Global contributions of mesoscale dynamics to meridional heat transport

Mesoscale ocean processes are prevalent in many parts of the global oceans, and may contribute substantially to the meridional movement of heat. Yet earlier global surveys of meridional heat transport (MHT) have not formally distinguished between mesoscale and large-scale contributions, or have defi...

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Main Authors: Delman, Andrew, Lee, Tong
Format: Text
Language:English
Published: 2021
Subjects:
Online Access:https://doi.org/10.5194/os-2021-9
https://os.copernicus.org/preprints/os-2021-9/
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spelling ftcopernicus:oai:publications.copernicus.org:osd92462 2023-05-15T17:31:30+02:00 Global contributions of mesoscale dynamics to meridional heat transport Delman, Andrew Lee, Tong 2021-02-03 application/pdf https://doi.org/10.5194/os-2021-9 https://os.copernicus.org/preprints/os-2021-9/ eng eng doi:10.5194/os-2021-9 https://os.copernicus.org/preprints/os-2021-9/ eISSN: 1812-0792 Text 2021 ftcopernicus https://doi.org/10.5194/os-2021-9 2021-02-08T17:22:14Z Mesoscale ocean processes are prevalent in many parts of the global oceans, and may contribute substantially to the meridional movement of heat. Yet earlier global surveys of meridional heat transport (MHT) have not formally distinguished between mesoscale and large-scale contributions, or have defined eddy contributions based on temporal rather than spatial characteristics. This work uses spatial filtering methods to separate large-scale (gyre and planetary wave) contributions from mesoscale (eddy, recirculation, and tropical instability wave) contributions to MHT by extending beyond a previous effort for the North Atlantic Ocean. Overall, mesoscale temperature fluxes produce a net poleward MHT at mid-latitudes and equatorward MHT in the tropics, thereby resulting in a net divergence of heat from the subtropics. Mesoscale temperature fluxes are often concentrated near the energetic currents at western boundaries, and the temperature difference between the boundary current and its recirculation determines the direction of the mesoscale temperature flux. The mesoscale contribution to MHT yields substantially different results from temporally-based <q>eddy</q> contributions to MHT, with the latter contributed substantially by gyre and planetary wave motions at low latitudes. Mesoscale temperature fluxes contribute the most to interannual and decadal variability of MHT in the Southern Ocean, the tropical Indo-Pacific, and the North Atlantic. Surface eddy kinetic energy (EKE) is not a good proxy for mesoscale temperature flux variability in regions with the highest time-mean EKE, though it does explain much of the temperature flux variability in regions of modest time-mean EKE. This approach to quantifying mesoscale fluxes can be used to improve parameterizations of mesoscale effects in coarse-resolution models, and assess regional impacts of mesoscale eddies and recirculations on tracer fluxes. Text North Atlantic Southern Ocean Copernicus Publications: E-Journals Pacific Southern Ocean
institution Open Polar
collection Copernicus Publications: E-Journals
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language English
description Mesoscale ocean processes are prevalent in many parts of the global oceans, and may contribute substantially to the meridional movement of heat. Yet earlier global surveys of meridional heat transport (MHT) have not formally distinguished between mesoscale and large-scale contributions, or have defined eddy contributions based on temporal rather than spatial characteristics. This work uses spatial filtering methods to separate large-scale (gyre and planetary wave) contributions from mesoscale (eddy, recirculation, and tropical instability wave) contributions to MHT by extending beyond a previous effort for the North Atlantic Ocean. Overall, mesoscale temperature fluxes produce a net poleward MHT at mid-latitudes and equatorward MHT in the tropics, thereby resulting in a net divergence of heat from the subtropics. Mesoscale temperature fluxes are often concentrated near the energetic currents at western boundaries, and the temperature difference between the boundary current and its recirculation determines the direction of the mesoscale temperature flux. The mesoscale contribution to MHT yields substantially different results from temporally-based <q>eddy</q> contributions to MHT, with the latter contributed substantially by gyre and planetary wave motions at low latitudes. Mesoscale temperature fluxes contribute the most to interannual and decadal variability of MHT in the Southern Ocean, the tropical Indo-Pacific, and the North Atlantic. Surface eddy kinetic energy (EKE) is not a good proxy for mesoscale temperature flux variability in regions with the highest time-mean EKE, though it does explain much of the temperature flux variability in regions of modest time-mean EKE. This approach to quantifying mesoscale fluxes can be used to improve parameterizations of mesoscale effects in coarse-resolution models, and assess regional impacts of mesoscale eddies and recirculations on tracer fluxes.
format Text
author Delman, Andrew
Lee, Tong
spellingShingle Delman, Andrew
Lee, Tong
Global contributions of mesoscale dynamics to meridional heat transport
author_facet Delman, Andrew
Lee, Tong
author_sort Delman, Andrew
title Global contributions of mesoscale dynamics to meridional heat transport
title_short Global contributions of mesoscale dynamics to meridional heat transport
title_full Global contributions of mesoscale dynamics to meridional heat transport
title_fullStr Global contributions of mesoscale dynamics to meridional heat transport
title_full_unstemmed Global contributions of mesoscale dynamics to meridional heat transport
title_sort global contributions of mesoscale dynamics to meridional heat transport
publishDate 2021
url https://doi.org/10.5194/os-2021-9
https://os.copernicus.org/preprints/os-2021-9/
geographic Pacific
Southern Ocean
geographic_facet Pacific
Southern Ocean
genre North Atlantic
Southern Ocean
genre_facet North Atlantic
Southern Ocean
op_source eISSN: 1812-0792
op_relation doi:10.5194/os-2021-9
https://os.copernicus.org/preprints/os-2021-9/
op_doi https://doi.org/10.5194/os-2021-9
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