Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..65..453a&link_type=abstract
Astrophysics and Space Science, vol. 65, no. 2, Oct. 1979, p. 453-458.
Astronomy and Astrophysics
Astrophysics
6
Convective Flow, Flat Layers, Magnetohydrodynamic Flow, Rotating Fluids, Thermal Diffusivity, Thermal Instability, Field Strength, Magnetic Fields, Magnetohydrodynamic Stability, Rayleigh Number, Rotating Plasmas, Thermal Conductivity, Two Dimensional Flow
Scientific paper
This paper explores the thermal instability of a plane fluid layer rotating rapidly about a vertical axis in the presence of a uniform vertical magnetic field. The thermal diffusivity is taken to be large compared with the magnetic diffusivity. For a range of parameters it is shown that an increase of the magnetic field leads to a decrease in the critical Rayleigh number, and two quite distinct physical mechanisms appear to be involved.
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