Imaging spectroscopy of solar radio burst fine structures

Radio observations of the solar atmosphere provide a unique view on the non-thermal processes in the outer atmosphere. Here the authors use LOFAR observations to demonstrate that the observed radio burst characteristics are dominated by propagation effects rather than underlying emission variations.

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Detalles Bibliográficos
Autores principales: E. P. Kontar, S. Yu, A. A. Kuznetsov, A. G. Emslie, B. Alcock, N. L. S. Jeffrey, V. N. Melnik, N. H. Bian, P. Subramanian
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2017
Materias:
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Acceso en línea:https://doaj.org/article/897c741ce92044c28801e3193f1ee1d2
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