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On the solar magnetic field polarity reversal during the activity cycle

Published online by Cambridge University Press:  14 March 2005

E. I. Mogilevsky  and
K. I. Nikolskaya
E. I. Mogilevsky
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, RAS, Troitsk, 142190, Russia email: knikol@izmiran.troitsk.ru
K. I. Nikolskaya
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, RAS, Troitsk, 142190, Russia email: knikol@izmiran.troitsk.ru
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Solar magnetic field polarity reversal (SMFPR) happens every 10-11 years. However untill now there is no clear understanding in what way this process is carried out. Results represented here are a by-product of the coronal hole study based on taken from Web-archive XUV corona images (Yohkoh and EIT/SOHO), white-light corona pictures(SOHO/LASCO) and Kitt Peak coronal hole (CH) 1083 nm maps. Observations used cover the minimum, maximum and a part of declining phase of 23-d cycle (1996-2004).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. 129 - 130
Copyright
© 2004 International Astronomical Union