Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4

Most CMIP5 (Coupled Model Intercomparison Project Phase 5) models unrealistically form Antarctic Bottom Water by open ocean deep convection in the Weddell and Ross seas. To identify the mechanisms triggering Southern Ocean deep convection in models, we perform sensitivity experiments on the ocean mo...

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Main Authors: C. Heuzé, J. K. Ridley, D. Calvert, D. P. Stevens, K. J. Heywood
Format: Article
Language:English
Published: Copernicus Publications 2015-10-01
Series:Geoscientific Model Development
Online Access:http://www.geosci-model-dev.net/8/3119/2015/gmd-8-3119-2015.pdf
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spelling doaj-8efbc2c333c1453fb7bebef9f1a0dcca2020-11-24T20:57:49ZengCopernicus PublicationsGeoscientific Model Development1991-959X1991-96032015-10-018103119313010.5194/gmd-8-3119-2015Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4C. Heuzé0J. K. Ridley1D. Calvert2D. P. Stevens3K. J. Heywood4Centre for Ocean and Atmospheric Sciences, University of East Anglia, Norwich, NR4 7TJ, UKMet Office, Hadley Centre, Exeter, EX1 3PB, UKMet Office, Hadley Centre, Exeter, EX1 3PB, UKCentre for Ocean and Atmospheric Sciences, University of East Anglia, Norwich, NR4 7TJ, UKCentre for Ocean and Atmospheric Sciences, University of East Anglia, Norwich, NR4 7TJ, UKMost CMIP5 (Coupled Model Intercomparison Project Phase 5) models unrealistically form Antarctic Bottom Water by open ocean deep convection in the Weddell and Ross seas. To identify the mechanisms triggering Southern Ocean deep convection in models, we perform sensitivity experiments on the ocean model NEMO3.4 forced by prescribed atmospheric fluxes. We vary the vertical velocity scale of the Langmuir turbulence, the fraction of turbulent kinetic energy transferred below the mixed layer, and the background diffusivity and run short simulations from 1980. All experiments exhibit deep convection in the Riiser-Larsen Sea in 1987; the origin is a positive sea ice anomaly in 1985, causing a shallow anomaly in mixed layer depth, hence anomalously warm surface waters and subsequent polynya opening. Modifying the vertical mixing impacts both the climatological state and the associated surface anomalies. The experiments with enhanced mixing exhibit colder surface waters and reduced deep convection. The experiments with decreased mixing give warmer surface waters, open larger polynyas causing more saline surface waters and have deep convection across the Weddell Sea until the simulations end. Extended experiments reveal an increase in the Drake Passage transport of 4 Sv each year deep convection occurs, leading to an unrealistically large transport at the end of the simulation. North Atlantic deep convection is not significantly affected by the changes in mixing parameters. As new climate model overflow parameterisations are developed to form Antarctic Bottom Water more realistically, we argue that models would benefit from stopping Southern Ocean deep convection, for example by increasing their vertical mixing.http://www.geosci-model-dev.net/8/3119/2015/gmd-8-3119-2015.pdf
collection DOAJ
language English
format Article
sources DOAJ
author C. Heuzé
J. K. Ridley
D. Calvert
D. P. Stevens
K. J. Heywood
spellingShingle C. Heuzé
J. K. Ridley
D. Calvert
D. P. Stevens
K. J. Heywood
Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4
Geoscientific Model Development
author_facet C. Heuzé
J. K. Ridley
D. Calvert
D. P. Stevens
K. J. Heywood
author_sort C. Heuzé
title Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4
title_short Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4
title_full Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4
title_fullStr Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4
title_full_unstemmed Increasing vertical mixing to reduce Southern Ocean deep convection in NEMO3.4
title_sort increasing vertical mixing to reduce southern ocean deep convection in nemo3.4
publisher Copernicus Publications
series Geoscientific Model Development
issn 1991-959X
1991-9603
publishDate 2015-10-01
description Most CMIP5 (Coupled Model Intercomparison Project Phase 5) models unrealistically form Antarctic Bottom Water by open ocean deep convection in the Weddell and Ross seas. To identify the mechanisms triggering Southern Ocean deep convection in models, we perform sensitivity experiments on the ocean model NEMO3.4 forced by prescribed atmospheric fluxes. We vary the vertical velocity scale of the Langmuir turbulence, the fraction of turbulent kinetic energy transferred below the mixed layer, and the background diffusivity and run short simulations from 1980. All experiments exhibit deep convection in the Riiser-Larsen Sea in 1987; the origin is a positive sea ice anomaly in 1985, causing a shallow anomaly in mixed layer depth, hence anomalously warm surface waters and subsequent polynya opening. Modifying the vertical mixing impacts both the climatological state and the associated surface anomalies. The experiments with enhanced mixing exhibit colder surface waters and reduced deep convection. The experiments with decreased mixing give warmer surface waters, open larger polynyas causing more saline surface waters and have deep convection across the Weddell Sea until the simulations end. Extended experiments reveal an increase in the Drake Passage transport of 4 Sv each year deep convection occurs, leading to an unrealistically large transport at the end of the simulation. North Atlantic deep convection is not significantly affected by the changes in mixing parameters. As new climate model overflow parameterisations are developed to form Antarctic Bottom Water more realistically, we argue that models would benefit from stopping Southern Ocean deep convection, for example by increasing their vertical mixing.
url http://www.geosci-model-dev.net/8/3119/2015/gmd-8-3119-2015.pdf
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