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Goff, C.P.; Van Driel-Gesztelyi, L.; Démoulin, P.; Culhane, J.L.; Matthews, S.A.; Harra, L.K.; Mandrini, C.H.; Klein, K.L.; Kurokawa, H. "A multiple flare scenario where the classic long-duration flare was not the source of a CME" (2007) Solar Physics. 240(2):283-299
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Abstract:

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, Hα 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. © Springer 2007.

Registro:

Documento: Artículo
Título:A multiple flare scenario where the classic long-duration flare was not the source of a CME
Autor:Goff, C.P.; Van Driel-Gesztelyi, L.; Démoulin, P.; Culhane, J.L.; Matthews, S.A.; Harra, L.K.; Mandrini, C.H.; Klein, K.L.; Kurokawa, H.
Filiación:Mullard Space Science Laboratory, University College London, Dorking, Surrey, RH5 6NT, United Kingdom
Observatoire de Paris, LESIA, UMR 8109 (CNRS), 92195 Meudon Principal Cedex, France
Konkoly Observatory, Hungarian Academy of Sciences, Budapest, Hungary
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC. 67, Suc. 28, 1428 Buenos Aires, Argentina
Hida and Kwasan Observatories, Kyoto University, Yamashina, Kyoto 607, Japan
Año:2007
Volumen:240
Número:2
Página de inicio:283
Página de fin:299
DOI: http://dx.doi.org/10.1007/s11207-007-0260-4
Título revista:Solar Physics
Título revista abreviado:Sol. Phys.
ISSN:00380938
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v240_n2_p283_Goff

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Citas:

---------- APA ----------
Goff, C.P., Van Driel-Gesztelyi, L., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., Mandrini, C.H.,..., Kurokawa, H. (2007) . A multiple flare scenario where the classic long-duration flare was not the source of a CME. Solar Physics, 240(2), 283-299.
http://dx.doi.org/10.1007/s11207-007-0260-4
---------- CHICAGO ----------
Goff, C.P., Van Driel-Gesztelyi, L., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., et al. "A multiple flare scenario where the classic long-duration flare was not the source of a CME" . Solar Physics 240, no. 2 (2007) : 283-299.
http://dx.doi.org/10.1007/s11207-007-0260-4
---------- MLA ----------
Goff, C.P., Van Driel-Gesztelyi, L., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., et al. "A multiple flare scenario where the classic long-duration flare was not the source of a CME" . Solar Physics, vol. 240, no. 2, 2007, pp. 283-299.
http://dx.doi.org/10.1007/s11207-007-0260-4
---------- VANCOUVER ----------
Goff, C.P., Van Driel-Gesztelyi, L., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., et al. A multiple flare scenario where the classic long-duration flare was not the source of a CME. Sol. Phys. 2007;240(2):283-299.
http://dx.doi.org/10.1007/s11207-007-0260-4