Energy input flux in the global quiet-sun corona

We present first results of a novel technique that provides, for the first time, constraints on the energy input flux at the coronal base (r ∼ 1.025 R o) of the quiet Sun at a global scale. By combining differential emission measure tomography of EUV images, with global models of the coronal magneti...

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Detalles Bibliográficos
Autores principales: Vasquez, Alberto Marcos, Lopez Fuentes, Marcelo Claudio, Nuevo, Federico Alberto
Publicado: 2017
Materias:
Sun: corona
Sun: fundamental parameters
Sun: magnetic fields
Sun: UV radiation
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v843_n1_p_MacCormack
http://hdl.handle.net/20.500.12110/paper_0004637X_v843_n1_p_MacCormack
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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