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Stability of the thermohaline circulation in different complexities and resolutions of earth system model (abstract of paper presented at 3rd EGU General Assembly)

Stability of the thermohaline circulation in different complexities and resolutions of earth system model (abstract of paper presented at 3rd EGU General Assembly)
Stability of the thermohaline circulation in different complexities and resolutions of earth system model (abstract of paper presented at 3rd EGU General Assembly)
We use the GENIE Earth system modelling framework to examine how the stability / hysteresis diagram of the thermohaline circulation (THC) depends on the use of complex (GCM) or simple (energy-moisture balance) atmosphere models and how it varies with ocean resolution.
The model versions all use the GOLDSTEIN frictional geostrophic ocean, but with 3 different horizontal resolutions (and 8 depth layers in each case): (i) 36x36 longitudesine (latitude), (ii) 72x72 longitude-sine(latitude), (iii) 64x32 longitude-latitude. To these we have coupled the Reading Intermediate General Circulation Model (IGCM) at T21 resolution with 7 vertical levels. We contrast this with earlier work using an energy-moisture balance model (EMBM) and ocean resolution (i).
For each model version, we construct an ensemble of runs in which we vary atmospheric freshwater transport from the Atlantic to Pacific. In some cases we also vary a parameter controlling equator to pole freshwater transport. The resulting ensembles are run toward equilibrium and then restarts are used to search parameter space for regions of THC bi-stability.
The resulting hundreds of thousands of years of 3D ocean-atmosphere model integration were achieved by using UK Grid computing resources, including 6 nodes of the National Grid Service, and additional clusters in Norwich, Southampton and Bristol. A specially developed database system was used to execute and manage the runs.
The results are expected to shed light on whether a dynamical atmosphere alters or removes the bi-stability of the THC, and whether THC stability is sensitive to ocean resolution.
1029-7006
8018
Marsh, R.
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Myerscough, R.J.
ae14f72e-fb09-4b64-bed2-899a7a97ca33
Lenton, T.M.
f2b4fe3d-ef5e-4c85-9677-bfc20c266b65
Price, A.R.
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Cox, S.J.
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Edwards, N.R.
e41b719b-784e-4748-acc4-6ccbc4643c7d
Lunt, D.J.
5bfca8db-49a7-45dd-9855-43606a58788b
Marsh, R.
702c2e7e-ac19-4019-abd9-a8614ab27717
Myerscough, R.J.
ae14f72e-fb09-4b64-bed2-899a7a97ca33
Lenton, T.M.
f2b4fe3d-ef5e-4c85-9677-bfc20c266b65
Price, A.R.
15a6667c-60da-42e9-b6dd-4c0e56c33c52
Cox, S.J.
0e62aaed-24ad-4a74-b996-f606e40e5c55
Edwards, N.R.
e41b719b-784e-4748-acc4-6ccbc4643c7d
Lunt, D.J.
5bfca8db-49a7-45dd-9855-43606a58788b

Marsh, R., Myerscough, R.J., Lenton, T.M., Price, A.R., Cox, S.J., Edwards, N.R. and Lunt, D.J. (2006) Stability of the thermohaline circulation in different complexities and resolutions of earth system model (abstract of paper presented at 3rd EGU General Assembly). Geophysical Research Abstracts, 8, 8018.

Record type: Article

Abstract

We use the GENIE Earth system modelling framework to examine how the stability / hysteresis diagram of the thermohaline circulation (THC) depends on the use of complex (GCM) or simple (energy-moisture balance) atmosphere models and how it varies with ocean resolution.
The model versions all use the GOLDSTEIN frictional geostrophic ocean, but with 3 different horizontal resolutions (and 8 depth layers in each case): (i) 36x36 longitudesine (latitude), (ii) 72x72 longitude-sine(latitude), (iii) 64x32 longitude-latitude. To these we have coupled the Reading Intermediate General Circulation Model (IGCM) at T21 resolution with 7 vertical levels. We contrast this with earlier work using an energy-moisture balance model (EMBM) and ocean resolution (i).
For each model version, we construct an ensemble of runs in which we vary atmospheric freshwater transport from the Atlantic to Pacific. In some cases we also vary a parameter controlling equator to pole freshwater transport. The resulting ensembles are run toward equilibrium and then restarts are used to search parameter space for regions of THC bi-stability.
The resulting hundreds of thousands of years of 3D ocean-atmosphere model integration were achieved by using UK Grid computing resources, including 6 nodes of the National Grid Service, and additional clusters in Norwich, Southampton and Bristol. A specially developed database system was used to execute and manage the runs.
The results are expected to shed light on whether a dynamical atmosphere alters or removes the bi-stability of the THC, and whether THC stability is sensitive to ocean resolution.

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Published date: 2006

Identifiers

Local EPrints ID: 28976
URI: http://eprints.soton.ac.uk/id/eprint/28976
ISSN: 1029-7006
PURE UUID: b9f01240-de8a-45a0-9835-e6954172970c

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Date deposited: 09 May 2006
Last modified: 22 Jul 2022 20:38

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Contributors

Author: R. Marsh
Author: R.J. Myerscough
Author: T.M. Lenton
Author: A.R. Price
Author: S.J. Cox
Author: N.R. Edwards
Author: D.J. Lunt

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