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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

✍ Scribed by N. S. Kaverin; M. M. Kobrin; A. I. Korshunov; V. V. Shushunov

Publisher
Springer
Year
1979
Tongue
English
Weight
476 KB
Volume
63
Category
Article
ISSN
0038-0938

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✦ Synopsis

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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