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https://doi.org/10.48550/arXiv.2408.16541
https://doi.org/10.48550/arXiv.2408.16541
10 Apr 2025
 | 10 Apr 2025

Causal Mechanisms of Subpolar Gyre Variability in CMIP6 Models

Swinda K. J. Falkena, Henk A. Dijkstra, and Anna S. von der Heydt

Abstract. The subpolar gyre is at risk of crossing a tipping point under future climate change associated with the collapse of deep convection. As such tipping can have significant climate impacts, it is important to understand the mechanisms at play and how they are represented in modern climate models. In this study we use causal inference to investigate the representation of several proposed mechanisms of subpolar gyre variability in CMIP6 models. As expected, an increase in sea surface salinity or a decrease in sea surface temperature leads to an increase in mixed layer depth in nearly all CMIP6 models due to an intensification of deep convection. However, the effect of convection to modify sea surface temperature due to restratification is less well captured. In most models the deepening of the mixed layer caused by an increase of sea surface salinity, does result in a cooling of the water at intermediate depths. The feedback from the subsurface temperature through density to the strength of the subpolar gyre circulation is more ambiguous, with fewer models indicating a significant link. Those that do show a significant link, do not agree on its sign. One model (CESM2) contains all proposed mechanisms, with both a negative and delayed positive feedback loop.

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Journal article(s) based on this preprint

21 Oct 2025
Causal mechanisms of subpolar gyre variability in CMIP6 models
Swinda K. J. Falkena, Henk A. Dijkstra, and Anna S. von der Heydt
Earth Syst. Dynam., 16, 1833–1844, https://doi.org/10.5194/esd-16-1833-2025,https://doi.org/10.5194/esd-16-1833-2025, 2025
Short summary
Swinda K. J. Falkena, Henk A. Dijkstra, and Anna S. von der Heydt

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-1570', Anonymous Referee #1, 10 Jun 2025
  • RC2: 'Comment on egusphere-2025-1570', Anonymous Referee #2, 15 Jun 2025

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-1570', Anonymous Referee #1, 10 Jun 2025
  • RC2: 'Comment on egusphere-2025-1570', Anonymous Referee #2, 15 Jun 2025

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Reconsider after major revisions (22 Jul 2025) by Richard Betts
AR by Swinda Falkena on behalf of the Authors (23 Jul 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (03 Aug 2025) by Richard Betts
RR by Anonymous Referee #1 (12 Aug 2025)
RR by Anonymous Referee #2 (17 Aug 2025)
ED: Publish as is (25 Aug 2025) by Richard Betts
AR by Swinda Falkena on behalf of the Authors (25 Aug 2025)  Manuscript 

Journal article(s) based on this preprint

21 Oct 2025
Causal mechanisms of subpolar gyre variability in CMIP6 models
Swinda K. J. Falkena, Henk A. Dijkstra, and Anna S. von der Heydt
Earth Syst. Dynam., 16, 1833–1844, https://doi.org/10.5194/esd-16-1833-2025,https://doi.org/10.5194/esd-16-1833-2025, 2025
Short summary
Swinda K. J. Falkena, Henk A. Dijkstra, and Anna S. von der Heydt

Model code and software

SPG_mechanism (v1.0) Swinda K. J. Falkena https://doi.org/10.5281/zenodo.1344975

Swinda K. J. Falkena, Henk A. Dijkstra, and Anna S. von der Heydt

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Short summary
The subpolar gyre is a wind-driven circulation in the North Atlantic Ocean, which enables the mixing of water between the surface and deeper layers. We investigate the interactions between the strength of the gyre circulation, salinity, temperature and mixing in climate models. We find that most models capture an increase in salinity or a decrease in temperature leading to mixing. However, the feedback from the density in the gyre centre to the strength of its circulation is poorly represented.
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