Controls on the Strength and Structure of the Atlantic Meridional Overturning Circulation in Climate Models
Abstract
State-of-the-art climate models simulate a large spread in the mean-state Atlantic meridional overturning circulation (AMOC), with strengths varying between 12 and 25 Sv. Here, we introduce a framework for understanding this spread by assessing the balance between the thermal-wind expression and surface water mass transformation in the North Atlantic. The intermodel spread in the mean-state AMOC strength is shown to be related to the overturning scale depth: climate models with a larger scale depth tend to have a stronger AMOC. We present a physically motivated scaling relationship that links intermodel variations in the scale depth to surface buoyancy fluxes and stratification in the North Atlantic, and thus connects North Atlantic surface processes to the interior overturning circulation. Climate models with a larger scale depth tend to have stronger surface buoyancy loss and weaker stratification in the North Atlantic. These results offer a framework for reducing mean-state AMOC biases in climate models.
Copyright and License
© 2024. The Author(s). This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
Acknowledgement
M.S.N is grateful for Caltech's Summer Undergraduate Research Fellowship (SURF) program and the Department of Physics at The Ohio State University for support of this research. D.B.B was supported by the National Science Foundation (NSF) Graduate Research Fellowship Program (NSF Grant DGE1745301). E.R.N was supported by NSF Grant OCE-2048576 and M2LInES research funding by the generosity of Eric and Wendy Schmidt by recommendation of the Schmidt Futures program. A.F.T was supported by NSF Grant OCE-2023259.
Data Availability
The authors thank the climate modeling groups for producing and making available their model output, which is accessible at the Earth System Grid Federation (ESGF) Portal (https://esgf-node.llnl.gov/search/cmip6/). A list of the CMIP6 models used in this study is provided in Figure 1 and described in Section 2.1.
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Additional details
- ISSN
- 1944-8007
- California Institute of Technology
- Summer Undergraduate Research Fellowship
- The Ohio State University
- National Science Foundation
- NSF Graduate Research Fellowship DGE-1745301
- National Science Foundation
- OCE‐2048576
- Schmidt Family Foundation
- National Science Foundation
- OCE‐2023259
- Caltech groups
- Division of Geological and Planetary Sciences