Local interstellar medium and modeling the heliosphere

被引：35
|
作者：
Ratkiewicz, R
Barnes, A
Spreiter, JR
机构：
[1] Ctr Space Res, PL-00716 Warsaw, Poland
[2] NASA, Ames Res Ctr, Div Space Sci, Moffett Field, CA 94035 USA
[3] Stanford Univ, Stanford, CA 94305 USA
来源：
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 2000年 / 105卷 / A11期
关键词：
D O I：
10.1029/1999JA005084
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We use the best currently available estimates for interstellar parameters to update and expand the earlier study of Ratkiewicz et al. [1998]. We report (1) a more complete survey of the morphology of the heliosphere and the ways it may be modified by variation of external interstellar parameters, (2) a detailed classification of the several asymmetries and distortions associated with exterior field-flow obliquity, including cross sections of the three-dimensional structure in all three principal planes, (3) an analysis of the transition from supermagnetosonic to nearly transmagnetosonic flow, and (4) specific results for the heliosphere for the best current understanding of conditions in the local interstellar medium.
引用
收藏
页码：25021 / 25031
页数：11
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