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Autores principales: Cheng, Sihao, Morel, Rudy, Allys, Erwan, Ménard, Brice, Mallat, Stéphane
Formato: Preprint
Publicado: 2023
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Acceso en línea:https://arxiv.org/abs/2306.17210
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author Cheng, Sihao
Morel, Rudy
Allys, Erwan
Ménard, Brice
Mallat, Stéphane
author_facet Cheng, Sihao
Morel, Rudy
Allys, Erwan
Ménard, Brice
Mallat, Stéphane
contents Physicists routinely need probabilistic models for a number of tasks such as parameter inference or the generation of new realizations of a field. Establishing such models for highly non-Gaussian fields is a challenge, especially when the number of samples is limited. In this paper, we introduce scattering spectra models for stationary fields and we show that they provide accurate and robust statistical descriptions of a wide range of fields encountered in physics. These models are based on covariances of scattering coefficients, i.e. wavelet decomposition of a field coupled with a point-wise modulus. After introducing useful dimension reductions taking advantage of the regularity of a field under rotation and scaling, we validate these models on various multi-scale physical fields and demonstrate that they reproduce standard statistics, including spatial moments up to 4th order. These scattering spectra provide us with a low-dimensional structured representation that captures key properties encountered in a wide range of physical fields. These generic models can be used for data exploration, classification, parameter inference, symmetry detection, and component separation.
format Preprint
id arxiv_https___arxiv_org_abs_2306_17210
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Scattering Spectra Models for Physics
Cheng, Sihao
Morel, Rudy
Allys, Erwan
Ménard, Brice
Mallat, Stéphane
Data Analysis, Statistics and Probability
Instrumentation and Methods for Astrophysics
Computer Vision and Pattern Recognition
Machine Learning
Physicists routinely need probabilistic models for a number of tasks such as parameter inference or the generation of new realizations of a field. Establishing such models for highly non-Gaussian fields is a challenge, especially when the number of samples is limited. In this paper, we introduce scattering spectra models for stationary fields and we show that they provide accurate and robust statistical descriptions of a wide range of fields encountered in physics. These models are based on covariances of scattering coefficients, i.e. wavelet decomposition of a field coupled with a point-wise modulus. After introducing useful dimension reductions taking advantage of the regularity of a field under rotation and scaling, we validate these models on various multi-scale physical fields and demonstrate that they reproduce standard statistics, including spatial moments up to 4th order. These scattering spectra provide us with a low-dimensional structured representation that captures key properties encountered in a wide range of physical fields. These generic models can be used for data exploration, classification, parameter inference, symmetry detection, and component separation.
title Scattering Spectra Models for Physics
topic Data Analysis, Statistics and Probability
Instrumentation and Methods for Astrophysics
Computer Vision and Pattern Recognition
Machine Learning
url https://arxiv.org/abs/2306.17210