Solution-adaptive magnetohydrodynamics for space plasmas:: Sun-to-earth simulations

被引：58

作者：

Gombosi, TI ^{[1
]}

Powell, KG

De Zeeuw, DL

Clauer, CR

Hansen, KC

Manchester, WB

Ridley, AJ

Roussev, II

Sokolov, IV

Stout, QF

Tóth, G

机构：

[1] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ctr Space Environm Modeling, Ann Arbor, MI 48109 USA

[2] Eotvos Lorand Univ, Budapest, Hungary

来源：

COMPUTING IN SCIENCE & ENGINEERING | 2004年 / 6卷 / 02期

基金：

美国国家航空航天局; 美国国家科学基金会; 匈牙利科学研究基金会;

关键词：

D O I：

10.1109/MCISE.2004.1267603

中图分类号：

TP39 [计算机的应用];

学科分类号：

081203 ; 0835 ;

摘要：

Space-environment simulations, particularly those involving space plasma, present significant computational challenges. Global computational models based on magnetohydrodynamics equations are essential to understanding the solar system's plasma phenomena, including the large-scale solar corona, the solar wind's interaction with planetary magnetospheres, comets, and interstellar medium, and the initiation, structure, and evolution of solar eruptive events.

引用

页码：14 / 35

页数：22

共 33 条

[1] A three-dimensional MHD study of solar wind mass loading processes at Venus: Effects of photoionization, electron impact ionization, and charge exchange [J].