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Energy stability of the Ekman boundary layer

Published online by Cambridge University Press:  29 March 2006

Joseph J. Dudis
Affiliation:
The Johns Hopkins University, Baltimore, Maryland
Stephen H. Davis
Affiliation:
The Johns Hopkins University, Baltimore, Maryland

Abstract

The critical value RE of the Reynolds number R is predicted by the application of the energy theory. When R < RE, the Ekman layer is the unique steady solution of the Navier-Stokes equations and the same boundary conditions, and is, further, stable in a slightly weaker sense than asymptotically stable in the mean. The critical value RE is determined by numerically integrating the relevant Euler-Lagrange equations. An analytic lower bound to RE is obtained. Comparisons are made between RE and RL, the critical value of R according to linear theory, in order to demark the region of parameter space, RE < R < RL, in which subcritical instabilities are allowable.

Type
Research Article
Copyright
© 1971 Cambridge University Press

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References

Barcilon, V. 1965 Tellus, 17, 53.
Dudis, J. J. & Davis, S. H. 1970 J. Fluid Mech. 47, 381.
Faller, A. J. 1963 J. Fluid Mech. 15, 560.
Faller, A. J. & Kaylor, R. E. 1966 J. Atm. Sci. 23, 466.
Gill, A. E. & Davey, A. 1969 J. Fluid Mech. 35, 775.
Greenspan, H. P. 1968 The Theory of Rotating Fluids. Cambridge University Press.
Lilly, D. K. 1966 J. Atmos. Sci. 23, 481.
Tatro, P. R. & Mollö-Christensen, E. L. 1967 J. Fluid Mech. 28, 531.
Veronis, G. 1967 Tellus, 19, 326.