Observations of Motions in a Solar Storm Centre
Abstract
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.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- March 1969
- DOI:
- 10.1017/S1323358000011371
- Bibcode:
- 1969PASA....1..188M