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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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