Convection in an imposed magnetic field. Part 1. The development of nonlinear convection
- 1 July 1981
- journal article
- research article
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 108, 247-272
- https://doi.org/10.1017/s0022112081002115
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.Keywords
This publication has 17 references indexed in Scilit:
- Convection and magnetic fields in starsThe Astrophysical Journal, 1981
- Magnetic flux ropes and convectionJournal of Fluid Mechanics, 1978
- Nonlinear interaction of magnetic field and convectionJournal of Fluid Mechanics, 1975
- Difference methods for time-dependent two-dimensional convectionComputer Physics Communications, 1973
- Two-dimensional Rayleigh-Benard convectionJournal of Fluid Mechanics, 1973
- Some Kinematical Models for Small-Scale Solar Magnetic FieldsPhysics of Fluids, 1966
- Kinematical Hydromagnetic Theory and its Application to the Low Solar Photosphere.The Astrophysical Journal, 1963
- The Structure of Sunspot Penumbras. II. Theoretical.The Astrophysical Journal, 1961
- Cellular convection with finite amplitude in a rotating fluidJournal of Fluid Mechanics, 1959
- Finite amplitude cellular convectionJournal of Fluid Mechanics, 1958