Using a 3-D MHD simulation to interpret propagation and evolution of a coronal mass ejection observed by multiple spacecraft: The 3 April 2010 event
文献类型：期刊论文
| 作者 | Zhou, Yufen; Feng, Xueshang; Zhao, Xinhua |
| 刊名 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
 |
| 出版日期 | 2014 |
| 卷号 | 119期号:12 |
| ISSN号 | 2169-9380 |
| 通讯作者 | Feng, XS (reprint author), Chinese Acad Sci, Ctr Space Sci & Appl Res, State Key Lab Space Weather, SIGMA Weather Grp, Beijing, Peoples R China. |
| 英文摘要 | The coronal mass ejection (CME) event on 3 April 2010 is the first fast CME observed by STEREO Sun Earth Connection Coronal and Heliospheric Investigation/Heliospheric Imager for the full Sun-Earth line. Such an event provides us a good opportunity to study the propagation and evolution of CME from the Sun up to 1 AU. In this paper, we study the time-dependent evolution and propagation of this event from the Sun to Earth using the 3-D SIP-CESE (Solar-InterPlanetary Conservation Element and Solution Element) MHD model. The CME is initiated by a simple spherical plasmoid model: a spheromak magnetic structure with high-speed, high-pressure, and high-plasma density plasmoid. The simulation performs a comprehensive study on the CME by comparing the simulation results with STEREO and Wind observations. It is confirmed from the comparison with observations that the MHD model successfully reproduces many features of both the fine solar coronal structure and the typical large-scale structure of the shock propagation and gives the shock arrival time at Earth with an error of similar to 2 h. Then we analyze in detail the several factors affecting the CME's geo-effectiveness: the CME's propagation trajectory, span angle, and velocity. |
| 收录类别 | SCI |
| 语种 | 英语 |
| 源URL | [http://ir.nssc.ac.cn/handle/122/4501]  |
| 专题 | 国家空间科学中心_空间科学部 |
| 推荐引用方式 GB/T 7714 | Zhou, Yufen,Feng, Xueshang,Zhao, Xinhua. Using a 3-D MHD simulation to interpret propagation and evolution of a coronal mass ejection observed by multiple spacecraft: The 3 April 2010 event[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2014,119(12). |
| APA | Zhou, Yufen,Feng, Xueshang,&Zhao, Xinhua.(2014).Using a 3-D MHD simulation to interpret propagation and evolution of a coronal mass ejection observed by multiple spacecraft: The 3 April 2010 event.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,119(12). |
| MLA | Zhou, Yufen,et al."Using a 3-D MHD simulation to interpret propagation and evolution of a coronal mass ejection observed by multiple spacecraft: The 3 April 2010 event".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 119.12(2014). |
入库方式： OAI收割
来源：国家空间科学中心
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