GCM Simulations of the Tropical Hydrogen Distribution Observed by Mars Odyssey

Details GCM Simulations of the Tropical Hydrogen Distribution Observed by Mars Odyssey GCM Simulations of the Tropical Hydrogen Distribution Observed by Mars Odyssey

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1518m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1518

Physics

Scientific paper

We use the GFDL Mars GCM with a fully coupled atmosphere-regolith water
cycle to understand the age of the hydrogen deposits observed by Mars
Odyssey. Trends in subsurface ice evolution are observed during various
obliquity and polar cap conditions.

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