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- W2017225568 abstract "An improved method of charge determination of heavy primary cosmic rays of nuclear charge Z = 10–28 has been obtained by measuring the Fowler–Perkins parameter in less-sensitive G-2 and G-0 emulsions for the determination of the primary ionization. It is found that reliable measurements of the primary ionization can be made for ionizations as high as ~1 000 times minimum. The average errors in the charge determinations by this method were found to be about 0.5, 0.7, and 1.0 unit of charge for H 1 (Z = 10–15), H 2 (Z = 16–19), and H 3 (Z = 20–30) groups of nuclei, respectively. This method has been applied to the study of the H 1 , H 2 , and H 3 groups of nuclei in an emulsion stack exposed over Fort Churchill, Canada, on June 18, 1963 at 4.3 g cm −2 of residual atmosphere for 11.1 h. The results are based on an analysis of 340 nuclei with [Formula: see text]. The charge composition and relative abundances of the H 1 , H 2 , and H 3 nuclei were obtained. The differential energy spectra of the H 1 , H 2 , H 3 , and [Formula: see text] groups of nuclei were determined in the energy interval 250–1 000 MeV/nucleon and integral fluxes for energy > 1 000 MeV/nucleon." @default.
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- W2017225568 date "1968-05-15" @default.
- W2017225568 modified "2023-09-27" @default.
- W2017225568 title "Charge and energy spectra of cosmic-ray nuclei with Z = 10–28" @default.
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- W2017225568 doi "https://doi.org/10.1139/p68-301" @default.
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