The visible channel of OMEGA-VIMS

Details The visible channel of OMEGA-VIMS The visible channel of OMEGA-VIMS

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stin...9016231f&link_type=abstract

Unknown

Physics

Design Analysis, Imaging Spectrometers, Infrared Spectrometers, Light (Visible Radiation), Thematic Mapping, Feasibility Analysis, Imaging Techniques, Space Programs, Systems Analysis, U.S.S.R.

Scientific paper

OMEGA-VIMS (Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activite - Visual and Infrared Mapping Spectrometer) is an infrared spectrometer selected for the Soviet mission Mars 94. The instrumentation is designed to support remote sensing of planetary surfaces by an infrared multispectral imager. It provides recognition of planetary bodies in the spectral range 0.30 to 1.05 microns. The main purpose of a visible channel for OMEGA-VIMS is to extend the mapping capability towards short wavelengths and to help the identification on the surface of features mapped in the infrared range. One of the purposes of this work is to explore the possibility of including the present design of the visible channel on missions, in terms of scientific return and technical feasibility. The optical, mechanical, electronical designs, together with considerations on interfacing problems, are presented.

Affiliated with

Also associated with

No associations

Rating

The visible channel of OMEGA-VIMS does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The visible channel of OMEGA-VIMS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The visible channel of OMEGA-VIMS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1521489