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Type III solar radio burst storms observed at low frequencies

✍ Scribed by Joseph Fainberg; R. G. Stone

Publisher
Springer
Year
1971
Tongue
English
Weight
511 KB
Volume
17
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

Type III solar radio burst storms observ
Type III solar radio burst storms observed at low frequencies
✍ Joseph Fainberg; R. G. Stone πŸ“‚ Article πŸ“… 1970 πŸ› Springer 🌐 English βš– 671 KB

Storms of type III solar radio bursts observed from 5.4 ot 0.2 MHz consist of a quasi-continuous production of type III events observable for half a solar rotation but persisting in some cases for well over a complete rotation (Fainberg and Stone, 1970). The observed burst drift rates are a function

Directivity of low frequency solar type
Directivity of low frequency solar type III radio bursts
✍ R. J. Fitzenreiter; J. Fainberg; R. B. Bundy πŸ“‚ Article πŸ“… 1976 πŸ› Springer 🌐 English βš– 443 KB

The occurrence rate of type III solar bursts in the frequency range 4.9 MHz to 30 kHz is analyzed as a function of burst intensity and burst arrival direction. We find that (a) the occurrence rate of bursts falls off with increasing flux, S, according to the power law S -1s, and (b) the distribution

Solar type III burst profiles at decamet
Solar type III burst profiles at decametre-wave frequencies
✍ C. H. Barrow; A. Achong πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 303 KB

Solar type III bursts have been observed at fixed frequencies of 18, 22, 26 and 36 MHz during the period 1970-1974. 103 profiles have been al~alyzed in the manner introduced by Aubier and . Boischot (1972) whose results are generally confirmed. Average values for the exciter function duration were f