Imaging spectroscopy of solar radio burst fine structures
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ID: 99532
2017
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Abstract
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.
| Reference Key |
kontar2017imagingnature
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| Authors | Kontar, E. P.;Yu, S.;Kuznetsov, A. A.;Emslie, A. G.;Alcock, B.;Jeffrey, N. L. S.;Melnik, V. N.;Bian, N. H.;Subramanian, P.; |
| Journal | Nature communications |
| Year | 2017 |
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