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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Bibliographic Details
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
Description
Summary:<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>
ISSN:1812-0784
1812-0792