Electrophysics offers a complete line of high-performance infrared cameras, thermal imaging and night vision cameras. Our products include: image intensifier, IR thermal imaging, low light products and more.
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    Home > Infrared Cameras > Cooled Focal Plane Arrays
   Cooled Focal Plane Arrays
     Features
  • Highest Performance Cooled IR Detectors
  • High Sensitivity down to <10mK
  • High Resolution up to 1280x1024
  • Short-wave, Mid-wave, Long-wave
     
    Overview
    Our cooled detectors are made by our parent company, Sofradir SAS, located outside Grenoble, France.

    Sofradir SAS develops and manufactures advanced infrared detectors for military, space and commercial applications. The company specializes in cooled IR detectors based on a sophisticated high performance Mercury Cadmium Telluride (MCT) technology. Since the company’s founding in 1986, Sofradir SAS has pioneered the development of second- and third-generation MCT IR detectors, and secured a vast product portfolio of scanning and staring arrays that covers the entire infrared spectrum using MCT, quantum well infrared photodetectors (QWIP) as well as microbolometer technology platforms.

    Sofradir SAS is the first company to successfully develop MCT technology and bring its industrial processes to maturity. It is among the very few who can produce large quantities of second-generation and third-generation IR detectors. In 2008, Sofradir SAS employed over 400 people and was considered the No. 1 supplier in Europe for high-grade IR detectors for application in thermal imagers, missile seekers, and other surveillance, targeting and homing infrared equipment, based on their historical deliveries of cooled MCT second-generation IR detector units. In addition, Sofradir also holds a unique position in Europe as the only company to have developed, qualified and deployed space-grade second generation IR detectors. Working in close cooperation with national space agencies and companies worldwide, Sofradir’s MCT IR detectors today observe deep space, observe Earth, monitor the environment, and provide data on meteorological phenomena.

    Click here to view all of our Cooled Focal Plane Arrays!
     
    Models Return to top of the page
     
    Jupiter MW1280 x 1024 / 3.7-4.8µm
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    Saturn SW1000 x 256 / 0.8-2.5µm
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    Scorpio MW640 x 512 / 3.7-4.8µm
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    Uranus MW640 x 512 / 3.7-4.8µm
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    Sirius LW640 x 512 / 7.9-9.1µm
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    Neptune SW500 x 256 / 0.8-2.5µm
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    Mercury LW480 x 6 / 7.7-10.3µm
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    Epsilon MW384 x 288 / 3.4-4.8µm
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    Venus LW384 x 288 / 7.7-9.5µm
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    Vega LW84 x 288 / 7.7-9.1µm
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    Mars SW320 x 256 / 0.8-2.5µm
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    Mars MW320 x 256 / 3.7-4.8µm
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    Mars LW320 x 256 / 7.7-9.5µm
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    Mars VLW320 x 256 / 7.7-9.5µm
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    Pluton LW288 x 4 / 7.7-9.5µm
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