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    Nonlinear Saturation of Baroclinic Instability. Part II: Continuously Stratified Fluid

    Source: Journal of the Atmospheric Sciences:;1988:;Volume( 046 ):;issue: 007::page 888
    Author:
    Shepherd, Theodore G.
    DOI: 10.1175/1520-0469(1989)046<0888:NSOBIP>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Rigorous upper bounds are derived that limit the finite-amplitude growth of arbitrary nonzonal disturbances to an unstable baroclinic zonal flow in a continuously stratified, quasi-geostrophic, semi-infinite fluid. Bounds are obtained bath on the depth-integrated eddy potential enstrophy and on the eddy available potential energy (APE) at the ground. The method used to derive the bounds is essentially analogous to that used in Part I of this study for the two-layer model: it relies on the existence of a nonlinear Liapunov (normed) stability theorem, which is a finite-amplitude generalization of the Charney-Stern theorem. As in Part I, the bounds are valid both for conservative (unforced, inviscid) flow, as well as for forced-dissipative flow when the dissipation is proportional to the potential vorticity in the interior, and to the potential temperature at the ground. The character of the results depends on the dimensionless external parameter ? = f02?/?0N2H, where ? is the maximum vertical shear of the zonal wind, H is the density scale height, and the other symbols have their usual meaning. When ? ? 1, corresponding to ?deep? unstable modes (vertical scale ≈H), the bound on the eddy potential enstrophy is just the total potential enstrophy in the system; but when ??1, corresponding to ?shallow? unstable modes (vertical scale ≈?H), the eddy potential enstrophy can be bounded well below the total amount available in the system. In neither case can the bound on the eddy APE prevent a complete neutralization of the surface temperature gradient which is in accord with numerical experience. For the special case of the Charney model of baroclinic instability, and in the limit of infinitesimal initial eddy disturbance amplitude, the bound states that the dimensionless eddy potential enstrophy cannot exceed (? + 1)2/24 here h = HN/f0L is the dimensionless scale height and L is the width of the channel. These bounds are very similar to (though of course generally larger than) ad hoc estimates based on baroclinic-adjustment arguments. The possibility of using these kinds of bounds for eddy-amplitude closure in a transient-eddy parameterization scheme is also discussed.
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      Nonlinear Saturation of Baroclinic Instability. Part II: Continuously Stratified Fluid

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4156221
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    contributor authorShepherd, Theodore G.
    date accessioned2017-06-09T14:28:51Z
    date available2017-06-09T14:28:51Z
    date copyright1989/04/01
    date issued1988
    identifier issn0022-4928
    identifier otherams-20037.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156221
    description abstractRigorous upper bounds are derived that limit the finite-amplitude growth of arbitrary nonzonal disturbances to an unstable baroclinic zonal flow in a continuously stratified, quasi-geostrophic, semi-infinite fluid. Bounds are obtained bath on the depth-integrated eddy potential enstrophy and on the eddy available potential energy (APE) at the ground. The method used to derive the bounds is essentially analogous to that used in Part I of this study for the two-layer model: it relies on the existence of a nonlinear Liapunov (normed) stability theorem, which is a finite-amplitude generalization of the Charney-Stern theorem. As in Part I, the bounds are valid both for conservative (unforced, inviscid) flow, as well as for forced-dissipative flow when the dissipation is proportional to the potential vorticity in the interior, and to the potential temperature at the ground. The character of the results depends on the dimensionless external parameter ? = f02?/?0N2H, where ? is the maximum vertical shear of the zonal wind, H is the density scale height, and the other symbols have their usual meaning. When ? ? 1, corresponding to ?deep? unstable modes (vertical scale ≈H), the bound on the eddy potential enstrophy is just the total potential enstrophy in the system; but when ??1, corresponding to ?shallow? unstable modes (vertical scale ≈?H), the eddy potential enstrophy can be bounded well below the total amount available in the system. In neither case can the bound on the eddy APE prevent a complete neutralization of the surface temperature gradient which is in accord with numerical experience. For the special case of the Charney model of baroclinic instability, and in the limit of infinitesimal initial eddy disturbance amplitude, the bound states that the dimensionless eddy potential enstrophy cannot exceed (? + 1)2/24 here h = HN/f0L is the dimensionless scale height and L is the width of the channel. These bounds are very similar to (though of course generally larger than) ad hoc estimates based on baroclinic-adjustment arguments. The possibility of using these kinds of bounds for eddy-amplitude closure in a transient-eddy parameterization scheme is also discussed.
    publisherAmerican Meteorological Society
    titleNonlinear Saturation of Baroclinic Instability. Part II: Continuously Stratified Fluid
    typeJournal Paper
    journal volume46
    journal issue7
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1989)046<0888:NSOBIP>2.0.CO;2
    journal fristpage888
    journal lastpage907
    treeJournal of the Atmospheric Sciences:;1988:;Volume( 046 ):;issue: 007
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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