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Piecewise mass flows within a solar prominence observed by the New Vacuum Solar Telescope
Li HB(李洪波)1,2,3; Liu Y(刘煜)1,2; Kuan Vai Tam4; Zhao MY(赵明宇)1; Zhang XF(张雪飞)1
发表期刊ASTROPHYSICS AND SPACE SCIENCE
2018-06-01
卷号363期号:6页码:5
DOI10.1007/s10509-018-3342-x
产权排序第1完成单位
收录类别SCI
关键词Sun: activity Sun: filaments, prominences Sun: magnetic fields
摘要

The material of solar prominences is often observed in a state of flowing. These mass flows (MF) are important and useful for us to understand the internal structure and dynamics of prominences. In this paper, we present a high resolution H alpha observation of MFs within a quiescent solar prominence. From the observation, we find that the plasma primarily has a circular motion and a downward motion separately in the middle section and legs of the prominence, which creates a piecewise mass flow along the observed prominence. Moreover, the observation also shows a clear displacement of MF's velocity peaks in the middle section of the prominence. All of these provide us with a detailed record of MFs within a solar prominence and show a new approach to detecting the physical properties of prominence.

资助项目National Scientific Foundation of China (NSFC)[11533009] ; National Scientific Foundation of China (NSFC)[11603074] ; National Scientific Foundation of China (NSFC)[11503084] ; National Scientific Foundation of China (NSFC)[11773068] ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; Macao Science and Technology Development Fund[FDCT-16-003-SSI] ; Group for Innovation of Yunnan Province
项目资助者National Scientific Foundation of China (NSFC)[11533009, 11603074, 11503084, 11773068] ; Key Laboratory of Geospace Environment, CAS, University of Science & Technology of China ; Macao Science and Technology Development Fund[FDCT-16-003-SSI] ; Group for Innovation of Yunnan Province
语种英语
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
学科门类理学 ; 理学::天文学
文章类型Article
出版者SPRINGER
出版地VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS
ISSN0004-640X
URL查看原文
WOS记录号WOS:000460284100001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]FLUX ROPE ; HINODE/SOT ; ERUPTION
引用统计
被引频次:3[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/19496
专题选址与日冕观测组
通讯作者Li HB(李洪波)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China
2.Key Laboratory of Geospace Environment, Chinese Academy of Sciences, University of Science & Technology of China, Hefei, 230026, China
3.University of Chinese Academy of Sciences, Beijing 100049, China
4.Space Science Institute, Macau University of Science and Technology, Avenida Wai Long, Taipa, Macau, 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
推荐引用方式
GB/T 7714
Li HB,Liu Y,Kuan Vai Tam,et al. Piecewise mass flows within a solar prominence observed by the New Vacuum Solar Telescope[J]. ASTROPHYSICS AND SPACE SCIENCE,2018,363(6):5.
APA Li HB,Liu Y,Kuan Vai Tam,Zhao MY,&Zhang XF.(2018).Piecewise mass flows within a solar prominence observed by the New Vacuum Solar Telescope.ASTROPHYSICS AND SPACE SCIENCE,363(6),5.
MLA Li HB,et al."Piecewise mass flows within a solar prominence observed by the New Vacuum Solar Telescope".ASTROPHYSICS AND SPACE SCIENCE 363.6(2018):5.
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