VNIR-VIMS: A visible mapping spectrometer for Mars-94

Details VNIR-VIMS: A visible mapping spectrometer for Mars-94 VNIR-VIMS: A visible mapping spectrometer for Mars-94

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stin...9113390f&link_type=abstract

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Computer Science

Performance

Infrared Spectrometers, Mars Surface, Multispectral Band Scanners, Planetary Mapping, Visible Spectrum, Cassini Mission, Comet Rendezvous Asteroid Flyby Mission, Planetary Orbits, Remote Sensing, Signal To Noise Ratios, Space Missions, Spectral Resolution

Scientific paper

Instrumentation designed to support remote sensing of planetary surfaces by an infrared multispectral imager is presented. OMEGA-VIMS (French proposed observatory for mineralogy, water, ice and activity - U.S. proposed Visual Infrared Mapping Spectrometer) is an infrared spectrometer selected for the Soviet mission Mars 94. The design was optimized for flexibility to the Cassini (Saturn, Titan) and CRAF (Comet Rendez-vous and Asteroid Flyby) missions. The visible channel design, its nominal performances, and their use along the orbit around Mars are discussed. The optical, mechanical and electronical designs and considerations on interfacing problems, and the performance (signal to noise ratio) foreseen at Mars are presented.

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