An extensive study of the IMP-6 and IMP-8 plasma and radio wave data has been performed to try to find electron plasma oscillations associated with type III radio noise bursts and low energy solar electrons. This study shows that electron plasma oscillations are seldom observed in association with s
โฆ LIBER โฆ
The source model of low-energy electrons responsible for type I and type III radio noise storms
โ Scribed by V. M. Gubchenko; V. V. Zaitsev
- Publisher
- Springer
- Year
- 1983
- Tongue
- English
- Weight
- 498 KB
- Volume
- 89
- 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