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. 2011 Mar 15;38(4):1919–1930. doi: 10.1118/1.3560422

Table 2.

Monte Carlo simulated beam characteristics of GSF spectra incident upon air at 20 °C under free-in-air conditions and under PMMA phantom backscatter conditions.

GSF spectrum codes Average energy (keV) Primary+backscatter versus primary
Primary (free-in-air) Primary+backscatter (on-phantom) Photon-fluence ratio Energy-fluence ratio Air kerma ratio
49 (UW-60M) 34.4 33.9 1.308 1.288 1.307
60 (UW-80M) 43.9 42.6 1.365 1.323 1.392
71 (UW-100M) 54.0 51.4 1.407 1.339 1.463
80 (UW-120M) 60.4 57.0 1.418 1.338 1.466