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    Mechanisms of Up-Valley Winds

    Source: Journal of the Atmospheric Sciences:;2004:;Volume( 061 ):;issue: 024::page 3097
    Author:
    Rampanelli, Gabriele
    ,
    Zardi, Dino
    ,
    Rotunno, Richard
    DOI: 10.1175/JAS-3354.1
    Publisher: American Meteorological Society
    Abstract: The basic physical mechanisms governing the daytime evolution of up-valley winds in mountain valleys are investigated using a series of numerical simulations of thermally driven flow over idealized three-dimensional topography. The three-dimensional topography used in this study is composed of two, two-dimensional topographies: one a slope connecting a plain with a plateau and the other a valley with a horizontal floor. The present two-dimensional simulations of the valley flow agree with results of previous investigations in that the heated sidewalls produce upslope flows that require a compensating subsidence in the valley core bringing down potentially warmer air from the stable free atmosphere. In the context of the three-dimensional valley?plain simulations, the authors find that this subsidence heating in the valley core is the main contributor to the valley? plain temperature contrast, which, under the hydrostatic approximation, is the main contributor to the valley? plain pressure difference that drives the up-valley wind.
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      Mechanisms of Up-Valley Winds

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    contributor authorRampanelli, Gabriele
    contributor authorZardi, Dino
    contributor authorRotunno, Richard
    date accessioned2017-06-09T16:51:57Z
    date available2017-06-09T16:51:57Z
    date copyright2004/12/01
    date issued2004
    identifier issn0022-4928
    identifier otherams-75543.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4217891
    description abstractThe basic physical mechanisms governing the daytime evolution of up-valley winds in mountain valleys are investigated using a series of numerical simulations of thermally driven flow over idealized three-dimensional topography. The three-dimensional topography used in this study is composed of two, two-dimensional topographies: one a slope connecting a plain with a plateau and the other a valley with a horizontal floor. The present two-dimensional simulations of the valley flow agree with results of previous investigations in that the heated sidewalls produce upslope flows that require a compensating subsidence in the valley core bringing down potentially warmer air from the stable free atmosphere. In the context of the three-dimensional valley?plain simulations, the authors find that this subsidence heating in the valley core is the main contributor to the valley? plain temperature contrast, which, under the hydrostatic approximation, is the main contributor to the valley? plain pressure difference that drives the up-valley wind.
    publisherAmerican Meteorological Society
    titleMechanisms of Up-Valley Winds
    typeJournal Paper
    journal volume61
    journal issue24
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/JAS-3354.1
    journal fristpage3097
    journal lastpage3111
    treeJournal of the Atmospheric Sciences:;2004:;Volume( 061 ):;issue: 024
    contenttypeFulltext
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