the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Identifying climate model structural inconsistencies allows for tight constraint of aerosol radiative forcing
Abstract. Aerosol radiative forcing uncertainty affects estimates of climate sensitivity and limits model skill at making climate projections. Efforts to improve the representations of physical processes in climate models, including extensive comparisons with observations, have not significantly constrained the range of possible aerosol forcing values. A far stronger constraint, in particular for the lower (most-negative) bound, can be achieved using global mean energy-balance arguments based on observed changes in historical temperature. Here, we show that structural deficiencies in a climate model, revealed as inconsistencies among observationally constrained cloud properties in the model, limit the effectiveness of observational constraint of the uncertain physical processes. We sample uncertainty in 37 model parameters related to aerosols, clouds and radiation in a perturbed parameter ensemble of the UK Earth System Model and evaluate 1 million model variants (different parameter settings from Gaussian Process emulators) against satellite-derived observations over several cloudy regions. We show that it is possible to reduce the parametric uncertainty in global mean aerosol forcing by more than 50 %, constraining it to a range in close agreement with energy-balance constraints (around −1.3 to −0.1 W m−2). However, our analysis of a very large set of model variants exposes model internal inconsistencies that would not be apparent in a small set of model simulations. Incorporating observations associated with these inconsistencies weakens the forcing constraint because they require a wider range of parameter values to accommodate conflicting information. Our estimated aerosol forcing range is the maximum feasible constraint using our structurally imperfect model and the chosen observations. Structural model developments targeted at the identified inconsistencies would enable a larger set of observations to be used for constraint, which would then narrow the uncertainty further. Such an approach provides a rigorous pathway to improved model realism and reduced uncertainty that has so far not been achieved through the normal model development approach.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
(1065 KB)
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Supplement
(2073 KB)
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(1065 KB) - Metadata XML
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Supplement
(2073 KB) - BibTeX
- EndNote
- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
- RC1: 'Comment on egusphere-2023-77', Anonymous Referee #1, 13 Mar 2023
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RC2: 'Comment on egusphere-2023-77', Anonymous Referee #2, 29 Mar 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-77/egusphere-2023-77-RC2-supplement.pdf
- AC1: 'Author Comment (AC) on egusphere-2023-77', Leighton A. Regayre, 12 May 2023
Interactive discussion
Status: closed
- RC1: 'Comment on egusphere-2023-77', Anonymous Referee #1, 13 Mar 2023
-
RC2: 'Comment on egusphere-2023-77', Anonymous Referee #2, 29 Mar 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-77/egusphere-2023-77-RC2-supplement.pdf
- AC1: 'Author Comment (AC) on egusphere-2023-77', Leighton A. Regayre, 12 May 2023
Peer review completion
Journal article(s) based on this preprint
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Leighton A. Regayre
Lucia Deaconu
Daniel P. Grosvenor
David M. H. Sexton
Christopher Symonds
Tom Langton
Duncan Watson-Paris
Jane P. Mulcahy
Kirsty J. Pringle
Mark Richardson
Jill S. Johnson
John W. Rostron
Hamish Gordon
Grenville Lister
Philip Stier
Ken S. Carslaw
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(1065 KB) - Metadata XML
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Supplement
(2073 KB) - BibTeX
- EndNote
- Final revised paper