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Observations of Motions in a Solar Storm Centre

Published online by Cambridge University Press:  25 April 2016

D. J. McLean
D. J. McLean*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

With a number of important exceptions associated with transitory flare activity, most persistent sources of solar radio emission observed to date with the 80 MHz Culgoora radioheliograph have been stable in position over periods of tens of minutes or hours even though they fluctuated greatly in intensity. During several hours on 1968 November 11, however, we observed some interesting activity which showed frequent changes in the position of a source.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 188 - 189
Copyright
Copyright © Astronomical Society of Australia 1969

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References

1 Kai, K., Proc. ASA, 1, 186 (1969).Google Scholar
2 Wild, J. P., Proc. ASA, 1, 137 (1968); 1, 181 (1969).Google Scholar