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    Reexamination of Wave-CISK Theory: Existence and Properties of Nonlinear Wave-CISK Modes

    Source: Journal of the Atmospheric Sciences:;1989:;Volume( 047 ):;issue: 024::page 3078
    Author:
    Lim, Hock
    ,
    Lim, Tian-Kuay
    ,
    Chang, C-P.
    DOI: 10.1175/1520-0469(1990)047<3078:ROWCTE>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Linear analyses of wave-CISK models often lead to the conclusion that the mechanism does not explain the scale selection of planetary-scale tropical motions. In particular, Kelvin or gravity wave-CISK tends to prefer cumulus-scale motions. On the other hand, numerical models with ?positive-only? heating did not experience much difficulty in generating large scale disturbances of realistic structure. A previous study explained these numerical results in terms of linear Kelvin wave-CISK modes, whose wave packages exhibit remarkable resemblence to the simulated disturbances. However, the linear theory can not explain how the simulated disturbances can maintain a ?wavenumber-l? structure against the explosive growth of short wavelength components. A reexamination of the wave-CISK theories is carried out in this paper. It is argued that the CISK mechanism possess inherently a very severe form of nonlinearity that takes full effect for even infinitesimal perturbations. The linearized CISK theories, therefore, do not give a correct description of a CISK-driven system at any stage of its development. A simple 5-level 64-wave spectral model demonstrates that the nonlinear effects of wave-CISK alone is able to produce exponentially growing ?wavenumber-1? flow patterns that propagate without change of shape. Since these flow patterns have well-defined structure, growth rate, and propagation speed, it is proposed to call them nonlinear wave-CISK modes. The nonlinear wave-CISK modes exhibit all the characteristics of the linear Kelvin wave-CISK packages of Chang and Lim (1988). The scale selection problem of their linear Kelvin wave-CISK theory has, however, been resolved. Introduction of a diffusion damping has no significant effect on the propagation speed and structure of these modes. The overall structure of the modes depends mainly on the growth rate. Varying other parameters may affect the growth rate; but modes of the same growth rate look rather like each other, irrespective of the other parameters.
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      Reexamination of Wave-CISK Theory: Existence and Properties of Nonlinear Wave-CISK Modes

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4156677
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    contributor authorLim, Hock
    contributor authorLim, Tian-Kuay
    contributor authorChang, C-P.
    date accessioned2017-06-09T14:30:05Z
    date available2017-06-09T14:30:05Z
    date copyright1990/12/01
    date issued1989
    identifier issn0022-4928
    identifier otherams-20448.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156677
    description abstractLinear analyses of wave-CISK models often lead to the conclusion that the mechanism does not explain the scale selection of planetary-scale tropical motions. In particular, Kelvin or gravity wave-CISK tends to prefer cumulus-scale motions. On the other hand, numerical models with ?positive-only? heating did not experience much difficulty in generating large scale disturbances of realistic structure. A previous study explained these numerical results in terms of linear Kelvin wave-CISK modes, whose wave packages exhibit remarkable resemblence to the simulated disturbances. However, the linear theory can not explain how the simulated disturbances can maintain a ?wavenumber-l? structure against the explosive growth of short wavelength components. A reexamination of the wave-CISK theories is carried out in this paper. It is argued that the CISK mechanism possess inherently a very severe form of nonlinearity that takes full effect for even infinitesimal perturbations. The linearized CISK theories, therefore, do not give a correct description of a CISK-driven system at any stage of its development. A simple 5-level 64-wave spectral model demonstrates that the nonlinear effects of wave-CISK alone is able to produce exponentially growing ?wavenumber-1? flow patterns that propagate without change of shape. Since these flow patterns have well-defined structure, growth rate, and propagation speed, it is proposed to call them nonlinear wave-CISK modes. The nonlinear wave-CISK modes exhibit all the characteristics of the linear Kelvin wave-CISK packages of Chang and Lim (1988). The scale selection problem of their linear Kelvin wave-CISK theory has, however, been resolved. Introduction of a diffusion damping has no significant effect on the propagation speed and structure of these modes. The overall structure of the modes depends mainly on the growth rate. Varying other parameters may affect the growth rate; but modes of the same growth rate look rather like each other, irrespective of the other parameters.
    publisherAmerican Meteorological Society
    titleReexamination of Wave-CISK Theory: Existence and Properties of Nonlinear Wave-CISK Modes
    typeJournal Paper
    journal volume47
    journal issue24
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1990)047<3078:ROWCTE>2.0.CO;2
    journal fristpage3078
    journal lastpage3091
    treeJournal of the Atmospheric Sciences:;1989:;Volume( 047 ):;issue: 024
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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