The CME dynamics associated to the

Abstract. We report on a complex study of a typical large W-limb CME event occurring on December 2, 2003 in the vicinity of AR 0508. It is associated with a prominence eruption which has been observed with the Pic du Midi Ha flux coronagraph as well as in EUV by both the SOHO/EIT and the Coronas/SPIRIT space telescopes. The eruption started with the emergence of a fast expanding loop between 9 and 10 UT, followed by a heating and an acceleration of the erupted material and resulted in three-part CME observed by LASCO after 10:50 UT. A temporal analysis of the prominence motion and the EUV dimming light curve have shown that both the frontal structure and the core of a CME were initiated simultaneously with the peak of the X-ray C7.2 flare. The total mass of the prominence including the Hα filament and EUV filament channel is close to the mass of the core but significantly less than the total CME mass. Keywords. Sun: corona, Sun: coronal mass ejections (CMEs) We report on a large W-limb event, which occurred on December 2, 2003, 9-14h (here-after UT), in the vicinity of an old multi-polar region 10508. The prominence eruption was observed in Hα with the HACO coronagraph, in EUV with SOHO/EIT and CORONAS-F/SPIRIT telescopes. The associated CME was observed later with the LASCO C2 an