Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976aujph..29..305v&link_type=abstract
Australian Journal of Physics, vol. 29, Aug. 1976, p. 305-310.
Astronomy and Astrophysics
Astrophysics
1
Convective Flow, Free Convection, Solar Atmosphere, Solar Magnetic Field, Solar Rotation, Astrophysics, Atmospheric Stratification, Current Density, Equations Of Motion, Rayleigh Number, Time Dependence, Vorticity
Scientific paper
Two different stationary solutions have been found for the basic equations describing finite amplitude convection in a rotating medium in the presence of a magnetic field. One of these displays strong convective motions, whereas the other is characterized by a marked increase in the vorticity and current density with Rayleigh number. The nature of the initial disturbance would ultimately decide which solution would become established, and a numerical investigation of this problem would require the solution of the time-dependent equations.
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