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Space Radio-Astronomy of Solar Bursts at All Frequencies: The Stereo Project*

Published online by Cambridge University Press:  14 August 2015

J. L. Steinberg  and
C. Caroubalos
J. L. Steinberg
Affiliation:
Observatoire de Meudon, France
C. Caroubalos
Affiliation:
Observatoire de Meudon, France

Abstract

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Most observed characteristics of type III bursts are accounted for by the ‘plasma hypothesis’ which implies that the radio energy is radiated from the coronal altitude where the local plasma frequency is close to the observing frequency and the index of refraction vanishes. Strong focusing is to be expected in the absence of scattering effects.

Type
Part IV: Radio Astronomy
Information
Symposium - International Astronomical Union , Volume 41: New Technique in Space Astronomy , 1971 , pp. 419
Copyright
Copyright © Reidel 1971