2020
DOI: 10.1016/j.lssr.2019.11.002
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A commentary on the impact of modelling results to inform mission planning and shield design

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“…Outside of the Earth's protective magnetosphere, crews are exposed to galactic cosmic rays (GCR) and solar proton events (SPE) that occur when particles emitted by the sun, mostly protons, become accelerated in the interplanetary space due to a coronal mass ejection shock [1]. The exposure to GCR in the form of high-energy (HZE) ions, secondary protons, and neutrons has high linear energy transfer values that evoke complex DNA and other cellular damage [2].…”
Section: Introductionmentioning
confidence: 99%
“…Outside of the Earth's protective magnetosphere, crews are exposed to galactic cosmic rays (GCR) and solar proton events (SPE) that occur when particles emitted by the sun, mostly protons, become accelerated in the interplanetary space due to a coronal mass ejection shock [1]. The exposure to GCR in the form of high-energy (HZE) ions, secondary protons, and neutrons has high linear energy transfer values that evoke complex DNA and other cellular damage [2].…”
Section: Introductionmentioning
confidence: 99%