Three-dimensional structure of the outer heliosphere in the presence of the interstellar and interplanetary magnetic fields

被引：0
|
作者：
Pogorelov, NV [1 ]
机构：
[1] Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
来源：
PHYSICS OF THE OUTER HELIOSPHERE | 2004年 / 719卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Three-dimensional structure of the heliosphere is analyzed for the effects of coupling between the interstellar and interplanetary magnetic fields (ISMF and IMF). The case when the ISMF is orthogonal to the velocity of the local interstellar medium, and tilted 60degrees to the ecliptic plane, is specifically investigated in view of the recent suggestion that this is the most probable ISMF orientation.
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页码：39 / 46
页数：8
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