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contributor authorHayashi, Yoshikazu
date accessioned2017-06-09T14:22:18Z
date available2017-06-09T14:22:18Z
date copyright1981/06/01
date issued1981
identifier issn0022-4928
identifier otherams-18142.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4154115
description abstractIn order to explain why the Aleutian high stands out in the winter stratosphere, a complex Fourier analysis is made of simulated and observed stationary waves. It is found that in the troposphere the envelope of the time mean geopotential height consisting of wavenumbers 1 ? 3 attains its major and minor maxima in the Pacific and Atlantic, respectively. The major maximum is dominated by wavenumbers 1 ? 2 and shifts eastward with height in the stratosphere in the approximate direction of the group velocity and strengthens the Aleutian high. The minor maximum is dominated by wavenumber 3 and is confined in the troposphere.
publisherAmerican Meteorological Society
titleVertical-Zonal Propagation of a Stationary Planetary Wave Packet
typeJournal Paper
journal volume38
journal issue6
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1981)038<1197:VZPOAS>2.0.CO;2
journal fristpage1197
journal lastpage1205
treeJournal of the Atmospheric Sciences:;1981:;Volume( 038 ):;issue: 006
contenttypeFulltext


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