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contributor authorHayashi, V.
contributor authorGolder, D. G.
date accessioned2017-06-09T14:23:48Z
date available2017-06-09T14:23:48Z
date copyright1983/04/01
date issued1983
identifier issn0022-4928
identifier otherams-18552.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4154570
description abstractSpace-time spectral analysis over a three year data set is made of transient planetary waves simulated by Geophysical Fluid Dynamics Laboratory (GFDL) spectral general circulation models with and without mountains. In both models westward moving ultralong waves have larger geopotential amplitude than eastward moving ultralong waves, being in agreement with observations. In both models westward moving ultralong waves are associated with little vertical tilt and a large meridional wavelength, while eastward moving ultralong waves are associated with some vertical tilt and a small meridional wavelength. In the absence of mountains westward moving ultralong waves are somewhat decreased, while eastward moving ultralong waves are somewhat increased, and eastward moving wavenumber 4?6 components are markedly increased in the Northern Hemisphere.
publisherAmerican Meteorological Society
titleTransient Planetary Waves Simulated by GFDL Spectral General Circulation Models. Part I: Effects of Mountains
typeJournal Paper
journal volume40
journal issue4
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1983)040<0941:TPWSBG>2.0.CO;2
journal fristpage941
journal lastpage950
treeJournal of the Atmospheric Sciences:;1983:;Volume( 040 ):;issue: 004
contenttypeFulltext


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