Type III events, flares and CMEs, in the extremely active period October-November 2003

Details Type III events, flares and CMEs, in the extremely active period October-November 2003 Type III events, flares and CMEs, in the extremely active period October-November 2003

2010-09-18

arxiv.org/abs/1009.3592v1

2006AIPC, 848, 234M

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Recent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conferen

Scientific paper

10.1063/1.2347984

The type III observations trace the propagation of energetic electron populations through the Solar Corona which, more often than not, precede or are associated with energy release on the Sun. A sample of Type III bursts in the range 20-650 MHz during the period of extraordinary solar activity (20 October to 4 November 2003) recorded by the ARTEMIS-IV1 radio spectrograph is analysed; its parameters are compared with characteristics of associated flares (Ha and GOES SXR) and CMEs, observed in the same period and reported in the SGR and the LASCO archives respectively. In this report we attempt to establish a correlation between energetic particles and major manifestations of solar activity such as flares and CMEs.

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