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Full waveform inversion by proximal Newton method using adaptive regularization

机译:使用自适应正规化的Proximal Newton方法全波形反转

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摘要

Regularization is necessary for solving non-linear ill-posed inverse problems arising in different fields of geosciences. The base of a suitable regularization is the prior expressed by the regularizer, which can be non-adaptive or adaptive (data-driven), smooth or non-smooth, variational-based or not. Nevertheless, tailoring a suitable and easy-to-implement prior for describing geophysical models is a non-trivial task. In this paper, we propose two generic optimization algorithms to implement arbitrary regularization in non-linear inverse problems such as full-waveform inversion (FWI), where the regularization task is recast as a denoising problem. We assess these optimization algorithms with the plug-and-play block matching (BM3D) regularization algorithm, which determines empirical priors adaptively without any optimization formulation. The non-linear inverse problem is solved with a proximal Newton method, which generalizes the traditional Newton step in such a way to involve the gradients/subgradients of a (possibly non-differentiable) regularization function through operator splitting and proximal mappings. Furthermore, it requires to account for the Hessian matrix in the regularized least-squares optimization problem. We propose two different splitting algorithms for this task. In the first, we compute the Newton search direction with an iterative method based upon the first-order generalized iterative shrinkage-thresholding algorithm (ISTA), and hence Newton-ISTA (NISTA). The iterations require only Hessian-vector products to compute the gradient step of the quadratic approximation of the non-linear objective function. The second relies on the alternating direction method of multipliers (ADMM), and hence Newton-ADMM (NADMM), where the least-squares optimization subproblem and the regularization subproblem in the composite objective function are decoupled through auxiliary variable and solved in an alternating mode. The least-squares subproblem can be solved with exact, inexact, or quasi-Newton methods. We compare NISTA and NADMM numerically by solving FWI with BM3D regularization. The tests show promising results obtained by both algorithms. However, NADMM shows a faster convergence rate than NISTA when using L-BFGS to solve the Newton system.
机译:正规化是解决在地质不同领域产生的非线性缺陷逆问题所必需的。合适的正则化的基础是由规范器的先前表达,它可以是非自适应或自适应(数据驱动的),平滑或非光滑,变分或不为基础。然而,在描述地球物理模型的情况下剪裁合适且易于实现的是一种非琐碎的任务。在本文中,我们提出了两个通用优化算法来实现非线性逆问题的任意正则化,例如全波形反转(FWI),其中正则化任务是作为去噪问题的重量。我们利用即插即用块匹配(BM3D)正则化算法评估这些优化算法,其在没有任何优化制剂的情况下自适应地确定经验前提。使用近端牛顿方法解决了非线性逆问题,其概括了传统的牛顿步骤,以涉及通过操作员分离和近端映射的(可能是非可微分)正则化函数的梯度/子分析。此外,它需要考虑正规化的最小二乘优化问题的Hessian矩阵。我们为此任务提出了两个不同的分割算法。首先,我们使用基于一阶广义迭代收缩 - 阈值算法(ISTA)的迭代方法计算牛顿搜索方向,因此Newton-Ista(Nista)。迭代仅需要Hessian-向量产品来计算非线性目标函数的二次近似的梯度步骤。第二次依赖于乘法器(ADMM)的交替方向方法,因此牛顿 - ADMM(NADMM),其中复合物镜函数中最小二乘优化子发电机和正则化子问题通过辅助变量解耦并在交替模式下解决。可以用精确,不精确或准牛顿方法解决最小二乘子问题。通过使用BM3D正规化,通过解决FWI来比较Nista和NADMM。测试显示了两种算法获得的有希望的结果。然而,当使用L-BFG来解决牛顿系统时,NADMM显示比NISTA更快的收敛速度。

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