Wide-band average spectra of solar radio bursts

Details Wide-band average spectra of solar radio bursts Wide-band average spectra of solar radio bursts

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...67..109d&link_type=abstract

Solar Physics, vol. 67, Aug. 1980, p. 109-120.

Astronomy and Astrophysics

Astronomy

Radio Astronomy, Solar Radio Bursts, Solar Spectra, Statistical Analysis, Broadband, Centimeter Waves, Decimeter Waves, Frequency Response, Sunspots

Scientific paper

Peak flux spectra of solar radio bursts in a wide frequency band have been statistically determined for different morphological types of bursts, for various ranges of magnetic field of the burst-associated sunspots and also for the bursts occurring in the central and limb region of the solar disk. The 106 multi-frequency burst-events were observed at least at eight frequencies. The data were collected by one station, the Sagamore Hill Radio Observatory, Mass., providing uniformity from which to compare and draw conclusions. Results are discussed, including the spectral location of flux density peaks, the identical spectral shape of various bursts, variations in radio emission intensity in the central and limb parts of the solar disk, and the uniformity of radio source characteristics with respect to optical thickness.

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