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
收藏
页码：145 / 156
页数：12
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