From NVST to CGST

	From NVST to CGST
	Liu Z(刘忠)
	2014-10
会议名称	7th Solar Polarization Workshop (SPW7)
会议日期	2013-09-09
会议地点	Kunming, PEOPLES R CHINA
卷号	489
页码	247-262
英文摘要	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.
收录类别	CPCI
产权排序	第一完成单位
会议网址	http://adsabs.harvard.edu/abs/2014ASPC..489..247L
会议录	Astronomical Society of the Pacific (ASP) Conference Series - SOLAR POLARIZATION 7
会议录出版者	ASTRONOMICAL SOC PACIFIC
会议录出版地	390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
学科主题	Astronomy & Astrophysics
语种	英语
ISBN号	978-1-58381-863-3; 978-1-58381-862-6
WOS记录号	WOS:000370308600024
研究领域[WOS]	Astronomy & Astrophysics
内容类型	会议论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/9657]
专题	云南天文台_抚仙湖太阳观测站
作者单位	Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, China
推荐引用方式 GB/T 7714	Liu Z. From NVST to CGST[C]. 见:7th Solar Polarization Workshop (SPW7). Kunming, PEOPLES R CHINA. 2013-09-09.http://adsabs.harvard.edu/abs/2014ASPC..489..247L.