The physics of wind-blown sand and dust

被引:922
作者
Kok, Jasper F. [1 ]
Parteli, Eric J. R. [2 ,3 ]
Michaels, Timothy I. [4 ]
Karam, Diana Bou [5 ]
机构
[1] Cornell Univ, Dept Earth & Atmospher Sci, Ithaca, NY 14850 USA
[2] Univ Fed Ceara, Dept Fis, Fortaleza, Ceara, Brazil
[3] Univ Erlangen Nurnberg, Inst Multiscale Simulat, D-91054 Erlangen, Germany
[4] SW Res Inst, Boulder, CO USA
[5] Univ Paris 06, CNRS, IPSL, LATMOS, Paris, France
基金
美国国家科学基金会;
关键词
MARS ORBITER CAMERA; GENERAL-CIRCULATION MODEL; TRANSVERSE AEOLIAN RIDGES; INTERTROPICAL DISCONTINUITY REGION; THRESHOLD FRICTION VELOCITY; SELF-ORGANIZED CRITICALITY; MINERAL AEROSOL PRODUCTION; ATMOSPHERIC ICE NUCLEI; BOUNDARY-LAYER MODEL; BED-LOAD TRANSPORT;
D O I
10.1088/0034-4885/75/10/106901
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The transport of sand and dust by wind is a potent erosional force, creates sand dunes and ripples, and loads the atmosphere with suspended dust aerosols. This paper presents an extensive review of the physics of wind-blown sand and dust on Earth and Mars. Specifically, we review the physics of aeolian saltation, the formation and development of sand dunes and ripples, the physics of dust aerosol emission, the weather phenomena that trigger dust storms, and the lifting of dust by dust devils and other small-scale vortices. We also discuss the physics of wind-blown sand and dune formation on Venus and Titan.
引用
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页数:72
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