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- W2091237692 abstract "This paper discusses the occurrence and intensity of solar radio bursts at four frequencies in the band 100 to 600 Mc/s. The observations cover 4010 hours during a 12-month period at sunspot maximum; the results refer essentially to bursts of intensity great than 10−1 mks unit and duration greater than 0.3 second; and the statistical information has been interpreted in terms of the spectral characteristics of the bursts. The experimental data were taken at Fort Davis, Texas, and the analysis shows that at 125 Mc/s burst radiation was recorded for 560 hours, of which 380 hours were of low intensity. At 200 Mc/s the burst radiation covered 350 hours, of which 240 hours were of low intensity. For these two frequencies the bursts occurred mainly in the form of noise storms (spectral type I). At 425 and 550 Mc/s the total times of the solar bursts were much less, being respectively 21 and 23 hours; for the most part, however, this radiation was of high intensity and appeared in the form of continuum radiation (spectral type IV) over a wide frequency range." @default.
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- W2091237692 date "1960-11-01" @default.
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- W2091237692 title "Some statistics of solar radio bursts at sunspot maximum" @default.
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- W2091237692 doi "https://doi.org/10.1029/jz065i011p03581" @default.
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