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    Slaving Principles, Balanced Dynamics, and the Hydrostatic Boussinesq Equations

    Source: Journal of the Atmospheric Sciences:;1997:;Volume( 054 ):;issue: 012::page 1662
    Author:
    Bokhove, Onno
    DOI: 10.1175/1520-0469(1997)054<1662:SPBDAT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The problem of finding higher-order generalizations of the quasigeostrophic and semigeostrophic models, that is, higher-order balanced models, is investigated systematically by using a slaving principle. It is shown that most existing balanced models are based on an underlying slave equation with varying master variables and that this slaving approach arises as an alternative to the secular conventional Rossby number expansions. While in the conventional expansions all variables are expanded in a power series in the Rossby number, the slaving approach suggests modified expansion or iteration procedures in which only the fast variables (associated with gravity modes) are expanded or iterated. The slow variables (associated with vortical modes) are now the master variables in the system; a well-known choice for large-scale extratropical flows in geophysical fluid dynamics is potential vorticity. To illustrate both the iteration and the modified expansion procedures, the slaving approach is applied to the rapidly rotating hydrostatic Boussinesq equations in a horizontally semi-infinite domain by using a Rossby number scaling. Higher-order generalizations of the quasigeostrophic equations result from modified expansions, and higher-order generalizations of the semigeostrophic equations result from nonlinear iterations. The validity of the latter for small Rossby numbers as well as small frontal parameters exemplifies the advantage nonlinear iterations have.
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      Slaving Principles, Balanced Dynamics, and the Hydrostatic Boussinesq Equations

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    contributor authorBokhove, Onno
    date accessioned2017-06-09T14:34:34Z
    date available2017-06-09T14:34:34Z
    date copyright1997/06/01
    date issued1997
    identifier issn0022-4928
    identifier otherams-22010.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4158414
    description abstractThe problem of finding higher-order generalizations of the quasigeostrophic and semigeostrophic models, that is, higher-order balanced models, is investigated systematically by using a slaving principle. It is shown that most existing balanced models are based on an underlying slave equation with varying master variables and that this slaving approach arises as an alternative to the secular conventional Rossby number expansions. While in the conventional expansions all variables are expanded in a power series in the Rossby number, the slaving approach suggests modified expansion or iteration procedures in which only the fast variables (associated with gravity modes) are expanded or iterated. The slow variables (associated with vortical modes) are now the master variables in the system; a well-known choice for large-scale extratropical flows in geophysical fluid dynamics is potential vorticity. To illustrate both the iteration and the modified expansion procedures, the slaving approach is applied to the rapidly rotating hydrostatic Boussinesq equations in a horizontally semi-infinite domain by using a Rossby number scaling. Higher-order generalizations of the quasigeostrophic equations result from modified expansions, and higher-order generalizations of the semigeostrophic equations result from nonlinear iterations. The validity of the latter for small Rossby numbers as well as small frontal parameters exemplifies the advantage nonlinear iterations have.
    publisherAmerican Meteorological Society
    titleSlaving Principles, Balanced Dynamics, and the Hydrostatic Boussinesq Equations
    typeJournal Paper
    journal volume54
    journal issue12
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1997)054<1662:SPBDAT>2.0.CO;2
    journal fristpage1662
    journal lastpage1674
    treeJournal of the Atmospheric Sciences:;1997:;Volume( 054 ):;issue: 012
    contenttypeFulltext
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