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The density of cosmic-ray neutrons in the atmosphere
1963Neutrons are produced in the atmosphere by the interaction of cosmic-ray particles with the nuclei of nitrogen and oxygen. The density of these neutrons was determined experimentally by means of ionization chambers filled with B^(10), B^(11)F_3, and argon.
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Cosmic-Ray Neutrons on the Ground and in the Atmosphere
MRS Bulletin, 2003AbstractNeutrons 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.
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The distribution of cosmic ray neutrons in the atmosphere.
1966An introduction to the demography of cosmic ray neutrons including a detailed description of neutron diffusion theory with special reference to diffusion in the atmosphere. The design and performance of the detectors, flight unit electronics, telemetry system and receiving and recording equipment are described.
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NEUTRONS IN THE ATMOSPHERE OF EARTH
Aerospace and Environmental Medicine, 2020openaire +1 more source
Cosmic-ray atmospheric cutoff energies of polar neutron monitors
Advances in Space Research, 2022Stepán Poluianov
exaly
Study of Effects of Atmospheric Humidity on Neutron Transportation and its Dose Field
IEEE Transactions on Nuclear Science, 2022Jianguo Wang, Yinghong Zuo
exaly
The Energy Distribution of Neutrons in the Atmosphere
Physical Review, 1948S. A. Korff, M. S. George, J. W. Kerr
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