The Berlin Mars Near Surface Thermal Model (BMST) -- Modeling the Formation and Evolution of Sublimation Lags on Mars

Details The Berlin Mars Near Surface Thermal Model (BMST) -- Modeling the Formation and Evolution of Sublimation Lags on Mars The Berlin Mars Near Surface Thermal Model (BMST) -- Modeling the Formation and Evolution of Sublimation Lags on Mars

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1521h&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Phoenix for the first time directly studied ice on Mars and the SHARAD
instrument detected clear evidence for glacial deposits in the
equatorial regions of Mars. We study with the BMST model if these
deposits are the remnants of an earlier climate cycle.

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