| Issue |
EAS Publications Series
Volume 55, 2012
4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
|
|
|---|---|---|
| Page(s) | 335 - 338 | |
| Section | CMEs and Space Weather | |
| DOI | https://doi.org/10.1051/eas/1255046 | |
| Published online | 27 June 2012 | |
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 335-338
Homologous flares inducing EUV filament oscillations with subsequent eruption
1
Institut d’Astrophysique Spatiale, UMR 8617, Bât. 121, Univ. Paris
Sud-CNRS, 91405
Orsay cedex,
France
2
Institut d’Astrophysique de Paris, UMR 7095, CNRS and
UPMC, 98 Bis Bd.
Arago, 75014
Paris,
France
3
Physics Department, Payame Noor University, 19395-3697
Tehran, R. of Iran, Iran
We focus our analysis on an event which occurred at the W-limb on May 30, 2003. The dynamical behavior of the filament, including damped oscillations, was investigated with the CDS and EIT (SoHO) experiments, as well as with Hα filtergrams (movies). The eruptive phase is analyzed taking into account the approximate phasing with other eruptive phenomena occurring at the same time or before, called homologous flares and eruptions.
© EAS, EDP Sciences 2012