000923005 001__ 923005
000923005 005__ 20151106224856.0
000923005 0247_ $$2DOI$$a10.1016/j.radmeas.2005.01.007
000923005 0248_ $$aoai:cds.cern.ch:923005$$pcerncds:CERN
000923005 041__ $$aeng
000923005 100__ $$aPálfalvia, J K
000923005 245__ $$aCosmic ray studies on the ISS using SSNTD, BRADOS projects, 2001–2003
000923005 260__ $$c2005
000923005 520__ $$aThe BRADOS 1–3 projects were organised by the Russian Space Agency (RZA) between 2001 and 2003. The aim was to study the contribution of the primary galactic cosmic rays and of the secondary particles to the dose received by the crew of the International Space Station (ISS). Several laboratories participated in these experiments. Two different stacks (constructed by the team of the Atomic Energy Research Institute, AERI, Budapest, Hungary) composed of solid-state nuclear track detectors (SSNTD) were exposed inside the Service Module at different locations. The calibrations were made at the CERN high-energy neutron reference field named CERF (Geneva, Swiss). Applying a multiple track etching technique (2–20 h etching time) and a sophisticated image analyser, the secondary neutron dose was deduced. The composition of stacks, the evaluation methods and the results will be presented here or referenced to previous papers.
000923005 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
000923005 690C_ $$aARTICLE
000923005 690C_ $$aCERN
000923005 693__ $$aXX$$eXX
000923005 700__ $$aSzabó, J
000923005 700__ $$aAkatov, Y
000923005 700__ $$aSajó-Bohus, L
000923005 700__ $$aEördögh, I
000923005 710__ $$5CERN?
000923005 773__ $$c428-432$$n2-6$$pRadiat. Meas.$$v40$$y2005
000923005 901__ $$uAt. Energy Res. Inst. Budapest
000923005 901__ $$uInst. Biomed. Probl. Moscow
000923005 901__ $$uUniv. Caracas
000923005 901__ $$uRes. Inst. Tech. Phys. Budapest
000923005 916__ $$sh$$w200603$$ya2005
000923005 960__ $$a13
000923005 961__ $$c20100608$$h1159$$lCER01$$x20060119
000923005 963__ $$aPUBLIC
000923005 970__ $$a002591006CER
000923005 980__ $$aARTICLE