Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare

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Solar flares observed in the 200-400 GHz radio domain may exhibit a slowly varying and time-extended component which follows a short (few minutes) impulsive phase and can last for a few tens of minutes to more than one hour. The few examples discussed in the literature indicate that such long-lastin...

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Detalles Bibliográficos
Autores principales: Trottet, G., Raulin, J.-P., Giménez de Castro, G., Lüthi, T., Caspi, A., Mandrini, C.H., Luoni, M.L., Kaufmann, P.
Formato: JOUR
Materias:
Chromosphere, active
Flares, relation to magnetic field
Radio bursts, association with flares
Radio bursts, microwave
X-ray bursts, association with flares
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00380938_v273_n2_p339_Trottet
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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