30 µm pixel pitch
320 x 256 FPA
7.7 - 9.5 µm spectral range
MCT Technology


  • Adapted for detecting fast moving targets
  • More resilient to solar glint
  • More sensitive through dust and smoke
  • Reduces blooming
  • High charge capacity and 2 gains for the best sensitivity
Detector spectral response 7.7 - 9.5 µm @80K
ROIC architecture Snapshot, Integrate then read
Frame rate Up to 320 Hz
NETD < 20 mK ( 50 % well fill, 200 Hz )
Array operability 99.8 %


Mars LW, manufactured in large quantities, is the reference LWIR (8-10 µm) staring array. 

Sofradir’s MCT technology allows operations in LWIR waveband, the preferred solution for ground-based applications. 

This high-performance IDCA takes full advantage of Sofradir’s state of the art technologies.


Datasheet Mars LW
Brochure Gas Detection

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