Physics
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220...37n&link_type=abstract
In ESA The Hydromagnetics of the Sun p 37-46 (SEE N85-25091 14-92)
Physics
11
Convection, Magnetohydrodynamics, Photosphere, Solar Atmosphere, Solar Magnetic Field, Atmospheric Stratification, Boussinesq Approximation, Chromosphere, Computerized Simulation, Solar Corona, Solar Physics
Scientific paper
The consensus about photosphere interaction of convection and magnetic fields is reviewed, especially the interaction of convection in the solar convection zone with magnetic fields on the scale of granulation and supergranulation. Computer simulations of Boussinesq systems are considered, and additional effects due to stratification and radiation are discussed. Mechanisms that determine the degree of evacuation of magnetic fields in the solar photosphere are treated, and limitations of the flux tube concept are pointed out. Results from numerical simulations of convection in a stratified medium with magnetic fields are examined, and possible consequences for activity in the chromosphere and corona are mentioned.
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