Magnetic reconnection phenomena in interplanetary space
文献类型：会议论文
| 作者 | Wei, F. S.; Hu, Q.; Feng, X. S.; Fan, Q. L. |
| 出版日期 | 2003 |
| 会议名称 | World Space Environment Forum (WSEF2002) |
| 会议日期 | 2003 |
| 会议地点 | Adelaide, Australia |
| 关键词 | interplanetary magnetic reconnection observational evidence numerical simulation |
| 页码 | 107-110 |
| 英文摘要 | Interplanetary magnetic reconnection(IMR) phenomena are explored based on the observational data with various time resolutions from Helios, IMP-8, ISEE3, Wind, etc. We discover that the observational evidence of the magnetic reconnection may be found in the various solar wind structures, such as at the boundary of magnetic cloud, near the current sheet, and small-scale turbulence structures, etc. We have developed a third order accuracy upwind compact difference scheme to numerically study the magnetic reconnection phenomena with high-magnetic Reynolds number (R-M = 2000-10000) in interplanetary space. The simulated results show that the magnetic reconnection process could occur under the typical interplanetary conditions. These obtained magnetic reconnection processes own basic characteristics of the high RM reconnection in interplanetary space, including multiple X-line reconnection, vortex velocity structures, filament current systems, splitting, collapse of plasma bulk, merging and evolving of magnetic islands, and lifetime in the range from minutes to hours, etc. These results could be helpful for further understanding the interplanetary basic physical processes. |
| 收录类别 | CPCI |
| 会议录 | Space science reviews
 |
| 会议录出版者 | Kluwer Academic Publ |
| 学科主题 | 空间物理 |
| 会议录出版地 | DORDRECHT |
| 语种 | 英语 |
| ISBN号 | 0038-6308 |
| 源URL | [http://ir.cssar.ac.cn/handle/122/936]  |
| 专题 | 国家空间科学中心_空间科学部 |
| 推荐引用方式 GB/T 7714 | Wei, F. S.,Hu, Q.,Feng, X. S.,et al. Magnetic reconnection phenomena in interplanetary space[C]. 见:World Space Environment Forum (WSEF2002). Adelaide, Australia. 2003. |
入库方式： OAI收割
来源：国家空间科学中心
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。