Storing, processing, and transmitting state confidential information are strictly prohibited on this website
JI Guo-shu, WANG Wei, LIU Fei, DOU Yu-jiang, CHEN Lin-jie, LIU Dong-hao, CHEN Zhi-jun, YAN Yi-hua. Choices of Antennas for the CSRH-I[J]. Astronomical Research and Technology, 2009, 6(3): 209-214.
Citation: JI Guo-shu, WANG Wei, LIU Fei, DOU Yu-jiang, CHEN Lin-jie, LIU Dong-hao, CHEN Zhi-jun, YAN Yi-hua. Choices of Antennas for the CSRH-I[J]. Astronomical Research and Technology, 2009, 6(3): 209-214.

Choices of Antennas for the CSRH-I

More Information
  • Received Date: February 09, 2008
  • Revised Date: March 10, 2008
  • Published Date: July 14, 2009
  • This paper first describes three system specifications of the CSRH(Chinese Spectral Radioheliograph):angular resolution, time resolution, and frequency resolution(-technical specifications in radio astronomy)as these are relevant to the achievements of scientific goals.The paper subsequently gives three key technical specifications of the CSRH, sensitivity, dynamic range, and polarization isolation(common technical specifications of a receiver).We expounds emphatically the effects of the number, size, main specifications(efficiency, noise, and axis ratio)of antennas on the six specifications mentioned above.
  • [1]
    颜毅华, 张坚, 陈志军, 等.关于太阳厘米分米波段频谱日像仪研究进展[J].天文学研究与技术-国家天文台台刊, 2006, 3(2):91-98.
    [2]
    王威, 颜毅华, 张坚, 等.CSRH阵列设计研究及馈源设计的初步考虑[J].天文学研究与技术-国家天文台台刊, 2006, 3(2):128-134.
    [3]
    姬国枢, 窦玉江, 王威, 等.CSRH模拟接收机设计[J].天文学研究与技术-国家天文台台刊, 2006, 3(2):135-142.
    [4]
    CSRH项目组.CSRH技术方案.内部资料, 2008.
    [5]
    颜毅华, 张坚, 黄光力.厘米-分米波高分辨频谱日像仪——项目建议书.中国科学院国家天文台, 2003.
    [6]
    王绶琯.密云综合孔径射电望远镜总体方案.1973.
    [7]
    K Rohlfs, T L Wilson.Radio Astronomy Tools.2000.
    [8]
    Peter J, Napier.The Very Large Array:Design and Performance of a Modern Synthesis Radio Telescope[J].IEEE, 1983, 71(11):1295-1320.
    [9]
    G B Taylor, C L Carilli, R A Perley.Synthesis Imaging in Radio Astronomy II[J].A S P CONF Ser, 1999, 180.
    [10]
    John D Kraus.Radio Astronomy[M].McGraw-Hill Book Company, 1966.
    [11]
    林昌禄, 宋锡明.圆极化天线[M].北京:人民邮电出版社, 1986.
    [12]
    吕洪生, 杨信德.实用卫星通信技术[M].武汉:电子科技大学出版社, 1994.
    [13]
    薄瓦H T.超高频天线[M].北京:高等教育出版社, 1959.
    [14]
    B N别凯托夫.超高频天线[M].北京:国防工业出版社, 1959.
  • Articles Related

    [1]Zhang Yankun, Dong Liang, Li Mingyue, He Lesheng, Wang Min. The Application of Ratio Correction in Radio Spectrum [J]. Astronomical Research and Technology, 2020, 17(3): 283-291.
    [2]Xiang Yongyuan, Jin Zhenyu. Simulation and Analysis of Signal-to-Noise Ratios for Statistics of Speckle Interferometry [J]. Astronomical Research and Technology, 2011, 8(3): 293-297.
    [3]Ji Guoshu, Liu Yuying, Wang Wei, Tan Chengming, Tan Baolin, Huang Chongxi, Liu Rongjun, Zhang Yuecheng. A Review of Designs of World's Solar Radio Telescopes [J]. Astronomical Research and Technology, 2011, 8(3): 248-254.
    [4]Zhang Yan, Yan Yihua, Tan Chengming, Wang Wei, Huang Yafang. Precise Adjustment of the Polar Axis of a Radio Telescope Antenna with a CCD Camera [J]. Astronomical Research and Technology, 2011, 8(1): 15-20.
    [5]Peng Zhi-min, Zhang Jiang-shui, Fan Jun-hui. Ratio of the Jet to the Unbeamed Luminosities for Blazars [J]. Astronomical Research and Technology, 2003, 0(S1): 103-106.
    [6]LIANG En-wei. The Temporal Evolution of the Hardness Ratio of Gamma-Ray Bursts [J]. Astronomical Research and Technology, 2003, 0(2): 18-28.
    [7]Kenji Mochizuki. 〔CII〕Continuum Intensity Ratio in the Far-Infrared Toward the Central Kiloparsec of the Nearby Spiral Galaxy M31 [J]. Publications of the Yunnan Observatory, 1999, 0(S1): 353-356.
    [8]Xu D. W, Wei J. Y, Dong X. Y, Hu J. Y. High X-Ray-to-Optical Flux Ratio Sources From RASS [J]. Publications of the Yunnan Observatory, 1999, 0(S1): 311-313.
    [9]Wu Guangjie. Signal to Noise Ratio and its Processing in Array Detector [J]. Publications of the Yunnan Observatory, 1997, 0(1): 65-69.
    [10]Su Bumei, Shi Shuobiao, Li Weihua. Adjustment of the Polar Axis of the 10-Meter Radio Telesoope [J]. Publications of the Yunnan Observatory, 1986, 0(1): 126-130.

Catalog

    Article views (128) PDF downloads (8) Cited by()

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return