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基于恒星优化选取的星敏感器在轨标定方法

On-Orbit Calibration Method for Star Sensor Based on Optimal Star Selection

  • 摘要: 针对航天器在轨运行中,其光学参数受到太空复杂环境的影响会产生一定的偏移,若不及时矫正光学参数会严重影响航天器姿态估计的精度问题,传统的在轨标定方法一般基于星角距不变原理,但其计算复杂度高,在计算和存储资源严重受限的深空探测器难以实现。引入基于奇异值分解不变原理的标定方法,通过奇异值大小去量化并标定系统的可观测性,并在此基础上基于可观测性优化选取恒星的分布与组合,并结合扩展卡尔曼滤波(Extended Kalman Filter,EKF)对星敏感器光学参数进行标定。仿真结果表明,与传统的恒星优选方法相比,提出的方法可较好地抑制恒星观测误差。

     

    Abstract: To address optical parameters are affected by the complex environment in space will produce a certain bias in spacecraft on-orbit operation, it will seriously affect the accuracy of spacecraft attitude estimation. The traditional on-orbit calibration method generally base on star angular distance invariance, but it has high computational complexity, the computational and storage resources of deep space probe are very limited, it is difficult to be realized. This paper introduces a calibration method based on singular value decomposition invariance, the size of the singular value is used to measure the observability of the calibration system, on this basis based on the observability to optimize the selection of star distribution and combination, combined with extended Kalman filtering to calibrate the optical parameters of the star tracker. The simulation results show that compared with the traditional star optimal selected model, the optimal selected model proposed in this paper has an advantage in calibrated accuracy and can better suppress the star observational error.

     

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