Laser & Optoelectronics Progress, Volume. 56, Issue 10, 101101(2019)

Method for Determining Optimal Radius Value of Defocused Image Spot of Star Sensor

Haiyong Wang1, Tengfei Wang1、*, Hongyu Zhu1, Tao Liu2, and Chengjun Ge2
Author Affiliations
  • 1 School of Astronautics, Beihang University, Beijing 100191, China
  • 2 Beijing Aerospace Wanyuan Science & Technology Co. Ltd., Beijing 100176, China;
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    Figures & Tables(5)
    Simulated star point based on IPSF model. (a) σs=0.6 pixel; (b) σs=1.5 pixel
    Three-dimensional distribution of centroid localization error σe with respect to Gaussian radius σs and background noise σg
    Fitting result of centroid localization error model
    Two-dimensional map of equal precision lines for centroid location
    • Table 1. Least square surface fitting coefficient matrix of error model

      View table

      Table 1. Least square surface fitting coefficient matrix of error model

      ji
      01234
      02.7311×10-22.5645×10-2-1.1732×10-25.7245×10-2-1.2370×10-2
      1-8.6410×10-2-5.9339×1023.8144×105-2.0382×1084.4994×10-2
      29.9384×10-25.5022×102-4.2957×1052.4146×108-5.3916×10-2
      3-4.9407×10-2-2.2699×1022.0010×105-1.1607×1082.6108×1010
      49.0078×10-33.4404×10-1-3.2924×10-41.9515×107-4.4130×10-9
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    Haiyong Wang, Tengfei Wang, Hongyu Zhu, Tao Liu, Chengjun Ge. Method for Determining Optimal Radius Value of Defocused Image Spot of Star Sensor[J]. Laser & Optoelectronics Progress, 2019, 56(10): 101101

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    Paper Information

    Category: Imaging Systems

    Received: Nov. 26, 2018

    Accepted: Dec. 7, 2018

    Published Online: Jul. 4, 2019

    The Author Email: Wang Tengfei (oktengfei@126.com)

    DOI:10.3788/LOP56.101101

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