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Shock Waves and the Ejection of Matter from the Sun: Radio Evidence

Published online by Cambridge University Press:  25 May 2016

D. J. McLean
D. J. McLean*
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

Abstract

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The passage of shock waves and ejected matter through the solar corona can produce type II and type IV radio bursts. This paper reviews the observations of these types of bursts and their interpretation, with particular emphasis on recent work.

Type
Part III Shock Waves and Plasma Ejection
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 301 - 321
Copyright
Copyright © Reidel 1974 

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