Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-13T10:05:23.044Z Has data issue: false hasContentIssue false

The CME dynamics associated to the prominence eruption of December 2, 2003

Published online by Cambridge University Press:  01 November 2006

Vladimir A. Slemzin
Affiliation:
P.N. Lebedev Physical Institute, Lenisky pr., 53, Moscow, 119991, Russia email: slem@lebedev.ru
S. Koutchmy
Affiliation:
Institut d'Astrophysique de Paris, CNRS and UPMC, France email: koutchmy@iap.fr
J.-C. Noens
Affiliation:
OMP and Pic du Midi observatory, France email: noens@ast.obs-mip.fr
D. Romeuf
Affiliation:
C.R.I. Claude Bernard Lyon I University, O.A.-Fiducial, France email: David.Romeuf@recherche.univ-lyon1.fr
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 H$\alpha$ filament and EUV filament channel is close to the mass of the core but significantly less than the total CME mass.

Type
Contributed Papers
Copyright
© 2006 International Astronomical Union