calDA(dose, minGrainSize, maxGrainSize, Ucontent, Thcontent, Kcontent, Wct, depth, altitude, latitude, longitude, bulkDensity = 2.5, alphaValue = 0.03, nsim = 10000, rdcf = 0.05, rba = 0.05, plot = TRUE)
dose
, Ucontent
, Thcontent
, Kcontent
, wct
should be two-element vectors with the form c(value,sd)
, as their measurement uncertainties are major error sources. Arguments such as depth
, altitude
, latitude
, longitude
, bulkDensity
, alphaValue
can be either a scalar of a two-element vector. This means that uncertainties from these quantities can be either ignored or taken into account during the simulation.
Fain J, Soumana S, Montret M, Miallier D, Pilleyre T, Sanzelle S, 1999. Luminescence and ESR dating Beta-dose attenuation for various grain shapes calculated by a Monte-Carlo method. Quaternary Science Reviews, 18(2): 231-234.
Prescott JR, Hutton JT, 1994. Cosmic ray contributions to dose rates for Luminescence and Esr dating: large depths and long-term time variations. Radiation Measurements, 23(2-3): 497-500.
calDA(dose=c(25.04,0.68), minGrainSize=90,
maxGrainSize=180, Ucontent=c(2.86,0.19),
Thcontent=c(8.63,0.34), Kcontent=c(2.00,0.11),
Wct=c(0.05,0.05), depth=c(1.1,0.05), altitude=c(1170,58.5),
latitude=c(37.64,1.88), longitude=c(103.16,5.16),
bulkDensity=c(2.5,0.1), nsim=10000, rdcf=0.05, rba=0.05)
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