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contributor authorSzeto, Kit K.
contributor authorLin, Charles A.
contributor authorStewart, Ronald E.
date accessioned2017-06-09T14:28:15Z
date available2017-06-09T14:28:15Z
date copyright1988/06/01
date issued1988
identifier issn0022-4928
identifier otherams-19823.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4155982
description abstractThe melting of snow extracts latent heat of fusion from the environment. The basic response of the atmosphere to this cooling-by-melting mechanism is investigated by using a nonlinear two-dimensional numerical model. It is found that the resultant melting-induced circulations consist of a forced downdraft which spreads out laterally like a gravity current and transients which are gravity waves. The characteristics of these mesoscale thermally driven circulations are studied under idealistic atmospheric conditions. Model results show that the melting associated with realistic precipitation rates (up to 10 mm h?1) can induce horizontal wind perturbations of several meters per second and vertical motions of tens of centimeters per second. Since the gravity waves and the cold outflow current propagate away from the source, they can have significant dynamic effects on the environment remote from the precipitation region. Moreover, the melting-induced, near O°C isothermal layer in the atmosphere alters the local static stability. It is inferred that thew melting-induced effects may significantly influence the momentum and moisture transports in mesoscale precipitation systems.
publisherAmerican Meteorological Society
titleMesoscale Circulations Forced by Melting Snow. Part I: Basic Simulations and Dynamics
typeJournal Paper
journal volume45
journal issue11
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1988)045<1629:MCFBMS>2.0.CO;2
journal fristpage1629
journal lastpage1641
treeJournal of the Atmospheric Sciences:;1988:;Volume( 045 ):;issue: 011
contenttypeFulltext


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