Influence of dust on the dynamics of the martian atmosphere above the first scale height

被引：23

作者：

Medvedev, Alexander S. ^{[1
]}

Kuroda, Takeshi ^{[1
,2
]}

Hartogh, Paul ^{[1
]}

机构：

[1] Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany

[2] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2525210, Japan

来源：

AEOLIAN RESEARCH | 2011年 / 3卷 / 02期

基金：

日本学术振兴会;

关键词：

Mars atmosphere; Atmospheric aerosol; Dust storms; General circulation; GENERAL-CIRCULATION MODEL; ZONAL-MEAN CIRCULATION; WINTER POLAR WARMINGS; MARS GLOBAL SURVEYOR; GRAVITY-WAVE DRAG; MIDDLE ATMOSPHERE; NORTHERN-HEMISPHERE; PLANETARY ATMOSPHERES; OPTICAL-PROPERTIES; VERTICAL STRUCTURE;

D O I：

10.1016/j.aeolia.2011.05.001

中图分类号：

P9 [自然地理学];

学科分类号：

0705 ; 070501 ;

摘要：

Dust suspended in the martian atmosphere strongly affects the radiative transfer. Diabatic heating and cooling it creates are prominent factors that drive the atmosphere at various scales. This paper provides a review of dust influence on the large-scale dynamics in the atmosphere of Mars above approximately 10 km. We outline the established properties of dust that influence the diabatic heating/cooling rates, and summarize the current knowledge of dust-related effects on the zonal-mean circulation and zonally asymmetric disturbances: planetary waves and tides. (C) 2011 Elsevier B.V. All rights reserved.

引用

页码：145 / 156

页数：12

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