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Estimating the mirror seeing for a large optical telescope with a numerical method
Zhang, En-Peng1,3; Cui, Xiang-Qun2; Li, Guo-Ping2; Zhang, Yong2; Shi, Jian-Rong1,3; Zhao, Yong-Heng1,3
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2018-05-01
卷号18期号:5页码:6
关键词astronomical instrumentation methods: numerical telescopes
ISSN号1674-4527
DOI10.1088/1674-4527/18/5/60
英文摘要It is widely accepted that mirror seeing is caused by turbulent fluctuations in the index of air refraction in the vicinity of a telescope mirror. Computational Fluid Dynamics (CFD) is a useful tool to evaluate the effects of mirror seeing. In this paper, we present a numerical method to estimate the mirror seeing for a large optical telescope (similar to 4 m) in cases of natural convection with the ANSYS ICEPAK software. We get the FWHM of the image for different inclination angles (i) of the mirror and different temperature differences (Delta T) between the mirror and ambient air. Our results show that the mirror seeing depends very weakly on i, which agrees with observational data from the Canada-France-Hawaii Telescope. The numerical model can be used to estimate mirror seeing in the case of natural convection although with some limitations. We can determine Delta T for thermal control of the primary mirror according to the simulation, empirical data and site seeing.
资助项目Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; National Key Basic Research Program of China[Y41J051N01]
WOS关键词FUTURE GIANT TELESCOPE ; SYSTEM ; DESIGN ; DOME
WOS研究方向Astronomy & Astrophysics
语种英语
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
WOS记录号WOS:000432273900012
资助机构Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Guo Shou Jing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; Large Scientific Equipments Repairing Project of Chinese Academy of Sciences: "Cooling Facility and Monitoring Instruments for LAMOST Dome Seeing Improvement" ; National Key Basic Research Program of China ; National Key Basic Research Program of China
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/21624]  
专题中国科学院国家天文台
通讯作者Zhang, En-Peng
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Jiangsu, Peoples R China
3.Chinese Acad Sci, Key Lab Opt Astron, Beijing 100101, Peoples R China
推荐引用方式
GB/T 7714
Zhang, En-Peng,Cui, Xiang-Qun,Li, Guo-Ping,et al. Estimating the mirror seeing for a large optical telescope with a numerical method[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2018,18(5):6.
APA Zhang, En-Peng,Cui, Xiang-Qun,Li, Guo-Ping,Zhang, Yong,Shi, Jian-Rong,&Zhao, Yong-Heng.(2018).Estimating the mirror seeing for a large optical telescope with a numerical method.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,18(5),6.
MLA Zhang, En-Peng,et al."Estimating the mirror seeing for a large optical telescope with a numerical method".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 18.5(2018):6.
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