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New vacuum solar telescope and observations with high resolution

查看全文 作  者:Zhong [1]Liu;Jun [1]Xu;Bo-Zhong [2]Gu;Sen [3]Wang;Jian-Qi [4]You;Long-Xiang [3]Shen;Ru-Wei [1]Lu;Zhen-Yu [1]Jin;Lin-Fei [1]Chen;Ke [1]Lou;Zhi [1]Li;Guang-Qian [1]Liu;Zhi [1]Xu;Chang-Hui [5]Rao;Qi-Qian [2]Hu;Ru-Feng [1]Li;Hao-Wen [1]Fu;Feng [6]Wang;Men-Xian [1]Bao;Ming-Chan [1]Wu;Bo-Rong [1]Zhang 高影响力作者 机构地区:[1]Yunnan Observatories Chinese Academy of Sciences;[2]Nanjing Institute of Astronomical Optics & Technology, National Astronomical Observatories,Chinese Academy of Sciences;[3]National Astronomical Observatories, Chinese Academy of Sciences;[4]Purple Mountain Observatory, Chinese Academy of Sciences;[5]Institute of Optics and Electronics, Chinese Academy of Sciences;[6]Kunming University of Science and Technology高影响力机构 出  处:《Research in Astronomy and Astrophysics》索引2014年第14卷第6期,共14页高影响力期刊 基  金:Supported by the National Natural Science Foundation of China 摘  要:The New Vacuum Solar Telescope(NVST) is a one meter vacuum solar telescope that aims to observe fine structures on the Sun. The main goals of NVST are high resolution imaging and spectral observations, including measurements of the solar magnetic field. NVST is the primary ground-based facility used by the Chinese solar research community in this solar cycle. It is located by Fuxian Lake in southwest China, where the seeing is good enough to perform high resolution observations. We first introduce the general conditions at the Fuxian Solar Observatory and the primary science cases of NVST. Then, the basic structures of this telescope and instruments are described in detail. Finally, some typical high resolution data of the solar photosphere and chromosphere are also shown. 关 键 词:高分辨率成像 太阳望远镜 光谱观测 真空 中国西南地区 太阳活动周期 太阳观测站 精细结构
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