In this article, the proposal of the International Commission on Radiation Units and Measurements/International Commission on Radiological Protection (ICRU/ICRP), that the ISO slab phantom should continue to be used as a calibration phantom for the new ICRU Report 95 operational quantity personal dose should be legitimised by simulation and performance of experiments to determine backscatter factors on the ISO slab phantom and, in comparison, on an anthropomorphic Alderson Rando phantom. The scope of this work was restricted to the photon energy range of radiation qualities commonly used in x-ray diagnostics. For this purpose, a shadow-free diagnostic (SFD) ionisation chamber was used to measure backscatter factors for X radiation in the energy range of 24 keV to 118 keV. The Monte Carlo code MCNP 6.2 was used to validate measurement results on the ISO slab phantom. Additionally, the influence of varying the SFD position on the Rando phantom on the backscatter factor was determined. Since backscatter factors on the ISO slab phantom differ only up to±5% from those on the Rando phantom, it could be concluded that it is not necessary to develop a new phantom for calibrations in terms of personal dose. A position variation of the detector by a few centimeters on the surface of the Rando phantom causes similarly large deviations and thus alone represents an equally large uncertainty contribution in practical personal dosimetry than that arising from the dissimilarity of the real human body to the ISO slab phantom.
Keywords: Monte Carlo; calibration; metrology; personal dose; personal dosimetry.
Creative Commons Attribution license.