The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument
International audience The ISS-CREAM instrument is the modified version of the Cosmic Ray Energetics And Mass (CREAM) experiment, which was flown on balloons multiple times over Antarctica and later installed on the International Space Station (ISS). Its primary objective is to measure the energy sp...
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ftunigrenoble:oai:HAL:hal-04474635v1 2024-05-19T07:30:10+00:00 The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument Yoon, Y.S Amare, Y 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 Kang, S.C Kim, H.J Kim, K.C Kim, M.H Lee, H.Y Lee, J Lee, M.H Liang, J Lu, L Lutz, L Menchaca-Rocha, A Mitchell, J.W Mognet, S.I Morton, S Nester, M Nutter, S Park, H Park, I.H Park, J.M Picot-Clémente, N Seo, E.S Smith, J.R Walpole, P Weinmann, R.P Wu, J Zhang, H.G Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ) Université Grenoble Alpes (UGA) 2024 https://hal.science/hal-04474635 https://doi.org/10.1016/j.astropartphys.2024.102947 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2024.102947 hal-04474635 https://hal.science/hal-04474635 doi:10.1016/j.astropartphys.2024.102947 INSPIRE: 2760970 Astropart.Phys. https://hal.science/hal-04474635 Astropart.Phys., 2024, 158, pp.102947. ⟨10.1016/j.astropartphys.2024.102947⟩ hadron CREAM Cosmic-ray instrument Direct measurements International space station TeV Elemental spectra measurements elements cosmic radiation charge time multiple satellite scintillation counter electron pixel silicon trigger energy spectrum calorimeter performance tungsten electronics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2024 ftunigrenoble https://doi.org/10.1016/j.astropartphys.2024.102947 2024-04-25T00:15:55Z International audience The ISS-CREAM instrument is the modified version of the Cosmic Ray Energetics And Mass (CREAM) experiment, which was flown on balloons multiple times over Antarctica and later installed on the International Space Station (ISS). Its primary objective is to measure the energy spectra of individual cosmic-ray elements for the charge range of Z = 1 to Z = 26, in the energy range of ∼ 10 12 to ∼ 10 15 eV. The instrument comprises a tungsten/scintillator calorimeter and a pixelated silicon charge detector as primary detectors to determine the energy and charge of cosmic rays. Additionally, it includes top and bottom scintillator counting detectors and a boronated scintillator detector to differentiate between electrons and hadrons for multi-TeV electron measurements. The ISS-CREAM instrument was installed on the ISS in August 2017 and operated until February 2019. This paper provides an overview of the instrument, focusing on its detectors, trigger systems, common electronics, and power systems. The paper highlights the modifications made to these components to optimize their performance for ISS operations. Article in Journal/Newspaper Antarc* Antarctica Université Grenoble Alpes: HAL Astroparticle Physics 158 102947 |
institution |
Open Polar |
collection |
Université Grenoble Alpes: HAL |
op_collection_id |
ftunigrenoble |
language |
English |
topic |
hadron CREAM Cosmic-ray instrument Direct measurements International space station TeV Elemental spectra measurements elements cosmic radiation charge time multiple satellite scintillation counter electron pixel silicon trigger energy spectrum calorimeter performance tungsten electronics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
hadron CREAM Cosmic-ray instrument Direct measurements International space station TeV Elemental spectra measurements elements cosmic radiation charge time multiple satellite scintillation counter electron pixel silicon trigger energy spectrum calorimeter performance tungsten electronics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Yoon, Y.S Amare, Y 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 Kang, S.C Kim, H.J Kim, K.C Kim, M.H Lee, H.Y Lee, J Lee, M.H Liang, J Lu, L Lutz, L Menchaca-Rocha, A Mitchell, J.W Mognet, S.I Morton, S Nester, M Nutter, S Park, H Park, I.H Park, J.M Picot-Clémente, N Seo, E.S Smith, J.R Walpole, P Weinmann, R.P Wu, J Zhang, H.G The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument |
topic_facet |
hadron CREAM Cosmic-ray instrument Direct measurements International space station TeV Elemental spectra measurements elements cosmic radiation charge time multiple satellite scintillation counter electron pixel silicon trigger energy spectrum calorimeter performance tungsten electronics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience The ISS-CREAM instrument is the modified version of the Cosmic Ray Energetics And Mass (CREAM) experiment, which was flown on balloons multiple times over Antarctica and later installed on the International Space Station (ISS). Its primary objective is to measure the energy spectra of individual cosmic-ray elements for the charge range of Z = 1 to Z = 26, in the energy range of ∼ 10 12 to ∼ 10 15 eV. The instrument comprises a tungsten/scintillator calorimeter and a pixelated silicon charge detector as primary detectors to determine the energy and charge of cosmic rays. Additionally, it includes top and bottom scintillator counting detectors and a boronated scintillator detector to differentiate between electrons and hadrons for multi-TeV electron measurements. The ISS-CREAM instrument was installed on the ISS in August 2017 and operated until February 2019. This paper provides an overview of the instrument, focusing on its detectors, trigger systems, common electronics, and power systems. The paper highlights the modifications made to these components to optimize their performance for ISS operations. |
author2 |
Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ) Université Grenoble Alpes (UGA) |
format |
Article in Journal/Newspaper |
author |
Yoon, Y.S Amare, Y 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 Kang, S.C Kim, H.J Kim, K.C Kim, M.H Lee, H.Y Lee, J Lee, M.H Liang, J Lu, L Lutz, L Menchaca-Rocha, A Mitchell, J.W Mognet, S.I Morton, S Nester, M Nutter, S Park, H Park, I.H Park, J.M Picot-Clémente, N Seo, E.S Smith, J.R Walpole, P Weinmann, R.P Wu, J Zhang, H.G |
author_facet |
Yoon, Y.S Amare, Y 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 Kang, S.C Kim, H.J Kim, K.C Kim, M.H Lee, H.Y Lee, J Lee, M.H Liang, J Lu, L Lutz, L Menchaca-Rocha, A Mitchell, J.W Mognet, S.I Morton, S Nester, M Nutter, S Park, H Park, I.H Park, J.M Picot-Clémente, N Seo, E.S Smith, J.R Walpole, P Weinmann, R.P Wu, J Zhang, H.G |
author_sort |
Yoon, Y.S |
title |
The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument |
title_short |
The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument |
title_full |
The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument |
title_fullStr |
The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument |
title_full_unstemmed |
The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument |
title_sort |
cosmic ray energetics and mass for the international space station (iss-cream) instrument |
publisher |
HAL CCSD |
publishDate |
2024 |
url |
https://hal.science/hal-04474635 https://doi.org/10.1016/j.astropartphys.2024.102947 |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
Astropart.Phys. https://hal.science/hal-04474635 Astropart.Phys., 2024, 158, pp.102947. ⟨10.1016/j.astropartphys.2024.102947⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2024.102947 hal-04474635 https://hal.science/hal-04474635 doi:10.1016/j.astropartphys.2024.102947 INSPIRE: 2760970 |
op_doi |
https://doi.org/10.1016/j.astropartphys.2024.102947 |
container_title |
Astroparticle Physics |
container_volume |
158 |
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102947 |
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1799484250542571520 |