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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ftmit:oai:dspace.mit.edu:1721.1/52347 2023-06-11T04:06:40+02:00 Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean Smith, K. Shafer Marshall, John C Massachusetts Institute of Technology. Department of Earth and Planetary Sciences Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Marshall, John C. 2007-07 application/pdf http://hdl.handle.net/1721.1/52347 en_US eng American Meteorological Society http://dx.doi.org/10.1175/2008JPO3880.1 Journal of Physical Oceanography 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 orcid:0000-0001-9230-3591 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. American Meteorological Society Article http://purl.org/eprint/type/JournalArticle 2007 ftmit https://doi.org/10.1175/2008JPO3880.1 2023-05-29T08:20:25Z 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 ... Article in Journal/Newspaper Antarc* Antarctic Southern Ocean DSpace@MIT (Massachusetts Institute of Technology) Antarctic Southern Ocean The Antarctic Journal of Physical Oceanography 39 1 50 69 |
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Open Polar |
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DSpace@MIT (Massachusetts Institute of Technology) |
op_collection_id |
ftmit |
language |
English |
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. National Science Foundation Geophysical Fluid ... |
author2 |
Massachusetts Institute of Technology. Department of Earth and Planetary Sciences Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Marshall, John C. |
format |
Article in Journal/Newspaper |
author |
Smith, K. Shafer Marshall, John C |
spellingShingle |
Smith, K. Shafer Marshall, John C Evidence for Enhanced Eddy Mixing at Middepth in the Southern Ocean |
author_facet |
Smith, K. Shafer Marshall, John C |
author_sort |
Smith, K. Shafer |
title |
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_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_sort |
evidence for enhanced eddy mixing at middepth in the southern ocean |
publisher |
American Meteorological Society |
publishDate |
2007 |
url |
http://hdl.handle.net/1721.1/52347 |
geographic |
Antarctic Southern Ocean The Antarctic |
geographic_facet |
Antarctic Southern Ocean The Antarctic |
genre |
Antarc* Antarctic Southern Ocean |
genre_facet |
Antarc* Antarctic Southern Ocean |
op_source |
American Meteorological Society |
op_relation |
http://dx.doi.org/10.1175/2008JPO3880.1 Journal of Physical Oceanography 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 orcid:0000-0001-9230-3591 |
op_rights |
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. |
op_doi |
https://doi.org/10.1175/2008JPO3880.1 |
container_title |
Journal of Physical Oceanography |
container_volume |
39 |
container_issue |
1 |
container_start_page |
50 |
op_container_end_page |
69 |
_version_ |
1768378713730187264 |