Abstract

Abstract Features of the γ-radiation of the induced activity in structural materials Al, Ti, Fe, Cu, W, Pb and in one of the alloys exposed to cosmic proton and albedo neutron fluxes in close-to-earth orbits are investigated by using a Monte Carlo simulation of internuclear cascade development. Disc-shaped targets of 100 cm in diameter and different thicknesses have been considered. The influence of the South Atlantic Anomaly is considered. The spectral distribution of the γ-background intensity is analysed for flight durations from 24 hours to several years. It is shown that the induced radioactivity is comparable to the orbital background γ-radiation and in some energy ranges even exceeds it.

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