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
Towards a better dynamic theory for type III radio bursts
โ Scribed by Dean F. Smith
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 517 KB
- Volume
- 33
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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Observations of impulsive solar flare X-rays > 10 keV made with the OGO-5 satellite are compared with ground based measurements of type III solar radio bursts in 10-580 MHz range. It is shown that the times of maxima of these two emissions, when detectable, agree within ~ 18 s. This maximum time dif