Non-stationary magnetic field geometry in the heliosphere

被引：0
|
作者：
Veselovsky, IS [1 ]
机构：
[1] Moscow MV Lomonosov State Univ, Inst Nucl Phys, Moscow 119899, Russia
来源：
OUTER HELIOSPHERE: THE NEXT FRONTIERS, PROCEEDINGS | 2001年 / 11卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The magnetic field in the heliosphere is dependent on space and time because of the imposed boundary conditions and internal dynamical processes (see, e.g., reviews by Mariani and Neubauer, 1990; Burlaga, 1991). Quasistationary and transient structures coexist in proportions varying with the solar cycle. The purpose of this paper is to present model examples showing magnetic field lines with different geometric properties in the heliosphere.
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页码：61 / 64
页数：4
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