Magnetic-flux transport by a convecting layer – topological, geometrical and compressible phenomena
- 1 July 1983
- journal article
- research article
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 132, 25-48
- https://doi.org/10.1017/s0022112083001457
Abstract
Numerical calculations by Drobyshevski & Yuferev (1974) of the redistribution of magnetic flux by a Bénard layer with cells of square planform have been extended to higher values of electrical conductivity and to other velocity patterns, using a computer code developed for another purpose. Reconnection does not proceed as they supposed, but leads to overall field enhancement, and although the energy is greater at the bottom, there is as much unsigned flux in the upper half as in the lower half of the layer. However, compressible velocity patterns can concentrate flux at their bases.Keywords
This publication has 16 references indexed in Scilit:
- MagnetoconvectionReports on Progress in Physics, 1982
- The Present Status of Dynamo TheoryAnnual Review of Astronomy and Astrophysics, 1981
- Dynamically consistent nonlinear dynamos driven by convection in a rotating spherical shellThe Astrophysical Journal Supplement Series, 1981
- Convection and magnetic fields in starsThe Astrophysical Journal, 1981
- Alpha-effect in flux ropes and sheetsPhysics of the Earth and Planetary Interiors, 1979
- Non-linear properties of thermal convectionReports on Progress in Physics, 1978
- Magnetic field transfer by two-dimensional convection and solar ?semi-dynamo?Astrophysics and Space Science, 1977
- The escape of magnetic flux from a turbulent body of gasThe Astrophysical Journal, 1975
- Topological pumping of magnetic flux by three-dimensional convectionJournal of Fluid Mechanics, 1974
- The Structure of Sunspot Penumbras. II. Theoretical.The Astrophysical Journal, 1961