A study of type II solar radio bursts recorded at 160 MHz by the Culgoora radioheliograph during 1980 to 1982 shows that the radio emission occurs above He filaments rather than above He flares. This suggests that the type II radio emission most probably originates from within a coronal helmet strea
Detailed correlation of type III radio bursts with Hα activity
✍ Scribed by T. B. H. Kuiper; Jay M. Pasachoff
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 842 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
It is observed that while there exists a strong correlation between the decay constant and the exciter duration for isolated type III radio bursts, it is absent for those type III radio bursts which are preceded by type IIIb radio bursts. A possible theoretical explanation for the presence of correl
With 13 figurcs. (Keccived 1965 July 15) Thc phenomenological features of type V radiation arc discussed a t the basis of fine structure rccords taken a t the Astrophysical Observatory Potsdam since 1958. A phenomenological subclassification is derived from the various forms of appearance. It is bel
We compare evidence of coronal magnetic fields from polarized metric type III radio bursts with (a) global potential field models, (b) direct averages of the observed photospheric magnetic field, and (c) Ha synoptic charts. The comparison clearly indicates both that the principal aspects of type III
With 5, figurcs. (lieccived 1965 July 22) Decameter type 111 and type III/V bursts observed during more than five years are investigated statistically concerning their association with microwavc bursts and chroinospheric flares. The effects of starting times, morphology, and spectrum of associated