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contributor authorDavies, Huw C.
date accessioned2017-06-09T14:21:36Z
date available2017-06-09T14:21:36Z
date copyright1980/07/01
date issued1980
identifier issn0022-4928
identifier otherams-17950.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153901
description abstractModels of wave-CISK are developed that possess a prescribed form for the vertical profile of the diabatic heating due to a cumulus cloud ensemble, and either an explicit or an implicit moisture budget constraint. A comparison is undertaken of the models that do not have an explicit moisture budget constraint but differ in that the amplitude of the cloud-induced diabatic heating is related to the vertical velocity field at different height levels in the lower troposphere. The comparison reveals the essential equivalence of these models. The neutral eigenmodes demark the transition between stability and instability, and the one associated with the lowest amplitude for the diabatic heating is independent of the height of the forcing level. The only difference between these models is shown to be in the interpretation and specification of the diabatic heating amplitude. It is further shown that the same neutral eigenmode pertains at the instability-stability boundary for a wave-CISK model with an explicit moisture budget constraint. The results obtained in this case are used to assess the potential for CISK in the tropics by examining the efficiency that the cloud ensemble must exhibit to sustain neutral modes. Finally, the imposition of an Artificial rigid-lid upper boundary condition is shown to prevent the occurrence of the aforementioned mode and there is a concomitant stabilizing effect upon the flow.
publisherAmerican Meteorological Society
titleAn Ubiquitous Property of Simple Wave-CISK Models and Its Implications
typeJournal Paper
journal volume37
journal issue7
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1980)037<1437:AUPOSW>2.0.CO;2
journal fristpage1437
journal lastpage1446
treeJournal of the Atmospheric Sciences:;1980:;Volume( 037 ):;issue: 007
contenttypeFulltext


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