Characterizing Daytime Erosion Potential on Mars Using the MRAMS LES

Details Characterizing Daytime Erosion Potential on Mars Using the MRAMS LES Characterizing Daytime Erosion Potential on Mars Using the MRAMS LES

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1964f&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

We present preliminary results of large eddy simulations of the Viking
Lander 1 and Phoenix landing sites, demonstrating that convective
activity ("gustiness") both enhances modeled dust entrainment and
differs in intensity at the two landing sites.

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