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From NVST to CGST
Liu Z(刘忠)
会议录名称Astronomical Society of the Pacific (ASP) Conference Series - SOLAR POLARIZATION 7
2014-10
卷号489
页码247-262
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收录类别CPCI
会议名称7th Solar Polarization Workshop (SPW7)
会议日期2013-09-09
会议地点Kunming, PEOPLES R CHINA
摘要The New Vacuum Solar Telescope (NVST) is a 1 m vacuum solar telescope. The main tasks of NVST are high resolution imaging and spectral observations, including the measurements of solar magnetic field. The Chinese Giant Solar Telescope (CGST) is the next generation ground-based solar telescope proposed by Chinese solar community. The differences between NVST and CGST are not only the differences of performance parameters but also the differences of science goals and the differences in design concepts. In this paper, the information of NVST and CGST are first introduced, including the science goals, the basic structures and typical instruments. Then, the general design principles of the next generation large solar telescope are discussed based on the comparisons and analyses.
语种英语
学科领域Astronomy & Astrophysics
文章类型Proceedings Paper
出版者ASTRONOMICAL SOC PACIFIC
出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN号978-1-58381-863-3; 978-1-58381-862-6
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归档日期2014-12-16
WOS记录号WOS:000370308600024
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR TELESCOPE ; SPECKLE MASKING ; PROGRESS ; CHINA
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文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9657
专题抚仙湖太阳观测站
作者单位Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, China
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Liu Z. From NVST to CGST[C]. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2014:247-262.
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