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Park, J.M.,Amare, Y.,Anderson, T.,Angelaszek, D.,Anthony, N.,Arnold, H.,Choi, G.H.,Copley, M.,Coutu, S.,Derome, L.,Ebongue, C.,Eraud, L.,Faddis, I.,Han, J.H.,Howley, I.J.,Huh, H.G.,Hwang, Y.S.,Hyun, H Elsevier 2018 ADVANCES IN SPACE RESEARCH Vol.62 No.10
<P><B>Abstract</B></P> <P>The Cosmic Ray Energetics and Mass experiment at the International Space Station (ISS-CREAM) is developed for studying the origin, acceleration and propagation mechanism of high energy cosmic rays. The Top and Bottom Counting Detectors (TCD/BCD), sub-detectors of the ISS-CREAM instrument, are developed for electron/ γ -ray physics. The TCD/BCD help distinguish electrons from protons by comparing the hit and shower width distributions for electrons and protons. The e/p separation capability of the TCD/BCD is studied by using the GEANT3 simulation package, and optimal parameters for the e/p separation are obtained.</P>