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Eolian erosion of the Martian surface,part 1: Erosion rate similitude
Authors:JD Iversen  R Greeley  BR White  JB Pollack
Institution:Department of Aerospace Engineering, Iowa State University, Ames, Iowa 50010, USA;Physics Department, University of Santa Clara, Santa Clara, California 95053, USA;Department of Aerospace Engineering, Iowa State University, Ames, Iowa 50010, USA;Space Sciences Division, NASA Ames Research Center, Moffet Field, California 94035, USA
Abstract:A similitude parameter is derived which is based on theoretical considerations of erosion due to sand in saltation. This parameter has been used to correlate wind tunnel experiments of particle flow over model craters. The characteristics of the flow field in the vicinity and downstream of a crater are discussed and it is shown that erosion is initiated in areas lying under a pair of trailing vortices. The erosion rate parameter is used to calculate erosion rates on Mars, reported in Part 2, to be published later.
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