• 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]
  • show less
    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

    Abstract

    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.
    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
    Download Citation