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- W2063414093 abstract "We present a model from which the angular and depth dependent atmospheric γ rays can be derived in the energy range of 0.3–10 MeV at λ = 40°. The model consists of an isotropic source function which depends on depth and energy expressed in the form S(E, x) = S0(E)[1 + b(E)x + c(E)x²]e−x/p(E) photons/(g air s MeV) and is determined semiempirically. We determined source strengths for 38 predicted atmospheric γ ray lines and for 10 different energies in the continuum. For the continuum a diffuse cosmic flux, consistent with the Apollo 15/16 data, is assumed in order to fit the measured data above 10 g/cm². Total and directional fluxes are computed at two different atmospheric depths. The computed flux compares well with other measurements and theoretical calculations." @default.
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- W2063414093 date "1975-08-01" @default.
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- W2063414093 title "A semiempirical model for atmospheric γ rays from 0.3 to 10 MeV at λ = 40°" @default.
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- W2063414093 doi "https://doi.org/10.1029/ja080i022p03241" @default.
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