Show simple item record

contributor authorStone, P. H.
date accessioned2017-06-09T14:14:50Z
date available2017-06-09T14:14:50Z
date copyright1969/05/01
date issued1969
identifier issn0022-4928
identifier otherams-15594.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151283
description abstractThe two-layer model is used to study how horizontal shear in a baroclinic zonal flow affects the structure of growing baroclinic waves. The solution is simplified by assuming that the radius of deformation is small compared to the planetary scale. The method of solution yields results for waves near neutral stability. For these waves, solutions are found for many different wind profiles. These solutions show: 1) that the waves have a natural meridional scale equal to the radius of deformation, the same as the zonal scale; 2) that the wave perturbation in the lower atmosphere is primarily confined to regions where the vertical shear of the unperturbed zonal flow is greatest; and 3) the horizontal eddy stresses always transport momentum against the horizontal gradient of the zonal flow. Thus, the baroclinic waves tend to increase the intensity of any jets present in the unperturbed zonal flow, no matter what their number or position, and they are accompanied by horizontal shearing and stretching deformation wind fields which are of comparable strength.
publisherAmerican Meteorological Society
titleThe Meridional Structure of Baroclinic Waves
typeJournal Paper
journal volume26
journal issue3
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1969)026<0376:TMSOBW>2.0.CO;2
journal fristpage376
journal lastpage389
treeJournal of the Atmospheric Sciences:;1969:;Volume( 026 ):;issue: 003
contenttypeFulltext


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record