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Planetary-geometric constraints on isopycnal slope in the Southern Ocean

Citation

Jones, DC and Ito, T and Birner, T and Klocker, A and Munday, D, Planetary-geometric constraints on isopycnal slope in the Southern Ocean, Journal of Physical Oceanography, 45, (12) pp. 2991-3004. ISSN 0022-3670 (2015) [Refereed Article]


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Copyright Statement

Copyright 2015 American Meteorological Society

DOI: doi:10.1175/JPO-D-15-0034.1

Abstract

On planetary scales, surface wind stress and differential buoyancy forcing act together to produce isopycnal surfaces that are relatively flat in the tropics/subtropics and steep near the poles, where they tend to outcrop. Tilted isopycnals in a rapidly rotating fluid are subject to baroclinic instability. The turbulent, mesoscale eddies generated by this instability have a tendency to homogenize potential vorticity (PV) along density surfaces. In the Southern Ocean (SO), the tilt of isopycnals is largely maintained by competition between the steepening effect of surface forcing and the flattening effect of turbulent, spatially inhomogeneous eddy fluxes of PV. Here quasigeostrophic theory is used to investigate the influence of a planetary–geometric constraint on the equilibrium slope of tilted density/buoyancy surfaces in the SO. If the meridional gradients of relative vorticity and PV are small relative to β, then quasigeostrophic theory predicts ds/dz = β/f0 = cot(ϕ0)/a, or equivalently r ≡ |∂zs/(β/f0)| = 1, where f is the Coriolis parameter, β is the meridional gradient of f, s is the isopycnal slope, ϕ0 is a reference latitude, a is the planetary radius, and r is the depth-averaged criticality parameter. It is found that the strict r = 1 condition holds over specific averaging volumes in a large-scale climatology. A weaker r = O(1) condition for depth-averaged quantities is generally satisfied away from large bathymetric features. The r = O(1) constraint is employed to derive a depth scale to characterize large-scale interior stratification, and an idealized sector model is used to test the sensitivity of this relationship to surface wind forcing. Finally, the possible implications for eddy flux parameterization and for the sensitivity of SO circulation/stratification to changes in forcing are discussed.

Item Details

Item Type:Refereed Article
Keywords:Southern Ocean, mesoscale eddies, planetary-geostrophic constraint
Research Division:Earth Sciences
Research Group:Oceanography
Research Field:Physical Oceanography
Objective Division:Environment
Objective Group:Climate and Climate Change
Objective Field:Climate and Climate Change not elsewhere classified
Author:Klocker, A (Dr Andreas Klocker)
ID Code:104988
Year Published:2015
Web of Science® Times Cited:1
Deposited By:IMAS Research and Education Centre
Deposited On:2015-12-02
Last Modified:2017-10-31
Downloads:0

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