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Primary observations of solar filaments using the multi-channel imaging system of the New Vacuum Solar Telescope
Xu Z(徐稚); Jin ZY(金振宇); Xu FY(许方宇); Liu Z(刘忠); the NVST team
会议录名称Proceedings of the International Astronomical Union (IAU) Symposium - Nature of Prominences and their role in Space Weather
2014-01
卷号300
页码117-120
DOI10.1017/S1743921313010831
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会议名称300th IAU Symposium - Nature of Prominences and their role in Space Weather
会议日期2013-06-10
会议地点Paris, France
关键词Ground-based Solar Facilities The Nvst Solar Prominences
摘要The New Vacuum Solar Telescope (NVST) is a new generation ground-based solar facility of China. One of the post-focus instruments is the multi-channel high-resolution imaging system, which is designed to simultaneously observe the dynamic gas motion in the solar photosphere and chromosphere. Since October of 2010 it has been operational in the NVST and some necessary updates were performed in past 2 years. Here we first give a general introduction of this system, and then we exhibit one near-limb observation of solar filaments obtained using this system. By this communication, we would like to show the potential ability to perform the high resolution observation of solar filaments (prominences) using the multi-channel imaging system in the NVST.
语种英语
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归档日期2015-11-24
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文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9676
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作者单位Fuxian Solar Observatory, Yunnan Observatory, Chinese Academy of Science, Kunming, 650011
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Xu Z,Jin ZY,Xu FY,et al. Primary observations of solar filaments using the multi-channel imaging system of the New Vacuum Solar Telescope[C],2014:117-120.
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