Physics – Fluid Dynamics
Scientific paper
Oct 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984gapfd..30..227f&link_type=abstract
Geophysical and Astrophysical Fluid Dynamics (ISSN 0309-1929), vol. 30, Oct. 1984, p. 227-239. Research supported by the Science
Physics
Fluid Dynamics
29
Annuli, Magnetohydrodynamic Stability, Magnetohydrodynamic Waves, Rotating Fluids, Eigenvectors, Field Strength, Momentum
Scientific paper
The results of a detailed numerical investigation of the properties of the resistive mode of instabilities in a differentially rotating toroidal magnetic field are presented. A variety of different magnetic field strengths are considered in order to isolate the key ingredient for instability. A solution is found for a series of equations which represents the theoretical limit to the resistivity. It is concluded that the resistivity of the instabilities is real and that it is probably similar to resistive instabilities encountered in plasma physics problems.
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