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Solar cycle 23 analysis

Published online by Cambridge University Press:  14 March 2005

Georgeta Mariş ,
Miruna Daniela Popescu  and
Diana Beşliu
Georgeta Mariş
Affiliation:
Astronomical Institute of the Romanian Academy Str. Cutitul de Argint 5, RO-040558 1 Bucharest, Romania e-mail: gmaris@aira.astro.ro
Miruna Daniela Popescu
Affiliation:
Astronomical Institute of the Romanian Academy Str. Cutitul de Argint 5, RO-040558 1 Bucharest, Romania e-mail: gmaris@aira.astro.ro Armagh Observatory, College Hill, Armagh, BT61 9DG, N. Ireland email: mdp@arm.ac.uk
Diana Beşliu
Affiliation:
Astronomical Institute of the Romanian Academy Str. Cutitul de Argint 5, RO-040558 1 Bucharest, Romania e-mail: gmaris@aira.astro.ro
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Abstract

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Here we analyse the solar cycle (SC) 23 behavior and we also make a comparison with some previous cycles and present a few aspects concerning the forecasts made for SC 23 maximum. As regards the following cycle, in accordance to other early predictions, our empirical method, based on observing the flare energy release during the descendant phase of the precedent SC, estimate that the amplitude of SC 24 will be low.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 127 - 128
Copyright
© 2004 International Astronomical Union