Posterior sampling for inverse imaging problems on the sphere in seismology and cosmology
Augustin Marignier, Jason D. McEwen, Ana M. G. Ferreira and, Thomas D. Kitching

TL;DR
This paper introduces a proximal MCMC framework for efficiently sampling high-dimensional spherical inverse problems, enabling full uncertainty quantification in seismology and cosmology applications.
Contribution
It develops a modified proximal MCMC algorithm tailored for spherical problems with wavelet priors, including computational strategies for spherical harmonic transforms.
Findings
Effective in moderate-resolution cosmological mass-mapping
Applicable to global seismic tomography problems
Provides full uncertainty quantification
Abstract
Inverse problems defined on the sphere arise in many fields, including seismology and cosmology where problems are defined on the globe and the cosmic sphere. These are generally high-dimensional and computationally very complex and, as a result, sampling the posterior of spherical inverse problems is a challenging task. In this work, we describe a framework that leverages a proximal Markov chain Monte Carlo (MCMC) algorithm to efficiently sample the high-dimensional space of spherical inverse problems with a sparsity-promoting wavelet prior. We detail the modifications needed for the algorithm to be applied to spherical problems, and give special consideration to the crucial forward modelling step which contains spherical harmonic transforms that are computationally expensive. By sampling the posterior, our framework allows for full and flexible uncertainty quantification, something…
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Taxonomy
TopicsStatistical and numerical algorithms · Medical Imaging Techniques and Applications · Sparse and Compressive Sensing Techniques
