5. Missile Approach Warning Systems – the Infrared vs. Ultraviolet Debate Geoff Van Hees

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This document explains the difference between IR MAWS and UV MAWS

Transcript of 5. Missile Approach Warning Systems – the Infrared vs. Ultraviolet Debate Geoff Van Hees

  • Missile Approach WarningThe Infrared vs Ultraviolet Debate

    Geoff van Hees

    10 March 2014

    EW Asia 2014, The Prince Hotel, Kuala Lumpur

  • What is a Missile Approach WarningSensor?

    Purpose: To detect IR-guided missiles that pose

    a threat to the platform

    Two approaches

    Active detection uses RF energy to illuminate environment and detect incoming threats.

    Passive/Optical detection relies on the signals emitted from the threat, typically from the missile motor

    plume.

    Two classes of passive detectors

    Ultraviolet Infrared

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  • Requirements for Optical MissileDetection

    Field of view

    Cover 360 in azimuth. Min 90 (preferably 180) in elevation.

    Number of Line Replaceable units, LRUs

    4 to 6 sensors for spherical coverage.

    Frame rate

    Frame rate of at least 10ms.

    Dwell time

    The higher the scan rate the shorter the dwell time Need staring arrays.

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  • Requirements for Optical MissileDetection

    Distance Estimation

    Needed for optimal counter-measure deployment. Passive systems provide an estimate of distance and

    time to impact, at best.

    All-weather operation

    Rain, fog, condensation and icing should not significantly affect the operation of the sensors.

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  • IR vs UVWavelength Choice

    IR Two traditional Wavelengths

    3-5 Band CO2 absorption limits useful bandwidth.

    8-12 Band Number of problems. Wavelength related pixel size requires large detector

    arrays and optics of impractically large size.

    High false alarm rate.

    UV Solar blind

    Technical challenge to create. Circumvents limiting factors of IR. Low false alarm rate from background radiation.

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  • IR vs UVPixel Resolution

    IR Needs High Resolution detector

    Cluttered background Surface to Air scenario. Clutter rejection is a major issue, increases

    exponentially in day light due to solar illumination.

    Possible with significant amounts of processing and tracking.

    UV Low resolution detector sufficient

    Solar Blind system no background radiation or reflections.

    Source below the ozone layer can be detected using a low resolution detector.

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  • IR vs UVDetection and Tracking

    IR Can track missile after motor burn-out

    Possible for air to air. Surface to air Low seeker head heat, background

    radiation. Dense, low-altitude atmosphere.

    UV Rocket motor must be burning

    Track initiated as soon as any energy is detected.

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  • IR vs UVSpectral Discrimination

    IR Two/Multi-Colour detection

    Needed to assist with suppression of background clutter.

    Measuring in two colours doubles the pixel count needed.

    Target smaller that 1 pixel, revert back to high-resolution with its attendant technical challenges

    UV Single-colour detection

    Few sources hot enough to radiate significant amounts of short-wavelength does include the threat to be

    detected.

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  • IR vs UVOptical Implications

    IR Physically large detectors to accommodate

    required pixel array

    Low optical image pixel image blurred reduced sensitivity and scene resolution.

    IR optical materials are expensive and fragile. Difficult to protect exposed large-aperture, wide-angle

    optics mounted outside of an aircraft in an operational

    environment.

    UV Extremely robust

    Optics made mostly from fused silica (quartz). Low resolution simple manufacturing process. Not necessary for high resolution across the FOV.

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  • IR vs UVCooling

    IR Cooled

    Need to reduce detector noise. Uncooled less sensitive. Cooling mechanical refrigeration or thermo-electrical. Increases power consumption, weight, complexity and

    life-cycle costs.

    Decreases system reliability.

    UV- Uncooled

    No cooling needed. Thermal noise does not approach the high energy of

    the UV photons that are detected.

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  • IR vs UVData Rates

    IR WOW!

    Assumption Large area IR detector that can read out the required frame rate and the resultant data rates can

    be computed.

    Readout of four 2-colour 16000 x 16000 pixel detectors at 100Hz and 12 bits per pixel 2.4 trillion bits per

    second Not currently practical for a cost-effective

    airborne or mobile application.

    UV No WOW factor

    Effective data rate of a UV system is at least 5 orders of magnitude lower than an IR system.

    Lower spatial resolution, bit depth and single colourspectral resolution.

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  • IR vs UVComparison

    IR Band

    Physical constraints You cant argue with physics. All weather operation not practical. Solar radiation saturates and blinds sensors impacts

    POW.

    High cost and complexity vs reduced reliability and performance.

    UV Band

    Solar blind phenomenon removes need for high detector resolution and large dynamic range.

    All weather capability not affected by water or moisture in the atmosphere.

    Significantly cheaper and more durable.PAGE 12

  • Conclusion

    IR technology delivers excellent results when its

    strengths are correctly exploited, it is not suitable

    as a missile warning application against surface

    launched missiles in the real world, all-weather

    scenario.

    Has advantages over UV in the air to air

    scenario based on ability for longer detection

    range and ability to track a missile after the

    motor has burnt out.

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