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Energy spectral properties of the twin-CME driven shocks
Wang, Xin1,2,3; Yan, Yi Hua2; Ding, Mind De4; Wang, Na1; Hao, Shan1
2017-07-20
Conference Name35th International Cosmic Ray Conference ICRC2017, 10-20 July, 2017
Source Publication35th International Cosmic Ray Conference ICRC2017, 10-20 July, 2017
Pages100
Conference Date20 July, 2017
Correspondent Emailwangxin@xao.ac.cn
Conference PlaceBexco, Busan, Korea
Contribution Rank1
Abstract

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.

Funding OrganizationXinjiang 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)
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Indexed By其他
Language英语
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/1823
Collection光学天文与技术应用研究室
计算机技术应用研究室
其它
Corresponding AuthorWang, Xin
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China
2.CAS Key Laboratory of Solar Activity, NAOC, Beijing 100012, China
3.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China
4.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wang, Xin,Yan, Yi Hua,Ding, Mind De,et al. Energy spectral properties of the twin-CME driven shocks[C],2017:100.
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