Spectral characteristics of solar S bursts

Details Spectral characteristics of solar S bursts Spectral characteristics of solar S bursts

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...78..253m&link_type=abstract

Solar Physics, vol. 78, June 1982, p. 253-269. Research supported by the Australian Research Grants Committee.

Physics

12

Radio Spectra, Solar Radio Bursts, Solar Spectra, Spectrum Analysis, Bandwidth, Diffraction Patterns, Drift Rate, Polarization Characteristics, Solar Activity, Solar Flux Density, Temporal Distribution

Scientific paper

Observations of solar S bursts using a radio telescope in the range 30-82 MHz were used to characterize the events. Bursts were observed in June-July, 1979, with one storm yielding over 1000 S events at 40 MHz. All the bursts displayed a negative frequency drift with a range less than 5 MHz. No systematic variation of duration with frequency was observed. The instantaneous bandwidth was found to be limited to 123 MHz to within 56 kHz while duration at a single frequency was only 49 plus or minus 34 msec. A tendency was also noted for some of the S bursts to appear as a series of fringes separated by 100 kHz.

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