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Fine structure of the S-component spectrum of the solar radio emission in the frequency range 5.0–7.0 GHz

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Abstract

Fine structure observations of the frequency spectrum of the S-component in the solar radio emission are described. Measurements were carried out in August 1976 and August 1977 using a 22 m parabolic antenna and a radiospectrograph operating over the frequency range 5.0 to 7.0 GHz, with the resolution 60 MHz. Measurement techniques are described. Fine structures (150–800 MHz) as great as 20% of the local source radiation level were observed in radio emission spectra of a number of these sources. The spectrum structures observed were changed in the process of active region development.

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Authors and Affiliations

  1. Radiophysical Research Institute, Gorky, USSR

    N. S. Kaverin, M. M. Kobrin, A. I. Korshunov & V. V. Shushunov

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  1. N. S. Kaverin
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  2. M. M. Kobrin
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  3. A. I. Korshunov
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  4. V. V. Shushunov
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Kaverin, N.S., Kobrin, M.M., Korshunov, A.I. et al. Fine structure of the S-component spectrum of the solar radio emission in the frequency range 5.0–7.0 GHz. Sol Phys 63, 379–388 (1979). https://doi.org/10.1007/BF00174542

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  • DOI: https://doi.org/10.1007/BF00174542

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