Star centroid error compensation based on the star triangle internal angles for celestial navigation with aero-optical degradation

被引:6
作者
Li, Tianqi [1 ]
Zhang, Chunxi [1 ]
Tian, Yizhuo [1 ]
Yang, Yanqiang [1 ]
机构
[1] Beihang Univ, Sch Instrumentat & Optoelect Engn, Sci & Technol Inertial Lab, Beijing 100191, Peoples R China
基金
中国国家自然科学基金;
关键词
Aero-optic effect; Star sensor; Celestial navigation; Centroid error compensation; BOUNDARY-LAYER; COMPUTATION; SIMULATION;
D O I
10.1016/j.measurement.2022.112229
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
In this paper, to solve the correction problem of star vector error induced by the aero-optic effect under hypersonic conditions, and to improve the navigation accuracy further, a novel method of star centroid error correction is proposed. The method is based on the star triangle internal angles, which can effectively use the prior information to estimate the aero-optical star centroid error. The method is verified by the Monte Carlo simulation and Hardware-In-Loop simulation. According to Hardware-In-Loop simulation, the star centroid error can be reduced by approximately 27%, and the attitude error can be reduced by approximately 14%. Therefore, the presented method is significant for the application of celestial navigation with hypersonic conditions.
引用
收藏
页数:13
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