[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] Qixiang ZHU, Qian XIE. Improving the detection capability of CCD for faint sky targets using spectral filtering technology. Spacecraft Recovery and Telecommunications, 17-24(1989).
[12] Weian XU. Application of spectral filtering device in daytime star measurement. Optics and Precision Engineering, 84-88(1996).
[13] Xiaobing SUN, Jin HONG, Donggen LUO et al. Daytime astronomical spectral polarization imaging technology and experimental research. Journal of Atmospheric and Environmental Optics, 2, 5(2007).
[14] Song YE, Yonghua FANG, Xiaobing SUN et al. A daytime observation method for stars based on polarization information. Journal of Atmospheric and Environmental Optics, 2, 5(2007).
[15] Ruijin ZHANG, Hao XIAN, Changhui RAO et al. Analysis of daytime skyglow background suppression using polarization filtering. Acta Optica Sinica, 32, 0501003(2012).
[16] STATES UNITED. National oceanic, atmospheric administration, united states. Air Force. US standard atmosphere, 1976. National Oceanic and Atmospheric Administration(1976).
[17] Wei WANG, Jinkui CHU, Yan CUI et al. Modeling of atmospheric polarization pattern based on vector radiative transfer. Chinese Journal of Lasers, 40, 0513001(2013).
[18] Su ZHANG, Juntong ZHAN, Qiang FU et al. Simulation research on sky polarization characteristics under complicated marine environment. Acta Optica Sinica, 40, 2201001(2020).
[19] G HANEL. The physical chemistry of atmospheric particles. Hygroscopic Aerosol, 1-20(1984).
[20] C E JUNGE. Atmospheric chemistry. Advances in geophysics, 4, 1-108(1958).
[21] Xiuhong CHEN, Heli WEI, Xuebin LI et al. Calculating model for aerosol extinction from visible to far infrared wavelength. High Power Laser and Particle Beams, 21, 183-189(2009).
[22] K N LIOU. An introduction to atmospheric radiation(2002).
[23] S Q DUNTLEY. The reduction of apparent contrast by the atmosphere. Journal of the Optical Society of America, 38, 179-191(1948).
[24] K F EVANS, G L STEPHENS. A new polarized atmospheric radiative transfer model. Journal of Quantitative Spectroscopy and Radiative Transfer, 46, 413-423(1991).
[25] M WENDISCH, P YANG. Theory of atmospheric radiative transfer: a comprehensive introduction(2012).
[26] Ruizhong RAO. Modern atmospheric optics(2012).