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
✦ LIBER ✦
On the spectra of type-III solar radio bursts observed at low frequencies
✍ Scribed by Héctor Alvarez
- Publisher
- Springer
- Year
- 1982
- Tongue
- English
- Weight
- 358 KB
- Volume
- 81
- Category
- Article
- ISSN
- 0038-0938
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