Abstract

Health risks from radiation exposure in space are an important factor for astronauts’ safety as they venture on long-duration missions to the Moon or Mars. It is important to assess the radiation level inside the human brain to evaluate the possible hazardous effects on the central nervous system especially during solar energetic particle (SEP) events. We use a realistic model of the head/brain structure and calculate the radiation deposit therein by realistic SEP events, also under various shielding scenarios. We then determine the relation between the radiation dose deposited in different parts of the brain and the properties of the SEP events and obtain some simple and ready-to-use functions which can be used to quickly and reliably forecast the event dose in the brain. Such a novel tool can be used from fast nowcasting of the consequences of SEP events to optimization of shielding systems and other mitigation strategies of astronauts in space.

Highlights

  • The dose-fluence relationships are shown for proton in different energies for each scenario to determine the best correlation coefficient, and the pivot energy

  • Using this function and parameter for each scenario, one can quickly calculate the SEP events induced dose at a certain part of the brain or the human head considering the different thickness of shielding around, given the intensity of the SEP events at the pivot energy

  • These results show that the pivot energy in the a human head with 10 cm of Al as a shield is about 300 MeV, which is the same as the pivot energy on the surface of Mars with ∼ 22 g/cm2 of vertical column depth of CO239

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Summary

Introduction

The dose-fluence relationships are shown for proton in different energies for each scenario to determine the best correlation coefficient, and the pivot energy. Using this function and parameter for each scenario, one can quickly calculate the SEP events induced dose at a certain part of the brain or the human head considering the different thickness of shielding around, given the intensity of the SEP events at the pivot energy.

Results
Conclusion
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