CMIP6 simulations with the compact Earth system model OSCAR v3.1

Reduced-complexity models, also called simple climate models or compact models, provide an alternative to Earth system models (ESMs) with lower computational costs, although at the expense of spatial and temporal information. It remains important to evaluate and validate these reduced-complexity mod...

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Main Authors: Quilcaille, Yann, id_orcid:0 000-0002-1474-0144, Gasser, Thomas, Ciais, Philippe, Boucher, Olivier
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus 2023
Subjects:
Online Access:https://hdl.handle.net/20.500.11850/601506
https://doi.org/10.3929/ethz-b-000601506
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spelling ftethz:oai:www.research-collection.ethz.ch:20.500.11850/601506 2024-02-04T10:03:54+01:00 CMIP6 simulations with the compact Earth system model OSCAR v3.1 Quilcaille, Yann id_orcid:0 000-0002-1474-0144 Gasser, Thomas Ciais, Philippe Boucher, Olivier 2023-02-16 application/application/pdf https://hdl.handle.net/20.500.11850/601506 https://doi.org/10.3929/ethz-b-000601506 en eng Copernicus info:eu-repo/semantics/altIdentifier/doi/10.5194/gmd-16-1129-2023 info:eu-repo/semantics/altIdentifier/wos/000938006500001 info:eu-repo/grantAgreement/EC/H2020/820829 http://hdl.handle.net/20.500.11850/601506 doi:10.3929/ethz-b-000601506 info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International Geoscientific Model Development, 16 (3) info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2023 ftethz https://doi.org/20.500.11850/60150610.3929/ethz-b-00060150610.5194/gmd-16-1129-2023 2024-01-08T00:51:49Z Reduced-complexity models, also called simple climate models or compact models, provide an alternative to Earth system models (ESMs) with lower computational costs, although at the expense of spatial and temporal information. It remains important to evaluate and validate these reduced-complexity models. Here, we evaluate a recent version (v3.1) of the OSCAR model using observations and results from ESMs from the current Coupled Model Intercomparison Project 6 (CMIP6). The results follow the same post-processing used for the contribution of OSCAR to the Reduced Complexity Model Intercomparison Project (RCMIP) Phase 2 regarding the identification of stable configurations and the use of observational constraints. These constraints succeed in decreasing the overestimation of global surface air temperature over 2000-2019 with reference to 1961-1900 from 0.60±0.11 to 0.55±0.04gK (the constraint being 0.54±0.05gK). The equilibrium climate sensitivity (ECS) of the unconstrained OSCAR is 3.17±0.63gK, while CMIP5 and CMIP6 models have ECSs of 3.2±0.7 and 3.7±1.1gK, respectively. Applying observational constraints to OSCAR reduces the ECS to 2.78±0.47gK. Overall, the model qualitatively reproduces the responses of complex ESMs, although some differences remain due to the impact of observational constraints on the weighting of parametrizations. Specific features of OSCAR also contribute to these differences, such as its fully interactive atmospheric chemistry and endogenous calculations of biomass burning, wetlands CH4 and permafrost CH4 and CO2 emissions. Identified main points of needed improvements of the OSCAR model include a low sensitivity of the land carbon cycle to climate change, an instability of the ocean carbon cycle, the climate module that is seemingly too simple, and the climate feedback involving short-lived species that is too strong. Beyond providing a key diagnosis of the OSCAR model in the context of the reduced-complexity models, this work is also meant to help with the upcoming calibration of OSCAR on ... Article in Journal/Newspaper permafrost ETH Zürich Research Collection
institution Open Polar
collection ETH Zürich Research Collection
op_collection_id ftethz
language English
description Reduced-complexity models, also called simple climate models or compact models, provide an alternative to Earth system models (ESMs) with lower computational costs, although at the expense of spatial and temporal information. It remains important to evaluate and validate these reduced-complexity models. Here, we evaluate a recent version (v3.1) of the OSCAR model using observations and results from ESMs from the current Coupled Model Intercomparison Project 6 (CMIP6). The results follow the same post-processing used for the contribution of OSCAR to the Reduced Complexity Model Intercomparison Project (RCMIP) Phase 2 regarding the identification of stable configurations and the use of observational constraints. These constraints succeed in decreasing the overestimation of global surface air temperature over 2000-2019 with reference to 1961-1900 from 0.60±0.11 to 0.55±0.04gK (the constraint being 0.54±0.05gK). The equilibrium climate sensitivity (ECS) of the unconstrained OSCAR is 3.17±0.63gK, while CMIP5 and CMIP6 models have ECSs of 3.2±0.7 and 3.7±1.1gK, respectively. Applying observational constraints to OSCAR reduces the ECS to 2.78±0.47gK. Overall, the model qualitatively reproduces the responses of complex ESMs, although some differences remain due to the impact of observational constraints on the weighting of parametrizations. Specific features of OSCAR also contribute to these differences, such as its fully interactive atmospheric chemistry and endogenous calculations of biomass burning, wetlands CH4 and permafrost CH4 and CO2 emissions. Identified main points of needed improvements of the OSCAR model include a low sensitivity of the land carbon cycle to climate change, an instability of the ocean carbon cycle, the climate module that is seemingly too simple, and the climate feedback involving short-lived species that is too strong. Beyond providing a key diagnosis of the OSCAR model in the context of the reduced-complexity models, this work is also meant to help with the upcoming calibration of OSCAR on ...
format Article in Journal/Newspaper
author Quilcaille, Yann
id_orcid:0 000-0002-1474-0144
Gasser, Thomas
Ciais, Philippe
Boucher, Olivier
spellingShingle Quilcaille, Yann
id_orcid:0 000-0002-1474-0144
Gasser, Thomas
Ciais, Philippe
Boucher, Olivier
CMIP6 simulations with the compact Earth system model OSCAR v3.1
author_facet Quilcaille, Yann
id_orcid:0 000-0002-1474-0144
Gasser, Thomas
Ciais, Philippe
Boucher, Olivier
author_sort Quilcaille, Yann
title CMIP6 simulations with the compact Earth system model OSCAR v3.1
title_short CMIP6 simulations with the compact Earth system model OSCAR v3.1
title_full CMIP6 simulations with the compact Earth system model OSCAR v3.1
title_fullStr CMIP6 simulations with the compact Earth system model OSCAR v3.1
title_full_unstemmed CMIP6 simulations with the compact Earth system model OSCAR v3.1
title_sort cmip6 simulations with the compact earth system model oscar v3.1
publisher Copernicus
publishDate 2023
url https://hdl.handle.net/20.500.11850/601506
https://doi.org/10.3929/ethz-b-000601506
genre permafrost
genre_facet permafrost
op_source Geoscientific Model Development, 16 (3)
op_relation info:eu-repo/semantics/altIdentifier/doi/10.5194/gmd-16-1129-2023
info:eu-repo/semantics/altIdentifier/wos/000938006500001
info:eu-repo/grantAgreement/EC/H2020/820829
http://hdl.handle.net/20.500.11850/601506
doi:10.3929/ethz-b-000601506
op_rights info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International
op_doi https://doi.org/20.500.11850/60150610.3929/ethz-b-00060150610.5194/gmd-16-1129-2023
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