The Frequency Splitting of Transient Solar Radio Bursts
- 1 March 1969
- journal article
- other
- Published by Cambridge University Press (CUP) in Publications of the Astronomical Society of Australia
- Vol. 1 (6) , 273-274
- https://doi.org/10.1017/s1323358000011851
Abstract
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.Keywords
This publication has 5 references indexed in Scilit:
- Fine Structure in the Spectra of Solar Radio BurstsAustralian Journal of Physics, 1969
- Magnetic Fields in the Solar CoronaNature, 1967
- Frequency Splitting of Solar Radio BurstsAustralian Journal of Physics, 1967
- The Nature and Velocity of the Sources of Type II Solar Radio BurstsAustralian Journal of Physics, 1965
- Spectral Observations of Solar Radio Bursts. II. Slow-Drift Bursts and Coronal Streamers.The Astrophysical Journal, 1962