| Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14 | |
| Wang, Xin; Yan, Yi-Hua; Wang, X (reprint author), Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Activ, Beijing 100012, Peoples R China. | |
| Department | 空间科学部 |
| Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
 |
| 2012 | |
| Volume | 12Issue:11Pages:1535-1548 |
| ISSN | 1674-4527 |
| Language | 英语 |
| Keyword | Acceleration Of Particles Shock Waves Sun: Coronal Mass Ejections (Cmes) Solar Wind Methods: Numerical |
| Abstract | In a solar flare or coronal mass ejection (CME), observations of the subsequent interplanetary shock provide us with strong evidence of particle acceleration to energies of multiple MeV, even up to GeV. Diffusive shock acceleration is an efficient mechanism for particle acceleration. For investigating the shock structure, the energy injection and energy spectrum of a CME-driven shock, we perform a dynamical Monte Carlo simulation of the CME-driven shock that occurred on 2006 December 14 using an anisotropic scattering law. The simulated results of the shock's fine structure, particle injection, and energy spectrum are presented. We find that our simulation results give a good fit to the observations from multiple spacecraft.; In a solar flare or coronal mass ejection (CME), observations of the subsequent interplanetary shock provide us with strong evidence of particle acceleration to energies of multiple MeV, even up to GeV. Diffusive shock acceleration is an efficient mechanism for particle acceleration. For investigating the shock structure, the energy injection and energy spectrum of a CME-driven shock, we perform a dynamical Monte Carlo simulation of the CME-driven shock that occurred on 2006 December 14 using an anisotropic scattering law. The simulated results of the shock's fine structure, particle injection, and energy spectrum are presented. We find that our simulation results give a good fit to the observations from multiple spacecraft. |
| Indexed By | SCI |
| Funding Project | 中国科学院空间科学与应用研究中心 |
| Document Type | 期刊论文 |
| Identifier | http://ir.nssc.ac.cn/handle/122/3131 |
| Collection | 空间科学部 |
| Corresponding Author | Wang, X (reprint author), Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Activ, Beijing 100012, Peoples R China. |
| Recommended Citation GB/T 7714 | Wang, Xin,Yan, Yi-Hua,Wang, X . Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2012,12(11):1535-1548. |
| APA | Wang, Xin,Yan, Yi-Hua,&Wang, X .(2012).Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,12(11),1535-1548. |
| MLA | Wang, Xin,et al."Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 12.11(2012):1535-1548. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| 201212111535.pdf（493KB） | 开放获取 | CC BY-NC-SA | Application Full Text | |||
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