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Correlated Bursts at Distant Sources on the Sun

Published online by Cambridge University Press:  25 April 2016

K. Kai
K. Kai*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

Since the start of high-resolution observations with the radioheliograph at the Culgoora Solar Observatory it has been noted that some bursts which occur from separate active regions could be physically correlated. It was suggested that the time delay between the correlated bursts is of the order of seconds, and that fast electrons provide the trigger. Wild found that shortly before a large flare weak bursts, stronelv polarized in the same sense, appeared simultaneously in different sources after a quiet period and he discussed the phenomenon in the light of flare mechanisms.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 186 - 188
Copyright
Copyright © Astronomical Society of Australia 1969

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References

1 Sheridan, K. V., Morimoto, M. and Wild, J. P., Proc. IRE Aust., 28, 380 (1967).Google Scholar
2 Kai, K., McLean, D. J., Payten, W. J., Sheridan, K. V. and Wild, J. P., Proc. ASA, 1, 79 (1968).Google Scholar
3 Wild, J. P., Proc. ASA, 1, 137 (1968).Google Scholar
4 Wild, J. P., Proceedings of Conference on ‘Plasma Instabilities in Astrophysics’, held at Pacific Grove, California, October 1968 (in press).Google Scholar