Mare Tyrrenium Region: Analysis of Dark Sand Dunes and Wind Direction Interpretations

Details Mare Tyrrenium Region: Analysis of Dark Sand Dunes and Wind Direction Interpretations Mare Tyrrenium Region: Analysis of Dark Sand Dunes and Wind Direction Interpretations

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1610c&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1610

Computer Science

Scientific paper

Our analysis of dune morphology in Mare Tyrrenium of Mars and GCM
indicates that simple dunes are consistent with present wind conditions,
but complex dunes reflect influences of local topography developing
secondary wind flows not predicted by GCM.

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