A New Spectral Characteristic in Solar Radio Emission

Details A New Spectral Characteristic in Solar Radio Emission A New Spectral Characteristic in Solar Radio Emission

Jan 1958

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1958natur.181...36m&link_type=abstract

Nature, Volume 181, Issue 4601, pp. 36-38 (1958).

Physics

18

Scientific paper

THE intense radio emissions from active areas on the Sun have been studied since 1942 on `single' fixed frequencies; but the first `spectral' or sweep frequency observations were not initiated until 1949, when Wild and McCready1 at Sydney commenced observations with equipment sweeping the band 70-130 Mc./s. These observations, which were later2 extended to 40-240 Mc./s., marked a notable advance in solar radio techniques, and greatly simplified the classification of solar radio phenomena.

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