The theory of solar activity

Details The theory of solar activity The theory of solar activity

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980izssr..44.2560g&link_type=abstract

(Seminar po Vzaimodeistviiu Kosmicheskikh Luchei so Sredoi, Leningrad, USSR, Nov. 30-Dec. 2, 1979.) Akademiia Nauk SSSR, Izvesti

Astronomy and Astrophysics

Astronomy

Dynamo Theory, Solar Activity, Solar Magnetic Field, Solar Wind, Astronomical Models, Magnetic Field Configurations, Plasma Turbulence, Solar Cycles

Scientific paper

A solar dynamo model is developed which takes into account the relationship between global and local magnetic fields. It is shown that the model can explain certain aspects of solar activity. In particular, local magnetic fields intensified by convection cells can be the cause of sunspot groups. The basic features of the dynamo model are in accord with the features of the solar cycle: i.e., the model indicates changes of the sign of background fields in polar regions in each 11-year cycle, as well as a correlation between spot-forming activity and toroidal fields (whose existence in subphotospheric layers is highly probable).

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