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A method to obtain the wind field characteristics of super-large aperture radio telescope site based on single-point wind tower and numerical simulation
He, Fei-Long1,2; Xu, Qian2; Wang, Na2; Zhu, Chun-Hua1
2020-12-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume20Issue:12Pages:199
Contribution Rank2
AbstractThe influence of wind on the pointing accuracy of large aperture radio telescopes is becoming increasingly serious, especially at high observing frequency. Obtaining the wind field characteristics efficiently is very important to reduce the wind disturbance on antenna structure. In this paper, an error evaluation of numerical simulation method is established based on the measured data of single point wind tower, and the wind field characteristics are obtained from the evaluated numerical simulation results combined with the measured data for the 110 m aperture QiTai radio Telescope (QTT) site. According to the simulation results, compared with the measured data, the root mean square error (RMSE) of wind speed is less than 1 m s(-1), and the minimum wind speed RMSE is 0.2 m s(-1). An analysis of the wind field characteristics of the QTT site suggests that the active wind resistance design of the antenna periphery should focus on the SSW (south-south-west) direction.
Keywordtelescopes site testing methods: data analysis
DOI10.1088/1674-4527/20/12/199
URL查看原文
Indexed BySCI
Language英语
WOS KeywordCFD SIMULATION ; PERFORMANCE ; ENVIRONMENT ; TERRAIN
Funding ProjectChinese Academy of Sciences (CAS) Light of West China Program[2017-XBQNXZ-B-024] ; Xinjiang Uygur Autonomous Region Tianshan innovation team[2018D14008] ; Youth Innovation Promotion Association, CAS[2016058] ; Operation, Maintenance and upgrading Fund for Astronomical Telescopes and Facility Instruments ; National Natural Science Foundation of China[11763007] ; Tianshan Youth Project of Xinjiang[2017Q014]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000607980800001
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Funding OrganizationChinese Academy of Sciences (CAS) Light of West China Program ; Xinjiang Uygur Autonomous Region Tianshan innovation team ; Youth Innovation Promotion Association, CAS ; Operation, Maintenance and upgrading Fund for Astronomical Telescopes and Facility Instruments ; National Natural Science Foundation of China ; Tianshan Youth Project of Xinjiang
Citation statistics
Cited Times:9[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3815
Collection射电天文研究室_天线技术实验室
110米口径全可动射电望远镜(QTT)_技术成果
Corresponding AuthorXu, Qian; Zhu, Chun-Hua
Affiliation1.Xinjiang Univ, Sch Phys & Technol, Urumqi 830046, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
He, Fei-Long,Xu, Qian,Wang, Na,et al. A method to obtain the wind field characteristics of super-large aperture radio telescope site based on single-point wind tower and numerical simulation[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2020,20(12):199.
APA He, Fei-Long,Xu, Qian,Wang, Na,&Zhu, Chun-Hua.(2020).A method to obtain the wind field characteristics of super-large aperture radio telescope site based on single-point wind tower and numerical simulation.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,20(12),199.
MLA He, Fei-Long,et al."A method to obtain the wind field characteristics of super-large aperture radio telescope site based on single-point wind tower and numerical simulation".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 20.12(2020):199.
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