Acta Photonica Sinica, Volume. 48, Issue 8, 811001(2019)

Astronomical Refraction Model Based on Real-time Parameters and Research of Radio Telescope Pointing Calibration Method

WU Yu-xiang1,2、*, ZHANG Hong-bo1,2, KONG De-qing1,2, ZHU Xin-ying1, ZHAO Rong-bing3, and YU Lin-feng3
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  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
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    Astronomical refraction in pointing error of large radio telescope was considered. An astronomical refraction model using real-time measured temperature, pressure and relative humidity was newly applied to pointing error calibration model. A simulation was used to compare traditional and real-time astronomical refraction model in different weather conditions. This calibration model was applied to pointing calibration of Shanghai Tianma 65 m Radio Telescope. The Ku-band experiment showed that the real-time astronomical refraction model is better than the traditional model. Pointing accuracy is 25.8% better under elevation of 20°, 45% better under elevation of 15° and 60% better under elevation of 10°. Pointing accuracy is 5.0″, which is 5.3% better than traditional model. The worsening of pointing accuracy at low elevation caused by astronomical refraction is basically removed.

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    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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    Paper Information

    Received: May. 10, 2019

    Accepted: --

    Published Online: Nov. 28, 2019

    The Author Email: Yu-xiang WU (wuyx@nao.cas.cn)

    DOI:10.3788/gzxb20194808.0811001

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