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Evolution of coronal mass ejection/shock system in interplanetary space
Xiang, C. Q.; Wei, F. S.; Feng, X. S.; Wang, J. F.; 北京8701信箱
Department空间天气学国家重点实验室
Source PublicationSpace Weather
2005
Volume36Issue:12Pages:2308-2312
ISSN0273-1177
Language英语
KeywordCoronal Mass Ejections Magnetic Clouds Magnetohydrodynamic Simulation Streamer
AbstractThe evolution of coronal mass ejection/shock system is investigated by numerically solving the usual set of two-dimensional single-fluid polytropic magnetohydrodynamic equations from 1 R-s to 1 AU in the meridian plane. The simulation result reveals that the coronal mass ejection/shock system formed near the sun evolves into the magnetic cloud/shock system near the earth's orbit through the following three phases: the initial formation, the dominant latitudinal expansion and the similar expansion. (c) 2005 Published by Elsevier Ltd on behalf of COSPAR.
Indexed BySCI
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/1035
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
Xiang, C. Q.,Wei, F. S.,Feng, X. S.,et al. Evolution of coronal mass ejection/shock system in interplanetary space[J]. Space Weather,2005,36(12):2308-2312.
APA Xiang, C. Q.,Wei, F. S.,Feng, X. S.,Wang, J. F.,&北京8701信箱.(2005).Evolution of coronal mass ejection/shock system in interplanetary space.Space Weather,36(12),2308-2312.
MLA Xiang, C. Q.,et al."Evolution of coronal mass ejection/shock system in interplanetary space".Space Weather 36.12(2005):2308-2312.
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