An advection-diffusion model of impact-driven lunar regolith gardening explains Fe-60 depth profiles from supernovae and predicts locations for r-process isotopes like Pu-244.
Reedy, A model for gcr-particle fluxes in stony me- teorites and production rates of cosmogenic nuclides, Journal of Geophysical Research: Solid Earth90, C722 (1985)
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Gardening on the Moon: An Advection-Diffusion Model to Guide the Search for Supernova Debris in the Lunar Regolith
An advection-diffusion model of impact-driven lunar regolith gardening explains Fe-60 depth profiles from supernovae and predicts locations for r-process isotopes like Pu-244.