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The polar belts of prominence occurence as an indicator of the solar magnetic field reversal

Published online by Cambridge University Press:  06 January 2014

Teodor Pintér ,
Milan Rybanský  and
Ivan Dorotovič
Teodor Pintér
Affiliation:
Slovak Central Observatory, Komárňanská 134, SK-94701 Hurbanovo, Slovak Republic email: [email protected], [email protected], [email protected]
Milan Rybanský
Affiliation:
Slovak Central Observatory, Komárňanská 134, SK-94701 Hurbanovo, Slovak Republic email: [email protected], [email protected], [email protected]
Ivan Dorotovič
Affiliation:
Slovak Central Observatory, Komárňanská 134, SK-94701 Hurbanovo, Slovak Republic email: [email protected], [email protected], [email protected]
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Abstract

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The global magnetic field of the Sun is the determining parameter of spreading the solar wind in the interplanetary space. The global field changes the polarity synchronically with the cycle of solar activity. The interesting indicator of the polarity change are the occurence so-called polar belts of the prominences. The article shows the performance of these belts on observational work from 1975 to 2009. A coordinated effort is suggested for the compilation of data from different observers following the method described by Rušin et al., 1988.

Keywords

Prominence occurencepolar beltssolar magnetic field reversal
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. 456 - 457
Copyright
Copyright © International Astronomical Union 2013 

References

Rušin, V., Rybanský, M., Dermendjiev, V., & Stavrev, K. Y. 1988, Contrib. Astron. Obs. Skalnaté Pleso, 17, 63Google Scholar
Svalgaard, L., Duvall, T. L. jr., & Scherrer, P. H. 1978, Solar Phys., 58, 225CrossRefGoogle Scholar