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Fast Wind-Induced Migration of Leddies in the South China Sea
Author(s) -
Doron Nof,
Yinglai Jia,
Eric P. Chassignet,
Alexandra Bozec
Publication year - 2011
Publication title -
journal of physical oceanography
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.706
H-Index - 143
eISSN - 1520-0485
pISSN - 0022-3670
DOI - 10.1175/2011jpo4530.1
Subject(s) - eddy , geology , drag coefficient , geophysics , vorticity , radius , drag , mechanics , meteorology , atmospheric sciences , physics , vortex , turbulence , computer security , computer science
Eddies off the Strait of Luzon (termed here as "Leddies," analogous to "Teddies" originating from the Indonesian Throughflow) are formed rapidly and migrate swiftly. Their migration rate (~10-20 cm s-1) is an order of magnitude faster than that of most eddies of the same scale (~1 cm s-1). Onthe basis of observations, it has been suggested earlier that the rapid generation process is due to the southeast monsoon. Here, the authors place this earlier suggestion on a more solid ground by developing both analytical and process-oriented numerical models. Because the eddies are formed by the injection of foreign, lighter Kuroshio water into the South China Sea (SCS), the eddies are modeled as lenses: that is, "bullets" that completely encapsulate the mass anomaly associated with them. It turns out that the rings migrate at an angle α (between 0° and 90°) to the right of the wind direction fi.e., tan-1[(2-γ)f2R/8g'CD], where in conventional notation γ is the vorticity, R the eddy radius, and CD the interfacial friction coefficient along the lower interface of the lensg. Their fast migration speed is given by 2(τS/ρW)(sina)/fH, where τS is the wind stress on the surface, ρw the water density, and H is the maximum eddy depth. With high interfacial drag (i.e., large CD), the rings move relatively slowly (but still a lot faster than Rossby waves) in the wind direction, whereas with low drag they move fast at 90° to the right. These analytically predicted values are in good agreement with isopycnic numerical simulations. © 2011 American Meteorological Society.

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