The boronated scintillator detector of the ISS-CREAM experiment

Y. Amare; T. Anderson; D. Angelaszek; N. Anthony; K. Cheryian; G. H. Choi; M. Copley; S. Coutu; L. Derome; L. Eraud; L. Hagenau; J. H. Han; H. G. Huh; Y. S. Hwang; H. J. Hyun; S. Im; H. B. Jeon; J. A. Jeon; S. Jeong; S. C. Kang; H. J. Kim; K. C. Kim; M. H. Kim; H. Y. Lee; J. Lee; M. H. Lee; J. Liang; J. T. Link; L. Lu; L. Lutz; A. Menchaca-Rocha; T. Mernik; J. W. Mitchell; S. I. Mognet; S. Morton; M. Nester; S. Nutter; O. Ofoha; H. Park; I. H. Park; J. M. Park; N. Picot-Clémente; R. Quinn; E. S. Seo; J. R. Smith; P. Walpole; R. P. Weinmann; J. Wu; Y. S. Yoon

doi:10.1016/j.nima.2019.162413

The boronated scintillator detector of the ISS-CREAM experiment

Y. Amare
, T. Anderson
, D. Angelaszek
, N. Anthony
, K. Cheryian
, G. H. Choi
, M. Copley
, S. Coutu
, L. Derome
, L. Eraud
, L. Hagenau
, J. H. Han
, H. G. Huh
, Y. S. Hwang
, H. J. Hyun
, S. Im
, H. B. Jeon
, J. A. Jeon
, S. Jeong
, S. C. Kang

H. J. Kim, K. C. Kim, M. H. Kim, H. Y. Lee, J. Lee, M. H. Lee, J. Liang, J. T. Link, L. Lu, L. Lutz, A. Menchaca-Rocha, T. Mernik, J. W. Mitchell, S. I. Mognet, S. Morton, M. Nester, S. Nutter, O. Ofoha, H. Park, I. H. Park, J. M. Park, N. Picot-Clémente, R. Quinn, E. S. Seo, J. R. Smith, P. Walpole, R. P. Weinmann, J. Wu, Y. S. Yoon

Research output: Contribution to journal › Article › peer-review

14 Scopus citations

Abstract

The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) instrument is a next-generation experiment for the direct detection and study of cosmic-ray nuclei and electrons. With a long exposure in low Earth orbit, the experiment will determine the particle fluxes and spectral details of cosmic-ray nuclei from hydrogen to iron, over an energy range of about 10¹² eV to >10¹⁵ eV, and of cosmic-ray electrons over an energy range of about 5 ×10¹⁰ eV to > 10¹³ eV. The instrument was deployed to the ISS in August 2017 on the SpaceX CRS-12 mission. We review the design, implementation and performance of one of the ISS-CREAM detector systems: a boron loaded scintillation detector used in discriminating electron-induced events from the much more abundant cosmic-ray nuclei.

Original language	English (US)
Article number	162413
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	943
DOIs	https://doi.org/10.1016/j.nima.2019.162413
State	Published - Nov 1 2019

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics
Instrumentation

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10.1016/j.nima.2019.162413

Cite this

Amare, Y., Anderson, T., Angelaszek, D., Anthony, N., Cheryian, K., Choi, G. H., Copley, M., Coutu, S., Derome, L., Eraud, L., Hagenau, L., Han, J. H., Huh, H. G., Hwang, Y. S., Hyun, H. J., Im, S., Jeon, H. B., Jeon, J. A., Jeong, S., ... Yoon, Y. S. (2019). The boronated scintillator detector of the ISS-CREAM experiment. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 943, Article 162413. https://doi.org/10.1016/j.nima.2019.162413

@article{2acb8a8f991d4bc2889f637f1510dfdc,

title = "The boronated scintillator detector of the ISS-CREAM experiment",

abstract = "The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) instrument is a next-generation experiment for the direct detection and study of cosmic-ray nuclei and electrons. With a long exposure in low Earth orbit, the experiment will determine the particle fluxes and spectral details of cosmic-ray nuclei from hydrogen to iron, over an energy range of about 1012 eV to >1015 eV, and of cosmic-ray electrons over an energy range of about 5 ×1010 eV to > 1013 eV. The instrument was deployed to the ISS in August 2017 on the SpaceX CRS-12 mission. We review the design, implementation and performance of one of the ISS-CREAM detector systems: a boron loaded scintillation detector used in discriminating electron-induced events from the much more abundant cosmic-ray nuclei.",

author = "Y. Amare and T. Anderson and D. Angelaszek and N. Anthony and K. Cheryian and Choi, \{G. H.\} and M. Copley and S. Coutu and L. Derome and L. Eraud and L. Hagenau and Han, \{J. H.\} and Huh, \{H. G.\} and Hwang, \{Y. S.\} and Hyun, \{H. J.\} and S. Im and Jeon, \{H. B.\} and Jeon, \{J. A.\} and S. Jeong and Kang, \{S. C.\} and Kim, \{H. J.\} and Kim, \{K. C.\} and Kim, \{M. H.\} and Lee, \{H. Y.\} and J. Lee and Lee, \{M. H.\} and J. Liang and Link, \{J. T.\} and L. Lu and L. Lutz and A. Menchaca-Rocha and T. Mernik and Mitchell, \{J. W.\} and Mognet, \{S. I.\} and S. Morton and M. Nester and S. Nutter and O. Ofoha and H. Park and Park, \{I. H.\} and Park, \{J. M.\} and N. Picot-Cl{\'e}mente and R. Quinn and Seo, \{E. S.\} and Smith, \{J. R.\} and P. Walpole and Weinmann, \{R. P.\} and J. Wu and Yoon, \{Y. S.\}",

note = "Publisher Copyright: {\textcopyright} 2019 Elsevier B.V.",

year = "2019",

month = nov,

day = "1",

doi = "10.1016/j.nima.2019.162413",

language = "English (US)",

volume = "943",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier B.V.",

}

Amare, Y, Anderson, T, Angelaszek, D, Anthony, N, Cheryian, K, Choi, GH, Copley, M, Coutu, S, Derome, L, Eraud, L, Hagenau, L, Han, JH, Huh, HG, Hwang, YS, Hyun, HJ, Im, S, Jeon, HB, Jeon, JA, Jeong, S, Kang, SC, Kim, HJ, Kim, KC, Kim, MH, Lee, HY, Lee, J, Lee, MH, Liang, J, Link, JT, Lu, L, Lutz, L, Menchaca-Rocha, A, Mernik, T, Mitchell, JW, Mognet, SI, Morton, S, Nester, M, Nutter, S, Ofoha, O, Park, H, Park, IH, Park, JM, Picot-Clémente, N, Quinn, R, Seo, ES, Smith, JR, Walpole, P, Weinmann, RP, Wu, J & Yoon, YS 2019, 'The boronated scintillator detector of the ISS-CREAM experiment', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 943, 162413. https://doi.org/10.1016/j.nima.2019.162413

TY - JOUR

T1 - The boronated scintillator detector of the ISS-CREAM experiment

AU - Amare, Y.

AU - Anderson, T.

AU - Angelaszek, D.

AU - Anthony, N.

AU - Cheryian, K.

AU - Choi, G. H.

AU - Copley, M.

AU - Coutu, S.

AU - Derome, L.

AU - Eraud, L.

AU - Hagenau, L.

AU - Han, J. H.

AU - Huh, H. G.

AU - Hwang, Y. S.

AU - Hyun, H. J.

AU - Im, S.

AU - Jeon, H. B.

AU - Jeon, J. A.

AU - Jeong, S.

AU - Kang, S. C.

AU - Kim, H. J.

AU - Kim, K. C.

AU - Kim, M. H.

AU - Lee, H. Y.

AU - Lee, J.

AU - Lee, M. H.

AU - Liang, J.

AU - Link, J. T.

AU - Lu, L.

AU - Lutz, L.

AU - Menchaca-Rocha, A.

AU - Mernik, T.

AU - Mitchell, J. W.

AU - Mognet, S. I.

AU - Morton, S.

AU - Nester, M.

AU - Nutter, S.

AU - Ofoha, O.

AU - Park, H.

AU - Park, I. H.

AU - Park, J. M.

AU - Picot-Clémente, N.

AU - Quinn, R.

AU - Seo, E. S.

AU - Smith, J. R.

AU - Walpole, P.

AU - Weinmann, R. P.

AU - Wu, J.

AU - Yoon, Y. S.

PY - 2019/11/1

Y1 - 2019/11/1

N2 - The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) instrument is a next-generation experiment for the direct detection and study of cosmic-ray nuclei and electrons. With a long exposure in low Earth orbit, the experiment will determine the particle fluxes and spectral details of cosmic-ray nuclei from hydrogen to iron, over an energy range of about 1012 eV to >1015 eV, and of cosmic-ray electrons over an energy range of about 5 ×1010 eV to > 1013 eV. The instrument was deployed to the ISS in August 2017 on the SpaceX CRS-12 mission. We review the design, implementation and performance of one of the ISS-CREAM detector systems: a boron loaded scintillation detector used in discriminating electron-induced events from the much more abundant cosmic-ray nuclei.

AB - The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) instrument is a next-generation experiment for the direct detection and study of cosmic-ray nuclei and electrons. With a long exposure in low Earth orbit, the experiment will determine the particle fluxes and spectral details of cosmic-ray nuclei from hydrogen to iron, over an energy range of about 1012 eV to >1015 eV, and of cosmic-ray electrons over an energy range of about 5 ×1010 eV to > 1013 eV. The instrument was deployed to the ISS in August 2017 on the SpaceX CRS-12 mission. We review the design, implementation and performance of one of the ISS-CREAM detector systems: a boron loaded scintillation detector used in discriminating electron-induced events from the much more abundant cosmic-ray nuclei.

UR - https://www.scopus.com/pages/publications/85069559941

UR - https://www.scopus.com/pages/publications/85069559941#tab=citedBy

U2 - 10.1016/j.nima.2019.162413

DO - 10.1016/j.nima.2019.162413

M3 - Article

AN - SCOPUS:85069559941

SN - 0168-9002

VL - 943

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

M1 - 162413

ER -

The boronated scintillator detector of the ISS-CREAM experiment

Abstract

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