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    Basin-Mode Interactions and Selection by the Mean Flow in a Reduced-Gravity Quasigeostrophic Model

    Source: Journal of Physical Oceanography:;2003:;Volume( 033 ):;issue: 011::page 2320
    Author:
    Ben Jelloul, Mahdi
    ,
    Huck, Thierry
    DOI: 10.1175/1520-0485(2003)033<2320:BIASBT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The selection mechanisms of Rossby basin modes are investigated in the reduced-gravity quasigeostrophic framework. The linear solution of the wind-driven circulation is decomposed in a steady forced?dissipated solution and a time-dependent component. The steady solution consists in a classical Sverdrup flow dissipated in a thin western boundary layer. The time-dependent solution is a sum of Rossby basin modes with arbitrary amplitudes. The effect of the nonlinear term is handled through a weakly nonlinear analysis providing a set of evolution equations for the mode amplitudes. It is shown both analytically (infinite Burger number) and numerically (finite Burger number) that mode stability is related to the gyre configuration. For cyclonic or anticyclonic single gyres, all basin modes are neutral. In the traditional (reversed) double-gyre case, large-scale basin modes are damped (unstable). Pure basin-mode interactions yield triads with cycling energy and subharmonic instabilities. The latter provide a potential mechanism for spectral reddening.
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      Basin-Mode Interactions and Selection by the Mean Flow in a Reduced-Gravity Quasigeostrophic Model

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4167225
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    contributor authorBen Jelloul, Mahdi
    contributor authorHuck, Thierry
    date accessioned2017-06-09T14:55:59Z
    date available2017-06-09T14:55:59Z
    date copyright2003/11/01
    date issued2003
    identifier issn0022-3670
    identifier otherams-29942.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4167225
    description abstractThe selection mechanisms of Rossby basin modes are investigated in the reduced-gravity quasigeostrophic framework. The linear solution of the wind-driven circulation is decomposed in a steady forced?dissipated solution and a time-dependent component. The steady solution consists in a classical Sverdrup flow dissipated in a thin western boundary layer. The time-dependent solution is a sum of Rossby basin modes with arbitrary amplitudes. The effect of the nonlinear term is handled through a weakly nonlinear analysis providing a set of evolution equations for the mode amplitudes. It is shown both analytically (infinite Burger number) and numerically (finite Burger number) that mode stability is related to the gyre configuration. For cyclonic or anticyclonic single gyres, all basin modes are neutral. In the traditional (reversed) double-gyre case, large-scale basin modes are damped (unstable). Pure basin-mode interactions yield triads with cycling energy and subharmonic instabilities. The latter provide a potential mechanism for spectral reddening.
    publisherAmerican Meteorological Society
    titleBasin-Mode Interactions and Selection by the Mean Flow in a Reduced-Gravity Quasigeostrophic Model
    typeJournal Paper
    journal volume33
    journal issue11
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/1520-0485(2003)033<2320:BIASBT>2.0.CO;2
    journal fristpage2320
    journal lastpage2332
    treeJournal of Physical Oceanography:;2003:;Volume( 033 ):;issue: 011
    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