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A MICRO CORONAL MASS EJECTION ASSOCIATED BLOWOUT EXTREME-ULTRAVIOLET JET
Hong JC(洪俊超); Jiang YC(姜云春); Zheng RS(郑瑞生); Yang JY(杨家艳); Bi Y(毕以); Yang B(杨波); Hong, JC (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China.
Source PublicationASTROPHYSICAL JOURNAL LETTERS
2011-09-10
Volume738Issue:2
DOI10.1088/2041-8205/738/2/L20
Contribution Rank第1完成单位
Indexed BySCI
KeywordSun: Coronal Mass Ejections (Cmes) Sun: Surface Magnetism Sun: Filaments Prominences
AbstractThe so-called mini coronal mass ejections (CMEs) were recently identified as small-scale eruptive events showing the same on-disk characteristics as large-scale CMEs, and Moore et al. further found that one-third of polar X-ray jets are the so-called blowout jets, in which the jet-base magnetic arch, often carrying a filament, undergoes a miniature version of the blowout eruptions that produce major CMEs. By means of the two viewpoint observations from the Solar Dynamics Observatory (SDO) and the Ahead of Solar Terrestrial Relations Observatory (STEREO A), in this Letter, we present the first observations that a blowout jet from the eruption of an EUV mini-filament channel in the quiet Sun was indeed associated with a real micro-CME. Captured by the on-disk SDO observations, the whole life of the mini-filament channel, from the formation to eruption, was associated with convergences and cancellations of opposite-polarity magnetic flux in the photosphere, and its eruption was accompanied by a small flare-like brightening, a small corona dimming, and posteruptive loops. The near-limb counterpart of the eruption observed by STEREO A, however, showed up as a small EUV jet followed by a white-light jet. These observations not only confirm the previous results that mini-filaments have characteristics common to large-scale ones, but also give clear evidences that blowout jets can result from the eruptions of mini-filaments and are associated with mini-CME.
Funding Organization973 Program [2011CB811403] ; Natural Science Foundation of China [10973038] ; Scientific Application Foundation of Yunnan Province [2007A112M, 2007A115M]
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN2041-8205
URL查看原文
Archive Date2011-11-25
WOS IDWOS:000294760700004
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordH-ALPHA SURGES ; QUIET SUN ; NONRADIAL ERUPTION ; WHITE-LIGHT ; FILAMENT ; FLUX ; STEREO
Citation statistics
Cited Times:54[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6175
Collection太阳物理研究组
Corresponding AuthorHong, JC (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China.
AffiliationNational Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Hong JC,Jiang YC,Zheng RS,et al. A MICRO CORONAL MASS EJECTION ASSOCIATED BLOWOUT EXTREME-ULTRAVIOLET JET[J]. ASTROPHYSICAL JOURNAL LETTERS,2011,738(2).
APA Hong JC.,Jiang YC.,Zheng RS.,Yang JY.,Bi Y.,...&Hong, JC .(2011).A MICRO CORONAL MASS EJECTION ASSOCIATED BLOWOUT EXTREME-ULTRAVIOLET JET.ASTROPHYSICAL JOURNAL LETTERS,738(2).
MLA Hong JC,et al."A MICRO CORONAL MASS EJECTION ASSOCIATED BLOWOUT EXTREME-ULTRAVIOLET JET".ASTROPHYSICAL JOURNAL LETTERS 738.2(2011).
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