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Numerical simulation and data analysis of the 23 July 2012 SEP event observed by ACE, STEREO-A, and STEREO-B
Alternative TitleWOS:000536189300012;20203008959494
Qin, G.; Qi, S. -Y.
Source PublicationASTRONOMY & ASTROPHYSICS
2020
Volume637Pages:A48
DOI10.1051/0004-6361/201936786
ISSN0004-6361
Language英语
Keywordshock waves turbulence scattering Sun coronal mass ejections (CMEs) Sun particle emission CORONAL MASS EJECTION SOLAR ENERGETIC PARTICLES HYDROMAGNETIC WAVE EXCITATION CHARGED-PARTICLES DRIVEN SHOCKS PERPENDICULAR DIFFUSION INTERPLANETARY SHOCKS ION-ACCELERATION COSMIC-RAYS PROPAGATION
AbstractAn extremely powerful, superfast interplanetary coronal mass ejection (ICME) from the Sun on 23 July 2012 was detected by widely separated multiple spacecraft, namely STEREO-A, STEREO-B, and ACE, together with the ICME-driven shock and associated solar energetic particles (SEPs). We use the Parker spiral magnetic field model to analyze the relationship between the propagation of the shock and the SEP flux. Furthermore, we simulate the SEP event by numerically solving the three-dimensional focused transport equation of SEPs considering the shock as the moving source of energetic particles. To deal with the fact that protons and electrons behave completely differently for both parallel and perpendicular diffusion, for simplicity, we use the same diffusion model format for the simulations of protons and electrons but with different parameters. We find that the analysis can qualitatively explain the important features of the SEP flux observed by the multiple spacecraft simultaneously. In addition, the numerical results for both energetic protons and electrons approximately agree with multi-spacecraft observations.
Indexed BySCI ; EI
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Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/7691
Collection中国科学院国家空间科学中心
Affiliation1.[Qin, G.] Harbin Inst Technol, Sch Sci, Shenzhen 518055, Peoples R China
2.[Qi, S. -Y.] Henan Agr Univ, Coll Sci, Zhengzhou 450002, Peoples R China
3.[Qi, S. -Y.] Chinese Acad Sci, State Key Lab Space Weather, Natl Space Sci Ctr, Beijing 100190, Peoples R China
4.[Qi, S. -Y.] Univ Chinese Acad Sci, Coll Earth Sci, Beijing 100049, Peoples R China
Recommended Citation
GB/T 7714
Qin, G.,Qi, S. -Y.. Numerical simulation and data analysis of the 23 July 2012 SEP event observed by ACE, STEREO-A, and STEREO-B[J]. ASTRONOMY & ASTROPHYSICS,2020,637:A48.
APA Qin, G.,&Qi, S. -Y..(2020).Numerical simulation and data analysis of the 23 July 2012 SEP event observed by ACE, STEREO-A, and STEREO-B.ASTRONOMY & ASTROPHYSICS,637,A48.
MLA Qin, G.,et al."Numerical simulation and data analysis of the 23 July 2012 SEP event observed by ACE, STEREO-A, and STEREO-B".ASTRONOMY & ASTROPHYSICS 637(2020):A48.
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