The dynamics of equatorially asymmetric thermohaline circulations

The three-dimensional dynamics of equatorially asymmetric thermohaline flow are investigated using an ocean general circulation model in a highly idealized configuration with no wind forcing and nearly fixed surface density. Small asymmetries in surface density lead to strongly asymmetric meridional...

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Main Authors: Marotzke, J., Klinger, B.A.
Format: Article in Journal/Newspaper
Language:unknown
Published: 2000
Subjects:
Online Access:https://eprints.soton.ac.uk/8757/
http://ams.allenpress.com/amsonline/?request=get-abstract&issn=1520-0485&volume=030&issue=05&page=0955
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spelling ftsouthampton:oai:eprints.soton.ac.uk:8757 2023-07-30T04:05:06+02:00 The dynamics of equatorially asymmetric thermohaline circulations Marotzke, J. Klinger, B.A. 2000 https://eprints.soton.ac.uk/8757/ http://ams.allenpress.com/amsonline/?request=get-abstract&issn=1520-0485&volume=030&issue=05&page=0955 unknown Marotzke, J. and Klinger, B.A. (2000) The dynamics of equatorially asymmetric thermohaline circulations. Journal of Physical Oceanography, 30 (5), 955-970. (doi:10.1175/1520-0485(2000)030<0955:TDOEAT>2.0.CO;2 <http://dx.doi.org/10.1175/1520-0485(2000)030<0955:TDOEAT>2.0.CO;2>). Article PeerReviewed 2000 ftsouthampton https://doi.org/10.1175/1520-0485(2000)030<0955:TDOEAT>2.0.CO;2 2023-07-09T20:29:31Z The three-dimensional dynamics of equatorially asymmetric thermohaline flow are investigated using an ocean general circulation model in a highly idealized configuration with no wind forcing and nearly fixed surface density. Small asymmetries in surface density lead to strongly asymmetric meridional overturning patterns, with deep water formed in the denser (northern) hemisphere filling the abyss. The poleward deep transport in the lighter hemisphere implies that the deep zonal-mean zonal pressure gradient reverses across the equator. Density along the eastern boundary and the zonally averaged density are nearly symmetric about the equator except at very high latitudes; the Southern Hemisphere western boundary thermocline, in contrast, is balanced by weaker upwelling and is hence broader than its northern counterpart. This pattern is explained through the spinup of the asymmetric circulation from a symmetric one, the timescale of which is set through advection by the mean deep western boundary current. For the strength of the interhemispheric transport, a lower bound of one-half the one-hemisphere overturning strength is derived theoretically for small finite forcing asymmetries, implying that the symmetric circulation is unlikely to be realized. Under asymmetric surface forcing, enhanced mixing in the denser hemisphere suppresses interhemispheric transport. Conversely, very strong cross-equatorial transport is caused by enhanced mixing in the lighter hemisphere. These results indicate that, once the surface densities determine that North Atlantic Deep Water is the dominant ventilating source, its export rate from the North Atlantic is controlled by mixing and upwelling in the rest of the World Ocean. Article in Journal/Newspaper North Atlantic Deep Water North Atlantic University of Southampton: e-Prints Soton
institution Open Polar
collection University of Southampton: e-Prints Soton
op_collection_id ftsouthampton
language unknown
description The three-dimensional dynamics of equatorially asymmetric thermohaline flow are investigated using an ocean general circulation model in a highly idealized configuration with no wind forcing and nearly fixed surface density. Small asymmetries in surface density lead to strongly asymmetric meridional overturning patterns, with deep water formed in the denser (northern) hemisphere filling the abyss. The poleward deep transport in the lighter hemisphere implies that the deep zonal-mean zonal pressure gradient reverses across the equator. Density along the eastern boundary and the zonally averaged density are nearly symmetric about the equator except at very high latitudes; the Southern Hemisphere western boundary thermocline, in contrast, is balanced by weaker upwelling and is hence broader than its northern counterpart. This pattern is explained through the spinup of the asymmetric circulation from a symmetric one, the timescale of which is set through advection by the mean deep western boundary current. For the strength of the interhemispheric transport, a lower bound of one-half the one-hemisphere overturning strength is derived theoretically for small finite forcing asymmetries, implying that the symmetric circulation is unlikely to be realized. Under asymmetric surface forcing, enhanced mixing in the denser hemisphere suppresses interhemispheric transport. Conversely, very strong cross-equatorial transport is caused by enhanced mixing in the lighter hemisphere. These results indicate that, once the surface densities determine that North Atlantic Deep Water is the dominant ventilating source, its export rate from the North Atlantic is controlled by mixing and upwelling in the rest of the World Ocean.
format Article in Journal/Newspaper
author Marotzke, J.
Klinger, B.A.
spellingShingle Marotzke, J.
Klinger, B.A.
The dynamics of equatorially asymmetric thermohaline circulations
author_facet Marotzke, J.
Klinger, B.A.
author_sort Marotzke, J.
title The dynamics of equatorially asymmetric thermohaline circulations
title_short The dynamics of equatorially asymmetric thermohaline circulations
title_full The dynamics of equatorially asymmetric thermohaline circulations
title_fullStr The dynamics of equatorially asymmetric thermohaline circulations
title_full_unstemmed The dynamics of equatorially asymmetric thermohaline circulations
title_sort dynamics of equatorially asymmetric thermohaline circulations
publishDate 2000
url https://eprints.soton.ac.uk/8757/
http://ams.allenpress.com/amsonline/?request=get-abstract&issn=1520-0485&volume=030&issue=05&page=0955
genre North Atlantic Deep Water
North Atlantic
genre_facet North Atlantic Deep Water
North Atlantic
op_relation Marotzke, J. and Klinger, B.A. (2000) The dynamics of equatorially asymmetric thermohaline circulations. Journal of Physical Oceanography, 30 (5), 955-970. (doi:10.1175/1520-0485(2000)030<0955:TDOEAT>2.0.CO;2 <http://dx.doi.org/10.1175/1520-0485(2000)030<0955:TDOEAT>2.0.CO;2>).
op_doi https://doi.org/10.1175/1520-0485(2000)030<0955:TDOEAT>2.0.CO;2
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