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Measurement of the K-band atmospheric opacity using the sky-dips method with a horn antenna
Wang, Kai1,2,3; Yan, Hao1,3; Ma, Jun1,3; Duan, Xuefeng1,3; Cao, Liang1,3; Ning, Yunwei1,3; Li, Xiaofei1,3; Chen, Maozheng1,3; Li, Mingshuai1; Xiang, Binbin1; Yang, Wenjun1
2022-11-01
Source PublicationASTROPHYSICS AND SPACE SCIENCE
ISSN0004-640X
Volume367Issue:11Pages:106
Contribution Rank1
AbstractThe attenuation of radio signals by the atmosphere is measured through atmospheric opacity. The atmospheric absorption effect must be corrected through an accurate amplitude calibration of the radio signals. Obtaining atmospheric mean temperature, sun brightness, sky dips, and radiosonde data modeling are the most commonly used methods for measuring atmospheric opacity. We develop an independent measuring system of K-band atmospheric opacity with a horn antenna to implement the sky-dips method to further investigate and explore the atmospheric opacity test. After many attempts, we employ the K-band atmospheric opacity measurement system to perform a comparison test with the K-band cryogenic receiver of the Nanshan 25 m telescope at the same time, with a comparison error of approximately 30%. Although the test error is due to the measurement accuracy of power and elevation, ground noise will be added in the side and back lobes if the corrugated horn is directly employed as the receiving antenna. To build the ground noise model of the test system, we employ the conventional hot and cold load method, as well as a load at ambient temperature, to cover the corrugated horn port surface and test the power output of the receiver at various elevation angles. The above opacity fitting data are corrected using the ground noise model. All the corrected data are properly fitted, and the comparison error with the 25 m telescope has been reduced to 10-20%. Although the initial test results of the system met the requirements of the atmospheric opacity test, it still needs to be improved in terms of the beam width, airmass, and side and back lobe.
KeywordReceiver Amplitude calibration Sky-dips Atmospheric opacity
DOI10.1007/s10509-022-04144-4
Indexed BySCI
Language英语
WOS KeywordTRANSMISSION
Funding ProjectNational Natural Science Foundation of China[11903073] ; National Natural Science Foundation of China[11973078] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2019D01A99] ; Chinese Academy of Sciences (CAS) Light of West China Program[2020-XBQNXZ-018] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000880322800001
PublisherSPRINGER
Funding OrganizationNational Natural Science Foundation of China ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; Chinese Academy of Sciences (CAS) Light of West China Program ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4945
Collection射电天文研究室_微波技术实验室
110米口径全可动射电望远镜(QTT)_技术成果
射电天文研究室_数字技术实验室
Corresponding AuthorYan, Hao
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Xinjiang Key Lab Microwave Technol, 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
Wang, Kai,Yan, Hao,Ma, Jun,et al. Measurement of the K-band atmospheric opacity using the sky-dips method with a horn antenna[J]. ASTROPHYSICS AND SPACE SCIENCE,2022,367(11):106.
APA Wang, Kai.,Yan, Hao.,Ma, Jun.,Duan, Xuefeng.,Cao, Liang.,...&Yang, Wenjun.(2022).Measurement of the K-band atmospheric opacity using the sky-dips method with a horn antenna.ASTROPHYSICS AND SPACE SCIENCE,367(11),106.
MLA Wang, Kai,et al."Measurement of the K-band atmospheric opacity using the sky-dips method with a horn antenna".ASTROPHYSICS AND SPACE SCIENCE 367.11(2022):106.
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