| The interaction and evolution of interplanetary shocks from 1 to beyond 60 AU | |
| Wang, C.; Richardson, J. D. | |
| Department | 空间天气学国家重点实验室 |
| Source Publication | Solar wind ten, proceedings |
| 2003 | |
| Pages | 725-728 |
| Language | 英语 |
| ISBN | 0094-243X;0-7354-0148-9 |
| Abstract | During the current solar maximum (Cycle 23), several major CMEs associated with solar flares produced large transient flows and shocks which were observed by widely-separated spacecraft such as Wind at Earth and Voyager 2 beyond 60 AU. Using data from these spacecraft and numerical models, we study shock propagation and interaction in the outer heliosphere. We demonstrate that a strong shock in the distant heliosphere could be an outer heliospheric remnant of a strong shock in the inner heliosphere ("one to one" relationship), or it could be an outcome of the successive interaction and merging of a series of interplanetary shocks ("one to many" relationship). |
| Conference Name | 10th International Solar Wind Conference |
| Conference Date | 2003 |
| Conference Place | Pisa, Italy |
| Indexed By | EI ; CPCI |
| Document Type | 会议论文 |
| Identifier | http://ir.nssc.ac.cn/handle/122/916 |
| Collection | 空间科学部 |
| Recommended Citation GB/T 7714 | Wang, C.,Richardson, J. D.. The interaction and evolution of interplanetary shocks from 1 to beyond 60 AU[C]. MELVILLE:Amer Inst Physics,2003:725-728. |
| Files in This Item: | Download All | |||||
| File Name/Size | DocType | Version | Access | License | ||
| 2003725728.pdf（316KB） | 会议论文 | 开放获取 | CC BY-NC-SA | View Download | ||
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