MHD turbulence model for global simulations of the solar wind and SEP acceleration

被引：0
|
作者：
Sokolov, Igor V. [1 ]
Roussev, Ilia I. [2 ]
机构：
[1] Univ Michigan, Dept AOSS, 2455 Hayward St, Ann Arbor, MI 48109 USA
[2] Univ Hawaii, Astron Inst, Honolulu, HI 96822 USA
来源：
PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND | 2008年 / 1039卷
关键词：
MHD-shock waves-turbulence-waves-acceleration of particles-Sun; coronal mass ejections (CMEs);
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The aim of the present work is to unify the various transport equations for turbulent waves that are used in different areas of space physics. We mostly focus on the magnetohydrodynamic (MHD) turbulence, in particular the Alfvenic turbulence.
引用
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页码：93 / +
页数：2
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