Radiation Protection Dosimetry Vol. 110 Nos. 1-4 © Oxford University Press 2004; all rights reserved
Averaged particle dose conversion coefficients in air crew dosimetry
1 University of Munich, Institute of Radiobiology, D-80336 Munich, Germany
2 CERN, TIS-RP, CH-1211 Geneva 23, Switzerland
3 GSF-National Research Center, D-85764 Neuherberg, Germany
* Corresponding author: mares{at}gsf.de
The MCNPX Monte Carlo code was used to calculate energy-dependent fluence-to-effective dose conversion coefficients for neutrons, protons, electrons, photons, charged pions and muons. The FLUKA Monte Carlo code was used to calculate the spectral particle fluences of secondary cosmic rays for different altitudes, and for different combinations of solar modulation and vertical cut-off rigidity parameters. The energy-averaged fluence-to-dose conversion coefficients were obtained by folding the particle fluence spectra with the conversion coefficients for effective dose and ambient dose equivalent. They show a slight dependence on altitude, solar activity and location in the geomagnetic field.
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