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Influence of the interstellar magnetic field direction on the shape of the global heliopause

被引：96
作者：
Pogorelov, NV
Matsuda, T
机构：
[1] Russian Acad Sci, Inst Problems Mech, Moscow 117526, Russia
[2] Kobe Univ, Fac Sci, Dept Earth & Planetary Sci, Nada Ku, Kobe, Hyogo 657, Japan
来源：
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1998年 / 103卷 / A1期
关键词：
D O I：
10.1029/97JA02446
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper we study the influence of the angle between the local interstellar medium velocity and magnetic field vectors on the interaction of this medium with the solar wind. Both winds are supposed supersonic. Applicability of the two-shock model of the interaction is discussed. Investigation is performed by numerical solution of the MHD equations for an ideal plasma in the one-fluid approximation.
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收藏
页码：237 / 245
页数：9
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