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contributor authorThompson, Luanne
contributor authorYoung, W. R.
date accessioned2017-06-09T14:49:07Z
date available2017-06-09T14:49:07Z
date copyright1989/02/01
date issued1989
identifier issn0022-3670
identifier otherams-27466.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4164474
description abstractLaboratory experiments show that ageostrophic instability can ?break up? a parallel flow into a sequence of axisymmetric eddies. This is a plausible scenario for the generation of sub-mesoscale coherent Vortices (SCVs). Here we show that conservation of mass, energy and potential vorticity enables one to very simply calculate the radius of the axisymmetric eddy and the wavelength of the nonlinear instability. The latter agrees more closely with laboratory experiments than does the wavelength predicted by linearized stability theory. It energy is not conserved, say because of wave radiation into the lower layer, then the preceding calculation establishes an upper bound on the radius of the eddy. We offer this as an explanation of the observed small size of SCVs.
publisherAmerican Meteorological Society
titleAn Upper Bound on the Size of Sub-mesoscale Coherent Vortices
typeJournal Paper
journal volume19
journal issue2
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(1989)019<0233:AUBOTS>2.0.CO;2
journal fristpage233
journal lastpage237
treeJournal of Physical Oceanography:;1989:;Volume( 019 ):;issue: 002
contenttypeFulltext


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