There is a characteristic maximum brightness temperature T~ ~-, 1015 K for type lII solar radio bursts in the solar wind. The suggestion is explored that the maximum observed values of TB may be attributed to saturation of the processes involved in the plasma emission. The processes leading to funda
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A relationship between the brightness temperatures for type III bursts
β Scribed by D. B. Melrose
- Publisher
- Springer
- Year
- 1974
- Tongue
- English
- Weight
- 463 KB
- Volume
- 35
- Category
- Article
- ISSN
- 0038-0938
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