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The Frequency Splitting of Transient Solar Radio Bursts
Published online by Cambridge University Press: 25 April 2016
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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