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导星辅助运动暗弱天体检测系统设计与仿真

张威 冯文全 孙国童 王春雷

张威,冯文全,孙国童,等. 导星辅助运动暗弱天体检测系统设计与仿真[J]. 北京航空航天大学学报,2025,51(9):3052-3061 doi: 10.13700/j.bh.1001-5965.2023.0503
引用本文: 张威,冯文全,孙国童,等. 导星辅助运动暗弱天体检测系统设计与仿真[J]. 北京航空航天大学学报,2025,51(9):3052-3061 doi: 10.13700/j.bh.1001-5965.2023.0503
ZHANG W,FENG W Q,SUN G T,et al. Design and simulation of guide star assisted moving faint object detection system[J]. Journal of Beijing University of Aeronautics and Astronautics,2025,51(9):3052-3061 (in Chinese) doi: 10.13700/j.bh.1001-5965.2023.0503
Citation: ZHANG W,FENG W Q,SUN G T,et al. Design and simulation of guide star assisted moving faint object detection system[J]. Journal of Beijing University of Aeronautics and Astronautics,2025,51(9):3052-3061 (in Chinese) doi: 10.13700/j.bh.1001-5965.2023.0503

导星辅助运动暗弱天体检测系统设计与仿真

doi: 10.13700/j.bh.1001-5965.2023.0503
详细信息
    通讯作者:

    E-mail:buaafwq@buaa.edu.cn

  • 中图分类号: TP317.4;P171

Design and simulation of guide star assisted moving faint object detection system

More Information
  • 摘要:

    暗弱空间运动小目标检测在航天及军事领域有着广泛的应用,为提高空间目标监视系统的探测能力,提出并设计了导星辅助运动暗弱天体检测系统,该系统由星图模拟、图像去噪、质心解算、运动先验信息反向传播和主焦面成像组成。对星表及星空环境进行研究,确保星点坐标和噪声模拟的准确性;通过引入抖动误差、噪声误差和运动先验误差,更真实地模拟望远镜所处星空环境造成的误差影响,同时设计导星辅助的方法消除上述误差,并通过运动先验信息反向传播模块调整系统。实验证明:所设计的系统不仅可以模拟真实星图,而且可以减弱星空环境对望远镜的误差影响。

     

  • 图 1  导星辅助的暗弱天体检测系统整体流程

    Figure 1.  Overall flow of guide star-assisted faint object detection system

    图 2  UCAC4星密度分布[2]

    Figure 2.  UCAC4 star density distribution[2]

    图 3  UCAC4坐标变换示意图

    Figure 3.  UCAC4 coordinate transformation diagram

    图 4  星图背景和目标灰度分布直方图

    Figure 4.  Star image background and target grayscale distribution histogram

    图 5  星图仿真去噪结果

    Figure 5.  Star map simulation denoising results

    图 6  实拍星图去噪结果

    Figure 6.  Real star map denoising results

    图 7  亚像素质心解算

    Figure 7.  Sub-pixel quality centroid solution

    图 8  2帧间导星运动示意图

    Figure 8.  Schematic diagram of guide star movement between two frames

    图 9  目标天体主焦面成像区域积分

    Figure 9.  Integral of the imaging area of the main focal plane of the target celestial body

    图 10  目标天体主焦面运动先验修正

    Figure 10.  A priori correction for the movement of the main focal plane of the target celestial body

    表  1  残差背景噪声统计

    Table  1.   Residual background noise statistics

    图像 均值/像素 标准差/像素
    原始图像 63.25 18.73
    背景消除图像 0.56 0.77
    下载: 导出CSV

    表  2  单导星多帧消融实验结果

    Table  2.   Results of ablation experiment for single guide star with multiple frames

    导星帧数/帧 运动先验误差/(像素·帧−1) 抖动误差/(像素·帧−1)
    2 1.37 0.631
    3 1.37 0.562
    4 1.37 0.560
    下载: 导出CSV

    表  3  多导星2帧消融实验结果

    Table  3.   Results of ablation experiment for multiple guide stars with two frames

    导星数/个 运动先验误差/(像素·帧−1) 抖动误差/(像素·帧−1)
    1 1.37 0.631
    2 1.37/0.751 0.491
    3 1.37/0.751/−0.107 0.412
    下载: 导出CSV

    表  4  条状目标端点定位结果

    Table  4.   Positioning results of strip target endpoints

    目标 坐标 精确坐标 检测坐标 修正坐标 原始定位误差/像素 修正定位误差/像素 定位误差降低量/像素
    目标1 x坐标 116.03 110.21 119.25 5.82 3.22 2.60
    y坐标 89.29 83.51 90.13 5.78 0.84 4.94
    目标2 x坐标 330.57 340.68 338.51 10.11 7.94 2.17
    y坐标 230.41 240.72 237.16 10.31 6.75 3.56
    目标3 x坐标 793.15 810.35 802.57 17.20 9.42 7.78
    y坐标 701.36 715.69 703.86 14.33 2.50 11.83
    下载: 导出CSV
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出版历程
  • 收稿日期:  2023-08-02
  • 录用日期:  2024-01-26
  • 网络出版日期:  2024-03-08
  • 整期出版日期:  2025-09-30

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