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Paired Type III Bursts

Published online by Cambridge University Press:  25 May 2016

C. Caroubalos ,
J. Heyvaerts ,
M. Pick  and
G. Trottet
C. Caroubalos
Affiliation:
Meudon Observatory, France
J. Heyvaerts
Affiliation:
Meudon Observatory, France
M. Pick
Affiliation:
Meudon Observatory, France
G. Trottet
Affiliation:
Meudon Observatory, France

Abstract

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Radioheliographic observations of type III bursts occurring by pairs in a repetitive fashion were made with the high time resolution E–W Nançay Radio heliograph (169 MHz). The data were available in digitized form with a rate of 25 E–W profiles per second. The study is based on two days of observations: for the first one (January 14, 1971) the radio source was at 16′W and for the second one (June 29, 1971) at only 4′W.

Type
Part II The Flash Phase of Solar Flares
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 243 - 244
Copyright
Copyright © Reidel 1974 

References

Caroubalos, C., Heyvaerts, J., Pick, M., and Trottet, G.: 1974, Solar Phys. 37, 205.Google Scholar