In situ produced 10Be measurements at great depths: implications for production rates by fast muons

By R. Braucher, E. Brown, D. Bourlès, F. Colin. 2003

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CosmoCalc: An Excel add‐in for cosmogenic nuclide calculations (2007, background): “Schaller et al. [2002] use not four but eight exponentials (two for neutrons, and three for each slow and fast muons), whereas others use three (one for each production mechanism) [e.g., Braucher et al., 2003; Miller et al., 2006] or only one exponential (neglecting muon production).”
Production rate calculations for cosmic-ray-muon-produced 10Be and 26Al benchmarked against geological calibration data (2017, background): “Cuiaba 707 At Cuiaba, Braucher et al. (2003) collected samples from two sites: a deep open- 708 pit excavation where the original soil surface was not present and the amount of pre- 709 stripping prior to excavation was not exactly known; and a second site, in a different 710 location from the main…”