Quasi-periodic solar emission has been observed with a radio spectrograph operating at 18-28 MHz during weak decametric continuum on August 22, 1972. The continuum activity was observed simultaneously on fixed frequency receivers at 18 MHz and at 26 MHz. The pulsations showed a mean period of 4 s an
Stellar activity at radio wavelengths
โ Scribed by George A. Dulk
- Publisher
- Elsevier Science
- Year
- 1986
- Tongue
- English
- Weight
- 165 KB
- Volume
- 6
- Category
- Article
- ISSN
- 0273-1177
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