Filament interaction modeled by flux rope reconnection

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Hα observations of solar active region NOAA 10501 on 2003 November 20 revealed a very uncommon dynamic process: during the development of a nearby flare, two adjacent elongated filaments approached each other, merged at their middle sections, and separated again, thereby forming stable configuration...

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Detalles Bibliográficos
Autores principales:	Török, T., Chandra, R., Pariat, E., Démoulin, P., Schmieder, B., Aulanier, G., Linton, M.G., Mandrini, C.H.
Formato:	Artículo publishedVersion
Lenguaje:	Inglés
Publicado:	2011
Materias:	Methods: numerical Sun: corona Sun: filaments, prominences
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v728_n1_p_Torok
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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