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

Park, J.M.; Amare, Y.; Anderson, Thomas R.; Angelaszek, D.; Anthony, N.; Arnold, H.; Choi, Gwan Hyun; Copley, M.; Coutu, S.; Derome, L.; Ebongue, C.; Eraud, L.; Faddis, I.; Han, Ji Hye; Howley, I.; Huh, H.G.; Hwang, Yong Seok; Hyun, H.J.; Im, S.; Jeon, H. B.; Jeon, Jin-A; Jeong, Sang Jin; Kang, Sinchul; Kim, D.Y.; Kim, H.J.; Kim, K.C.; Kim, M.H.; King, Philip; Lee, H.Y.; Lee, J.; Lee, M.H.; Liang, Jian‐Gang; Link, J. T.; Lutz, L.; Menchaca‐Rocha, A.; Mitchell, J. W.; Morton, S.; Nester, M.; Nutter, S.; Ofoha, O.; Park, H.; Park, Inah; Picot-Clémente, N.; Seo, E. S.; Smith, Jacob; Walpole, P.; Weinmann, R.; Wu, Jian; Yon, B.; Yoon, Y. S.

doi:10.1016/j.asr.2017.10.037

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“…They have already demonstrated their capabilities of determining the charge and energy of high-energy cosmic rays for the proton to iron elemental range with excellent resolution [6]. In addition, the Top and Bottom Counting Detectors (TCD/BCD) located above and below the CAL, respectively, help electron measurements by using different shower profiles to distinguish electrons from protons [7,8]. They also provide a low energy trigger while the CAL provides a high energy trigger.…”

Section: Instrumentmentioning

confidence: 99%