Time-Dependent Perpendicular Transport of Energetic Particles

被引:0
作者
Shalchi, A. [1 ]
机构
[1] Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada
来源
18TH ANNUAL INTERNATIONAL ASTROPHYSICS CONFERENCE | 2019年 / 1332卷
关键词
GUIDING CENTER THEORY; FIELD-LINE DIFFUSION; CHARGED-PARTICLES; COSMIC-RAYS; MODULATION; COEFFICIENTS; TURBULENCE; COMPOUND; VELOCITY; MINIMUM;
D O I
10.1088/1742-6596/1332/1/012014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The motion of energetic particles in magnetic turbulence across a mean magnetic field can be explored analytically. The approach discussed in this paper allows for a full time-dependent description of the transport, including compound sub-diffusion. For the first time it is shown systematically that as soon as there is transverse structure of the turbulence, diffusion is restored even if no Coulomb collisions are invoked. Compared to other non-linear theories the new approach has the advantage that a diffusion approximation is no longer part of that theory. Criteria for sub-diffusion and normal Markovian diffusion are provided as well. A comparison with test-particle simulations is also discussed.
引用
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页数:18
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