An interferometric spectral mapper for the Cassini mission to Saturn and Titan

Details An interferometric spectral mapper for the Cassini mission to Saturn and Titan An interferometric spectral mapper for the Cassini mission to Saturn and Titan

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991wusl.rept.....s&link_type=abstract

Final Report Washington Univ., Saint Louis, MO.

Astronomy and Astrophysics

Astronomy

Astronomical Interferometry, Cassini Mission, Equipment Specifications, Infrared Detectors, Interferometers, Planetary Atmospheres, Atmospheric Composition, Satellite Atmospheres, Space Exploration, Titan

Scientific paper

The research reported resulted in a detailed proposal for the Cassini Mission that addressed fundamental atmospheric structure and composition questions for both Saturn and Titan. Due to the brief time available between the initiation of the research and the proposal date, it was necessary to develop the science goals in close synchronicity with the instrument design. A major goal of the program was to acquire, implement, and test SWIR and MWIR arrays suitable for use with the DIGITAL ARRAY SCANNED INTERFEROMETERS, (DASI's), for the extended goal of developing DASI's for a range of spectral mapping research in solar system exploration. These goals were all reached or exceeded in the course of this work.

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