Other
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....97.7719c&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. E5, May 25, 1992, p. 7719-7734.
Other
177
Infrared Spectrometers, Mars Atmosphere, Mars Observer, Mars Surface, Thermal Emission, Aerosols, Atmospheric Composition, Particle Size Distribution, Planetary Composition
Scientific paper
The paper describes the thermal emission spectrometer (TES) designed for the Mars Observer mission. The TES measurements of the surface and the atmosphere of Mars will be used to determine and map the composition of the surface rocks, minerals, and the condensates. Examples of information that will be obtained from TES data include mineral abundance maps, condensate properties and their distribution in time and space, aerosol properties and their distribution in time and space, the rock abundance, the polar energy balance, and properties of gaseous species. Where appropriate, these derived parameters will be distributed in the form of gridded map, to allow direct comparison with other derived data sets.
Anderson Donald L.
Bandiera Nuno
Brown F. G.
Carpenter James
Chase Stillman C.
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