Storing, processing, and transmitting state confidential information are strictly prohibited on this website
Zhao Cong, Xu Qian, Wang Na, Xing Binbin. The Prime Focus Receiver Positioner Design of Xinjiang QiTai 110m Radio Telescope[J]. Astronomical Research and Technology, 2017, 14(2): 172-178.
Citation: Zhao Cong, Xu Qian, Wang Na, Xing Binbin. The Prime Focus Receiver Positioner Design of Xinjiang QiTai 110m Radio Telescope[J]. Astronomical Research and Technology, 2017, 14(2): 172-178.

The Prime Focus Receiver Positioner Design of Xinjiang QiTai 110m Radio Telescope

More Information
  • Received Date: May 11, 2016
  • Revised Date: May 29, 2016
  • Available Online: November 20, 2023
  • With the rapid development of radio astronomy research, the requirements to the sensitivity and resolution of telescopes, as well as wider observing band, constantly grow.The low frequency receivers are usually installed at the primary focus of the telescope so that the feed horns are smaller and lighter. The switching system of prime focus receivers must be effective and compact to avoid affecting normal use of the receivers on the secondary focus. A steerable 100m aperture radio telescope is supposed to be built in Qitai, Xinjiang (QiTai radio Telescope, QTT).This paper introduces a new solution of the switching system for the QTT primary focus receivers by using a linear module. Through the modeling and simulation of this scheme, and analyzing of the aperture interception to the observing signals, it is shown that our design well satisfies the efficiency requirement of QTT.
  • [1]
    Shen Zhiqiang. The Shanghai 65m RT[R]. Beijing: The 65m Radio Telescope Team, 2013.
    [2]
    Nan Rendong, Li Di, Jin Chengjin, et al. The Five-hundred-meter Aperture Spherical Radio Telescope (FAST) project[J]. International Journal of Modern Physics D, 2011, 20: 989-1024.
    [3]
    王娜. 新疆奇台110米射电望远镜[J]. 中国科学: 物理学 力学 天文学, 2014, 44(8): 783-794.

    Wang Na. Xinjiang Qitai 110m radio telescope (in Chinese)[J]. Scientia Sinica: Physica, Mechanica & Astronomica, 2014, 44(8): 783-794.
    [4]
    Wilson T L, Rohlfs K, Hüttemeister S. Tools of radio astronomy[M]. Berlin: Spriger-Verlag, 2009: 177-179.
    [5]
    Wielebinski R, Junkes N, Grahl B H. The Effelsberg 100 radio telescope: construction and forty years of radio astronomy[J]. Journal of Astronomy History and Heritage, 2011, 14(1): 3-21.
    [6]
    Prestage R M, Constantikes K T, Hunter T R, et al. The green bank telescope[J]. Proceedings of the IEEE, 2009, 97(8): 1382-1390.
    [7]
    Olmi L,Grueff G. SRT: design and technical specifications[J]. Memoriedella Società Astronomica Italiana Supplement, 2006,10: 19-24.
    [8]
    成大先. 机械设计手册[M]. 北京: 化学工业出版社, 2008: 1244-1247.
    [9]
    朱钟淦, 叶尚辉. 天线结构设计[M]. 北京: 国防工业出版社, 1980: 221-222.
    [10]
    银秋华, 周建寨. 反射面天线增益的快速估算[J]. 无线电通信技术, 2013, 39(4): 50-52.

    Yin Qiuhua, Zhou Jianzhai. Quick estimation the gain of reflector antenna[J]. Radio Communications Technology, 2013, 39(4): 50-52.
    [11]
    肖明, 王娜, 刘志勇. 大气折射对射电望远镜高精度指向的影响[J]. 天文研究与技术, 2016, 13(1): 44-51.

    Xiao Ming, Wang Na, Liu Zhiyong. Atmospheric refractions and radio telescope pointing corrections[J]. Astronomical Research & Technology, 2016, 13(1): 44-51.
    [12]
    项斌斌, 刘志勇, 杨文军. 基于FS系统对乌鲁木齐VLBI射电望远镜进行天线测量[J]. 天文研究与技术——国家天文台台刊, 2014, 11(4): 343-349.

    Xiang Binbin, Liu Zhiyong, Yang Wenjun. Measurement of the antenna characteristics of the VLBI radio telescope of the Urumqi station[J]. Astronomical Research & Technology——Publications of National Astronomical Observatories of China, 2014, 11(4): 343-349.
  • Articles Related

    [1]Lin Zheyu, Xu Zhi. Research on Fourier Demodulation Method Based on Continuous Rotating Waveplate Modulation [J]. Astronomical Techniques and Instruments, 2023, 20(4): 341-352. DOI: 10.14005/j.cnki.issn1672-7673.20230314.001
    [2]Sun Xiao, Wang Qingmei, Li Zhenwei, Qiao Feng, Chu Jingjing. Multi-linear Regression Model to Estimate Temperature Signal in FAST Project Active Reflective Surface Health Monitoring System [J]. Astronomical Research and Technology, 2022, 19(5): 493-499. DOI: 10.14005/j.cnki.issn1672-7673.20220113.003
    [3]Ning Yunwei, Yan Hao, Cao Liang, Ma Jun, Li Xiaofei, Liu Feng, Chen Yong. The Design of Four Channel Equalization Amplifier Module for Radio Astronomy Receiver [J]. Astronomical Research and Technology, 2022, 19(5): 432-437. DOI: 10.14005/j.cnki.issn1672-7673.20210930.001
    [4]Huang Zhen, Bai Zhengyao, Guo Shaojie. Research on Spectrum Resolution Based on Modulated Wideband Converter [J]. Astronomical Research and Technology, 2022, 19(4): 353-358. DOI: 10.14005/j.cnki.issn1672-7673.20210707.001
    [5]Dai Wei, Wei Bingtao, Hao Longfei, Wei Shoulin, Liang Bo. A Short-term Scheduling Method Based on Linear Programming for Yunnan 40-meter Radio Telescope [J]. Astronomical Research and Technology, 2022, 19(3): 221-226. DOI: 10.14005/j.cnki.issn1672-7673.20210528.001
    [6]Yu Yike, Wang Meng. Comparitive Studies of Signal-Modulation Methods Based on the CAPS [J]. Astronomical Research and Technology, 2014, 11(3): 224-229.
    [7]Gan Tong, Ma Guanyi. An Algorithm for Signal Synthesis and Acquisition of CAPS Based on Dual-Linear Polarization Antennas [J]. Astronomical Research and Technology, 2013, 10(1): 36-41.
    [8]BU Zhao-hui. Research on Data Reduction Module of High-speed FX Correlator [J]. Astronomical Research and Technology, 2003, 0(4): 12-18.
    [9]Chen Guoqiang. The Application and Test on the Principal Performance of the Solar Radio Fast Recording System at the PIN Modulator [J]. Publications of the Yunnan Observatory, 1995, 0(4): 72-75.
    [10]Xiong Guanzhu, Chen Jianbao. Linearization Method for Fitting the Infrared Spectrum of the Late Type Stars [J]. Publications of the Yunnan Observatory, 1995, 0(2): 36-41.

Catalog

    Article views (532) PDF downloads (389) Cited by()

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return