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The theoretical calculations of the production of neutrinos via cosmic rays incident upon the earth’s atmosphere (Barr et al., 1989; Becker-Szendy et al., 1992; Bugaev & Naumov, 1989; Gaisser et al, 1988; Honda et al., 1995) are examined. These calculations use a one-dimensional approximation in the production, transport, and decay of the produced particles. Examined are various additional effects of the earth’s magnetic field and the three-dimensional nature of the problem which have the effect of decreasing the calulated ratio of muon neutrinos to electron neutrinos.

生成讲解博客的中文版本

生成AI智能校验的中文版本