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Axisymmetric stability of the flow between two exactly counter-rotating disks with large aspect ratio

Published online by Cambridge University Press:  21 December 2005

L. MARTIN WITKOWSKI
Affiliation:
Université Paris VI, 4 place Jussieu, F-75252 Paris Cedex 05, France LIMSI-CNRS, UPR 3251, BP 133, F-91403 Orsay Cedex, France
I. DELBENDE
Affiliation:
Université Paris VI, 4 place Jussieu, F-75252 Paris Cedex 05, France LIMSI-CNRS, UPR 3251, BP 133, F-91403 Orsay Cedex, France
J. S. WALKER
Affiliation:
Department of Mechanical and Industrial Engineering, University of Illinois, 1206 W. Green St., Urbana, IL 61801, USA
P. LE QUÉRÉ
Affiliation:
LIMSI-CNRS, UPR 3251, BP 133, F-91403 Orsay Cedex, France

Abstract

We study the first bifurcation in the axisymmetric flow between two exactly counter-rotating disks with very large aspect ratio $ \Gamma\,{\equiv}\, R/H$, where $R$ is the disk radius and $2 H$ is the inter-disk spacing. The scaling law for the critical Reynolds number is found to be $\Rey_c \propto \Gamma^{-1/2}$, with $\Rey \,{\equiv}\, \Omega H^2/\nu$, $\Omega$ being the magnitude of the angular velocity and $\nu$ the kinematic viscosity. An asymptotic analysis for large $\Gamma$ is developed, in which curvature is neglected, but the centrifugal acceleration term is retained. The Navier–Stokes equations then reduce to leading order to those in a Cartesian frame, and the axisymmetric base flow to a parallel flow. This allows us locally to use a Fourier decomposition along the radial direction. In this framework, we explain the physical mechanism of the instability invoking the linear azimuthal velocity profile and the effect of centrifugal acceleration.

Type
Papers
Copyright
© 2005 Cambridge University Press

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