A thorough detector characterization method is described and applied to ana
lyze the data from the proton switches flown on the Combined Release and Ra
diation Effects Satellite (CRRES). The results are compared with the CRRESP
RO model based on observations of the proton telescope (PROTEL), which was
on board the same satellite. A general good agreement is observed at positi
ons where the flux of high energy protons is low. In regions of harder prot
on spectra, the CRRESPRO fluxes are higher than those deduced from the prot
on switches data. One possible explanation for this discrepancy may be that
high energy protons penetrating into the PROTEL detector ly accounted for.