Relation between different theories for cosmic ray cross field diffusion

被引：20

作者：

Dosch, A. ^{[1
]}

Shalchi, A. ^{[1
]}

Weinhorst, B. ^{[1
]}

机构：

[1] Ruhr Univ Bochum, Inst Theoret Phys, Lehrstuhl Weltraum & Astrophys 4, D-44780 Bochum, Germany

来源：

ADVANCES IN SPACE RESEARCH | 2009年 / 44卷 / 11期

关键词：

Diffusion; Magnetic fields; Turbulence; Cosmic rays; Solar wind; GUIDING CENTER THEORY; PERPENDICULAR DIFFUSION; RANDOM-WALK; CHARGED-PARTICLES; VELOCITY CORRELATION; NONLINEAR PARALLEL; TRANSPORT; LINES; COMPOUND; TURBULENCE;

D O I：

10.1016/j.asr.2009.07.007

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

In the past few year several theories have been presented for describing cosmic ray scattering across the mean magnetic field. It is the purpose of the present article to discuss the relation between these different theories in order to improve our understanding of cosmic ray perpendicular scattering and to explore the parameter regimes for which these different theories are valid. (C) 2009 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：1326 / 1336

页数：11

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