PITCH-ANGLE DIFFUSION COEFFICIENTS OF CHARGED PARTICLES FROM COMPUTER SIMULATIONS

被引:58
|
作者
Qin, G. [1 ]
Shalchi, A. [1 ,2 ]
机构
[1] Chinese Acad Sci, State Key Lab Space Weather, Ctr Space Sci & Appl Res, Beijing 100190, Peoples R China
[2] Ruhr Univ Bochum, Inst Theoret Phys, Lehrstuhl Weltraum & Astrophys 4, D-44780 Bochum, Germany
来源
ASTROPHYSICAL JOURNAL | 2009年 / 707卷 / 01期
基金
美国国家科学基金会;
关键词
diffusion; magnetic fields; turbulence; COSMIC-RAY PROPAGATION; GUIDING CENTER THEORY; PERPENDICULAR DIFFUSION; SUBDIFFUSIVE TRANSPORT; NONLINEAR PARALLEL; MAGNETIC-FIELD; RANDOM-WALK; TURBULENCE; SCATTERING; COMPOUND;
D O I
10.1088/0004-637X/707/1/61
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Pitch-angle diffusion is a key process in the theory of charged particle scattering by turbulent magnetic plasmas. This process is usually assumed to be diffusive and can, therefore, be described by a pitch-angle diffusion or Fokker Planck coefficient. This parameter controls the parallel spatial diffusion coefficient as well as the parallel mean free path of charged particles. In the present paper, we determine pitch-angle diffusion coefficients from numerical computer simulations. These results are then compared with results from analytical theories. Especially, we compare the simulations with quasilinear, second-order, and weakly nonlinear diffusion coefficients. Such a comparison allows the test of previous theories and will lead to an improved understanding of the mechanism of particle scattering.
引用
收藏
页码:61 / 66
页数:6
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