Wind-driven Particle Mobility on Mars: Insights from MER Observations at "El Dorado" and Surroundings at Gusev Crater

Details Wind-driven Particle Mobility on Mars: Insights from MER Observations at "El Dorado" and Surroundings at Gusev Crater Wind-driven Particle Mobility on Mars: Insights from MER Observations at "El Dorado" and Surroundings at Gusev Crater

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2092s&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

Spirit observations indicate: (1) smaller TARs seen across Mars likely
are coarse-grained ripples; (2) pervasive induration of sandy regolith,
and dust occurring as easily-entrained aggregates, explain disparity
between mobilization of sand vs. dust.

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