中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 云南天文台
  3. 中国科学院云南天文台
  4. 抚仙湖太阳观测站
Multiwavelength Observations for a Double-decker Filament Channel in AR 13102

文献类型：期刊论文

作者Zhang, Yin4,5; Tan, Baolin3,4,5; Wang, Quan3,4,5; Huang, Jing3,4,5; Xu Z(徐喆)2; Ji KF(季凯帆)2; Yang, Xiao4,5; Chen, Jie4,5; Bai, Xianyong3,4,5; Hou, Zhenyong1
刊名ASTROPHYSICAL JOURNAL
出版日期2024-09-01
卷号973期号:1
ISSN号0004-637X
DOI10.3847/1538-4357/ad5d70
产权排序第4完成单位
文献子类Article
英文摘要We present the observational evidence of the existence of a double-decker filament channel (FC) by using observations in extreme ultraviolet and H alpha wavelengths. For both FCs, the east foot-point roots in the active region (AR), while the west one roots in the remote quiet region. The bottom FC (FC1) appears as intermittent filaments. Within the AR, the FC1 appears as an S-shaped filament (F1), which consisted of two J-shaped filaments (F1S/F1N for the south/north one). For the upper one (FC2), only the east part is filled with dark plasma and visible as a small filament (F2). Its east foot-point roots around the junction of F1S and F1N. Initially, due to the recurrent reconnections, F1N and F1S link to each other and form a new filament (F3) thread by thread. Meanwhile, the heated plasma, which appears as brightening features, flows from the east foot-point of F2 to the west, and becomes invisible about 1.1 x 105 km away. The failed eruption of F1S is triggered by the reconnection, which appears as the brightening threads changing their configuration from crossed to quasiparallel in between the F1S and F3, and is confined by the upper magnetic field. Associated with the eruption, the distant invisible plasma becomes visible as a brightening feature. It continuously flows to the remote foot-point, and becomes invisible before reaching it. The brightening plasma flow outlines the skeleton of FC2 gradually. The observations show the existence of a double-decker FC, as a magnetic structure, before they appear as a brightening/dark feature when fully filled with hot/cool plasma.
学科主题天文学 ; 太阳与太阳系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词ACTIVE-REGION FILAMENT ; VACUUM SOLAR TELESCOPE ; FLUX-ROPE ; PARTIAL ERUPTION ; MAGNETIC RECONNECTION ; SMALL-SCALE ; SLOW RISE ; DRIVEN ; EVOLUTION ; MOTION
资助项目National Key R&D Program of China[2022YFF0503800]; National Key R&D Program of China[2021YFA1600500]; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009]; NSFC[12373058]; NSFC[12173050]; NSFC[12003048]; NSFC[12373115]; NSFC[12203097]; Beijing Natural Science Foundation[1222029]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560302]; International Partnership Program of Chinese Academy of Sciences[183311KYSB20200003]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001309730700001
出版者IOP Publishing Ltd
资助机构National Key R&D Program of China[2022YFF0503800, 2021YFA1600500] ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009] ; NSFC[12373058, 12173050, 12003048, 12373115, 12203097] ; Beijing Natural Science Foundation[1222029] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560302] ; International Partnership Program of Chinese Academy of Sciences[183311KYSB20200003]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27590]  
专题云南天文台_抚仙湖太阳观测站
天文技术实验室
作者单位1.School of Earth and Space Sciences, Peking University, Beijing 100871, People's Republic of China
2.Yunnan Astronomical Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
3.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
4.Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, People's Republic of China;
5.CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China;
推荐引用方式
GB/T 7714		 Zhang, Yin,Tan, Baolin,Wang, Quan,et al. Multiwavelength Observations for a Double-decker Filament Channel in AR 13102[J]. ASTROPHYSICAL JOURNAL,2024,973(1).
APA Zhang, Yin.,Tan, Baolin.,Wang, Quan.,Huang, Jing.,徐喆.,...&Deng, Yuanyong.(2024).Multiwavelength Observations for a Double-decker Filament Channel in AR 13102.ASTROPHYSICAL JOURNAL,973(1).
MLA Zhang, Yin,et al."Multiwavelength Observations for a Double-decker Filament Channel in AR 13102".ASTROPHYSICAL JOURNAL 973.1(2024).

入库方式： OAI收割

来源：云南天文台

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。