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A study on the relationship of type III radio bursts CME and solar flares during the active period October-November 2003

Published online by Cambridge University Press:  01 September 2008

Michaella Thanassa ,
Eleftheria Mitsakou ,
Panagiota Preka-Papadema ,
Xenophon Moussas ,
Panagiotis Tsitsipis  and
Athanasios Kontogeorgos
Michaella Thanassa
Affiliation:
Department of Physics, University of Athens, 15784 Athens, Greece
Eleftheria Mitsakou
Affiliation:
Department of Physics, University of Athens, 15784 Athens, Greece
Panagiota Preka-Papadema
Affiliation:
Department of Physics, University of Athens, 15784 Athens, Greece
Xenophon Moussas
Affiliation:
Department of Physics, University of Athens, 15784 Athens, Greece
Panagiotis Tsitsipis
Affiliation:
Department of Electronics, Technological Education Institute of Lamia, Lamia, Greece
Athanasios Kontogeorgos
Affiliation:
Department of Electronics, Technological Education Institute of Lamia, Lamia, Greece
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Abstract

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Within a period of intense activity (20 October to 5 November 2003), the injection and propagation of near relativistic electrons, resulted in hundreds of type III bursts recorded by the ARTEMISIV radio spectrograph (20–650 MHz). For a number of these type III events association with GOES SXR/Hα flare and/or SOHO/LASCO CME was established. We study the variation of characteristic type III parameters and their relationship with features of the associated flares and/or CMEs.

Keywords

Sun: coronal mass ejections (CMEs)Sun: flaresSun: radio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 361 - 363
Copyright
Copyright © International Astronomical Union 2009

References

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