Author Affiliations
1College of Microelectronics and Communication Engineering, Chongqing University, Chongqing 400044, China2Key Laboratory of Dependable Service Computing in Cyber Physical Society of Ministry of Education, Chongqing University, Chongqing 400044, China3Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China4Key Laboratory of Beam Control, Chinese Academy of Sciences, Chengdu 610209, Chinashow less
Fig. 1. Intensity histogram and gradient histogram images of space object in deep space background
Fig. 2. Intensity histogram and gradient histogram images of space object at different exposure levels
Fig. 3. Intensity histogram and gradient histogram images of space object in ground background
Fig. 4. Fitting the gradient distribution of space object image with each prior
Fig. 5. Sparse representation of space object 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
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
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
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
Fig. 10. 月球观测图像反演结果比较Compare of inversion results of lunar observation 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 kernel | SSIM/GMG | Krishnan’s | Zhang’s | Perrone’s | Pan’s | Lin’s | Our method | σ=1 | 0.868/2.369 | 0.862/3.445 | 0.857/3.580 | 0.931/4.001 | 0.890/4.133 | 0.938/3.542 | σ=2 | 0.868/1.780 | 0.873/2.391 | 0.864/2.314 | 0.923/2.362 | 0.917/2.612 | 0.928/2.632 | σ=3 | 0.884/1.505 | 0.866/2.015 | 0.865/1.639 | 0.906/2.078 | 0.901/2.053 | 0.918/2.264 | σ=4 | 0.878/1.423 | 0.869/1.908 | 0.864/1.670 | 0.879/1.877 | 0.890/1.997 | 0.914/2.116 | σ=5 | 0.874/1.393 | 0.845/1.886 | 0.863/1.787 | 0.857/1.854 | 0.904/2.036 | 0.902/1.894 |
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Table 1. SSIM and GMG of the inversion results of Gaussian degraded maritime satellite image
Standard deviation of Gaussian blur kernel | SSIM/GMG | Krishnan’s | Zhang’s | Perrone’s | Pan’s | Lin’s | Our method | σ=1 | 0.873/8.617 | 0.776/8.656 | 0.515/9.442 | 0.903/9.348 | 0.926/9.784 | 0.947/9.981 | σ=2 | 0.795/4.074 | 0.808/5.399 | 0.565/4.940 | 0.833/4.835 | 0.849/5.558 | 0.857/5.620 | σ=3 | 0.734/3.640 | 0.710/4.734 | 0.558/4.200 | 0.772/4.654 | 0.801/4.811 | 0.824/4.665 | σ=4 | 0.695/5.195 | 0.757/4.397 | 0.549/4.766 | 0.652/5.829 | 0.829/5.121 | 0.806/4.746 | σ=5 | 0.674/5.013 | 0.685/4.483 | 0.548/5.069 | 0.636/6.383 | 0.824/5.005 | 0.834/4.955 |
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Table 2. SSIM and GMG of the inversion results of Gaussian degraded space station image
Blur scale of motion blur | SSIM/GMG | Krishnan’s | Zhang’s | Perrone’s | Pan’s | Lin’s | Our method | 9 | 0.859/3.934 | 0.885/3.532 | 0.841/3.706 | 0.891/4.126 | 0.936/4.063 | 0.951/3.983 | 13 | 0.875/3.369 | 0.863/3.187 | 0.856/3.163 | 0.850/3.711 | 0.928/3.627 | 0.935/3.814 | 17 | 0.876/3.617 | 0.859/3.059 | 0.853/2.998 | 0.822/3.434 | 0.916/3.561 | 0.921/3.729 | 21 | 0.820/3.143 | 0.852/2.916 | 0.854/2.953 | 0.799/3.455 | 0.913/3.485 | 0.915/3.492 | 25 | 0.815/3.248 | 0.846/2.713 | 0.853/2.652 | 0.814/3.179 | 0.904/3.259 | 0.898/3.310 |
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Table 3. SSIM and GMG of the inversion results of motion degraded maritime satellite image
Standard deviation of Gaussian blur kernel | SSIM/GMG | Krishnan’s | Zhang’s | Perrone’s | Pan’s | Lin’s | Our method | 9 | 0.719/5.480 | 0.799/7.227 | 0.515/8.104 | 0.652/8.131 | 0.842/8.761 | 0.869/8.794 | 13 | 0.649/4.819 | 0.763/6.490 | 0.520/8.190 | 0.627/7.942 | 0.807/8.175 | 0.844/8.203 | 17 | 0.615/6.608 | 0.752/5.568 | 0.531/6.862 | 0.550/7.770 | 0.836/6.842 | 0.850/6.711 | 21 | 0.567/5.967 | 0.741/5.402 | 0.546/6.821 | 0.495/7.108 | 0.847/6.859 | 0.851/6.617 | 25 | 0.543/5.975 | 0.726/4.889 | 0.547/6.000 | 0.493/5.859 | 0.813/5.758 | 0.836/6.294 |
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Table 4. SSIM and GMG of the inversion results of motion degraded space station image
Degraded image | Evaluation indexes | Krishnan’s | Zhang’s | Perrone’s | Pan’s | Lin’s | Ours | lunar image | GMG | 2.8182.845 | 2.8202.685 | 2.8643.264 | 2.8092.580 | 2.8493.110 | 2.8973.623 | Saturn image | GMG | 3.719 22.924 9 | 3.648 52.698 5 | 3.742 93.012 4 | 3.530 32.407 90 | 3.644 92.700 8 | 3.729 84.328 6 |
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Table 5. Objective evaluation results of the estimated real space object image