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contributor authorKillworth, Peter D.
contributor authorBlundell, Jeffrey R.
date accessioned2017-06-09T14:56:08Z
date available2017-06-09T14:56:08Z
date copyright2003/04/01
date issued2003
identifier issn0022-3670
identifier otherams-29982.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4167269
description abstractRay theory is used to predict phase and group velocities for long planetary waves under realistic, albeit slowly varying, oceanic conditions. The results are compared with local theory using fields smoothed to the same amount (9° latitude/longitude) as well as those with much less smoothing (1°). The agreement is excellent, showing that local theory forms a good proxy for ray theory results. The predicted speeds agree well with observations of planetary waves deduced from sea surface height data. The theory uses purely baroclinic mean flow; the inclusion of barotropic flow has little effect except at high latitudes.
publisherAmerican Meteorological Society
titleLong Extratropical Planetary Wave Propagation in the Presence of Slowly Varying Mean Flow and Bottom Topography. Part II: Ray Propagation and Comparison with Observations
typeJournal Paper
journal volume33
journal issue4
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(2003)33<802:LEPWPI>2.0.CO;2
journal fristpage802
journal lastpage821
treeJournal of Physical Oceanography:;2003:;Volume( 033 ):;issue: 004
contenttypeFulltext


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