On the dynamics of the heliosphere on intermediate and long time-scales

被引：42

作者：

Borrmann, T ^{[1
]}

Fichtner, H ^{[1
]}

机构：

[1] Ruhr Univ Bochum, Inst Theoret Phys Weltraum & Astrophys, D-44780 Bochum, Germany

来源：

DYNAMIC HELIOSPHERE | 2005年 / 35卷 / 12期

关键词：

heliospheric dynamics; interstellar clouds; solar activity; termination shock;

D O I：

10.1016/j.asr.2005.08.039

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

A time-dependent, three-dimensional model of the dynamics of the heliosphere as a result of solar activity and a time-varying local interstellar medium is presented. The model is based on a recent version of the well known ZEUS code and employs parallel processing. It includes the solar and interstellar plasma components as well as neutral atoms, and contains the heliospheric magnetic field in a kinematic fashion. We study the dynamics of the heliosphere due to solar activity on periods of months to years up to the so-called Schwabe (11-year) cycle as well as due to time variations of the local interstellar medium, all of which have drawn increasing attention during recent years, as the significance of their direct or indirect effect on the Earth and its environment is under lively debate. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：2091 / 2101

页数：11

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