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               Directed Infrared Countermeasures (DIRCM) Principles



                                         Instructor:

                                     John L. Minor




ATI Course Schedule:   http://www.ATIcourses.com/schedule.htm
ATI's DIRCM:     http://www.aticourses.comDirected_Infrared_Countermeasures_DIRCM_Principles.htm
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Course Overview

               0.            Intro, Administrative, and Course Overview
               1.            Electromagnetic Spectrum & Infrared Fundamentals
               2.            The Infrared Threat
               3.            Missile Warning Receivers
               4.            Aircraft Signatures
               5.            Infrared Missile System Principles
               6.            DIRCM Systems
                          –             Increasing J/S Requirement
                          –             Legacy DIRCM (Broadband and Flash Lamp) Systems
                          –             Laser Jam (Closed Loop) DIRCM Systems
               7. Test and Evaluation of DIRCM Systems
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
End of Module 0




                                                                   QUESTIONS?
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Next Up

           1. Electromagnetic Spectrum & Infrared Fundamentals




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Module 1
                                                 The Electromagnetic Spectrum
                                                      & IR Fundamentals




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Course Overview
        1.            Electromagnetic Spectrum & Infrared Fundamentals
        2.            The Infrared Threat
        3.            Missile Warning Receivers
        4.            Aircraft Signatures
        5.            Infrared Missile System Principles
        6.            DIRCM Systems
                   –             Increasing J/S Requirement
                   –             Legacy DIRCM (Broadband and Flash Lamp) Systems
                   –             Laser Jam (Closed Loop) DIRCM Systems
        7. Test and Evaluation of DIRCM Systems

© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Module 1 Overview

                     •         Electromagnetic (EM) Wave Basics
                     •         Properties of EM Waves and Light
                     •         Regions of Interest in the EM Spectrum
                     •         Infrared Basics
                     •         Blackbody Radiation Physics and Terminology




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Propagation of Light as EM Waves




•         ALL Electromagnetic radiation consists of an electric (E) field and a magnetic (H) field
•         The wave propagates at the speed of light, at right angles to the E/H field planes
•         If you cross the E Field vector with the H Field vector, you get the direction of travel of the EM
          wave (known as the right hand rule)



© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
The Speed of Light




• Light, like all electromagnetic waves, travels at the same fixed
  velocity (in a vacuum)  186,000 miles/second = 3 X 108 meters/second

• C = the speed light = 3 X 108 meters/second


• C = f or you can always remember the 2 Greeks >> C =                                 
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
EM Wave Terminology




    • The amplitude is related to the intensity of the light in Volts/Meter.
    • The period (T) is the time between crests of the wave in seconds.
    • The wavelength ( ) is the physical distance between wave crests
    • The frequency (or f ) is the inverse of the period, and vice-versa.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Polarization
                                                                                Direction of E field determines the
                                                                            E   polarization of an EM wave.

                                                                                With E field in vertical direction
                                                                                wave is said to be vertically polarized

                                                                                Direction of travel by the right hand
                                                                                rule crossing the E vector into the H
                                                                                vector


                                           H
                                                                   Horizontal                   Circular
                                                                                                        Can be right or left
             E                                                                                          hand circularly
                                                                                                        polarized




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
EM Wave Polarization Video




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Diffraction




• When light passes through a narrow opening, it tends to spread out
  as if the opening itself were a very small point source of light

•The bending of light when it passes through a narrow opening or
 along the edge of a barrier is known as diffraction

Note: Diffraction limits the resolution of an optical system

© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
The Electromagnetic Spectrum




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Optical Band of the
                                                                   Electromagnetic Spectrum




                                                                                                                 ROYGBV


            Optical frequencies, or light can be both visible and invisible to the unaided eye
            Note: Boundaries, UV, & IR Band Nomenclature are somewhat arbitrary and are
            author/text dependent

© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.           Red, orange, yellow, green, blue, violet
Electromagnetic Spectrum Charts (cont.)




                                                                                                                       This is the
                                                                                                                       IR Threat




                                                X-Band Radar                               Older IR   Modern         FLIR
                                                10 GHz, 3 cm       UV MWS       NVG        Missiles   IR Missile   3-5, 8-12
                                                                   0.1-0.4   (0.65-0.95)   Near IR    Threat
                                                                                                      3-5
          EO Wavelengths shown in microns (m)                               CCD TV
                                                                             0.55-0.95


© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Diffraction Limited Resolution




                                                                     ~ 1.22 
                                                                   R D
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Phase Angle Properties




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Interference Properties of Light

                                                                   • When two or more light waves meet
                                                                   at the same place and time, their
                                                                   amplitudes will add by the principle of
                                                                   superposition

                                                                   • If crests meet crests they add
                                                                   together to produce a larger amplitude
                                                                   and this is constructive interference

                                                                   • If crests meet with troughs they add
                                                                   together to produce a smaller
                                                                   amplitude and this in know as
                                                                   destructive interference




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
The Interaction of Light With Matter

      When light (EM energy) strikes the boundary of some type of matter,
      three things can happen:
                                                                                                                               3


1                                                                    Medium 1           Medium 2                        2
                                 Boundary between two different media such as air/glass or air/water
1. REFLECTION -                                                    Radiation is turned back into the first medium ()

2. REFRACTION -                                                    Radiation is passed or transmitted into the second media
                                                                   (also called transmission). If the index of refraction is
                                                                   different between the two medium, the light will be bent
                                                                   or refracted () according to Snell’s Law

3. ABSORPTION -                                                    Process in which the energy of the incident photons are
                                                                   absorbed and changed into molecular energy & heat ( )

                                           Note: The sum of these three coefficients ( must = 1
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
The Discovery of Infrared
                                                                       On 11 February 1800, Sir William Herschel was
                                                                       testing filters for viewing the sun so he could observe
                                                                       sun spots

                                                                       When using a red filter he found there was a lot of
                                                                       heat produced

                                                                       Herschel discovered infrared radiation by passing
                                                                       sunlight through a prism and holding a thermometer
                                                                       just beyond the red end of the visible spectrum

                                                                       This thermometer was meant to be a control to
                                                                       measure the ambient air temperature in the room

                                                                       He was shocked when it showed a higher
                                                                       temperature than the visible spectrum

                                                                       Further experimentation led to Herschel's conclusion
                                                                       that there must be an invisible form of light beyond
                                                                       the visible spectrum.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
The Infrared Spectrum
       When we speak of infrared, we mean that portion of the electromagnetic
       spectrum that lies between visible light on one side and microwaves on the
       other. Quantitatively, is is expressed as the region extending from a
       wavelength of ~ 0.7 microns to ~1000 microns




                                                                                       ~0.7-1000 microns



                                                                             IR




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Radiometry
                                                                                    • A source at the origin radiates
                                                                                      optical power such that P0 is
                                                                                      radiated into a cone as shown
                                                                               A2   • Other powers may be radiated in
                                                                                      other directions.
                                                                   R1    A1
                                                                        P0          • For the first cone, the power per
                                                                              R2      unit area at a distance R1 away is…
                                                                                        P0/A1
                                                                                        and is called the “Irradiance”
                                                                                    • The Irradiance at distance R2 is
                                                                                        P0/A2

             • Since the illuminated area increases as the square of R, i.e. A2/A1=(R2/R1)2,
               in a non-absorbing medium the Irradiance produced by the source varies
               as inverse R-squared.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Radiometry (cont.)


                                                                                    • Irradiance is given the symbol “E”
                                                                                      and is expressed in the units W/cm2.
                                                                               A2   • Missiles care about the quantity
                                                                                      “Irradiance” because the power
                                                                   R1    A1           they receive Pr is determined by
                                                                        P0            that value and by the missiles’s
                                                                              R2      collection area Am. That is…
                                                                                      Pr2=E2 x Am =(P0/A2) x Am
                                                                                      is the power the missile receives
                                                                                      when it is at the range R2



             • Since the Irradiance increases as the inverse-square of R, the missile
               receives greater and greater power as it flies toward the source.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Radiometry (cont.)
                                                                                    • The angular region contained in the
                                                                                      cone is called the “solid angle” of the
                                                                               A2     cone,  and is given by

                                                                   R1    A1
                                                                                      =A/R2.
                                                                        P0
                                                                                    • This definition is true for any arbitrary
                                                                              R2      angular region which can differ from
                                                                                      that of a cone.
                                                                                    • Since the illuminated area varies as R-
                                                                                      squared, the solid angle of the
                                                                                      illuminated region does not change
                                                                                      with range.

             • A radiometric quantity called “Radiant Intensity” has been defined and is
               calculated using the expression P/.. Since the power P0 uniformly fills
               the solid angle region, in a non-absorbing medium, the Radiant Intensity
               does not vary with range.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Radiometry (cont.)
                                                                                      • Radiant intensity is given the
                                                                                        symbol “I” and is expressed in the
                                                                                        units W/sr.
                                                                                      • IRCM engineers care about the
                                                                               A2       quantity “Radiant Intensity”
                                                                                        because that value describes the
                                                                   R1                   strength of target and jammer
                                                                         A1
                                                                        P0              sources without specifying range *
                                                                              R2      • Irradiance can be found from
                                                                                        Radiant Intensity by dividing by
                                                                                        the range-squared. That is…
                                                                                           E2=I/(R2)2
                                                                                           Is the Irradiance produced at a
                                                                                           range R2 by a source of Radiant
                                                                                           Intensity “I”.

                                                                                    * This is true for a non-absorbing medium.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Radiometry (cont.)
               • Aircraft targets and jamming transmitters are optical sources whose
                 radiation strengths may be expressed in terms of Radiant Intensity or
                 Irradiance.
               • Whatever radiometric quantity is used, IRCM engineers refer to the
                 aircraft radiation strength as “S” for signature, and to the Jammer
                 strength as “J”. The IRCM system’s J/S is then determined as the
                 ratio.
               • Since aircraft and jamming systems can radiate different amounts in
                 different directions, the apparent values of S, of J, and of J/S, can vary
                 with the observer’s viewing perspective.
               • As an example, a fixed-wing aircraft signature may be 1000 W/sr at a
                 tail perspective where aircraft engines are unobscured, but may be
                 only 100 W/sr when viewed nose-on.
               • Since the atmosphere will typically remove power from any radiating
                 cone through absorption, values of J and S may change with range
                 beyond the standard R-squared multiplier.
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
RADIOMETRIC UNITS
                                                                   Watts
• The watt is the fundamental unit of optical power and
measurement, and is defined as a rate of energy of one
joule per second

• It is a function of both the number of photons and the
wavelength of the photons

• Each photon carries an energy = h = hc/
                         where h = Planck’s constant = 6.623 x 10 -34 Joule-sec
                               c = speed of light = 3 x 10 8 meters / sec
                                wavelength of the photons



© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Radiator Response Curves

                                                                                     Emissivity () = 1 (black body at 300° 
                                                (Watt/cm3 - micron)
                                                                                      = 0.9 (gray body)
                                                                                          = varies as wavelength
                              Energy Density
                              Monochromatic




                                                                                                (Selective Radiator)




                                                                      0         10         20                  30       (m)

                    Need to specify the  for the spectral band of interest
                          • Usually specified as an average  over a given spectral band
                          • For example:  = 0.3avg at 8-12 microns


© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Important Laws of Radiation

                                                  • Inverse Square Law

                                                  • Lambert’ s Cosine Law

                                                  • Stefan-Boltzman’s Law

                                                  • Wien’s Law

                                                  • Planck’s Law



© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Inverse Square Law
Defines the relationship between the irradiance (illuminance) from
a point source and the distance to it




                                                                            The intensity per unit
                                                                            area varies in inverse
                                                                            proportion to the square
                                                                            of the distance -- why?


© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Inverse Square Law
                                                                   Inverse Square Law & Divergence




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Stefan-Boltzman’s Law
                                                         (Thermal Radiation Law)
                                                                   The amount of radiation emitted by a body is
                                                                   proportional to the emissivity and to the fourth
                                                                   power of the absolute temperature of the body


                                                                                                       4
                                                                                W          T
                                                                          =     Stefan Boltzman’s Constant
                                                                                                 W
                                                                                  5.670 x 10-8
                                                                                               cm2 k4
                                                                          =      Emissivity

                                                                          T=      Temperature (absolute)
         Note that if T is doubled, the
                                                                                  FOR A BLACKBODY
         radiated emittance is
         increased sixteen times                                                           = 1.0
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Wien’s Displacement Law
                                                                   The wavelength at which the maximum radiance
                                                                   occurs is inversely proportional to the absolute
                                                                   temperature of the body (Kelvin):




                                                                          9.6m    max    2900/T microns

                                         300




                                                                          8   12




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Planck’s Law

                   • In physics, Planck's law describes the spectral radiance of
                     electromagnetic radiation at all wavelengths from a black
                     body at temperature T. As a function of frequency ν,
                     Planck's law is written as:




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Planck’s Law

                                                                          Weins Law
                                                                                                               Solar
                                                                          All bodies emit radiation at all
                                                                                  wavelengths as
                                                                         a function of the bodies absolute
                                                                                   temperature
                                                                                                             Rocket
                                                                                                             Exhaust

                                                                                                             Jet Engine
                                                                                                              Exhaust
                                                                                                               Earth
                                                                                                             (terrain)



© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Lambert’s (Cosine) Law
• The irradiance or the
illuminance falling on any
surface varies as the cosine
of the incident angle

• Maximum at 90 degrees to
the surface (shown as 0
degrees here)

The perceived measurement
area orthogonal to the incident
flux is reduced at oblique
angles causing the light to
spread out over a wider area
than it would if perpendicular
to the measurement plane


© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
IRCM Terminology




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Common IRCM Terms

                          •         IR spectrum                             •   Open loop IRCM
                          •         Band pass                               •   Closed loop IRCM
                          •         Radiant intensity                       •   Optical break lock
                          •         Watts per steradian                     •   Guidance suppression
                          •         Watts per cm2                           •   J/S ratio
                          •         IR signature




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Module 1

                                                                   Questions?




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Next Up
        1.            Electromagnetic Spectrum & Infrared Fundamentals
        2.            The Infrared Threat
        3.            Missile Warning Receivers
        4.            Aircraft Signatures
        5.            Infrared Missile System Principles
        6.            DIRCM Systems
                   –             Increasing J/S Requirement
                   –             Legacy DIRCM (Broadband and Flash Lamp) Systems
                   –             Laser Jam (Closed Loop) DIRCM Systems
        7. Test and Evaluation of DIRCM Systems

© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Module 5



                                                      Infrared Missile Systems




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Course Overview

               0.            Intro, Administrative, and Course Overview
               1.            Electromagnetic Spectrum & Infrared Fundamentals
               2.            The Infrared Threat
               3.            Missile Warning Receivers
               4.            Aircraft Signatures
               5.            Infrared Missile System Principles
               6.            DIRCM Systems
               –             Increasing J/S Requirement
               –             Legacy DIRCM (Broadband and Flash Lamp) Systems
               –             Laser Jam (Closed Loop) DIRCM Systems
               7. Test and Evaluation of DIRCM Systems
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Module 5 Overview


              •        How IR Missiles Work
              •        Video – Basics of How IR Missiles Work
              •        Threat Development Timeline & History
              •        Missile Guidance Basics
              •        Intro to IRCM Basics to Defeat IR Missiles




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
IR Missile Guidance Loop Description
                                                                   Detector




                                                                                                                    Steering Commands
                                                                                                          Spin             To Fins
                                                                                      Carrier
                                                                                 AMP Band Pass Envelope Band Pass
                                                                                                                          Guidance
                                                                                                                         Processing



                                                                    Precession



                                                                         Pointing Commands To Seeker Gyro




                                                 Reticle, Mirror/Gyro

                                                 MODULATION                                       • Tracks small targets (points sources)
                                                                                                  more efficiently than large sources

                                                                                                  • Has problems with extended sharply
                                                                                                  defined edges (horizon line)
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
IR Missile Threat Evolution




© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Threat Development Timeline vs. Band


         1960s                              1970s                  1970/80s        1980s           1990s
                                                                                                           2000
                                                                                                               Scanning
                                                                                                               Imagers

                                                                    Cooled                     Pseudo-
     Spin Scan                           Con Scan                                 FRCCM
                                                                    Seeker                     Imagers
                                                                                                           2005

                             reticle-based seekers
                                                                                                                1st Gen
                                                                                                            Staring Imagers
                                                                                              Stgr-POST
         SA-7                                                       SA-14
                                            Redeye                               Stgr-BASIC   SA-18
         HN-5                                                       SA-16
                                                                                              Mistral
                                                                                                           2010

   Band I                                Band II                                    Band IV
                                                                                                               2nd Gen
 (hot metal)                           (hot metal)                            (jet engine plume)            Spectral Imagers



© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Rosette

                                                                                                  Detector IFOV

     • Pseudo Imaging
     • Small Field-of-View Detector                                         Target
                                                                                                     Petal

       Scanning a Rosette Pattern Using                                     Image

       Two-Counter-Rotating Optical
                                                                             A Rosette Scanning Pattern
       Elements
     • Small IFOV
                 –     Provides Greater Sensitivity
                                                                            Petal Scan
                 –     Resistant to Jammers                          S(t)     Time
                 –     Resistant to False Targets                      1


                                                                       0                                          t
                                                                                 Normalized Signal Pulse
                                                                               Sequence for On-Axis Image
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Imaging

                              • Produces an Image
                              • Takes Advantage of State-of-the-Art Technology
                                          – Processing Capability
                                          – Software Track Algorithms
                                                                                                         Rectangular Detector Arrays
                                          Linear Detector Array




                                                                                                                 Target Scene
                                                                                                                    Image
                                                                         Target Scene


                                 Linear Detector Array Scanning                         Rectangular Detector Array
                                        of a Target Scene                                   and Target Scene

                                                                   Illustration of Imaging Detectors
© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Flare Decoy

        Objective: Present a more attractive
        IR target to the missile
      • Shortcomings
                  -Flares operate at higher
                  temperatures than aircraft, emitting
                  primarily in Bands 1 & 2 (versus
                  modern Band 4 threats)
                  -Very effective against Band 1 & 2
                  (1st and 2nd Generation) missiles
                  -Limited performance against newer
                  Band 4 missiles due to output
                  energy limitations and inclusion of
                  flare CCM techniques in missile
                  design

© Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
Directed Infrared Countermeasures (DIRCM) Principles

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Directed Infrared Countermeasures (DIRCM) Principles

  • 1. Slides From ATI Professional Development Short Course Directed Infrared Countermeasures (DIRCM) Principles Instructor: John L. Minor ATI Course Schedule: http://www.ATIcourses.com/schedule.htm ATI's DIRCM: http://www.aticourses.comDirected_Infrared_Countermeasures_DIRCM_Principles.htm
  • 2. www.ATIcourses.com Boost Your Skills 349 Berkshire Drive Riva, Maryland 21140 with On-Site Courses Telephone 1-888-501-2100 / (410) 965-8805 Tailored to Your Needs Fax (410) 956-5785 Email: ATI@ATIcourses.com The Applied Technology Institute specializes in training programs for technical professionals. Our courses keep you current in the state-of-the-art technology that is essential to keep your company on the cutting edge in today’s highly competitive marketplace. Since 1984, ATI has earned the trust of training departments nationwide, and has presented on-site training at the major Navy, Air Force and NASA centers, and for a large number of contractors. Our training increases effectiveness and productivity. Learn from the proven best. For a Free On-Site Quote Visit Us At: http://www.ATIcourses.com/free_onsite_quote.asp For Our Current Public Course Schedule Go To: http://www.ATIcourses.com/schedule.htm
  • 3. Course Overview 0. Intro, Administrative, and Course Overview 1. Electromagnetic Spectrum & Infrared Fundamentals 2. The Infrared Threat 3. Missile Warning Receivers 4. Aircraft Signatures 5. Infrared Missile System Principles 6. DIRCM Systems – Increasing J/S Requirement – Legacy DIRCM (Broadband and Flash Lamp) Systems – Laser Jam (Closed Loop) DIRCM Systems 7. Test and Evaluation of DIRCM Systems © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 4. End of Module 0 QUESTIONS? © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 5. Next Up 1. Electromagnetic Spectrum & Infrared Fundamentals © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 6. Module 1 The Electromagnetic Spectrum & IR Fundamentals © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 7. Course Overview 1. Electromagnetic Spectrum & Infrared Fundamentals 2. The Infrared Threat 3. Missile Warning Receivers 4. Aircraft Signatures 5. Infrared Missile System Principles 6. DIRCM Systems – Increasing J/S Requirement – Legacy DIRCM (Broadband and Flash Lamp) Systems – Laser Jam (Closed Loop) DIRCM Systems 7. Test and Evaluation of DIRCM Systems © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 8. Module 1 Overview • Electromagnetic (EM) Wave Basics • Properties of EM Waves and Light • Regions of Interest in the EM Spectrum • Infrared Basics • Blackbody Radiation Physics and Terminology © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 9. Propagation of Light as EM Waves • ALL Electromagnetic radiation consists of an electric (E) field and a magnetic (H) field • The wave propagates at the speed of light, at right angles to the E/H field planes • If you cross the E Field vector with the H Field vector, you get the direction of travel of the EM wave (known as the right hand rule) © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 10. The Speed of Light • Light, like all electromagnetic waves, travels at the same fixed velocity (in a vacuum)  186,000 miles/second = 3 X 108 meters/second • C = the speed light = 3 X 108 meters/second • C = f or you can always remember the 2 Greeks >> C =  © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 11. EM Wave Terminology • The amplitude is related to the intensity of the light in Volts/Meter. • The period (T) is the time between crests of the wave in seconds. • The wavelength ( ) is the physical distance between wave crests • The frequency (or f ) is the inverse of the period, and vice-versa. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 12. Polarization Direction of E field determines the E polarization of an EM wave. With E field in vertical direction wave is said to be vertically polarized Direction of travel by the right hand rule crossing the E vector into the H vector H Horizontal Circular Can be right or left E hand circularly polarized © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 13. EM Wave Polarization Video © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 14. Diffraction • When light passes through a narrow opening, it tends to spread out as if the opening itself were a very small point source of light •The bending of light when it passes through a narrow opening or along the edge of a barrier is known as diffraction Note: Diffraction limits the resolution of an optical system © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 15. The Electromagnetic Spectrum © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 16. Optical Band of the Electromagnetic Spectrum ROYGBV Optical frequencies, or light can be both visible and invisible to the unaided eye Note: Boundaries, UV, & IR Band Nomenclature are somewhat arbitrary and are author/text dependent © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC. Red, orange, yellow, green, blue, violet
  • 17. Electromagnetic Spectrum Charts (cont.) This is the IR Threat X-Band Radar Older IR Modern FLIR 10 GHz, 3 cm UV MWS NVG Missiles IR Missile 3-5, 8-12 0.1-0.4 (0.65-0.95) Near IR Threat 3-5 EO Wavelengths shown in microns (m) CCD TV 0.55-0.95 © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 18. Diffraction Limited Resolution ~ 1.22  R D © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 19. Phase Angle Properties © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 20. Interference Properties of Light • When two or more light waves meet at the same place and time, their amplitudes will add by the principle of superposition • If crests meet crests they add together to produce a larger amplitude and this is constructive interference • If crests meet with troughs they add together to produce a smaller amplitude and this in know as destructive interference © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 21. The Interaction of Light With Matter When light (EM energy) strikes the boundary of some type of matter, three things can happen: 3 1 Medium 1 Medium 2 2 Boundary between two different media such as air/glass or air/water 1. REFLECTION - Radiation is turned back into the first medium () 2. REFRACTION - Radiation is passed or transmitted into the second media (also called transmission). If the index of refraction is different between the two medium, the light will be bent or refracted () according to Snell’s Law 3. ABSORPTION - Process in which the energy of the incident photons are absorbed and changed into molecular energy & heat ( ) Note: The sum of these three coefficients ( must = 1 © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 22. The Discovery of Infrared On 11 February 1800, Sir William Herschel was testing filters for viewing the sun so he could observe sun spots When using a red filter he found there was a lot of heat produced Herschel discovered infrared radiation by passing sunlight through a prism and holding a thermometer just beyond the red end of the visible spectrum This thermometer was meant to be a control to measure the ambient air temperature in the room He was shocked when it showed a higher temperature than the visible spectrum Further experimentation led to Herschel's conclusion that there must be an invisible form of light beyond the visible spectrum. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 23. The Infrared Spectrum When we speak of infrared, we mean that portion of the electromagnetic spectrum that lies between visible light on one side and microwaves on the other. Quantitatively, is is expressed as the region extending from a wavelength of ~ 0.7 microns to ~1000 microns ~0.7-1000 microns IR © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 24. Radiometry • A source at the origin radiates optical power such that P0 is radiated into a cone as shown A2 • Other powers may be radiated in other directions. R1 A1 P0 • For the first cone, the power per R2 unit area at a distance R1 away is… P0/A1 and is called the “Irradiance” • The Irradiance at distance R2 is P0/A2 • Since the illuminated area increases as the square of R, i.e. A2/A1=(R2/R1)2, in a non-absorbing medium the Irradiance produced by the source varies as inverse R-squared. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 25. Radiometry (cont.) • Irradiance is given the symbol “E” and is expressed in the units W/cm2. A2 • Missiles care about the quantity “Irradiance” because the power R1 A1 they receive Pr is determined by P0 that value and by the missiles’s R2 collection area Am. That is… Pr2=E2 x Am =(P0/A2) x Am is the power the missile receives when it is at the range R2 • Since the Irradiance increases as the inverse-square of R, the missile receives greater and greater power as it flies toward the source. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 26. Radiometry (cont.) • The angular region contained in the cone is called the “solid angle” of the A2 cone,  and is given by R1 A1 =A/R2. P0 • This definition is true for any arbitrary R2 angular region which can differ from that of a cone. • Since the illuminated area varies as R- squared, the solid angle of the illuminated region does not change with range. • A radiometric quantity called “Radiant Intensity” has been defined and is calculated using the expression P/.. Since the power P0 uniformly fills the solid angle region, in a non-absorbing medium, the Radiant Intensity does not vary with range. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 27. Radiometry (cont.) • Radiant intensity is given the symbol “I” and is expressed in the units W/sr. • IRCM engineers care about the A2 quantity “Radiant Intensity” because that value describes the R1 strength of target and jammer A1 P0 sources without specifying range * R2 • Irradiance can be found from Radiant Intensity by dividing by the range-squared. That is… E2=I/(R2)2 Is the Irradiance produced at a range R2 by a source of Radiant Intensity “I”. * This is true for a non-absorbing medium. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 28. Radiometry (cont.) • Aircraft targets and jamming transmitters are optical sources whose radiation strengths may be expressed in terms of Radiant Intensity or Irradiance. • Whatever radiometric quantity is used, IRCM engineers refer to the aircraft radiation strength as “S” for signature, and to the Jammer strength as “J”. The IRCM system’s J/S is then determined as the ratio. • Since aircraft and jamming systems can radiate different amounts in different directions, the apparent values of S, of J, and of J/S, can vary with the observer’s viewing perspective. • As an example, a fixed-wing aircraft signature may be 1000 W/sr at a tail perspective where aircraft engines are unobscured, but may be only 100 W/sr when viewed nose-on. • Since the atmosphere will typically remove power from any radiating cone through absorption, values of J and S may change with range beyond the standard R-squared multiplier. © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 29. RADIOMETRIC UNITS Watts • The watt is the fundamental unit of optical power and measurement, and is defined as a rate of energy of one joule per second • It is a function of both the number of photons and the wavelength of the photons • Each photon carries an energy = h = hc/ where h = Planck’s constant = 6.623 x 10 -34 Joule-sec c = speed of light = 3 x 10 8 meters / sec  wavelength of the photons © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 30. Radiator Response Curves Emissivity () = 1 (black body at 300°  (Watt/cm3 - micron)  = 0.9 (gray body)  = varies as wavelength Energy Density Monochromatic (Selective Radiator) 0 10 20 30  (m) Need to specify the  for the spectral band of interest • Usually specified as an average  over a given spectral band • For example:  = 0.3avg at 8-12 microns © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 31. Important Laws of Radiation • Inverse Square Law • Lambert’ s Cosine Law • Stefan-Boltzman’s Law • Wien’s Law • Planck’s Law © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 32. Inverse Square Law Defines the relationship between the irradiance (illuminance) from a point source and the distance to it The intensity per unit area varies in inverse proportion to the square of the distance -- why? © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 33. Inverse Square Law Inverse Square Law & Divergence © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 34. Stefan-Boltzman’s Law (Thermal Radiation Law) The amount of radiation emitted by a body is proportional to the emissivity and to the fourth power of the absolute temperature of the body 4 W T = Stefan Boltzman’s Constant W 5.670 x 10-8 cm2 k4 = Emissivity T= Temperature (absolute) Note that if T is doubled, the FOR A BLACKBODY radiated emittance is increased sixteen times  = 1.0 © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 35. Wien’s Displacement Law The wavelength at which the maximum radiance occurs is inversely proportional to the absolute temperature of the body (Kelvin): 9.6m max  2900/T microns 300 8 12 © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 36. Planck’s Law • In physics, Planck's law describes the spectral radiance of electromagnetic radiation at all wavelengths from a black body at temperature T. As a function of frequency ν, Planck's law is written as: © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 37. Planck’s Law Weins Law Solar All bodies emit radiation at all wavelengths as a function of the bodies absolute temperature Rocket Exhaust Jet Engine Exhaust Earth (terrain) © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 38. Lambert’s (Cosine) Law • The irradiance or the illuminance falling on any surface varies as the cosine of the incident angle • Maximum at 90 degrees to the surface (shown as 0 degrees here) The perceived measurement area orthogonal to the incident flux is reduced at oblique angles causing the light to spread out over a wider area than it would if perpendicular to the measurement plane © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 39. IRCM Terminology © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 40. Common IRCM Terms • IR spectrum • Open loop IRCM • Band pass • Closed loop IRCM • Radiant intensity • Optical break lock • Watts per steradian • Guidance suppression • Watts per cm2 • J/S ratio • IR signature © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 41. Module 1 Questions? © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 42. Next Up 1. Electromagnetic Spectrum & Infrared Fundamentals 2. The Infrared Threat 3. Missile Warning Receivers 4. Aircraft Signatures 5. Infrared Missile System Principles 6. DIRCM Systems – Increasing J/S Requirement – Legacy DIRCM (Broadband and Flash Lamp) Systems – Laser Jam (Closed Loop) DIRCM Systems 7. Test and Evaluation of DIRCM Systems © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 43. Module 5 Infrared Missile Systems © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 44. Course Overview 0. Intro, Administrative, and Course Overview 1. Electromagnetic Spectrum & Infrared Fundamentals 2. The Infrared Threat 3. Missile Warning Receivers 4. Aircraft Signatures 5. Infrared Missile System Principles 6. DIRCM Systems – Increasing J/S Requirement – Legacy DIRCM (Broadband and Flash Lamp) Systems – Laser Jam (Closed Loop) DIRCM Systems 7. Test and Evaluation of DIRCM Systems © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 45. Module 5 Overview • How IR Missiles Work • Video – Basics of How IR Missiles Work • Threat Development Timeline & History • Missile Guidance Basics • Intro to IRCM Basics to Defeat IR Missiles © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 46. IR Missile Guidance Loop Description Detector Steering Commands Spin To Fins Carrier AMP Band Pass Envelope Band Pass Guidance Processing Precession Pointing Commands To Seeker Gyro Reticle, Mirror/Gyro MODULATION • Tracks small targets (points sources) more efficiently than large sources • Has problems with extended sharply defined edges (horizon line) © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 47. IR Missile Threat Evolution © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 48. Threat Development Timeline vs. Band 1960s 1970s 1970/80s 1980s 1990s 2000 Scanning Imagers Cooled Pseudo- Spin Scan Con Scan FRCCM Seeker Imagers 2005 reticle-based seekers 1st Gen Staring Imagers Stgr-POST SA-7 SA-14 Redeye Stgr-BASIC SA-18 HN-5 SA-16 Mistral 2010 Band I Band II Band IV 2nd Gen (hot metal) (hot metal) (jet engine plume) Spectral Imagers © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 49. Rosette Detector IFOV • Pseudo Imaging • Small Field-of-View Detector Target Petal Scanning a Rosette Pattern Using Image Two-Counter-Rotating Optical A Rosette Scanning Pattern Elements • Small IFOV – Provides Greater Sensitivity Petal Scan – Resistant to Jammers S(t) Time – Resistant to False Targets 1 0 t Normalized Signal Pulse Sequence for On-Axis Image © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 50. Imaging • Produces an Image • Takes Advantage of State-of-the-Art Technology – Processing Capability – Software Track Algorithms Rectangular Detector Arrays Linear Detector Array Target Scene Image Target Scene Linear Detector Array Scanning Rectangular Detector Array of a Target Scene and Target Scene Illustration of Imaging Detectors © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.
  • 51. Flare Decoy Objective: Present a more attractive IR target to the missile • Shortcomings -Flares operate at higher temperatures than aircraft, emitting primarily in Bands 1 & 2 (versus modern Band 4 threats) -Very effective against Band 1 & 2 (1st and 2nd Generation) missiles -Limited performance against newer Band 4 missiles due to output energy limitations and inclusion of flare CCM techniques in missile design © Copyright 2010 by John L. Minor, American Eagle Aerospace LLC.