The procedure developed in Smith (1974) to model the radiation source for type 11I bursts is modified to include scattering of radiation in the source itself. Since the inhomogeneities in the source must have the same statistical properties as the inhomogeneities used in tracing radiation from the s
A dynamic theory of type III solar radio bursts
โ Scribed by V. V. Zaitsev; N. A. Mityakov; V. O. Rapoport
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 756 KB
- Volume
- 24
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
The required electron density to excite a type III solar burst can be predicted from different theories, using the low frequency radio observations of the RAE-1 satellite. Electron flux measurements by satellite in the vicinity of 1 AU then give an independent means of comparing these predicted exci
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