Statistics – Computation
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1057r&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Sept.-Oct. 1987, p. 1057-1065. In Russian.
Statistics
Computation
7
Computational Astrophysics, Dynamo Theory, Solar Magnetic Field, Solar Rotation, Angular Velocity, Asymptotic Methods
Scientific paper
An analytical solution of the mean-field solar dynamo equations is obtained. The asymptotic method used allows the finding of the basic features of magnetic fields, excited as dynamo-waves under arbitrary angular velocities of rotation. The dynamo-wave migrates along the surfaces close to the isorotational ones. The maximum of its amplitude is shifted from the location of maximum intensity of the sources in the direction of migration. Generally, there are two dynamo-waves on the solar surface, diverging from a certain latitude towards the pole and the equator. The first one is weakened, and the other is more intense. From the observed surface fields, the regions of field generation are localized; the conditions are imposed on the distribution of the rotational angular velocity in these regions, which agree with the modern helioseismology data.
Ruzmajkin A. A.
Starchenko Sergey V.
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