Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea

A high-resolution coupled ocean-sea ice model is set up within the Labrador Sea. With a horizontal resolution of 1/60°, this simulation is capable of resolving the multitude of eddies which transport heat and freshwater into the interior of the Labrador Sea. The transport of these fluxes strongly go...

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Main Authors: Pennelly, Clark, Myers, Paul G.
Format: Text
Language:English
Published: 2020
Subjects:
Online Access:https://doi.org/10.5194/gmd-2020-111
https://gmd.copernicus.org/preprints/gmd-2020-111/
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spelling ftcopernicus:oai:publications.copernicus.org:gmdd85130 2023-05-15T16:27:09+02:00 Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea Pennelly, Clark Myers, Paul G. 2020-04-30 application/pdf https://doi.org/10.5194/gmd-2020-111 https://gmd.copernicus.org/preprints/gmd-2020-111/ eng eng doi:10.5194/gmd-2020-111 https://gmd.copernicus.org/preprints/gmd-2020-111/ eISSN: 1991-9603 Text 2020 ftcopernicus https://doi.org/10.5194/gmd-2020-111 2020-07-20T16:22:13Z A high-resolution coupled ocean-sea ice model is set up within the Labrador Sea. With a horizontal resolution of 1/60°, this simulation is capable of resolving the multitude of eddies which transport heat and freshwater into the interior of the Labrador Sea. The transport of these fluxes strongly governs the overall stratification, deep convection, and subsequent production of Labrador Sea Water. We implement nested domains within our regional configuration to reduce computational costs, allowing for a simulation that spans over 10 years. Three passive tracers are also included: Greenland runoff, Labrador Sea Water produced during convection, and Irminger Water which enters the Labrador Sea along Greenland. We describe the configuration setup and compare against similarly forced lower-resolution simulations to better describe how horizontal resolution impacts the Labrador Sea. Text Greenland Labrador Sea Sea ice Copernicus Publications: E-Journals Greenland
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description A high-resolution coupled ocean-sea ice model is set up within the Labrador Sea. With a horizontal resolution of 1/60°, this simulation is capable of resolving the multitude of eddies which transport heat and freshwater into the interior of the Labrador Sea. The transport of these fluxes strongly governs the overall stratification, deep convection, and subsequent production of Labrador Sea Water. We implement nested domains within our regional configuration to reduce computational costs, allowing for a simulation that spans over 10 years. Three passive tracers are also included: Greenland runoff, Labrador Sea Water produced during convection, and Irminger Water which enters the Labrador Sea along Greenland. We describe the configuration setup and compare against similarly forced lower-resolution simulations to better describe how horizontal resolution impacts the Labrador Sea.
format Text
author Pennelly, Clark
Myers, Paul G.
spellingShingle Pennelly, Clark
Myers, Paul G.
Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea
author_facet Pennelly, Clark
Myers, Paul G.
author_sort Pennelly, Clark
title Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea
title_short Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea
title_full Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea
title_fullStr Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea
title_full_unstemmed Introducing LAB60: A 1/60° NEMO 3.6 numerical simulation of the Labrador Sea
title_sort introducing lab60: a 1/60° nemo 3.6 numerical simulation of the labrador sea
publishDate 2020
url https://doi.org/10.5194/gmd-2020-111
https://gmd.copernicus.org/preprints/gmd-2020-111/
geographic Greenland
geographic_facet Greenland
genre Greenland
Labrador Sea
Sea ice
genre_facet Greenland
Labrador Sea
Sea ice
op_source eISSN: 1991-9603
op_relation doi:10.5194/gmd-2020-111
https://gmd.copernicus.org/preprints/gmd-2020-111/
op_doi https://doi.org/10.5194/gmd-2020-111
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