Multidecadal preconditioning of the Maud Rise polynya region

<p>In this paper, we consider Maud Rise polynya formation in a long (250-year) high-resolution (ocean 0.1<span class="inline-formula"><sup>∘</sup></span>, atmosphere 0.5<span class="inline-formula"><sup>∘</sup></span> horizont...

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Main Authors: R. M. van Westen, H. A. Dijkstra
Format: Article
Language:English
Published: Copernicus Publications 2020-11-01
Series:Ocean Science
Online Access:https://os.copernicus.org/articles/16/1443/2020/os-16-1443-2020.pdf
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spelling doaj-41549f34f1744a6a8d02b648adc348592020-11-25T04:11:59ZengCopernicus PublicationsOcean Science1812-07841812-07922020-11-01161443145710.5194/os-16-1443-2020Multidecadal preconditioning of the Maud Rise polynya regionR. M. van Westen0H. A. Dijkstra1H. A. Dijkstra2Institute for Marine and Atmospheric research Utrecht, Department of Physics, Utrecht University, Utrecht, the NetherlandsInstitute for Marine and Atmospheric research Utrecht, Department of Physics, Utrecht University, Utrecht, the NetherlandsCenter for Complex Systems Studies, Utrecht University, Utrecht, the Netherlands<p>In this paper, we consider Maud Rise polynya formation in a long (250-year) high-resolution (ocean 0.1<span class="inline-formula"><sup>∘</sup></span>, atmosphere 0.5<span class="inline-formula"><sup>∘</sup></span> horizontal model resolution) of the Community Earth System Model. We find a dominant multidecadal timescale in the occurrence of these Maud Rise polynyas. Analysis of the results leads us to the interpretation that a preferred timescale can be induced by the variability of the Weddell Gyre, previously identified as the Southern Ocean Mode. The large-scale pattern of heat content variability associated with the Southern Ocean Mode modifies the stratification in the Maud Rise region and leads to a preferred timescale in convection through preconditioning of the subsurface density and consequently to polynya formation.</p>https://os.copernicus.org/articles/16/1443/2020/os-16-1443-2020.pdf
collection DOAJ
language English
format Article
sources DOAJ
author R. M. van Westen
H. A. Dijkstra
H. A. Dijkstra
spellingShingle R. M. van Westen
H. A. Dijkstra
H. A. Dijkstra
Multidecadal preconditioning of the Maud Rise polynya region
Ocean Science
author_facet R. M. van Westen
H. A. Dijkstra
H. A. Dijkstra
author_sort R. M. van Westen
title Multidecadal preconditioning of the Maud Rise polynya region
title_short Multidecadal preconditioning of the Maud Rise polynya region
title_full Multidecadal preconditioning of the Maud Rise polynya region
title_fullStr Multidecadal preconditioning of the Maud Rise polynya region
title_full_unstemmed Multidecadal preconditioning of the Maud Rise polynya region
title_sort multidecadal preconditioning of the maud rise polynya region
publisher Copernicus Publications
series Ocean Science
issn 1812-0784
1812-0792
publishDate 2020-11-01
description <p>In this paper, we consider Maud Rise polynya formation in a long (250-year) high-resolution (ocean 0.1<span class="inline-formula"><sup>∘</sup></span>, atmosphere 0.5<span class="inline-formula"><sup>∘</sup></span> horizontal model resolution) of the Community Earth System Model. We find a dominant multidecadal timescale in the occurrence of these Maud Rise polynyas. Analysis of the results leads us to the interpretation that a preferred timescale can be induced by the variability of the Weddell Gyre, previously identified as the Southern Ocean Mode. The large-scale pattern of heat content variability associated with the Southern Ocean Mode modifies the stratification in the Maud Rise region and leads to a preferred timescale in convection through preconditioning of the subsurface density and consequently to polynya formation.</p>
url https://os.copernicus.org/articles/16/1443/2020/os-16-1443-2020.pdf
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