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Parsons 2000
Parsons, J.D. (2000). Are fast-growing martian dust storms compressible?. Geophysical Research Letters 27: doi: 10.1029/1999GL008456. issn: 0094-8276.

A simple scale analysis demonstrates that rapidly-expanding Martian dust storms are driven by extremely large density differences. Thermal gradients appear to be inadequate to produce these density contrasts. When dust produces the densities required, the storms become compressible because of the slowing of the speed of sound due to the addition of particles. Though compressible, particle-laden flows have never been analyzed due to their highly complex nature, pressure waves produced by these flows could be hypothesized to provide a positive feedback capable of producing rapid growth. Âż 2000 American Geophysical Union

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Abstract

Keywords
Atmospheric Composition and Structure, Aerosols and particles (0345, 4801), Planetology, Solid Surface Planets, Atmospheres—structure and dynamics, Planetology, Solar System Objects, Mars
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
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