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The Positions of Associated Type II and Type III Solar Radio Bursts

Published online by Cambridge University Press:  25 April 2016

R. A. Duncan
R. A. Duncan*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

Large solar radio outbursts at metre wavelengths often consist of a group of type III bursts followed a few minutes later by a type II burst; in both spectral types the intense burst radiation drifts towards lower frequencies with time (Figure 1).

Type
Solar
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 5 , September 1974 , pp. 255 - 258
Copyright
Copyright © Astronomical Society of Australia 1974

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References

Dulk, G. A., Altschuler, M. D., and Smerd, S. F., Astrophys. Lett., 8, 235 (1971).Google Scholar
Snedecor, G. W., and Cochran, W. G., Statistical Methods, p. 116, Iowa State University Press, 1967.Google Scholar
Uchida, Y., Altschuler, M. D., and Newkirk, G., Solar Phys., 28, 495 (1973).Google Scholar
Wild, J. P., and Smerd, S. F., Annu. Rev. Astron. Astrophys., 10, 159 (1972).Google Scholar
Wild, J. P., Roberts, J. A., and Murray, J. D., Nature, 173, 532 (1954).Google Scholar