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contributor authorFuchs, Željka
contributor authorRaymond, David J.
date accessioned2017-06-09T14:37:41Z
date available2017-06-09T14:37:41Z
date copyright2002/05/01
date issued2002
identifier issn0022-4928
identifier otherams-23111.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159637
description abstractA minimal model of a moist equatorial atmosphere is presented in which the precipitation rate is assumed to depend on just the vertically averaged saturation deficit and the convective available potential energy. When wind-induced surface heat exchange (WISHE) and cloud?radiation interactions are turned off, there are no growing modes. Gravity waves with wavenumbers smaller than a certain limit respond to a reduced static stability due to latent heat release, and therefore propagate more slowly than dry modes, while those with larger wavenumbers respond to the normal dry static stability. In addition, there exists a stationary mode that decays slowly with time. For realistic parameter values, the effect of reduced static stability on gravity waves is limited to wavelengths greater than the circumference of the earth. WISHE and cloud?radiation interactions both destabilize the stationary mode, but not the gravity waves.
publisherAmerican Meteorological Society
titleLarge-Scale Modes of a Nonrotating Atmosphere with Water Vapor and Cloud–Radiation Feedbacks
typeJournal Paper
journal volume59
journal issue10
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(2002)059<1669:LSMOAN>2.0.CO;2
journal fristpage1669
journal lastpage1679
treeJournal of the Atmospheric Sciences:;2002:;Volume( 059 ):;issue: 010
contenttypeFulltext


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