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On the Propagation of the Electrons Related to Type III Bursts

Published online by Cambridge University Press:  14 August 2015

G.V. de Genouillac
Affiliation:
Observatoire de Meudon, 92190 Meudon France
D.F. Escande
Affiliation:
Ecole Polytechnique, 9II20 Palaiseau France

Extract

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Type III solar radio bursts are known to be excited by solar electron clouds travelling outwards through the solar corona and interplanetary medium. According to the “plasma hypothesis”, electron plasma oscillations are created by the passing beam, which are in turn converted into electromagnetic waves.

Type
Session V - Solar Bursts - Meter-Decameter Wavelengths
Copyright
Copyright © Reidel 1980