The thermal-convective instability in a stellar atmosphere with rotation and Hall effects

Details The thermal-convective instability in a stellar atmosphere with rotation and Hall effects The thermal-convective instability in a stellar atmosphere with rotation and Hall effects

Jun 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974znata..29..867s&link_type=abstract

Zeitschrift für Naturforschung, Teil a, vol. 29a, June 1974, p. 867-869.

Physics

1

Convective Flow, Hall Effect, Stellar Atmospheres, Stellar Magnetic Fields, Thermal Instability, Boundary Value Problems, Perturbation Theory, Roots Of Equations

Scientific paper

The problem of thermal-convective instability of a stellar atmosphere is
considered to include the effects due to rotation and Hall currents in
the presence of a uniform vertical magnetic field. The criterion for
monotonic instability is found to be unchanged by the presence of
rotation and Hall effects.

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