YNAO OpenIR  > 选址与日冕观测组
Stereoscopic observation of simultaneous longitudinal and transverse oscillations in a single filament driven by two-sided-loop jet
Tan S(谭宋)1,2; Shen YD(申远灯)1,2,3,4; Zhou, Xinping5; Tang ZH(汤泽浩)1,2; Zhou CR(周承瑞)1,2; Duan YD(段雅丹)1,2; Yao SR(姚苏芮)1,2
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023-02-07
卷号520期号:2页码:3080-3088
DOI10.1093/mnras/stad295
产权排序第1完成单位
收录类别SCI ; EI
关键词Sun: atmosphere Sun: filaments/prominences Sun: magnetic fields Sun: oscillations
摘要We report the first observations of simultaneous large-amplitude longitudinal and transverse oscillations of a quiescent filament trigged by a two-sided-loop jet formed by the magnetic reconnection between the filament and an emerging loop in the filament channel, recorded by the Solar Dynamics Observatory and the Solar TErrestrial RElations Observatory . The north arm of the jet firstly pushed the filament mass moving northwardly along the magnetic field lines consisting of the coronal cavity, then some ele v ated filament mass fell back and started to oscillate longitudinally at the bottom of the cavity (i.e. the magnetic dip). The northernmost part of the filament also showed transverse oscillation simultaneously. The amplitude and period of the longitudinal (transverse) oscillation are 12.96 (2.99) Mm and 1.18 (0.33) h, respectively. By using the method of filament seismology, the radius of curvature of the magnetic dip is about 151 Mm, consistent with that obtained by the 3D reconstruction (166 Mm). Using different physical parameters of the observed longitudinal and transverse oscillations, the magnetic field strength of the filament is estimated to be about 23 and 21 Gauss, respectively. By calculating the energy of the moving filament mass, the minimum energy of the jet is estimated to be about 1 . 96 x 10 (28) erg . We conclude that the newly formed jet can not only trigger simultaneous longitudinal and transverse oscillations in a single filament, but also can be used as a seismology tool for diagnosing filament information, such as the magnetic structure, magnetic field strength, and magnetic twists.
资助项目Natural Science Foundation of China[11922307] ; Natural Science Foundation of China[12173083] ; Natural Science Foundation of China[11773068] ; Yunnan Science Foundation for Distinguished Young Scholars[202101AV070004] ; National Key R&D Program of China[2019YFA0405000] ; Specialized Research Fund for State Key Laboratories ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG07009]
项目资助者Natural Science Foundation of China[11922307, 12173083, 11773068] ; Yunnan Science Foundation for Distinguished Young Scholars[202101AV070004] ; National Key R&D Program of China[2019YFA0405000] ; Specialized Research Fund for State Key Laboratories ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG07009]
语种英语
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
文章类型Article
出版者OXFORD UNIV PRESS
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
WOS记录号WOS:000943150500017
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR PROMINENCES ; MAGNETIC RECONNECTION ; MORETON WAVE ; EUV WAVE ; PERIODIC MOTION ; ERUPTIONS ; DYNAMICS ; MODELS ; ORIGIN
EI入藏号20232214166544
EI主题词Seismology
EI分类号484.1 Earthquake Measurements and Analysis - 701.2 Magnetism: Basic Concepts and Phenomena - 723.2 Data Processing and Image Processing
引用统计
被引频次:4[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/25875
专题选址与日冕观测组
通讯作者Tan S(谭宋); Shen YD(申远灯)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China;
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, China;
3.State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing 100190, China;
4.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming, 650216, China;
5.College of Physics and Electronic Engineering, Sichuan Normal University, Chengdu, 610068, China
第一作者单位中国科学院云南天文台
通讯作者单位中国科学院云南天文台
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Tan S,Shen YD,Zhou, Xinping,et al. Stereoscopic observation of simultaneous longitudinal and transverse oscillations in a single filament driven by two-sided-loop jet[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,520(2):3080-3088.
APA Tan S.,Shen YD.,Zhou, Xinping.,Tang ZH.,Zhou CR.,...&Yao SR.(2023).Stereoscopic observation of simultaneous longitudinal and transverse oscillations in a single filament driven by two-sided-loop jet.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,520(2),3080-3088.
MLA Tan S,et al."Stereoscopic observation of simultaneous longitudinal and transverse oscillations in a single filament driven by two-sided-loop jet".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 520.2(2023):3080-3088.
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