| Radiation Detection |
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Monitoring of crew exposures has been a normal part of the space programme since the dawn of human space exploration. Over the last decades, a broad variety of detector systems has been developed and applied on board different spacecraft, either in the form of passive integrating devices or as active real-time radiation monitors. The effective dose essentially depends on altitude and inclination of the orbit. The highest doses were observed during the high-altitude Shuttle flights at low inclinations with up to 4 mSv per day and during the Apollo programme with ~3 mSv per day. For the purpose of comparison, the mean daily dose on Earth from natural sources of radiation (including radon) is ~7 µSv. Following the recommendations of NRCP Report No. 142, operational radiation monitoring on board the ISS consisting of area monitors and personal dosimeters shall provide experimental data of sufficient accuracy for:
The active area radiation monitoring systems are based on the concepts of microdosimetry, silicon detector technology and ionization chamber principles. As a semi-active device, the Hungarian PILLE system comprises an automated on-board reader for passive thermoluminescence detectors (TLDs) and is applied on a regular base for dose assessment of cosmonauts on extravehicular activity (EVA). The main advantage of active radiation monitors are their real-time data viewing capabilities and built-in ‘radiation alarm functions’. The dosimetric area monitoring data have mostly been achieved by passive devices which do not need a power supply. Such equipment includes TLDs and plastic nuclear track detectors (PNTDs) to assess absorbed dose, ionization density spectra and dose equivalent in space. References and Notes
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