Spectral characteristics of solar radio bursts associated with shortwave fadeouts

Physics

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Atmospheric Attenuation, Ionospheric Propagation, Microwave Attenuation, Short Wave Radiation, Solar Radio Bursts, Spectrum Analysis, Microwave Spectra, Radiant Flux Density, Solar Spectra, Solar X-Rays, Sudden Ionospheric Disturbances

Scientific paper

Spectral characteristics of centimeter-wavelength solar radio bursts as measured at the Sagamore Hill Radio Observatory were correlated with shortwave fadeouts (SWF). It was found that there is a definite relation between the intensity and shape of the spectrum of a solar radio burst and the occurrence of a SWF. These results imply 'threshold' values for the cm/wavelength component of the radio spectrum if the accompanying X-ray emissions are to be intense enough to cause a SWF.

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