Performance modeling of the adaptive optics system on the 2.16 m telescope

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	Performance modeling of the adaptive optics system on the 2.16 m telescope
	JIA Peng ; ZHANG SiJiong
刊名	SCIENCE CHINA Physics, Mechanics & Astronomy
	2013-03
卷号	56 期号:3 页码:658–662
关键词	adaptive and segmented optics optical telescopes Monte Carlo methods computer modeling and simulation
英文摘要	The adaptive optics system on the 2.16 m telescope is modeled and simulated using an ends-to-ends Monte Carlo method in this paper. Under the optimized parameters, the Strehl ratio can be increased from about 0.02 to more than 0.2 in the J, H and K bands with a classical adaptive optics system. Based on the simulation results, the practical system design is also considered and discussed.
学科主题	自适应光学
WOS记录号	WOS:000314912300028
公开日期	2014-02-11
内容类型	期刊论文
源URL	[http://ir.niaot.ac.cn/handle/114a32/734]
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_期刊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_期刊论文
推荐引用方式 GB/T 7714	JIA Peng,ZHANG SiJiong. Performance modeling of the adaptive optics system on the 2.16 m telescope[J]. SCIENCE CHINA Physics, Mechanics & Astronomy,2013,56(3):658–662.
APA	JIA Peng,&ZHANG SiJiong.(2013).Performance modeling of the adaptive optics system on the 2.16 m telescope.SCIENCE CHINA Physics, Mechanics & Astronomy,56(3),658–662.
MLA	JIA Peng,et al."Performance modeling of the adaptive optics system on the 2.16 m telescope".SCIENCE CHINA Physics, Mechanics & Astronomy 56.3(2013):658–662.