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Fig. A.1.

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Oversimplified sketch of the formation of cosmogenic-isotope records in terrestrial (panel a) and lunar (panel b) archives. Primary cosmic-ray particles CR1 and CR2 with energies E1 and E2 < E1 are denoted by blue dots, nuclear reactions by stars, secondaries by arrows, and produced cosmogenic isotopes by red dots. Two different moments of time t1 and t2 > t1 are shown on the left- and right-hand sides, respectively.

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