Oceanic control of multidecadal variability in an idealized coupled GCM
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Author(s) • • • •
Jamet, Quentin
Huck, Thierry
Arzel, Olivier
Campin, Jean-Michel
de Verdière, Alain Colin
Date Issued
July 2015
Journal
Climate Dynamics
Publisher
Springer Berlin Heidelberg
Citation
Jamet, QuJamet, Quentin et al. “Oceanic Control of Multidecadal Variability in an Idealized Coupled GCM.” Climate Dynamics 46.9–10 (2016): 3079–3095.
Version
Author's final manuscript
Abstract
Idealized ocean models are known to develop intrinsic multidecadal oscillations of the meridional overturning circulation (MOC). Here we explore the role of ocean–atmosphere interactions on this low-frequency variability. We use a coupled ocean–atmosphere model set up in a flat-bottom aquaplanet geometry with two meridional boundaries. The model is run at three different horizontal resolutions (4°, 2° and 1°) in both the ocean and atmosphere. At all resolutions, the MOC exhibits spontaneous variability on multidecadal timescales in the range 30–40 years, associated with the propagation of large-scale baroclinic Rossby waves across the Atlantic-like basin. The unstable region of growth of these waves through the long wave limit of baroclinic instability shifts from the eastern boundary at coarse resolution to the western boundary at higher resolution. Increasing the horizontal resolution enhances both intrinsic atmospheric variability and ocean–atmosphere interactions. In particular, the simulated atmospheric annular mode becomes significantly correlated to the MOC variability at 1° resolution. An ocean-only simulation conducted for this specific case underscores the disruptive but not essential influence of air–sea interactions on the low-frequency variability. This study demonstrates that an atmospheric annular mode leading MOC changes by about 2 years (as found at 1° resolution) does not imply that the low-frequency variability originates from air–sea interactions.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
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DOI of Published Version
https://doi.org/10.1007/s00382-015-2754-3