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dc.contributor.author
Harra, Louise K.
dc.contributor.author
Crooker, Nancy U.
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Mandrini, Cristina Hemilse
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van Driel Gesztelyi, Lidia
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Dasso, Sergio Ricardo
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Wang, Jingxiu
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Elliott, Heather
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Attrill, Gemma
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Jackson, Bernard V.
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Bisi, Mario M.
dc.date.available
2017-08-07T18:33:45Z
dc.date.issued
2007-12
dc.identifier.citation
Harra, Louise K.; Crooker, Nancy U.; Mandrini, Cristina Hemilse; van Driel Gesztelyi, Lidia; Dasso, Sergio Ricardo; et al.; How does large flaring activity from the same active region produce oppositely directed magnetic clouds?; Springer; Solar Physics; 244; 1-2; 12-2007; 95-114
dc.identifier.issn
0038-0938
dc.identifier.uri
http://hdl.handle.net/11336/21954
dc.description.abstract
We describe the interplanetary coronal mass ejections (ICMEs) that occurred as a result of a series of solar flares and eruptions from 4 to 8 November 2004. Two ICMEs/magnetic clouds occurring from these events had opposite magnetic orientations. This was despite the fact that the major flares related to these events occurred within the same active region that maintained the same magnetic configuration. The solar events include a wide array of activities: flares, trans-equatorial coronal loop disappearance and reformation, trans-equatorial filament eruption, and coronal hole interaction. The first major ICME/magnetic cloud was predominantly related to the active region 10696 eruption. The second major ICME/magnetic cloud was found to be consistent with the magnetic orientation of an erupting trans-equatorial filament or else a rotation of 160° of a flux rope in the active region. We discuss these possibilities and emphasize the importance of understanding the magnetic evolution of the solar source region before we can begin to predict geoeffective events with any accuracy.
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 Floares
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Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
How does large flaring activity from the same active region produce oppositely directed magnetic clouds?
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-08-04T15:43:58Z
dc.journal.volume
244
dc.journal.number
1-2
dc.journal.pagination
95-114
dc.journal.pais
Alemania
dc.journal.ciudad
Berlin
dc.description.fil
Fil: Harra, Louise K.. Mullard Space Science Laboratory; Reino Unido
dc.description.fil
Fil: Crooker, Nancy U.. Boston University; Estados Unidos
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
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Fil: van Driel Gesztelyi, Lidia. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
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Fil: Dasso, Sergio Ricardo. 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: Wang, Jingxiu. National Astronomical Observatory; China
dc.description.fil
Fil: Elliott, Heather. Southwest Research Institute; Estados Unidos
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Fil: Attrill, Gemma. Mullard Space Science Laboratory; Reino Unido
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Fil: Jackson, Bernard V.. University of California at San Diego; Estados Unidos
dc.description.fil
Fil: Bisi, Mario M.. University of California at San Diego; Estados Unidos
dc.journal.title
Solar Physics
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s11207-007-9002-x
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs11207-007-9002-x
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