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Homology of solar radio events

Published online by Cambridge University Press:  14 August 2015

A. D. Fokker
A. D. Fokker*
Affiliation:
Sterrewacht ‘Sonnenborgh’, Utrecht, The Netherlands

Abstract

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Successive flares within the same centre of activity sometimes produce radio events that are remarkably similar. The occurrence of such homologous radio events is commonly restricted to periods of less than 48 hours.

Typical for certain centres of activity is their tendency to give rise to impulsive microwave bursts. Such bursts may occur repeatedly during a period of more than a week. The distributions of the lengths of periods during which series of homologous bursts and of impulsive microwave bursts occur are compared.

Type
Part VIII: Radio Structure of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 551 - 555
Copyright
Copyright © Reidel 1968 

References

Ellison, M.A., McKenna, S.M.P., Reid, J.H. (1960) Dunsink Obs. Publ., 1, No. 1.Google Scholar
Fokker, A.D., Roosen, J. (1961) Bull. astron. Inst. Netherl., 16, 83.Google Scholar