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contributor authorDickinson, Robert E.
date accessioned2017-06-09T14:14:40Z
date available2017-06-09T14:14:40Z
date copyright1968/11/01
date issued1968
identifier issn0022-4928
identifier otherams-15520.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151202
description abstractThe role of horizontal wind shears in the vertical propagation of planetary Rossby waves is investigated using an adiabatic linear model. We discuss wave guides formed by regions of weak westerly wind. If the wave guide is formed by trapping of waves between strong westerlies and/or the geometric poles, the ducting occurs as a wave propagation in discrete normal modes of the internal wave guide. On the other hand, for wave guides formed by one or more lines of zero wind, waves are absorbed rather than reflected at the zero wind line so that there are no normal modes of the wave guide. Disturbances excited in the lower stratosphere in the equatorial zero wind wave guide will terminate somewhere in the equatorial stratosphere, but eddy motions may be maintained in the tropics at higher levels by leakage from the Aleutian high planetary wave propagating vertically in a polar wave guide. The Aleutian high should he significantly attenuated by such leakage. The theory of zero wind line absorption suggests a planetary wave coupling with the biennial oscillation.
publisherAmerican Meteorological Society
titlePlanetary Rossby Waves Propagating Vertically Through Weak Westerly Wind Wave Guides
typeJournal Paper
journal volume25
journal issue6
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1968)025<0984:PRWPVT>2.0.CO;2
journal fristpage984
journal lastpage1002
treeJournal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 006
contenttypeFulltext


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