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Observation of the magnetic structure of a type IV solar radio outburst

✍ Scribed by J. P. Wild

Book ID
105558501
Publisher
Springer
Year
1969
Tongue
English
Weight
254 KB
Volume
9
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

Expanding arch structure of a solar radi
Expanding arch structure of a solar radio outburst
✍ K. Kai πŸ“‚ Article πŸ“… 1970 πŸ› Springer 🌐 English βš– 423 KB

A flare-associated complex outburst was observed on 1968, October 23-24 with the 80 MHz Culgoora radioheliograph. Two harmonic type II bursts were followed by two successive extended sources with arch structure which appeared further beyond the optical limb than the preceding sources. The second arc

Observations and interpretation of movin
Observations and interpretation of moving type IV solar radio bursts
✍ R. D. Robinson πŸ“‚ Article πŸ“… 1978 πŸ› Springer 🌐 English βš– 855 KB

Properties of 23 moving type IV bursts observed with the Culgoora Radioheliograph are summarized. Both shock and plasmoid models are examined. It is found that the theories invoking shocks have limited application and that plasmoid models have several problems with regard to plasmoid formation as we

Interferometer observation of pulsating
Interferometer observation of pulsating sources associated with a type IV solar radio burst
✍ Keizo Kai; Akio Takayanagi πŸ“‚ Article πŸ“… 1973 πŸ› Springer 🌐 English βš– 995 KB

An extremely complex outburst, part of which showed unsually rapid intensity fluctuations of a few second interval, was observed on 1970 November 5 with the 160 MHz interferometer of the Nobeyama Solar Radio Station. The pulsating source, which was stable in position and strongly circularly polarize