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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
Source PublicationASTROPHYSICAL JOURNAL
2018-12-10
Volume869Issue:1Pages:12
DOI10.3847/1538-4357/aaeac1
Contribution Rank第1完成单位
Indexed BySCI
Keywordmagnetic reconnection Sun: activity Sun: coronal mass ejections (CMEs) Sun: magnetic fields
Abstract

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.

Funding ProjectNational 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
Funding OrganizationNational 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
Language英语
Subject Area天文学 ; 太阳与太阳系 ; 太阳物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS IDWOS:000452824300007
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordX-RAY JETS ; H-ALPHA SURGES ; EMERGING FLUX ; MAGNETIC RECONNECTION ; ACTIVE-REGION ; WHITE-LIGHT ; EUV WAVE ; SOLAR ; DICHOTOMY ; EMERGENCE
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/18644
Collection选址与日冕观测组
Corresponding AuthorMiao YH(苗玉虎)
Affiliation1.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
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
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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