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      The physics of wind-blown sand and dust

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          Abstract

          The transport of sand and dust by wind is a potent erosional force, creates sand dunes and ripples, and loads the atmosphere with suspended dust aerosols. This article presents an extensive review of the physics of wind-blown sand and dust on Earth and Mars. Specifically, we review the physics of aeolian saltation, the formation and development of sand dunes and ripples, the physics of dust aerosol emission, the weather phenomena that trigger dust storms, and the lifting of dust by dust devils and other small-scale vortices. We also discuss the physics of wind-blown sand and dune formation on Venus and Titan.

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          Most cited references24

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          Improved general circulation models of the Martian atmosphere from the surface to above 80 km

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            A study of the thermal and dynamical structure of the martian lower atmosphere

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              Eolian deposits and dunes on Mars

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                Author and article information

                Journal
                20 January 2012
                2012-09-20
                Article
                10.1088/0034-4885/75/10/106901
                1201.4353
                525e7cdb-d246-4b33-8ea1-8abaaeb9afa6

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
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                Kok, J. F., E. J. R. Parteli, T. I. Michaels, and D. Bou Karam, Rep. Prog. Phys. 75, 106901, 2012
                72 journal pagers, 49 figures
                astro-ph.EP cond-mat.soft physics.ao-ph

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