| Performance modeling of the adaptive optics system on the 2.16 m telescope | |
JIA Peng ; ZHANG SiJiong
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| 2013-03 | |
| Source Publication | SCIENCE CHINA Physics, Mechanics & Astronomy
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| Volume | 56Issue: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. |
| Keyword | Adaptive And Segmented Optics Optical Telescopes Monte Carlo Methods Computer Modeling And Simulation |
| Subject Area | 自适应光学 |
| WOS ID | WOS:000314912300028 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.niaot.ac.cn/handle/114a32/734 |
| Collection | 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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| Performance modeling（655KB） | 开放获取 | CC BY-NC-ND | View Download | |||
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