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Particles Acceleration in Converged Shocks
Xin Wang1,2,3,4,5; Joe Giacalone2; Yihua Yan3; Mingde Ding4; Na Wang1,5; Hao Shan1,5
2016-07-01
Conference Name41st COSPAR Scientific Assembly, abstracts from the meeting that was to be held 30 July - 7 August at the Istanbul Congress Center (ICC), Turkey, but was cancelled. See http://cospar2016.tubitak.gov.tr/en/, Abstract D2.1-38-16.
Source Publication41st COSPAR Scientific Assembly
Volume41
Conference Date2016-07-01
Correspondent Emailwangxin@xao.ac.cn
Conference PlaceTurkey
Project Number2014211A069
Contribution Rank1
Abstract

Observations show that there is a proton spectral ``break" with E_{break} at 1-10MeV in some large CME-driven shocks. However, the understanding of this energy spectral ``break" from the diffusive shock acceleration theory still remains uncertain. Although previous numerical methods can hardly predict this ``break" from current theoretical models due to high computational expense, the present paper focuses on simulating this energy spectrum in converged two shocks by Monte Carlo numerical method. Considering the Dec 13 2006 CME-driven shock interaction with an Earth bow shock, we examine whether the energy spectral ``break" could occur on an interaction between two shocks. As result, we indeed obtain the maximum proton energy up to 10MeV, and we further find a proton spectral ``break" appears distinctly at the energy ˜5MeV.

Funding OrganizationXinjiang Natural Science Foundation(2014211A069) ; Xinjiang Natural Science Foundation(2014211A069) ; Xinjiang Natural Science Foundation(2014211A069) ; Xinjiang Natural Science Foundation(2014211A069)
KeywordAcceleration Of Particles Methods:Numerical Shock Waves Solar Wind Sun:Coronal Mass Ejections(Cmes)
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Indexed By其他
Language英语
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/1776
Collection其它
光学天文与技术应用研究室
计算机技术应用研究室
Corresponding AuthorXin Wang
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China
2.Lunar and Planetary Laboratory, University of Arizona, Tucson AZ 85721, American
3.Key Laboratory of Solar Activities, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
4.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University)Ministry of Education, Nanjing 210093, China
5.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Xin Wang,Joe Giacalone,Yihua Yan,et al. Particles Acceleration in Converged Shocks[C],2016.
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