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

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

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 fla...

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Veröffentlicht in:Proceedings of the International Astronomical Union 2008-09, Vol.4 (S257), p.361-363
Hauptverfasser: Thanassa, Michaella, Mitsakou, Eleftheria, Preka-Papadema, Panagiota, Moussas, Xenophon, Tsitsipis, Panagiotis, Kontogeorgos, Athanasios
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Contributed Papers
Solar flares
Sun
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Zusammenfassung: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.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921309029573