How does large flaring activity from the same active region produce oppositely directed magnetic clouds?
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 relat...
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Autores principales: | 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. |
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Formato: | JOUR |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v244_n1-2_p95_Harra |
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