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A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event
Miao YH(苗玉虎)1,2,3; Liu Y(刘煜)1; Li HB(李洪波)1,3; Shen YD(申远灯)1,4,5; Yang, S.5; Elmhamdi, A.6; Kordi, A. S.6; Abidin, Z. Z.7
发表期刊ASTROPHYSICAL JOURNAL
2018-12-10
卷号869期号:1页码:12
DOI10.3847/1538-4357/aaeac1
产权排序第1完成单位
收录类别SCI
关键词magnetic reconnection Sun: activity Sun: coronal mass ejections (CMEs) Sun: magnetic fields
摘要

In this paper, we present a detailed analysis of a coronal blowout jet eruption that was associated with an obvious extreme-ultraviolet (EUV) wave and one complicated coronal mass ejection (CME) event based on the multiwavelength and multi-view-angle observations from the Solar Dynamics Observatory and the Solar Terrestrial Relations Observatory. It is found that the triggering of the blowout jet was due to the emergence and cancellation of magnetic fluxes on the photosphere. During the rising stage of the jet, the EUV wave appeared just ahead of the jet top, lasting about 4 minutes and at a speed of 458-762 kms(-1). In addition, obvious dark material is observed along the EUV jet body, which confirms the observation of a mini-filament eruption at the jet base in the chromosphere. Interestingly, two distinct but overlapped CME structures can be observed in corona together with the eruption of the blowout jet. One is a narrow jet shape, while the other one is a bubble shape. The jet-shaped component was unambiguously related to the outwardly running jet itself, while the bubble-like one might either be produced due to the reconstruction of the high coronal fields or by the internal reconnection during the mini-filament ejection according to the double-CME blowout jet model first proposed by Shen et al., suggesting more observational evidence should be supplied to clear the current ambiguity based on large samples of blowout jets in future studies.

资助项目National Scientific Foundation of China (NSFC)[11533009] ; National Scientific Foundation of China (NSFC)[11773068] ; Specialized Research Fund for Shandong Provincial Key Laboratory ; project of the Group for Innovation of Yunnan Province ; Strategic Priority Research Program of CAS[XDA-17040507] ; University of Malaya Faculty of Science grant[GPF040B-2018] ; King Saud University, Deanship of Scientific Research, College of Science Research Center
项目资助者National Scientific Foundation of China (NSFC)[11533009, 11773068] ; Specialized Research Fund for Shandong Provincial Key Laboratory ; project of the Group for Innovation of Yunnan Province ; Strategic Priority Research Program of CAS[XDA-17040507] ; University of Malaya Faculty of Science grant[GPF040B-2018] ; King Saud University, Deanship of Scientific Research, College of Science Research Center
语种英语
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
学科门类理学 ; 理学::天文学
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:000452824300007
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]X-RAY JETS ; H-ALPHA SURGES ; EMERGING FLUX ; MAGNETIC RECONNECTION ; ACTIVE-REGION ; WHITE-LIGHT ; EUV WAVE ; SOLAR ; DICHOTOMY ; EMERGENCE
引用统计
被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/18644
专题选址与日冕观测组
通讯作者Miao YH(苗玉虎)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, People's Republic of China
2.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment Shandong University, Weihai, 264209, People's Republic of China
3.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing, 100012, People's Republic of China
5.CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Beijing 100012, People's Republic of China
6.Department of Physics and Astronomy, King Saud University, P.O. Box 2455, Riyadh 11451, Saudi Arabia
7.Radio Cosmology Lab, Department of Physics, Faculty of Science, University of Malaya, 50603 Kuala Lumpur, Malaysia
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GB/T 7714
Miao YH,Liu Y,Li HB,et al. A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event[J]. ASTROPHYSICAL JOURNAL,2018,869(1):12.
APA Miao YH.,Liu Y.,Li HB.,Shen YD.,Yang, S..,...&Abidin, Z. Z..(2018).A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event.ASTROPHYSICAL JOURNAL,869(1),12.
MLA Miao YH,et al."A Blowout Jet Associated with One Obvious Extreme-ultraviolet Wave and One Complicated Coronal Mass Ejection Event".ASTROPHYSICAL JOURNAL 869.1(2018):12.
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