An Aerodynamic Roughness Map Derived from Martian Rock Abundance Data and its Effects on Aeolian Erosion Thresholds in a MGCM

Details An Aerodynamic Roughness Map Derived from Martian Rock Abundance Data and its Effects on Aeolian Erosion Thresholds in a MGCM An Aerodynamic Roughness Map Derived from Martian Rock Abundance Data and its Effects on Aeolian Erosion Thresholds in a MGCM

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9057h&link_type=abstract

Third International Workshop on The Mars Atmosphere: Modeling and Observations, held November 10-13, 2008 in Williamsburg, Virgi

Physics

Scientific paper

We have applied to Mars a recent physical model designed to account for
the influence of the surface characteristics on the spatio-temporal
variability of dust emission in arid terrestrial environments.

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