中国空间科学技术 ›› 2026, Vol. 46 ›› Issue (5): 26-37.doi: 10.16708/j.cnki.1000-758X.2026.0074

• 深空与月球导航技术专题 • 上一篇    下一篇

恒星光行差导航系统偏差自校正方法

熊凯*,徐超,黄翔宇   

  1. 北京控制工程研究所空间智能控制技术全国重点实验室,北京100094
  • 收稿日期:2025-12-31 修回日期:2026-02-26 录用日期:2026-03-02 发布日期:2026-09-23 出版日期:2026-09-30

Systematic bias self-calibration method for stellar aberration navigation system

XIONG Kai*,XU Chao,HUANG Xiangyu   

  1. National Key Laboratory of Space Intelligent Control, Beijing Institute of Control Engineering, Beijing 100094, China
  • Received:2025-12-31 Revision received:2026-02-26 Accepted:2026-03-02 Online:2026-09-23 Published:2026-09-30

摘要: 为了减小系统偏差对恒星光行差导航性能的影响,提出一种基于参数化模型和扩展卡尔滤波器(Extended Kalman Filter, EKF)的系统偏差估计和补偿方法。将系统偏差统一描述为敏感器相对安装误差的形式,建立了综合考虑航天器运动状态、敏感器测量噪声和系统偏差等因素的恒星光行差导航偏差校正系统模型。在此基础上,设计了同时进行系统偏差校正和定位测速解算的导航滤波器。通过计算导航系统的克拉美劳下界(Cramer-Rao Lower Bound, CRLB),分析了系统偏差自校正方法的可行性。以环绕中心天体飞行的航天器为例开展数学仿真研究,结果表明,所提方法能够有效抑制系统偏差的不利影响,在恒星角距测量精度为0.1″的情况下,经过系统偏差校正,恒星光行差导航定位精度由约50km提升至3km以内。与文献中已有方法将系统偏差建模为恒星角距测量偏差的处理方式相比,所提方法的主要优势在于待估计的状态量维数与恒星角距观测量的数量无关,有利于简化星上导航算法设计。

关键词: 航天器, 自主导航, 恒星光行差, 系统偏差, 扩展卡尔曼滤波器

Abstract: In order to reduce the effect of systematic bias on the performance of stellar aberration navigation system, a systematic bias estimation and compensation method based on a parametric model and an extended Kalman filter (EKF) is proposed. The systematic bias is described uniformly as relative installation errors of sensors. A stellar aberration navigation system model is established where spacecraft motion state, measurement noise and systematic bias are taken into consideration. Then a navigation filter is designed based on the model to estimate the systematic bias parameters together with the position and velocity of the spacecraft. The feasibility of the systematic bias self-calibration method is analyzed through the calculation of the Cramer-Rao lower bound (CRLB). The numerical simulation is implemented for an Earth satellite. It shows that the unfavorable effect of the system is suppressed evidently by using the proposed method. With an inter-star angle measurement accuracy of 0.1″, after the systematic bias self-calibration, the positioning accuracy of the stellar aberration navigation system is improved from about 50km to less than 3km. In comparison with the existing approach where the systematic bias is modeled as the inter-star angle measurement bias, the main advantage of the proposed method is that the dimension of the state vector to be estimated is independent of the number of the measurement, which facilitates the design of the onboard navigation algorithms.

Key words: spacecraft, autonomous navigation, stellar aberration, systematic bias, extended Kalman filter