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Observations of Solar Type III Radio Bursts with the Nancay Radioheliograph
1980
Symposium - International astronomical union
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Results on the space-time evolution of type III burst sources are summarized (Raoult and Pick, 1979) and observations on the temporal characteristics of the circular polarization are presented. It is shown that type III burst sources can be resolved into narrow components. Complex or very large sources may be explained by the occurrence of electron beams which propagate along different diverging paths. Propagating effects in a scattering corona are not required to explain the observations. The
doi:10.1017/s0074180900036883
fatcat:vaysd47obbg6vniu3ybaukogou