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contributor authorLindzen, Richard S.
date accessioned2017-06-09T14:28:04Z
date available2017-06-09T14:28:04Z
date copyright1988/02/01
date issued1988
identifier issn0022-4928
identifier otherams-19759.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4155910
description abstractThe usual assumption that vertically propagating internal gravity waves will cease growing with height once their amplitudes are such as to permit convective instability anywhere within the wave is reexamined. Two factors lead to amplitude limitation: (i) wave clipping associated with convective mixing, and (ii) energetic constraints associated with the rate at which the wave can supply energy to the convection. It is found that these two factors limit supersaturation to about 50% for waves with short horizontal wavelengths and high relative phase speeds. Usually the degree of supersaturation will be much less. These factors also lead to a gradual, rather than sudden, cessation of wave growth with height.
publisherAmerican Meteorological Society
titleSupersaturation of Vertically Propagating Internal Gravity Waves
typeJournal Paper
journal volume45
journal issue4
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1988)045<0705:SOVPIG>2.0.CO;2
journal fristpage705
journal lastpage711
treeJournal of the Atmospheric Sciences:;1988:;Volume( 045 ):;issue: 004
contenttypeFulltext


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