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Terrestrial cosmic rays

The work

AuthorsJ. F. Ziegler
Editors
Typearticle
Year1996
Citekeyziegler1996terrestrial

Where it appeared

Published inIBM Journal of Research and Development
PublisherIBM
Volume40
Issue1
Pages19--39

Identifiers

DOI10.1147/rd.401.0019
OpenAlexW2033346530

From OpenAlex, which stores abstracts as an index of words and their positions: what is shown is rebuilt from that, and reads fluently whether or not it is what the author wrote.

Abstract

This paper reviews the basic physics of those cosmic rays which can affect terrestrial electronics. Cosmic rays at sea level consist mostly of neutrons, protons, pions, muons, electrons, and photons. The particles which cause significant soft fails in electronics are those particles with the strong interaction: neutrons, protons, and pions. At sea level, about 95% of these particles are neutrons. The quantitative flux of neutrons can be estimated to within 3×, and the relative variation in neutron flux with latitude, altitude, diurnal time, earth's sidereal position, and solar cycle is known with even higher accuracy. The possibility of two particles of a cascade interacting with a single circuit to cause two simultaneous errors is discussed. The terrestrial flux of nucleons can be attenuated by shielding, making a significant reduction in the electronic system soft-error rate. Estimates of such attenuation are made.

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Added2026-10-26 00:15 UTC
Not denied bya person 2026-10-29 17:12 UTC

Filed under

ibm-jrd

Cite it as

@article{ziegler1996terrestrial,
  title        = {Terrestrial cosmic rays},
  author       = {J. F. Ziegler},
  year         = {1996},
  journal      = {IBM Journal of Research and Development},
  publisher    = {IBM},
  volume       = {40},
  number       = {1},
  pages        = {19--39},
  doi          = {10.1147/rd.401.0019},
}

This record lives at https://refs.drheap.org/ziegler1996terrestrial/ and will keep doing so.