• Optics and Precision Engineering
  • Vol. 32, Issue 23, 3436 (2024)
Liduo SONG1, Kainan YAO1,*, Zhiqiang XU1, Jianli WANG1..., Jian GU2, Sheng QUAN1,3, Ming CHEN4 and Haoran JIA5|Show fewer author(s)
Author Affiliations
  • 1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun30033, China
  • 263768Troop, PLA, Xi'an 710600, China
  • 3University of Chinese Academy of Sciences, Beijing100049, China
  • 432011Troop, PLA, Beijing 10009, China
  • 5Changchun University of Science and Technology, Changchun130022, China
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    DOI: 10.37188/OPE.20243223.3436 Cite this Article
    Liduo SONG, Kainan YAO, Zhiqiang XU, Jianli WANG, Jian GU, Sheng QUAN, Ming CHEN, Haoran JIA. Stars removal of all day time mid-high orbit target detection system[J]. Optics and Precision Engineering, 2024, 32(23): 3436 Copy Citation Text show less
    Data flow of star removal algorithm
    Fig. 1. Data flow of star removal algorithm
    Comparison between original and background image
    Fig. 2. Comparison between original and background image
    Comparison of extraction effects
    Fig. 3. Comparison of extraction effects
    Bounding rectangle of target
    Fig. 4. Bounding rectangle of target
    Comparison between noise and star
    Fig. 5. Comparison between noise and star
    Flowchart of single frame detection
    Fig. 6. Flowchart of single frame detection
    Flowchart of multi frame detection
    Fig. 7. Flowchart of multi frame detection
    Schematic diagram of replacement principle
    Fig. 8. Schematic diagram of replacement principle
    Experimental 500 mm all day time detection optical telescope
    Fig. 9. Experimental 500 mm all day time detection optical telescope
    Stars removed effect
    Fig. 10. Stars removed effect
    Comparison of multi-frame algorithm effects
    Fig. 11. Comparison of multi-frame algorithm effects
    Remove failed situation
    Fig. 12. Remove failed situation
    Algorithm time consumption statistics
    Fig. 13. Algorithm time consumption statistics
    ParameterValue
    Spectral range/(Μ·m)0.9~1.7
    Pixel pitch/(Μ·m)15
    Pixel depth/Bit16
    Field of view/(')10(Diagonal)
    Max frame rate/Hz100
    Optical aperture/(M·m)500
    Focal length/(M·m)4 000
    Tracking accuracy/(″)<2
    Table 1. Main parameters of telescope
    VmagHip numIncompletelyUnrecognizedSuccess
    1.1637 826100%0%0%
    1.9946 390100%0%0%
    3.1143 813100%0%0%
    4~9-0%0%100%
    10.1639 3920%86%14%
    Table 2. Success rate of removing stars during daytime
    VmagHip numIncompletelyUnrecognizedSuccess
    1.17113 368100%0%0%
    2.043 419100%0%0%
    3.05100 345100%0%0%
    4.04111 49719%0%81%
    5~9-0%0%100%
    10.1139 3920%18%72%
    Table 3. Success rate of removing stars during night
    ModuleModel
    CPUIntel(R) Core(TM) i7-6700HQ CPU @ 2.60 GHz
    GPUNVIDIA GeForce GTX 960M
    OSWindows 10
    LanguageC++, OpenCL
    Table 4. Algorithm processing platform
    Liduo SONG, Kainan YAO, Zhiqiang XU, Jianli WANG, Jian GU, Sheng QUAN, Ming CHEN, Haoran JIA. Stars removal of all day time mid-high orbit target detection system[J]. Optics and Precision Engineering, 2024, 32(23): 3436
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