World-wide radiation dosage calculations for air crew members.

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.

Overview of atmospheric ionizing radiation (AIR) research: SST-present.

The Supersonic Transport (SST) program, proposed in 1961, first raised concern for the exposure of pregnant occupants by solar energetic particles (SEP), and neutrons were suspected to have a main role in particle propagation deep into the atmosphere. An eight-year flight program confirmed the role of SEP as a significant hazard and of the neutrons as contributing over half of the galactic cosmic ray exposures, with the largest contribution from neutrons above 10 MeV. The FAA Advisory Committee on the Radiobiological Aspects of the SST provided operational requirements. The more recent lowering of ICRP-recommended exposure limits (1990) with the classification of aircrew as "radiation workers" renewed interest in GCR background exposures at commercial flight altitudes and stimulated epidemiological studies in Europe, Japan, Canada and the USA. The proposed development of a High Speed Civil Transport (HSCT) required validation of the role of high-energy neutrons, and this resulted in ER-2 flights at solar minimum (June 1997) and studies on effects of aircraft materials on interior exposures. Recent evaluation of health outcomes of DOE nuclear workers resulted in legislation for health compensation in year 2000 and recent European aircrew epidemiological studies of health outcomes bring renewed interest in aircraft radiation exposures. As improved radiation models become available, it is imperative that a corresponding epidemiological program of US aircrew be implemented.

Radiation exposure during air travel: guidance provided by the Federal Aviation Administration for air carrier crews.

Air carrier crews are occupationally exposed to ionizing radiation, principally from galactic cosmic radiation. To promote radiation safety in aviation the Federal Aviation Administration has: issued educational material on the nature of the radiation received during air travel; recommended radiation exposure limits for pregnant and nonpregnant aircrew members; developed computer programs that estimate for a given flight profile the amount of galactic radiation received on a current flight or on one flown at any time back to January 1958; published tables that enable aircrew members to estimate possible health risks associated with their occupational exposure to radiation; and conducted research on effects of radiation during pregnancy. References for this material are given in the article. In addition, graphic and tabular data in the article show how galactic radiation levels and the composition of the galactic radiation has changed between 1958 and 1999. Also given are estimates of effective doses received by air travelers on a wide variety of air carrier flights.

Perspectives of those impacted: airline pilot's perspective.

The airline pilot operates within an environment that consists of circadian dysrhythmia, reduced atmospheric pressure, mild hypoxia, low humidity, and exposure to sound, vibration, cosmic-radiation, and magnetic-field exposure. These occupational exposures present physiological challenges to the long term health of the airline pilot. In particular, exposure to cosmic radiation and its carcinogenic potential have recently received considerable attention. Given the complexity of the environment and possible synergistic exposures, there is an immediate requirement for comprehensive research into both cosmic-radiation and magnetic-field exposures in airline pilots. In response, the Airline Pilots Association International in conjunction with the Medical University of South Carolina (Department of Biometry and Epidemiology) has initiated an extensive research program into these occupational exposures. These investigations include ground based calculations, flight-dose estimates, epidemiological survey and exposure assessment, and biological marker analysis.

Galactic cosmic radiation exposure of pregnant flight crewmembers.

BACKGROUND: In recommending the occupational dose limit of ionizing radiation for pregnant women, the International Commission on Radiological Protection apparently assumes that the dose to the conceptus from ionizing radiation exposure is about half the dose at the surface of the mother's abdomen. METHODS: To test this assumption with respect to galactic cosmic radiation, calculations were made using FAA computer program CARI-LF2, which calculates equivalent doses from galactic cosmic rays at selected depths in soft tissue at any specified location in the atmosphere or on user-entered flight profiles. RESULTS: The calculations showed that the equivalent dose of galactic radiation was almost the same at all depths. CONCLUSIONS: Thus the assumption of considerable shielding of the conceptus being provided by the woman's body is not correct with respect to galactic cosmic radiation, the principal type of radiation to which aircrews are exposed. The effective dose as calculated with FAA computer program CARI-5E, which calculates effective dose in an anthropomorphic phantom at any specified location in the atmosphere or on user-entered flight profiles, was found to be a good estimate of the equivalent dose at the depth of the conceptus.

Prenatal survival of mouse embryos irradiated in utero with fission neutrons or 250 kV X-rays during the two-cell stage of development.

PURPOSE: To investigate the relationship between radiation dose at the two-cell stage and prenatal survival. MATERIALS AND METHODS: Pregnant mice were irradiated with fast neutrons (0.53-1.94 Gy) or X-rays (1.50-5.00 Gy), or sham irradiated. At selected times up to gestation day 16, the mice were killed and the uterine contents examined. RESULTS: At doses up to 0.82 Gy of neutrons and 2.50 Gy of X-rays, all or virtually all the radiation-induced deaths occurred during the period from the time of implantation to gestation day 10. At higher doses an appreciable proportion of the deaths occurred after day 10. Many neutron-induced deaths in the period from implantation to day 10 occurred before day 7. A mathematical model was developed for estimating survival to gestation day 16 as a function of neutron dose. CONCLUSIONS: The mortality pattern, in which low radiation doses led to early deaths and high doses to both late and early deaths, suggests the existence of two lethal processes. The relationship between neutron dose and survival to gestation day 7 has been interpreted as indicating that the early deaths involved predominantly a two-event inactivation mechanism. An individual cell of a two-cell embryo was found to be less sensitive to lethal radiation injury than a pronuclear zygote.

The atmospheric cosmic- and solar energetic particle radiation environment at aircraft altitudes.

Galactic cosmic rays interact with the solar wind, the earth's magnetic field and hadron, lepton and photon fields at aircraft altitudes. In addition to cosmic rays, energetic particles generated by solar activity bombard the earth from time to time. These particles, while less energetic than cosmic rays, also produce radiation fields at aircraft altitudes which have qualitatively the same properties as atmospheric cosmic rays. We have used a code based on transport theory to calculate atmospheric cosmic-ray quantities and compared them with experimental data. Agreement with these data is seen to be good. We have then used this code to calculate equivalent doses to aircraft crews. We have also used the code to calculate radiation doses from several large solar energetic particle events which took place in 1989, including the very large event that occurred on September 29th and 30th of that year. The spectra incident on the atmosphere were determined assuming diffusive shock theory.

Atmospheric cosmic rays and solar energetic particles at aircraft altitudes.

Galactic cosmic rays, which are thought to be produced and accelerated by a variety of mechanisms in the Milky Way galaxy, interact with the solar wind, the earth's magnetic field, and its atmosphere to produce hadron, lepton, and photon fields at aircraft altitudes that are quite unlike anything produced in the laboratory. The energy spectra of these secondary particles extend from the lowest possible energy to energies over an EeV. In addition to cosmic rays, energetic particles, generated on the sun by solar flares or coronal mass ejections, bombard the earth from time to time. These particles, while less energetic than cosmic rays, also produce radiation fields at aircraft altitudes which have qualitatively the same properties as cosmic rays. The authors have calculated atmospheric cosmic-ray angular fluxes, spectra, scalar fluxes, and ionization, and compared them with experimental data. Agreement with these data is seen to be good. These data have been used to calculate equivalent doses in a simplified human phantom at aircraft altitudes and the estimated health risks to aircraft crews. The authors have also calculated the radiation doses from several large solar energetic particle events (known as GLEs, or Ground Level Events), which took place in 1989, including the very large event known as GLE 42, which took place on September 29th and 30th of that year. The spectra incident on the atmosphere were determined assuming diffusive shock theory. Unfortunately, there are essentially no experimental data with which to compare these calculations.

Galactic cosmic radiation exposure and associated health risks for air carrier crewmembers.

The dose equivalent to air carrier crewmembers from galactic cosmic radiation was estimated for each of 32 nonstop flights on a variety of routes to and from, or within, the contiguous United States. Flying times were from 0.4 to 13 hours. The annual dose equivalents received on the flights ranged from 0.2 to 9.1 mSv (20 to 910 mrem), or 0.4 to 18% of the recommended annual limit for occupational exposure of an adult. We reviewed some of the characteristics of galactic and solar cosmic radiation and provided example calculations for estimating radiation-induced risks of fatal cancer, genetic defects and harm to an embryo or fetus. The estimated increased risk of dying from cancer because of galactic radiation exposure received during 20 years of flying ranged from 0.1 to 5 in 1,000. For the adult U.S. population the risk of dying from cancer is about 220 in 1,000.

Dose-incidence relationships for exencephalia, anophthalmia and prenatal mortality in mouse embryos irradiated with fission neutrons or 250 kV X-rays.

Groups of pregnant mice were irradiated at selected times between 10.00 hours on gestation day 7 and 16.00 hours on day 8. Each group received 0.39 Gy of neutrons or 1.60 Gy of X-rays, or was sham irradiated. We identified a period of high susceptibility of the embryos to radiation-induced exencephalia, anophthalmia and prenatal mortality early in gestation day 8. Dose-incidence relationships in this period were investigated with 0.19-0.48 Gy of neutrons and with 0.40-2.00 Gy of X-rays. With increasing neutron dose, incidence of exencephalia in live embryos rose and then declined. This response suggests that embryos with neutron injury of the type that leads to exencephalia are at a greater risk of dying in utero than are similarly irradiated embryos not so injured, and that this risk increases with dose. A model is proposed that accounts for the shape of the neutron dose-incidence curve. X-ray-induced exencephalia showed only an increase with dose. In X-irradiated litters, almost invariably, the incidence of anophthalmia was higher in exencephalic than in nonexencephalic embryos and the ratio of these incidences (relative risk) decreased toward 1 with increasing dose. A model is proposed that accounts for these observations. The incidence of bilateral anophthalmia in X-irradiated embryos was higher than would be expected if the bilateral form resulted solely from independent injury at each of two equally susceptible sites.

Hymenolepis nana: intestinal tissue phase in actively immunized mice.

We investigated the fate of the intestinal cestode Hymenolepis nana in immunized mice. Immunity was induced by infection with the parasite eggs. These immunized animals and unimmunized controls were then challenged with 50,000 H. nana eggs. The mice were killed 4 to 90 hr after challenge, and H. nana in the intestinal tissue were counted. At 4 hr after challenge the unimmunized and immunized animals had approximately equal numbers of oncospheres. By 12 hr there were fewer parasites in the immunized than in the unimmunized animals. At 90 hr, no H. nana were seen in the immunized mice, whereas in the unimmunized animals the median number of cysticercoids was more than 1,000. It appears, therefore, that in mice well immunized to H. nana by infection, challenge oncospheres can burrow into the intestinal tissue before they are killed. The reduced number of oncospheres in the immunized mice 12 hr after challenge, and the accumulation of eosinophils near individual oncospheres still present, indicate that an immune response to the parasite was taking place. Absence of a lymphocyte infiltration near any of the oncospheres suggests that the mechanism of immunity was not lymphocyte mediated; thus, the histopathology of the reaction is consistent with that of humoral immunity.

Fast-neutron irradiation of mouse embryos in the pronuclear zygote stage: mortality curves and neoplastic diseases in 30-day postnatal survivors.

Mouse embryos in the pronuclear zygote stage were either irradiated in utero with a dose of 15 rad of fast neutrons or were sham-irradiated. Those animals that survived at least 30 days after birth were observed until their natural death. We investigated the percentage incidence and mean age at death for each of the principal neoplastic diseases seen on postmortem examination and also cumulative mortality distributions. No statistically significant differences were found between irradiated and sham-irradiated mice of the same sex.