View source: R/balco2017production.R
mu_model1b | R Documentation |
Compute muons production profile as a function of depth below the surface z (g/cm2) and site atmospheric pressure h (hPa). According to model 1B from Balco (2017)
mu_model1b(z, h, Rc, Sphi, cst)
z |
depth below the surface z (g/cm2) |
h |
site atmospheric pressure h (hPa) |
Rc |
cutoff rigidity (GV) |
Sphi |
solar modulation parameter |
cst |
list of nuclide specific parameters (see below) |
Adapted from G. Balco matlab code
Balco, G. (2017). Production rate calculations for cosmic-ray-muon-produced 10Be and 26Al benchmarked against geological calibration data. Quaternary Geochronology, 39, 150–173. https://doi.org/10.1016/j.quageo.2017.02.001
cst is a list containing nuclide-specific constants, as follows: cst$Natoms - atom number density of the target atom (atoms/g) cst$k_neg - summary cross-section for negative muon capture (atoms/muon) cst$sigma190 - 190 GeV x-section for fast muon production (cm2)
Add the following code to your website.
For more information on customizing the embed code, read Embedding Snippets.