Lingyun Yang, Omar M. Saad, Guochen Wu, Tariq Alkhalifah
{"title":"Conditional Image Prior for Uncertainty Quantification in Full Waveform Inversion","authors":"Lingyun Yang, Omar M. Saad, Guochen Wu, Tariq Alkhalifah","doi":"arxiv-2408.09975","DOIUrl":null,"url":null,"abstract":"Full Waveform Inversion (FWI) is a technique employed to attain a high\nresolution subsurface velocity model. However, FWI results are effected by the\nlimited illumination of the model domain and the quality of that illumination,\nwhich is related to the quality of the data. Additionally, the high\ncomputational cost of FWI, compounded by the high dimensional nature of the\nmodel space, complicates the evaluation of model uncertainties. Recent work on\napplying neural networks to represent the velocity model for FWI demonstrated\nthe network's ability to capture the salient features of the velocity model.\nThe question we ask here is how reliable are these features in representing the\nobserved data contribution within the model space (the posterior distribution).\nTo address this question, we propose leveraging a conditional Convolutional\nNeural Network (CNN) as image prior to quantify the neural network\nuncertainties. Specifically, we add to the deep image prior concept a\nconditional channel, enabling the generation of various models corresponding to\nthe specified condition. We initially train the conditional CNN to learn\n(store) samples from the prior distribution given by Gaussian Random Fields\n(GRF) based perturbations of the current velocity model. Subsequently, we use\nFWI to update the CNN model representation of the priors so that it can\ngenerate samples from the posterior distribution. These samples can be used to\nmeasure the approximate mean and standard deviation of the posterior\ndistribution, as well as draw samples representing the posterior distribution.\nWe demonstrate the effectiveness of the proposed approach on the Marmousi model\nand in a field data application.","PeriodicalId":501270,"journal":{"name":"arXiv - PHYS - Geophysics","volume":"21 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Geophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.09975","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Full Waveform Inversion (FWI) is a technique employed to attain a high
resolution subsurface velocity model. However, FWI results are effected by the
limited illumination of the model domain and the quality of that illumination,
which is related to the quality of the data. Additionally, the high
computational cost of FWI, compounded by the high dimensional nature of the
model space, complicates the evaluation of model uncertainties. Recent work on
applying neural networks to represent the velocity model for FWI demonstrated
the network's ability to capture the salient features of the velocity model.
The question we ask here is how reliable are these features in representing the
observed data contribution within the model space (the posterior distribution).
To address this question, we propose leveraging a conditional Convolutional
Neural Network (CNN) as image prior to quantify the neural network
uncertainties. Specifically, we add to the deep image prior concept a
conditional channel, enabling the generation of various models corresponding to
the specified condition. We initially train the conditional CNN to learn
(store) samples from the prior distribution given by Gaussian Random Fields
(GRF) based perturbations of the current velocity model. Subsequently, we use
FWI to update the CNN model representation of the priors so that it can
generate samples from the posterior distribution. These samples can be used to
measure the approximate mean and standard deviation of the posterior
distribution, as well as draw samples representing the posterior distribution.
We demonstrate the effectiveness of the proposed approach on the Marmousi model
and in a field data application.