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performancemodelingoftheadaptiveopticssystemonthe216mtelescope
Jia Peng1; Zhang Sijiong2
2013
Source Publicationsciencechinaphysicsmechanicsastronomy
ISSN1674-7348
Volume56Issue:3Pages:658–662
AbstractThe 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.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/53434
Collection中国科学院国家天文台
Affiliation1.南京大学
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
Jia Peng,Zhang Sijiong. performancemodelingoftheadaptiveopticssystemonthe216mtelescope[J]. sciencechinaphysicsmechanicsastronomy,2013,56(3):658–662.
APA Jia Peng,&Zhang Sijiong.(2013).performancemodelingoftheadaptiveopticssystemonthe216mtelescope.sciencechinaphysicsmechanicsastronomy,56(3),658–662.
MLA Jia Peng,et al."performancemodelingoftheadaptiveopticssystemonthe216mtelescope".sciencechinaphysicsmechanicsastronomy 56.3(2013):658–662.
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