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A new Point Spread Function estimation approach for recovery of atmospheric turbulence degraded photographs

机译:一种新的点扩散函数估计方法,用于恢复大气湍流退化的照片

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Images acquired by an optical system are usually degraded by atmospheric turbulence, which exists in the path between the targets and the imaging system. The estimation of atmospheric turbulence degraded Point Spread Function (PSF) without any prior knowledge of clear images is the most challenging and significant technique on image restoration. In this paper, a new PSF estimation approach is proposed for long-exposure atmospheric turbulence degraded images, and is applied to image restoration successfully. The PSF is estimated via an isosceles model which is proposed to approximate one component of the original image's Fourier amplitude. On degraded image restoration, the short-exposure image frames are transformed into a single long-exposure image, and then the restored image is obtained by using the estimated PSF and Wiener Filter. Numerical experiments suggest that this algorithm can obtain accurate PSF from both synthetic and real images. It is also shown objectively that the quality of restored images is greatly enhanced, by applying the Gray Mean Grads and Laplacian Sum standards.
机译:由光学系统获取的图像通常会由于大气湍流而退化,大气湍流存在于目标与成像系统之间的路径中。在没有任何先验清晰图像知识的情况下,估计大气湍流退化点扩展函数(PSF)是图像恢复中最具挑战性和最重要的技术。本文针对长时间曝光的大气湍流退化图像提出了一种新的PSF估计方法,并将其成功地应用于图像复原。通过等腰模型估计PSF,该模型被提出来近似原始图像的傅立叶振幅的一个分量。在降级图像恢复中,将短曝光图像帧转换为单个长曝光图像,然后使用估计的PSF和维纳滤波器获得恢复的图像。数值实验表明,该算法可以从合成图像和真实图像中获得准确的PSF。还客观地表明,通过应用灰度平均等级和拉普拉斯求和标准,可以大大提高恢复图像的质量。

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