The VNIR-VIMS experiment for Craf/Cassini

Details The VNIR-VIMS experiment for Craf/Cassini The VNIR-VIMS experiment for Craf/Cassini

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15.1179f&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 6, p. 1179-1192.

Physics

3

Cassini Mission, Multispectral Band Cameras, Saturn (Planet), Space Exploration, Spaceborne Photography, Satellite Atmospheres, Saturn Rings, Saturn Satellites, Spectral Reflectance, Spectral Resolution

Scientific paper

VNIR, the visible channel of the VIMS (Visual Near-Infrared Mapping Spectrometer), has the task to cover the 0.35-5-micron wavelength range by means of three channels, one in the visible and two in the near IR. Here, the visible channel is discussed with particular reference to the Cassini mission. The discussion covers the scientific background of the mission, the study of Saturn rings, atmospheric studies, and a description of the VNIR hardware and capabilities.

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