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Thermobaric control of gravitational potential energy generation by diapycnal mixing in the deep ocean

Thermobaric control of gravitational potential energy generation by diapycnal mixing in the deep ocean
Thermobaric control of gravitational potential energy generation by diapycnal mixing in the deep ocean
Sources and sinks of gravitational potential energy (GPE) play a rate-limiting role in the large-scale ocean circulation. A key source is turbulent diapycnal mixing, whereby irreversible mixing across isoneutral surfaces is enhanced by turbulent straining of these surfaces. This has motivated international observational efforts to map diapycnal mixing in the global ocean. However, in order to accurately relate the GPE supplied to the large-scale circulation by diapycnal mixing to the mixing energy source, it is first necessary to determine the ratio, ?, of the GPE generation rate to the available potential energy dissipation rate associated with turbulent mixing. Here the link between GPE and hydrostatic pressure is used to derive the GPE budget for a compressible ocean with a nonlinear equation of state. The role of diapycnal mixing is isolated and from this a global climatological distribution of ? is calculated. It is shown that, for a given source of mixing energy, typically three times as much GPE is generated if the mixing takes place in bottom waters rather than in the pycnocline. This is due to GPE destruction by cabbelling in the pycnocline, as opposed to thermobaric enhancement of GPE generation by diapycnal mixing in the deep ocean.
diapycnal mixing, equation of state, thermodynamics, meridional overturning, circulation
0094-8276
327-331
Oliver, Kevin I.C.
588b11c6-4d0c-4c59-94e2-255688474987
Tailleux, Remi
aa2f0d61-931e-4587-9575-fb30e5ac384c
Oliver, Kevin I.C.
588b11c6-4d0c-4c59-94e2-255688474987
Tailleux, Remi
aa2f0d61-931e-4587-9575-fb30e5ac384c

Oliver, Kevin I.C. and Tailleux, Remi (2013) Thermobaric control of gravitational potential energy generation by diapycnal mixing in the deep ocean. Geophysical Research Letters, 40 (2), 327-331. (doi:10.1029/2012GL054235).

Record type: Article

Abstract

Sources and sinks of gravitational potential energy (GPE) play a rate-limiting role in the large-scale ocean circulation. A key source is turbulent diapycnal mixing, whereby irreversible mixing across isoneutral surfaces is enhanced by turbulent straining of these surfaces. This has motivated international observational efforts to map diapycnal mixing in the global ocean. However, in order to accurately relate the GPE supplied to the large-scale circulation by diapycnal mixing to the mixing energy source, it is first necessary to determine the ratio, ?, of the GPE generation rate to the available potential energy dissipation rate associated with turbulent mixing. Here the link between GPE and hydrostatic pressure is used to derive the GPE budget for a compressible ocean with a nonlinear equation of state. The role of diapycnal mixing is isolated and from this a global climatological distribution of ? is calculated. It is shown that, for a given source of mixing energy, typically three times as much GPE is generated if the mixing takes place in bottom waters rather than in the pycnocline. This is due to GPE destruction by cabbelling in the pycnocline, as opposed to thermobaric enhancement of GPE generation by diapycnal mixing in the deep ocean.

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More information

e-pub ahead of print date: 25 January 2013
Published date: 28 January 2013
Keywords: diapycnal mixing, equation of state, thermodynamics, meridional overturning, circulation
Organisations: Physical Oceanography

Identifiers

Local EPrints ID: 347746
URI: http://eprints.soton.ac.uk/id/eprint/347746
ISSN: 0094-8276
PURE UUID: 3a8e0464-baa4-40da-805c-afddb7c2fe18

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Date deposited: 29 Jan 2013 14:19
Last modified: 14 Mar 2024 12:51

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Author: Remi Tailleux

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