• Acta Photonica Sinica
  • Vol. 49, Issue 2, 0210001 (2020)
Zheng-zhou LI1、2、3、4, Lin QING1、2, Bo LI1、2, Cheng CHEN1、2, and Bo QI3、4
Author Affiliations
  • 1College of Microelectronics and Communication Engineering, Chongqing University, Chongqing 400044, China
  • 2Key Laboratory of Dependable Service Computing in Cyber Physical Society of Ministry of Education, Chongqing University, Chongqing 400044, China
  • 3Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China
  • 4Key Laboratory of Beam Control, Chinese Academy of Sciences, Chengdu 610209, China
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    DOI: 10.3788/gzxb20204902.0210001 Cite this Article
    Zheng-zhou LI, Lin QING, Bo LI, Cheng CHEN, Bo QI. Sparse Prior-based Space Objects Image Blind Inversion Algorithm[J]. Acta Photonica Sinica, 2020, 49(2): 0210001 Copy Citation Text show less
    Intensity histogram and gradient histogram images of space object in deep space background
    Fig. 1. Intensity histogram and gradient histogram images of space object in deep space background
    Intensity histogram and gradient histogram images of space object at different exposure levels
    Fig. 2. Intensity histogram and gradient histogram images of space object at different exposure levels
    Intensity histogram and gradient histogram images of space object in ground background
    Fig. 3. Intensity histogram and gradient histogram images of space object in ground background
    Fitting the gradient distribution of space object image with each prior
    Fig. 4. Fitting the gradient distribution of space object image with each prior
    Sparse representation of space object image
    Fig. 5. Sparse representation of space object image
    海事卫星图像高斯退化反演结果比较Compare of inversion results of Gaussian degraded maritime satellite image
    Fig. 6. 海事卫星图像高斯退化反演结果比较Compare of inversion results of Gaussian degraded maritime satellite image
    空间站图像高斯退化反演结果比较Compare of inversion results of Gaussian degraded space station image
    Fig. 7. 空间站图像高斯退化反演结果比较Compare of inversion results of Gaussian degraded space station image
    海事卫星图像运动退化反演结果比较Compare of inversion results of motion degraded maritime satellite image
    Fig. 8. 海事卫星图像运动退化反演结果比较Compare of inversion results of motion degraded maritime satellite image
    空间站图像运动退化反演结果比较Compare of inversion results of motion degraded space station image
    Fig. 9. 空间站图像运动退化反演结果比较Compare of inversion results of motion degraded space station image
    月球观测图像反演结果比较Compare of inversion results of lunar observation image
    Fig. 10. 月球观测图像反演结果比较Compare of inversion results of lunar observation image
    土星退化图像反演结果比较Compare of inversion results of real Saturn degraded image
    Fig. 11. 土星退化图像反演结果比较Compare of inversion results of real Saturn degraded image
    Standard deviation of Gaussian blur kernelSSIM/GMG
    Krishnan’sZhang’sPerrone’sPan’sLin’sOur method
    σ=10.868/2.3690.862/3.4450.857/3.5800.931/4.0010.890/4.1330.938/3.542
    σ=20.868/1.7800.873/2.3910.864/2.3140.923/2.3620.917/2.6120.928/2.632
    σ=30.884/1.5050.866/2.0150.865/1.6390.906/2.0780.901/2.0530.918/2.264
    σ=40.878/1.4230.869/1.9080.864/1.6700.879/1.8770.890/1.9970.914/2.116
    σ=50.874/1.3930.845/1.8860.863/1.7870.857/1.8540.904/2.0360.902/1.894
    Table 1. SSIM and GMG of the inversion results of Gaussian degraded maritime satellite image
    Standard deviation of Gaussian blur kernelSSIM/GMG
    Krishnan’sZhang’sPerrone’sPan’sLin’sOur method
    σ=10.873/8.6170.776/8.6560.515/9.4420.903/9.3480.926/9.7840.947/9.981
    σ=20.795/4.0740.808/5.3990.565/4.9400.833/4.8350.849/5.5580.857/5.620
    σ=30.734/3.6400.710/4.7340.558/4.2000.772/4.6540.801/4.8110.824/4.665
    σ=40.695/5.1950.757/4.3970.549/4.7660.652/5.8290.829/5.1210.806/4.746
    σ=50.674/5.0130.685/4.4830.548/5.0690.636/6.3830.824/5.0050.834/4.955
    Table 2. SSIM and GMG of the inversion results of Gaussian degraded space station image
    Blur scale of motion blurSSIM/GMG
    Krishnan’sZhang’sPerrone’sPan’sLin’sOur method
    90.859/3.9340.885/3.5320.841/3.7060.891/4.1260.936/4.0630.951/3.983
    130.875/3.3690.863/3.1870.856/3.1630.850/3.7110.928/3.6270.935/3.814
    170.876/3.6170.859/3.0590.853/2.9980.822/3.4340.916/3.5610.921/3.729
    210.820/3.1430.852/2.9160.854/2.9530.799/3.4550.913/3.4850.915/3.492
    250.815/3.2480.846/2.7130.853/2.6520.814/3.1790.904/3.2590.898/3.310
    Table 3. SSIM and GMG of the inversion results of motion degraded maritime satellite image
    Standard deviation of Gaussian blur kernelSSIM/GMG
    Krishnan’sZhang’sPerrone’sPan’sLin’sOur method
    90.719/5.4800.799/7.2270.515/8.1040.652/8.1310.842/8.7610.869/8.794
    130.649/4.8190.763/6.4900.520/8.1900.627/7.9420.807/8.1750.844/8.203
    170.615/6.6080.752/5.5680.531/6.8620.550/7.7700.836/6.8420.850/6.711
    210.567/5.9670.741/5.4020.546/6.8210.495/7.1080.847/6.8590.851/6.617
    250.543/5.9750.726/4.8890.547/6.0000.493/5.8590.813/5.7580.836/6.294
    Table 4. SSIM and GMG of the inversion results of motion degraded space station image
    Degraded imageEvaluation indexesKrishnan’sZhang’sPerrone’sPan’sLin’sOurs
    lunar imageGMG2.8182.8452.8202.6852.8643.2642.8092.5802.8493.1102.8973.623
    Saturn imageGMG3.719 22.924 93.648 52.698 53.742 93.012 43.530 32.407 903.644 92.700 83.729 84.328 6
    Table 5. Objective evaluation results of the estimated real space object image
    Zheng-zhou LI, Lin QING, Bo LI, Cheng CHEN, Bo QI. Sparse Prior-based Space Objects Image Blind Inversion Algorithm[J]. Acta Photonica Sinica, 2020, 49(2): 0210001
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