Shallow Water and Seasonal Deposits of Carbon Dioxide on Mars: Neutron Data Deconvolution of HEND/Odyssey

Details Shallow Water and Seasonal Deposits of Carbon Dioxide on Mars: Neutron Data Deconvolution of HEND/Odyssey Shallow Water and Seasonal Deposits of Carbon Dioxide on Mars: Neutron Data Deconvolution of HEND/Odyssey

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufm.p21a..05m&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #P21A-05

Mathematics

Logic

5410 Composition, 5416 Glaciation, 5460 Physical Properties Of Materials, 5462 Polar Regions

Scientific paper

The latest results are presented of 20 months mapping of Mars by High Energy Neutron Detector (HEND) onboard NASA Mars Odyssey. The water content is estimated for distinct geological regions at high and medium latitudes of Mars according to the model of double-layered subsurface. The structure of poleward regions of water-ice permafrost is presented for northern and southern hemispheres. Several spots at equatorial latitudes with the highest observable content of shallow water are discussed in more details. The seasonal time history of carbon dioxide circulation is presented, and the total mass of deposition is estimated for winter at north and south.

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