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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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