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CMEs and the structure of low corona above associated active regions according to observations at microwaves

Published online by Cambridge University Press:  14 March 2005

N.N. Kardapolova ,
S.V. Lesovoi ,
T.P. Borisevich ,
N.G. Peterova  and
B.I. Ryabov
N.N. Kardapolova
Affiliation:
Institute of Solar-Terrestrial Physics, Irkutsk, Russia
S.V. Lesovoi
Affiliation:
Institute of Solar-Terrestrial Physics, Irkutsk, Russia
T.P. Borisevich
Affiliation:
Central astronomical observatory at Pulkovo of RAS, St.-Petersburg, Russia
N.G. Peterova
Affiliation:
St.-Petersburg branch of the Special Astrophysical Observatory, St.-Petersburg, Russia
B.I. Ryabov
Affiliation:
Ventspils International Radioastronomical Centre, Riga, Latviya
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Abstract

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The phenomena ($\sim 15$ cases) observed with Siberian Solar Radio Telescope (SSRT) in 2003–2004 years are under investigations. These phenomena are identified with CMEs by LASCO and with the associated active regions (ARs). The structure of low corona above these ARs is studied using the observations with RATAN–600. The aim of this cooperative investigation is to follow this phenomenon at the earliest stage when it is developing in low corona.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. 265 - 266
Copyright
© 2004 International Astronomical Union