Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model

Open-ocean polynyas (OOPs) in the Southern Ocean are ice-free areas within the winter ice pack that are associated with deep convection, potentially contributing to the formation of Antarctic Bottom Water. To enhance the credibility of Earth system models (ESMs), their ability to simulate OOPs reali...

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Published in:Journal of Climate
Main Authors: Kurtakoti, Prajvala, Veneziani, Milena, Stössel, Achim, Weijer, Wilbert
Language:unknown
Published: 2021
Subjects:
Online Access:http://www.osti.gov/servlets/purl/1483544
https://www.osti.gov/biblio/1483544
https://doi.org/10.1175/JCLI-D-18-0392.1
id ftosti:oai:osti.gov:1483544
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spelling ftosti:oai:osti.gov:1483544 2023-07-30T03:59:10+02:00 Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model Kurtakoti, Prajvala Veneziani, Milena Stössel, Achim Weijer, Wilbert 2021-07-28 application/pdf http://www.osti.gov/servlets/purl/1483544 https://www.osti.gov/biblio/1483544 https://doi.org/10.1175/JCLI-D-18-0392.1 unknown http://www.osti.gov/servlets/purl/1483544 https://www.osti.gov/biblio/1483544 https://doi.org/10.1175/JCLI-D-18-0392.1 doi:10.1175/JCLI-D-18-0392.1 58 GEOSCIENCES 54 ENVIRONMENTAL SCIENCES 2021 ftosti https://doi.org/10.1175/JCLI-D-18-0392.1 2023-07-11T09:30:11Z Open-ocean polynyas (OOPs) in the Southern Ocean are ice-free areas within the winter ice pack that are associated with deep convection, potentially contributing to the formation of Antarctic Bottom Water. To enhance the credibility of Earth system models (ESMs), their ability to simulate OOPs realistically is thus crucial. Here we investigate OOPs that emerge intermittently in a high-resolution (HR) preindustrial simulation with the Energy Exascale Earth System Model, version 0.1 (E3SMv0), an offspring of the Community Earth System Model (CESM). While low-resolution (LR) simulations with E3SMv0 show no signs of OOP formation, the preindustrial E3SMv0-HR simulation produces both large Weddell Sea polynyas (WSPs) as well as small Maud Rise polynyas (MRPs). The latter are associated with a prominent seamount in the eastern Weddell Sea, and their preconditioning and formation is the focus of this study. The steep flanks of the rugged topography in this region are in E3SMv0-HR sufficiently well resolved for the impinging flow to produce pronounced Taylor caps that precondition the region for convection. Aided by an accumulation of heat in the Weddell Deep Water layer, the ultimate trigger of convection that leads to MRPs is the advection of anomalously high upper-ocean-layer salinity. The crucial difference to WSP-producing LR ESM simulations is that in E3SMv0-HR, WSPs are realistically preceded by MRPs, which in turn are a result of the flow around bathymetry being represented with unprecedented detail. Other/Unknown Material Antarc* Antarctic ice pack Southern Ocean Weddell Sea SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) Antarctic Southern Ocean Weddell Sea Weddell Maud Rise ENVELOPE(3.000,3.000,-66.000,-66.000) Journal of Climate 31 23 9659 9678
institution Open Polar
collection SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy)
op_collection_id ftosti
language unknown
topic 58 GEOSCIENCES
54 ENVIRONMENTAL SCIENCES
spellingShingle 58 GEOSCIENCES
54 ENVIRONMENTAL SCIENCES
Kurtakoti, Prajvala
Veneziani, Milena
Stössel, Achim
Weijer, Wilbert
Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model
topic_facet 58 GEOSCIENCES
54 ENVIRONMENTAL SCIENCES
description Open-ocean polynyas (OOPs) in the Southern Ocean are ice-free areas within the winter ice pack that are associated with deep convection, potentially contributing to the formation of Antarctic Bottom Water. To enhance the credibility of Earth system models (ESMs), their ability to simulate OOPs realistically is thus crucial. Here we investigate OOPs that emerge intermittently in a high-resolution (HR) preindustrial simulation with the Energy Exascale Earth System Model, version 0.1 (E3SMv0), an offspring of the Community Earth System Model (CESM). While low-resolution (LR) simulations with E3SMv0 show no signs of OOP formation, the preindustrial E3SMv0-HR simulation produces both large Weddell Sea polynyas (WSPs) as well as small Maud Rise polynyas (MRPs). The latter are associated with a prominent seamount in the eastern Weddell Sea, and their preconditioning and formation is the focus of this study. The steep flanks of the rugged topography in this region are in E3SMv0-HR sufficiently well resolved for the impinging flow to produce pronounced Taylor caps that precondition the region for convection. Aided by an accumulation of heat in the Weddell Deep Water layer, the ultimate trigger of convection that leads to MRPs is the advection of anomalously high upper-ocean-layer salinity. The crucial difference to WSP-producing LR ESM simulations is that in E3SMv0-HR, WSPs are realistically preceded by MRPs, which in turn are a result of the flow around bathymetry being represented with unprecedented detail.
author Kurtakoti, Prajvala
Veneziani, Milena
Stössel, Achim
Weijer, Wilbert
author_facet Kurtakoti, Prajvala
Veneziani, Milena
Stössel, Achim
Weijer, Wilbert
author_sort Kurtakoti, Prajvala
title Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model
title_short Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model
title_full Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model
title_fullStr Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model
title_full_unstemmed Preconditioning and Formation of Maud Rise Polynyas in a High-Resolution Earth System Model
title_sort preconditioning and formation of maud rise polynyas in a high-resolution earth system model
publishDate 2021
url http://www.osti.gov/servlets/purl/1483544
https://www.osti.gov/biblio/1483544
https://doi.org/10.1175/JCLI-D-18-0392.1
long_lat ENVELOPE(3.000,3.000,-66.000,-66.000)
geographic Antarctic
Southern Ocean
Weddell Sea
Weddell
Maud Rise
geographic_facet Antarctic
Southern Ocean
Weddell Sea
Weddell
Maud Rise
genre Antarc*
Antarctic
ice pack
Southern Ocean
Weddell Sea
genre_facet Antarc*
Antarctic
ice pack
Southern Ocean
Weddell Sea
op_relation http://www.osti.gov/servlets/purl/1483544
https://www.osti.gov/biblio/1483544
https://doi.org/10.1175/JCLI-D-18-0392.1
doi:10.1175/JCLI-D-18-0392.1
op_doi https://doi.org/10.1175/JCLI-D-18-0392.1
container_title Journal of Climate
container_volume 31
container_issue 23
container_start_page 9659
op_container_end_page 9678
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