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.

Bibliographic Details
Main Authors:	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
Format:	Article
Language:	English
Published:	Nature Publishing Group 2017-11-01
Series:	Nature Communications
Online Access:	https://doi.org/10.1038/s41467-017-01307-8

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spelling	doaj-897c741ce92044c28801e3193f1ee1d22021-05-11T07:16:35ZengNature Publishing GroupNature Communications2041-17232017-11-01811910.1038/s41467-017-01307-8Imaging spectroscopy of solar radio burst fine structuresE. P. Kontar0S. Yu1A. A. Kuznetsov2A. G. Emslie3B. Alcock4N. L. S. Jeffrey5V. N. Melnik6N. H. Bian7P. Subramanian8School of Physics and Astronomy, University of GlasgowNew Jersey Institute of TechnologyInstitute of Solar-Terrestrial PhysicsDepartment of Physics & Astronomy, Western Kentucky UniversitySchool of Physics and Astronomy, University of GlasgowSchool of Physics and Astronomy, University of GlasgowInstitute of Radio Astronomy, National Academy of Sciences of UkraineSchool of Physics and Astronomy, University of GlasgowIndian Institute of Science Education and ResearchRadio 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.https://doi.org/10.1038/s41467-017-01307-8
collection	DOAJ
language	English
format	Article
sources	DOAJ
author	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
spellingShingle	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 Imaging spectroscopy of solar radio burst fine structures Nature Communications
author_facet	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
author_sort	E. P. Kontar
title	Imaging spectroscopy of solar radio burst fine structures
title_short	Imaging spectroscopy of solar radio burst fine structures
title_full	Imaging spectroscopy of solar radio burst fine structures
title_fullStr	Imaging spectroscopy of solar radio burst fine structures
title_full_unstemmed	Imaging spectroscopy of solar radio burst fine structures
title_sort	imaging spectroscopy of solar radio burst fine structures
publisher	Nature Publishing Group
series	Nature Communications
issn	2041-1723
publishDate	2017-11-01
description	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.
url	https://doi.org/10.1038/s41467-017-01307-8
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Imaging spectroscopy of solar radio burst fine structures

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