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    Thermal Convection in a Rotating Annulus of Liquid: Effect of Viscosity on the Transition Between Axisymmetric and Non-Axisymmetric Flow Regimes

    Source: Journal of the Atmospheric Sciences:;1965:;Volume( 022 ):;issue: 005::page 541
    Author:
    Hide, R.
    ,
    Fowlis, W. W.
    DOI: 10.1175/1520-0469(1965)022<0541:TCIARA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: When a vertical rotating annulus of liquid is subject to a horizontal temperature gradient, provided that the coefficient of kinematical viscosity, ??, is not too great and the angular velocity of rotation,Ω is sufficiently high, four distinct regimes of hydrodynamical flow are possible, as shown in previous work by Hide. Only one of these regimes is characterized by symmetry about the axis of rotation. The principal properties of the flow depend largely on the dimensionless parameters ?2≡d/(b?a), ?4gd??/??Ω2(b?a)2, ?5≡4Ω2(b?a)5/??2d and ?6≡??/??, where d is the depth of the fluid,b and a are the radi of curvature of the surfaces of the annulus, g is the acceleration of gravity, ?? is the mean density of the fluid, ?? is the density contrast associated with the impressed horizontal temperature gradient and ?? is the thermal diffusivity of the fluid. In a diagram with log10?5 as abscissa and log10?4 as ordinate, axisymmetric flow is found outside an anvil-shaped region whose upper boundary lies below the line 11,&=2.0, the flow being symmetric for an 114 when 115 where lis. The lower boundary of the anvil-shaped region is given by the equation. log10(II4II6) = ? (0.864±0.043) log10(II2II5) + 5.05±0.30?(standard errors) Theory suggests that the non-axisymmetric flow is a manifestation of ?baroclinic instability,? a process first studied in the investigation of planetary-scale atmospheric motions. The experimental results are discussed in terms of Eady' theoretical baroclinic instability model, as extended by others to include effects due to viscous boundary layers. Qualitatively, agreement between theory and experiment is satisfactory, and at the highest values of II attained in the experiments the quantitative agreement is remarkably good. The poor quantitative agreement found at the lowest values of II5 attained indicates that a major source of frictional dissipation has not yet been properly accounted for in the theory.
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      Thermal Convection in a Rotating Annulus of Liquid: Effect of Viscosity on the Transition Between Axisymmetric and Non-Axisymmetric Flow Regimes

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    contributor authorHide, R.
    contributor authorFowlis, W. W.
    date accessioned2017-06-09T14:13:37Z
    date available2017-06-09T14:13:37Z
    date copyright1965/09/01
    date issued1965
    identifier issn0022-4928
    identifier otherams-15131.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150770
    description abstractWhen a vertical rotating annulus of liquid is subject to a horizontal temperature gradient, provided that the coefficient of kinematical viscosity, ??, is not too great and the angular velocity of rotation,Ω is sufficiently high, four distinct regimes of hydrodynamical flow are possible, as shown in previous work by Hide. Only one of these regimes is characterized by symmetry about the axis of rotation. The principal properties of the flow depend largely on the dimensionless parameters ?2≡d/(b?a), ?4gd??/??Ω2(b?a)2, ?5≡4Ω2(b?a)5/??2d and ?6≡??/??, where d is the depth of the fluid,b and a are the radi of curvature of the surfaces of the annulus, g is the acceleration of gravity, ?? is the mean density of the fluid, ?? is the density contrast associated with the impressed horizontal temperature gradient and ?? is the thermal diffusivity of the fluid. In a diagram with log10?5 as abscissa and log10?4 as ordinate, axisymmetric flow is found outside an anvil-shaped region whose upper boundary lies below the line 11,&=2.0, the flow being symmetric for an 114 when 115 where lis. The lower boundary of the anvil-shaped region is given by the equation. log10(II4II6) = ? (0.864±0.043) log10(II2II5) + 5.05±0.30?(standard errors) Theory suggests that the non-axisymmetric flow is a manifestation of ?baroclinic instability,? a process first studied in the investigation of planetary-scale atmospheric motions. The experimental results are discussed in terms of Eady' theoretical baroclinic instability model, as extended by others to include effects due to viscous boundary layers. Qualitatively, agreement between theory and experiment is satisfactory, and at the highest values of II attained in the experiments the quantitative agreement is remarkably good. The poor quantitative agreement found at the lowest values of II5 attained indicates that a major source of frictional dissipation has not yet been properly accounted for in the theory.
    publisherAmerican Meteorological Society
    titleThermal Convection in a Rotating Annulus of Liquid: Effect of Viscosity on the Transition Between Axisymmetric and Non-Axisymmetric Flow Regimes
    typeJournal Paper
    journal volume22
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1965)022<0541:TCIARA>2.0.CO;2
    journal fristpage541
    journal lastpage558
    treeJournal of the Atmospheric Sciences:;1965:;Volume( 022 ):;issue: 005
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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