The transport of charged particles in a flowing medium

被引:10
作者
Lu, JY [1 ]
Zank, GP
Rankin, R
Marchand, R
机构
[1] Univ Alberta, Dept Phys, Edmonton, AB T6G 2J1, Canada
[2] Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
[3] Univ Alberta, Dept Phys, Edmonton, AB T6G 2J1, Canada
[4] Chinese Acad Sci, Ctr Space Sci & Appl Res, Beijing, Peoples R China
关键词
acceleration of particles; cosmic rays; methods : numerical; plasmas; solar wind;
D O I
10.1086/341734
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The propagating source method for solving the time-dependent Boltzmann equation describing particle propagation in a magnetically turbulent medium is extended to a more realistic case that includes focusing and adiabatic deceleration. The solutions correspond to beam propagation in the solar wind. Pitch-angle scattering away from 90degrees is described by standard quasi-linear theory (QLT), while scattering through 90degrees is approximated by a BGK operator representing a slow mirroring process. The detailed numerical technique for solving the Fokker-Planck equation for two particular spectra is presented. Comparisons are made between our modified QLT (MQLT) model and a BGK model, between highly anisotropic scattering and moderately anisotropic scattering, and between fast particles and slow particles. It is shown that: (1) for moderately anisotropic pitch-angle scattering, the initial ring-beam distribution finally evolves into a broad Gaussian distribution and the QLT isotropic and MQLT anisotropic models could be rather well approximated by the simple relaxation time operator. (2) For highly anisotropic pitch-angle scattering, a moving pulse with a spatially extended at tail is formed, and there exist some differences between the MQLT and BGK models. Specifically, at a particular pitch angle, the spatial distribution from MQLT model occupies a much wider region than that in the BGK model. (3) In the highly anisotropic scattering medium, more particles are cooled by adiabatic deceleration, some particles move a little faster, and the spatial distribution at a specific pitch angle is much more dispersed than that in the case of moderately anisotropic scattering. (4) Compared with the BGK model, the anisotropy persists for a little longer and some particles move a little slower; consequently, intensity profiles have a greater amplitude at later times in the MQLT model. (5) Finally, fast and slow particles have similar distribution characteristics, except that convection is much more important for slow particles.
引用
收藏
页码:574 / 586
页数:13
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