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contributor authorBen Jelloul, Mahdi
contributor authorHuck, Thierry
date accessioned2017-06-09T14:55:59Z
date available2017-06-09T14:55:59Z
date copyright2003/11/01
date issued2003
identifier issn0022-3670
identifier otherams-29942.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4167225
description abstractThe selection mechanisms of Rossby basin modes are investigated in the reduced-gravity quasigeostrophic framework. The linear solution of the wind-driven circulation is decomposed in a steady forced?dissipated solution and a time-dependent component. The steady solution consists in a classical Sverdrup flow dissipated in a thin western boundary layer. The time-dependent solution is a sum of Rossby basin modes with arbitrary amplitudes. The effect of the nonlinear term is handled through a weakly nonlinear analysis providing a set of evolution equations for the mode amplitudes. It is shown both analytically (infinite Burger number) and numerically (finite Burger number) that mode stability is related to the gyre configuration. For cyclonic or anticyclonic single gyres, all basin modes are neutral. In the traditional (reversed) double-gyre case, large-scale basin modes are damped (unstable). Pure basin-mode interactions yield triads with cycling energy and subharmonic instabilities. The latter provide a potential mechanism for spectral reddening.
publisherAmerican Meteorological Society
titleBasin-Mode Interactions and Selection by the Mean Flow in a Reduced-Gravity Quasigeostrophic Model
typeJournal Paper
journal volume33
journal issue11
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(2003)033<2320:BIASBT>2.0.CO;2
journal fristpage2320
journal lastpage2332
treeJournal of Physical Oceanography:;2003:;Volume( 033 ):;issue: 011
contenttypeFulltext


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