Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-25T23:26:06.834Z Has data issue: false hasContentIssue false

Observations of Motions in a Solar Storm Centre

Published online by Cambridge University Press:  25 April 2016

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

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