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Absorbed dose in 1 s as a function of energy during solar minimum (ϕ = 400 MV) is shown here using four panels corresponding to the four selected GCR species, as indicated in the lower center of each panel. Full lines are used for silicon detectors, while dashed lines are used for H2O detectors. We observe that the smaller sphere and slab detectors suffer a higher dose at lower energies, while for the low-Z nuclei above 1 GeV, the ICRU detector (phantom) suffers a slightly higher dose.
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