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The density of cosmic-ray neutrons in the atmosphere

1963
Neutrons 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, 2003
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.
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The distribution of cosmic ray neutrons in the atmosphere.

1966
An 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, 2020
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Cosmic-ray atmospheric cutoff energies of polar neutron monitors

Advances in Space Research, 2022
Stepán Poluianov
exaly  

Study of Effects of Atmospheric Humidity on Neutron Transportation and its Dose Field

IEEE Transactions on Nuclear Science, 2022
Jianguo Wang, Yinghong Zuo
exaly  

The Energy Distribution of Neutrons in the Atmosphere

Physical Review, 1948
S. A. Korff, M. S. George, J. W. Kerr
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Neutron Star Atmospheres

1995
G. G. Pavlov   +3 more
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