A global optimization algorithm for laboratory star sensors calibration problem

Abstract To achieve high-precision calibration for star sensors before utilizing, the existing models are so complex to introduce the meaningless parameters or ignore intrinsic relationship between the parameters, which leads to additional errors. To address these issues, a global optimization model combing with pitching azimuth turntable (PAT) is proposed in this study. It uses the maximum likelihood and the least-squares to obtain the initial estimates of the star sensor. In the final step, we use the Levenberg-Marquardt algorithm to optimize all of the star sensor’s parameters with the initial estimates. The proposed method gives full consideration to the influence between parameters, which can yield an ideal calibration result. Compared with the initial method, Li method and the two-step method, the proposed method exhibited better performance. The experimental results of simulation and real data show that the proposed method can optimize all of the star sensor’s parameters with high accuracy and efficiency.

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