Pickup Ion Mediated Plasmas: Shock Wave Structure

被引：2

作者：

Mostafavi, P. ^{[1
,2
]}

Zank, G. P. ^{[1
,2
]}

Webb, G. M. ^{[1
,2
]}

机构：

[1] Univ Alabama, CSPAR, Huntsville, AL 35805 USA

[2] Univ Alabama, Dept Space Sci, Huntsville, AL 35805 USA

来源：

PROCEEDINGS OF THE FOURTEENTH INTERNATIONAL SOLAR WIND CONFERENCE (SOLAR WIND 14) | 2016年 / 1720卷

关键词：

COSMIC-RAY SHOCKS; TERMINATION SHOCK; SOLAR-WIND;

D O I：

10.1063/1.4943855

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

Energetic particles such as pickup ions, solar energetic particles, or cosmic rays play an important role in determining shock structure. Cosmic-ray modified shocks were discussed by Axford et al. [2]. Jokipii and Williams [8] considered the e ff ect of cosmic ray viscosity on the structure of cold thermal gas shocks mediated by cosmic rays. In the present paper, we consider a background thermal gas of arbitrary temperature to extend their work. The Zank et al. [7] model is used to determine the shock structure when energetic particle collisionless heat flux and viscosity is included.

引用

页数：4

共 13 条

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