Space radiation quality factor for Galactic Cosmic Rays and typical space mission scenarios using a microdosimetric approach

Space radiation exposure from omnipresent Galactic Cosmic Rays (GCRs) in interplanetary space poses a serious carcinogenic risk to astronauts due to the—limited or absent—protective effect of the Earth’s magnetosphere and, in particular, the terrestrial atmosphere. The radiation risk is directly inf...

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Veröffentlicht in:Radiation and environmental biophysics 2023-05, Vol.62 (2), p.221-234
Hauptverfasser: Papadopoulos, Alexis, Kyriakou, Ioanna, Incerti, Sébastien, Santin, Giovanni, Nieminen, Petteri, Daglis, Ioannis A., Li, Weibo, Emfietzoglou, Dimitris
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container_issue 2
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container_title Radiation and environmental biophysics
container_volume 62
creator Papadopoulos, Alexis
Kyriakou, Ioanna
Incerti, Sébastien
Santin, Giovanni
Nieminen, Petteri
Daglis, Ioannis A.
Li, Weibo
Emfietzoglou, Dimitris
description Space radiation exposure from omnipresent Galactic Cosmic Rays (GCRs) in interplanetary space poses a serious carcinogenic risk to astronauts due to the—limited or absent—protective effect of the Earth’s magnetosphere and, in particular, the terrestrial atmosphere. The radiation risk is directly influenced by the quality of the radiation, i.e., its pattern of energy deposition at the micron/DNA scale. For stochastic biological effects, radiation quality is described by the quality factor, Q , which can be defined as a function of Linear Energy Transfer (LET) or the microdosimetric lineal energy ( y ). In the present work, the average Q of GCR for different mission scenarios was calculated using a modified version of the microdosimetric Theory of Dual Radiation Action (TDRA). NASA’s OLTARIS platform was utilized to generate the radiation environment behind different aluminum shielding (0–30 g/cm 2 ) for a typical mission scenario in low-earth orbit (LEO) and in deep space. The microdosimetric lineal energy spectra of ions ( Z ≥ 1 ) in 1 μm liquid water spheres were calculated by a generalized analytical model which considers energy-loss fluctuations and δ-ray transport inside the irradiated medium. The present TDRA-based Q -values for the LEO and deep space missions were found to differ by up to 10% and 14% from the corresponding ICRP-based Q -values and up to 3% and 6% from NASA’s Q -model. In addition, they were found to be in good agreement with the Q -values measured in the International Space Station (ISS) and by the Mars Science Laboratory (MSL) Radiation Assessment Detector (RAD) which represent, respectively, a LEO and deep space orbit.
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subjects Aluminum
Astronauts
Biological and Medical Physics
Biological effects
Biophysics
Carcinogens
Cosmic Radiation
Cosmic rays
Deep space
Earth magnetosphere
Earth orbits
Ecosystems
Effects of Radiation/Radiation Protection
Energy spectra
Energy transfer
Environmental Physics
Extraterrestrial radiation
Galactic cosmic rays
Humans
International Space Station
Interplanetary space
Ions
Linear energy transfer (LET)
Low earth orbits
Mathematical models
Monitoring/Environmental Analysis
Original
Original Article
Physics
Physics and Astronomy
Q factors
Radiation
Radiation effects
Radiation Exposure
Radiation shielding
Relative Biological Effectiveness
Space Flight
Space missions
Water
title Space radiation quality factor for Galactic Cosmic Rays and typical space mission scenarios using a microdosimetric approach
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