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Fine Structure in Type IV Solar Radio Bursts

Published online by Cambridge University Press:  25 May 2016

C. Caroubalos ,
M. Pick ,
C. Chiuderi ,
R. Giachetti ,
H. Rosenberg  and
C. Slottje
C. Caroubalos
Affiliation:
Observatoire de Paris, Meudon, France
M. Pick
Affiliation:
Observatoire de Paris, Meudon, France
C. Chiuderi
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italy
R. Giachetti
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italy
H. Rosenberg
Affiliation:
Sterrewacht ‘Sonnenborgh’, Utrecht, The Netherlands
C. Slottje
Affiliation:
Sterrewacht ‘Sonnenborgh’, Utrecht, The Netherlands

Abstract

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(Solar Phys.). The fine structure in solar type IV radio bursts was studied using the 169 MHz Nançay radioheliograph and the 60 channel radiospectrograph at Utrecht (160–320 MHz). The observed fine structure includes pulsating structure, zebra patterns (parallel drifting bands) and intermediate drift bursts. All are considered as modulation of high frequency radiation by low frequency oscillations or as the result of up conversion of low frequency oscillations to higher frequencies (Rosenberg, 1973).

Type
Part II The Flash Phase of Solar Flares
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 291 - 292
Copyright
Copyright © Reidel 1974 

References

Caroubalos, C., Pick, M., Rosenberg, H., and Slottje, C.: 1973, Solar Phys. 30, 473.CrossRefGoogle Scholar
Chiuderi, C., Giachetti, R., and Rosenberg, H.: 1973, Solar Phys. 33, 225.CrossRefGoogle Scholar
Chiuderi, C., Giachetti, R., and Rosenberg, H.: 1974, to be published.Google Scholar
Rosenberg, H.: 1973, , Utrecht.Google Scholar