Show simple item record

contributor authorNadiga, Balasubramanya T.
contributor authorMargolin, Len G.
date accessioned2017-06-09T14:54:46Z
date available2017-06-09T14:54:46Z
date copyright2001/08/01
date issued2001
identifier issn0022-3670
identifier otherams-29513.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4166749
description abstractRecently a new class of coarse-grained equations, known as α models, have been proposed for the mean motion of an ideal incompressible fluid. The use of one such model to represent the time-mean component of a turbulent ?-plane circulation characterized by potential vorticity mixing is considered. In particular, the focus is on the wind-driven circulation in a shallow ocean basin, a problem well studied as a prototype of more realistic ocean dynamics. The authors demonstrate the ability of an α model to reproduce qualitatively the structure of a four-gyre circulation that forms (in the time mean) when the barotropic vorticity equation is driven by a symmetric, double-gyre wind forcing, and when the dissipation is weak. This is offered as a first step in assessing the utility of the α-model approach to simulating more complex geophysical flows.
publisherAmerican Meteorological Society
titleDispersive–Dissipative Eddy Parameterization in a Barotropic Model
typeJournal Paper
journal volume31
journal issue8
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(2001)031<2525:DDEPIA>2.0.CO;2
journal fristpage2525
journal lastpage2531
treeJournal of Physical Oceanography:;2001:;Volume( 031 ):;issue: 008
contenttypeFulltext


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record