Three solar outbursts which show pulsating radio emissions at metric waves (239 MHz) are examined. The behaviour of the single frequency, high-time resolution records and the spectral diagrams seem to indicate that such phenomena are peculiar phases of type IV radiation, perhaps connected with absor
On a cold emission in the solar corona
โ Scribed by K. V. Alikayeva
- Publisher
- Springer
- Year
- 1975
- Tongue
- English
- Weight
- 432 KB
- Volume
- 41
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
The faint emission of hydrogen, helium and metals in the corona which appeared near an active prominence is studied. The calculations showed that the temperature of the emission region is in the limits from 10000 K to 30000 K and the electron density is between 109-10 x~ cm -3, respectively.
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