Evidence for arc sec radio burst sources in the upper corona |
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| Authors: | David McConnell |
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| Affiliation: | 1. Astronomy Program, University of Maryland, 20742, College Park, MD, U.S.A.
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| Abstract: | Some interpretations of solar S burst spectra are presented. It is shown that the spectra provide evidence for small (～ 500 km) radio sources in the corona which radiate at the fundamental plasma frequency. The possibility of S burst fringes corresponding to coronal MHD waves of wavelength λ ～- 103 km is discussed. |
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