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    HARMONIC WAVE SOLUTIONS OF THE NON-LINEAR VORTICITY EQUATION FOR A ROTATING VISCOUS FLUID

    Source: Journal of Meteorology:;1954:;volume( 011 ):;issue: 005::page 373
    Author:
    Kao, Shih-Kung
    DOI: 10.1175/1520-0469(1954)011<0373:HWSOTN>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: With the assumption of non-divergent horizontal flow, harmonic wave solutions of the non-linear hydrodynamic equations for a rotating, viscous fluid are obtained both for the plane and for the sphere. These solutions yield waves which may be damped, amplified, or remain unchanged, depending on the longitudinal and latitudinal extents of the waves, and also on the vertical profile of the stream function. For plane flow, the vertical profile of the velocity components is shown to be a sinusoidal function, or a hyperbolic sine and cosine of z, proportional to or independent of z, the elevation. For spherical flow, the vertical profile is shown to be proportional to a Bessel function of order n + ½, and n, an integer, is the degree of a surface spherical harmonic. Harmonic waves are amplified, neutral or damped, depending respectively on whether the argument of the Bessel function is imaginary, zero or real. No steady wave is possible in spherical viscous flow, although quasi-stationary waves, which may be defined as waves with zero wave-velocity but changing wave-amplitude, may occur under certain circumstances.
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      HARMONIC WAVE SOLUTIONS OF THE NON-LINEAR VORTICITY EQUATION FOR A ROTATING VISCOUS FLUID

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4149619
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    contributor authorKao, Shih-Kung
    date accessioned2017-06-09T14:11:03Z
    date available2017-06-09T14:11:03Z
    date copyright1954/10/01
    date issued1954
    identifier issn0095-9634
    identifier otherams-14096.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4149619
    description abstractWith the assumption of non-divergent horizontal flow, harmonic wave solutions of the non-linear hydrodynamic equations for a rotating, viscous fluid are obtained both for the plane and for the sphere. These solutions yield waves which may be damped, amplified, or remain unchanged, depending on the longitudinal and latitudinal extents of the waves, and also on the vertical profile of the stream function. For plane flow, the vertical profile of the velocity components is shown to be a sinusoidal function, or a hyperbolic sine and cosine of z, proportional to or independent of z, the elevation. For spherical flow, the vertical profile is shown to be proportional to a Bessel function of order n + ½, and n, an integer, is the degree of a surface spherical harmonic. Harmonic waves are amplified, neutral or damped, depending respectively on whether the argument of the Bessel function is imaginary, zero or real. No steady wave is possible in spherical viscous flow, although quasi-stationary waves, which may be defined as waves with zero wave-velocity but changing wave-amplitude, may occur under certain circumstances.
    publisherAmerican Meteorological Society
    titleHARMONIC WAVE SOLUTIONS OF THE NON-LINEAR VORTICITY EQUATION FOR A ROTATING VISCOUS FLUID
    typeJournal Paper
    journal volume11
    journal issue5
    journal titleJournal of Meteorology
    identifier doi10.1175/1520-0469(1954)011<0373:HWSOTN>2.0.CO;2
    journal fristpage373
    journal lastpage379
    treeJournal of Meteorology:;1954:;volume( 011 ):;issue: 005
    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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