Thermal-convective instability of a composite rotating stellar atmosphere in the presence of a variable magnetic field

Details Thermal-convective instability of a composite rotating stellar atmosphere in the presence of a variable magnetic field Thermal-convective instability of a composite rotating stellar atmosphere in the presence of a variable magnetic field

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.143..241s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 143, no. 2, April 1988, p. 241-247.

Astronomy and Astrophysics

Astrophysics

2

Convective Heat Transfer, Magnetohydrodynamic Stability, Stellar Atmospheres, Stellar Magnetic Fields, Stellar Rotation, Thermal Instability, Atmospheric Temperature, Buoyancy, Magnetic Field Configurations, Temperature Gradients

Scientific paper

The thermal-convective instability of a composite stellar atmosphere is
considered in the presence of rotation, variable horizontal magnetic
field, and collisional effects. The criteria for monotonic instability
are obtained which generalize the criterion derived for
thermal-convective instability in the absence of above effects.

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