Heliospheric termination shock strength from a multi-fluid model

被引：0
|
作者：
Mueller, Hans-R. [1 ,2 ]
Woodman, Laura M. [1 ]
Zank, Gary P. [2 ]
机构：
[1] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[2] Univ Alabama, Ctr Spa Plasma & Aeronom Res, Huntsville, AL 35805 USA
来源：
PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND | 2008年 / 1039卷
关键词：
heliospheric termination shock;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A suite of 64 global heliospheric models, for which the interstellar densities and temperatures are varied within reasonable bounds, is analyzed with respect to the location of the termination shock on and off the stagnation axis, its temperature, and its compression ratio. The empirical relations regarding the termination shock, the heliopause and the interstellar bow shock, are discussed, as are the physical reasons behind these relations.
引用
收藏
页码：384 / +
页数：2
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