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

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