Neutron exposure at civil flight levels

This paper gives a review on the current knowledge of neutron exposure to men at civil flight altitudes due to neutrons, and presents recent experimental and calculation data of the authors. The ICRP proposed in 1991 to consider air crews and other frequently flying persons as occupationally exposed people. As neutrons contribute the major part to the radiologically relevant dose at civil flight levels to men, special considerations are necessary with respect to the required basic data for the determination of the risk relevant radiation doses. The quantification of the dose, suffers from spectral data available especially in the energy range above 20 MeV. Experimental data were obtained at a low flight level on top of the mountain Zugspitze at 3000 m using a modified Bonner sphere spectrometer. The resulting spectra are compared with Monte Carlo transport calculations from top of the atmosphere down to 700 g/cm2. These data and others from the literature are used to calculate the operational and risk related quantities, i.e. ambient dose equivalent, effective dose and effective dose equivalent. The question of the proper choice of the operational quantity ambient dose equivalent to estimate the risk related doses is elucidated.

[1]  Takashi Nakamura,et al.  Altitude variation of cosmic-ray neutrons. , 1987, Health physics.

[2]  V. Mareš,et al.  High energy response functions of bonner spectrometers , 1997 .

[3]  Icrp ICRP Publication 60: 1990 Recommendations of the International Commission on Radiological Protection , 1991 .

[4]  Wilmot N. Hess,et al.  COSMIC-RAY NEUTRON ENERGY SPECTRUM , 1959 .

[5]  H. Schraube,et al.  Experimental Determination of the Response of Four Bonner Sphere Sets to Monoenergetic Neutrons (II) , 1988 .

[6]  M. Merker The contribution of galactic cosmic rays to the atmospheric neutron maximum dose equivalent as a function of neutron energy and altitude. , 1973, Health Physics.

[7]  J. B. McCaslin,et al.  Ames collaborative study of cosmic ray neutrons: mid-latitude flights. , 1978, Health physics.

[8]  A. Sannikov,et al.  Ambient dose equivalent conversion factors for high energy neutrons based on the icrp 60 recommendations , 1997 .

[9]  E. B. Darden,et al.  Galactic cosmic radiation exposure and associated health risks for air carrier crewmembers. , 1989, Aviation, space, and environmental medicine.

[10]  V. Mareš,et al.  Improved response matrices of Bonner sphere spectrometers with 6LiI scintillation detector and 3He proportional counter between 15 and 100 MeV , 1995 .

[11]  H. Hsu,et al.  A new Bonner-sphere set for high energy neutron measurements: Monte Carlo simulation , 1994 .

[12]  K. C. Chandler,et al.  Calculations of neutron flux spectra induced in the Earth's atmosphere by galactic cosmic rays , 1973 .

[13]  V. Mareš,et al.  Organ Doses and Dose Equivalents for Neutrons above 20 MeV , 1997 .

[14]  V. Mareš,et al.  Calculation of the Neutron Ambient Dose Equivalent on the Basis of the ICRP Revised Quality Factors , 1992 .

[15]  H. Schuhmacher,et al.  Quality factors, ambient and personal dose equivalent for neutrons, based on the new ICRU stopping power data for protons and alpha particles , 1995 .

[16]  V. Mareš,et al.  Calculated neutron response of a Bonner sphere spectrometer with 3He counter , 1991 .

[17]  James F. Ziegler,et al.  Terrestrial cosmic rays , 1996, IBM J. Res. Dev..

[18]  N. Hertel,et al.  Effective dose equivalents and effective doses for neutrons from 30 to 180 MeV , 1993 .