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Solar Cycle in Photosphere and Corona

Published online by Cambridge University Press:  14 March 2005

Elena E. Benevolenskaya
Elena E. Benevolenskaya
Affiliation:
Stanford University, Stanford, CA 94305, USA email: [email protected] Pulkovo Astronomical Observatory, St. Petersburg, Russia
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Abstract

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The solar cycle in photosphere and corona reflects the internal dynamics on the Sun. According to the modern understanding the observed behavior of solar activity is related to the dynamo process in convection zone and photosphere and it is closely connected with the evolution of the coronal structures. The observational data from ground and space allow us to investigate the solar cycle as a complex phenomenon and to clarify the most important features such as polar magnetic field reversals, non-uniform distributions of the solar activity complexes and fine structure of the solar cycle.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 33 - 40
Copyright
© 2004 International Astronomical Union