Tharsis Montes Ice Sheet Models at High Obliquity Driven by GMC Results

Details Tharsis Montes Ice Sheet Models at High Obliquity Driven by GMC Results Tharsis Montes Ice Sheet Models at High Obliquity Driven by GMC Results

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1119f&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

We describe the use of results from an atmospheric GCM for Mars at high
obliquity that favors deposition of snow on the flanks of Tharsis
volcanoes; we use predicted accumulation rates to drive an ice sheet
model that is then seen to be in agreement with

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