On thermal-convective instability in a stellar atmosphere with finite Larmor radius and Hall effects

Details On thermal-convective instability in a stellar atmosphere with finite Larmor radius and Hall effects On thermal-convective instability in a stellar atmosphere with finite Larmor radius and Hall effects

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..31...43s&link_type=abstract

Astrophysics and Space Science, vol. 31, Nov. 1974, p. 43-47.

Astronomy and Astrophysics

Astrophysics

1

Convective Heat Transfer, Hall Effect, Magnetohydrodynamic Stability, Stellar Atmospheres, Stellar Rotation, Thermal Instability, Larmor Precession, Magnetic Field Configurations, Perturbation Theory, Stellar Magnetic Fields

Scientific paper

The thermal-convective instability of a stellar atmosphere is considered
to include rotation, finite Larmor radius and Hall effects in the
presence of a uniform vertical magnetic field. The criterion for
monotonic instability is found to be the same even if the above effects
are included

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