cascade control for a dc machine. this control strategy was possible because Ω is a function of Va as shown in Fig. 9.19. However, there are two blocks between these two variables (Fig. 9.19), which repre- sent the electrical and mechanical dynamics for the motor. Fig. 9.26 suggests another solution along with just one block in between the variable used to control (Va) and the variable under control (Ia). The control scheme using an outer controller for the speed (Ω) and an inner controller for the armature current (Ia) is also known as a cascade control, which is in fact the same principle as applied for the rectifier circuit presented in Section 9.6.1. The cascade control is possible in this case because the mechanical and electrical dynamics are completely different, with the internal loop much faster than the external one. Both controllers C𝜔(s) and Ci(s) are PI type of controllers, since it is enough to guarantee null error for the dc variables (Ia and Ω). Although using two controllers, instead of just one as in Fig. 9.20, the main advantage of the cascade control is the possibility to limit the armature current, which brings additional protection for the machine. Assuming that the mechanical variables are constants for the electrical variables perspective, the internal control loop can be simplified as in Fig. 9.27. In this case, the open loop transfer function is given by Fi(s) = ki s ( s kp kI + 1 ) ( 1 Tss + 1 ) ⎛ ⎜ ⎜ ⎝ 1∕ra La ra s + 1 ⎞ ⎟ ⎟ ⎠ (9.43) + + – – Ia * Va * Va Ia Ea 1 Ci(s) Cv(s) Ra + sLa Figure 9.27 Internal control scheme for the block diagram of Fig. 9.26.
  • 306. 292 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS Canceling the zero of the controller with the pole of the motor, it yields Fi(s) = ki s ( 1∕ra Tss + 1 ) (9.44) Consequently the close loop transfer function for the current control is given by Mi(s) = ki∕ra Tss2 + s + ki∕ra (9.45) As seen before, the gain ki can be obtained by using either a root locus approach or making identical poles, which means ki = ra∕(4Ts); then Mi(s) = 1 (2Tss + 1)2 (9.46) Since Ts is a small value, Mi(s) becomes Mi(s) = 1 4Tss + 1 (9.47) The external loop of the block diagram shown in Fig. 9.26 is given in Fig. 9.28. Considering Tl as a perturbation to be compensated by the controller, the open loop transfer function for the speed controller is given by F𝜔(s) = ki𝜔kc𝜆f Bm (kp𝜔 ki𝜔 s + 1 ) s ( Jm Bm s + 1 ) (4Tss + 1) (9.48) Cancelling the zero with the pole we have F𝜔(s) = ki𝜔kc𝜆f Bm 1 s(4Tss + 1) (9.49) Then the close loop transfer function is given by M𝜔(s) = ki𝜔kc𝜆f Bm 4Tss2 + s + ki𝜔kc𝜆f Bm (9.50) Making identical poles we have M𝜔(s) = 1 (8Tss + 1)2 (9.51) Ia + – * Ia 1 Ω Ω* Te Kc Λf Mi(s) Cω(s) Bm + sJm + – Tl Figure 9.28 External loop of the controller in Fig. 9.26.
  • 307. REFERENCES 293 From this approach it is possible to design the gains of the controller as follows: kp𝜔 ki𝜔 = Jm Bm with ki𝜔 = Bm 16Tskckf . 9.7 SUMMARY This chapter presented the basic principles of controllers for systems using power converters as actuators. This is indeed a preparation for the next chapters that will need feedback control actions to guarantee the correct operation of the back-to-back converters. This chapter is divided into two parts: nonlinear and linear control tech- niques. Section 9.3 dealt with a nonlinear control technique, that is, hysteresis control, highlighting some advantages and disadvantages. Two applications were also con- sidered in this section: dc motor drive system and regulation of an ac variable. The classic linear controllers (P, PI, and PID) were presented in Section 9.4 for dc vari- ables, while Section 9.5 presented a linear type of controller for ac variables. A more complex control technique was presented in Section 9.6 with a cascade strategy to introduce back-to-back converters, which are described in the following chapters. More details on the control techniques described can be found from 1 to 18. REFERENCES [1] L. Shang, D. Sun, J. Hu, Sliding-mode-based direct power control of grid-connected voltage-sourced inverters under unbalanced network conditions, Power Electron, IET, vol. 4, no. 5, pp. 570–579, May 2011. [2] R.-J. Wai, C.-Y. Lin, Dual active low-frequency ripple control for clean-energy power-conditioning mechanism, IEEE Trans Ind Electron, vol. 58, no. 11, pp. 5172–5185, Nov. 2011. [3] B. Labbe, B. Allard, X. Lin-Shi, D. Chesneau, An integrated sliding-mode buck converter with switching frequency control for battery-powered applications, IEEE Trans Power Electron, vol. 28, no. 9, pp. 4318–4326, Sept. 2013. [4] J. Hu, L. Shang, Y. He, Z.Q. Zhu, Direct active and reactive power regulation of grid-connected DC/AC converters using sliding mode control approach, IEEE Trans Power Electron, vol. 26, no. 1, pp. 210–222, Jan. 2011. [5] R. Haroun, A. Cid-Pastor, A.E. Aroudi, L. Martinez-Salamero, Synthesis of canonical elements for power processing in DC distribution systems using cascaded converters and sliding-mode control, IEEE Trans Power Electron, vol. 29, no. 3, pp. 1366–1381, March 2014. [6] M. Khazraei, H. Sepahvand, M. Ferdowsi, K.A. Corzine, Hysteresis-based control of a single-phase multilevel flying capacitor active rectifier, IEEE Trans Power Electron, vol. 28, no. 1, pp. 154–164, Jan. 2013. [7] D.G. Holmes, R. Davoodnezhad, B.P. McGrath, An improved three-phase variable-band hysteresis current regulator, IEEE Trans Power Electron, vol. 28, no. 1, pp. 441–450, Jan. 2013. [8] T.-W. Chun, Q.-V. Tran, H.-H. Lee, H.-G. Kim, Sensorless control of BLDC motor drive for an automotive fuel pump using a hysteresis comparator, IEEE Trans Power Electron, vol. 29, no. 3, pp. 1382–1391, March 2014. [9] S. Gautam, R. Gupta, Unified time-domain formulation of switching frequency for hysteresis cur- rent controlled AC/DC and DC/AC grid connected converters, Power Electron, IET, vol. 6, no. 4, pp. 683–692, April 2013. [10] Dash AR, Babu BC, Mohanty KB, Dubey R. Analysis of PI and PR controllers for distributed power generation system under unbalanced grid faults. 2011 International Conference on Power and Energy Systems (ICPS); 2011 22–24 Dec. p. 1–6.
  • 308. 294 CHAPTER 9 CONTROL STRATEGIES FOR POWER CONVERTERS [11] Geethalakshmi B, Saraswathi A, Dananjayan P. Comparing and evaluating the performance of SSSC with Fuzzy Logic controller and PI controller for transient stability enhancement. IICPE 2006. India International Conference on Power Electronics; 2006 Dec 19–21. p. 140–143. [12] Mikkili S, Panda AK, Patnaik SS, Suresh Y. Comparison of two compensation control strategies for SHAF in 3ph 4wire system by using PI controller. 2010 India International Conference on Power Electronics (IICPE); 2011 Jan 28–30. p. 1–7. [13] Tsengenes G, Adamidis G. Comparative evaluation of Fuzzy-PI and PI control methods for a three phase grid connected inverter. Proceedings of the 2011-14th European Conference on Power Elec- tronics and Applications (EPE 2011); Aug. 30 2011-Sept. 1 2011. p. 1–10. [14] P. Kasinathan, R. Vairamani, S. Sundramoorthy, Dynamic performance investigation of d–q model with PID controller-based unified power-flow controller, Power Electron, IET, vol. 6, no. 5, pp. 843–850, May 2013. [15] Z. Shen, N. Yan, H. Min, A multimode digitally controlled boost converter with PID autotuning and constant frequency/constant off-time hybrid PWM control, IEEE Trans Power Electronics, vol. 26, no. 9, pp. 2588–2598, Sept. 2011. [16] M.Y.-K. Chui, W.-H. Ki, C.-Y. Tsui, A programmable integrated digital controller for switching con- verters with dual-band switching and complex pole-zero compensation, IEEE J Solid-State Circuits, vol. 40, no. 3, pp. 772–780, March 2005. [17] M.M. Peretz, S. Ben-Yaakov, Time-domain design of digital compensators for PWM DC-DC con- verters, “IEEE Trans Power Electron,” vol. 27, no. 1, pp. 284–293, Jan. 2012. [18] Rasoanarivo I, Arab-Tehrani K, Sargos FM. Fractional Order PID and Modulated Hysteresis for high performance current control in multilevel inverters. 2011 IEEE Industry Applications Society Annual Meeting (IAS); 2011 Oct 9–13. p. 1–7.
  • 309. CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER 10.1 INTRODUCTION Single-phase two-stage energy conversion systems are considered in this chapter. Such conversion systems, also known as back-to-back converters, deal with recti- fication and inversion through a dc-link capacitor. The control goals are high power factor and sinusoidal current at the input side of the converter and regulated voltage at its output side. Several applications require this type of conversion system, such as line voltage regulators, universal active power filters, standby power supplies, and uninterruptible power supplies. Power blocks are again employed in this chapter as an effective way to under- stand how the topologies presented in the technical literature have been conceived. Furthermore, many of the subjects considered in the previous chapters (e.g., opti- mized PWM and control strategies) are used to improve the converter’s operation in terms of total harmonic distortion (THD) and efficiency, as well as to regulate the variables of the back-to-back converter, such as grid power factor and dc-link voltage. This chapter describes the full-bridge topology for single-phase ac–dc–ac con- version in Section 10.2. In addition to the model, pulse width modulation (PWM), and control strategies, a power analysis and an expression for the dc-link capaci- tor oscillation are also presented in the section. Three sections of this chapter deal with nonconventional topologies, that is, topologies with reduced (Section 10.3) and increased (Sections 10.4 and 10.5) number of power semiconductor devices. Semi- conductor component count reduction is obtained by either sharing a leg or by using the dc-link mid-point connection. On the other hand, topologies with increased num- ber of components are addressed by connecting back-to-back converters both in par- allel and series. This will allow THD improvements and reducing power processed by each converter. A summary of the chapter is presented in Section 10.6, while Section 10.7 shows the references. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 295
  • 310. 296 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER 10.2 FULL-BRIDGE CONVERTER 10.2.1 Model By connecting two PBs back-to-back, it is possible to build a single-phase to single-phase ac–dc–ac as presented in Fig. 10.1(a). The representation using switches is given in Fig. 10.1(b). The conversion system consists of a single-phase utility grid, input inductor (with reactance Xg), capacitor bank at the dc-link with two capacitors (each one with capacitance equal to C), rectifier, inverter, and a single-phase load. Technically, the dc-link capacitor bank in Fig. 10.1 could be implemented with just one capacitance. However, for the sake of modeling, it is convenient to draw this circuit with two capac- itors to have access to the point “0.” The inductive element (Lg) between the utility grid and the input converter side is needed to avoid short-circuit between both volt- age source type of element (grid and input converter side). Also, the dc-link bank is needed to decouple input and output converter sides. Moreover, it is expected that the input side of the converter in Fig. 10.1 operates as boost converter since the dc-link voltage should be bigger than the grid voltage to guarantee grid current control. The rectifier circuit constitutes switches qg1 and qg2, and their complementary switches given respectively by qg1 and qg2. The inverter, in turn, constitutes switches ql1 and ql2 and their complementary switches ql1 and ql2. As considered in previous chapters, the conduction state of the switches is represented by a binary variable, where q = 1 indicates a closed switch while q = 0 is an open one with = g1, g2, l1, and l2. From Fig. 10.1(b), the following equations can be derived for both input and output con- verter sides as in equations (10.1) and (10.2), respectively: 𝑣g = 𝑣g10 − 𝑣g20 (10.1) (a) (b) – + – – + – + + ig iC vC il vl eg vg Xg qg1 qg2 g1 g2 ql2 ql1 ql2 ql1 l1 l2 0 2 qg2 qg1 vC vl 2 Figure 10.1 Two-leg converter supplying a single-phase load: (a) blocks and (b) switch representation.
  • 311. 10.2 FULL-BRIDGE CONVERTER 297 𝑣l = 𝑣l10 − 𝑣l20 (10.2) where the pole voltages can be written as a function of the states of the switches, as follows: 𝑣g10 = (2qg1 − 1) 𝑣C 2 (10.3) 𝑣g20 = (2qg2 − 1) 𝑣C 2 (10.4) 𝑣l10 = (2ql1 − 1) 𝑣C 2 (10.5) 𝑣l20 = (2ql2 − 1) 𝑣C 2 (10.6) Equation (10.7) furnishes the dynamic model for the variables of the grid con- verter side: 𝑣g = eg − rgig − lg dig dt (10.7) where rg and lg represent the resistances and inductances of the input inductor. The capacitor voltage can be obtained as follows: 𝑣c = 1 C∫ [(qg1 − qg2)ig + (ql2 − ql1)il]dt (10.8) with the interval of integration equal to the switching frequency. It is worth mentioning that the same approach used earlier in this book is con- sidered in this chapter: (i) modeling the system by writing the voltage generated by the converter as a function of the switching states, (ii) defining the switching states by using a PWM technique, and (iii) obtaining the desired voltages for the PWM with closed-loop operation. 10.2.2 PWM Strategy The optimized PWM strategy presented in Chapter 8 can be employed for the full-bridge configuration presented in Fig. 10.1 to improve either THD or efficiency at both sides (input and output) of the converter. If the desired input and output voltages are given respectively by 𝑣∗ g and 𝑣∗ l , the reference pole voltages can be written as follows: 𝑣∗ g10 = 𝑣∗ g + 𝑣∗ gh (10.9) 𝑣∗ g20 = 𝑣∗ gh (10.10) 𝑣∗ l10 = 𝑣∗ l + 𝑣∗ lh (10.11) 𝑣∗ l20 = 𝑣∗ lh (10.12)
  • 312. 298 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER The auxiliary voltages 𝑣∗ gh and 𝑣∗ lh are given respectively by 𝑣∗ gh = 𝑣C ( 𝜇g − 1 2 ) + (𝜇g − 1)V∗ gmax − 𝜇gV∗ gmin (10.13) 𝑣∗ lh = 𝑣C ( 𝜇l − 1 2 ) + (𝜇l − 1)V∗ lmax − 𝜇lV∗ lmin (10.14) where Vgmax = MAX{𝑣∗ g, 0}, Vgmin = MIN{𝑣∗ g, 0} and Vlmax = MAX{𝑣∗ l , 0}, Vlmin = MIN{𝑣∗ l , 0}; 𝜇g and 𝜇l are the distribution factor and determine how the free-wheeling time can be distributed throughout the switching period. Note that 𝑣∗ gh and 𝑣∗ lh are independent of each other. Equations (10.13) and (10.14) were deduced in Section 8.2.2. Once the reference pole voltages have been defined in equations (10.9)–(10.12), the pulse widths 𝜏g1, 𝜏g2, 𝜏l1, and 𝜏l2 can be calculated by equations (10.15)–(10.18), as follows: 𝜏g1 = ( 𝑣∗ g10 𝑣C + 1 2 ) Ts (10.15) 𝜏g2 = ( 𝑣∗ g20 𝑣C + 1 2 ) Ts (10.16) 𝜏l1 = ( 𝑣∗ l10 𝑣C + 1 2 ) Ts (10.17) 𝜏l2 = ( 𝑣∗ l20 𝑣C + 1 2 ) Ts (10.18) where Ts is the switching period. 10.2.3 Control Approach Figure 10.2 presents the control block diagram for the system in Fig. 10.1. The input power factor and the dc-link capacitor voltage are both controlled by using this control approach. The output voltage is obtained by open-loop operation just setting up the PWM signals for the legs l1 (i.e., switches ql1 –ql1) and l2 (i.e., switches ql2 –ql2). Note that a cascade control approach is employed since the dynamics of the capacitor voltage is completely different from the inner loop that deals with grid current. The dc-link voltage 𝑣C is adjusted to its reference value 𝑣∗ C using the controller RC, which is implemented with a standard PI controller. This controller provides the amplitude of the reference grid current I∗ g . To maintain the power factor close to one with a sinusoidal grid current, the instantaneous reference current i∗ g must be syn- chronized with the input voltage eg. Such a synchronization scheme can be obtained via a PLL algorithm. The block Ge –ig is responsible for generating the reference sinusoidal grid current in phase with the grid voltage i∗ g = I∗ g sin(𝜔gt + Φg), which means that Φg is the phase angle of the grid voltage and 𝜔g is the grid frequency. The current controller loop must deal with sinusoidal waveforms, which means that the
  • 313. 10.2 FULL-BRIDGE CONVERTER 299 – – + + ig * vg * vgh * vlh * vl * ig * * vC vC eg Σ Σ ig μg μl RC Ri PWM Load Rectifier/Inverter Voltage sensor Voltage sensor Current sensor Grid Ge-ig Equation (13) Equation (14) qg1 qg2 ql2 ql1 Figure 10.2 Control strategy for the single-phase to single-phase converter. conventional PI controller will not guarantee null error in steady-state operation – a modified PI controller can be employed instead (see Section 9.5). As presented in Fig. 10.2 and mentioned earlier, the output voltage control is obtained by open-loop operation. The PWM block presented in Fig. 10.2 can be implemented either from equations (10.15)–(10.18) or by comparing these reference pole voltages with high frequency carrier signals. Exercise 10.1 Draw a block diagram system with a hysteresis current control instead of using the linear controller Ri in Fig. 10.2. Is there any change for the number of current and voltage sensors employed with the hysteresis control scheme? 10.2.4 Power Analysis To find an expression of the capacitor voltage as a function of the system’s vari- ables including the power demanded by the load, let us assume the following general scenario: Grid Voltage. eg(t) = Eg cos(𝜔gt) Low Frequency Voltage of the Input Converter Side. 𝑣g(t) = Vg cos(𝜔gt − 𝜃g) Grid Current. ig(t) = Ig cos(𝜔gt + Φg)
  • 314. 300 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER vg eg ig vl il ϕg ε θg ϕl Figure 10.3 Phasor diagram for the low frequency converter variables of Fig. 10.1. Low Frequency Voltage of the Output Converter Side. 𝑣l(t) = Vl cos(𝜔lt + 𝜀) Load Current. il(t) = Il cos(𝜔lt + 𝜀 + Φl) All these variables are depicted in the phasor diagram presented in Fig. 10.3. The effect of the high frequency voltages generated by the converters are neglected to simplify the analysis. Also, for the sake of simplification, the phasors of the input and output variables are considered in the same figure, which means that they have the same frequencies. The input and output powers are given by pg(t) = 𝑣g(t)ig(t) and pl(t) = 𝑣l(t)il(t), respectively. Neglecting the converter power losses, the dc-link capacitor power can be obtained as pc(t) = pg(t) − pl(t) (10.19) or pc(t) = [ VgIg 2 cos ( 𝜃g + Φg ) − VlIl 2 cos(Φl) ] + [ VgIg 2 cos ( 2𝜔gt − 𝜃g + Φg ) − VlIl 2 cos(2𝜔lt + 2𝜖 + Φl) ] (10.20) As long as the converter losses are neglected, the active power demanded by the load is generated by the single-phase grid without losses through the conversion stage, that is, VgIg cos(𝜃g + Φg) = VlIl cos(Φl) (10.21) Substituting (10.21) into (10.20), the capacitor power is given by pc(t) = VgIg 2 cos(2𝜔gt − 𝜃g + Φg) − VlIl 2 cos(2𝜔lt + 2𝜖 + Φl) (10.22) or pc(t) = Nl cos(Φl) cos(𝜃g + Φg) cos(2𝜔gt − 𝜃g + Φg) − Nl cos(2𝜔lt + 2𝜖 + Φl) (10.23) where Nl = VlIl∕2.
  • 315. 10.2 FULL-BRIDGE CONVERTER 301 Equation (10.23) suggests that the pulsating powers inherent from single-phase systems (at input and output sides of the converter) appear on the dc-link capaci- tor bank. One of the desired operation conditions is input power factor close to one, which is obtained imposing Φg = 0 (see Fig. 10.3). Although there is no control for some of the parameters in equation (10.23), such as Nl and Φl, the phase angle 𝜖 can be employed to reduce the pulsating power on the dc-link capacitors if both input and output converter sides have the same frequencies. Exercise 10.2 Considering the input converter side modeled as a controlled voltage source (𝑣g), as depicted in the figure below, determine the value of Xg for an input power factor equal to one and assuming the following conditions: eg(t) = 170 cos(2𝜋60t + 12∘), 𝑣g(t) = 204 cos(2𝜋60t) and with the amplitude of the grid current equal to 10A. Assume an ideal inductance. vg ig Xg + – eg + – 10.2.5 dc-link Capacitor Voltage The capacitor voltage can be achieved from capacitor power. Notice that pc(t) = 𝑣cic = C𝑣c d𝑣c dt (10.24) this leads to 𝑣c d𝑣c dt = Nl C [ cos ( Φl ) cos(𝜃g + Φg) cos(2𝜔gt − 𝜃g + Φg) − cos(2𝜔lt + 2𝜖 + Φl) ] (10.25) Applying an integral at both sides of equation (10.25), it is possible to write 𝑣2 c = Nl ⎡ ⎢ ⎢ ⎣ cos ( Φl ) cos(𝜃g + Φg) Xcg sin(2𝜔gt − 𝜃g + Φg)− Xcl sin(2𝜔lt + 2𝜖 + Φl) ⎤ ⎥ ⎥ ⎦ + 𝑣c (10.26) where Xcg = 1 𝜔gC , Xcl = 1 𝜔lC and 𝑣c is a dc value of 𝑣c.
  • 316. 302 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER vc Δvc t 0 Vc Figure 10.4 Typical dc-link voltage in single-phase back-to-back converters. Therefore, the capacitor voltage can be written as follows: 𝑣c = √ 𝑣c + ̃ 𝑣c (10.27) where ̃ 𝑣c = NlXcl [ cos(Φl) cos(𝜃g+Φg) fl fg sin(2𝜔gt − 𝜃g + Φg) − sin(2𝜔lt + 2𝜖 + Φl) ] Once the dc-link voltage is well known as being composed of a dc value overlapped by a small ac component, as in Fig. 10.4, it is possible to expand equation (10.27) in a Taylor series around Vc. Since the Taylor series represents a function as an infinite sum of terms that are calculated from the values of the functions derivatives at a single point, the dc-link voltage can be expressed as follows: 𝑣c = Vc + ̃ 𝑣c 2Vc − ̃ 𝑣2 c 8Vc + ∞ ∑ n=3 [ (−1)n+1 n! ̃ 𝑣n c 2ñ 𝑣 2n−1 c n ∏ j=2 (2j − 3) ] (10.28) The power series in (10.28) shows that the capacitor voltage consists of a dc component and an ac component with infinite number of elements. However, for practical values of the capacitor size and the dc-link reference voltage, the capaci- tor voltage is well represented by the first two terms in (10.28) (i.e., Vc + (̃ 𝑣c∕2Vc)). This approximation results in the following expression: 𝑣c ≃ Vc + NlXcl 2Vc [ cos ( Φl ) cos(𝜃g + Φg) fl fg sin(2𝜔gt − 𝜃g + Φg) − sin(2𝜔lt + 2𝜖 + Φl) ] (10.29) In order to analyze the voltage fluctuation, it is convenient to define the maxi- mum (peak-to-peak) capacitor voltage as Δ𝑣c = 𝑣cmax − 𝑣cmin, where 𝑣cmax and 𝑣cmin are the maximum and minimum values of 𝑣c in (10.29). The maximum value (𝑣cmax) occurs when sin(2𝜔gt − 𝜃g + Φg) = 1 and sin(2𝜔lt + 2𝜖 + Φl) = −1 happen simulta- neously, and the minimum value (𝑣cmin) occurs when sin(2𝜔gt − 𝜃g + Φg) = −1 and sin(2𝜔lt + 2𝜖 + Φl) = 1 happen simultaneously. Hence, 𝑣cmax ≃ Vc + NlXcl 2Vc [ cos ( Φl ) cos(𝜃g + Φg) fl fg + 1 ] (10.30)
  • 317. 10.2 FULL-BRIDGE CONVERTER 303 𝑣cmin ≃ Vc − NlXcl 2Vc [ cos ( Φl ) cos(𝜃g + Φg) fl fg + 1 ] (10.31) The dc-link voltage fluctuation is given by Δ𝑣c ≃ NlXcl Vc [ cos ( Φl ) cos(𝜃g + Φg) fl fg + 1 ] (10.32) From (10.32), it can be seen that the increase of the capacitance size reduces the peak-to-peak voltage. For same grid and load frequencies (𝜔g = 𝜔l = 𝜔) and unitary input power factor (cos Φg = 1), (10.29) can be written as follows: 𝑣c(t) ≃ Vc + NlXc 2Vc k𝜖 cos(2𝜔 + 𝛽) (10.33) where k𝜖 = √ k2 Φ − 2kΦ cos(𝜃g + 2𝜖 + Φl) + 1 kΦ = cos(Φl)∕ cos(𝜃g), Xc = 1∕𝜔C and 𝛽 = tan−1 [ cos Φl − cos ( 2𝜖 + Φl ) cos Φl tan 𝜃g + sin(2𝜖 + Φl) ] The term k𝜖 plays an important role for reduction of the pulsating voltage (Δ𝑣c) on the capacitor voltage. If both grid and load have the same frequencies (e.g., unin- terrupted power supply (UPS)) it is possible to use synchronization of the input and output voltages to reduce k𝜖 and consequently reduce Δ𝑣c. The maximum, minimum, and fluctuation values of 𝑣c are given respectively by 𝑣cmax ≃ Vc + NlXc 2Vc k𝜖 (10.34) 𝑣cmin ≃ Vc − NlXc 2Vc k𝜖 (10.35) Δ𝑣c ≃ NlXc Vc k𝜖 (10.36) The term k𝜖 reaches its maximum and minimum values for 𝜖 = −(𝜃g + 𝜙l + 𝜋)∕2 and 𝜖 = −(𝜃g + 𝜙l)∕2, respectively. Figure 10.5 shows k𝜖 as a function of the load power factor 𝜙l for the following conditions: Nl = 1pu and Vl = Eg = √ 2pu. 𝜖 = 0 also guarantees a considerable reduction for k𝜖. In Fig. 10.5, 𝜙l < 0 means a lagging power factor, while 𝜙l > 0 means a leading power factor. Exercise 10.3 UPS is an electrical apparatus that is designed to provide power to a load even when the input utility grid is not available. Such a device normally employs
  • 318. 304 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER ε = 0 k ε ε = –(θg + ϕl)/2 –90 0 0.5 1 1.5 2 2.5 –60 –30 0 30 60 90 ε = –(θg + ϕl + π)/2 ϕl (°) Figure 10.5 k𝜀 as a function of the load power factor 𝜙l. energy storage elements like batteries to furnish energy to the load when the mains power fails. Assuming a single-phase to single-phase back-to-back con- verter (as in Fig. 10.1) employed as an UPS with a set of batteries connected to the dc-link voltage, and with a load frequency equal to the grid frequency, determine the phase angle of the load voltage (𝜀) to obtain the minimum value for the capacitor voltage oscillation. Consider that 𝜃g = 12∘, and that the input and output power factors are given respectively by 1 and 0.85. 10.2.6 Capacitor Bank Design In order to apply the input voltage with amplitude Vg and the output voltage with amplitude Vl, the dc-link voltage 𝑣c should be larger than both Vg and Vl at any instant of time. Figure 10.6(a) shows a case where an ideal scenario is considered with a dc-link voltage without any fluctuation. The grid reference voltage is also pre- sented in this figure. On the other hand, Fig. 10.6(b) depicts the case in which the desired grid voltage cannot be generated appropriately because of the dc-link volt- age fluctuation. Therefore, the minimum value of 𝑣c given in (10.35) must satisfy the following equation: 𝑣cmin ≥ max{Vg, Vl} (10.37) By choosing equation (10.37) as a minimum value for 𝑣c, the impedance Xcl can be written from (10.31) as Xcl = Vc − max{Vg, Vl} Nl 2Vc ( cos(Φl) cos(𝜃g + Φg) fl fg + 1 ) (10.38)
  • 319. 10.2 FULL-BRIDGE CONVERTER 305 vc Δvc vg * vg * t t 0 0 Vc vc Vc (a) (b) Figure 10.6 dc-Link voltage in single-phase back-to-back converters: (a) ideal scenario with no oscillation and (b) real scenario with a pulsating voltage on 𝑣c. Once load and grid voltages are specified, the average value of the capacitance must be chosen, based on the acceptable voltage fluctuation. Hence, the impedance Xcl, and consequently the capacitor C, can be calculated from (10.38). Exercise 10.4 For a single-phase back-to-back converter supplying a load with apparent power equal to 2000 V-A, determine the capacitance value for the dc-link assuming: 𝜃g = 12∘ with input and output power factors given respectively by 1 and 0.85. It is also known that the input and output voltages are the same and are given by 120 V(RMS)–60Hz. Assume a maximum dc-link voltage oscillation equal to 10 V. Application (Uninterrupted Power Supply – UPS) As mentioned earlier in this chapter, the single-phase back-to-back converter can be employed as a UPS. The figure below (top) shows a simplified schematic of an online UPS highlighting the operation modes, while the bottom part of the figure shows the implementation of the online UPS with the configuration presented in Fig. 10.1. This system is characterized by its ability to supply conditioned and regu- lated power to a critical load during the normal and backup operations. Note that the inverter is between the primary source of energies (grid or battery) and the load – this system is also known as inverter-preferred or double-conversion UPS. In the case of malfunction of the inverter, the bypass switch is turned on. Normal operation Backup operation Load Inverter Rectifier Grid Bypass switch dc–dc Battery
  • 320. 306 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER Bypass switch Bidirectional dc–dc converter dc–dc LPF + – vl + – eg Another type of UPS is the line-interactive with the schematic presented in the figure below. During the normal operation, the grid is connected to the load directly through static switches. These switches are connected to multiple taps on the secondary transformer to compensate grid voltage variation. Also, during nor- mal operation, the circuit should be able to charge the battery without any additional hardware – such a condition is obtained when the grid is feeding the load and con- sequently there is voltage at the primary transformer. If both bottom switches of the H-bridge converter are turned on simultaneously (i.e., short-circuit of the transformer at the primary side) the current iBat will increase quickly. If the bottom switch is turned off iBat will flow through the antiparallel diode of the top switch to the battery and consequently charge it. The charging process is a high-frequency operation that allows the current to go from the grid to the battery without any additional compo- nent. During the backup operation, the load voltage is furnished with the following parts: battery, H-bridge configuration, transformer, and capacitor. In this case the static switches are all turned off. Normal operation Backup operation Load Grid dc–ac Battery Static switch
  • 321. 10.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 307 Static switch 1:n + – vl + – eg iBat 10.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 10.3.1 Model Another single-phase back-to-back power converter is obtained by combining the first and third PB-ac as in Fig. 10.7(a). Figure 10.7(b) shows the same configuration with the switches represented. Note that the leg constituted by the switches qs –qs is shared between the input and output sides of the converter. As compared to the topology in Fig. 10.1 there is a reduction of 25% of the number of power switches employed in the shared-leg converter. However, it is evi- dent that the leg constituted by the switches qs and qs will handle a current that is dependent on the input and output currents (ig − il). Also, as discussed later in this section, the shared-leg plays an important role in the voltage capability of the con- verter. It is worth mentioning that the cost reduction will be effective if what is saved by reducing the number of semiconductor devices is not lost in higher device ratings and more electrolytic capacitor energy storage to keep the same conditions as in the full-bridge converter. The following equations can be derived from Fig. 10.7(b) for both input and output converter sides: 𝑣g = 𝑣g0 − 𝑣s0 (10.39) 𝑣l = 𝑣l0 − 𝑣s0 (10.40) The pole voltages can be written as a function of the states of the switches: 𝑣g0 = (2qg − 1) 𝑣C 2 (10.41) 𝑣s0 = (2qs − 1) 𝑣C 2 (10.42) 𝑣l0 = (2ql − 1) 𝑣C 2 (10.43)
  • 322. 308 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER (a) (b) – – + + – – + + ig vg iC vC il vl eg vg Xg qg qs ql qg qs ql ql1 s l 0 vl Figure 10.7 Shared-leg single-phase to single-phase back-to-back converter: (a) block and (b) switch representation. Equation (10.7) is still valid for modeling the input converter side. However, the capacitor voltage is given by 𝑣c = 1 C∫ [igqg + (il − ig)qs − ilql]dt (10.44) with the interval of integration equal to the switching period. 10.3.2 PWM Strategy If the desired input and output voltages are given respectively by 𝑣∗ g and 𝑣∗ l , one option for the reference pole voltages is as follows: 𝑣∗ g0 = 𝑣∗ g + 𝑣∗ h (10.45) 𝑣∗ s0 = 𝑣∗ h (10.46) 𝑣∗ l0 = 𝑣∗ l + 𝑣∗ h (10.47) Unlike the previous full-bridge converter that has employed two auxiliary volt- ages 𝑣∗ gh and 𝑣∗ lh to optimize both converter sides independently, the PWM strategy presented in (10.45)-(10.47) uses just one variable 𝑣∗ h due to the coupling between the input and output sides of the converter through the leg constituted by the switches
  • 323. 10.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 309 qs –qs. 𝑣∗ h is given by 𝑣∗ h = 𝑣C ( 𝜇 − 1 2 ) + (𝜇 − 1)V∗ max − 𝜇V∗ min (10.48) with Vmax = MAX{𝑣∗ g, 0, 𝑣∗ l } and Vmin = MIN{𝑣∗ g, 0, 𝑣∗ l }. Once the reference pole voltages have been defined, pulse widths 𝜏g, 𝜏s, and 𝜏l are given by 𝜏g = ( 𝑣∗ g0 𝑣C + 1 2 ) Ts (10.49) 𝜏s = ( 𝑣∗ s0 𝑣C + 1 2 ) Ts (10.50) 𝜏l = ( 𝑣∗ l0 𝑣C + 1 2 ) Ts (10.51) Exercise 10.5 Draw the control block diagram for the converter shown in Fig. 10.7 by adapt- ing the cascade control strategy shown in Fig. 10.2. 10.3.3 dc-link Voltage Requirement As aforementioned, the shared-leg presented in Fig. 10.7 will affect the dc-link volt- age needed to guarantee the same input and output voltages as in the full-bridge circuit. To simplify the analysis let us assume that the dc-link capacitance is large enough to have Δ𝑣c ≃ 0. The dc-link voltage for the converter shown in Fig. 10.1 must obey the requirement of 𝑣c ≥ max{𝑣g, 𝑣l}, where 𝑣g and 𝑣l are the voltage desir- able at the input and output converter sides, respectively. Indeed, 𝑣c is obtained from the statement that the maximum value of the difference between any combinations of pole voltages will define the dc-link voltage. For the topology with shared-leg in Fig. 10.7 it yields 𝑣c ≥ max{𝑣∗ g0 − 𝑣∗ s0, 𝑣∗ l0 − 𝑣∗ s0, 𝑣∗ g0 − 𝑣∗ l0} (10.52) or 𝑣c ≥ max{𝑣∗ g, 𝑣∗ l , 𝑣∗ g − 𝑣∗ l } (10.53) If the load and grid frequencies are different, the term 𝑣∗ g − 𝑣∗ l will be bigger than either 𝑣∗ g or 𝑣∗ l and consequently will define 𝑣c. However, if both sides of the converter require the same frequency, the output voltage can be generated to minimize the effect of the term 𝑣∗ g − 𝑣∗ l . This will allow the shared-leg converter to operate with the same dc-link voltage as the full-bridge converter.
  • 324. 310 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER (a) (b) – – + + – – + + ig vg iC vC il vl eg vg Xg qg g ql l l2 0 qg ql vl Figure 10.8 Half-bridge single-phase to single-phase back-to-back converter: (a) block and (b) switch representation. 10.3.4 Half-Bridge Converter A back-to-back configuration with half-bridge at both converter sides (as in Fig. 10.8) guarantees another level of component count reduction as compared to the topology in Fig. 10.7. However, in this case there is a low frequency current flowing through the capacitors due to the dc-link midpoint connection to the load and grid, which will increase the voltage fluctuation on these elements and affect their losses. The voltage at the input and output converter sides are determined directly from the pole voltages 𝑣g0 and 𝑣l0, which are defined by equations (10.41) and (10.43), respectively. Also, the PWM equations are straightforward since there is no degree of freedom, that is, there are only two legs to process two voltages. In this case, it is not possible to use auxiliary voltage to optimize some parameters of the circuit. 10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) The search for topologies with a reduced number of components continued over a considerable period of time. This can be, in part, explained by the high cost of the power switch when compared to other elements of the converter. However, as the price of the semiconductor was going down, this tendency changed, and recently
  • 325. 10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 311 Figure 10.9 Single-phase to single-phase back-to-back converter with switches in parallel. the configurations with an increased number of components appear as an interesting option, especially in terms of reliability, efficiency, and distortions improvement. Particularly, the connection of converters in parallel can be justified if the rat- ings of the power switches available in the market cannot handle the level of current demanded for a specific application. Indeed, connecting switches in parallel is the simplest solution when the currents needed are higher than the rated currents of the switches, as shown in Fig. 10.9 for the single-phase back-to-back converter. Although the number of power switches is twice as compared to that in Fig. 10.1, the characteristics of the converter in Fig. 10.9 in terms of quality of the waveform generated are the same as in the conventional solution. As described in the following sections, connecting back-to-back converters in parallel instead of switches in parallel have the following benefits: (i) increase the current capability of the converter and (ii) improve the quality of the waveforms generated by the converter at the input and output sides. 10.4.1 Model Connecting converters in parallel allows reducing the level of current and conse- quently power processed by each converter. Another advantage is reducing outer current ripple with interleaved technique. Figure 10.10 shows a single-phase to single-phase energy conversion unit with two back-to-back converters in parallel. Such a conversion unit consists of four PBs-ac [see Fig. 10.10(a)], or in other words, the converters 1, 2, 3, and 4 [see Fig. 10.10(b)], single-phase load, four inductive filters (L1a, L1b, L3a, and L3b) at the grid side, four more inductive filters (L2a, L2b, L4a, and L4b) at the load side, and two dc-link capacitor banks. Considering converters 1 and 3 (converters at the grid side), it is possible to write the following equations: eg = z1ai1a − z1bi1b + 𝑣1 (10.54) eg = z3ai3a − z3bi3b + 𝑣3 (10.55) ig = i1a + i3a (10.56)
  • 326. 312 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER (a) (b) – + + – + – ig eg iC il vl vg L1a i1a i1b L1b L2a i2a i2b L2b q1a q1b 1a 1b 2a 2b 01 q2b q2a Converter 1 Converter 2 vl vC1 2 + – vC1 2 q1a q1b q2b q2a + – iC L3b i3b i3a L3a L4b i4b i4a L4a q3a q3b 3a 3b 4a 4b 02 q4b q4a Converter 3 Converter 4 vC2 2 + – vC2 2 q3a q3b q4b q4a Figure 10.10 Single-phase to single-phase back-to-back converter connected in parallel: (a) block and (b) switch representation. where z1a = r1a + l1ap, z1b = r1b + l1bp, z3a = r3a + l3ap, and z3b = r3b + l3bp are the impedances of the inductors L1a, L1b, L3a, and L3b, respectively; with p = d∕dt. The voltages 𝑣1 and 𝑣3 are given by 𝑣1a01 − 𝑣1b01 and 𝑣3a02 − 𝑣3b02 , respectively. For the converters at the load side, it yields: 𝑣l = −z2ai2a + z2bi2b + 𝑣2 (10.57) 𝑣l = −z4ai4a + z4bi4b + 𝑣4 (10.58) il = i2a + i4a (10.59) where z2a = r2a + l2ap, z2b = r2b + l2bp, z4a = r4a + l4ap, and z4b = r4b + l4bp are the impedances of the inductors L2a, L2b, L4a, and L4b, respectively. The voltages 𝑣2 and 𝑣4 are given by 𝑣2a01 − 𝑣1b01 and 𝑣4a02 − 𝑣4b02 , respectively.
  • 327. 10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 313 i1o i2o i3o i4o io io io 0 io Figure 10.11 Circulating current between both back-to-back converters in parallel. Since there is no transformer for isolation purpose, there exists a circulation current between both back-to-back converters as highlighted in Fig. 10.11. The fol- lowing equations can be written from the circuit in Fig. 10.10: z1ai1a − z3ai3a + z2ai2a − z4ai4a + 𝑣1a01 − 𝑣3a02 − 𝑣2a01 + 𝑣4a02 = 0 (10.60) z1ai1a − z3ai3a + z2bi2b − z4bi4b + 𝑣1a01 − 𝑣3a02 − 𝑣2b01 + 𝑣4b02 = 0 (10.61) z1bib − z3bi3b + z2ai2a − z4ai4a + 𝑣1b01 − 𝑣3b02 − 𝑣2a01 + 𝑣4a02 = 0 (10.62) z1bi1b − z3bi3b + z2bi2b − z4bi4b + 𝑣1b01 − 𝑣3b02 − 𝑣2b01 + 𝑣4b02 = 0 (10.63) Equations (10.60)–(10.63) were obtained with the following meshes (see Fig. 10.10) 1a–2a–4a–3a, 1a–2b–4b–3a, 1b–2a–3b–4a, and 1b–2b–3b–4b, respectively. An expression for the circulating voltage can be obtained by adding equations (10.60)–(10.63): 𝑣o = z1ai1a + z1bi1b − z3ai3a − z3bi3b + z2ai2a + z2bi2b − z4ai4a − z4bi4b (10.64) with 𝑣o = −𝑣1a01 − 𝑣1b01 + 𝑣3a02 + 𝑣3b02 + 𝑣2a01 + 𝑣2b01 − 𝑣4a02 − 𝑣4b02 (10.65)
  • 328. 314 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER The circulating currents in Fig. 10.11 are given by i1o = i1a + i1b (10.66) i3o = i3a + i3b (10.67) i2o = i2a + i2b (10.68) i4o = i4a + i4b (10.69) As seen in Fig. 10.11, the circulating current is in fact a single current that circulates among the converters. Such a current can be written as io = i1o = −i3o = i2o = −i4o (10.70) Then substituting equations (10.66)–(10.69) into (10.54)–(10.59), it is possi- ble to model the parallel converter as follows: eg = (z1a + z1b)i1a − z1bio + 𝑣1 (10.71) eg = (z3a + z3b)i3a + z3bio + 𝑣3 (10.72) el = −(z2a + z2b)i2a + z2bio + 𝑣2 (10.73) el = −(z4a + z4b)i4a + z4bio + 𝑣4 (10.74) 𝑣o = (z1a − z1b)i1a − (z3a − z3b)i3a − (z2a − z2b)i2a + (z4a − z4b)i4a + (z1b + z3b + z2b + z4b)io (10.75) There are two components for the circulating current, that is, high and low frequencies components. The high-frequency component is due to the difference of the deadtime for each converter and also due to asymmetry of the power switches employed in both stages. Such high-frequency components are not modeled in equation (10.75). However, the model furnished in (10.75) considers the low fre- quency component for the circulating current. For instance, any level of imbalance between Lxa and Lxb (with x = 1, 2, 3, and 4) can be identified from this model. The current io can be compensated (tracking a zero reference) with an additional controller, as described in Section 10.4.3. Also, the dynamic model obtained from equations (10.71)–(10.75) suggests that the voltage 𝑣1 is employed to control i1a, and the voltage 𝑣3 is employed to control i3a. With these two currents (i1a and i3a) under control, the grid current is also controlled [see equation (10.56)]. The voltage 𝑣o is employed to control io. Considering a balanced case where z1a = z1b = z3a = z3b = z1 and z2a = z2b = z4a = z4b = z2, the dynamic model is simplified by the following equations: eg = 2z1i1a − z1io + 𝑣1 (10.76) eg = 2z1i3a + z1io + 𝑣3 (10.77) el = −2z2i2a + z2io + 𝑣2 (10.78) el = −2z2i4a − z2io + 𝑣4 (10.79) 𝑣o = 2(z1 + z2)io (10.80)
  • 329. 10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 315 10.4.2 PWM Strategy From the model presented earlier, it is possible to write the reference voltages as a function of the reference pole voltages: 𝑣∗ 1 = 𝑣∗ 1a01 − 𝑣∗ 1b01 (10.81) 𝑣∗ 2 = 𝑣∗ 2a01 − 𝑣∗ 2b01 (10.82) 𝑣∗ 3 = 𝑣∗ 3a02 − 𝑣∗ 3b02 (10.83) 𝑣∗ 4 = 𝑣∗ 4a02 − 𝑣∗ 4b02 (10.84) 𝑣∗ o = −𝑣∗ 1a01 − 𝑣∗ 1b01 + 𝑣∗ 3a02 + 𝑣∗ 3b02 + 𝑣∗ 2a01 + 𝑣∗ 2b01 − 𝑣∗ 4a02 − 𝑣∗ 4b02 (10.85) There are eight pole voltages and just five variables to control, two variables associated to the grid current (𝑣∗ 1 and 𝑣∗ 3 ), one variable to deal with the circulating current (𝑣∗ o), and finally two more variables to handle load voltage control (𝑣∗ 2 and 𝑣∗ 4 ). There exist, therefore, three degrees of freedom, that is, three auxiliary variables. Those auxiliary variables can be defined as follows: 𝑣∗ x = 𝑣∗ 1a01 + 𝑣∗ 1b01 2 (10.86) 𝑣∗ y = 𝑣∗ 2a01 + 𝑣∗ 2b01 2 (10.87) 𝑣∗ z = 𝑣∗ 4a02 + 𝑣∗ 4b02 2 (10.88) From equations (10.86)–(10.88) it is possible to define the reference pole volt- ages as follows: 𝑣∗ 1a01 = 𝑣∗ 1 2 + 𝑣∗ x (10.89) 𝑣∗ 1b01 = − 𝑣∗ 1 2 + 𝑣∗ x (10.90) 𝑣∗ 3a02 = 𝑣∗ 3 2 + 𝑣∗ o 2 − 𝑣∗ y + 𝑣∗ z + 𝑣∗ x (10.91) 𝑣∗ 3b02 = − 𝑣∗ 3 2 + 𝑣∗ o 2 − 𝑣∗ y + 𝑣∗ z + 𝑣∗ x (10.92) 𝑣∗ 2a01 = 𝑣∗ 2 2 + 𝑣∗ y (10.93) 𝑣∗ 2b01 = − 𝑣∗ 2 2 + 𝑣∗ y (10.94) 𝑣∗ 4a02 = 𝑣∗ 4 2 + 𝑣∗ z (10.95) 𝑣∗ 4b02 = − 𝑣∗ 4 2 + 𝑣∗ z (10.96) The reference pole voltages are defined as a function of the desirable voltages (defined by the controllers) 𝑣∗ 1 , 𝑣∗ 2 , 𝑣∗ 3 , and 𝑣∗ 4 as well as the auxiliary voltages 𝑣∗ x , 𝑣∗ y ,
  • 330. 316 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER and 𝑣∗ z . Note that the auxiliary voltages can be defined independently as follows, if equations (10.100)–(10.105) are satisfied: 𝑣∗ x = 𝜇x𝑣∗ xMAX + (1 − 𝜇x)𝑣∗ xMIN (10.97) 𝑣∗ y = 𝜇y𝑣∗ yMAX + (1 − 𝜇y)𝑣∗ yMIN (10.98) 𝑣∗ z = 𝜇z𝑣∗ zMAX + (1 − 𝜇z)𝑣∗ zMIN (10.99) where 𝑣∗ xMAX = 𝑣∗ c1 2 − max|V∗ x | (10.100) 𝑣∗ xMIN = − 𝑣∗ c1 2 − min|V∗ x | (10.101) 𝑣∗ yMAX = 𝑣∗ c1 2 − max|V∗ y | (10.102) 𝑣∗ yMIN = − 𝑣∗ c1 2 − min|V∗ y | (10.103) 𝑣∗ zMAX = 𝑣∗ c2 2 − max|V∗ z | (10.104) 𝑣∗ zMIN = − 𝑣∗ c2 2 − min|V∗ z | (10.105) with V∗ x = {𝑣∗ 1 2 , −𝑣∗ 1 2 , 𝑣∗ 3 2 + 𝑣∗ o 2 − 𝑣∗ y + 𝑣∗ z , − 𝑣∗ 3 2 + 𝑣∗ o 2 − 𝑣∗ y + 𝑣∗ z } , V∗ y = {𝑣∗ 2 2 , − 𝑣∗ 2 2 } and V∗ z = {𝑣∗ 4 2 , − 𝑣∗ 4 2 } ; and 0 ≤ 𝜇x ≤ 1, 0 ≤ 𝜇y ≤ 1, and 0 ≤ 𝜇z ≤ 1. The gating signals of the power switches can be obtained by either comparing the reference pole voltages (10.89)–(10.96) with carrier waveforms or in a digital way by programming timers. Since there are two converters connected in parallel, an interleaved technique can be employed to reduce the current ripple. Figure 10.12 shows the carrier signals (𝑣∗ t1 and 𝑣∗ t2 ) for the interleaved technique. In this case, 𝑣∗ t1 is employed for converters 1 and 2, while 𝑣∗ t2 is employed for converters 3 and 4. Figure 10.13 shows the output of the parallel topology highlighting the influence of the interleaved technique. Notice that since the ripple of i2a is shifted by 180 electri- cal degrees (considering the switching frequency) from the ripple of i4a, the output current will have a smoother ripple since il = i2a + i4a. 10.4.3 Control Strategy The control block diagram for the parallel back-to-back converter is given in Fig. 10.14. The dc-link voltages are regulated by the controllers Rc1 and Rc3. The output of these controllers defines the amplitude of the currents in converters 1 and 3, respectively. The block Gi creates sinusoidal currents (i∗ 1a and i∗ 3a ) in phase with the grid voltage; this is a PLL-based block. The controllers Ri1 and Ri3 regulate the currents i1a and i3a, and the output of these controllers define the voltages (𝑣∗ 1 and 𝑣∗ 3 ) employed in the PWM technique described previously. The circulating current is
  • 331. 10.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 317 vt1 * vt2 * t Figure 10.12 Carrier signals for the interleaved technique applied to the parallel converters. i2a i4a i2a 2a L2a i4a 4a L4a il il il Figure 10.13 Output of the parallel back-to-back converter with interleaved technique. regulated by using the controller Ro. The block k𝑣 can be employed to compensate imbalance among the inductors; for a balanced case k𝑣 = 0.5. Exercise 10.6 Assuming well-designed controllers for the parallel topology presented in Fig. 10.10, that is, power factor equal to one, circulating current equal to zero, and dc-link capacitor voltages under control, specify the power switches employed in this configuration in terms of current and voltage with: (i) the active power of the load is Pl = 1700W with cos(Φl) = 0.85, load voltage with 120Vrms – 60 Hz, (ii) dc-link voltage fluctuation equal to zero, and (iii) a drop voltage due to the inductors Lxa and Lxb (x = 1, 2, 3, 4) equal to 5Vrms on each inductor.
  • 332. 318 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER – – + – + – – – – vC1 * vC1 – + vl – + vC2 v1 * v3 * v2 * v4 * vo * I1 * i1a * io i3a i1a q1a L1a L1b L3b L3a L2a L2b L4b L4a q3a q3b q1b q2a Conv. 2 Conv. 3 Conv. 1 Conv. 4 q4a q4b q2b i1a i1b i3a * io * vl * I3 * vC2 * vC1 eg vC2 Rc1 Gi Ri1 Ri3 Ro1 PWM kv (1 – kv) Rc3 Σ Σ Σ Σ Σ Σ Figure 10.14 Control block diagram of the parallel single-phase back-to-back converter. 10.5 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN SERIES) Connecting single-phase to single-phase converters in parallel brings up interest- ing characteristics such as reduction of the current processed by each power switch and interleaved PWM, which allows current ripple reduction. Following a similar approach, it is also possible to connect single-phase to single-phase back-to-back converters in series as seen in Fig. 10.15. Figure 10.15(a) shows the power block representation while Fig. 10.15(b) depicts the representation with switches. In this case, it is necessary for half of the dc-link voltage to have the same voltage capability of the conventional single back-to-back converter. Also the load and grid will give the back-to-back converters an H-bridge cascade configuration, that is, as a multi- level converter (see Chapter 5). The only difference between the input/output of the converter in Fig. 10.15 and the cascade topology in Chapter 5 is a circulating current between both back-to-back units since there is no isolation. Such a circulating current can be determined from the model, as described in the later. It is worth mentioning that the majority of the topologies presented in Chapter 5 have isolated dc sources. The following equations can be derived from the converter in Fig. 10.15(b). eg = z1ig + 𝑣1ab + z2i′ g + 𝑣2ab (10.106) 𝑣l = 𝑣1cd + 𝑣2cd (10.107)
  • 333. 10.5 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN SERIES) 319 (a) (b) + – + – ig io eg vl vg L1 q1a q1b q1c q1d q1a q1b q1c q1d 1a 01 1b 1c 1d Converter 1 Converter 2 vC1 2 + – + – vC1 2 + – L2 q2a q2a q2b q2c q2d q2b q2c q2d 2a 02 2b 2c 2d vC2 2 + – vC2 2 ig ′ il ′ il vl Figure 10.15 Series connection of the single-phase to single-phase back-to-back converters. where z1 = r1 + pl1, z2 = r2 + pl2 with p = d∕dt; 𝑣1ab = 𝑣1a01 − 𝑣1b01 , 𝑣2ab = 𝑣2a02 − 𝑣2b02 , 𝑣1cd = 𝑣1c01 − 𝑣1d01 , and 𝑣2cd = 𝑣2c02 − 𝑣2d02 . Since this is a transformerless configuration, there are circulating meshes, which can be modeled by equations (10.108) and (10.109): eg = z1ig + 𝑣1ac + 𝑣l − 𝑣2bd (10.108) 0 = 𝑣1bd − 𝑣2ac − z2i′ g (10.109)
  • 334. 320 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER Adding (10.108) and (10.109), it is possible to define the circulating voltage as follows: 𝑣o = eg − z1ig + z2i′ g = 𝑣1ac + 𝑣1bd − 𝑣2ac − 𝑣2bd + 𝑣l (10.110) Ideally ig = i′ g and il = −i′ l . However, due to the circulating current we have i′ g = ig − io (10.111) i′ l = −il + io (10.112) The dynamic model of the converter can be rewritten from (10.106) as follows: eg = z1ig + z2ig − z2io + 𝑣g (10.113) where 𝑣g = 𝑣1ab + 𝑣2ab. From equation (10.110), the model for the circulating voltage can be written in terms of io as 𝑣o = eg + (z2 − z1)ig − z2io (10.114) For a balanced case with z1 = z2 we have eg = 2z1ig − z1io + 𝑣g (10.115) 𝑣o = eg − z2io (10.116) The PWM approach described for the series back-to-back converter can be adapted from the solution employed in the parallel converter presented in the previous section. – – – – – + – + Ig * vg * vg * vo * vl * vl – +vC2 – +vC1 io * io v1ab * v2ab * v1cd * v2cd * ig * vC1+vC2 vC1 * * vC1+vC2 * vC1 eg ig Σ Σ Σ Σ Rc Rc1 Ro ½ ½ Gi Rg k1 L1 L2 k1 (1–k1) PWM Conv. 1 (Rectif.) Conv. 1 (Invert.) Conv. 2 (Invert.) Conv. 2 (Rectif.) q1a q2a q1b q2b q1c q2c q1d q2d Figure 10.16 Control block diagram of the single back-to-back converter series connected.
  • 335. REFERENCES 321 The control strategy is shown in Fig. 10.16. Since the current ig affects both dc-link voltages 𝑣C1 and 𝑣C2, the controller Rc has been employed to regulate (𝑣C1 + 𝑣C2). The output of this controller defines I∗ g , the instantaneous sinusoidal current i∗ g synchronized with the grid voltage (in order to obtain high power factor) is deter- mined by the PLL-based block Gi. The inner control loop should be designed to guarantee grid current control; the output of the block Rg defines 𝑣∗ g. It is impor- tant to highlight that 𝑣g is the voltage generated by both rectifiers in converters 1 and 2 to guarantee grid current control [see equation (10.115)]. In fact, although 𝑣g is viewed from the grid as only one-component voltage, it is constituted by two terms, that is, 𝑣g = 𝑣1ab + 𝑣2ab. The term k1 determines the level of voltage that should be processed by the rectifiers of converters 1 and 2 to keep the voltage 𝑣C1 under con- trol. Hence, the controllers Rc and Rc1 are employed to control the dc-link voltages (𝑣C1 and 𝑣C2), while the controller Rg along with the block Gi are used to control grid power factor. The circulating current must track a zero reference (i∗ g = 0) with the controller Ro, and the output voltage 𝑣∗ l defines the voltages 𝑣∗ 1cd and 𝑣∗ 2cd . Although the load voltage control in Fig. 10.16 is done in open-loop operation, a closed-loop can be easily obtained from this control block diagram. Exercise 10.7 Repeat Exercise 10.6 with the same conditions for the series topology in Fig. 10.15. 10.6 SUMMARY This chapter presented several circuits able to implement a single-phase back-to-back converter. A comprehensive analysis for the full-bridge topology was presented in Section 10.2. The following aspects were considered for this topology: (i) model, (ii) PWM, (iii) control, (iv) power analysis, and (v) dc-link capacitor voltage, and (vi) capacitor bank design. Section 10.3 dealt with topologies with reduced number of power switches. Two strategies were considered: utilization of shared-leg and dc-link capacitor midpoint connections as valid ways to reduce the number of switches. On the other hand, the topologies with increased number semiconductor devices were presented in Sections 10.4 and 10.5, with configurations in parallel and series, respec- tively. The model, PWM and control approaches highlighting the presence of the circulating current were also presented for both topologies. More information can be found in references from 1 to 35. REFERENCES [1] Asiminoaei L, Aeloiza E, Enjeti PN, Blaabjerg F, Danfoss G. Shunt active-power-filter topology based on parallel interleaved inverters. IEEE Trans Ind Electron 2008;55(3):1175–1189.
  • 336. 322 CHAPTER 10 SINGLE-PHASE TO SINGLE-PHASE BACK-TO-BACK CONVERTER [2] Ramos R, Biel D, Fossas E, Guinjoan F. Interleaving quasisliding-mode control of parallel-connected buck-based inverters. IEEE Trans Ind Electron 2008;55(11):3865–3873. [3] Chen Y-T, Jiang R-S, Liang R-H. Analysis and design of zero-voltage-switching parallel interleaved current-doubler converters with coupled output inductors. IET Power Electron 2012;5(4):467–476. [4] Chunkag V, Kamnarn U. Parallelling three-phase ac to dc converter using cuk rectifier modules based on power balance control technique. IET Power Electron 2010;3(4):511–524. DOI: 10.1049/iet-pel.2008.0209. [5] Ye Z, Boroyevich D, Choi J-Y, Lee FC. Control of circulating current in two parallel three-phase boost rectifiers. IEEE Trans Power Electron 2002;17(5):609–615. [6] Vilathgamuwa DM, Gajanayake CJ, Loh PC. Modulation and control of three-phase paral- leled z-source inverters for distributed generation applications. IEEE Trans Energy Convers 2009;24(1):173–183. [7] Pan C-T, Liao Y-H. Modeling and control of circulating currents for parallel three-phase boost rec- tifiers with different load sharing. IEEE Trans Ind Electron 2008;55(7):2776–2785. [8] Wang J. Design a parallel buck derived converter system using the primary current droop sharing control. IET Power Electron 2011;4(5):491–502. DOI: 10.1049/iet-pel.2010.0042. [9] Singh RP, Khambadkone AM. Current sharing and sensing in n-paralleled converters using single current sensor. IEEE Trans Ind Appl 2010;46(3):1212–1219. [10] Cuzner RM, Nowak DJ, Bendre A, Oriti G, Julian AL. Mitigating circulating common-mode currents between parallel soft-switched drive systems. IEEE Trans Ind Appl 2007;43(5):1284–1294. [11] Li R, Xu D. Parallel operation of full power converters in permanent-magnet direct-drive wind power generation system. IEEE Trans Ind Electron 2013;60(4):1619–1629. [12] Ko Y-J, Lee K-B, Lee D-C, Kim J-M. Fault diagnosis of three-parallel voltage-source converter for a high-power wind turbine. IET Power Electron 2012;5(7):1058–1067. [13] Hou C-C. A multicarrier pwm for parallel three-phase active front-end converters. IEEE Trans Power Electron 2013;28(6):2753–2759. [14] Xu Z, Li R, Zhu H, Xu D, Zhang C. Control of parallel multiple converters for direct-drive permanent-magnet wind power generation systems. IEEE Trans on Power Electron 2012;27(3):1259– 1270. DOI: 10.1109/TPEL.2011.2165224. [15] Zhang D, Wang F, Burgos R, Lai R, Boroyevich D. Interleaving impact on ac passive components of paralleled three-phase voltage-source converters. IEEE Trans Ind Appl 2010;46(3):1042–1054. [16] Itkonen T, Luukko J, Sankala A, Laakkonen T, Pollanen R. Modeling and analysis of the dead-time effects in parallel pwm two-level three-phase voltage-source inverters. IEEE Trans Power Electron 2009;24(11):2446–2455. [17] Genc N, Iskender I. DSP-based current sharing of average current controlled two-cell interleaved boost power factor correction converter. IET Power Electronics 2011;4(9):1015–1022. DOI: 10.1049/iet-pel.2010.0349. [18] Chen Y-T, Jiang R-S, Liang R-H. Analysis and design of zero-voltage-switching parallel interleaved current-doubler converters with coupled output inductors. IET Power Electronics 2012;5(4):467–476. DOI: 10.1049/iet-pel.2010.0163. [19] Park HW, Park SJ, Park JG, Kim CU. A novel high-performance voltage regulator for single-phase AC sources. IEEE Trans Ind Electron 2001;48(3):554–562. [20] Choi J-H, Kwon J-MB, Jung J-H, Kwon B-H. Highperformance online UPS using three-leg-type converter. IEEE Trans Ind Electron 2005;52(3):889–897. [21] Rocha N, Jacobina CB, dos Santos EJ, de Cavalcanti RMB. Parallel connection of two single-phase ac-dc-ac three-leg converter with interleaved technique. Proc. of IEEE Ind Electron, IECON 2012; p 639–644. [22] Holtz J. Pulsewidth modulation for electronic power conversion. Proc IEEE 1994;82(8):1194–1214. [23] Ojo O, Kshirsagar PM. Concise modulation strategies for four-leg voltage source inverters. IEEE Trans Power Electron 2004;19(1):46–53. [24] Jacobina CB, Lima AMN, da Silva ERC, Alves RNC, Seixas PF. Digital scalar pulse-width mod- ulation: a simple approach to introduce non-sinusoidal modulating waveforms. IEEE Trans Power Electron 2001;16(3):351–359. [25] Panda AK, Suresh Y. Research on cascade multilevel inverter with single dc source by using three-phase transformers. Int J Electr Power Energy Syst 2012;40(1):9–20.
  • 337. REFERENCES 323 [26] Malinowski M, Kazmierkowski MP, Trzynadlowski AM. A comparative study of control techniques for PWM rectifiers in AC adjustable speed drives. IEEE Trans Power Electron 2003;18(6):1390–1396. [27] Filho RMS, Seixas PF, Cortizo PC, Torres LAB, Souza AF. Comparison of three single-phase pll algorithms for ups applications. IEEE Trans Ind Electron 2008;55(8):2923–2932. [28] Verdelho P, Marques GD. Four-wire current-regulated PWM voltage converter. IEEE Trans Ind Elec- tron 1998;45(5):761–770. [29] Abu-Rub H, Guzinski J, Krzeminski Z, Toliyat H. Predictive current control of voltage-source invert- ers. IEEE Trans Ind Electron 2004;51(3):585–593. [30] Dong G, Ojo O. Current regulation in four-leg voltage-source converters. IEEE Trans Ind Electron 2007;54(4):2095–2105. [31] Jacobina CB, de Correa MB, Oliveira TM, Lima AMN, da Silva ERC. Current control of unbalanced electrical systems. IEEE Trans Ind Electron 2001;48(3):517–525. [32] Babaeia E, Hosseinia SH, Gharehpetianb GB. Reduction of the and low order harmonics with sym- metrical output current for single-phase ac/ac matrix converters. Int J Electr Power Energy Syst 2010;32(3):225–235. [33] Kieferndorf F, Forster M, Lipo T. Reduction of dc-bus capacitor ripple current with PAM/PWM converter. IEEE Trans Ind Applic 2004;40(2):607–614. [34] Kolar J, Round S. Analytical calculation of the rms current stress on the dc-link capac- itor of voltage-PWM converter systems. Electric Power Applications, IEE Proceedings 2006;153(4):535–543. [35] Cavalcanti M, da Silva E, Boroyevich D, Dong W, Jacobina C. A feasible loss model for igbt in soft-switching inverters. Proc IEEE PESC 2003;3:1845–1850.
  • 338. CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS 11.1 INTRODUCTION A three-phase back-to-back converter is an important electrical apparatus with a wide range of applications on systems demanding a processed three-phase voltage. Although the operation principle is similar to the single-phase to single-phase back-to-back converter presented in the previous chapter, the characteristics of the three-phase version are quite different, especially due to the nonexistent pulsating power on the dc-link capacitor voltages. Note that the power at the input (grid-side) and output (load-side) of the converter are constant for a bal- anced case. The concept of power blocks is considered to provide a broader perception of how the topologies presented in the technical literature have been conceived. Following the introduction, this chapter is organized in six sections. Section11.2 deals with the full-bridge ac–dc–ac converter presenting its model, pulse width modulation (PWM), and control strategies. Topologies with component count reduction are presented in Section 11.3, while Sections 11.4 and 11.5 describe the model, PWM, and control for configurations with an increased number of semi- conductor devices. A similar approach as in the previous chapter is employed for the three-phase back-to-back converters, that is, shared-leg and dc-link capacitor midpoint connections for reducing the number of semiconductor devices, while con- necting back-to-back converters in parallel and series are considered in Sections 11.4 and 11.5, respectively. Section 11.6 presents other converters, especially for single-phase to three-phase conversion and for a six-phase motor drive system. Finally, Section 11.7 summarizes the chapter. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. 324
  • 339. 11.2 FULL-BRIDGE CONVERTER 325 11.2 FULL-BRIDGE CONVERTER 11.2.1 Model Since the control goals are active power factor and regulation of the dc-link capac- itor voltage, the equations derived in this section highlight both grid current and capacitor voltage variables. Although an open loop operation is assumed for the out- put of the converter, a closed loop control can be easily implemented for the output converter side. The three-phase back-to-back converter can be obtained directly by using two PBs back-to-back connected per phase as presented in Fig. 11.1(a). The representation of the three-phase back-to-back converter using switches is furnished in Fig. 11.1(b). The conversion system is composed of a three-phase utility grid, input inductors (with reactance equal to Xg1, Xg2, and Xg3), capacitor bank at the dc-link with two capacitors (each one with capacitance equal to C), controlled rectifier, inverter, and a three-phase load. The rectifier circuit comprises the switches qg1, qg2, and qg3 and their complementary switches: qg1, qg2, and qg3. Similarly, the inverter comprises the switches ql1, ql2, and ql3 and their complementary switches ql1 , ql2 , and ql3 . Binary variables are employed to define the conduction states of the switches. The model of the back-to-back converter can be obtained from Fig. 11.1(b) as follows: 𝑣g1 = 𝑣g10 − 𝑣ng0 (11.1) (a) (b) + – + – + – + – + – – + ig1 ig2 ig3 iC vC il1 il2 il3 vl3 vl2 vl1 eg1 eg2 eg3 vg3 vg2 vg1 Xg1 Xg2 Xg3 qg1 qg2 qg3 g1 ng g2 g3 ql2 ql3 nl ql1 ql2 ql1 l1 l2 l3 0 2 qg2 qg3 qg1 ql3 vC vl1 – +vl2 – +vl3 2 Figure 11.1 Three-phase to three-phase back-to-back converter: (a) block and (b) switch representation.
  • 340. 326 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS 𝑣g2 = 𝑣g20 − 𝑣ng0 (11.2) 𝑣g3 = 𝑣g30 − 𝑣ng0 (11.3) 𝑣l1 = 𝑣l10 − 𝑣nl0 (11.4) 𝑣l2 = 𝑣l20 − 𝑣nl0 (11.5) 𝑣l3 = 𝑣l30 − 𝑣nl0 (11.6) where the pole voltages can be written as a function of the states of the switches, as below: 𝑣g10 = (2qg1 − 1) 𝑣C 2 (11.7) 𝑣g20 = (2qg2 − 1) 𝑣C 2 (11.8) 𝑣g30 = (2qg3 − 1) 𝑣C 2 (11.9) 𝑣l10 = (2ql1 − 1) 𝑣C 2 (11.10) 𝑣l20 = (2ql2 − 1) 𝑣C 2 (11.11) 𝑣l30 = (2ql3 − 1) 𝑣C 2 (11.12) with 𝑣ng0 = 1 3 (𝑣g10 + 𝑣g20 + 𝑣g30) and 𝑣nl0 = 1 3 (𝑣l10 + 𝑣l20 + 𝑣l30) for a balanced case. Equations (11.13)–(11.15) furnish the dynamic model for the variables at the grid side: 𝑣g1 = eg1 − rgig1 − lg dig1 dt (11.13) 𝑣g2 = eg2 − rgig2 − lg dig2 dt (11.14) 𝑣g3 = eg3 − rgig3 − lg dig3 dt (11.15) where rg and lg represent the resistances and inductances of the input inductor. The capacitor voltage can be obtained as 𝑣c = 1 C∫ (qg1ig1 + qg2ig2 + qg3ig3 − ql1il1 − ql2il2 − ql3il3)dt (11.16) with the interval of integration equal to the switching period.
  • 341. 11.2 FULL-BRIDGE CONVERTER 327 11.2.2 PWM Strategy The optimized PWM strategy presented in Chapter 8 can be employed for the full-bridge configuration presented in Fig. 11.1 to improve either total harmonic distortion (THD) or efficiency at both sides. If the desired input and output voltages are given respectively by 𝑣∗ g1 , 𝑣∗ g2 , 𝑣∗ g3 and 𝑣∗ l1 , 𝑣∗ l2 , 𝑣∗ l3 , the reference pole voltages can be written as follows: 𝑣∗ g10 = 𝑣∗ g1 + 𝑣∗ gh (11.17) 𝑣∗ g20 = 𝑣∗ g2 + 𝑣∗ gh (11.18) 𝑣∗ g30 = 𝑣∗ g3 + 𝑣∗ gh (11.19) 𝑣∗ l10 = 𝑣∗ l1 + 𝑣∗ lh (11.20) 𝑣∗ l20 = 𝑣∗ l2 + 𝑣∗ lh (11.21) 𝑣∗ l30 = 𝑣∗ l3 + 𝑣∗ lh (11.22) The auxiliary voltages 𝑣∗ gh and 𝑣∗ lh are given respectively by 𝑣∗ gh = 𝑣C ( 𝜇g − 1 2 ) + (𝜇g − 1)V∗ gmax − 𝜇gV∗ gmin (11.23) 𝑣∗ lh = 𝑣C ( 𝜇l − 1 2 ) + (𝜇l − 1)V∗ lmax − 𝜇lV∗ lmin (11.24) where Vgmax = MAX{𝑣∗ g1 , 𝑣∗ g2 , 𝑣∗ g3 }, Vgmin = MIN{𝑣∗ g1 , 𝑣∗ g2 , 𝑣∗ g3 } and Vlmax = MAX{𝑣∗ l1 , 𝑣∗ l2 , 𝑣∗ l3 }, Vlmin = MIN{𝑣∗ l1 , 𝑣∗ l2 , 𝑣∗ l3 }; 𝜇g and 𝜇l are the distribution factor and determine how the free-wheeling time can be distributed throughout the switch- ing period. Note that, since the grid and load sides of the converter are decoupled by the dc-link capacitor bank, 𝑣∗ gh and 𝑣∗ lh are independent of each other. Once the reference pole voltages have been defined, pulse widths 𝜏g1, 𝜏g2, 𝜏g3, 𝜏l1, 𝜏l2, and 𝜏l3 can be calculated from equations (11.25)–(11.30), as below: 𝜏g1 = ( 𝑣∗ g10 𝑣C + 1 2 ) Ts (11.25) 𝜏g2 = ( 𝑣∗ g20 𝑣C + 1 2 ) Ts (11.26) 𝜏g3 = ( 𝑣∗ g30 𝑣C + 1 2 ) Ts (11.27) 𝜏l1 = ( 𝑣∗ l10 𝑣C + 1 2 ) Ts (11.28) 𝜏l2 = ( 𝑣∗ l20 𝑣C + 1 2 ) Ts (11.29)
  • 342. 328 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS 𝜏l3 = ( 𝑣∗ l30 𝑣C + 1 2 ) Ts (11.30) where Ts is the switching period. The state of the switches qg1, qg2, qg3, ql1, ql2, and ql3 can be defined directly from the previous equations by programming timers in a digital implementation of the PWM. Note that the reference voltages 𝑣∗ g1 , 𝑣∗ g2 , and 𝑣∗ g3 employed in (11.25)–(11.27) are obtained as the output of controllers (as presented in Section 11.2.3.) Although the voltages 𝑣∗ l1 , 𝑣∗ l2 , and 𝑣∗ l3 can be defined with either open-loop or closed-loop, the open loop operation is considered in this section. 11.2.3 Control Approach Figure 11.2 presents the control block diagram for the three-phase back-to-back con- verter. While the output voltage is controlled by open-loop operation, the dc-link capacitor voltage and the grid power factor are regulated by the controllers RC and Ri1, Ri2, Ri3, respectively. Since the dynamic of the capacitor voltage is slow as com- pared to the grid current, a cascade control approach has been employed to guarantee regulation of both variables. The dc-link voltage 𝑣C is adjusted to its reference value 𝑣∗ C by using the con- troller RC, which could be implemented with a standard PI controller. This controller – + – – – + + + Ig * vgh * vl10 * vg30 * vg20 * vg10 * vl20 * vl1 * vl2 * vl3 * vlh * vl30 * ig1 * vg1 * vg2 * vg3 * ig1 ig2 ig3 ig2 * ig3 * * vc vc eg1 Σ Σ Σ Σ Σ Σ Σ Σ Σ Σ μl μg Rc Ri1 Ri2 Ri3 PWM Load Rectifier/Inverter Voltage sensor Voltage sensor Current sensor Grid Ge-ig Eq.(11.23) Eq.(11.24) qg1 qg2 qg3 ql1 ql2 ql3 Figure 11.2 Control strategy for the three-phase back-to-back converter.
  • 343. 11.2 FULL-BRIDGE CONVERTER 329 provides the amplitude of the reference grid current I∗ g . To maintain the power fac- tor close to one with a sinusoidal grid current, the instantaneous reference currents i∗ g1 , i∗ g2 and i∗ g3 must be synchronized with the input voltage eg1, eg2, and eg3, respec- tively. Such a synchronization scheme can be obtained through a phase locked loop (PLL)-based control. The block Ge − ig is responsible for generating the reference sinusoidal grid current in phase with the grid voltage, that is, i∗ g1 = I∗ g sin(𝜔gt + Φg), i∗ g2 = I∗ g sin(𝜔gt + Φg + 120∘), i∗ g3 = I∗ g sin(𝜔gt + Φg + 240∘). The current controller loop must deal with sinusoidal waveforms, which means that a conventional PI con- troller will not guarantee null error in steady-state operation – a modified PI controller can be employed instead. The PWM block shown in Fig. 11.2 can be implemented either from equations (11.17)–(11.22) or by comparing these reference pole voltages with high-frequency carrier signals. Application (Universal Active Power Filter) Also known as Universal Power Quality Conditioner (UPQC), the Universal Active power filter uses the back-to-back schematic circuit to improve the quality of both voltage and current in a three-phase electrical system. The electrical energy gen- erators in power plants furnish voltages nearly sinusoidal. However, the quality of this voltage can be deteriorated due to steady-state and/or transient phenomena at a given point of the electrical system. Examples of these phenomena are nonlinear loads and faults in part of the power circuit resulting in current distortion and voltage sags/swells. The universal active power filter can be employed to compensate dynam- ically such disturbances for both steady-state and transient problems, with the ability to deal with the correction of grid voltage disturbance and fluctuation. As presented in the figure below, one side (grid side) of the back-to-back converter is employed to compensate the voltage disturbance by adding voltage through a three-phase trans- former, while the other side is used to inject the current at the load side to guarantee sinusoidal grid current with power factor close to one. The universal active power filter is especially recommended to protect critical loads at the point of installation as well as compensate the grid from current harmonics generated at the load side. The voltage 𝑣g is used to compensate any disturbance on eg, since 𝑣l = eg + 𝑣ngnl − 𝑣g. The current if has been employed to guarantee a sinusoidal grid current in phase with the grid voltage, since ig = il + if . Although several techniques are presented in the literature for active power filter control, the main structure is based on two control loops: a dc-link voltage outer loop and a current inner loop. The outer loop regulates the dc-link voltage while the inner loop tracks the reference current necessary to compensate harmonics and/or fundamental reactive power. Two basic methods are considered in the litera- ture to generate current reference signal: direct method and indirect method. In the direct method the disturbance to be compensated is sensed directly from the load and employed as the filter reference current signal. In the indirect method the disturbance to be compensated is sensed on the grid and controlled to a minimum value through a closed-loop. The last method has reduced cost since it uses less number of sensors, while the first one is more accurate.
  • 344. 330 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS + – + – – + eg vg ig if il nl vl ng 11.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 11.3.1 Model Another three-phase to three-phase ac–dc–ac power converter is obtained by remov- ing one of the PBs-ac as shown in Fig. 11.3(a). Figure 11.3(b) shows the same con- figuration with switch representation. Note that the leg constituted by the switches qs − qs is shared between the input and output sides of the converter, and conse- quently such a leg will handle a current that is a sum of input and output currents (il3 − ig3). Also, the shared-leg will play an important role for the voltage capability of the converter. Unlike the previous back-to-back converter where both input and output converter sides are decoupled, the shared-leg topology in Fig. 11.3 presents coupling due to the leg qs − qs. The following equations can be derived from Fig. 11.3(b) for both input and output converter sides: 𝑣g1 = 𝑣g10 − 𝑣ng0 (11.31) 𝑣g2 = 𝑣g20 − 𝑣ng0 (11.32) 𝑣g3 = 𝑣s0 − 𝑣ng0 (11.33) 𝑣l1 = 𝑣l10 − 𝑣nl0 (11.34) 𝑣l2 = 𝑣l20 − 𝑣nl0 (11.35) 𝑣l3 = 𝑣s0 − 𝑣nl0 (11.36)
  • 345. 11.3 TOPOLOGY WITH COMPONENT COUNT REDUCTION 331 (a) (b) + – + – + – + – – + ig1 ig2 ig3 iC vC il1 il2 il3 vl3 vl2 vl1 eg1 eg2 eg3 vg3 vg2 vg1 Xg1 Xg2 Xg3 qg1 qg2 qs g1 ng g2 s ql2 nl ql1 ql2 ql1 l1 l2 0 2 qg2 qs qg1 + – vC 2 vl1 – +vl2 – +vl3 Figure 11.3 Shared-leg three-phase back-to-back converter: (a) block and (b) switch representation. The pole voltages can be written as in equations (11.7)–(11.12) with 𝑣ng0 = 1 3 (𝑣g10 + 𝑣g20 + 𝑣s0) and 𝑣nl0 = 1 3 (𝑣l10 + 𝑣l20 + 𝑣s0). Also, equations (11.13)–(11.15) are still valid for modeling the input converter side. However, the capacitor voltage for the shared-leg topology in Fig. 11.3 is given by 𝑣c = 1 C∫ [qg1ig1 + qg2ig2 + qs(ig3 − il3) − ql1il1 − ql2il2]dt (37) with the interval of integration equal to the switching period. 11.3.2 PWM Strategies If the desired input and output voltages are given respectively by 𝑣∗ g1 , 𝑣∗ g2 , 𝑣∗ g3 and 𝑣∗ l1 , 𝑣∗ l2 , 𝑣∗ l3 , one option for the reference pole voltage is given below: 𝑣∗ g10 = 𝑣∗ g1 − 𝑣∗ g3 + 𝑣∗ h (11.38) 𝑣∗ g20 = 𝑣∗ g2 − 𝑣∗ g3 + 𝑣∗ h (11.39) 𝑣∗ s0 = 𝑣∗ h (11.40) 𝑣∗ l10 = 𝑣∗ l1 − 𝑣∗ l3 + 𝑣∗ h (11.41) 𝑣∗ l20 = 𝑣∗ l2 − 𝑣∗ l3 + 𝑣∗ h (11.42) Due to the shared-leg, which connects both input and output sides of the con- verter, there is only one voltage 𝑣∗ h that optimizes both converter sides. The 𝑣∗ h can be
  • 346. 332 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS defined as follows: 𝑣∗ h = 𝑣C ( 𝜇 − 1 2 ) + (𝜇 − 1)V∗ max − 𝜇V∗ min (11.43) where Vmax = MAX{𝑣∗ g1 − 𝑣∗ g3 , 𝑣∗ g2 − 𝑣∗ g3 , 0, 𝑣∗ l1 − 𝑣∗ l3 , 𝑣∗ l2 − 𝑣∗ l3 } and Vmin = MIN{𝑣∗ g1 − 𝑣∗ g3 , 𝑣∗ g2 − 𝑣∗ g3 , 0, 𝑣∗ l1 − 𝑣∗ l3 , 𝑣∗ l2 − 𝑣∗ l3 }. Once the reference pole voltages have been defined, pulse widths can be obtained as in equations (11.25)–(11.30). In this case, instead of defining 𝜏g3 and 𝜏l3, the pulse width 𝜏s is defined by (𝑣∗ s ∕𝑣C + 1∕2)Ts. 11.3.3 dc-link Voltage Requirement To guarantee the same input and output voltages as in the full-bridge converter, the minimum dc-link voltage for the shared leg topology must obey the following require- ment: 𝑣c ≥ max{𝑣∗ gx0 − 𝑣∗ gy0, 𝑣∗ gx0 − 𝑣∗ s0, 𝑣∗ lx0 − 𝑣∗ ly0, 𝑣∗ lx0 − 𝑣∗ s0, 𝑣∗ gx0 − 𝑣∗ ly0} (44) with x = 1, 2; y = 1, 2; and x ≠ y. If the load frequency is different from the grid frequency, the term 𝑣∗ gx0 − 𝑣∗ ly0 is dominant and defines 𝑣c. However, if both sides of the converter require the same frequency, the output voltage can be generated, synchronized to the input voltage to minimize the effect of the term 𝑣∗ gx0 − 𝑣∗ ly0 . This will allow the shared-leg converter to operate with the same dc-link voltage as the full-bridge converter. 11.3.4 Half-Bridge Converter The half-bridge configuration at both converter sides is presented in Fig. 11.4). In this case there is a low frequency current flowing through the capacitors due to the dc-link midpoint connection, which increases the voltage fluctuation on these elements and consequently affects their losses. The voltage at the input and output converter sides is defined directly from the poles voltages 𝑣g10, 𝑣g20 and 𝑣l10, 𝑣l20, which are defined by equations (11.7), (11.8), (11.10), and (11.11), respectively. Also, the PWM equations are defined straightfor- ward since there is no degree of freedom to be explored, that is, there are only two legs to process two voltages. 11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) The connection of converters in parallel can be employed when the power ratings of the switches available do not handle the level of current needed by the circuit. The simplest solution when the currents demanded by the load are higher than the rated currents of the switches is connecting switches in parallel, as shown in Fig. 11.5 for the three-phase back-to-back converter. Although the number of power switches is twice as compared to those in Fig. 11.1, the characteristics of this converter in terms
  • 347. 11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 333 (a) (b) + – + – + – + – – + ig1 ig2 ig3 iC vC il1 il2 il3 vl3 vl2 vl1 eg1 eg2 eg3 vg3 vg2 vg1 Xg1 Xg2 Xg3 qg1 q2g g1 ng g2 ql2 nl ql1 ql2 ql1 l1 l2 0 2 qg2 qg1 + – vC 2 vl1 – + vl2 – + vl3 Figure 11.4 Half-bridge three-phase back-to-back converter: (a) block and (b) switch representation. Figure 11.5 Three-phase back-to-back converter with switches in parallel. of quality of the waveform generated are the same as in the conventional solution (see Fig. 11.1). As considered in Chapter 10 for the single-phase back-to-back converters, con- necting converters in parallel instead of switches in parallel will bring the following benefits: (i) increase the current capability of the conversion system, (ii) improve the quality of the waveforms generated at the input and output sides of the converter, and (iii) reduce the stress on the dc-link capacitors. 11.4.1 Model Although connecting converters in parallel allows reducing the level of power processed by each converter, as well as current ripple reduction, a circulating current
  • 348. 334 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS (a) (b) Converter 1 Converter 2 Converter 3 Converter 4 + – + – + – + – + – l vl3 vl2 vl1 eg1 vC1 iC1 + – eg2 + – eg3 vg3 vg2 vg1 X1a q1a q1b q1c q2c q2b q2a i2a il1 vl1 vl2 vl3 il2 il3 i2b i2c 1a 2a 01 1b 2b 1c 2c i1a i1b i1c X1b X1c X2a X2b X2c g 2 + – vC1 2 q1a q1b q1c q2c q2b q2a + – vC2 iC2 X3c q3a q1b q1c q4c q4b q4a i4c i4b i4a 3a 4a 02 3b 4b 3c 4c i3c i3b i3a X3b X3a X4a X4b X4c 2 + – vC2 2 q3a q3b q3c q4c q4b q4a Figure 11.6 Parallel three-phase back-to-back converter: (a) block and (b) switch representation. exists between both back-to-back converters. To model such a circulating current it is necessary to write down all equations of the system. Figure 11.6 shows a three-phase to three-phase energy conversion unit with two back-to-back converters connected in parallel. Note that, although increasing the complexity of the system, other back-to-back converters can be added in parallel, which reduces the power processed by each unit. Such a conversion unit can be represented by either power blocks [Fig. 11.6(a)] or power switches [Fig. 11.6(b)]. This conversion system consists of a three-phase load, six inductance filters (Xja, Xjb, and Xjc with j = 1, 3) at the grid side, six inductance filters (Xma, Xmb, and Xmc with m = 2, 4) at the load side, and two dc-link capacitor banks. Considering converters 1 and 3 (converters connected at the grid side), it is possible to write the following equations: eg1 = z1ai1a + 𝑣1a01 − 𝑣g01 (11.45)
  • 349. 11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 335 eg2 = z1bi1b + 𝑣1b01 − 𝑣g01 (11.46) eg3 = z1ci1c + 𝑣1c01 − 𝑣g01 (11.47) eg1 = z3ai3a + 𝑣3a02 − 𝑣g02 (11.48) eg2 = z3bi3b + 𝑣3b02 − 𝑣g02 (11.49) eg3 = z3ci3c + 𝑣3c02 − 𝑣g02 (11.50) for a balanced case 𝑣g01 and 𝑣g02 are given respectively by: 𝑣g01 = 1 3 (𝑣1a01 + 𝑣1b01 + 𝑣1c01 ) (11.51) 𝑣g02 = 1 3 (𝑣3a02 + 𝑣3b02 + 𝑣3c02 ) (11.52) where z1a = r1a + l1ap, z1b = r1b + l1bp, z1c = r1c + l1cp, z3a = r3a + l3ap, z3b = r3b + l3bp, and z3c = r3c + l3cp are the impedances of the elements X1a, X1b, X1c, X3a, X3b, and X3c, respectively; with p = d∕dt. 𝑣g01 and 𝑣g02 are the voltages between the neutral of the grid and the dc-link midpoints 01 and 02, respectively. Similar equations are obtained for converters 2 and 4 connected to the load, as follows: 𝑣l1 = −z2ai2a + 𝑣2a01 − 𝑣l01 (11.53) 𝑣l2 = −z2bi2b + 𝑣2b01 − 𝑣l01 (11.54) 𝑣l3 = −z2ci2c + 𝑣2c01 − 𝑣l01 (11.55) 𝑣l1 = −z4ai4a + 𝑣4a02 − 𝑣l02 (11.56) 𝑣l2 = −z4bi4b + 𝑣4b02 − 𝑣l02 (11.57) 𝑣l3 = −z4ci4c + 𝑣4c02 − 𝑣l02 (11.58) for a balanced case 𝑣l01 and 𝑣l02 are given respectively by: 𝑣l01 = 1 3 (𝑣2a01 + 𝑣2b01 + 𝑣2c01 ) (11.59) 𝑣l02 = 1 3 (𝑣4a02 + 𝑣4b02 + 𝑣4c02 ) (11.60) As expected, due to the connection of both converters in parallel, there is a cir- culating mesh that originates a circulating current between both ac–dc–ac conversion units, as highlighted in Fig. 11.7. z1ai1a + z2ai2a − z4ai4a − z3ai3a + 𝑣1a01 − 𝑣2a01 + 𝑣4a02 − 𝑣3a02 = 0 (11.61) z1ai1a + z2bi2b − z4bi4b − z3ai3a + 𝑣1a01 − 𝑣2b01 + 𝑣4b02 − 𝑣3a02 = 0 (11.62) z1ai1a + z2ci2c − z4ci4c − z3ai3a + 𝑣1a01 − 𝑣2c01 + 𝑣4c02 − 𝑣3a02 = 0 (11.63) z1bi1b + z2ai2a − z4ai4a − z3bi3b + 𝑣1b01 − 𝑣2a01 + 𝑣4a02 − 𝑣3b02 = 0 (11.64) z1bi1b + z2bi2b − z4bi4b − z3bi3b + 𝑣1b01 − 𝑣2b01 + 𝑣4b02 − 𝑣3b02 = 0 (11.65) z1bi1b + z2ci2c − z4ci4c − z3bi3b + 𝑣1b01 − 𝑣2c01 + 𝑣4c02 − 𝑣3b02 = 0 (11.66)
  • 350. 336 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS i1o i2o i3o i4o io io io io Figure 11.7 Circulating current between both back-to-back converters in parallel. z1ci1c + z2ai2a − z4ai4a − z3ci3c + 𝑣1c01 − 𝑣2a01 + 𝑣4a02 − 𝑣3c02 = 0 (11.67) z1ci1c + z2bi2b − z4bi4b − z3ci3c + 𝑣1c01 − 𝑣2b01 + 𝑣4b02 − 𝑣3c02 = 0 (11.68) z1ci1c + z2ci2c − z4ci4c − z3ci3c + 𝑣1c01 − 𝑣2c01 + 𝑣4c02 − 𝑣3c02 = 0 (11.69) Note that equations (11.61)–(11.69) exist due to the parallel connection of the back-to-back converters. If a transformer is employed for isolation purposes, the cur- rent io would be zero and equations (11.61)–(11.69) would no longer exist. An expression for the circulating voltage can be obtained by adding equations (11.61)–(11.69), to give the following expression: 𝑣o = c ∑ n=a z1ni1n + c ∑ n=a z2ni2n − c ∑ n=a z4ni4n − c ∑ n=a z3ni3n (11.70) with 𝑣o = − c ∑ n=a 𝑣1n01 + c ∑ n=a 𝑣2n01 + c ∑ n=a 𝑣3n02 − c ∑ n=a 𝑣4n02 (11.71) From the currents of the converters it is possible to define the circulating current as follows: i1o = 1 √ 3 (i1a + i1b + i1c) (11.72) i2o = 1 √ 3 (i2a + i2b + i2c) (11.73) i3o = 1 √ 3 (i3a + i3b + i3c) (11.74) i4o = 1 √ 3 (i4a + i4b + i4c) (11.75)
  • 351. 11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 337 As presented in Fig. 11.7, the circulating current can be represented as a single current that circulates among the converters. Such a current can be written as io = i1o = −i3o = i2o = −i4o (11.76) Since the parallel back-to-back converter deals with three-phase systems at both sides of the converter (i.e., grid and load sides), it is convenient to use the transfor- mation of variables from 123 to odq as follows: xg123 = Pxgodq (11.77) xl123 = Pxlodq (11.78) xkabc = Pxkodq (11.79) with xg123 = [xg1 xg2 xg3]T , xl123 = [xl1 xl2 xl3]T and xkabc = [xka xkb xkc]T, where x can be either voltage or current and k = 1, 2, 3, 4. Defining the voltages 𝑣1n = 𝑣1n01 − 𝑣g01 , 𝑣2n = 𝑣2n01 − 𝑣l01 , 𝑣3n = 𝑣3n02 − 𝑣g02 , and 𝑣4n = 𝑣4n02 − 𝑣l02 , with n = a, b, c, it is possible to determine the model of the system as follows: egdq = z1odqi1odq + 𝑣1dq (11.80) egdq = z3odqi3odq + 𝑣3dq (11.81) eldq = −z2odqi2odq + 𝑣2dq (11.82) eldq = −z4odqi4odq + 𝑣4dq (11.83) where egdq = [egd egq]T, eldq = [eld elq]T, ikodq = [iko ikd ikq]T, 𝑣kdq = [𝑣kd 𝑣kq]T , and zkodq = 1 6 [√ 2 ( 2zka − zkb − zkc ) (4zka + zkb + zkc) √ 3(zkc − zkb) √ 6(zkb − zkc) √ 3(zkc − zkb) 3(zkb + zkc) ] Then it is possible to write the equation for the circulating current as follows: 𝑣o = √ 3 [( 4 ∑ k=1 zko ) io + ∑ j=d,q z1oji1j + ∑ j=d,q z2oji2j − ∑ j=d,q z3oji3j − ∑ j=d,q z4oji4j ] (11.84) with zko = 2 6 (zka + zkb + zkc), zkod = √ 2 6 (2zka − zkb − zkc), and zkoq = √ 6 6 (zkb − zkc) It is also convenient to write the model in dq components since: (i) the voltages 𝑣1dq and 𝑣3dq will be employed to control the currents i1odq and i3odq and consequently the grid power factor, (ii) the load variables will be controlled by the voltages 𝑣2dq and 𝑣4dq, and (iii) the circulating current will be regulated by 𝑣o. Assuming a balanced case: z1n = z3n = z1 and z2n = z4n = z2 with n = a, b, c, it is possible to rewrite the model as follows: egdq = z1i1dq + 𝑣1dq (11.85) egdq = z1i3dq + 𝑣3dq (11.86) eldq = z2i2dq + 𝑣2dq (11.87) eldq = z2i4dq + 𝑣4dq (11.88)
  • 352. 338 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS with z1 = [ z1 0 0 z1 ] and z2 = [ z2 0 0 z2 ] From equations (11.80), (11.81) it is possible to obtain dq grid current: 𝑣gd = 𝑣1d + 𝑣3d 2 = egd − z1 2 igd (11.89) 𝑣gq = 𝑣1q + 𝑣3q 2 = egq − z1 2 igq (11.90) By following the same strategy, 𝑣ld and 𝑣lq are given by: 𝑣ld = 𝑣2d + 𝑣4d 2 = eld − z2 2 ild (11.91) 𝑣lq = 𝑣2q + 𝑣4q 2 = elq − z2 2 ilq (11.92) Defining zg = z1∕2 and zl = z2∕2, yields 𝑣gd = egd − zgigd (11.93) 𝑣gq = egq − zgigq (11.94) 𝑣ld = eld − zlild (11.95) 𝑣lq = elq − zlilq (11.96) 11.4.2 PWM As described in the model of the three-phase back-to-back converter, the reference voltages 𝑣∗ kd , 𝑣∗ kq , and 𝑣∗ o (k = 1, 2, 3, 4) are furnished by the controllers to regulate the input, output, and circulating variables, respectively. By employing a transformation of variables, it is possible to write the 123 voltages as a function of odq as follows: 𝑣∗ ka = √ 2 3 𝑣∗ kd (11.97) 𝑣∗ kb = √ 2 3 ( 1 2 𝑣∗ kd + √ 3 2 𝑣∗ kq ) (11.98) 𝑣∗ kc = √ 2 3 ( − 1 2 𝑣∗ kd − √ 3 2 𝑣∗ kq ) (11.99) The reference pole voltages employed for the PWM techniques can be defined as a function of auxiliary voltages as follows: 𝑣∗ 1a01 = 𝑣∗ 1a + 𝑣∗ x (11.100) 𝑣∗ 1b01 = 𝑣∗ 1b + 𝑣∗ x (11.101) 𝑣∗ 1c01 = 𝑣∗ 1c + 𝑣∗ x (11.102)
  • 353. 11.4 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN PARALLEL) 339 𝑣∗ 2a01 = 𝑣∗ 2a + 𝑣∗ y (11.103) 𝑣∗ 2b01 = 𝑣∗ 2b + 𝑣∗ y (11.104) 𝑣∗ 2c01 = 𝑣∗ 2c + 𝑣∗ y (11.105) 𝑣∗ 3a02 = 𝑣∗ 3a + 𝑣∗ o 3 − 𝑣∗ y + 𝑣∗ z + 𝑣∗ x (11.106) 𝑣∗ 3b02 = 𝑣∗ 3b + 𝑣∗ o 3 − 𝑣∗ y + 𝑣∗ z + 𝑣∗ x (11.107) 𝑣∗ 3c02 = 𝑣∗ 3c + 𝑣∗ o 3 − 𝑣∗ y + 𝑣∗ z + 𝑣∗ x (11.108) 𝑣∗ 4a01 = 𝑣∗ 4a + 𝑣∗ z (11.109) 𝑣∗ 4b01 = 𝑣∗ 4b + 𝑣∗ z (11.110) 𝑣∗ 4c01 = 𝑣∗ 4c + 𝑣∗ z (11.111) The voltages 𝑣∗ x , 𝑣∗ y and 𝑣∗ z can be defined by following the same approach as in equations (11.23) and (11.24). 11.4.3 Control Strategies Figure 11.8 shows the control block diagram of the parallel three-phase back-to-back converter. The dc-link voltages 𝑣C1 and 𝑣C2 are regulated by the controllers Rc1 and Rc2, respectively. These controllers furnish the amplitudes of the reference currents I∗ 1 and I∗ 3 required at the input side of the converters 1 and 3. The power factor control, in turn, is obtained by synchronization of the reference grid current i∗ 1abc (i∗ 1a , i∗ 1b , i∗ 1c ) – – + – + – – – + + + + I1 * I3 * i3abc * i1abc * eldq * eldq i1dq * v1dq * vo1 * vdq * el123 eldq v2dq * v4dq * vξ * vc12 i1dq i1abc q1abc q3abc q2abc q4abc eg123 i3abc i1odq i3dq * v3dq * io1 * io1 i3dq i3dq * vc1 vc1 vc2 * vc2 eg1 Σ Σ Σ Σ Σ Σ Rc1 Rvdq Gv24 Ri1dq Ri3dq Ro1 PWM Converters 1 and 3 Converters 2 and 4 Rc2 Gir dq 123 dq 123 dq 123 dq 123 Figure 11.8 Control block diagram of the parallel three-phase converter.
  • 354. 340 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS and i∗ 3abc (i∗ 3a , i∗ 3b , i∗ 3c ) with the three-phase voltages. Such a synchronization is done in block Gir, which employs a PLL-based technique. The output of block Gir are instantaneous reference currents that are converted to dq variables through the transformation 123/dq, based on the block dq. As a con- sequence, the output of these blocks are the reference currents i∗ 1dq (i∗ 1d , i∗ 1q ) and i∗ 3dq (i∗ 3d , i∗ 3q ). A double-sequence type of controller is employed on Ri1dq and Ri3dq to reg- ulate the sinusoidal currents i∗ 1dq and i∗ 3dq . The output of the controllers Ri1dq and Ri3dq define the reference voltages 𝑣∗ 1dq and 𝑣∗ 3dq . The circulating current is regulated by Ro1 with i∗ o1 = 0. The output of block Ro1 is circulating voltage 𝑣∗ o1 . The load voltage controller is obtained via block R𝑣dq. The output of this controller defines 𝑣∗ dq (𝑣∗ d and 𝑣∗ q). The voltage applied for each converter can be considered as half of the voltage 𝑣dq, the block G𝑣24 gives 𝑣∗ 2dq = 𝑣∗ 4dq = 𝑣∗ dq ∕2. Finally the reference voltages gener- ated by the controllers 𝑣∗ 1dq , 𝑣∗ 3dq , 𝑣∗ o1 , 𝑣∗ 2dq , and 𝑣∗ 4dq , and the auxiliary voltages (𝑣∗ 𝜉 with 𝜉 = x, y, and z) are applied to the PWM block. The output of this block generates the state of the switches. 11.5 TOPOLOGIES WITH INCREASED NUMBER OF SWITCHES (CONVERTERS IN SERIES) The series connection (i.e., cascade connection) of the three-phase back-to-back con- verters can be obtained as shown in Fig. 11.9(a) for the power blocks representation, while Fig. 11.9(b) shows the same conversion system with power switches. Note that the line-to-line voltages viewed by both grid and load sides will be two connected H-bridge converter series. The same advantages as described for the single-phase back-to-back converter are observed in this topology. Also, it is necessary to regulate the circulating current among the conversion units to increase the efficiency of the converter. 11.6 OTHER BACK-TO-BACK CONVERTERS In the power distribution systems, the single-phase grid has been considered as an alternative for either rural or remote areas, due to its lower cost feature, especially when compared with the three-phase solution. Hence, the single-phase voltage avail- able as the power supply is quite common where there is a large area to be covered. On the other hand, loads connected in a three-phase arrangement present some advan- tages when compared to single-phase loads. This is especially true when a motor is the load connected to the converter, due to its reduced size, constant torque and con- stant power at balanced conditions. In this scenario, there is a need for single-phase to three-phase power conversion systems. The back-to-back converter, able to interface a three-phase load and a single-phase grid, is presented in Fig. 11.10. Such a single-phase to three-phase power conversion presents an inherent asymmetry, that is, constant power at the output converter side (three-phase load)
  • 355. 11.6 OTHER BACK-TO-BACK CONVERTERS 341 (a) (b) Converter 1 Converter 2 Converter 3 + – + – + – + – + – nl vl3 vl2 vl1 eg1 vC1 + – eg2 ig2 ig3 ig1 + – eg3 vg3 vg2 vg1 X1a X1a q1a 1a 1b 1d 1c q1b q1c q1d il1 vl1 vl2 vl3 il2 il3 01 X2a X2a X3a X3a ng 2 + – vC1 2 q1a q1b q1c q1d + – vC2 q2a 2a 2b 2d 2c q2b q2c q2d 02 2 + – vC2 2 q2a q2b q2c q2d + – vC3 q3a 3a 3b 3d 3c q3b q3c q3d 03 2 + – vC3 2 q3a q3b q3c q3d Figure 11.9 Three-phase configuration with back-to-back converter series connected: (a) block and (b) switch representation.
  • 356. 342 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS Figure 11.10 Single-phase to three-phase back-to-back converter. + + – – (a) (b) Rectifier Pulsating power Constant power Inverter iin iout υin υout Figure 11.11 (a) Power asymmetry of the single-phase to three-phase converter (b) a potential solution to deal with the asymmetry.
  • 357. 11.6 OTHER BACK-TO-BACK CONVERTERS 343 Figure 11.12 Three-phase to three-phase four-wire back-to-back converter. is6 vs6 is2 vs2 is4 vs4 is3 vs3 vs3 is5 vs5 is1 vs1 – – – – – + + vs2 – + vs1 – + vs4 – + vs5 – + vs6 – + + + + + + Six-phase machine Six-phase machine n n m m Figure 11.13 (a) Six-phase machine drive system based on three-phase back-to-back converters (b) model of the motor drive system.
  • 358. 344 CHAPTER 11 THREE-PHASE TO THREE-PHASE AND OTHER BACK-TO-BACK CONVERTERS and a pulsating power at the input converter side (single-phase grid), as highlighted in Fig. 11.11(a). The direct consequence of this asymmetry is the low frequency voltage oscillation observed in the dc-link capacitors; also, the power switches of the rectifier and inverter operate with different current ratings. Normally, the three-phase motor rated voltage is higher than that furnished by the single-phase grid, which means that the rectifier circuit must boost the grid voltage to guarantee the motor rated voltage. Consequently, the current relationship between input and output converter sides also implies converter asymmetry with the input current higher than the output current. There are different ways to deal with this challenge; one way is to employ the topology presented in Fig. 11.11(b) with a parallel converter used at the rectifier stage. Another example of three-phase back-to-back converters is presented in Fig. 11.12, which deals with a load demanding a three-phase system with four wires. Note that this configuration is able to generate a regulated three-phase voltage at the load side where both three-phase and single-phase loads can be connected. Lastly, Fig. 11.13(a) shows a six-phase machine drive system based on ac–dc–ac converter topologies connected in paralleled without isolation trans- former. Note that unlike the previous parallel configurations presented in this chapter, the motor drive system in Fig. 11.13(a) does not have circulating current since the neutrals (n and m) of the six-phase machine are not connected between themselves, as highlighted in the model in Fig. 11.13(b). The six-phase machine is in fact constituted by two sets of three-phase windings, which present benefits such as reduced ripple on the torque. Another advantage of the six-phase motor drive system compared to the three-phase one is the fact that the currents processed by each switch of the inverter are lower. 11.7 SUMMARY This chapter dealt with three-phase back-to-back converters. Section 11.2 presented the full-bridge ac–dc–ac converter, its model, PWM, and control strategies. Topologies with component count reduction were presented in Section 11.3, while Sections 11.4 and 11.5 showed the model, PWM, and control for configurations with an increased number of semiconductor devices. Shared-leg and dc-link capacitor midpoint connections were also considered for reducing the number of semiconduc- tor devices, while connecting back-to-back converters in parallel and series. Other three-phase arrangements were considered in Section 11.6. Readers can find more details from References 1 to 8. REFERENCES [1] H. W. van der Broeck and J. D. van Wyk, A comparative investigation of a three-phase induction machine drive with a component minimized voltage-fed inverter under different control options, IEEE Trans Ind Appl, vol. IA-20, no. 2, pp. 309–320, Mar./Apr. 1984. [2] P. Enjeti and A. Rahman, A new single phase to three phase converter with active input current shaping for low cost AC motor drives, IEEE Trans Ind Appl, vol. 29, no. 4, pp. 806–813, Jul./Aug. 1993.
  • 359. REFERENCES 345 [3] Blaabjerg F, Freysson S, Hansen HH, and Hansen S. Comparison of a space-vector modulation strategy for a three phase standard and a component minimized voltage source inverter. Proceedings EPE; 1995. p. 1806–1813. [4] Kim GT and Lipo TA. VSI-PWM rectifier/inverter system with a reduced switch count. Conference. Rec. IEEE IAS Annual Meeting; 1995. p. 2327–2332. [5] C. B. Jacobina, M. B. R. Correa, E. R. C. da Silva, and A. M. N. Lima, Induction motor drive system for low-power applications, IEEE Trans Ind Appl, vol. 35, no. 1, pp. 52–61, Jan./Feb. 1999. [6] F. Blaabjerg, D. O. Neacsu, and J. K. Pedersen, Adaptive SVM to compensate dc-link voltage ripple for four-switch three-phase voltage-source inverters, IEEE Trans Power Electron, vol. 14, no. 4, pp. 743–752, Jul. 1999. [7] E. Ledezma, B. McGrath, A. Muñoz, and T. A. Lipo, Dual AC-drive system with a reduced switch count, IEEE Trans Ind Appl, vol. 37, no. 5, pp. 1325–1333, Sep./Oct. 2001. [8] J. R. Rodríguez, J. W. Dixon, J. R. Espinoza, J. Pontt, and P. Lezana, PWM regenerative rectifiers: State of the art, IEEE Trans Ind Electron, vol. 52, no. 1, pp. 5–22, Feb. 2005.
  • 361. INDEX A ac–dc conversion, 43–50 controlled rectifiers, 45 full-bridge controlled, 49 PWM control, 47 single split-phase rectifier with free-wheeling diode, 48 three-phase controlled rectifier, 49 three-phase half-bridge controlled rectifier, 48 uncontrolled rectifiers, 43 ac–dc–ac configurations, 81–85 PBG application in, 81–85 single-phase to single-phase configurations, 85 three-phase to three-phase configurations, 82–85 ac–dc–ac converter, 3 active switch ANPC converters, 214 active-neutral-point-clamped (ANPC) converters, 211–214 configuration, 211–212 alternate phase opposite disposition (APOD), 167 analog PWM implementation, 228 applications of power electronics converters, 6–9 in a distributed generation system, 7 Energy-Control-Center (ECC), 8 field, 8–9 that process ac voltage, 6 B back-to-back converters, 324–344, See also three-phase to three-phase converters single-phase to three-phase back-to-back converter, 342 power asymmetry of, 342 Advanced Power Electronics Converters: PWM Converters Processing AC Voltages, Forty Fifth Edition. Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva. © 2015 The Institute of Electrical and Electronics Engineers, Inc. Published 2015 by John Wiley & Sons, Inc. three-phase to three-phase four-wire back-to-back converter, 343 basic power converters, 25–43, See also ac–dc conversion; dc–ac conversion; dc–dc conversion; power semiconductor devices building, principles for, 27 connecting source to load, ways to, 28 bidirectional controlled thyristor (BCT), 12 bipolar junction transistor (BJT), 12, 19 bipolar modulation, 38 boost converter, 31 topological states for, 32 buck converter, 28 with basic cell switch, 29 with real switches, 29 topological states for, 29 buck-boost converter, 33 C capacitor bank design, 304–307 capacitor current spectrum, 239 carrier-based PWM (CPWM), 221 configurations with, 247–252 our-leg converter, 249–252 three-leg converter, two-phase machine, 247–249 nonconventional topologies with, 252–261 cascade configuration, 72–75, 125–170 single H-bridge converter, 126–128 three-phase Converter one H-bridge converter per phase, 140–144 two cascade H-bridges per phase, 149–162 347
  • 362. 348 INDEX cascade configuration (Continued) two H-bridge converters, 144–146 cascade control strategies, 289–293 motor drive, speed-current control, 290–293 rectifier circuit, voltage-current control, 289–290 chopper, 3 classifications of power electronics topologies, 3 component count reduction, topology with, 307–310 dc-link voltage requirement, 309–310 half-bridge converter, 310 model, 307–308 PWM strategy, 308–309 control approach full-bridge converter, 328–330 controlled conduction/controlled blocking devices, 19–22 bipolar junction transistor (BJT), 19 IGBT, 21 gate turn-off (GTO), 21–22 IGCT, 22 reverse blocking IGCT (RBIGCT), 22 MOSFET, 19, 20–21 controlled conduction/spontaneous blocking devices, 18–19 silicon-controlled rectifier (SCR), 18 TRIode AC (TRIAC), 18–19 controlled rectifiers, 45 controlled ac–dc converter using switching cell, 46 phase control, 45 single-phase rectifier, 46–47 conventional diode, 17–18 cuk converter, 33 current-source inverters (CSIs), 33, 43 cycle converter, 3 D dc–ac conversion, 33–40 current-source inverters (CSIs), 33 impedance-source inverters (ZSIs), 33 three-phase inverter, 38 voltage-source inverters (VSIs), 33, 34 dc–ac–dc converter, 3 dc–dc conversion, 28–33 boost converter, 31 buck converter, 28 buck-boost converter, 33 cuk converter, 33 single-ended primary-inductor converter (SEPIC) converter, 33 zeta converter, 33 dc-link capacitor voltage, 301–304 dc-link voltage requirement, 309–310 differential converter, 218 digital PWM implementation, 228–231 dynamic controllability, ideal switches, 12–15 controlled turn off, 14 controlled turn on, 14 spontaneous turn off, 14 spontaneous turn on, 14 dynamic voltage restorer (DVR), 251–252 E electromotive force (emf), 276 Energy-Control-Center (ECC), 8 F five-level FC topology, 188 five-level NPC configuration, 119–123 PB representation, 121 with pyramid structure, 122 flying capacitor (FC) converter, 172–197 configuration, 75–79 four-level configuration, 189–196, See also individual entry full-bridge topology, 181–183 generalization, 196–197 nonconventional FC converters with three-level legs, 186–189 three-level configuration, 173–176 three-phase FC converter, 183–186 voltage control, 179–181 forward blocking voltage, 16 forward voltage capability, 16 forward voltage drop, 16 four H-bridge converters and generalization, 169 four-leg converter, 249–252 dynamic voltage restorer (DVR), 251–252 supplying a three-phase four-wire load, 249 supplying four-phase machine, 250 four-level FC configuration, 189–196 converter with four switches, 194–195 four-level FC configuration with PBs, 191
  • 363. INDEX 349 four-level FC half-bridge converter, 194 gating signal generation, modulation strategy for, 193 general four-level output voltage, generation of, 192 single-phase full-bridge four-level FC converter, 196 three-phase two-leg FC converter, 190 four-level NPC configuration, 112–115 open-end motor drive system, 121 three-phase NPC converter, 120 four-wire back-to-back converter, 343 full-bridge converter, 36, 296–307, 325–330 capacitor bank design, 304–307 control approach, 298–299, 328–330 dc-link capacitor voltage, 301–304 model, 296–297, 325 power analysis, 299–301 PWM strategy, 297–298, 327–328 single-phase full-bridge inverter, 36–37 full-bridge single-phase converter, 95–98 using four-level NPC legs, 118–119 full-bridge topology, flying capacitor (FC) converter, 181–183 G gate turn-off (GTO), 4, 21–22 gate-assisted turnoff thyristor (GATT), 4 gating signal generation, modulation strategy for, 193 generalization, FC converter, 196–197 H half-bridge converter, 310, 332 half-bridge inverter, 34 half-bridge topology, 93–95, 177–178 hexagonal-field-effect-transistor (HEXFET), 20 hybrid topology, 107 hysteresis control, 271–279 for dc motor drive, 275–278 defining the state of the switches, 272 measured load current, 273 reference load current, 273 for regulating an ac variable, 278–279 startup transient for, 273 I ideal switches, 11–15 characteristics, 11 dynamic controllability, 12–15 power electronics devices as, 11–15 static characteristics, 12 impedance-source inverters (ZSIs), 33 indirect ac–dc–ac conversion, 50–51 in-phase disposition (IPD), 167 insulated bipolar junction transistor (IGBT), 12 insulated-gate-bipolar transistor (IGBT), 4, 58 Integrated gate commutation thyristor (IGCT), 22 interdisciplinary nature of power electronics, 2 L linear control, ac variable, 288–289 linear control, dc variable, 279–288 proportional controller, 279–280 dc motor drive system, 280–283 RL load, 279–280 proportional-integral controller, 283–285 dc motor, 285–286 RL load, 283–285 proportional-integral-derivative controller, 286–288 dc motor, 286–288 linear regulators, 5 M macro grid, 7 magnetic element at the output, topology with, 205–211 five-level topology, 209 modular multilevel converter, 211 with PBs, 210 three-level configurations, 206 maximum peak nonrepetitive forward and reverse voltage, 16 metal oxide semiconductor field-effect transistors (MOSFETs), 4, 19, 20–21, 58 micro grid, 7–8 mixed NPC/FC converters, 215–216 using flying capacitor, 217 and first PB-ac, 217 first/second PB-ac, 217 modular multilevel converter (MMC), 199 MOS-controlled thyristor (MCT), 4, 22 motor drive, speed-current control, 290–293
  • 364. 350 INDEX multilevel configurations, 79–81, 199–219, See also active-neutral-point-clamped (ANPC) converters; active switch ANPC converters; mixed NPC/FC converters; nested multilevel configurations N nested multilevel configurations, 200–205 with block representation, 200 generalization of, 205 PWM approach for, 204 with switches representation, 201 three-phase four-level nested configurations, 204 neutral-point-clamped (NPC) configuration, 88–124, 172 five-level configuration, 119–123 four-level NPC configuration, 112–115 full-bridge and other circuits (four-level configuration), 118–119 nonconventional arrangements by using three-level legs, 101–108 three-level configuration, 89–93 full-bridge topologies, 95–98 three-phase NPC converter, 98–101 unbalanced capacitor voltage, 108–112 neutral-point-clamped (NPC) inverter, 67 configuration, 68–72 NPC multilevel legs, construction, 69 nonconventional arrangements by using three-level legs, 101–108 five-level single-phase converter, 103 four-level single-phase converter, 103 hybrid topology, 107 nonconventional FC converters with three-level legs, 186–189 five-level FC topology, 188 four-level FC topology, 188 nonconventional topologies with CPWM, 252–261 open-end winding motor drive system, 257–261 split-wound coupled inductors, inverter with, 252–254 Z-source converter, 254–257 O on-state current, 16 on-state root mean square (RMS) current, 16 open-end winding motor drive system, 257–261 optimized PWM approach, 221–261, See also space vector modulation (SVPWM); two-leg converter P peak repetitive forward current, 16 peak surge forward current, 16 phase control, 45 phase opposite disposition (POD), 167 photovoltaic (PV) power system, 135–140 point of common coupling (PCC), 8 power blocks geometry (PBG), 56–86 application in multilevel configurations, 67–81 cascade configuration, 72–75 flying capacitor configuration, 75–79 multilevel configurations, 79–81 neutral-point-clamped configuration, 68–72 basic units used in, 61 concepts, 58 configurations employing four controlled switches, 59 configurations employing six controlled switches, 60 description of power blocks, 62–67 variables associated with, 63–65 principles of, 58–62 propositions, 58 power converters applications of, 6–9 basic control principles, 265–271 ATLAB code, 266, 269 discretization method, 265 control strategies for, 264–293, See also cascade control strategies; hysteresis control; linear control, ac variable; linear control, dc variable history of, 4–6 processing ac voltage, 56–86, See also power blocks geometry (PBG) synthesize ac voltage, 57 power losses, 17 power semiconductor devices, 16–25 controlled conduction/controlled blocking devices, 19–22, See also individual entry
  • 365. INDEX 351 controlled conduction/spontaneous blocking devices, 18–19 forward and reverse voltage capability, 16 forward blocking voltage, 16 forward voltage drop, 16 maximum peak nonrepetitive forward and reverse voltage, 16 nonideal device characteristics, 16 peak repetitive forward current, 16 peak surge forward current, 16 power losses, 17 reverse blocking voltage, 16 spontaneous conduction/controlled blocking devices, 22–24 spontaneous conduction/spontaneous blocking, 17–18 on-state current, 16 on-state root mean square (RMS) current, 16 turn-off time, 17 turn-on time, 16 power switches, 10–52, See also ideal switches history of, 4–6 powerblock geometry (PBG), 172 pulse width modulation (PWM), 10, 88, 172, 221–261, See also optimized PWM approach generation, 105 analog implementation, 105 waveforms, 105 implementation, 125 four-level configuration, 115–118 of single H-bridge converter, 129–140 of two cascade H-bridges, 146–149 half-bridge topology, 93–95, 177–178 PWM control, 47 pulsed voltage source, 57 pulse-width modulation (PWM) converters, 10 R rectifier or inverter, 3 rectifier circuit, 289–290 voltage-current control, 289–290 reverse blocking IGCT (RBIGCT), 22 reverse blocking voltage, 16 reverse voltage capability, 16 S Schottky diode, 18 Siemens-Power Metal Oxide Silicon (SIPMOS), 20 silicon-controlled rectifier (SCR), 6, 18 single H-bridge converter, 126–128 one h-bridge converter per phase, 140–144 PWM implementation of, 129–140 two-level H-bridge converter, 131 single-ended primary-inductor converter (SEPIC) converter, 33 single-phase full-bridge inverter, 36–37 single-phase rectifier, 46–47 single-phase to single-phase back-to-back converter, 295–321, See also full-bridge converter component count reduction, topology with, 307–310 topologies with increased number of switches converters in parallel, 310–318 converters in series, 318–321 single-phase to single-phase configurations, 85 sinusoidal pulse width modulation (SPWM), 34, 221 space vector modulation (SVPWM), 221, 243–247 graphical analysis for, 245 split-wound coupled inductors, inverter with, 252–254 spontaneous conduction/controlled blocking devices, 22–24 static induction thyristor (SITH), 23–24 static induction transistor (SIT), 22–23 spontaneous conduction/spontaneous blocking, 17–18 conventional diode, 17–18 Schottky diode, 18 static characteristics, ideal switches, 12 static induction thyristor (SITH), 23–24 static induction transistor (SIT), 22–23 switching power suppliers, 5 T T flowing current metal oxide silicon (TMOS), 20 three H-bridge converters, 164–169 analog control circuitries, 167, 168
  • 366. 352 INDEX three H-bridge converters (Continued) Δ connections for the outer converters, 165 level shift multicarrier modulation, 168 open-winding machine, 165 three-phase Y-connected, 165 three-phase Δ-connected, 165 three-leg converter, two-phase machine, 247–249 three-level configuration flying capacitor (FC) converter, 173–176 three-level NPC configuration, 89–93 three-phase converter, 149–162 FC converter, 183–186 two cascade H-bridges per phase, 149–162 fault-tolerant converter with triacs, 155 fault-tolerant strategy, 160 motor drive system with open-end winding topology, 157 open-circuit type of fault, 153 post-fault configuration, 159 pre-fault configuration, 158 short-circuit type of fault, 153 three-phase four-level nested configurations, 204 three-phase inverter, 38 line-to-line voltage, 40 load phase voltage, 40 modes of operation, 41 pole voltages, 40 zero-sequence voltage, 40 three-phase machine connection, 238–242 influence over inverter variables, 238–242 three-phase NPC converter, 98–101 three-phase switching matrix, 51 three-phase to three-phase converters, 324–344, See also full-bridge converter block representation, 325 configurations, 82–85 switch representation, 325 topologies with increased number of switches converters in parallel, 332–340 converters in series, 340 topology with component count reduction, 330–332 topologies with increased number of switches, 310–318, 332–340 control strategy, 316–318 converters in parallel, 332–340 control strategies, 339–340 half-bridge three-phase back-to-back converter, 333 model, 333–338 PWM strategy, 338–339 three-phase back-to-back converter with switches in parallel, 333 converters in series, 340 model, 311–314 topology with component count reduction, 330–332 dc-link voltage requirement, 332 half-bridge converter, 332 model, 330–331 PWM strategies, 331–332 total harmonic distortion (THD), 67 TRIode AC (TRIAC), 18–19 two cascade H-bridges, PWM implementation of, 146–149 two H-bridge converters, 144–146, 162–164 seven- and nine-level topologies, 162–164 two-leg converter, 222–233 analog implementation, 228–231 digital implementation, 228–231 model, 222–223 PWM implementation, 223–228 𝜇 influence for, 231–233, 236–238 and three-phase load, 233–242 analog implementation, 236 digital implementation, 236 model, 233–235 PWM implementation, 235–236 U unbalanced capacitor voltage, 108–112 uncontrolled rectifiers, 43 uninterrupted power supply (UPS), 303, 305 unipolar modulation, 38 Universal Power Quality Conditioner (UPQC), 329
  • 367. INDEX 353 V voltage control, flying capacitor, 179–181 voltage-source inverters (VSIs), 33, 34 full-bridge, 36 half-bridge inverter, 34 W weighted total harmonic distortion (WTHD), 236–237 Z zeta converter, 33 Z-source converter, 254–257
  • 369. IEEE Press Series on Power Engineering Series Editor: M. E. El-Hawary, Dalhousie University, Halifax, Nova Scotia, Canada The mission of IEEE Press Series on Power Engineering is to publish leading- edge books that cover the broad spectrum of current and forward-looking tech- nologies in this fast-moving area. The series attracts highly acclaimed authors from industry/academia to provide accessible coverage of current and emerging topics in power engineering and allied fields. Our target audience includes the power engineering professional who is interested in enhancing their knowledge and perspective in their areas of interest. 1. Principles of Electric Machines with Power Electronic Applications, Second Edition M. E. El-Hawary 2. Pulse Width Modulation for Power Converters: Principles and Practice D. Grahame Holmes and Thomas Lipo 3. Analysis of Electric Machinery and Drive Systems, Second Edition Paul C. Krause, Oleg Wasynczuk, and Scott D. Sudhoff 4. Risk Assessment for Power Systems: Models, Methods, and Applications Wenyuan Li 5. Optimization Principles: Practical Applications to the Operations of Markets of the Electric Power Industry Narayan S. Rau 6. Electric Economics: Regulation and Deregulation Geoffrey Rothwell and Tomas Gomez 7. Electric Power Systems: Analysis and Control Fabio Saccomanno 8. Electrical Insulation for Rotating Machines: Design, Evaluation, Aging, Testing, and Repair, Second Edition Greg Stone, Edward A. Boulter, Ian Culbert, and Hussein Dhirani 9. Signal Processing of Power Quality Disturbances Math H. J. Bollen and Irene Y. H. Gu 10. Instantaneous Power Theory and Applications to Power Conditioning Hirofumi Akagi, Edson H. Watanabe, and Mauricio Aredes 11. Maintaining Mission Critical Systems in a 24/7 Environment Peter M. Curtis
  • 370. 12. Elements of Tidal-Electric Engineering Robert H. Clark 13. Handbook of Large Turbo-Generator Operation and Maintenance, Second Edition Geoff Klempner and Isidor Kerszenbaum 14. Introduction to Electrical Power Systems Mohamed E. El-Hawary 15. Modeling and Control of Fuel Cells: Distributed Generation Applications M. Hashem Nehrir and Caisheng Wang 16. Power Distribution System Reliability: Practical Methods and Applications Ali A. Chowdhury and Don O. Koval 17. Introduction to FACTS Controllers: Theory, Modeling, and Applications Kalyan K. Sen and Mey Ling Sen 18. Economic Market Design and Planning for Electric Power Systems James Momoh and Lamine Mili 19. Operation and Control of Electric Energy Processing Systems James Momoh and Lamine Mili 20. Restructured Electric Power Systems: Analysis of Electricity Markets with Equilibrium Models Xiao-Ping Zhang 21. An Introduction to Wavelet Modulated Inverters S.A. Saleh and M.A. Rahman 22. Control of Electric Machine Drive Systems Seung-Ki Sul, 23. Probabilistic Transmission System Planning Wenyuan Li 24. Electricity Power Generation: The Changing Dimensions Digambar M. Tigare 25. Electric Distribution Systems Abdelhay A. Sallam and Om P. Malik 26. Practical Lighting Design with LEDs Ron Lenk and Carol Lenk 27. High Voltage and Electrical Insulation Engineering Ravindra Arora and Wolfgang Mosch 28. Maintaining Mission Critical Systems in a 24/7 Environment, Second Edition Peter Curtis 29. Power Conversion and Control of Wind Energy Systems Bin Wu, Yongqiang Lang, Navid Zargari, and Samir Kouro
  • 371. 30. Integration of Distributed Generation in the Power System Math H. Bollen and Fainan Hassan 31. Doubly Fed Induction Machine: Modeling and Control for Wind Energy Generation Applications Gonzalo Abad, Jesus Lopez, Miguel Rodrigues, Luis Marroyo, and Grzegorz Iwanski 32. High Voltage Protection for Telecommunications Steven W. Blume 33. Smart Grid: Fundamentals of Design and Analysis James Momoh 34. Electromechanical Motion Devices, Second Edition Paul C. Krause, Oleg Wasynczuk, and Steven D. Pekarek 35. Electrical Energy Conversion and Transport: An Interactive Computer-Based Approach, Second Edition George G. Karady and Keith E. Holbert 36. ARC Flash Hazard and Analysis and Mitigation J. C. Das 37. Handbook of Electrical Power System Dynamics: Modeling, Stability, and Control Mircea Eremia and Mohammad Shahidehpour 38. Analysis of Electric Machinery and Drive Systems, Third Edition Paul Krause, Oleg Wasynczuk, S. D. Sudhoff, and Steven D. Pekarek 39. Extruded Cables for High-Voltage Direct-Current Transmission: Advances in Research and Development Giovanni Mazzanti and Massimo Marzinotto 40. Power Magnetic Devices: A Multi-Objective Design Approach S. D. Sudhoff 41. Risk Assessment of Power Systems: Models, Methods, and Applications, Second Edition Wenyuan Li 42. Practical Power System Operation Ebrahim Vaahedi 43. The Selection Process of Biomass Materials for the Production of Bio-Fuels and Co-Firing Najib Altawell 44. Electrical Insulation for Rotating Machines: Design, Evaluation, Aging, Testing, and Repair, Second Edition Greg C. Stone, Ian Culbert, Edward A. Boulter, Hussein Dhirani
  • 372. 45. Principles of Electrical Safety Peter E. Sutherland 46. Advanced Power Electronics Converters: PWM Converters Processing AC Voltages Euzeli Cipriano dos Santos Jr. and Edison Roberto Cabral da Silva
  • 373. WILEY END USER LICENSE AGREEMENT Go to www.wiley.com/go/eula to access Wiley’s ebook EULA.