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The effects on oceanic planetary waves of coupling with an atmospheric energy balance model

The effects on oceanic planetary waves of coupling with an atmospheric energy balance model
The effects on oceanic planetary waves of coupling with an atmospheric energy balance model
This paper shows the existence of a growing planetary-wave-like ocean mode, with a decadal period and growth rate, which appears when a stratified, diffusive ocean is coupled to a simple atmosphere via an energy balance model (EBM). Such modes are not found when simpler surface ocean conditions are applied. The mode is low order in the vertical and, because of its slow growth, is likely to be observed in Earth System Models using an EBM in place of a fuller set of atmospheric dynamics. There is no apparent physical energy source for such a mode, and therefore it should not be expected to arise in such a model. The mode is analysed through a hierarchy of simple models, which differ only through their surface boundary condition.
0280-6495
742-757
Farneti, R.
673f8147-87ca-49a2-95e6-fb3da4fa4ab8
Killworth, P.D.
9fc0c4a0-e1fb-4073-8997-436b59c74bf2
Farneti, R.
673f8147-87ca-49a2-95e6-fb3da4fa4ab8
Killworth, P.D.
9fc0c4a0-e1fb-4073-8997-436b59c74bf2

Farneti, R. and Killworth, P.D. (2005) The effects on oceanic planetary waves of coupling with an atmospheric energy balance model. Tellus A, 57 (5), 742-757. (doi:10.1111/j.1600-0870.2005.00144.x).

Record type: Article

Abstract

This paper shows the existence of a growing planetary-wave-like ocean mode, with a decadal period and growth rate, which appears when a stratified, diffusive ocean is coupled to a simple atmosphere via an energy balance model (EBM). Such modes are not found when simpler surface ocean conditions are applied. The mode is low order in the vertical and, because of its slow growth, is likely to be observed in Earth System Models using an EBM in place of a fuller set of atmospheric dynamics. There is no apparent physical energy source for such a mode, and therefore it should not be expected to arise in such a model. The mode is analysed through a hierarchy of simple models, which differ only through their surface boundary condition.

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Published date: 2005

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Local EPrints ID: 17476
URI: http://eprints.soton.ac.uk/id/eprint/17476
ISSN: 0280-6495
PURE UUID: 1a07beef-e6a8-4bed-89b8-88b6b4ddf1b3

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Date deposited: 30 Sep 2005
Last modified: 15 Mar 2024 06:00

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Contributors

Author: R. Farneti
Author: P.D. Killworth

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