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Cyclical evolution of solar corona by observation in line FeXIV 5303Å

Published online by Cambridge University Press:  14 March 2005

R.N. Ikhsanov  and
V.G. Ivanov
R.N. Ikhsanov
Affiliation:
Central Astronomical Observatory at Pulkovo, Saint-Petersburg, Russia; E-mail: solar1@gao.spb.ru
V.G. Ivanov
Affiliation:
Central Astronomical Observatory at Pulkovo, Saint-Petersburg, Russia; E-mail: solar1@gao.spb.ru
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Abstract

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We investigate the series of the green corona (GC) intensity by the combined catalogues of Rybansky, Tlatov and the original series of Kislovodsk station.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. 255 - 256
Copyright
© 2004 International Astronomical Union