Mass Ejected from Martian Dust Devils as a Function of Height and Dust Devil Morphology

Details Mass Ejected from Martian Dust Devils as a Function of Height and Dust Devil Morphology Mass Ejected from Martian Dust Devils as a Function of Height and Dust Devil Morphology

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2409h&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

An investigation of morphology, density, vertical velocities, and mass
flux characteristics of martian dust devils observed by MER. The
conservation of mass is utilized to estimate quantity and height of dust
ejected into the martian atmosphere by dust devils.

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