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Steady turbulent density currents on a slope in a rotating fluid

Published online by Cambridge University Press:  02 April 2014

G. E. Manucharyan*
Affiliation:
Yale University, New Haven, CT 06520, USA
W. Moon
Affiliation:
Yale University, New Haven, CT 06520, USA
F. Sévellec
Affiliation:
Yale University, New Haven, CT 06520, USA University of Southampton, Southampton SO14 3ZH, UK
A. J. Wells
Affiliation:
Yale University, New Haven, CT 06520, USA University of Oxford, Oxford OX1 3PU, UK
J.-Q. Zhong
Affiliation:
Yale University, New Haven, CT 06520, USA Tongji University, Shanghai 200092, PR China
J. S. Wettlaufer
Affiliation:
Yale University, New Haven, CT 06520, USA University of Oxford, Oxford OX1 3PU, UK
*
Email address for correspondence: [email protected]

Abstract

We consider the dynamics of actively entraining turbulent density currents on a conical sloping surface in a rotating fluid. A theoretical plume model is developed to describe both axisymmetric flow and single-stream currents of finite angular extent. An analytical solution is derived for flow dominated by the initial buoyancy flux and with a constant entrainment ratio, which serves as an attractor for solutions with alternative initial conditions where the initial fluxes of mass and momentum are non-negligible. The solutions indicate that the downslope propagation of the current halts at a critical level where there is purely azimuthal flow, and the boundary layer approximation breaks down. Observations from a set of laboratory experiments are consistent with the dynamics predicted by the model, with the flow approaching a critical level. Interpretation in terms of the theory yields an entrainment coefficient $E\propto 1/\Omega $ where the rotation rate is $\Omega $. We also derive a corresponding theory for density currents from a line source of buoyancy on a planar slope. Our theoretical models provide a framework for designing and interpreting laboratory studies of turbulent entrainment in rotating dense flows on slopes and understanding their implications in geophysical flows.

Type
Papers
Copyright
© 2014 Cambridge University Press 

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