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    Supercritical Dynamics of Baroclinic Disturbances in the Presence of Asymmetric Ekman Dissipation

    Source: Journal of the Atmospheric Sciences:;1986:;Volume( 043 ):;issue: 017::page 1781
    Author:
    Chou, Shih-Hung
    ,
    Loesch, Arthur Z.
    DOI: 10.1175/1520-0469(1986)043<1781:SDOBDI>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Finite-amplitude dynamics of baroclinic waves are examined in the presence of asymmetric Ekman pumping at the lower and upper boundaries. Both asymptotic and spectral numerical methods are employed. The resulting amplitude equations yield time evolutions that can lead to an eventual equilibration, a regular perpetual vacillation or a chaotic vacillation depending on the actual values of the supercriticality, the dissipation and the stratification parameters and the fundamental zonal wavenumber. Within the limits of strong bottom dissipation and weak supercriticality, the system always eventually equilibrates and the asymptotic results compare favorably with the numerical results. The vacillation is most likely to occur when the bottom dissipation is weak, supercriticality is strong or the viscous asymmetry is high. Vacillatory final states are possible for up to an order of magnitude larger bottom dissipation than predicted by the symmetric configuration, provided the top dissipation is small in comparison.
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      Supercritical Dynamics of Baroclinic Disturbances in the Presence of Asymmetric Ekman Dissipation

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4155442
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    contributor authorChou, Shih-Hung
    contributor authorLoesch, Arthur Z.
    date accessioned2017-06-09T14:26:36Z
    date available2017-06-09T14:26:36Z
    date copyright1986/09/01
    date issued1986
    identifier issn0022-4928
    identifier otherams-19337.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4155442
    description abstractFinite-amplitude dynamics of baroclinic waves are examined in the presence of asymmetric Ekman pumping at the lower and upper boundaries. Both asymptotic and spectral numerical methods are employed. The resulting amplitude equations yield time evolutions that can lead to an eventual equilibration, a regular perpetual vacillation or a chaotic vacillation depending on the actual values of the supercriticality, the dissipation and the stratification parameters and the fundamental zonal wavenumber. Within the limits of strong bottom dissipation and weak supercriticality, the system always eventually equilibrates and the asymptotic results compare favorably with the numerical results. The vacillation is most likely to occur when the bottom dissipation is weak, supercriticality is strong or the viscous asymmetry is high. Vacillatory final states are possible for up to an order of magnitude larger bottom dissipation than predicted by the symmetric configuration, provided the top dissipation is small in comparison.
    publisherAmerican Meteorological Society
    titleSupercritical Dynamics of Baroclinic Disturbances in the Presence of Asymmetric Ekman Dissipation
    typeJournal Paper
    journal volume43
    journal issue17
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1986)043<1781:SDOBDI>2.0.CO;2
    journal fristpage1781
    journal lastpage1795
    treeJournal of the Atmospheric Sciences:;1986:;Volume( 043 ):;issue: 017
    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
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