Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean

The aim of this study is to clarify the role of the Southern Ocean storms on interior mixing and meridional overturning circulation. A periodic and idealized numerical model has been designed to represent the key physical processes of a zonal portion of the Southern Ocean located between 70 and 40°...

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Published in:Ocean Science
Main Authors: Jouanno, Julien, Capet, Xavier, Madec, Gurvan, Roullet, Guillaume, Klein, Patrice
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/os-12-743-2016
https://os.copernicus.org/articles/12/743/2016/
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spelling ftcopernicus:oai:publications.copernicus.org:os49362 2023-05-15T18:24:09+02:00 Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean Jouanno, Julien Capet, Xavier Madec, Gurvan Roullet, Guillaume Klein, Patrice 2018-09-15 application/pdf https://doi.org/10.5194/os-12-743-2016 https://os.copernicus.org/articles/12/743/2016/ eng eng doi:10.5194/os-12-743-2016 https://os.copernicus.org/articles/12/743/2016/ eISSN: 1812-0792 Text 2018 ftcopernicus https://doi.org/10.5194/os-12-743-2016 2020-07-20T16:24:08Z The aim of this study is to clarify the role of the Southern Ocean storms on interior mixing and meridional overturning circulation. A periodic and idealized numerical model has been designed to represent the key physical processes of a zonal portion of the Southern Ocean located between 70 and 40° S. It incorporates physical ingredients deemed essential for Southern Ocean functioning: rough topography, seasonally varying air–sea fluxes, and high-latitude storms with analytical form. The forcing strategy ensures that the time mean wind stress is the same between the different simulations, so the effect of the storms on the mean wind stress and resulting impacts on the Southern Ocean dynamics are not considered in this study. Level and distribution of mixing attributable to high-frequency winds are quantified and compared to those generated by eddy–topography interactions and dissipation of the balanced flow. Results suggest that (1) the synoptic atmospheric variability alone can generate the levels of mid-depth dissipation frequently observed in the Southern Ocean (10 −10 –10 −9 W kg −1 ) and (2) the storms strengthen the overturning, primarily through enhanced mixing in the upper 300 m, whereas deeper mixing has a minor effect. The sensitivity of the results to horizontal resolution (20, 5, 2 and 1 km), vertical resolution and numerical choices is evaluated. Challenging issues concerning how numerical models are able to represent interior mixing forced by high-frequency winds are exposed and discussed, particularly in the context of the overturning circulation. Overall, submesoscale-permitting ocean modeling exhibits important delicacies owing to a lack of convergence of key components of its energetics even when reaching Δ x = 1 km. Text Southern Ocean Copernicus Publications: E-Journals Southern Ocean Ocean Science 12 3 743 769
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The aim of this study is to clarify the role of the Southern Ocean storms on interior mixing and meridional overturning circulation. A periodic and idealized numerical model has been designed to represent the key physical processes of a zonal portion of the Southern Ocean located between 70 and 40° S. It incorporates physical ingredients deemed essential for Southern Ocean functioning: rough topography, seasonally varying air–sea fluxes, and high-latitude storms with analytical form. The forcing strategy ensures that the time mean wind stress is the same between the different simulations, so the effect of the storms on the mean wind stress and resulting impacts on the Southern Ocean dynamics are not considered in this study. Level and distribution of mixing attributable to high-frequency winds are quantified and compared to those generated by eddy–topography interactions and dissipation of the balanced flow. Results suggest that (1) the synoptic atmospheric variability alone can generate the levels of mid-depth dissipation frequently observed in the Southern Ocean (10 −10 –10 −9 W kg −1 ) and (2) the storms strengthen the overturning, primarily through enhanced mixing in the upper 300 m, whereas deeper mixing has a minor effect. The sensitivity of the results to horizontal resolution (20, 5, 2 and 1 km), vertical resolution and numerical choices is evaluated. Challenging issues concerning how numerical models are able to represent interior mixing forced by high-frequency winds are exposed and discussed, particularly in the context of the overturning circulation. Overall, submesoscale-permitting ocean modeling exhibits important delicacies owing to a lack of convergence of key components of its energetics even when reaching Δ x = 1 km.
format Text
author Jouanno, Julien
Capet, Xavier
Madec, Gurvan
Roullet, Guillaume
Klein, Patrice
spellingShingle Jouanno, Julien
Capet, Xavier
Madec, Gurvan
Roullet, Guillaume
Klein, Patrice
Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean
author_facet Jouanno, Julien
Capet, Xavier
Madec, Gurvan
Roullet, Guillaume
Klein, Patrice
author_sort Jouanno, Julien
title Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean
title_short Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean
title_full Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean
title_fullStr Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean
title_full_unstemmed Dissipation of the energy imparted by mid-latitude storms in the Southern Ocean
title_sort dissipation of the energy imparted by mid-latitude storms in the southern ocean
publishDate 2018
url https://doi.org/10.5194/os-12-743-2016
https://os.copernicus.org/articles/12/743/2016/
geographic Southern Ocean
geographic_facet Southern Ocean
genre Southern Ocean
genre_facet Southern Ocean
op_source eISSN: 1812-0792
op_relation doi:10.5194/os-12-743-2016
https://os.copernicus.org/articles/12/743/2016/
op_doi https://doi.org/10.5194/os-12-743-2016
container_title Ocean Science
container_volume 12
container_issue 3
container_start_page 743
op_container_end_page 769
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