Acta Photonica Sinica, Volume. 50, Issue 2, 155(2021)

An On-orbit Correction Method for High Dynamic APS Star Tracker Based on Adaptive Filtering

Yaxian HOU1,2,3, Rujin ZHAO1,2,3, Yuebo MA1,2,3, Longdong HE1,2,3, and Zifa ZHU1,2,3
Author Affiliations
  • 1Institute of Optics and Electronics of Chinese Academy of Sciences, Chengdu60209, China
  • 2University of Chinese Academy of Sciences, Beijing100049, China
  • 3Key Laboratory of Science and Technology on Space Optoelectronic Precision Measurement, Chinese Academy of Sciences, Chengdu610209, China
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    Figures & Tables(14)
    Workflow of star sensor
    Simulation star point
    Star centroid extraction process
    Algorithm block diagram
    Star point area and correction matrix diagram
    Schematic diagram of star centroid moving in continuous frame of image at low speed
    The process of obtaining correction matrix C at low speed
    Schematic diagram of star centroid moving in continuous frame of image at high speed
    Correction results using different methods at different angular velocities
    The 3D map of star point at different angular velocities
    Correction results using different methods at different angular velocities
    Centroid error of star before and after correction under different noise intensity
    The 3D map of star point under different noise intensity
    • Table 1. Parameters of real star sensor

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      Table 1. Parameters of real star sensor

      Star sensor parameters
      Field of view/(°)20×20
      Exposure time/ms118
      Frame rate/Hz10
      Imager size/pixel21 024×1 024
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    Yaxian HOU, Rujin ZHAO, Yuebo MA, Longdong HE, Zifa ZHU. An On-orbit Correction Method for High Dynamic APS Star Tracker Based on Adaptive Filtering[J]. Acta Photonica Sinica, 2021, 50(2): 155

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    Paper Information

    Category: Instrumentation, Measurement and Metrology

    Received: --

    Accepted: --

    Published Online: Aug. 26, 2021

    The Author Email:

    DOI:10.3788/gzxb20215002.0212004

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