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A Confined Partial Eruption of Double-decker Filaments
Zheng,Ruisheng7; Yang,Shuhong1,2; Rao,Changhui3,4; Liu,Yangyi3,4; Zhong,Libo3,4; Wang,Bing7; Song,Hongqiang7; Li,Zhen5,6; Chen,Yao7
刊名The Astrophysical Journal
2019-04-17
卷号875期号:1
关键词Sun: activity Sun: corona Sun: filaments, prominences
ISSN号0004-637X
DOI10.3847/1538-4357/ab0f3f
英文摘要Abstract Filament eruptions, one of the most energetic explosions on the Sun, release large quantities of magnetized plasma into the interplanetary space. Hence, the understanding of the initiation and evolution of filament eruptions can provide broader implications for space weather and geospace climate. Here, we present a confined partial eruption of double-decker structure that consisted of two vertically separated filaments on 2016 April 16. Only the upper filament erupted, and the eruption was closely associated with an episode of flux cancellation, surrounding transient brightenings, and unambiguous tether-cutting reconnections of the overlying sheared loops. However, the lower filament was nearly intact through the eruption. Interestingly, the erupting material moved along large-scale external loops and eventually arrived at remote sites, indicating a confined partial eruption. All the results show that the partial eruption involved two magnetic reconnections at least, and the bottom magnetic cancellation and internal tether-cutting reconnections between filaments both play critical roles in triggering the eruption. We conjecture that the newly formed low-lying loops due to tether-cutting reconnections and the flare loops resulting from the partial eruption likely contribute to maintaining the equilibrium of the lower filament. It is also suggested that the restriction of some large-scale external magnetic structures is crucial to turn the successful partial eruption into a confined event.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-875-1-AB0F3F
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/26018]  
专题中国科学院国家天文台
作者单位1.CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
3.The Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, P.O. Box 350, Shuangliu, Chengdu 610209, Sichuan, People's Republic of China
4.The Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, P.O. Box 350, Shuangliu, Chengdu 610209, Sichuan, People's Republic of China
5.School of Astronomy and Space Science, Nanjing University, Nanjing 210023, People’s Republic of China
6.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210023, People’s Republic of China
7.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, and Institute of Space Sciences, Shandong University, 264209 Weihai, People's Republic of China; ruishengzheng@sdu.edu.cn, chrao@ioe.ac.cn
推荐引用方式
GB/T 7714
Zheng,Ruisheng,Yang,Shuhong,Rao,Changhui,et al. A Confined Partial Eruption of Double-decker Filaments[J]. The Astrophysical Journal,2019,875(1).
APA Zheng,Ruisheng.,Yang,Shuhong.,Rao,Changhui.,Liu,Yangyi.,Zhong,Libo.,...&Chen,Yao.(2019).A Confined Partial Eruption of Double-decker Filaments.The Astrophysical Journal,875(1).
MLA Zheng,Ruisheng,et al."A Confined Partial Eruption of Double-decker Filaments".The Astrophysical Journal 875.1(2019).
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