中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Calibration of K-band Cryogenic Receiver for Nanshan 26m Radio Telescope

文献类型:会议论文

作者Wang, Kai; Yan, Hao; Chen, Maozheng; Ma, Jun; Li, Xiaofei; Cao, Liang
出版日期2019-08-15
会议日期July 18, 2019 - July 19, 2019
会议地点Taiyuan, China
关键词Calibration Cryogenics Low noise amplifiers Radio astronomy Radio telescopes Receivers (containers) Signal receivers
DOI10.1109/CSQRWC.2019.8799351
国家China
英文摘要The K-band cryogenic receiver of the 26m radio telescope at Nanshan Station, Xinjiang Astronomical Observatory, Chinese Academy of Sciences is mainly used for the observation of molecular spectral lines, active galactic nuclei and very long baseline interferometry. The calibration method of receiver takes noise injection mode, which is to inject standard noise into the rear stage of the feed to calibrate the amplitude response of the received signal. After replacing the low noise amplifiers, the K-band cryogenic receiver is calibrated in five typical frequency bands again. By comparing with the previous calibration results, the latest test results could satisfy the calibration requirements, and the latest calibration parameters can be further applied to the radio source amplitude calibration. 2019 IEEE.
产权排序1
会议录2019 Cross Strait Quad-Regional Radio Science and Wireless Technology Conference, CSQRWC 2019, July 18, 2019 - July 19, 2019
会议录出版者Institute of Electrical and Electronics Engineers Inc.
语种英语
URL标识查看原文
ISBN号9781728113722
源URL[http://ir.xao.ac.cn/handle/45760611-7/3913]  
专题微波接收机技术实验室
作者单位Microwave Technology Lab, Xinjiang Astronomical Observatory (Chinese Academy of Sciences), Urumqi, China
推荐引用方式
GB/T 7714
Wang, Kai,Yan, Hao,Chen, Maozheng,et al. Calibration of K-band Cryogenic Receiver for Nanshan 26m Radio Telescope[C]. 见:. Taiyuan, China. July 18, 2019 - July 19, 2019.

入库方式: OAI收割

来源:新疆天文台

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