Ground layer adaptive optics system simulation for the 2.5m telescope in Dome A
Peng Jia ; Sijiong Zhang
2012-09-13
会议日期2012-7-1
会议地点Amsterdam, Netherlands
关键词Antarctic telescope ground layer adaptive optics rotation mirror single laser guide star
卷号8447
期号8447
页码Vol.8447 5J-1-8
英文摘要
The Antarctic is an ideal place for optical and infrared astronomy observations. Chinese scientists are planning to build a 2.5m telescope in Dome A. The telescope will be built in a tower about 15 meters high to avoid the ground layer atmospheric turbulence. The Ground layer Adaptive Optics system (GLAO) will also be suggested to be installed to further reduce the seeing. The GLAO system with one laser guide star, one deformable mirror and one wide field Shack-Hartmann wavefront sensor is designed and simulated. The Strehl ratio has increased 2 to 3 times in visible and infrared band in 20 arc min field of view.
会议主办者The International Society for Optical Engineering
会议录Adaptive Optics Systems III
会议录出版者SPIE
学科主题郭守敬望远镜(LAMOST) ; 自适应光学
内容类型会议论文
源URL[http://ir.niaot.ac.cn/handle/114a32/661]  
专题南京天文光学技术研究所_中科院南京天光所知识成果_会议论文
南京天文光学技术研究所_中科院天文光学技术重点实验室_会议论文
推荐引用方式
GB/T 7714
Peng Jia,Sijiong Zhang. Ground layer adaptive optics system simulation for the 2.5m telescope in Dome A[C]. 见:. Amsterdam, Netherlands. 2012-7-1.
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