A simulation study of Top and Bottom Counting Detectors in ISS-CREAM experiment for cosmic ray electron physics

energy: high satellite cosmic radiation: energy electron: cosmic radiation time-to-digital converter showers acceleration ISS-CREAM 530 01 natural sciences 7. Clean energy TDC/BCD gamma ray propagation 0103 physical sciences GEANT electron p [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] e/p Separation CREAM Cosmic rays
DOI: 10.1016/j.asr.2017.10.037 Publication Date: 2017-10-31T23:31:17Z
ABSTRACT
Abstract 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.
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