Decay of eddies at the South-West Indian Ridge

The South-West Indian Ridge in the Indian sector of the Southern Ocean is a region recognised for the creation of particularly intense eddy disturbances in the mean flow of the Antarctic Circumpolar Current. Eddies formed at this ridge have been extensively studied over the past decade using hydrogr...

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Main Authors: Jonathan Durgadoo, Isabelle Ansorge, Beverly de Cuevas, Johann Lutjeharms, Andrew Coward
Format: Article
Language:English
Published: Academy of Science of South Africa 2011-11-01
Series:South African Journal of Science
Subjects:
Online Access:http://192.168.0.121/index.php/sajs/article/view/9789
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author Jonathan Durgadoo
Isabelle Ansorge
Beverly de Cuevas
Johann Lutjeharms
Andrew Coward
author_facet Jonathan Durgadoo
Isabelle Ansorge
Beverly de Cuevas
Johann Lutjeharms
Andrew Coward
author_sort Jonathan Durgadoo
collection DOAJ
description The South-West Indian Ridge in the Indian sector of the Southern Ocean is a region recognised for the creation of particularly intense eddy disturbances in the mean flow of the Antarctic Circumpolar Current. Eddies formed at this ridge have been extensively studied over the past decade using hydrographic, satellite, drifter and float data and it is hypothesised that they could provide a vehicle for localised meridional heat and salt exchange. The effectiveness of this process is dependent on the rate of decay of the eddies. However, in order to investigate eddy decay, logistically difficult hydrographic monitoring is required. This study presents the decay of cold eddies at the South-West Indian Ridge, using outputs from a high-resolution ocean model. The model's representation of the dynamic nature of this region is fully characteristic of observations. On average, 3-4 intense and well-defined cold eddies are generated per year; these eddies have mean longevities of 5.0±2.2 months with average advection speeds of 5±2 km/day. Most simulated eddies reach their peak intensity within 1.5-2.5 months after genesis and have depths of 2000 m - 3000 m. Thereafter they dissipate within approximately 3 months. The decay of eddies is generally characterised by a decrease in their sea surface height signature, a weakening in their rotation rates and a modification in their temperature-salinity characteristics. Subantarctic top predators are suspected to forage preferentially along the edges of eddies. The process of eddy dissipation may thus influence their feeding behaviour.
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spelling doaj.art-e977c65b41894491bc50abd86f5fc5ba2022-12-21T22:10:48ZengAcademy of Science of South AfricaSouth African Journal of Science1996-74892011-11-0110711/12Decay of eddies at the South-West Indian RidgeJonathan Durgadoo0Isabelle Ansorge1Beverly de Cuevas2Johann Lutjeharms3Andrew Coward4Department of Oceanography, University of Cape TownDepartment of Oceanography, University of Cape TownMarine Systems Modelling Group, National Oceanography Centre, University of SouthamptonDepartment of Oceanography, University of Cape TownMarine Systems Modelling Group, National Oceanography Centre, University of SouthamptonThe South-West Indian Ridge in the Indian sector of the Southern Ocean is a region recognised for the creation of particularly intense eddy disturbances in the mean flow of the Antarctic Circumpolar Current. Eddies formed at this ridge have been extensively studied over the past decade using hydrographic, satellite, drifter and float data and it is hypothesised that they could provide a vehicle for localised meridional heat and salt exchange. The effectiveness of this process is dependent on the rate of decay of the eddies. However, in order to investigate eddy decay, logistically difficult hydrographic monitoring is required. This study presents the decay of cold eddies at the South-West Indian Ridge, using outputs from a high-resolution ocean model. The model's representation of the dynamic nature of this region is fully characteristic of observations. On average, 3-4 intense and well-defined cold eddies are generated per year; these eddies have mean longevities of 5.0±2.2 months with average advection speeds of 5±2 km/day. Most simulated eddies reach their peak intensity within 1.5-2.5 months after genesis and have depths of 2000 m - 3000 m. Thereafter they dissipate within approximately 3 months. The decay of eddies is generally characterised by a decrease in their sea surface height signature, a weakening in their rotation rates and a modification in their temperature-salinity characteristics. Subantarctic top predators are suspected to forage preferentially along the edges of eddies. The process of eddy dissipation may thus influence their feeding behaviour.http://192.168.0.121/index.php/sajs/article/view/9789eddy kinetic energy hotspotSouthern OceanDEIMECOCCAMPrince Edward Islands
spellingShingle Jonathan Durgadoo
Isabelle Ansorge
Beverly de Cuevas
Johann Lutjeharms
Andrew Coward
Decay of eddies at the South-West Indian Ridge
South African Journal of Science
eddy kinetic energy hotspot
Southern Ocean
DEIMEC
OCCAM
Prince Edward Islands
title Decay of eddies at the South-West Indian Ridge
title_full Decay of eddies at the South-West Indian Ridge
title_fullStr Decay of eddies at the South-West Indian Ridge
title_full_unstemmed Decay of eddies at the South-West Indian Ridge
title_short Decay of eddies at the South-West Indian Ridge
title_sort decay of eddies at the south west indian ridge
topic eddy kinetic energy hotspot
Southern Ocean
DEIMEC
OCCAM
Prince Edward Islands
url http://192.168.0.121/index.php/sajs/article/view/9789
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