CHARGED-PARTICLE MOTION IN MULTIDIMENSIONAL MAGNETIC-FIELD TURBULENCE

被引:107
作者
GIACALONE, J [1 ]
JOKIPII, JR [1 ]
机构
[1] UNIV ARIZONA,DEPT ASTRON,TUCSON,AZ 85721
关键词
COSMIC RAYS; DIFFUSION; MAGNETIC FIELDS; TURBULENCE;
D O I
10.1086/187457
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new analysis of the fundamental physics of charged-particle motion in a turbulent magnetic field using a numerical simulation. The magnetic field fluctuations are taken to be static and to have a power spectrum which is Kolmogorov. The charged particles are treated as test particles. It is shown that when the field turbulence is independent of one coordinate (i.e., k lies in a plane), the motion of these particles across the magnetic field is essentially zero, as required by theory. Consequently, the only motion across the average magnetic field direction that is allowed is that due to field-line random walk. On the other hand, when a fully three-dimensional realization of the turbulence is considered, the particles readily cross the field. Transport coefficients both along and across the ambient magnetic field are computed. This scheme provides a direct computation of the Fokker-Planck coefficients based on the motions of individual particles, and allows for comparison with analytic theory.
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页码:L137 / L140
页数:4
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