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contributor authorThompson, Rory O. R. Y.
date accessioned2017-06-09T14:21:32Z
date available2017-06-09T14:21:32Z
date copyright1980/06/01
date issued1980
identifier issn0022-4928
identifier otherams-17928.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153876
description abstractWaves are forced by moving sources and sinks of mass on a beta-plane with Ekman friction. If the motion is retrograde and not too fast, these are Rossby waves with a nonzero Reynolds stress u?v??. This stress forces a meridional mass flux which builds up a pressure gradient to allow a compensating mass flux in the Ekman layer. In a rotating system, this meridional pressure gradient requires a zonal flow u?(y)=??/?y(u?v??)/E½Ω,which is also the momentum accumulated by the Reynolds stress in one spindown time. An example shows how excitation of Rossby waves brings momentum into the source of energy, causing a prograde jet there, with retrograde currents on each side. A laboratory experiment confirms the theory, which is proposed as an explanation of the observed ?negative viscosity? of the jet stream in the atmosphere and the Gulf Stream in the ocean.
publisherAmerican Meteorological Society
titleA Prograde Jet Driven by Rossby Waves
typeJournal Paper
journal volume37
journal issue6
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1980)037<1216:APJDBR>2.0.CO;2
journal fristpage1216
journal lastpage1226
treeJournal of the Atmospheric Sciences:;1980:;Volume( 037 ):;issue: 006
contenttypeFulltext


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