Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-13T12:40:55.835Z Has data issue: false hasContentIssue false
  • English
  • Français

Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001

Published online by Cambridge University Press:  03 June 2005

Olga A. Sheiner  and
Vladimir M. Fridman
Olga A. Sheiner
Affiliation:
Radiophysical Research Institute (NIRFI), 25 Bol'shaya Pecherskaya Street, Nizhny Novgorod, 603950 Russia email: rfj@nirfi.sci-nnov.ru
Vladimir M. Fridman
Affiliation:
Radiophysical Research Institute (NIRFI), 25 Bol'shaya Pecherskaya Street, Nizhny Novgorod, 603950 Russia email: fridman@nirfi.sci-nnov.ru
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The results of solar microwave observations in the Radio Astronomical Observatory NIRFI “Zimenki” are examined. Data analysis shows the presence of periodic component, that arose prior to burst connected to CMEs onset, and its absence after burst. Obtained data are compared with the dynamics of the development of activity on the solar disk. Results can be considered as the illustration of the dynamics of wave motions in the periods of flare activity.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: radio radiationoscillationscoronal mass ejections (CMEs)evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 235 - 237
Copyright
© 2005 International Astronomical Union