Omicron-Stability Analysis of Hydromagnetic Instabilities in Stars with Toroidal Magnetic Fields

Details Omicron-Stability Analysis of Hydromagnetic Instabilities in Stars with Toroidal Magnetic Fields Omicron-Stability Analysis of Hydromagnetic Instabilities in Stars with Toroidal Magnetic Fields

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..667g&link_type=abstract

Space Science Reviews, Volume 27, Issue 3-4, pp. 667-672

Physics

1

Scientific paper

σ-stability analysis is used to investigate the adiabatic stability of a star containing an axisymmetric toroidal magnetic field. Necessary and sufficient conditions for σ-stability are derived. Special attention is devoted to the typical hydromagnetic instabilities that can be introduced by a weak toroidal magnetic field in a star that is stably stratified in the absence of any magnetic field. An expression for the maximum growth rate of instability is derived and the basic properties of the displacement fields associated with the instabilities are indicated.

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