The production of cosmogenic nuclides in stony meteoroids by galactic cosmic‐ray particles

By I. Leya, H.-J. Lange, Sonja Neumann, R. Wieler, R. Michel. 2000

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Cosmogenic nuclides in stony meteorites revisited (2009, methodology): “Briefly, the neutron excitation functions are extracted from production rates obtained in five thick target simulation experiments (e.g., Michel et al. 1985, 1989, 1993; Lüpke 1993; Leya et al. 2000b).”
An updated simulation of particle fluxes and cosmogenic nuclide production in the Earth's atmosphere (2009, methodology): “A similar approach based on a combination of thin target cross sections with calculated particle fluxes was used by Michel et al. [1995] and Bhandari et al. [1993] to calculate cosmogenic nuclide production rates in stony meteorites [Leya et al., 2000].”
Irradiation Records, Cosmic-Ray Exposure Ages, and Transfer Times of Meteorites (2006, methodology): “Toward the interior (depths >15 cm) of larger meteorites, fluxes of both primary and secondary particles eventually decrease, typically exponentially with a half thickness of about 40 cm in stones (Leya et al., 2000).”