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- W2027998740 abstract "Abstract An extensive series of balloon flights was conducted during the peak of the present solar maximum, utilizing instruments identical with those which had been flown previously during the declining portion of the preceding solar cycle (1949–1952). During the interval July, 1957, to September, 1958, no sporadic increases in intensity were detected at Swarthmore, Pennsylvania, by quadruple coincidence counter trains containing 86 g/cm 2 of absorber. In eight cases, solar flares of Importance 2 or greater occurred while the instruments were aloft, and on one occasion (22 Aug. 1958) a large increase in the flux of low energy cosmic rays was observed at balloon altitudes elsewhere. A recurrence tendency with a periodicity of 28 ± 1 days was followed for about 5 months. The fluctuations in the counting rates of the balloon-borne instruments were correlated with those observed by ground-based neutron monitors, and the mean factor relating the relative changes is 1.6 ± 0.3.However, it is unlikely that this ratio remains constant." @default.
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- W2027998740 date "1960-03-01" @default.
- W2027998740 modified "2023-09-30" @default.
- W2027998740 title "Balloon flight investigations of primary cosmic rays during solar disturbances" @default.
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- W2027998740 doi "https://doi.org/10.1016/0016-0032(60)90287-8" @default.
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