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
Solar radio pulsations at 410 MHz
โ Scribed by C. S. Wright; G. J. Nelson
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 522 KB
- Volume
- 111
- Category
- Article
- ISSN
- 0038-0938
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