Cosmic-Ray Neutrons on the Ground and in the Atmosphere
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AbstractNeutrons from collisions of cosmic rays with the nuclei of atoms in the atmosphere are an irremovable external radiation that causes single-event upsets in microelectronic devices. Predicting soft error rates requires knowledge of the flux and energy distribution of the cosmic-ray-induced neutrons. This article reviews cosmic-ray neutrons in the atmosphere and on the ground, the factors that determine their intensity, and recent calculations and state-of-the-art measurements of neutron spectra covering 12 decades of energy, from the thermal energy range up to 10 GeV.
2014 ◽
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pp. 1550007
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1994 ◽
Vol 41
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pp. 2063-2070
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1996 ◽
Vol 26
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pp. 959-965
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Vol 18
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pp. 2229-2366
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2014 ◽
Vol 23
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pp. 1450081
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2011 ◽
Vol 58
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pp. 506-515
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