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Global Positioning System
Presented by: Prantik Chowdhury
Dept. of Mechanical Engineering
3rdYear, B/1, 1457082.
Contents:
▪ Basics
▪ History
▪ Satellites
▪ Receivers
▪ Ground Stations
▪ Working
▪ Errors
▪ Error Correction
▪ Applications
Basics
▪ GPS stands forGlobal Positioning System which measures 3-D
locations on Earth surface using satellites
▪ GPS operates using radio signals sent from satellites orbiting the earth
▪ Created and Maintained by the US Dept. of Defense
▪ System as a whole consists of three segments
– Satellites (space segment)
– Receivers (user segment)
– Ground stations (control segment)
History
▪ Development began in 1973
▪ First satellite became operational in 1978
▪ Declared completely functional in 1995
▪ A total of 52 satellites have been launched
in 4 phases
▪ 30 satellites are currently functional
▪ Managed by the U.S. Department of
Defense
– Originally developed for submarines
– Now part of modern “smart bombs” and highly
accurate missiles
Satellites
▪ At least 4 satellites are above
the horizon anytime anywhere
▪ GPS satellites are also known as
“NAVSTAR satellites”
▪ The satellites transmit time
according to very accurate
atomic clocks onboard each one
▪ The precise positions of
satellites are known to the GPS
receivers from a GPS almanac
A visual example of a 24 satellite GPS
constellation in motion with the earth
rotating. Notice how the number of satellites
in view from a given point on the earth's
surface, in this example in Golden CO
(39.7469° N, 105.2108° W), changes with
time.
Satellites(Contd.)
▪ The satellites are in motion
around the earth
▪ Like the sun and moon satellites
rise and set as they cross the sky
▪ Locations on earth are
determined from available
satellites (i.e., those above the
horizon) at the time the GPS
data are collected
Receivers
▪ Ground-based devices read and interpret the radio
signals from several of the NAVSTAR satellites at once
▪ Geographic position is determined using the time it
takes signals from the satellites to reach the GPS
receiver
▪ Calculations result in varying degrees of accuracy that
depend on:
– Quality of the receiver
– User operation of the receiver (e.g., skill of user and
receiver settings)
– Atmospheric conditions
– Local conditions (i.e., objects that block or reflect the
signals)
– Current status of system A handheld GPS
receiver.
Ground Stations
▪ Control stations
– Master station at Falcon (Schriever)AFB, Colorado
– 4 additional monitoring stations distributed around the world
▪ Responsibilities
– Monitor satellite orbits & clocks
– Broadcast orbital data and clock corrections to satellites
Map from P. Dana,The Geographer's Craft Project, Dept. of Geography, U.Texas-Austin.
How GPS Works: Overview
▪ Satellites have accurate atomic clocks onboard and all GPS
satellites transmit the same time signal at the same time
– Think “synchronize your watches”
▪ The satellite signals contain information that includes
– Satellite number
– Time of transmission
How GPS Works: Overview
▪ Receivers use an almanac that includes
– The position of all satellites every second
– This is updated monthly from control stations
▪ The satellite signal is received, compared with the
receiver’s internal clock, and used to calculate the distance
from that satellite
▪ Trilateration (similar to triangulation) is used to determine
location from multiple satellite signals
How GPS Works: Signal
Processing
▪ Distances between satellites and receivers is determined by the time
is takes the signal to travel from satellite to receiver
– Radio signals travel at speed of light (186,000 miles/second)
– All satellites send the identical time, which is also generated by the receivers
– Signal travel time = offset between the satellite signal and the receiver signal
– Distance from each satellite to receiver = signal travel time * 186,000
miles/second
1sec
Receiver signal
Satellite signal
How GPS Works: Trilateration
How GPS Works: Trilateration
▪ Start by determining distance between a GPS satellite and your
position
▪ Adding more distance measurements to satellites narrows down
your possible positions
▪ The 4th satellite in trilateration is to resolve any signal timing error
– UnlikeGPS satellites, GPS receivers do not contain an atomic clock
– To make sure the internal clock in the receiver is set correctly we use the signal
from the 4th satellite
Errors
▪ Satellite errors:
Satellite position error (i.e., satellite not exactly where it’s supposed to be)
Atomic clocks, though very accurate, are not perfect
▪ Atmospheric
Electro-magnetic waves travel at light speed only in a vacuum
Atmospheric molecules, particularly those in the ionosphere, change the signal
speed
Errors(Contd.)
▪ Multi-path distortion
The signal may "bounce" off structures before reaching the GPS receiver – the
reflected signal arrives a little later
▪ Receiver error
Due to the receiver clock or internal noise
▪ Selective Availability
No longer an issue
Sources of Errors
▪ Satellite Clock & Satellite Position
• Atomic clock errors
+/- 2 meters of error
• Satellite is not in precise orbit
+/- 2.5 meters of error
Sources of Errors(Contd.)
▪ Atmospheric Delays/Bending
– +/- 5 meters or error
Sources of Errors(Contd.)
▪ Multi Path Interference (signal bouncing off of buildings, trees, etc.)
– +/- 1 meter of error
Sources of Errors(Contd.)
▪ ReceiverTiming/Rounding Errors
– +/- 1 meter of error (depends on the quality of the GPS receiver)
GPS - Selective Availability
▪ A former significant source of error
– Error intentionally introduced into the satellite signal by the U.S. Dept. of
Defense for national security reasons
– Selective Availability turned off early May 2, 2000
GPS Error: Position Dilution
of Precision
▪ Satellite Coverage: Position Dilution of Precision (PDOP)
▪ Remember that satellites are moving, causing the satellite
constellation to change
▪ Some configurations of satellites are better than others
▪ PDOP values range from 1 to 50, with values < 6 considered “good”
Poor PDOP Good PDOP
GPS: Error Budget
▪ Example of typically observed error from a consumerGPS receiver:
• Typical Observed errors (meters)
satellite clocks 0.6
orbit (position error) 0.6
receiver errors 1.2
atmosphere 3.7
• Total 6.1
• Multiplied by PDOP (1-6)
• Total error ~ 6.1 - 36.6 meters
Meters
Atmosphere
Receivers
Orbit Error
Satellite
Clocks
0 6 12 18 24 30
GPS: Error Correction
▪ Methods:
– Point Averaging
– Differential Correction
Point Averaging
▪ Point Averaging is one of the simplest ways to correct GPS
point locations
– Collect many GPS measurements at the same location and then
average them to get one point
– The averaged point should have greater accuracy than a single
point measurement
– Accuracy varies with this method but you should have a position
that is within 5 meters of its true location 95% of the time
Point Averaging
Averaged
Location
This figure shows a successive series of 3-D positions taken using a receiver kept at the same
location, and then averaged
Differential Correction
▪ Differential correction collects points using a receiver at a
known location (known as a base station) while you collect
points in the field at the same time (known as a rover
receiver)
▪ Any errors in a GPS signal are likely to be almost the same
among all receivers within ~ 300 miles of each other
~ 300 miles (~ 480 km) or less
Base station (known location) Rover receiver
Differential Correction
▪ The base station knows its own location
▪ It compares this location with its location at that moment obtained
using GPS satellites, and computes error
▪ This known error (difference in x and y coordinates) is applied to the
rover receiver (hand-held unit) at the same moment
Time GPS Lat GPS Long Lat. error Long. error
3:12.5
3:13.0
3:13.5
3:14.0
3:14.5
3:15.0
35.50
35.05
34.95
36.00
35.35
35.20
79.05
78.65
79.55
80.45
79.30
79.35
.5
.05
-.05
1.0
.35
.20
.5
-.35
.55
1.45
.30
.35
Example: Base Station File
Differential Correction
▪ GPS error when using differential correction:
1 – 3 meters
▪ There are two ways that differential correction can be
applied:
– Post-processing differential correction
▪ Does the error calculations after the rover has collected the points
▪ Requires downloading a base-station file
– Real-time differential correction
▪ Done in real time by receiving a broadcasted correction signal
▪ May require additional hardware
Applications
• Emergency/firefighter/police/ambulance dispatch
• Car & boat navigation
• Roadside assistance
• Business vehicle/fleet management
• Mineral/resource exploration
• Wildlife tracking
• Recreational (fishing, hunting, hiking, etc.)
• Ski patrol/medical staff location monitoring
Bibliography
▪ wikipedia.com
▪ gps.gov
▪ howstuffworks.com
▪ physics.org
▪ explainthatstuff.com
Thank you

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Global Positioning System

  • 1. Global Positioning System Presented by: Prantik Chowdhury Dept. of Mechanical Engineering 3rdYear, B/1, 1457082.
  • 2. Contents: ▪ Basics ▪ History ▪ Satellites ▪ Receivers ▪ Ground Stations ▪ Working ▪ Errors ▪ Error Correction ▪ Applications
  • 3. Basics ▪ GPS stands forGlobal Positioning System which measures 3-D locations on Earth surface using satellites ▪ GPS operates using radio signals sent from satellites orbiting the earth ▪ Created and Maintained by the US Dept. of Defense ▪ System as a whole consists of three segments – Satellites (space segment) – Receivers (user segment) – Ground stations (control segment)
  • 4. History ▪ Development began in 1973 ▪ First satellite became operational in 1978 ▪ Declared completely functional in 1995 ▪ A total of 52 satellites have been launched in 4 phases ▪ 30 satellites are currently functional ▪ Managed by the U.S. Department of Defense – Originally developed for submarines – Now part of modern “smart bombs” and highly accurate missiles
  • 5. Satellites ▪ At least 4 satellites are above the horizon anytime anywhere ▪ GPS satellites are also known as “NAVSTAR satellites” ▪ The satellites transmit time according to very accurate atomic clocks onboard each one ▪ The precise positions of satellites are known to the GPS receivers from a GPS almanac A visual example of a 24 satellite GPS constellation in motion with the earth rotating. Notice how the number of satellites in view from a given point on the earth's surface, in this example in Golden CO (39.7469° N, 105.2108° W), changes with time.
  • 6. Satellites(Contd.) ▪ The satellites are in motion around the earth ▪ Like the sun and moon satellites rise and set as they cross the sky ▪ Locations on earth are determined from available satellites (i.e., those above the horizon) at the time the GPS data are collected
  • 7. Receivers ▪ Ground-based devices read and interpret the radio signals from several of the NAVSTAR satellites at once ▪ Geographic position is determined using the time it takes signals from the satellites to reach the GPS receiver ▪ Calculations result in varying degrees of accuracy that depend on: – Quality of the receiver – User operation of the receiver (e.g., skill of user and receiver settings) – Atmospheric conditions – Local conditions (i.e., objects that block or reflect the signals) – Current status of system A handheld GPS receiver.
  • 8. Ground Stations ▪ Control stations – Master station at Falcon (Schriever)AFB, Colorado – 4 additional monitoring stations distributed around the world ▪ Responsibilities – Monitor satellite orbits & clocks – Broadcast orbital data and clock corrections to satellites Map from P. Dana,The Geographer's Craft Project, Dept. of Geography, U.Texas-Austin.
  • 9. How GPS Works: Overview ▪ Satellites have accurate atomic clocks onboard and all GPS satellites transmit the same time signal at the same time – Think “synchronize your watches” ▪ The satellite signals contain information that includes – Satellite number – Time of transmission
  • 10. How GPS Works: Overview ▪ Receivers use an almanac that includes – The position of all satellites every second – This is updated monthly from control stations ▪ The satellite signal is received, compared with the receiver’s internal clock, and used to calculate the distance from that satellite ▪ Trilateration (similar to triangulation) is used to determine location from multiple satellite signals
  • 11. How GPS Works: Signal Processing ▪ Distances between satellites and receivers is determined by the time is takes the signal to travel from satellite to receiver – Radio signals travel at speed of light (186,000 miles/second) – All satellites send the identical time, which is also generated by the receivers – Signal travel time = offset between the satellite signal and the receiver signal – Distance from each satellite to receiver = signal travel time * 186,000 miles/second 1sec Receiver signal Satellite signal
  • 12. How GPS Works: Trilateration
  • 13. How GPS Works: Trilateration ▪ Start by determining distance between a GPS satellite and your position ▪ Adding more distance measurements to satellites narrows down your possible positions ▪ The 4th satellite in trilateration is to resolve any signal timing error – UnlikeGPS satellites, GPS receivers do not contain an atomic clock – To make sure the internal clock in the receiver is set correctly we use the signal from the 4th satellite
  • 14. Errors ▪ Satellite errors: Satellite position error (i.e., satellite not exactly where it’s supposed to be) Atomic clocks, though very accurate, are not perfect ▪ Atmospheric Electro-magnetic waves travel at light speed only in a vacuum Atmospheric molecules, particularly those in the ionosphere, change the signal speed
  • 15. Errors(Contd.) ▪ Multi-path distortion The signal may "bounce" off structures before reaching the GPS receiver – the reflected signal arrives a little later ▪ Receiver error Due to the receiver clock or internal noise ▪ Selective Availability No longer an issue
  • 16. Sources of Errors ▪ Satellite Clock & Satellite Position • Atomic clock errors +/- 2 meters of error • Satellite is not in precise orbit +/- 2.5 meters of error
  • 17. Sources of Errors(Contd.) ▪ Atmospheric Delays/Bending – +/- 5 meters or error
  • 18. Sources of Errors(Contd.) ▪ Multi Path Interference (signal bouncing off of buildings, trees, etc.) – +/- 1 meter of error
  • 19. Sources of Errors(Contd.) ▪ ReceiverTiming/Rounding Errors – +/- 1 meter of error (depends on the quality of the GPS receiver)
  • 20. GPS - Selective Availability ▪ A former significant source of error – Error intentionally introduced into the satellite signal by the U.S. Dept. of Defense for national security reasons – Selective Availability turned off early May 2, 2000
  • 21. GPS Error: Position Dilution of Precision ▪ Satellite Coverage: Position Dilution of Precision (PDOP) ▪ Remember that satellites are moving, causing the satellite constellation to change ▪ Some configurations of satellites are better than others ▪ PDOP values range from 1 to 50, with values < 6 considered “good” Poor PDOP Good PDOP
  • 22. GPS: Error Budget ▪ Example of typically observed error from a consumerGPS receiver: • Typical Observed errors (meters) satellite clocks 0.6 orbit (position error) 0.6 receiver errors 1.2 atmosphere 3.7 • Total 6.1 • Multiplied by PDOP (1-6) • Total error ~ 6.1 - 36.6 meters Meters Atmosphere Receivers Orbit Error Satellite Clocks 0 6 12 18 24 30
  • 23. GPS: Error Correction ▪ Methods: – Point Averaging – Differential Correction
  • 24. Point Averaging ▪ Point Averaging is one of the simplest ways to correct GPS point locations – Collect many GPS measurements at the same location and then average them to get one point – The averaged point should have greater accuracy than a single point measurement – Accuracy varies with this method but you should have a position that is within 5 meters of its true location 95% of the time
  • 25. Point Averaging Averaged Location This figure shows a successive series of 3-D positions taken using a receiver kept at the same location, and then averaged
  • 26. Differential Correction ▪ Differential correction collects points using a receiver at a known location (known as a base station) while you collect points in the field at the same time (known as a rover receiver) ▪ Any errors in a GPS signal are likely to be almost the same among all receivers within ~ 300 miles of each other ~ 300 miles (~ 480 km) or less Base station (known location) Rover receiver
  • 27. Differential Correction ▪ The base station knows its own location ▪ It compares this location with its location at that moment obtained using GPS satellites, and computes error ▪ This known error (difference in x and y coordinates) is applied to the rover receiver (hand-held unit) at the same moment Time GPS Lat GPS Long Lat. error Long. error 3:12.5 3:13.0 3:13.5 3:14.0 3:14.5 3:15.0 35.50 35.05 34.95 36.00 35.35 35.20 79.05 78.65 79.55 80.45 79.30 79.35 .5 .05 -.05 1.0 .35 .20 .5 -.35 .55 1.45 .30 .35 Example: Base Station File
  • 28. Differential Correction ▪ GPS error when using differential correction: 1 – 3 meters ▪ There are two ways that differential correction can be applied: – Post-processing differential correction ▪ Does the error calculations after the rover has collected the points ▪ Requires downloading a base-station file – Real-time differential correction ▪ Done in real time by receiving a broadcasted correction signal ▪ May require additional hardware
  • 29. Applications • Emergency/firefighter/police/ambulance dispatch • Car & boat navigation • Roadside assistance • Business vehicle/fleet management • Mineral/resource exploration • Wildlife tracking • Recreational (fishing, hunting, hiking, etc.) • Ski patrol/medical staff location monitoring
  • 30. Bibliography ▪ wikipedia.com ▪ gps.gov ▪ howstuffworks.com ▪ physics.org ▪ explainthatstuff.com