地球卫星星光折射导航量测量及其性能对比

doi:10.7527/S1000-6893.2020.23536

Abstract

Abstract: Stellar refraction celestial navigation is an important autonomous navigation method for earth satellites. Measurements are an important factor influencing the navigation accuracy. The refraction apparent height, stellar refraction angles, and refraction star pixel coordinates (refraction star vectors) are three commonly used measurements of the satellite stellar refraction navigation. The obtainment methods and measurement models of the three measurements are introduced on the basis of the fundamental principle of the stellar refraction navigation. Under the same conditions, the navigation performance of these three measurements are compared through simulation and observability analysis. The simulation results show that the observability of the refraction star pixel coordinates is high, because this measurement contains both the magnitude and direction of the star refraction rays, while the stellar refraction angle and the refraction apparent height can only reveal the magnitude of the stellar refraction, exhibiting low direction observability. Therefore, the navigation performance of the refraction star pixel coordinates (refraction star vectors) is better than that of the other two measurements. Furthermore, the influence of three factors, namely, the accuracy of the star sensor, the satellite orbit height, and the installation angle of the star sensor, on the navigation performance of the three methods is analyzed.

Key words: stellar refraction navigation, refraction apparent height, stellar refraction angle, refraction star pixel coordinates, measurements

CLC Number:

V249.31

NING Xiaolin, LIANG Xiaoyu, SUN Xiaohan, WANG Fan, WANG Longhua, FANG Jiancheng. Satellite stellar refraction navigation measurements and their performance: A comparison[J]. ACTA AERONAUTICAET ASTRONAUTICA SINICA, 2020, 41(8): 623536-623536.

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Satellite stellar refraction navigation measurements and their performance: A comparison

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