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Successive Two-sided Loop Jets Caused by Magnetic Reconnection between Two Adjacent Filamentary Threads
Tian, Zhanjun1,2,3; Liu, Yu1,4,5; Shen, Yuandeng1,2,4,5,6; Elmhamdi, Abouazza7; Su, Jiangtao3,4,6; Liu, Ying D.2,3; Kordi, Ayman. S.7
2017-08-20
Source PublicationASTROPHYSICAL JOURNAL
Volume845Issue:2
AbstractWe present observational analysis of two successive two-sided loop jets observed by the ground-based New Vacuum Solar Telescope and the space-borne Solar Dynamics Observatory. The two successive two-sided loop jets manifested similar evolution processes and both were associated with the interaction of two small-scale adjacent filamentary threads, magnetic emerging, and cancellation processes at the jet's source region. High temporal and high spatial resolution observations reveal that the two adjacent ends of the two filamentary threads are rooted in opposite magnetic polarities within the source region. The two threads approached each other, and then an obvious brightening patch is observed at the interaction position. Subsequently, a pair of hot plasma ejections are observed heading in opposite directions along the paths of the two filamentary threads at a typical speed for two-sided loop jets of the order 150 km s(-1). Close to the end of the second jet, we report the formation of a bright hot loop structure at the source region, which suggests the formation of new loops during the interaction. Based on the observational results, we propose that the observed two-sided loop jets are caused by magnetic reconnection between the two adjacent filamentary threads, largely different from the previous scenario that a two-sided loop jet is generated by magnetic reconnection between an emerging bipole and the overlying horizontal magnetic fields.
SubtypeArticle
KeywordSun: Activity Sun: Filaments Prominences Sun: Flares Sun: Magnetic Fields
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNatural Science Foundation of China(11533009 ; Natural Science Foundation of China(11533009 ; Yunnan Science Foundation(2015FB191 ; Yunnan Science Foundation(2015FB191 ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; King Saud University, College of Science Research Center ; King Saud University, College of Science Research Center ; 11403097 ; 11403097 ; 2017FB006) ; 2017FB006) ; 11633008) ; 11633008) ; Natural Science Foundation of China(11533009 ; Natural Science Foundation of China(11533009 ; Yunnan Science Foundation(2015FB191 ; Yunnan Science Foundation(2015FB191 ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; King Saud University, College of Science Research Center ; King Saud University, College of Science Research Center ; 11403097 ; 11403097 ; 2017FB006) ; 2017FB006) ; 11633008) ; 11633008)
DOI10.3847/1538-4357/aa8095
WOS KeywordX-RAY JETS ; VACUUM SOLAR TELESCOPE ; H-ALPHA SURGES ; HIGH-RESOLUTION ; ACTIVE-REGION ; CORONAL HOLE ; EUV JETS ; MISSION ; SIMULATIONS ; SPICULES
Indexed BySCI
Language英语
Funding OrganizationNatural Science Foundation of China(11533009 ; Natural Science Foundation of China(11533009 ; Yunnan Science Foundation(2015FB191 ; Yunnan Science Foundation(2015FB191 ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; King Saud University, College of Science Research Center ; King Saud University, College of Science Research Center ; 11403097 ; 11403097 ; 2017FB006) ; 2017FB006) ; 11633008) ; 11633008) ; Natural Science Foundation of China(11533009 ; Natural Science Foundation of China(11533009 ; Yunnan Science Foundation(2015FB191 ; Yunnan Science Foundation(2015FB191 ; Specialized Research Fund for State Key Laboratories ; Specialized Research Fund for State Key Laboratories ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Key Laboratory of Solar Activity of Chinese Academy of Sciences(KLSA201601) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Youth Innovation Promotion Association of Chinese Academy of Sciences(2014047) ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; King Saud University, College of Science Research Center ; King Saud University, College of Science Research Center ; 11403097 ; 11403097 ; 2017FB006) ; 2017FB006) ; 11633008) ; 11633008)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000407801100004
Citation statistics
Cited Times:9[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20083
Collection太阳物理研究部
Affiliation1.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
2.Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R China
3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
4.Chinese Acad Sci, Ctr Astron Mega Sci, Beijing 100012, Peoples R China
5.Univ Sci & Technol China, Chinese Acad Sci, Key Lab Geospace Environm, Hefei 230026, Peoples R China
6.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
7.King Saud Univ, Dept Phys & Astron, POB 2455, Riyadh 11451, Saudi Arabia
Recommended Citation
GB/T 7714
Tian, Zhanjun,Liu, Yu,Shen, Yuandeng,et al. Successive Two-sided Loop Jets Caused by Magnetic Reconnection between Two Adjacent Filamentary Threads[J]. ASTROPHYSICAL JOURNAL,2017,845(2).
APA Tian, Zhanjun.,Liu, Yu.,Shen, Yuandeng.,Elmhamdi, Abouazza.,Su, Jiangtao.,...&Kordi, Ayman. S..(2017).Successive Two-sided Loop Jets Caused by Magnetic Reconnection between Two Adjacent Filamentary Threads.ASTROPHYSICAL JOURNAL,845(2).
MLA Tian, Zhanjun,et al."Successive Two-sided Loop Jets Caused by Magnetic Reconnection between Two Adjacent Filamentary Threads".ASTROPHYSICAL JOURNAL 845.2(2017).
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