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Interaction of Two Active Region Filaments Observed by NVST and SDO
Yang LH(杨丽恒)1,2,3,4; Yan XL(闫晓理)1,3; Li, Ting2,3; Xue ZK(薛志科)1,3; Xiang YY(向永源)1,3
刊名ASTROPHYSICAL JOURNAL
2017-04-01
卷号838期号:2
关键词Sun: activity Sun: corona Sun: filaments, prominences Sun: flares Supporting material: animations
ISSN号0004-637X
通讯作者Yang, Liheng(Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China)
产权排序第1完成单位
英文摘要Using high spatial and temporal resolution Ha data from the New Vacuum Solar Telescope (NVST) and simultaneous observations from the Solar Dynamics Observatory, we present the rare event of the interaction between two filaments (F1 and F2) in AR 11967 on 2014 January 31. The adjacent two filaments were almost perpendicular to each other. Their interaction was driven by the movement of F1 and started when the two filaments collided with each other. During the interaction, the threads of F1 continuously slipped from the northeast to the southwest, and were accompanied by the brightenings at the junction of two filaments and the northeast footpoint of F2. Part of F1 and the main body of F2 became invisible in Ha wavelength due to the heating and the motion of F2. At the same time, bright material initiated from the junction of two filaments were observed to move along F1. The magnetic connectivities of F1 were found to be changed after their interaction. These observations suggest that magnetic reconnection was involved in the interaction of two filaments and resulted in the eruption of one filament.
学科主题天文学
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]CORONAL MASS EJECTIONS ; DYNAMICS-OBSERVATORY SDO ; FLUX ROPE ; MAGNETIC-FIELD ; KINK INSTABILITY ; SPECKLE MASKING ; SOLAR FILAMENT ; ERUPTION ; RECONNECTION ; FLARE
收录类别SCI
原文出处http://stacks.iop.org/0004-637X/838/i=2/a=131?key=crossref.037fe356a1b80daa259d4e626dd35062
语种英语
WOS记录号WOS:000398296700007
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/10020]  
专题云南天文台_抚仙湖太阳观测站
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China
2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
3.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing, 100012, China
4.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210093, China
推荐引用方式
GB/T 7714
Yang LH,Yan XL,Li, Ting,et al. Interaction of Two Active Region Filaments Observed by NVST and SDO[J]. ASTROPHYSICAL JOURNAL,2017,838(2).
APA Yang LH,Yan XL,Li, Ting,Xue ZK,&Xiang YY.(2017).Interaction of Two Active Region Filaments Observed by NVST and SDO.ASTROPHYSICAL JOURNAL,838(2).
MLA Yang LH,et al."Interaction of Two Active Region Filaments Observed by NVST and SDO".ASTROPHYSICAL JOURNAL 838.2(2017).
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