| 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 Publication | Space Weather
 |
| 2005 | |
| Volume | 36Issue:12Pages:2308-2312 |
| ISSN | 0273-1177 |
| Language | 英语 |
| Keyword | Coronal Mass Ejections Magnetic Clouds Magnetohydrodynamic Simulation Streamer |
| Abstract | The 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 By | SCI |
| Funding Project | 中国科学院空间科学与应用研究中心 |
| Document Type | 期刊论文 |
| Identifier | http://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. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| 200536122308.pdf（368KB） | 开放获取 | CC BY-NC-SA | Application Full Text | |||
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