Abstract

The health effects of cosmic radiation on astronauts need to be precisely quantified and controlled. This task is important not only in perspective of the increasing human presence at the International Space Station (ISS), but also for the preparation of safe human missions beyond low earth orbit. From a radiation protection point of view, the baseline quantity for radiation risk assessment in space is the effective dose equivalent. The present work reports the first successful attempt of the experimental determination of the effective dose equivalent in space, both for extra-vehicular activity (EVA) and intra-vehicular activity (IVA). This was achieved using the anthropomorphic torso phantom RANDO® equipped with more than 6,000 passive thermoluminescent detectors and plastic nuclear track detectors, which have been exposed to cosmic radiation inside the European Space Agency MATROSHKA facility both outside and inside the ISS. In order to calculate the effective dose equivalent, a numerical model of the RANDO® phantom, based on computer tomography scans of the actual phantom, was developed. It was found that the effective dose equivalent rate during an EVA approaches 700 μSv/d, while during an IVA about 20 % lower values were observed. It is shown that the individual dose based on a personal dosimeter reading for an astronaut during IVA results in an overestimate of the effective dose equivalent of about 15 %, whereas under an EVA conditions the overestimate is more than 200 %. A personal dosemeter can therefore deliver quite good exposure records during IVA, but may overestimate the effective dose equivalent received during an EVA considerably.

Highlights

  • Astronauts living and working on-board the International Space Station (ISS) at altitudes of about 400 km are exposed to radiation levels that are up to two orders of magnitude higher than at sea level

  • DTLD-low represents the average absorbed organ dose rate measured by thermoluminescent detectors (TLDs) for linear energy transfer (LET) \10 keV/lm, and the DPNTD-high represents the absorbed dose rate measured by plastic nuclear track detectors (PNTDs) for LET [10 keV/lm

  • A human torso phantom equipped with radiation detectors was used as part of the MATROSHKA facility to measure the doses at several locations inside and on the ‘skin’ of the phantom, which has been mounted outside the ISS simulating an astronaut during extra-vehicular activity (EVA)

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Summary

Introduction

Astronauts living and working on-board the International Space Station (ISS) at altitudes of about 400 km are exposed to radiation levels that are up to two orders of magnitude higher than at sea level. Radiat Environ Biophys (2014) 53:719–727 and heavy ions (baryon component), with energies from several tens up to 1012 MeV or more, and 2 % electrons and positrons (lepton component). Inside the ISS, a secondary radiation field with a significant contribution of neutrons is produced, due to nuclear interactions of the GCR with the atoms of the shielding material and the human body. The contribution of these sources to the radiation hazard to astronauts varies with the altitude, the solar activity and the local shielding by the ISS itself (NCRP 2000)

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