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Effects of Palagonitic Dust Coatings on Thermal Emission Spectra of Rocks and Minerals: Implications for Mineralogical Characterization of the Martian Surface by MGS-TESThermal emission measurements on dust-coated rocks and minerals show that a 300 5m thick layer is required to mask emission from the substrate and that non-linear effects are present. Additional information is contained in the original extended abstract.
Document ID
20010045028
Document Type
Conference Paper
Authors
Graff, T. G.
(Arizona State Univ. Tempe, AZ United States)
Morris, R.
(NASA Johnson Space Center Houston, TX United States)
Christensen, P.
(Arizona State Univ. Tempe, AZ United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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