We present the distribution of the production heights of atmospheric neutrinos as a function of zenith angle and neutrino energy. The distributions can be used as the input for evaluation of neutrino propagation under various hypotheses for neutrino flavor oscillations.

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Gaisser et al. (Sun,) studied this question.

synapsesocial.com/papers/6a121c16ea48cb855a343a58 https://doi.org/https://doi.org/10.1103/physrevd.57.1977

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Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Comparison of atmospheric neutrino flux calculations at low energies1996 · 70 citations
2Low-energy atmospheric neutrinos1988 · 20 citations
3Measurement of cosmic-ray proton and helium spectra during the 1987 solar minimum1991 · 149 citations
4Prompt-muon production in cosmic rays1987 · 46 citations
5Atmospheric neutrino anomaly and its statistical significance1995 · 36 citations

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