The spectrum and diameter of the source of the S-component emission (McMath Plage No. 244) observed on March 4, 1968 has been investigated at 3.3 ram, 4.3 ram, 8.5 mm, 2 cm, 9.1 cm, 21 cm, and 43 cm wavelengths.
A model for solar oscillations at cm and mm wavelengths
โ Scribed by W. L. H. Shuter
- Publisher
- Springer
- Year
- 1976
- Tongue
- English
- Weight
- 142 KB
- Volume
- 48
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
It is suggested that large scale oscillations of the Sun give rise to the periodic fluctuations observed in the quiet Sun at radio wavelengths. These fluctuations would be most readily observed from regions where there is a large gradient of electron temperature with electron density, and are thus more readily observed at cm wavelengths than at millimetre wavelengths.
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