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The balance of magnetic fluxes in active regions

Published online by Cambridge University Press:  14 August 2015

Jan Olof Stenflo
Jan Olof Stenflo*
Affiliation:
Astronomical Observatory, Lund, Sweden

Extract

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According to modern theories of the solar cycle, active regions on the Sun are caused by a magnetic disturbance penetrating the solar surface from below. Sunspots, filaments, flares and other conspicuous events in an active region seem to be only secondary phenomena, the basic feature being the magnetic field itself.

Information

Type
Part I: General Development of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 47 - 49
Copyright
Copyright © Reidel 1968 

References

Grotrian, W., Künzel, H. (1950) Z. Astrophys., 28, 28.Google Scholar
Severny, A. B. (1967) Izv. Krym. astrofiz. Obs., 36, 22.Google Scholar
Steshenko, N. V. (1967) Izv. Krym. astrofiz. Obs., 37, 21.Google Scholar