RESUMEN
The assessment of the exposure to cosmic radiation onboard aircraft is one of the preoccupations of bodies responsible for radiation protection. Cosmic particle flux is significantly higher onboard aircraft than at ground level and its intensity depends on the solar activity. The dose is usually estimated using codes validated by the experimental data. In this paper, a comparison of various codes is presented, some of them are used routinely, to assess the dose received by the aircraft crew caused by the galactic cosmic radiation. Results are provided for periods close to solar maximum and minimum and for selected flights covering major commercial routes in the world. The overall agreement between the codes, particularly for those routinely used for aircraft crew dosimetry, was better than +/-20 % from the median in all but two cases. The agreement within the codes is considered to be fully satisfactory for radiation protection purposes.
Asunto(s)
Aeronaves , Aviación , Exposición Profesional/análisis , Protección Radiológica/métodos , Radiometría/instrumentación , Radiometría/métodos , Altitud , Simulación por Computador , Radiación Cósmica , Europa (Continente) , Humanos , Dosis de Radiación , Monitoreo de Radiación , Programas Informáticos , Actividad SolarRESUMEN
A sophisticated flight code named FREE (acronym for Flight Route Effective Dose Estimation) was built for professional commercial usage. During its creation special precautions have been taken to take correctly into account all existing dependencies and details, so that the best possible result is achieved. Some of these factors are presented in detail and their effect on doses or dose rates is estimated. Detailed comparisons to more recent measurements for both quiescent as well as disturbed conditions are presented. The agreement at undisturbed conditions turns out to be excellent and also the comparisons to measured transient effects are very satisfactory.
Asunto(s)
Aeronaves , Aviación , Exposición Profesional/análisis , Protección Radiológica/métodos , Radiometría/instrumentación , Radiometría/métodos , Altitud , Simulación por Computador , Radiación Cósmica , Europa (Continente) , Humanos , Dosis de Radiación , Monitoreo de Radiación , Actividad SolarRESUMEN
A greatly improved version of the computer program to calculate radiation dosage to air crew members is now available. Designated CARI-6, this program incorporates an updated geomagnetic cutoff rigidity model and a revision of the primary cosmic ray spectrum based on recent work by Gaisser and Stanev (1998). We believe CARI-6 provides the most accurate available method for calculating the radiation dosage to air crew members. The program is now utilized by airline companies around the world and provides unification for subsequent world-wide studies on the effects of natural radiation on aircrew members.
Asunto(s)
Aviación/estadística & datos numéricos , Radiación Cósmica , Exposición Profesional/estadística & datos numéricos , Monitoreo de Radiación/estadística & datos numéricos , Programas Informáticos , Actividad Solar , Medicina Aeroespacial , Aeronaves , Humanos , Magnetismo , Modelos Estadísticos , Dosis de Radiación , Reproducibilidad de los Resultados , Medición de RiesgoRESUMEN
As a result of the recent recommendations of the ICRP 60, and in anticipation of possible regulation on occupational exposure of Canadian-based aircrew, an extensive study was carried out by the Royal Military College of Canada over a one-year period to measure the cosmic radiation at commercial jet altitudes. A tissue-equivalent proportional counter was used to measure the ambient total dose equivalent rate on 62 flight routes, resulting in over 20,000 data points at one-minute intervals at various altitudes and geomagnetic latitudes (i.e. which span the full cut-off rigidity of the Earth's magnetic field). These data were then compared to similar experimental work at the Physikalisch Technische Bundesanstalt, using a different suite of equipment, to measure separately the low and high linear energy transfer components of the mixed radiation field, and to predictions with the LUIN transport code. All experimental and theoretical results were in excellent agreement. From these data, a semiempirical model was developed to allow for the interpolation of the dose rate for any global position, altitude and date (i.e. heliocentric potential). Through integration of the dose rate function over a great circle flight path, a computer code was developed to provide an estimate of the total dose equivalent on any route worldwide at any period in the solar cycle.