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Formation and evolution of different type coronal holes

Published online by Cambridge University Press:  14 March 2005

I.A. Bilenko
Affiliation:
Sternberg State Astronomical Institute, Moscow, Russia, email: bilenko@sai.msu.ru Present address: Sternberg State Astronomical Institute, Universitetsky pr. 13, Moscow, Russia, 119992.
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Abstract

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Formation and evolution of coronal holes of different type are investigated. Occurrence and evolution of coronal holes in active regions are connected to the processes occurring in these active regions in particular with flares and CMEs. Coronal holes which are not connected to active regions reflect distribution of large-scale solar magnetic fields and their dynamics determined by global solar magnetic field structure changes.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union