Horizontal dispersion of near-inertial oscillations in a turbulent mesoscale eddy field
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ID: 302296
2001
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Abstract
We study the dispersion of wind-induced near-inertial oscillations (NIOs) in a fully turbulent baroclinic mesoscale eddy eld characterized by a continuous wavenumber spectrum.The in uence of the eddy eld on the horizontal dispersion of the different NIO modes is analyzed using a vertical normal mode expansion.Previous studies have identi ed two dispersion regimes: trapping and strong dispersion.We examine the modes in physical and spectral space to assess which regime prevails.Numerical and analytical results show the prevalence of a trapping regime.For each NIO mode, there exists a critical horizontal wavenumber, k c , that separates large-scale NIO structures, where trapping dominates, from the much less energetic small-scale NIO structures, where strong dispersion dominates.The maximum ef ciency of dispersion for scales close to k c concentrates NIO kinetic energy at these scales.The wavenumber k c results from a balance between refraction and dispersion.This balance rst occurs at the highest wavenumber.Thereafter, k c , which has dimensional expression k c 2 5 p/( ftR m 2 ), decreases with time at a rate inversely proportional to the radius of deformation, R m , of the baroclinic NIO mode considered.As a consequence, at any given time, higher NIO baroclinic mode energy can mostly be found in small-scale negative vorticity structures, such as laments near sharp vorticity fronts, whereas lower NIO mode energy is concentrated within the core of mesoscale anticyclonic vortices.For large times, a saturation mechanism stops the time-evolution of k c at a value close to the peak of the kinetic energy spectrum of the QG ow eld.
| Reference Key |
openalex_W3209519559
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| Authors | Patrice Klein, Stefan G. Llewellyn Smith |
| Journal | journal of marine research |
| Year | 2001 |
| DOI |
10.1357/002224001762674908
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| URL | |
| Keywords | Keywords not found |
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