Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-19T08:49:24.157Z Has data issue: false hasContentIssue false

The ‘sliced-cylinder’ laboratory model of the wind-driven ocean circulation. Part 1. Steady forcing and topographic Rossby wave instability

Published online by Cambridge University Press:  29 March 2006

R. C. Beardsley
Affiliation:
Department of Meteorology, Massachusetts Institute of Technology, Cambridge
K. Robbins
Affiliation:
Department of Meteorology, Massachusetts Institute of Technology, Cambridge

Abstract

The nonlinear response of the ‘sliced-cylinder’ laboratory model for the wind-driven ocean circulation is re-examined here in part 1 for the case of strong steady forcing. Introduced by Pedlosky & Greenspan (1967), the model consists of a rapidly rotating right cylinder with a planar sloping bottom. The homogeneous contained fluid is driven by the slow rotation of the flat upper lid relative to the rest of the basin. Except in thin Ekman and Stewartson boundary layers on the solid surfaces of the basin, the horizontal flow in the interior and western boundary layer is constrained by the rapid rotation of the basin to be independent of depth. The model thus effectively simulates geophysical flows through the physical analogy between topographic vortex stretching in the laboratory model and the creation of relative vorticity in planetary flows by the β effect.

As the forcing is increased, the flow in both the sliced-cylinder laboratory and numerical models first exhibits downstream intensification in the western boundary layer. At greater forcing, separation of the western boundary current occurs with the development of stationary topographic Rossby waves in the western boundary-layer transition regions. The observed flow ultimately becomes unstable when a critical Ekman-layer Reynolds number is exceeded. We first review and compare the experimental and numerical descriptions of this low-frequency instability, then present a simple theoretical model which successfully explains this observed instability in terms of the local breakdown of the finite-amplitude topographic Rossby waves embedded in the western boundary current transition region. The inviscid stability analysis of Lorenz (1972) is extended to include viscous effects, with the consequence that dissipative processes in the sliced-cylinder problem (i.e. lateral and bottom friction) are shown to inhibit the onset of the instability until the topographic Rossby wave slope exceeds a finite critical value.

Type
Research Article
Copyright
© 1975 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Beardsley, R. C. 1969 A laboratory model of the wind-driven ocean circulation J. Fluid Mech. 38, 255.Google Scholar
Beardsley, R. C. 1973a A numerical model of the wind-driven ocean circulation in a circular basin. Geophys. Fluid Dyn. 4, 211.Google Scholar
Beardsley, R. C. 1973b A numerical investigation of a laboratory analogy of the wind-driven ocean circulation. Proc. 1972 NAS Symp. on Numerical Models of Ocean Circulation.Google Scholar
Bryan, K. 1963 A numerical investigation of a nonlinear model of a wind-driven ocean J. Atmos. Sci. 20, 596.Google Scholar
Gill, A. 1974 Stability of planetary waves Geophys. Fluid Dyn. 6, 29.Google Scholar
Greenspan, H. P. 1968 The Theory of Rotating Fluids. Cambridge University Press.
Greenspan, H. P. 1969 A note on the laboratory simulation of planetary flows Studies in Appl. Math. 48, 147.Google Scholar
Israeli, M. 1970 A fast implicit numerical method for time dependent viscous flows Studies in Appl. Math., 49, 327.Google Scholar
LONGUET-HIGGINS, M. S. & Gill, A. E. 1967 Resonant interactions between planetary waves. Proc. Roy. Soc A 299, 120140.Google Scholar
Lorenz, E. N. 1972 Barotropic instability of Rossby wave motion J. Atmos. Sci. 29, 258.Google Scholar
Munk, W. H. 1950 On the wind-driven ocean circulation J. Meteor. 7, 7993.Google Scholar
Orszag, S. & Israeli, M. 1972 Numerical flow simulation by spectral methods. Proc. 1972 NAS Symp. on Numerical Models of Ocean Circulation.Google Scholar
Pearson, C. E. 1965 A computational method for viscous flow problems J. Fluid Mech. 21, 611.Google Scholar
Pedlosky, J. & Greenspan, H. P. 1967 A simple laboratory model for the oceanic circulation J. Fluid Mech. 27, 291.Google Scholar
Stommel, H. 1948 The westward intensification of wind-driven ocean currents Trans. Am. Geophys. Un. 29, 202.Google Scholar
Sverdrup, H. 1947 Wind-driven currents in a baroclinic ocean Proc. Nat. Acad. Sci. 33, 318.Google Scholar