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    Barotropic Instability of a Zonal Jet: From Nondivergent Perturbations on the β Plane to Divergent Perturbations on a Sphere

    Source: Journal of Physical Oceanography:;2006:;Volume( 036 ):;issue: 012::page 2271
    Author:
    Paldor, Nathan
    ,
    Dvorkin, Yona
    DOI: 10.1175/JPO2960.1
    Publisher: American Meteorological Society
    Abstract: The linear instability of divergent perturbations that evolve on a cos2 mean steady zonal jet embedded in a zonal channel on the ? plane and on a rotating sphere is studied for zonally propagating wavelike perturbations of the shallow-water equations. The complex phase speeds result from the imposition of the no-flow boundary conditions at the channel walls on the numerical solutions of the linear differential equations for the wave latitude-dependent amplitude. In addition, the same numerical method is applied to the traditional problem of linear instability of nondivergent perturbations on the ? plane where results reaffirm the classical, analytically derived, features. For these nondivergent perturbations, the present study shows that the growth rate increases monotonically with the jet maximal speed and that the classical result of a local maximum at some finite westward-directed speed results from scaling the growth rates on the jet?s speed. In contrast to nondivergent perturbations, divergent perturbations on the ? plane have no short-wave cutoff, and so the nondivergent solution does not provide an estimate for the divergent solution, even when the ocean is 1000 km deep (i.e., when the speed of gravity waves exceeds 10 Mach). For realistic values of the ocean depth, the growth rates of divergent perturbations are smaller than those of nondivergent perturbations, but with the increase in the ocean depth they become larger than those of nondivergent perturbations. For both perturbations, a slight asymmetry exists between eastward- and westward-flowing jets. The growth rates of divergent perturbations on a sphere are similar to those on the ? plane for the same values of the model parameters, but the asymmetry between eastward and westward jets is more conspicuous on a sphere. The value of g?H? (g? is the reduced gravity; H? is the equivalent mean layer thickness), which is filtered out in nondivergent theory, determines for divergent perturbations the relative magnitude of zonal velocity, meridional velocity, and height but has little effect on the growth rates.
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      Barotropic Instability of a Zonal Jet: From Nondivergent Perturbations on the β Plane to Divergent Perturbations on a Sphere

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    https://yetl.yabesh.ir/yetl1/handle/yetl/4225994
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    contributor authorPaldor, Nathan
    contributor authorDvorkin, Yona
    date accessioned2017-06-09T17:18:22Z
    date available2017-06-09T17:18:22Z
    date copyright2006/12/01
    date issued2006
    identifier issn0022-3670
    identifier otherams-82836.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4225994
    description abstractThe linear instability of divergent perturbations that evolve on a cos2 mean steady zonal jet embedded in a zonal channel on the ? plane and on a rotating sphere is studied for zonally propagating wavelike perturbations of the shallow-water equations. The complex phase speeds result from the imposition of the no-flow boundary conditions at the channel walls on the numerical solutions of the linear differential equations for the wave latitude-dependent amplitude. In addition, the same numerical method is applied to the traditional problem of linear instability of nondivergent perturbations on the ? plane where results reaffirm the classical, analytically derived, features. For these nondivergent perturbations, the present study shows that the growth rate increases monotonically with the jet maximal speed and that the classical result of a local maximum at some finite westward-directed speed results from scaling the growth rates on the jet?s speed. In contrast to nondivergent perturbations, divergent perturbations on the ? plane have no short-wave cutoff, and so the nondivergent solution does not provide an estimate for the divergent solution, even when the ocean is 1000 km deep (i.e., when the speed of gravity waves exceeds 10 Mach). For realistic values of the ocean depth, the growth rates of divergent perturbations are smaller than those of nondivergent perturbations, but with the increase in the ocean depth they become larger than those of nondivergent perturbations. For both perturbations, a slight asymmetry exists between eastward- and westward-flowing jets. The growth rates of divergent perturbations on a sphere are similar to those on the ? plane for the same values of the model parameters, but the asymmetry between eastward and westward jets is more conspicuous on a sphere. The value of g?H? (g? is the reduced gravity; H? is the equivalent mean layer thickness), which is filtered out in nondivergent theory, determines for divergent perturbations the relative magnitude of zonal velocity, meridional velocity, and height but has little effect on the growth rates.
    publisherAmerican Meteorological Society
    titleBarotropic Instability of a Zonal Jet: From Nondivergent Perturbations on the β Plane to Divergent Perturbations on a Sphere
    typeJournal Paper
    journal volume36
    journal issue12
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/JPO2960.1
    journal fristpage2271
    journal lastpage2282
    treeJournal of Physical Oceanography:;2006:;Volume( 036 ):;issue: 012
    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