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

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

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...63..379k&link_type=abstract

Solar Physics, vol. 63, Sept. 1979, p. 379-388.

Astronomy and Astrophysics

Astronomy

4

Fine Structure, Radio Astronomy, Solar Radio Emission, Solar Spectra, Emission Spectra, Frequency Response, Spectrographs, Sunspots

Scientific paper

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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