Acta Photonica Sinica, Volume. 52, Issue 5, 0552210(2023)
Atmospheric Effects of Star Imaging(Ⅱ):Atmospheric Turbulence
Fig. 1. Schematic diagram of the split-step beam propagation model
Fig. 2. Turbulence profiles at Sansha,Dachaidan and Hefei for four time periods of one day on January 1,2008
Fig. 3. Scintillation index of starlight as a function of zenith angle 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
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
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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
Category: Special Issue for Advanced Science and Technology of Astronomical Optics
Received: Mar. 1, 2023
Accepted: Apr. 19, 2023
Published Online: Jul. 19, 2023
The Author Email: DAI Congming (cmdai@aiofm.ac.cn)