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Nonlinear image recovery with half-quadratic regularization

机译:具有半二次正则化的非线性图像恢复

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One popular method for the recovery of an ideal intensity image from corrupted or indirect measurements is regularization: minimize an objective function that enforces a roughness penalty in addition to coherence with the data. Linear estimates are relatively easy to compute but generally introduce systematic errors; for example, they are incapable of recovering discontinuities and other important image attributes. In contrast, nonlinear estimates are more accurate but are often far less accessible. This is particularly true when the objective function is nonconvex, and the distribution of each data component depends on many image components through a linear operator with broad support. Our approach is based on an auxiliary array and an extended objective function in which the original variables appear quadratically and the auxiliary variables are decoupled. Minimizing over the auxiliary array alone yields the original function so that the original image estimate can be obtained by joint minimization. This can be done efficiently by Monte Carlo methods, for example by FFT-based annealing using a Markov chain that alternates between (global) transitions from one array to the other. Experiments are reported in optical astronomy, with space telescope data, and computed tomography.
机译:从损坏的或间接的测量中恢复理想强度图像的一种流行方法是正则化:除与数据的一致性外,最小化强制执行粗糙度损失的目标函数。线性估计相对容易计算,但通常会引入系统误差。例如,它们无法恢复不连续性和其他重要的图像属性。相反,非线性估计更准确,但通常很难获得。当目标函数是非凸的并且每个数据分量的分布取决于具有广泛支持的线性算子时,这取决于许多图像分量,这一点尤其正确。我们的方法基于一个辅助数组和一个扩展目标函数,其中原始变量呈二次方出现,辅助变量解耦。仅通过最小化辅助阵列即可产生原始函数,从而可以通过联合最小化来获得原始图像估计。这可以通过蒙特卡洛方法有效地完成,例如通过使用从一个阵列到另一个阵列的(全局)转换之间交替的马尔可夫链进行基于FFT的退火。光学天文学,太空望远镜数据和计算机断层扫描技术报道了实验。

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