Energy spectral properties of the twin-CME driven shocks | |
Hao, Shan2![]() ![]() ![]() | |
2017-07-20 | |
会议日期 | 20 July, 2017 |
会议地点 | Bexco, Busan, Korea |
页码 | 100 |
英文摘要 | More and more observations show that large ground-level enhancement (GLE) events are often associated with twin coronal mass ejections (CMEs). In the twin-shock scenario, the preceding CME-driven shock provides an enhanced-level turbulence at the upcoming CME-driven shock. In this work, we focus on the GLE event on 2012 May 17, which would be associated with the twinshock interactions. Using the particle simulation method to examine the effect of the preceding CMEs being surrounded by the forthcoming CMEs on the energy spectrum. We use the preceding CMEs-driven shock to produce an enhanced seed population injecting into the later CME-driven shock for particle re-acceleration. As results, we simulate the twin-shock interactions and obtain the compound proton spectrum. Therefore we suggest that the twin-shock interactions would produce an GLE event with an “ankle-like” proton spectral slope. |
产权排序 | 1 |
会议录 | 35th International Cosmic Ray Conference ICRC2017, 10-20 July, 2017
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资助机构 | Xinjiang Natural Science Foundation (No. 2014211A069) ; Korean Federation of Science and Technology Societies ; Xinjiang Natural Science Foundation (No. 2014211A069) ; Korean Federation of Science and Technology Societies ; Xinjiang Natural Science Foundation (No. 2014211A069) ; Korean Federation of Science and Technology Societies ; Xinjiang Natural Science Foundation (No. 2014211A069) ; Korean Federation of Science and Technology Societies ; CAS Key Laboratory of Solar Activity, NAOC ; CAS Key Laboratory of Solar Activity, NAOC ; CAS Key Laboratory of Solar Activity, NAOC ; CAS Key Laboratory of Solar Activity, NAOC ; NSFC(No.11673056) ; NSFC(No.11673056) ; NSFC(No.11673056) ; NSFC(No.11673056) |
语种 | 英语 |
URL标识 | 查看原文 |
内容类型 | 会议论文 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/1823] ![]() |
专题 | 新疆天文台_光学天文与技术应用研究室 新疆天文台_其它 新疆天文台_计算机技术室 |
通讯作者 | Wang, Xin |
作者单位 | 1.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China 2.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China 3.CAS Key Laboratory of Solar Activity, NAOC, Beijing 100012, China 4.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China |
推荐引用方式 GB/T 7714 | Hao, Shan,Wang, Na,Ding, Mind De,et al. Energy spectral properties of the twin-CME driven shocks[C]. 见:. Bexco, Busan, Korea. 20 July, 2017. |
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