Characterizing the 3-D Water Distribution on the Mars Surface

Details Characterizing the 3-D Water Distribution on the Mars Surface Characterizing the 3-D Water Distribution on the Mars Surface

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1253t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1253

Computer Science

Scientific paper

The Mars Odyssey Neutron Spectrometer (MONS) and the Mars Reconnaissance Orbiter-Compact Reconnaissance Imaging Spectrometer (MRO-CRISM) have produced two data-sets that sample the top layers of the Martian soil in a complementary way: while MONS samples the top metre of the martian soil MRO-CRISM sample the top few mm's. We have devised a statistical approach that makes use these two complementary pieces of information to characterize the 3-D distribution of water on the Mars surface.

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