Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean

Satellite altimetric observations of the ocean reveal surface pressure patterns in the core of the Antarctic Circumpolar Current (ACC) that propagate downstream (eastward) but slower than the mean surface current by about 25%. The authors argue that these observations are suggestive of baroclinicall...

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Main Authors: Smith, K. Shafer, Marshall, John C
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: American Meteorological Society 2010
Online Access:http://hdl.handle.net/1721.1/52347
https://orcid.org/0000-0001-9230-3591
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author Smith, K. Shafer
Marshall, John C
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Smith, K. Shafer
Marshall, John C
author_sort Smith, K. Shafer
collection MIT
description Satellite altimetric observations of the ocean reveal surface pressure patterns in the core of the Antarctic Circumpolar Current (ACC) that propagate downstream (eastward) but slower than the mean surface current by about 25%. The authors argue that these observations are suggestive of baroclinically unstable waves that have a steering level at a depth of about 1 km. Detailed linear stability calculations using a hydrographic atlas indeed reveal a steering level in the ACC near the depth implied by the altimetric observations. Calculations using a nonlinear model forced by the mean shear and stratification observed close to the core of the ACC, coinciding with a position where mooring data and direct eddy flux measurements are available, reveal a similar picture, albeit with added details. When eddy fluxes are allowed to adjust the mean state, computed eddy kinetic energy and eddy stress are close to observed magnitudes with steering levels between 1 and 1.5 km, broadly consistent with observations. An important result of this study is that the vertical structure of the potential vorticity (PV) eddy diffusivity is strongly depth dependent, implying that the diffusivity for PV and buoyancy are very different from one another. It is shown that the flow can simultaneously support a PV diffusivity peaking at 5000 m[superscript 2] s[superscript −1] or so near the middepth steering level and a buoyancy diffusivity that is much smaller, of order 1000 m[superscript 2] s[superscript −1], exhibiting less vertical structure. An effective diffusivity calculation, using an advected and diffused tracer transformed into area coordinates, confirms that the PV diffusivity more closely reflects the mixing properties of the flow than does the buoyancy diffusivity, and points explicitly to the need for separating tracer and buoyancy flux parameterizations in coarse-resolution general circulation models. Finally, implications for the eddy-driven circulation of the ACC are discussed.
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spelling mit-1721.1/523472024-05-28T21:15:47Z Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean Smith, K. Shafer Marshall, John C Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Marshall, John C. Marshall, John C. Satellite altimetric observations of the ocean reveal surface pressure patterns in the core of the Antarctic Circumpolar Current (ACC) that propagate downstream (eastward) but slower than the mean surface current by about 25%. The authors argue that these observations are suggestive of baroclinically unstable waves that have a steering level at a depth of about 1 km. Detailed linear stability calculations using a hydrographic atlas indeed reveal a steering level in the ACC near the depth implied by the altimetric observations. Calculations using a nonlinear model forced by the mean shear and stratification observed close to the core of the ACC, coinciding with a position where mooring data and direct eddy flux measurements are available, reveal a similar picture, albeit with added details. When eddy fluxes are allowed to adjust the mean state, computed eddy kinetic energy and eddy stress are close to observed magnitudes with steering levels between 1 and 1.5 km, broadly consistent with observations. An important result of this study is that the vertical structure of the potential vorticity (PV) eddy diffusivity is strongly depth dependent, implying that the diffusivity for PV and buoyancy are very different from one another. It is shown that the flow can simultaneously support a PV diffusivity peaking at 5000 m[superscript 2] s[superscript −1] or so near the middepth steering level and a buoyancy diffusivity that is much smaller, of order 1000 m[superscript 2] s[superscript −1], exhibiting less vertical structure. An effective diffusivity calculation, using an advected and diffused tracer transformed into area coordinates, confirms that the PV diffusivity more closely reflects the mixing properties of the flow than does the buoyancy diffusivity, and points explicitly to the need for separating tracer and buoyancy flux parameterizations in coarse-resolution general circulation models. Finally, implications for the eddy-driven circulation of the ACC are discussed. National Science Foundation Geophysical Fluid Dynamics Program 2010-03-05T17:06:43Z 2010-03-05T17:06:43Z 2008-06 2007-07 Article http://purl.org/eprint/type/JournalArticle 1520-0485 http://hdl.handle.net/1721.1/52347 Smith, K. Shafer, and John Marshall. “Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean.” Journal of Physical Oceanography (2009): 50-69. © 2010 American Meteorological Society https://orcid.org/0000-0001-9230-3591 en_US http://dx.doi.org/10.1175/2008JPO3880.1 Journal of Physical Oceanography Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Meteorological Society American Meteorological Society
spellingShingle Smith, K. Shafer
Marshall, John C
Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean
title Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean
title_full Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean
title_fullStr Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean
title_full_unstemmed Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean
title_short Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean
title_sort evidence for enhanced eddy mixing at middepth in the southern ocean
url http://hdl.handle.net/1721.1/52347
https://orcid.org/0000-0001-9230-3591
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