• Acta Photonica Sinica
  • Vol. 48, Issue 8, 811001 (2019)
WU Yu-xiang1、2、*, ZHANG Hong-bo1、2, KONG De-qing1、2, ZHU Xin-ying1, ZHAO Rong-bing3, and YU Lin-feng3
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
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    DOI: 10.3788/gzxb20194808.0811001 Cite this Article
    WU Yu-xiang, ZHANG Hong-bo, KONG De-qing, ZHU Xin-ying, ZHAO Rong-bing, YU Lin-feng. Astronomical Refraction Model Based on Real-time Parameters and Research of Radio Telescope Pointing Calibration Method[J]. Acta Photonica Sinica, 2019, 48(8): 811001 Copy Citation Text show less
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    [2] AKINS D R, MARTIN R. 35-meter deep space antennapointing calibration system[C]. Space OPS, 2004.

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    [4] KONG De-qing, WANG Song-gen, WANG Jin-qing, et al. A new calibration model for pointing a radio telescope that considers nonlinear errors in the azimuth axis[J]. Research in Astronomy and Astrophysics, 2014, 14(6): 733.

    [5] LEHN W H, VAN D W S. Atmospheric refraction: a history[J]. Applied Optics, 2005, 44(27): 5624-5636.

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    [22] WANG Jin-qing, YU Lin-feng, JIANG Yong-bin,et al. Antenna performance measurements in Ku, K, Ka,and Q bands for the TM65 m radio telescope[J]. Acta Astronomica Sinica, 2017, 58(4): 70-85.

    [23] SU Jie, ZHANG Yi-gong, YANG Lei,et al. A new method to establish actual atmospheric refraction measurement model[J]. Journal of Yunnan University(Natural Sciences Edition), 2018, 40(2): 287-294.

    WU Yu-xiang, ZHANG Hong-bo, KONG De-qing, ZHU Xin-ying, ZHAO Rong-bing, YU Lin-feng. Astronomical Refraction Model Based on Real-time Parameters and Research of Radio Telescope Pointing Calibration Method[J]. Acta Photonica Sinica, 2019, 48(8): 811001
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