6.2.1.1. Base@CRData¶
Selection of generic data sets to load and specific list of experiment and quantities (in the data sets) to renormalise the model to.
Group@subgroup@parameter | Description |
---|---|
Base@CRData@fCRData (M=0) | Path [1] to file containing USINE-formatted CR data, e.g. $USINE/inputs/crdata_crdb20170523.dat. More on the format in Cosmic ray data. |
Base@CRData@NormList (M=0) | Qties1:Exp1|Eval1|Etype1;Qties2:Exp2|Eval2|Etype2;… with xtype = kEKN, kR or kETOT (e.g., H,He:PAMELA|20.|kEKN;C,N,O,Si,Fe:HEAO|10.6|kEKN ). During propagation, source abundances are rescaled to NormList data point selection (sought in fCRData), unless the normalisation is a fit parameter (in UsineRun@FitFreePars) or data name appears in Base@ListOfCRs@PureSecondaries. |
Note
Renormalising source abundances to elemental fluxes in the model (keeping the same isotopic relative abundances) is the standard/fastest way to run USINE. To bypass this renormalisation, one has to fix individual source abundances or fit these abundances on the data.
Footnote
[1] | Environment variables in path (e.g. $USINE/ ) are enabled and correctly interpreted |