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Performance modeling of the adaptive optics system on the 2.16 m telescope
JIA Peng; ZHANG SiJiong
2013-03
Source PublicationSCIENCE CHINA Physics, Mechanics & Astronomy
Volume56Issue:3Pages:658–662
Abstract
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.
KeywordAdaptive And Segmented Optics Optical Telescopes Monte Carlo Methods Computer Modeling And Simulation
Subject Area自适应光学
WOS IDWOS:000314912300028
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/734
Collection中国科学院南京天文光学技术研究所_期刊论文
中科院天文光学技术重点实验室_期刊论文
Recommended Citation
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.
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