| Literature DB >> 25899609 |
M B Smith1, S Khulapko2, H R Andrews3, V Arkhangelsky4, H Ing3, M R Koslowksy3, B J Lewis5, R Machrafi5, I Nikolaev6, V Shurshakov4.
Abstract
Bubble detectors have been used to characterise the neutron dose and energy spectrum in several modules of the International Space Station (ISS) as part of an ongoing radiation survey. A series of experiments was performed during the ISS-34, ISS-35, ISS-36 and ISS-37 missions between December 2012 and October 2013. The Radi-N2 experiment, a repeat of the 2009 Radi-N investigation, included measurements in four modules of the US orbital segment: Columbus, the Japanese experiment module, the US laboratory and Node 2. The Radi-N2 dose and spectral measurements are not significantly different from the Radi-N results collected in the same ISS locations, despite the large difference in solar activity between 2009 and 2013. Parallel experiments using a second set of detectors in the Russian segment of the ISS included the first characterisation of the neutron spectrum inside the tissue-equivalent Matroshka-R phantom. These data suggest that the dose inside the phantom is ∼70% of the dose at its surface, while the spectrum inside the phantom contains a larger fraction of high-energy neutrons than the spectrum outside the phantom. The phantom results are supported by Monte Carlo simulations that provide good agreement with the empirical data.Mesh:
Year: 2015 PMID: 25899609 PMCID: PMC4884878 DOI: 10.1093/rpd/ncv181
Source DB: PubMed Journal: Radiat Prot Dosimetry ISSN: 0144-8420 Impact factor: 0.972