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dc.contributor.author
Golf, C. P.
dc.contributor.author
van Driel Gesztelyi, Lidia
dc.contributor.author
Démoulin, Pascal
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Culhane, J. L.
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Matthews, S. A.
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Harra, L. K.
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Mandrini, Cristina Hemilse
dc.contributor.author
Klein, K. L.
dc.contributor.author
Kurokawa, H.
dc.date.available
2017-07-19T21:56:08Z
dc.date.issued
2007-12
dc.identifier.citation
Golf, C. P.; van Driel Gesztelyi, Lidia; Démoulin, Pascal; Culhane, J. L.; Matthews, S. A.; et al.; A Multiple Flare Scenario where the Classic Long-Duration Flare Was Not the Source of a CME; Springer; Solar Physics; 240; 2; 12-2007; 283-299
dc.identifier.issn
0038-0938
dc.identifier.uri
http://hdl.handle.net/11336/20978
dc.description.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.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Springer
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Solar Flares
dc.subject.classification
Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
A Multiple Flare Scenario where the Classic Long-Duration Flare Was Not the Source of a CME
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-07-18T14:52:06Z
dc.journal.volume
240
dc.journal.number
2
dc.journal.pagination
283-299
dc.journal.pais
Alemania
dc.journal.ciudad
Berlin
dc.description.fil
Fil: Golf, C. P.. Mullard Space Science Laboratory; Reino Unido
dc.description.fil
Fil: van Driel Gesztelyi, Lidia. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
dc.description.fil
Fil: Démoulin, Pascal. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
dc.description.fil
Fil: Culhane, J. L.. Mullard Space Science Laboratory; Reino Unido
dc.description.fil
Fil: Matthews, S. A.. Mullard Space Science Laboratory; Reino Unido
dc.description.fil
Fil: Harra, L. K.. Mullard Space Science Laboratory; Reino Unido
dc.description.fil
Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
dc.description.fil
Fil: Klein, K. L.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
dc.description.fil
Fil: Kurokawa, H.. Kyoto university; Japón
dc.journal.title
Solar Physics
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s11207-007-0260-4
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs11207-007-0260-4
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