SIMPLE ANALYTICAL FORMS OF THE PERPENDICULAR DIFFUSION COEFFICIENT FOR TWO-COMPONENT TURBULENCE. I. MAGNETOSTATIC TURBULENCE

被引:23
|
作者
Shalchi, A. [1 ]
机构
[1] Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada
来源
ASTROPHYSICAL JOURNAL | 2013年 / 774卷 / 01期
基金
加拿大自然科学与工程研究理事会;
关键词
diffusion; magnetic fields; turbulence; GUIDING CENTER THEORY; CHARGED-PARTICLES; MAGNETIC-FIELD; TRANSPORT; ACCELERATION; ENERGY; DERIVATION; ELECTRONS; RECOVERY;
D O I
10.1088/0004-637X/774/1/7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We explore perpendicular diffusion based on the unified nonlinear transport theory. We derive simple analytical forms for the perpendicular mean free path and investigate the influence of different model spectra. We show that for cases where the field line random walk is normal diffusive, the perpendicular diffusion coefficient consists of only two transport regimes. Details of the spectral shape are less important, especially those of the inertial range. Only the macroscopic properties of the turbulence spectrum control the perpendicular diffusion coefficient. Simple formulae for the perpendicular diffusion coefficient are derived which can easily be implemented in solar modulation or shock acceleration codes.
引用
收藏
页数:6
相关论文
共 20 条