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Nonlinear adjustment of density fronts. Part 1. The Rossby scenario and the experimental reality

Published online by Cambridge University Press:  01 March 2004

A. STEGNER
Affiliation:
Laboratoire de Météorologie Dynamique, IPSL, ENS, 24 Rue Lhomond, 75005 Paris, Francestegner@lmd.ens.fr
P. BOURUET-AUBERTOT
Affiliation:
Laboratoire d'Océanographie Dynamique et Climatologique, IPSL, Université Pierre et Marie Curie, Jussieu, 75252 Paris Cedex 05, Francepba@lodyc.jussieu.fr
T. PICHON
Affiliation:
UME, ENSTA Centre de l'Yvette, Chemin de la huniere, 91120 Palaiseau Cedex, France

Abstract

This study deals with the nonlinear cyclo-geostrophic adjustment of a circular density front in a two-layer fluid. Laboratory experiments have been performed to investigate the dynamical evolution of a fixed volume of buoyant water, initially confined within a bottomless cylinder, which is quickly released in a dense rotating fluid. This configuration corresponds to a rapid input of potential energy in a geostrophic fluid layer and reproduces some dynamical processes which occur during oceanic upwelling or stratospheric warming events. We focus our efforts on the visualization techniques in order to have simultaneous and independent measurements of both the horizontal velocity field and the vertical density field. We thus obtained, for the first time, quantitative measurements of the potential vorticity and the flow balance after a geostrophic adjustment process. The density profile of the mean adjusted state observed in the experiment is in good agreement with the prediction of the standard adjustment theory based on Lagrangian conservation of potential vorticity except in the frontal region. There, strong three-dimensional motions (plume structures, shocks and rapid transient instabilities) take place during the early stage of adjustment. These transient three-dimensional motions could dissipate up to 50% of the initial energy of the system, especially when the size of the initial density anomaly is close to or larger than the deformation radius. Therefore, it significantly changes the velocity and the energy budget predicted by the standard Rossby adjustment. Both the kinetic energy of the mean adjusted state and the energy transferred to inertia–gravity wave modes are reduced by these transient dissipative processes.

Type
Papers
Copyright
© 2004 Cambridge University Press

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