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Global magnetic field cycle evolution and prominence eruptions

Published online by Cambridge University Press:  06 January 2014

Irina A. Bilenko
Irina A. Bilenko*
Affiliation:
Moscow M. V. Lomonosov State Univercity, Sternberg Astronomiczl Institute, Moscow, Russia email: bilenko@sai.msu.ru
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Abstract

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A comparison of changes in the structure of the global solar magnetic field and that in the prominence parameters, in solar cycles 21–23, are presented. It is proposed that the observed global magnetic field structure changes and periodicities in the mean solar magnetic field are the result of the excitation of large-scale Rossby waves. The changes in the prominence parameters are assumed to be the result of the global magnetic field structure changes, which may be triggered or modulated quasi-periodically by large-scale Rossby waves.

Keywords

magnetic fieldsprominencesoscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 168 - 171
Copyright
Copyright © International Astronomical Union 2013 

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