Periodic Structure in Solar Radio Bursts and its Relation to Burst Energy
β Scribed by CRIBBENS, A. H.; MATTHEWS, P. A.
- Book ID
- 109667038
- Publisher
- Nature Publishing Group
- Year
- 1969
- Tongue
- English
- Weight
- 182 KB
- Volume
- 222
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/222158b0
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Fifteen examples o[ quasi-periodic 2.8 GHz burst emission observed at the La Posta Astrogeophysical Observatory during the period December 1966 through May 1973 were identified. The periods of these events and those of 22 additional events pre~iously reported in the literature were plotted against b
A moving Type IV burst, observed with the Culgoora radioheliograph on 1970 April 29, moved out to about 3 R o and attained high circular polarization before fading. The appearance of the moving Type IV source suggests an isolated, self-contained, synchrotron emitting plasmoid. Magnetic field maps of
The results of 2 89 years (July 1967 monitoring of solar radio bursts at 71 GHz (2 = 4.2 mm) at the Radio and Space Research Station, Slough are presented. During this period only seven events were positively identified as 71 GHz bursts. One of these events (6 July, 1968) is among the largest solar
The solar burst of 13 July, 1986 at 2I cm wavelength was recorded with a time constant of 8 ms. In the course of the burst lasting for about 40 min there appeared distinct stages of the burst's evolution. They consisted of the pattern of energy release in flares which was proposed by Sturrock et al.