Niveo-Aeolian Process Interactions and Resultant Martian Polar Dune Morphology

Details Niveo-Aeolian Process Interactions and Resultant Martian Polar Dune Morphology Niveo-Aeolian Process Interactions and Resultant Martian Polar Dune Morphology

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2192d&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2192

Physics

Scientific paper

We hypothesize that the distinctive martian polar dune lee slope
morphology is formed through a niveo-aeolian process. We will evaluate
three formation hypotheses: ice-cementation of the dune core, seasonal
frost sublimation, or reversing winds.

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