A Study of Ice Accumulation and Stability in Martian Craters Under past Orbital Conditions Using the LMD Mesoscale Model

Details A Study of Ice Accumulation and Stability in Martian Craters Under past Orbital Conditions Using the LMD Mesoscale Model A Study of Ice Accumulation and Stability in Martian Craters Under past Orbital Conditions Using the LMD Mesoscale Model

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1664m&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1664

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The goal of this study is to better understand the climate conditions
under which ice-related features present in impact craters formed, using
geological observations and mesoscale climate simulations of the
corresponding regions.

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