Surface photometric properties in Gusev crater from CRISM observation onboard MRO spacecraft

Details Surface photometric properties in Gusev crater from CRISM observation onboard MRO spacecraft Surface photometric properties in Gusev crater from CRISM observation onboard MRO spacecraft

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1410f&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1410

Physics

Scientific paper

CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) onboard MRO (Mars Reconnaissance Orbiter) acquires observations under varied geometry conditions in visible/near infrared and provides constraints on the surface physical properties in Gusev crater. First, we select appropriate CRISM observations. Second, we applied an original inversion method to retrieve the atmospheric optical thickness considering a nonlambertian surface hypothesis. Third, we estimate the physical parameters using a 2-term phase function Hapke inversion procedure using the retrieved surface reflectance. The present results can be compared to previous photometric studies from orbital and in situ instruments.

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