A Multiple Flare Scenario where the Classic Long-Duration Flare Was Not the Source of a CME

VAN DRIEL-GESZTELYI, L.; DÉMOULIN, P.; CULHANE, J.L.; MATTHEWS, S.A.; HARRA, L.K.; MANDRINI, C.H.; KLEIN, K.-L.; KUROKAWA, H.

SOLAR PHYSICS

Springer

Año: 2007 vol. 240 p. 283 - 299

0038-0938

A series of flares (GOES class M, M and C) and a CME were observed in close succession on 20 January 2004 in NOAA 10540. Radio observations, which took the form of types II, III and N bursts, were associated with these events. We use the combined observations from TRACE, EIT, Há images from Kwasan, MDI magnetograms and GOES to understand the complex development of this event. Contrary to a standard interpretation, we conclude that the first two impulsive flares are part of the CME launch process while the following long-duration event flare represents simply the recovery phase. Observations show that the flare ribbons not only separate but also shift along the magnetic inversion line so that magnetic reconnection progresses stepwise to neighboring flux tubes. We conclude that “tether cutting” reconnection in the sheared arcade progressively transforms it to a twisted flux tube, which becomes unstable, leading to a CME. We interpret the third flare, a long-duration event, as a combination of the classical two-ribbon flare with the relaxation process following forced reconnection between the expanding CME structure and neighboring magnetic fields.