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Harra, L.K.; Crooker, N.U.; Mandrini, C.H.; Van Driel-Gesztelyi, L.; Dasso, S.; Wang, J.; Elliott, H.; Attrill, G.; Jackson, B.V.; Bisi, M.M. "How does large flaring activity from the same active region produce oppositely directed magnetic clouds?" (2007) Solar Physics. 244(1-2):95-114
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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. © 2007 Springer Science+Business Media B.V.

Registro:

Documento: Artículo
Título:How does large flaring activity from the same active region produce oppositely directed magnetic clouds?
Autor:Harra, L.K.; Crooker, N.U.; Mandrini, C.H.; Van Driel-Gesztelyi, L.; Dasso, S.; Wang, J.; Elliott, H.; Attrill, G.; Jackson, B.V.; Bisi, M.M.
Filiación:Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom
Center for Space Physics, Boston University, Boston, MA, United States
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC. 67, Suc. 28, Buenos Aires 1428, Argentina
Observatoire de Paris, LESIA, FRE 2461 (CNRS), Meudon Principal Cedex 92195, France
Konkoly Observatory, Hungarian Academy of Sciences, Budapest, Hungary
National Astronomical Observatory, Chinese Academy of Sciences, Beijing, China
Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires 1428, Argentina
Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238, United States
Center for Astrophysics and Space Sciences, University of California, San Diego, San Diego, CA, United States
Año:2007
Volumen:244
Número:1-2
Página de inicio:95
Página de fin:114
DOI: http://dx.doi.org/10.1007/s11207-007-9002-x
Título revista:Solar Physics
Título revista abreviado:Sol. Phys.
ISSN:00380938
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v244_n1-2_p95_Harra

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Citas:

---------- APA ----------
Harra, L.K., Crooker, N.U., Mandrini, C.H., Van Driel-Gesztelyi, L., Dasso, S., Wang, J., Elliott, H.,..., Bisi, M.M. (2007) . How does large flaring activity from the same active region produce oppositely directed magnetic clouds?. Solar Physics, 244(1-2), 95-114.
http://dx.doi.org/10.1007/s11207-007-9002-x
---------- CHICAGO ----------
Harra, L.K., Crooker, N.U., Mandrini, C.H., Van Driel-Gesztelyi, L., Dasso, S., Wang, J., et al. "How does large flaring activity from the same active region produce oppositely directed magnetic clouds?" . Solar Physics 244, no. 1-2 (2007) : 95-114.
http://dx.doi.org/10.1007/s11207-007-9002-x
---------- MLA ----------
Harra, L.K., Crooker, N.U., Mandrini, C.H., Van Driel-Gesztelyi, L., Dasso, S., Wang, J., et al. "How does large flaring activity from the same active region produce oppositely directed magnetic clouds?" . Solar Physics, vol. 244, no. 1-2, 2007, pp. 95-114.
http://dx.doi.org/10.1007/s11207-007-9002-x
---------- VANCOUVER ----------
Harra, L.K., Crooker, N.U., Mandrini, C.H., Van Driel-Gesztelyi, L., Dasso, S., Wang, J., et al. How does large flaring activity from the same active region produce oppositely directed magnetic clouds?. Sol. Phys. 2007;244(1-2):95-114.
http://dx.doi.org/10.1007/s11207-007-9002-x