3 - 14 µm (MW, LW, VLW)
600 x 3 (x 4)
30 µm
MCT Technology
Features
- Versatile Architecture
- 100% Operability
- Space Proven Architecture
- On Board TRISHNA Mission
- Operating Characteristics - Nominal Frame rate: 4.5 kHz @3MHz pixel rate (Available operation up to 8MHz pixel rate) Integration time: From 15 μs up to (Frame time – 15μs)
Sensitive Arrays
4 channels [8 – 12μm] / 2 arrays (LWIR & VLWIR)
Format
9 readout lines of 600 pixels / 30 μm pixel pitch (nominal)
Operating Temperature
60K (nominal)
Description
Specially designed for earth observation space imaging applications
LYNRED Linear PEGA is a large linear detector specially tailored for earth observation applications from MWIR up to VLWIR spectral range. Based on LYNRED space proven MCT technology, LYNRED Linear PEGA detector, developped in the frame of TRISHNA mission offers the highest level in terms of performance (100% operability, high frame rate, large dynamic range...) and versatility (compatible design with staggered/butted configuration, external TDI, gain selection, integration time adjustment per readout line...).
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Related Applications
Earth Observation & Resource Management
Earth mapping and atmospheric monitoring provide valuable imagery for a better understanding of our planets conditions, characterization, and resource utilization.
Planetery Exploration
Exploring the solar system for planetary surface composition, mineralogical definition, and the detection of trace gases is accomplished using any one of our most common IR detectors from UV to VLWIR.
Scientific R&D Defense
Infrared imaging is an extremely valuable technology used extensively in engineering and scientific research centers around the world.
National Space
Infrared imaging is an extremely valuable technology used extensively in engineering and scientific research centers around the world.
