Multidecadal Preconditioning of the Maud Rise Polynya Region

In this paper, we consider Maud Rise polynya formation in a long (250 years) high-resolution (ocean 0.1°, atmosphere 0.5° horizontal model resolution) of the Community Earth System Model. We find a dominant multidecadal time scale in the occurrence of these Maud Rise polynyas. Analysis of the result...

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Main Authors: Westen, René M., Dijkstra, Henk A.
Format: Text
Language:English
Published: 2020
Subjects:
Online Access:https://doi.org/10.5194/os-2020-25
https://os.copernicus.org/preprints/os-2020-25/
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spelling ftcopernicus:oai:publications.copernicus.org:osd84789 2023-05-15T18:24:40+02:00 Multidecadal Preconditioning of the Maud Rise Polynya Region Westen, René M. Dijkstra, Henk A. 2020-04-16 application/pdf https://doi.org/10.5194/os-2020-25 https://os.copernicus.org/preprints/os-2020-25/ eng eng doi:10.5194/os-2020-25 https://os.copernicus.org/preprints/os-2020-25/ eISSN: 1812-0792 Text 2020 ftcopernicus https://doi.org/10.5194/os-2020-25 2020-07-20T16:22:17Z In this paper, we consider Maud Rise polynya formation in a long (250 years) high-resolution (ocean 0.1°, atmosphere 0.5° horizontal model resolution) of the Community Earth System Model. We find a dominant multidecadal time scale in the occurrence of these Maud Rise polynyas. Analysis of the results leads us to the interpretation that a preferred time scale 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 time scale in convection through preconditioning of the subsurface density, and consequently to polynya formation. Text Southern Ocean Copernicus Publications: E-Journals Maud Rise ENVELOPE(3.000,3.000,-66.000,-66.000) Southern Ocean Weddell
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description In this paper, we consider Maud Rise polynya formation in a long (250 years) high-resolution (ocean 0.1°, atmosphere 0.5° horizontal model resolution) of the Community Earth System Model. We find a dominant multidecadal time scale in the occurrence of these Maud Rise polynyas. Analysis of the results leads us to the interpretation that a preferred time scale 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 time scale in convection through preconditioning of the subsurface density, and consequently to polynya formation.
format Text
author Westen, René M.
Dijkstra, Henk A.
spellingShingle Westen, René M.
Dijkstra, Henk A.
Multidecadal Preconditioning of the Maud Rise Polynya Region
author_facet Westen, René M.
Dijkstra, Henk A.
author_sort Westen, René M.
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
publishDate 2020
url https://doi.org/10.5194/os-2020-25
https://os.copernicus.org/preprints/os-2020-25/
long_lat ENVELOPE(3.000,3.000,-66.000,-66.000)
geographic Maud Rise
Southern Ocean
Weddell
geographic_facet Maud Rise
Southern Ocean
Weddell
genre Southern Ocean
genre_facet Southern Ocean
op_source eISSN: 1812-0792
op_relation doi:10.5194/os-2020-25
https://os.copernicus.org/preprints/os-2020-25/
op_doi https://doi.org/10.5194/os-2020-25
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