Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-23T20:09:03.544Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Get access Rights & Permissions [Opens in a new window]

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

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

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