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    Circularly Polarized Inertial Wave Vectors in Rotating Fluids

    Source: Journal of the Atmospheric Sciences:;1976:;Volume( 033 ):;issue: 007::page 1223
    Author:
    Cogley, Allen C.
    DOI: 10.1175/1520-0469(1976)033<1223:CPIWVI>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The Navier-Stokes equations for a rotating fluid are harmonically analyzed for planar motion in an infinite half-space. All solutions are shown to be a sum of two inertial wave vectors, one circularly polarized to the left (CPL) and the other circularly polarized to the right (CPR). These basic solutions are therefore presented in the same nomenclature and form as that found useful by experimentalists in analyzing now data (called ?rotary spectra?). The CPL wave acts counter to the Coriolis force and consequently has a slower phase speed and larger damping than the CPR wave. At resonance (forcing frequency=Coriolis frequency) the CPR wave has an infinite phase speed and no damping and is the important component leading to the singular nature of the solutions for certain boundary conditions. All possible resonant singularities are explicitly shown. The unsteady development of these unbounded (limited space structure), cyclic (no time origin or structure) flows is presented to show that with time structure the resonant singularities evolve in a self-similar manner.
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      Circularly Polarized Inertial Wave Vectors in Rotating Fluids

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    contributor authorCogley, Allen C.
    date accessioned2017-06-09T14:19:00Z
    date available2017-06-09T14:19:00Z
    date copyright1976/07/01
    date issued1976
    identifier issn0022-4928
    identifier otherams-17095.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4152951
    description abstractThe Navier-Stokes equations for a rotating fluid are harmonically analyzed for planar motion in an infinite half-space. All solutions are shown to be a sum of two inertial wave vectors, one circularly polarized to the left (CPL) and the other circularly polarized to the right (CPR). These basic solutions are therefore presented in the same nomenclature and form as that found useful by experimentalists in analyzing now data (called ?rotary spectra?). The CPL wave acts counter to the Coriolis force and consequently has a slower phase speed and larger damping than the CPR wave. At resonance (forcing frequency=Coriolis frequency) the CPR wave has an infinite phase speed and no damping and is the important component leading to the singular nature of the solutions for certain boundary conditions. All possible resonant singularities are explicitly shown. The unsteady development of these unbounded (limited space structure), cyclic (no time origin or structure) flows is presented to show that with time structure the resonant singularities evolve in a self-similar manner.
    publisherAmerican Meteorological Society
    titleCircularly Polarized Inertial Wave Vectors in Rotating Fluids
    typeJournal Paper
    journal volume33
    journal issue7
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1976)033<1223:CPIWVI>2.0.CO;2
    journal fristpage1223
    journal lastpage1233
    treeJournal of the Atmospheric Sciences:;1976:;Volume( 033 ):;issue: 007
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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