fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models

Mass loss due to dynamic changes in ice sheets is a significant contributor to sea level rise, and this contribution is expected to increase in the future. Numerical codes simulating the evolution of ice sheets can potentially quantify this future contribution. However, the uncertainty inherent in t...

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Main Authors: Koziol, Conrad P., Todd, Joe A., Goldberg, Daniel N., Maddison, James R.
Format: Text
Language:English
Published: 2021
Subjects:
Online Access:https://doi.org/10.5194/gmd-2021-90
https://gmd.copernicus.org/preprints/gmd-2021-90/
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spelling ftcopernicus:oai:publications.copernicus.org:gmdd93665 2023-05-15T16:40:20+02:00 fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models Koziol, Conrad P. Todd, Joe A. Goldberg, Daniel N. Maddison, James R. 2021-03-29 application/pdf https://doi.org/10.5194/gmd-2021-90 https://gmd.copernicus.org/preprints/gmd-2021-90/ eng eng doi:10.5194/gmd-2021-90 https://gmd.copernicus.org/preprints/gmd-2021-90/ eISSN: 1991-9603 Text 2021 ftcopernicus https://doi.org/10.5194/gmd-2021-90 2021-04-05T16:22:16Z Mass loss due to dynamic changes in ice sheets is a significant contributor to sea level rise, and this contribution is expected to increase in the future. Numerical codes simulating the evolution of ice sheets can potentially quantify this future contribution. However, the uncertainty inherent in these models propagates into projections of sea level rise, and hence is crucial to understand. Key variables of ice sheet models, such as basal drag or ice stiffness, are typically initialized using inversion methodologies to ensure that models match present observations. Such inversions often involve tens or hundreds of thousands of parameters, with unknown uncertainties and dependencies. The computationally intensive nature of inversions along with their high number of parameters mean traditional methods such as Monte Carlo are expensive for uncertainty quantification. Here we develop a framework to estimate the posterior uncertainty of inversions, and project them onto sea level change projections over the decadal timescale. The framework treats parametric uncertainty as multivariate Gaussian, and exploits the equivalence between the Hessian of the model and the inverse covariance of the parameter set. The former is computed efficiently via algorithmic differentiation, and the posterior covariance is propagated in time using a time-dependent model adjoint to produce projection error bars. This work represents an important step in quantifying the internal uncertainty of projections of ice-sheet models. Text Ice Sheet Copernicus Publications: E-Journals
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Mass loss due to dynamic changes in ice sheets is a significant contributor to sea level rise, and this contribution is expected to increase in the future. Numerical codes simulating the evolution of ice sheets can potentially quantify this future contribution. However, the uncertainty inherent in these models propagates into projections of sea level rise, and hence is crucial to understand. Key variables of ice sheet models, such as basal drag or ice stiffness, are typically initialized using inversion methodologies to ensure that models match present observations. Such inversions often involve tens or hundreds of thousands of parameters, with unknown uncertainties and dependencies. The computationally intensive nature of inversions along with their high number of parameters mean traditional methods such as Monte Carlo are expensive for uncertainty quantification. Here we develop a framework to estimate the posterior uncertainty of inversions, and project them onto sea level change projections over the decadal timescale. The framework treats parametric uncertainty as multivariate Gaussian, and exploits the equivalence between the Hessian of the model and the inverse covariance of the parameter set. The former is computed efficiently via algorithmic differentiation, and the posterior covariance is propagated in time using a time-dependent model adjoint to produce projection error bars. This work represents an important step in quantifying the internal uncertainty of projections of ice-sheet models.
format Text
author Koziol, Conrad P.
Todd, Joe A.
Goldberg, Daniel N.
Maddison, James R.
spellingShingle Koziol, Conrad P.
Todd, Joe A.
Goldberg, Daniel N.
Maddison, James R.
fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
author_facet Koziol, Conrad P.
Todd, Joe A.
Goldberg, Daniel N.
Maddison, James R.
author_sort Koziol, Conrad P.
title fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
title_short fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
title_full fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
title_fullStr fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
title_full_unstemmed fenics_ice 1.0: A framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
title_sort fenics_ice 1.0: a framework for quantifying initialisation uncertainty fortime-dependent ice-sheet models
publishDate 2021
url https://doi.org/10.5194/gmd-2021-90
https://gmd.copernicus.org/preprints/gmd-2021-90/
genre Ice Sheet
genre_facet Ice Sheet
op_source eISSN: 1991-9603
op_relation doi:10.5194/gmd-2021-90
https://gmd.copernicus.org/preprints/gmd-2021-90/
op_doi https://doi.org/10.5194/gmd-2021-90
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