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首页> 外文期刊>Acta Automatica Sinica >Restoring Turbulence-Degraded Images Based on Estimation of Turbulence Point Spread Function Values
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Restoring Turbulence-Degraded Images Based on Estimation of Turbulence Point Spread Function Values

机译:基于湍流点扩展函数值估计的湍流退化图像恢复

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摘要

A new method is proposed for estimating the PSF(point spread function) values of turbulence from turbulence-degraded images. Instead of previously used natural or artificial guide star images to measure the PSF, two consecutive frames of short-exposure turbulence-degraded images are used directly as the input. Appropriate extension are made for the images in the spatial domain and a series of equations for calculating the PSF values are developed and chosen in the frequency domain. In order to overcome the interference of noise, the PSF calculation is transformed into the optimization estimation under the constraints of the PSF being non-negative and spatial smoothing. The values of the PSF are estimated by minimization criteria function and then the degraded images are restored. Experimental results show that the proposed method is highly effective with good performance.
机译:提出了一种从湍流退化图像中估计湍流的PSF(点扩散函数)值的新方法。代替先前使用的自然或人工制导星图像来测量PSF,直接将短曝光湍流退化图像的两个连续帧用作输入。在空间域中对图像进行适当的扩展,并在频域中开发和选择用于计算PSF值的一系列方程。为了克服噪声的干扰,在PSF为非负和空间平滑的约束下,将PSF计算转换为优化估计。通过最小化标准函数估计PSF的值,然后恢复退化的图像。实验结果表明,该方法是一种高效,高效的方法。

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