Physics
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..783p&link_type=abstract
(Astronomicheskii Zhurnal, vol. 61, July-Aug. 1984, p. 783-788) Soviet Astronomy (ISSN 0038-5301), vol. 28, July-Aug. 1984, p. 4
Physics
4
Dynamo Theory, Solar Activity, Solar Cycles, Solar Magnetic Field, Solar Physics, Finite Difference Theory, Interplanetary Medium, Photosphere
Scientific paper
The influence of a hypothetical, quasi-steady primary field of the sun on the behavior of solar activity and the background magnetic field during the 22-year solar cycle is considered. It is shown that allowance for the primary solar field in Leighton's model makes it possible to explain the main regularities of behavior of the surface magnetic field of the sun and the solar activity during the 22-year cycle. These regularities are confirmed by a direct comparison with experimental results. The possibility in principle of experimentally detecting the internal field of the sun and estimating its parameters from its manifestations in the surface layers is thereby demonstrated.
Benevolenskaya Elena E.
Pudovkin Mikhail I.
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