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High-precision beam pointing control based on global non-singular attitude estimation

GUO Ming FAN Yi-di WANG Peng-cheng AN Ke LU Wei CHEN Wen ZHANG Yong-he LIN Bao-jun

郭明, 范一迪, 王鹏程, 安轲, 卢苇, 陈雯, 张永合, 林宝军. 基于全局非奇异姿态估计的星间光束精密指向控制[J]. 中国光学(中英文). doi: 10.37188/CO.EN-2026-0004
引用本文: 郭明, 范一迪, 王鹏程, 安轲, 卢苇, 陈雯, 张永合, 林宝军. 基于全局非奇异姿态估计的星间光束精密指向控制[J]. 中国光学(中英文). doi: 10.37188/CO.EN-2026-0004
GUO Ming, FAN Yi-di, WANG Peng-cheng, AN Ke, LU Wei, CHEN Wen, ZHANG Yong-he, LIN Bao-jun. High-precision beam pointing control based on global non-singular attitude estimation[J]. Chinese Optics. doi: 10.37188/CO.EN-2026-0004
Citation: GUO Ming, FAN Yi-di, WANG Peng-cheng, AN Ke, LU Wei, CHEN Wen, ZHANG Yong-he, LIN Bao-jun. High-precision beam pointing control based on global non-singular attitude estimation[J]. Chinese Optics. doi: 10.37188/CO.EN-2026-0004

基于全局非奇异姿态估计的星间光束精密指向控制

详细信息
  • 中图分类号: TP394.1;TH691.9

High-precision beam pointing control based on global non-singular attitude estimation

doi: 10.37188/CO.EN-2026-0004
Funds: This work was supported by National Key R&D Program of China (No. 2022YFC2203700, No. 2021YFC2202600,) and the Shanghai Science and Technology Innovation Action Plan (No. 24YF2742600).
More Information
    Author Bio:

    GUO Ming (1991—), male, born in Laiwu, Shandong Province. Ph.D. candidate at the Innovation Academy for Microsatellites, Chinese Academy of Sciences, his research mainly focuses on spacecraft system design. Email: guom@microsate.com

    FAN Yi-di (1993–), female, born in Lianyungang, Jiangsu Province. She received her Ph.D. from the Harbin Institute of Technology and is now an assistant research fellow. Her research focuses on spacecraft dynamics and control. Email: fanyd@microsate.com

    Corresponding author: fanyd@microsate.com
  • 摘要:

    针对空间引力波探测航天器的星间建链任务,研究了基于多源信息融合的光束精密指向控制问题。结合引力波探测航天器的结构和载荷特性,建立包含移动光学组件运动的全系统状态方程,利用误差四元数将非独立变量描述的非线性测量方程转化为独立变量描述的线性方程,并融合惯性传感器的测量信息进行滤波估计以提高卫星平台的定姿精度。此外,针对超远距离星间激光传输时间和两星之间高速相对运动导致的超前指向问题,推导了随时间变化的超前角解析表达式,并仿真分析了轨道周期内超前角的变化趋势,为星间链路建立与维持过程的超前角伺服补偿提供了理论依据。通过三星系统的闭环仿真验证了所设计的高精度指向估计算法在稳定性和估计精度方面的优越性,结合鲁棒抗扰控制器实现了光束的精密指向,为我国引力波探测计划的顺利实施提供必要的技术支撑。

     

  • Figure 1.  Formation of the GW detection spacecrafts

    Figure 2.  Structure of each spacecraft with MOSAs and TMs

    Figure 3.  TM measurement noise model

    Figure 4.  Point-ahead angle representation

    Figure 5.  PAA change of the 3 spacecrafts during an orbit period

    Figure 6.  schematic diagram of the control scheme [16]

    Figure 7.  Simulation system of formation and spacecraft

    Figure 8.  The framework of the closed-loop

    Figure 9.  Variations of the Euler angles of the SC

    Figure 10.  Attitude Measurement error and Estimation error

    Figure 11.  Control error of the spacecraft attitude

    Table  1.   Parameters of Simulation System

    ItemValue
    Duration4000s
    Step-size0.1s
    Environmental Noisesolar radiation pressure noise
    Gravitational Perturbationsthe sun and the eight planets
    Sensor ConfigurationStar Tracker:FoV:17.5°×13.5°
    Accuracy:15μrad
    Inertial SensorNoise:Fig.3
    Actuator ConfigurationThrusterRange:1~100μN
    Resolution:0.1μN
    Noise:0.1μN/Hz1/2
    Inertial SensorNoise:1×10−14 N/Hz1/2
    Spacecraft ParametersSpacecraft Mass700kg
    Spacecraft Moment of Inertia$ \left[\begin{matrix}450 & & \\ & 450 & \\ & & 450\end{matrix}\right]kg\cdot {m}^{2} $
    TM mass1.96kg
    TM Moment of Inertia$ \left[\begin{matrix}6.9 & & \\ & 6.9 & \\ & & 6.9\end{matrix}\right]{10}^{-4}kg\cdot {m}^{2} $
    下载: 导出CSV

    Table  2.   Performance of the estimator for SC attitude

    State Variables x/rad y/rad $\textit{z} $/rad
    $ {\overline{e}}_{m} $ $ 4.99\times {10}^{-6} $ $ 5.02\times {10}^{-6} $ $ 5.01\times {10}^{-6} $
    $ {\overline{e}}_{e} $ $ 8.96\times {10}^{-7} $ $ 9.57\times {10}^{-7} $ $ 9.17\times {10}^{-7} $
    ERR 82.04% 80.94% 81.70%
    下载: 导出CSV
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出版历程
  • 收稿日期:  2026-01-08
  • 录用日期:  2026-03-05
  • 网络出版日期:  2026-08-07

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