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-last...

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Detalles Bibliográficos
Autor principal: Luoni, Maria Luisa
Publicado: 2012
Materias:
active
association with flares
Chromosphere
Flares
microwave
Radio bursts
relation to magnetic field
X-ray bursts
Energy management
Energy resources
Microwaves
Chromophores
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_97814614_v9781461444039_n_p33_Trottet
http://hdl.handle.net/20.500.12110/paper_97814614_v9781461444039_n_p33_Trottet
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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