Piecewise mass flows within a solar prominence observed by the New Vacuum Solar Telescope
文献类型:期刊论文
作者 | 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 |
刊名 | ASTROPHYSICS AND SPACE SCIENCE |
出版日期 | 2018-06-01 |
卷号 | 363期号:6页码:5 |
ISSN号 | 0004-640X |
关键词 | Sun: activity Sun: filaments, prominences Sun: magnetic fields |
DOI | 10.1007/s10509-018-3342-x |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | 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. |
学科主题 | 天文学 ; 太阳与太阳系 ; 太阳物理学 |
URL标识 | 查看原文 |
出版地 | VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS |
WOS关键词 | FLUX ROPE ; HINODE/SOT ; ERUPTION |
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 |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | SPRINGER |
WOS记录号 | WOS:000460284100001 |
资助机构 | 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 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/19495] |
专题 | 云南天文台_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 |
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. |
入库方式: OAI收割
来源:云南天文台
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