An experimental and theoretical investigation of the onset of convection in rotating spherical shells

Author:

Carrigan C. R.,Busse F. H.

Abstract

Convection in a rapidly rotating spherical layer with constant-temperature boundary conditions is studied in a laboratory experiment. The asymptotic theory of Busse (1970) is extended to permit a comparison with the observations of the onset of convection and its properties. It is found that the prediction of the power-law dependences of the critical buoyancy number and the critical wavenumber on the rotation rate are borne out, although discrepancies in the actual values of these quantities do exist. Calculations on the basis of equations proposed by Roberts (1968) show that a thermal wind that is present in the basic state of the model has a stabilizing influence on the onset of convection. Stewartson layers not taken into account in the asymptotic analysis for vanishing Ekman number E appear to be responsible for the remaining disagreement between theoretical predictions and observations at finite values of E.

Publisher

Cambridge University Press (CUP)

Subject

Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics

Reference9 articles.

1. Busse, F. H. & Cuong, P. G. 1977 Convection in rapidly rotating spherical fluid shells Geophys. Astrophys. Fluid Dyn. 8,17–44.

2. Soward, A. M. 1977 On the finite amplitude thermal instability of a rapidly rotating fluid sphere Geophys. Astrophys. Fluid Dyn. 9,19–74.

3. Busse, F. H. & Carrigan, C. R. 1976 Laboratory simulation of thermal convection in rotating planets and stars Science 191,81–83.

4. Gilman, P. A. 1976 Theory of convection in a deep rotating spherical shell and its application to the Sun. In Proc. IAU Symp. no. 71. Basic Mechanisms of Solar Activity (ed. V. Bumba & J. Kleczek ),pp.207–228.Reidel.

5. Busse, F. H. 1970 Thermal instabilities in rapidly rotating systems J. Fluid Mech. 44,441–460.

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