Convection in an imposed magnetic field. Part 1. The development of nonlinear convection

Author:

Weiss N. O.

Abstract

Nonlinear two-dimensional magnetoconvection in a Boussinesq fluid has been studied in a series of numerical experiments with values of the Chandrasekhar number Q ≤ 4000 and the ratio ζ of the magnetic to the thermal diffusivity in the range 1 ≥ ζ ≥ 0·025. If the imposed field is strong enough, convection sets in as overstable oscillations which give way to steady convection as the Rayleigh number R is increased. In the dynamical regime that follows, magnetic flux is concentrated into sheets at the sides of the cells, from which the motion is excluded.

Publisher

Cambridge University Press (CUP)

Subject

Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics

Reference37 articles.

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2. Clark, A. & Johnson, A. C. 1967 Magnetic field accumulation in supergranules.Solar Phys. 2,433–440.

3. Galloway, D. J. & Weiss, N. O. 1981 Convection and magnetic fields in stars.Astrophys. J. 243,945–953.

4. Proctor, M. R. E. & Weiss, N. O. 1978 Magnetic flux ropes. In Rotating Fluids in Geophysics (ed. P. H. Roberts & A. M. Soward ),pp.389–408.Academic.

5. Busse, F. H. 1975 Nonlinear interaction of magnetic field and convection.J. Fluid Mech. 71,193–206.

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