eddy parameterization
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2013 ◽  
Vol 64 ◽  
pp. 12-28 ◽  
Author(s):  
S. Bachman ◽  
B. Fox-Kemper

2011 ◽  
Vol 24 (19) ◽  
pp. 4992-4998 ◽  
Author(s):  
Peter R. Gent ◽  
Gokhan Danabasoglu

Results from two perturbation experiments using the Community Climate System Model version 4 where the Southern Hemisphere zonal wind stress is increased are described. It is shown that the ocean response is in accord with experiments using much-higher-resolution ocean models that do not use an eddy parameterization. The key to obtaining an appropriate response in the coarse-resolution climate model is to specify a variable coefficient in the Gent and McWilliams eddy parameterization, rather than a constant value. This result contrasts with several recent papers that have suggested that coarse-resolution climate models cannot obtain an appropriate response.


2010 ◽  
Vol 32 (3-4) ◽  
pp. 118-131 ◽  
Author(s):  
E. Pérez-Pérez ◽  
P.L. Read ◽  
I.M. Moroz

2008 ◽  
Vol 38 (7) ◽  
pp. 1607-1613 ◽  
Author(s):  
David P. Marshall ◽  
Alberto C. Naveira Garabato

Abstract The parameterization of geostrophic eddies represents a large sink of energy in most ocean models, yet the ultimate fate of this eddy energy in the ocean remains unclear. The authors conjecture that a significant fraction of the eddy energy may be transferred to internal lee waves and oscillations over rough bottom topography, leading to bottom-enhanced diapycnal mixing. A range of circumstantial evidence in support of this conjecture is presented and discussed. The authors further propose a modification to the Gent and McWilliams eddy parameterization to account for the bottom-enhanced diapycnal mixing.


2005 ◽  
Vol 35 (2) ◽  
pp. 175-187 ◽  
Author(s):  
Allen Kuo ◽  
R. Alan Plumb ◽  
John Marshall

Abstract The equilibrium of a modeled wind- and buoyancy-driven, baroclinically unstable, flow is analyzed using the transformed Eulerian-mean (TEM) approach described in Part I. Within the near-adiabatic interior of the flow, Ertel potential vorticity is homogenized along mean isopycnals—a finding readily explained using TEM theory, given the geometry of the domain. The equilibrium, zonal-mean buoyancy structure at the surface is determined entirely by a balance between imposed surface fluxes and residual mean and eddy buoyancy transport within a “surface diabatic layer.” Balance between these same processes and the wind stress determines the stratification, and hence potential vorticity, immediately below this layer. Ertel potential vorticity homogenization below then determines the mean buoyancy structure everywhere. Accordingly, the equilibrium structure of this flow can be described—and quantitatively reproduced—from knowledge of the eddy mixing rates within the surface diabatic zone and the depth of this zone, together with potential vorticity homogenization beneath. These results emphasize the need to include near-surface buoyancy transport, as well as interior PV transport, in eddy parameterization schemes. They also imply that, in more realistic models, the surface buoyancy balances may be impacted by processes in remote locations that allow diapycnal flow.


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