• Acta Photonica Sinica
  • Vol. 52, Issue 5, 0552210 (2023)
Zhiwei TAO1,2,3, Congming DAI1,3,*, Pengfei WU1,3, Yichong REN4..., Haiping MEI1,3, Jie TONG1,3,5, Chuankai LUO1,3, Chun QING1,3, Yunsong FENG2, Heli WEI1,3 and Ruizhong RAO1,3|Show fewer author(s)
Author Affiliations
  • 1Key Laboratory of Atmospheric Optics, Anhui Institute of Optics and Fine Mechanics, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China
  • 2Infrared and Low Temperature Plasma Key Laboratory of Anhui Province, Electronic Countermeasure College, National University of Defense Technology, Hefei 230037, China
  • 3Advanced Laser Technology Anhui Laboratory, Hefei 230037, China
  • 4School of Physics, Hefei University of Technology, Hefei 230601, China
  • 5Science Island Branch, Graduate School of University of Science and Technology of China, Hefei 230026, China
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    DOI: 10.3788/gzxb20235205.0552210 Cite this Article
    Zhiwei TAO, Congming DAI, Pengfei WU, Yichong REN, Haiping MEI, Jie TONG, Chuankai LUO, Chun QING, Yunsong FENG, Heli WEI, Ruizhong RAO. Atmospheric Effects of Star Imaging(Ⅱ):Atmospheric Turbulence[J]. Acta Photonica Sinica, 2023, 52(5): 0552210 Copy Citation Text show less
    Schematic diagram of the split-step beam propagation model
    Fig. 1. Schematic diagram of the split-step beam propagation model
    Turbulence profiles at Sansha,Dachaidan and Hefei for four time periods of one day on January 1,2008
    Fig. 2. Turbulence profiles at Sansha,Dachaidan and Hefei for four time periods of one day on January 1,2008
    Scintillation index of starlight as a function of zenith angle in Sansha,Dachaidan and Hefei under different observation altitudes
    Fig. 3. Scintillation index of starlight as a function of zenith angle in Sansha,Dachaidan and Hefei under different observation altitudes
    Arrival angle of the far-field optical spot as a function of the zenith angle at four times of the day in Sansha,Dachaidan and Hefei under different observation altitudes
    Fig. 4. Arrival angle of the far-field optical spot as a function of the zenith angle at four times of the day in Sansha,Dachaidan and Hefei under different observation altitudes
    Arrival angle fluctuation of the far-field optical spot as a function of the zenith angle at four times of the day in Sansha,Dachaidan and Hefei under different observation altitudes
    Fig. 5. Arrival angle fluctuation of the far-field optical spot as a function of the zenith angle at four times of the day in Sansha,Dachaidan and Hefei under different observation altitudes
    Zhiwei TAO, Congming DAI, Pengfei WU, Yichong REN, Haiping MEI, Jie TONG, Chuankai LUO, Chun QING, Yunsong FENG, Heli WEI, Ruizhong RAO. Atmospheric Effects of Star Imaging(Ⅱ):Atmospheric Turbulence[J]. Acta Photonica Sinica, 2023, 52(5): 0552210
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