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	1.8-m solar telescope in China: Chinese Large Solar Telescope
	Rao, Changhui1,2; Gu, Naiting1,2; Zhu, Lei1,2; Huang, Jinlong1; Li, Cheng1,2; Cheng, Yuntao1; Liu, Yangyi1,2,3; Cao, Xuedong1; Zhang, Ming1; Zhang, Lanqiang1,2,3
刊名	Journal of Astronomical Telescopes, Instruments, and Systems
	2015
卷号	1期号:2
ISSN号	2329-4124
通讯作者	Gu, Naiting (gunaiting@ioe.ac.cn)
中文摘要	For better understanding and forecasting of solar activity, high resolution observations for the Sun are needed. Therefore, the Chinese Large Solar Telescope (CLST) with a 1.8-m aperture is being built. The CLST is a classic Gregorian configuration telescope with an open structure, alt-azimuth mount, retractable dome, and a large mechanical de-rotator. The optical system with an all reflective design has a field of view of larger than 3 arc-min. The 1.8-m primary mirror is a honeycomb sandwich fused silica lightweight mirror with an ultra lower expansion material and active cooling. The adaptive optics system will be developed to provide the capability for diffraction-limited observations at visible wavelengths. The CLST design and development phase began in 2011 and 2012, respectively. We plan for the CLST's start of commission to be in 2017. A multiwavelength tomographic imaging system, ranging from visible to near-infrared, is considered as the first light scientific instrument. The main system configuration and the corresponding postfocal instruments are described. Furthermore, the latest progress and current status of the CLST are also reported. © 2015 Society of Photo-Optical Instrumentation Engineers (SPIE).
英文摘要	For better understanding and forecasting of solar activity, high resolution observations for the Sun are needed. Therefore, the Chinese Large Solar Telescope (CLST) with a 1.8-m aperture is being built. The CLST is a classic Gregorian configuration telescope with an open structure, alt-azimuth mount, retractable dome, and a large mechanical de-rotator. The optical system with an all reflective design has a field of view of larger than 3 arc-min. The 1.8-m primary mirror is a honeycomb sandwich fused silica lightweight mirror with an ultra lower expansion material and active cooling. The adaptive optics system will be developed to provide the capability for diffraction-limited observations at visible wavelengths. The CLST design and development phase began in 2011 and 2012, respectively. We plan for the CLST's start of commission to be in 2017. A multiwavelength tomographic imaging system, ranging from visible to near-infrared, is considered as the first light scientific instrument. The main system configuration and the corresponding postfocal instruments are described. Furthermore, the latest progress and current status of the CLST are also reported. © 2015 Society of Photo-Optical Instrumentation Engineers (SPIE).
学科主题	Adaptive optics - Fused silica - Infrared devices - Mirrors - Optical systems - Solar energy - Tomography
收录类别	EI
语种	英语
内容类型	期刊论文
源URL	[http://ir.ioe.ac.cn/handle/181551/6421]
专题	光电技术研究所_自适应光学技术研究室（八室）
作者单位	1.Chinese Academy of Sciences, Institute of Optics and Electronics, No. 1 Guangdian Road, Shuangliu County, Chengdu, China 2.Chinese Academy of Sciences, Key Laboratory on Adaptive Optics, No. 1 Guangdian Road, Shuangliu County, Chengdu, China 3.University of Chinese Academy of Sciences, No.19A Yuquan Road, Beijing, China
推荐引用方式 GB/T 7714	Rao, Changhui,Gu, Naiting,Zhu, Lei,et al. 1.8-m solar telescope in China: Chinese Large Solar Telescope[J]. Journal of Astronomical Telescopes, Instruments, and Systems,2015,1(2).
APA	Rao, Changhui.,Gu, Naiting.,Zhu, Lei.,Huang, Jinlong.,Li, Cheng.,...&Li, Mei.(2015).1.8-m solar telescope in China: Chinese Large Solar Telescope.Journal of Astronomical Telescopes, Instruments, and Systems,1(2).
MLA	Rao, Changhui,et al."1.8-m solar telescope in China: Chinese Large Solar Telescope".Journal of Astronomical Telescopes, Instruments, and Systems 1.2(2015).

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