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    Nonlinear Interactions Among Equatorial Waves

    Source: Journal of the Atmospheric Sciences:;1977:;Volume( 034 ):;issue: 003::page 486
    Author:
    Domaracki, Alan
    ,
    Lossch, Arthur Z.
    DOI: 10.1175/1520-0469(1977)034<0486:NIAEW>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The asymptotic method multiple scales is used to investigate nonlinear interactions among equatorial waves (Kelvin, mixed Rossby-gravity, Rossby, eastward and westward propagating inertial-gravity) using a divergent equatorial beta-plane model. The Hermite polynomial meridional structure of equatorial waves results in a relaxation of the kinematic resonance conditions in the present model as compared to similar investigations in a mid-latitude context. Numerical solutions of the resonance conditions establish that triads composed of the same as well as different wave types exist. Energy solutions obtained in the absence of spatial and phase modulations show that the triad members having maximum absolute frequency always grows (decays) at the expense of the remaining triad members. It is suggested that a single finite-amplitude equatorial wave may be unstable with respect to lower frequency ?parasitic? resonant wave perturbations. In the tropical atmosphere, nonlinear wave instability may he an important energy redistribution mechanism where naturally occurring forcing mechanisms excite selected wave types over a restricted range of wavenumbers.
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      Nonlinear Interactions Among Equatorial Waves

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4153131
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    contributor authorDomaracki, Alan
    contributor authorLossch, Arthur Z.
    date accessioned2017-06-09T14:19:26Z
    date available2017-06-09T14:19:26Z
    date copyright1977/03/01
    date issued1977
    identifier issn0022-4928
    identifier otherams-17257.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153131
    description abstractThe asymptotic method multiple scales is used to investigate nonlinear interactions among equatorial waves (Kelvin, mixed Rossby-gravity, Rossby, eastward and westward propagating inertial-gravity) using a divergent equatorial beta-plane model. The Hermite polynomial meridional structure of equatorial waves results in a relaxation of the kinematic resonance conditions in the present model as compared to similar investigations in a mid-latitude context. Numerical solutions of the resonance conditions establish that triads composed of the same as well as different wave types exist. Energy solutions obtained in the absence of spatial and phase modulations show that the triad members having maximum absolute frequency always grows (decays) at the expense of the remaining triad members. It is suggested that a single finite-amplitude equatorial wave may be unstable with respect to lower frequency ?parasitic? resonant wave perturbations. In the tropical atmosphere, nonlinear wave instability may he an important energy redistribution mechanism where naturally occurring forcing mechanisms excite selected wave types over a restricted range of wavenumbers.
    publisherAmerican Meteorological Society
    titleNonlinear Interactions Among Equatorial Waves
    typeJournal Paper
    journal volume34
    journal issue3
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1977)034<0486:NIAEW>2.0.CO;2
    journal fristpage486
    journal lastpage498
    treeJournal of the Atmospheric Sciences:;1977:;Volume( 034 ):;issue: 003
    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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