An atmospheric refractive index estimation method based on multispectral stellar observation data

Xueying Wang; Yuan Huang; Feng Zhang

doi:10.1117/12.2667924

21 March 2023 An atmospheric refractive index estimation method based on multispectral stellar observation data

Xueying Wang, Yuan Huang, Feng Zhang

Proceedings Volume 12595, Advanced Fiber Laser Conference (AFL2022); 1259515 (2023) https://doi.org/10.1117/12.2667924
Event: Advanced Fiber Laser Conference (AFL2022), 2022, Changsha, China

Abstract

The theoretical model of atmospheric refractive index based on the standard atmospheric environment cannot explain the atmospheric refractive index when optical satellites detect targets. Aiming at this problem, a method for estimating the refractive index of the atmosphere based on multispectral stellar observation data is proposed. Based on optical satellites’ multispectral stellar observation data, according to the principle of deflection when the stellar light passes through the atmosphere, the optical path model of the stellar light refracted by the atmosphere is established under the assumption of a layered spherical atmosphere. A method of using multispectral segment stars to measure the actual light and the iterative forward feedback of stellar theoretical light is proposed, to estimate the refractive index of each layer of the atmosphere of the layered atmosphere to different spectral segments of light.

Citation Download Citation

Xueying Wang, Yuan Huang, and Feng Zhang "An atmospheric refractive index estimation method based on multispectral stellar observation data", Proc. SPIE 12595, Advanced Fiber Laser Conference (AFL2022), 1259515 (21 March 2023); https://doi.org/10.1117/12.2667924

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