Share Email Print
cover

Proceedings Paper

High-resolution infrared detector and its electronic unit for space application
Author(s): M. Meftah; F. Montmessin; O. Korablev; A. Trokhimovsky; G. Poiet; J.-B. Bel
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

High-resolution infrared detector is used extensively for military and civilian purposes. Military applications include target acquisition, surveillance, night vision, and tracking. Civilian applications include, among others, scientific observations. For our space systems, we want to use the products developed by SOFRADIR Company. Thus, we have developed a space electronic unit that is used to control the high-resolution SCORPIO-MW infrared detector, which has a format of 640×512 pixels with 15μm×15μm pixel pitch. The detector within microelectronics based on infrared mid-wave (MW) complementary metal oxide semiconductors (CMOS) uses a micro-cooler in order to keep its temperature around 100 K. The standard wavelength range (3 to 5μm) is adapted to the 2.2 to 4.3μm wavelength range thanks to adaptation of the optical interface of the detector and with an antireflection coating. With our electronic system, we can acquire 3 images per second. To increase the signal to noise ratio, we have the opportunity to make a summation of 15 frames per image. Through this article, we will describe the space electronic system that we have developed in order to achieve space observations (e.g. Atmospheric Chemistry Suite package for ExoMars Trace Gas Orbiter).

Paper Details

Date Published: 22 May 2015
PDF: 11 pages
Proc. SPIE 9469, Sensors and Systems for Space Applications VIII, 946905 (22 May 2015); doi: 10.1117/12.2177435
Show Author Affiliations
M. Meftah, Univ. Versailles St-Quentin, Sorbonne Univ., UPMC Univ. Paris 06, CNRS (France)
F. Montmessin, Univ. Versailles St-Quentin, Sorbonne Univ., UPMC Univ. Paris 06, CNRS (France)
O. Korablev, Space Research Institute (Russian Federation)
Moscow Institute of Physics and Technology (Russian Federation)
A. Trokhimovsky, Space Research Institute (Russian Federation)
Moscow Institute of Physics and Technology (Russian Federation)
G. Poiet, Univ. Versailles St-Quentin, Sorbonne Univ., UPMC Univ. Paris 06, CNRS (France)
J.-B. Bel, SOFRADIR (France)


Published in SPIE Proceedings Vol. 9469:
Sensors and Systems for Space Applications VIII
Khanh D. Pham; Genshe Chen, Editor(s)

© SPIE. Terms of Use
Back to Top