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- W2150410043 abstract "A large increase in the atmospheric neutron flux was observed at balloon altitudes on September 3, 1966, during a solar proton event. The flux and energy spectrum of the solar particles are known with some precision from satellite detectors, as well as from our balloon measurements. From these data quantitative comparisons have been made with the predictions of Lingenfelter and Flamm (1964) on the production of neutrons in the atmosphere by proton interactions. The theory is in satisfactory agreement with the observations, although there is considerable uncertainty about the fraction of neutrons that leaked out of the atmosphere." @default.
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- W2150410043 date "1970-09-01" @default.
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- W2150410043 title "The neutron flux at balloon altitudes during a solar proton event" @default.
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- W2150410043 doi "https://doi.org/10.1029/ja075i025p04595" @default.
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