Decametric N burst: A consequence of the interaction of two coronal mass ejections

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Radio emissions of electron beams in the solar corona and interplanetary space are tracers of the underlying magnetic configuration and of its evolution. We analyse radio observations from the Culgoora and WIND/WAVES spectrographs, in combination with SOHO/LASCO and SOHO/MDI data, to understand the...

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Detalles Bibliográficos
Autores principales:	Démoulin, P., Klein, K.-L., Goff, C.P., Van Driel-Gesztelyi, L., Culhane, J.L., Mandrini, C.H., Matthews, S.A., Harra, L.K.
Formato:	JOUR
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00380938_v240_n2_p301_Demoulin
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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