• Acta Photonica Sinica
  • Vol. 51, Issue 3, 0304002 (2022)
Di PAN, Qi ZHOU*, Xuan LIU, Bing LIU, and Hui FANG
Author Affiliations
  • Shanghai Aerospace Control Technology Institute,Shanghai Key Laboratory of Aerospace Intelligent Control Technology,Shanghai 201109,China
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    DOI: 10.3788/gzxb20225103.0304002 Cite this Article
    Di PAN, Qi ZHOU, Xuan LIU, Bing LIU, Hui FANG. Modeling and Detection of Star Spot in High Dynamic Condition[J]. Acta Photonica Sinica, 2022, 51(3): 0304002 Copy Citation Text show less
    Static star spot model
    Fig. 1. Static star spot model
    Static star spot model in guide star catalogue
    Fig. 2. Static star spot model in guide star catalogue
    Flow diagram for dynamic star spot template generation
    Fig. 3. Flow diagram for dynamic star spot template generation
    Dynamic star spot generation process
    Fig. 4. Dynamic star spot generation process
    Star sensor experiment diagram
    Fig. 5. Star sensor experiment diagram
    Angle distance error curves of three star point extraction methods under three angular velocities
    Fig. 6. Angle distance error curves of three star point extraction methods under three angular velocities
    Angle distance error curves of three star point extraction methods under three exposure time
    Fig. 7. Angle distance error curves of three star point extraction methods under three exposure time
    FOV/(°)Area array/(pix×pix)Pixel size Dp/μmFocal length f/mm
    201 024×1 0241851.957
    Table 1. Optical system parameters of the star sensor
    Angular velocity ω/(°·s-1

    Angle distance error

    Δθ/(")

    Extraction rate

    γ

    Time

    t/ s

    Mean3sigmaMeanMaximumMinimum
    18.213.461.001.001.004.16
    211.695.340.991.000.934.65
    322.3513.180.981.000.914.87
    Table 2. Experimental results of cross correlation template matching method using simple template at three angular velocities
    Angular velocity ω/(°·s-1

    Angle distance error

    Δθ/(")

    Extraction rate

    γ

    Time

    t/ s

    Mean3sigmaMeanMaximumMinimum
    18.052.501.001.001.001 896.64
    211.056.020.991.000.932 260.05
    320.9114.100.981.000.912 387.73
    Table 3. Experimental results of cross correlation template matching method using complex template at three angular velocities
    Angular velocity ω/(°·s-1

    Angle distance error

    Δθ/(")

    Extraction rate

    γ/%

    Time

    t/ s

    Mean3sigmaMeanMaximumMinimum
    110.725.340.971.000.974.05
    216.019.060.941.000.824.57
    333.4820.660.831.000.734.69
    Table 4. Experimental results of traditional method at three angular velocities

    Exposure time

    tex/ ms

    Angle distance error Δθ/(")Extraction rate γ

    Time

    t/ s

    Mean3sigmaMeanMaximumMinimum
    8622.0513.220.981.000.945.03
    62.513.178.860.991.000.934.76
    5010.144.480.971.000.914.38
    Table 5. Experimental results of cross correlation template matching method using simple template at three exposure time

    Exposure time

    tex/ ms

    Angle distance error Δθ/(")Extraction rate γ

    Time

    t/ s

    Mean3sigmaMeanMaximumMinimum
    8621.4912.770.981.000.942 368.98
    62.513.479.130.991.000.932 056.19
    5010.605.200.971.000.911 934.20
    Table 6. Experimental results of cross correlation template matching method using complex template at three exposure time

    Exposure time

    tex/ ms

    Angle distance error Δθ/(")Extraction rate γ

    Time

    t/ s

    Mean3sigmaMeanMaximumMinimum
    8633.9320.760.891.000.594.56
    62.520.5613.500.821.000.654.36
    5018.0914.630.711.000.594.49
    Table 7. Experimental results of traditional method at three exposure time
    Di PAN, Qi ZHOU, Xuan LIU, Bing LIU, Hui FANG. Modeling and Detection of Star Spot in High Dynamic Condition[J]. Acta Photonica Sinica, 2022, 51(3): 0304002
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