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Mars: Local Structure of Dust Storms

Published online by Cambridge University Press:  14 August 2015

G. I. Barenblatt  and
G. S. Golitsyn
G. I. Barenblatt
Affiliation:
Institute of Mechanics of Moscow University, Moscow, U.S.S.R.
G. S. Golitsyn
Affiliation:
Institute of Atmospheric Physics, Academy of Sciences of the U.S.S.R., Moscow, U.S.S.R.

Abstract

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A hydronamical theory describing the motion of the dusty flow including the effects of thermal stratification is presented. It is shown that the dust, while decreasing the intensity of turbulence in the flow, can accelerate the wind. Applied to Mars, the theory reveals that these effects may be important there in understanding the nature and the long duration of Martian dust storms.

Type
Part II Terrestrial Planets
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 317
Copyright
Copyright © Reidel 1974