No abstract

No abstract

No abstract

No abstract

187from self-consistent calculations and are not necessarily identical with the actual energy spectra. C. Correction FactorsThe relative number of photon events recorded by the detector for the early and late spectra shown in Fig. 9 is given by CV= E ezNr, i where ex is the detection efficiency for the 7th energy bin. The correction factor was obtained by taking the ratio of the totals for the two spectra. The result is 1.142, 1 H.