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The Frequency Splitting of Transient Solar Radio Bursts

Published online by Cambridge University Press:  25 April 2016

G. R. A. Ellis
G. R. A. Ellis*
Affiliation:
Department of Physics, University of Tasmania
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Extract

Observations of transient solar radio emissions lasting 0.2 to 2 s in the frequency range 25-50 MHz have demonstrated the existence of a characteristic and relatively common type of burst (the split pair) made up of two narrow band components separated in frequency by about 0.1 MHz.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 6 , September 1969 , pp. 273 - 274
Copyright
Copyright © Astronomical Society of Australia 1969

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References

1 Ellis, G. R. A. and McCulloch, P. M., Aust. J. Phys., 20, 583 (1967).CrossRefGoogle Scholar
2 Ellis, G. R. A., Nature, 213, 790 (1967).Google Scholar
3 Ellis, G. R. A., Aust. J. Phys., 22, 177 (1969).Google Scholar
4 Zaitsev, V. V., Sov. Astron., 9, 572 (1966).Google Scholar
5 Zaitsev, V. V., Sov. Astron., 12, 610 (1969).Google Scholar
6 Weiss, A. A., Aust. J. Phys., 18, 167 (1965).CrossRefGoogle Scholar
7 Maxwell, A. and Thompson, A., Ap. J., 135, 138 (1962).Google Scholar