MHD numerical study of the latitudinal deflection of coronal mass ejection
文献类型：期刊论文
| 作者 | Y. F. Zhou ; X. S. Feng |
| 刊名 | Journal of Geophysical Research: Space Physics
 |
| 出版日期 | 2013 |
| 卷号 | 118期号:10页码:6007-6018 |
| ISSN号 | 2169-9402 |
| 关键词 | CME latitudinal deflection numerical study |
| 通讯作者 | 北京8701信箱 |
| 中文摘要 | In this paper, we analyze and quantitatively study the deflection of coronal mass ejection (CME) in the latitudinal direction during its propagation from the Corona to interplanetary (IP) space using a three-dimensional (3-D) numerical magnetohydrodynamics (MHD) simulation. To this end, 12 May 1997 CME event during the Carrington rotation 1922 is selected. First, we try to reproduce the physical properties for this halo CME event observed by the WIND spacecraft. Then, we study the deflection of CME, and quantify the effect of the background magnetic field and the initiation parameters (such as the initial magnetic polarity and the parameters of the CME model) on the latitudinal deflection of CMEs. The simulations show that the initial magnetic polarity substantially affects the evolution of CMEs. The “parallel” CMEs (with the CME's initial magnetic field parallel to that of the ambient field) originating from high latitude show a clear Equatorward deflection at the beginning and then propagate almost parallel to heliospheric current sheet and the “antiparallel” CMEs (with the CME's initial magnetic field opposite to that of the ambient field) deflect toward the pole. Our results demonstrate that the latitudinal deflection extent of the “parallel” CMEs is mainly controlled not only by the background magnetic field strength but also by the initial magnetic field strength of the CMEs. There is an anticorrelation between the latitudinal deflection extent and the CME average transit speed and the energy ratio Ecme/Esw. |
| 学科主题 | 空间物理 |
| 语种 | 英语 |
| 源URL | [http://ir.cssar.ac.cn/handle/122/1522]  |
| 专题 | 国家空间科学中心_空间科学部 |
| 推荐引用方式 GB/T 7714 | Y. F. Zhou,X. S. Feng. MHD numerical study of the latitudinal deflection of coronal mass ejection[J]. Journal of Geophysical Research: Space Physics,2013,118(10):6007-6018. |
| APA | Y. F. Zhou,&X. S. Feng.(2013).MHD numerical study of the latitudinal deflection of coronal mass ejection.Journal of Geophysical Research: Space Physics,118(10),6007-6018. |
| MLA | Y. F. Zhou,et al."MHD numerical study of the latitudinal deflection of coronal mass ejection".Journal of Geophysical Research: Space Physics 118.10(2013):6007-6018. |
入库方式： OAI收割
来源：国家空间科学中心
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