Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..525z&link_type=abstract
(Advanced School of Astronomy, Course on the Sun, a Tool for Stellar Physics, 6th, Erice, Italy, Aug. 8-21, 1976.) Società Astro
Astronomy and Astrophysics
Astronomy
18
Magnetic Field Configurations, Photosphere, Solar Atmosphere, Solar Magnetic Field, Stellar Atmospheres, Stellar Magnetic Fields, Convective Flow, Dynamo Theory, Fine Structure, Stellar Rotation, Stellar Structure, Sunspots, Velocity Distribution
Scientific paper
Following a review of the principal observational data on the magnetic structures in the solar photosphere and low chromosphere, some simple models are examined which provide a semi-quantative interpretation of the observed structures. The interplay between the magnetic field and the velocity fields (rotation, convection), is examined, along with its role in the emergence and redistribution of magnetic flux over the solar surface. The magnetic structure to be expected in stars with convective zones is studied, along with the observational indications for stellar magnetic activity.
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