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Collision of anticyclonic, lens‐like eddies with a meridional western boundary
Author(s) -
Sansón L. Zavala,
Graef F.,
Pavía E. G.
Publication year - 1998
Publication title -
journal of geophysical research: oceans
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/98jc02547
Subject(s) - eddy , zonal and meridional , anticyclone , geology , radius , latitude , mechanics , geophysics , physics , geometry , atmospheric sciences , geodesy , turbulence , mathematics , computer security , computer science
The collision of anticyclonic, lens‐like eddies with a meridional western boundary is investigated as a function of two independent, nondimensional numbers: β = β 0 R / f 0 and ε = ω/ f 0 , where f 0 and β 0 are the Coriolis parameter and its rate of change with latitude, respectively, both evaluated at the reference latitude. R is the eddy's radius, and ω is its angular frequency. The numerical experiments show that in all cases there is a southward expulsion of mass proportional to both β and ε. which is estimated during the eddy‐boundary interaction. The eddies are invariably deformed with the initial collision, but afterward, they reacquire a new circular shape. There is a meridional translation of the eddy along the boundary which depends exclusively on the initial ratio r = ε/β. If r >1, the eddy goes southward, but if r <1, the eddy goes northward first and then southward. As the eddy loses mass and reacquires a new circular shape, there is a readjustment of β and ε such that β decreases because its radius becomes smaller and ε increases by energy conservation. This implies that the eddies ultimately migrate southward. A formula, derived for the meridional speed of the center of mass of the eddy is consistent with the numerical results. A physical interpretation shows that after collision a zonal force is exerted on the eddy by the wall which is balanced by a meridional migration. Nonlinearities induce a southward motion, while high β values could produce northward motion, depending on the mass distribution along the wall.

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