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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*
Affiliation:
Department of Physics, University of Tasmania

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
Copyright
Copyright © Astronomical Society of Australia 1969

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References

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