Multi-scale reconnections in a complex CME

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A series of three flares of GOES class M, M and C, and a CME were observed on 20 January 2004 occurring in close succession in NOAA 10540. Types II, III, and N radio bursts were associated. We use the combined observations from TRACE, EIT, Hα images from Kwasan Observatory, MDI magnetograms, GOES, a...

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Detalles Bibliográficos
Autores principales: van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., Mandrini, C.H., Klein, K.-L., Kurokawa, H.
Formato: JOUR
Materias:
Magnetic reconnection
Radio burst
Sun: coronal mass ejection
Sun: EUV
Sun: flares
Sun: magnetic fields
Sun: radio
Astrophysics
Crystallography
Magnetic fields
Magnetic materials
Magnetic structure
Field lines
Flux ropes
Magnetic (CE)
Magnetic loops
Magnetic reconnection (MR)
Magnetic-field lines
MDI magnetograms
Multi scaling
Open field lines
radio bursts
radio observations
Radio wavelengths
Solar radius
Magnetism
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_02731177_v42_n5_p858_vanDrielGesztelyi
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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