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    Stability of Thin Non-Rotating Hadley Circulations

    Source: Journal of the Atmospheric Sciences:;1972:;Volume( 029 ):;issue: 004::page 687
    Author:
    Hart, J. E.
    DOI: 10.1175/1520-0469(1972)029<0687:SOTNRH>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A simple parallel flow model is derived for a thin (depth to length ratio ?1) Hadley circulation in a two-dimensional box with rigid horizontal boundaries maintained at a temperature which increases linearly with the horizontal coordinate x. Vertical velocities are assumed to he confined to narrow regions near the ends. The stability of this solution is discussed. Several modes of energy transfer to and from the mean kinetic and potential energies exist. As opposed to the case of thermal convection between isothermal plates in a constant shear, transverse disturbances with symmetry normal to the shear vector are always more unstable than longitudinal disturbances with symmetry parallel to the shear vector. Implications of these results for recent theoretical ideas on the Venusian circulation are discussed.
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      Stability of Thin Non-Rotating Hadley Circulations

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    contributor authorHart, J. E.
    date accessioned2017-06-09T14:16:23Z
    date available2017-06-09T14:16:23Z
    date copyright1972/05/01
    date issued1972
    identifier issn0022-4928
    identifier otherams-16167.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151920
    description abstractA simple parallel flow model is derived for a thin (depth to length ratio ?1) Hadley circulation in a two-dimensional box with rigid horizontal boundaries maintained at a temperature which increases linearly with the horizontal coordinate x. Vertical velocities are assumed to he confined to narrow regions near the ends. The stability of this solution is discussed. Several modes of energy transfer to and from the mean kinetic and potential energies exist. As opposed to the case of thermal convection between isothermal plates in a constant shear, transverse disturbances with symmetry normal to the shear vector are always more unstable than longitudinal disturbances with symmetry parallel to the shear vector. Implications of these results for recent theoretical ideas on the Venusian circulation are discussed.
    publisherAmerican Meteorological Society
    titleStability of Thin Non-Rotating Hadley Circulations
    typeJournal Paper
    journal volume29
    journal issue4
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1972)029<0687:SOTNRH>2.0.CO;2
    journal fristpage687
    journal lastpage697
    treeJournal of the Atmospheric Sciences:;1972:;Volume( 029 ):;issue: 004
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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