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Filament Disparition Brusque and CME – September 25–26, 1996 Event

  • L. van Driel-Gesztelyi (a1), B. Schmieder (a1), G. Aulanier (a1), P. Démoulin (a1), P.C.H. Martens (a2), D. Zarro (a3), C. DeForest (a3), B. Thompson (a3), C.St. Cyr (a3), T. Kucera (a3), J.T. Burkepile (a4), O.R. White (a4), Y. Hanaoka (a5) and N. Nitta (a6)...

Abstract

During the September 1996 campaign of multi-wavelength observations with the SOHO (SUMER, CDS, EIT, MDI, LASCO) and Yohkoh (SXT) spacecraft, the HAO Mauna Loa Solar Observatory Chromospheric Helium Imaging Photometer and the Nobeyama radioheliograph, a filament disparition brusque (DB) associated with a Coronal Mass Ejection (CME) was observed. The timeline of this complex event, which lasted for tens of hours, shows that the CME had started before the DB of a filament, while the main “bubble” of the CME was probably launched hours after the DB from the so-called “zipper” region. All these suggest that a general reorganization of large-scale fields was taking place on the Sun, and both the DB and the CME were symptoms of this.

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References

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McAllister, A.H., Hundhausen, A.J., Burkepile, J.T., McIntosh, P. and Hiei, E. 1998, Geophys, J.. Res., to be submitted
van Driel-Gesztelyi, L. et al. 1998, Solar Physics, to be submitted
White, O.R. et al. 1998, in preparation

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