Radiation Risk Assessment Associated With Terrestrial Gamma Ray Flashes for Commercial Flights
Résumé
Terrestrial gamma ray flashes (TGFs) are bursts of high-energy photons produced in thunderstorms. Photons are produced by bremsstrahlung from high-energy electrons, gaining energy through the electric field in the thunderstorm. Both electrons and photons are ionizing radiation and could have an impact on the radiation exposure of commercial aircrews and passengers. Previous works from Dwyer et al. (2010) and Pallu et al. (2021) have quantified doses possibly delivered by TGFs. They showed that the photon doses are sufficiently low so as not to be taken into account in the calculation of the radiation doses received during flights. However, electrons could deliver high doses up to 1 Sv, though in a compact area around the TGF source. In this work, we estimate an upper bound of the probability for a commercial flight to find itself in the electron beam of a TGF. Using the first Fermi-Gamma ray Burst Monitor TGF catalog and both simulated routes between airports as a first step and real flight routes from Air France airline for 2.5 years as a second step, we show that the probability is lower than one aircraft hit every 2 years for the total air traffic. Knowing that we did not take into account altitudes and the fact that pilots usually avoid thunderstorms, it is likely that no aircraft would have been hit by the source of a TGF since the beginning of the commercial aviation.
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JGR Atmospheres - 2023 - Pallu - Radiation Risk Assessment Associated With Terrestrial Gamma Ray Flashes for Commercial.pdf (2.12 Mo)
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