Variations in brightness over Callisto's surface as measured by the Galileo ultraviolet spectrometer

Details Variations in brightness over Callisto's surface as measured by the Galileo ultraviolet spectrometer Variations in brightness over Callisto's surface as measured by the Galileo ultraviolet spectrometer

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..549h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 549.

Computer Science

Brightness, Galileo Spacecraft, Spacecraft Instruments, Ultraviolet Spectrometers, Callisto, Field Of View, Albedo

Scientific paper

The Galileo UVS F-channel observations of Callisto's Asgard multiring basin represent the first disk-resolved UV information on this body, allowing study of spectral variations across the surface that may be indicative of differences in composition or grain size. An examination is conducted of spectral variations across the crater, in order to look for evidence of debris throughout the rings and their surroundings, as well as of spectral variations across the polar regions; these are all compared with measurements obtained from the rest of Callisto.

Affiliated with

Also associated with

No associations

Rating

Variations in brightness over Callisto's surface as measured by the Galileo ultraviolet spectrometer 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 Variations in brightness over Callisto's surface as measured by the Galileo ultraviolet spectrometer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variations in brightness over Callisto's surface as measured by the Galileo ultraviolet spectrometer will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-872054