Physics
Scientific paper
Nov 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..948..309b&link_type=abstract
UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP Conference Proceedings, Volume 948, pp. 309-3
Physics
Stellar Rotation, Electric And Magnetic Fields, Solar Magnetism, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Solar Interior
Scientific paper
We construct models of the structure and evolution of the Sun which include rotation and magnetic fields. The effects of rotation are to generate magnetic fields, redistribute magnetic angular momentum in the solar interior and to mix the elements. The effects of the magnetic fields are the corrections to the thermodynamics variables. We investigate mainly the correlation between the interior rotational properties and magnetic fields inside the Sun. We find that the magnetic fields in the solar interior are strongly affected by the rotation rate and gradient.
Bi Shaolan
Yang Wuming
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