JOURNAL OF COMPUTATIONAL PHYSICS | 卷:341 |
Combining multiple surrogate models to accelerate failure probability estimation with expensive high-fidelity models | |
Article | |
Peherstorfer, Benjamin1  Kramer, Boris1  Willcox, Karen1  | |
[1] MIT, Dept Aeronaut & Astronaut, 77 Massachusetts Ave, Cambridge, MA 02139 USA | |
关键词: Multifidelity; Model reduction; Uncertainty quantification; Failure probability estimation; Surrogate modeling; Rare event simulation; | |
DOI : 10.1016/j.jcp.2017.04.012 | |
来源: Elsevier | |
【 摘 要 】
In failure probability estimation, importance sampling constructs a biasing distribution that targets the failure event such that a small number of model evaluations is sufficient to achieve a Monte Carlo estimate of the failure probability with an acceptable accuracy; however, the construction of the biasing distribution often requires a large number of model evaluations, which can become computationally expensive. We present a mixed multifidelity importance sampling (MMFIS) approach that leverages computationally cheap but erroneous surrogate models for the construction of the biasing distribution and that uses the original high-fidelity model to guarantee unbiased estimates of the failure probability. The key property of our MMFIS estimator is that it can leverage multiple surrogate models for the construction of the biasing distribution, instead of a single surrogate model alone. We show that our MMFIS estimator has a mean-squared error that is up to a constant lower than the mean-squared errors of the corresponding estimators that uses any of the given surrogate models alone even in settings where no information about the approximation qualities of the surrogate models is available. In particular, our MMFIS approach avoids the problem of selecting the surrogate model that leads to the estimator with the lowest mean-squared error, which is challenging if the approximation quality of the surrogate models is unknown. We demonstrate our MMFIS approach on numerical examples, where we achieve orders of magnitude speedups compared to using the high-fidelity model only. (C) 2017 Elsevier Inc. All rights reserved.
【 授权许可】
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