Searching for Correlation Between Neutron Albedo and Near-IR Albedo of Mars Surface Using HEND/Odyssey and MOLA/MGS Data

Details Searching for Correlation Between Neutron Albedo and Near-IR Albedo of Mars Surface Using HEND/Odyssey and MOLA/MGS Data Searching for Correlation Between Neutron Albedo and Near-IR Albedo of Mars Surface Using HEND/Odyssey and MOLA/MGS Data

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1640d&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

1

Scientific paper

Strong negative correlation between HEND neutron albedo and MOLA near-IR
albedo is found within two broad latitude belts: 40°N-80°N and
40°S-60°S. Interpretation: water ice in these belts is buried
below the dry skin layer, which thickness is determined

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