Compute low energy neutron flux using the analytical formulation of Sato et al. (2008)

sato_neutrons_low(h, Rc, s, w)

Arguments

h

atmospheric pressure (hPa)

Rc

cutoff rigidity (GV)

s

solar modulation potential

w

gravimetric fractional water content (non-dimensional)

Details

Adaption of matlab code from Lifton et al. (2014)

Lifton, N., Sato, T., & Dunai, T. J. (2014). Scaling in situ cosmogenic nuclide production rates using analytical approximations to atmospheric cosmic-ray fluxes. Earth and Planetary Science Letters, 386, 149–160. https://doi.org/10.1016/j.epsl.2013.10.052