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On the Determining Physical Factor of Jet-related Coronal Mass Ejections' Morphology in the High Corona
Duan, Yadan1; Shen, Yuandeng2; Tang ZH(汤泽浩)3,4; Zhou CR(周承瑞)3,4; Tan, Song5
发表期刊ASTROPHYSICAL JOURNAL
2024-06-01
卷号968期号:2
DOI10.3847/1538-4357/ad445c
产权排序第3完成单位
收录类别SCI
摘要A solar jet can often cause coronal mass ejections (CMEs) with different morphologies in the high corona, for example, jet-like CMEs, bubble-like CMEs, and so-called twin CMEs that include a pair of simultaneous jet-like and bubble-like CMEs. However, what determines the morphology of a jet-related CME is still an open question. Using high spatiotemporal resolution stereoscopic observations taken by the Solar Dynamics Observatory and the Solar Terrestrial Relations Observatory from 2010 October to 2012 December, we performed a statistical study of jet-related CMEs to study the potential physical factors that determine the morphology of CMEs in the outer corona. Our statistical sample includes 16 jet-related CME events of which seven are twin CME events and nine are jet-like narrow CMEs. We find that all CMEs in our sample were accompanied by filament-driven blowout jets and Type III radio bursts during their initial formation and involved magnetic reconnection between filament channels and the surrounding magnetic fields. Most of our cases occurred in a fan-spine magnetic configuration. Our study suggests that the bubble-like components of twin CMEs lacking an obvious core are related to the expansion of the closed-loop systems next to the fan-spine topology, while the jet-like component is from the coronal extension of the jet plasma along open fields. Based on the statistical results, we conclude that the morphology of jet-related CMEs in the high corona may be related to the filament length and the initial magnetic null point height of the fan-spine structures.
资助项目Beijing Natural Science Foundation[1244053]; National Postdoctoral Programs[GZC20230097]; National Postdoctoral Programs[2023M740112]; Natural Science Foundation of China[12173083]; Natural Science Foundation of China[11922307]; Yunnan Science Foundation for Distinguished Young Scholars[202101AV070004]; National Key R&D Program of China[2019YFA0405000]
项目资助者Beijing Natural Science Foundation[1244053] ; National Postdoctoral Programs[GZC20230097, 2023M740112] ; Natural Science Foundation of China[12173083, 11922307] ; Yunnan Science Foundation for Distinguished Young Scholars[202101AV070004] ; National Key R&D Program of China[2019YFA0405000]
语种英语
学科领域天文学 ; 太阳与太阳系
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001249460000001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]PARTIAL FILAMENT ERUPTION ; X-RAY JETS ; BLOWOUT JET ; STEREOSCOPIC OBSERVATIONS ; 1ST OBSERVATION ; BREAKOUT MODEL ; SOLAR FILAMENT ; ELECTRON-BEAMS ; SPACE WEATHER ; WHITE-LIGHT
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条目标识符http://ir.ynao.ac.cn/handle/114a53/27417
专题选址与日冕观测组
作者单位1.School of Earth and Space Sciences, Peking University, Beijing, 100871, People's Republic of China;
2.Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen 518055, People's Republic of China; [email protected];
3.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, People's Republic of China;
4.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
5.Leibniz Institute for Astrophysics Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
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Duan, Yadan,Shen, Yuandeng,Tang ZH,et al. On the Determining Physical Factor of Jet-related Coronal Mass Ejections' Morphology in the High Corona[J]. ASTROPHYSICAL JOURNAL,2024,968(2).
APA Duan, Yadan,Shen, Yuandeng,汤泽浩,周承瑞,&Tan, Song.(2024).On the Determining Physical Factor of Jet-related Coronal Mass Ejections' Morphology in the High Corona.ASTROPHYSICAL JOURNAL,968(2).
MLA Duan, Yadan,et al."On the Determining Physical Factor of Jet-related Coronal Mass Ejections' Morphology in the High Corona".ASTROPHYSICAL JOURNAL 968.2(2024).
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