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    Dispersive–Dissipative Eddy Parameterization in a Barotropic Model

    Source: Journal of Physical Oceanography:;2001:;Volume( 031 ):;issue: 008::page 2525
    Author:
    Nadiga, Balasubramanya T.
    ,
    Margolin, Len G.
    DOI: 10.1175/1520-0485(2001)031<2525:DDEPIA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Recently 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.
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      Dispersive–Dissipative Eddy Parameterization in a Barotropic Model

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4166749
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    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
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian