Feasibility of an uncooled imaging spectrometer for the exploration of the solar system

Details Feasibility of an uncooled imaging spectrometer for the exploration of the solar system Feasibility of an uncooled imaging spectrometer for the exploration of the solar system

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988spie..890...46l&link_type=abstract

IN: Infrared systems and components II; Proceedings of the Meeting, Los Angeles, CA, Jan. 14, 15, 1988 (A89-15891 04-32). Bellin

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Imaging Techniques, Infrared Spectrometers, Cryogenic Cooling, Feasibility Analysis, Mars Probes, Solar System, Visible Spectrum

Scientific paper

A state-of-the-art imaging spectrometer concept is presented for visible-midwavelength IR spectral region studies of the solar system that obviates the until-now essential use of cryogenic cooling. This uncooled imaging spectrometer configuration is evaluated in view of the prospective environments of the instrument in various spacecraft orbits, as well as in light of various available photodetector materials and sensor focal plane array configurations.

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