Causal Mechanisms of Subpolar Gyre Variability in CMIP6 Models
Swinda K.J. Falkena, Henk A. Dijkstra, Anna S. von der Heydt

TL;DR
This study uses causal inference to analyze how various mechanisms influence subpolar gyre variability in CMIP6 climate models, revealing complex and sometimes ambiguous feedbacks relevant to climate tipping points.
Contribution
It provides a detailed causal analysis of subpolar gyre mechanisms in CMIP6 models, highlighting the variability and significance of different feedback loops under climate change.
Findings
Increase in salinity or decrease in temperature deepens mixed layer in most models.
Deepening mixed layer often cools intermediate depths, but effects vary.
Models with expected feedback signs also show abrupt shifts in climate scenarios.
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 re-stratification is less clear. 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…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsMagnetic confinement fusion research · Ionosphere and magnetosphere dynamics
