Mars 5, 146-158, 2010 | doi:10.1555/mars.2010.0006
Submitted: May 12, 2010; Reviewed: July 12, 2010; Revised: August 19, 2010; Accepted: August 27, 2010; Published: December 10, 2010
Mars is both a windy and dusty environment. Our purpose is to show how mesoscale models and large-eddy simulations help to explore small-scale circulation patterns which are potentially important for lifting dust into the atmosphere but which are unresolved by global climate models.
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