The use of non-linear inverse problem and enthalpy method in GTAW process of aluminum

Author(s):  
Elisan dos Santos Magalhães ◽  
Solidônio Rodrigues de Carvalho ◽  
Ana Lúcia Fernandes de Lima E Silva ◽  
Sandro Metrevelle Marcondes Lima E Silva
2017 ◽  
Vol 33 (8) ◽  
pp. 085010
Author(s):  
Giulia Denevi ◽  
Sara Garbarino ◽  
Alberto Sorrentino

2020 ◽  
Vol 2020 (14) ◽  
pp. 146-1-146-8
Author(s):  
K. Aditya Mohan ◽  
Dilworth Y. Parkinson ◽  
Jefferson A. Cuadra

X-ray phase contrast tomography (XPCT) is widely used for 3D imaging of objects with weak contrast in X-ray absorption index but strong contrast in refractive index decrement. To reconstruct an object imaged using XPCT, phase retrieval algorithms are first used to estimate the X-ray phase projections, which is the 2D projection of the refractive index decrement, at each view. Phase retrieval is followed by refractive index decrement reconstruction from the phase projections using an algorithm such as filtered back projection (FBP). In practice, phase retrieval is most commonly solved by approximating it as a linear inverse problem. However, this linear approximation often results in artifacts and blurring when the conditions for the approximation are violated. In this paper, we formulate phase retrieval as a non-linear inverse problem, where we solve for the transmission function, which is the negative exponential of the projections, from XPCT measurements. We use a constraint to enforce proportionality between phase and absorption projections. We do not use constraints such as large Fresnel number, slowly varying phase, or Born/Rytov approximations. Our approach also does not require any regularization parameter tuning since there is no explicit sparsity enforcing regularization function. We validate the performance of our non-linear phase retrieval (NLPR) method using both simulated and real synchrotron datasets. We compare NLPR with a popular linear phase retrieval (LPR) approach and show that NLPR achieves sharper reconstructions with higher quantitative accuracy.


2020 ◽  
Author(s):  
Ondřej Tichý ◽  
Václav Šmídl

<div>The basic linear inverse problem of atmospheric release can be formulated as <strong>y</strong> = M <strong>x</strong> + <strong>e</strong> , where <strong>y</strong> is the measurement vector which is typically in the form of gamma dose rates or concentrations, M is the source-receptor-sensitivity (SRS) matrix, <strong>x</strong> is the unknown source term to be estimated, and <strong>e</strong> is the model residue. The SRS matrix M is computed using an atmospheric transport model coupled with meteorological reanalyses. The inverse problem is typically ill-conditioned due to number of uncertainties, hence, the estimation of the source term is not straightforward and additional information, e.g. in the form of regularization or the prior source term, is often needed. Besides, traditional techniques rely on assumption that the SRS matrix is correct which is not realistic due to the number of approximations made during its computation. Therefore, we propose relaxation of the inverse model using introduction of the term Δ<sub>M</sub> such as <strong>y</strong> = ( M+ Δ<sub>M</sub> ) <strong>x</strong> + <strong>e</strong> leading to non-linear inverse problem formulation, where Δ<sub>M</sub> can be, as an example, parametric perturbation of the SRS matrix M in the spatial or temporal domain. We estimate parameters of this perturbation together with solving the inverse problem using variational Bayes procedure. The method will be validated on synthetic dataset as well as demonstrated on real case scenario such as the controlled tracer experiment ETEX or episode of ruthenium-106 release over the Europe on the fall of 2017.</div>


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