[1] Mu DING. Research on the application of star sensor based on spectral polarization technique for airborne platform(2017).
[2] Jiawei HE. Study on the key technologies for high-accuracy and all-time star sensor(2013).
[3] Li HAN. Research on dim star signal extraction and star tracking algorithm(2014).
[4] D DRAVINS, L LINDEGREN, E MEZEY et al. Atmospheric intensity scintillation of stars, I. statistical distributions and temporal properties. Publications of the Astronomical Society of the Pacific, 109, 173(1997).
[5] M A ELLISON, H SEDDON. Some experiments on the scintillation of stars and planets. Monthly Notices of the Royal Astronomical Society, 112, 73-87(1952).
[6] B H BRIGGS, I A PARKIN. On the variation of radio star and satellite scintillations with zenith angle. Journal of Atmospheric and Terrestrial Physics, 25, 339-366(1963).
[7] H E BUTLER. Observations of stellar scintillation, 54, 321-340(1951).
[8] B STECKLUM. Measurements of stellar scintillation using photon counting statistics. Astronomische Nachrichten, 306, 145-156(1985).
[9] J J BURKE. Observations of the wavelength dependence of stellar scintillation. Journal of the Optical Society of America, 60, 1262-1264(1970).
[10] F J FUENTES, J J FUENSALIDA, C SANCHEZ-MAGRO. Measurements of the near-infrared stellar scintillation above the Observatorio del Teide (Tenerife). Monthly Notices of the Royal Astronomical Society, 226, 769-783(1987).
[11] V I TATARSKI. Wave propagation in a turbulent medium(2016).
[12] A D WHEELON. Electromagnetic scintillation: volume 1, geometrical optics(2001).
[13] J D SCHMIDT. Numerical simulation of optical wave propagation: with examples in MATLAB(2010).
[14] A DIPANKAR, R MARCHIANO, P SAGAUT. Trajectory of an optical vortex in atmospheric turbulence. Physical Review E, 80, 046609(2009).
[15] J M MARTIN, S M FLATTE. Intensity images and statistics from numerical simulation of wave propagation in 3-D random media. Applied Optics, 27, 2111-2126(1988).
[16] W A COLES, J P FILICE, R G FREHLICH et al. Simulation of wave propagation in three-dimensional random media. Applied Optics, 34, 2089-2101(1995).
[17] B M WELSH. Fourier-series-based atmospheric phase screen generator for simulating anisoplanatic geometries and temporal evolution, 3125, 327-338(1997).
[18] R G LANE, A GLINDEMANN, J C DAINTY. Simulation of a Kolmogorov phase screen. Waves in Random Media, 2, 209(1992).
[19] R E HUFNAGEL, N R STANLEY. Modulation transfer function associated with image transmission through turbulent media. Journal of the Optical Society of America, 54, 52-61(1964).
[20] F H RUGGIERO, D A DEBENEDICTIS. Forecasting optical turbulence from mesoscale numerical weather prediction models, 10-14(2002).
[21] E M DEWAN. A Model for C2n (optical turbulence) profiles using radiosonde data. Directorate of Geophysics, Air Force Materiel Command(1993).
[22] C QING, X WU, X LI et al. Use of weather research and forecasting model outputs to obtain near-surface refractive index structure constant over the ocean. Optics Express, 24, 13303-13315(2016).
[23] C QING, X WU, H HUANG et al. Estimating the surface layer refractive index structure constant over snow and sea ice using Monin-Obukhov similarity theory with a mesoscale atmospheric model. Optics Express, 24, 20424-20436(2016).
[24] Xianmei QIAN, Wenyue ZHU, Ruizhong RAO. Phase screen distribution for simulating laser propagation along inhomogeneous atmospheric path. Acta Physica Sinica, 58, 6633-6639(2009).
[25] L C ANDREWS, R L PHILLIPS. Laser beam propagation through random media. Laser Beam Propagation Through Random Media: Second Edition(2005).
[26] F MOLL. Experimental characterization of intensity scintillation in the LEO downlink, 31-35(2015).
[27] Z WANG, R MALANEY, B BURNETT. Satellite-to-earth quantum key distribution via orbital angular momentum. Physical Review Applied, 14, 064031(2020).
[28] X QIANG, J SONG, J FENG. Aperture averaging effect on irradiance scintillation of laser beams through the atmosphere, 1-2(2009).
