Acta Photonica Sinica, Volume. 52, Issue 5, 0552209(2023)
Atmospheric Effects of Star Imaging（
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Fig. 1. Temperature profile of Malan region and the U.S. standard atmosphere
Fig. 2. Aerosol extinction profile in Malan region on November 27，2015（measured by lidar）
Fig. 3. Variation of the elements of the scattering phase matrix with scattering angle under different wavelengths in the lowest atmospheric layer
Fig. 4. Flow chart for solving sky polarization distribution characteristics based on the doubling and adding method
Fig. 5. Variation of spectral radiant flux density with wavelength under AM1.5 standard
Fig. 7. Distribution of sky irradiance（I component）at a solar zenith angle of
Fig. 8. Distribution of sky Q component at a solar zenith angle of
Fig. 9. Distribution of sky U component at a solar zenith angle of
Fig. 10. Distribution of sky polarization at solar zenith angle of
Fig. 11. Distribution of sky polarization at solar zenith angle of
Fig. 12. Distribution of sky polarization at solar zenith angle of
Fig. 13. Distribution of sky polarization at solar zenith angle of
Fig. 14. Distribution of sky polarization at solar zenith angle of
Fig. 15. Distribution of sky polarization at solar zenith angle of
Fig. 16. Variation of polarization with observation angle for different observation altitudes at 0.55 μm
Fig. 17. Variation of polarization with observation angle for different observation altitudes at 0.9 μm
Fig. 18. Variation of polarization with observation angle for different observation altitudes at 1.65 μm
Fig. 19. Variation of polarization with observation angle for different solar zenith angles at a wavelength of 1.65 μm and an azimuth of
Fig. 20. Variation of polarization with observation angle for different solar zenith angles at a wavelength of 1.65 μm and an azimuth of
Fig. 21. Variation of polarization with observation angle at different wavelengths for a solar zenith angle of
Fig. 22. Variation of polarization with observation angle at different wavelengths for a solar zenith angle of
Fig. 23. Variation of polarization with observation angle at different wavelengths for a solar zenith angle of
Table 1. The relationship between the wavelength and the spectral radiant flux density used in this calculation
View tableView in ArticleTable 1. The relationship between the wavelength and the spectral radiant flux density used in this calculation
Wavelength Solar radiant flux density/（ ） 0.55 1561.5 0.9 748.5 1 746.5 1.1 412.6 1.2 423.6 1.3 413.1 1.5 182.1 1.65 234.8
Table 2. Fixed parameters used in this calculation
View tableView in ArticleTable 2. Fixed parameters used in this calculation
Parameter type Input value Number of quadrature directions 8 Order of azimuth expansion 8 Type of quadrature Gaussian type Delta-M scaling No Radiation type Solar radiation Surface temperature 273.9 K Surface type Lambertian surface Surface albedo 0.25 Sky temperature 0 K Number of output azimuths 37
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Zhiwei TAO, Congming DAI, Pengfei WU, Yichong REN, Haiping MEI, Wenqing XU, Gang XU, Jie TONG, Yunsong FENG, Ruizhong RAO, Heli WEI. Atmospheric Effects of Star Imaging（
Paper Information
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)
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