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contributor authorBenzi, Roberto
contributor authorMalguzzi, Piero
date accessioned2017-06-09T14:30:59Z
date available2017-06-09T14:30:59Z
date copyright1992/09/01
date issued1992
identifier issn0022-4928
identifier otherams-20744.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4157006
description abstractThe problem of resonance and meridional confinement of planetary-scale waves is investigated in the framework of a quasigeostrophic, two-layer, ?-plane model with lateral sponge layers. It is shown that the model resonant wavenumber is meridionally confined despite the predictions of the linear barotropic theory based on the time-mean zonal wind. As a consequence, the fully nonlinear model exhibits a resonant response to orographic forcing significantly higher than that predicted by the linearized (baroclinic) version of the model itself.The model response to a localized (zonally and meridionally) orography is also studied and found to be consistent with previous results observed in spherical geometry. The significance of this result and the mechanisms leading to meridional confinement are discussed. It is suggested that nonlinearity and the inverse energy cascade process are responsible for the observed, enhanced wave confinement.
publisherAmerican Meteorological Society
titleAmplification and Meridional Confinement of Stationary and Quasi-stationary Eddies in a Two-Layer Model
typeJournal Paper
journal volume49
journal issue17
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1992)049<1585:AAMCOS>2.0.CO;2
journal fristpage1585
journal lastpage1593
treeJournal of the Atmospheric Sciences:;1992:;Volume( 049 ):;issue: 017
contenttypeFulltext


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