The Effects of Topography of the Mars upon the Atmospheric Motion of the Mars and the Possible Mechanism That Produced the Dust Storm on the Mars

Li Mai-cun; Xie Ying-qi

doi:10.11728/cjss1984.04.314

Volume 4 Issue 4

Dec. 1984

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Li Mai-cun, Xie Ying-qi. The Effects of Topography of the Mars upon the Atmospheric Motion of the Mars and the Possible Mechanism That Produced the Dust Storm on the Mars[J]. Chinese Journal of Space Science, 1984, 4(4): 314-323. doi: 10.11728/cjss1984.04.314

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Li Mai-cun, Xie Ying-qi. The Effects of Topography of the Mars upon the Atmospheric Motion of the Mars and the Possible Mechanism That Produced the Dust Storm on the Mars[J]. Chinese Journal of Space Science, 1984, 4(4): 314-323. doi: 10.11728/cjss1984.04.314

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The Effects of Topography of the Mars upon the Atmospheric Motion of the Mars and the Possible Mechanism That Produced the Dust Storm on the Mars

doi: 10.11728/cjss1984.04.314 cstr: 32142.14.cjss1984.04.314

Li Mai-cun¹,
Xie Ying-qi²

1.
Institute of Atmospheric Physics, Academia Sinica
2.
Dept. of Geophysics, Yunnan University

Received Date: 1983-12-23
Rev Recd Date: 1900-01-01
Publish Date: 1984-12-24

Abstract

Abstract

In this paper, the influence of the surface topography to the atmosphere of the Mars is examined on the assumption of a quasi-geostrophic model, and a rough explanation is given for the possible physical mechanism that produces the dust storm on the Mars.