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Unlocking Large Scale Uncertainty Quantification with In Transit Iterative Statistics
Alejandro Ribés, Théophile Terraz, Yvan Fournier, Bertrand Iooss, Bruno Raffin

Unlocking Large Scale Uncertainty Quantification with In Transit Iterative Statistics

Science & Mathematics Published 2022 Verification Pending

Overview & Synopsis

Multi-run numerical simulations using supercomputers are increasingly used by physicists and engineers for dealing with input data and model uncertainties. Most of the time, the input parameters of a simulation are modeled as random variables, then simulations are run a (possibly large) number of times with input parameters varied according to a specific design of experiments. Uncertainty quantification for numerical simulations is a hard computational problem, currently bounded by the large size of the produced results. This book chapter is about using in situ techniques to enable large scale uncertainty quantification studies. We provide a comprehensive description of Melissa, a file avoiding, adaptive, fault-tolerant, and elastic framework that computes in transit statistical quantities of interest. Melissa currently implements the on-the-fly computation of the statistics necessary for the realization of large scale uncertainty quantification studies: moment-based statistics (mean, standard deviation, higher orders), quantiles, Sobol' indices, and threshold exceedance.

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Document Information

Document Title Unlocking Large Scale Uncertainty Quantification with In Transit Iterative Statistics
Author / Organization Alejandro Ribés, Théophile Terraz, Yvan Fournier, Bertrand Iooss, Bruno Raffin
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2022
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-205736
Original Source Link Visit Source Page on hal.science »