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contributor authorHart, J. E.
date accessioned2017-06-09T14:16:23Z
date available2017-06-09T14:16:23Z
date copyright1972/05/01
date issued1972
identifier issn0022-4928
identifier otherams-16167.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151920
description abstractA simple parallel flow model is derived for a thin (depth to length ratio ?1) Hadley circulation in a two-dimensional box with rigid horizontal boundaries maintained at a temperature which increases linearly with the horizontal coordinate x. Vertical velocities are assumed to he confined to narrow regions near the ends. The stability of this solution is discussed. Several modes of energy transfer to and from the mean kinetic and potential energies exist. As opposed to the case of thermal convection between isothermal plates in a constant shear, transverse disturbances with symmetry normal to the shear vector are always more unstable than longitudinal disturbances with symmetry parallel to the shear vector. Implications of these results for recent theoretical ideas on the Venusian circulation are discussed.
publisherAmerican Meteorological Society
titleStability of Thin Non-Rotating Hadley Circulations
typeJournal Paper
journal volume29
journal issue4
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1972)029<0687:SOTNRH>2.0.CO;2
journal fristpage687
journal lastpage697
treeJournal of the Atmospheric Sciences:;1972:;Volume( 029 ):;issue: 004
contenttypeFulltext


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