Measurements of cosmic-ray proton and helium spectra from the ISS-CREAM experiment

The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) payload was developed to measure the elemental spectra for a charge range of Z = 1 to 26, with an energy range from ∼10^12 to ∼10^15eV. Launched in August 2017, the ISS-CREAM payload successfully collected data for 539 days until February 2019. The ISS-CREAM instrument consists of several particle detectors: a Silicon Charge Detector (SCD) for charge measurements and a calorimeter (CAL) with carbon targets for energy measurements. It also includes a top counting detector (TCD), a bottom counting detector (BCD), and a boronated scintillator detector (BSD) to help separate electrons from protons. For this analysis, SCD and CAL were used for the charge and energy measurement, respectively, while TCD/BCD and CAL were used for the trigger. The ISS-CREAM proton spectrum has been reported in the energy range of 1.6 − 655 TeV. This proton spectrum deviates from a single power-law, softening at ∼ 9 TeV. This study presents the preliminary helium spectrum from the ISS-CREAM experiment in the energy range of 6 TeV to ∼ 1.1 PeV.

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Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.0028
Primary Topic
Solar and Space Plasma Dynamics
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article
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Measurements of cosmic-ray proton and helium spectra from the ISS-CREAM experiment

L. Lutz, Y. C. Chen, H. J. Kim, L. Eraud et al.
Solar and Space Plasma Dynamics
article

Measurements of cosmic-ray proton and helium spectra from the ISS-CREAM experiment

L. Lutz, Y. C. Chen, H. J. Kim, L. Eraud, Siniša Maričić, Gwangho Choi, O. Ofoha, R. Scrandis, Y. S. Yoon, E. S. Seo, D. Angelaszek, J. Lee, M. J. Lee, Il Han Park, H. Park, J. M. Park, M. H. Lee, H. Wu, L. Derome, M.H. Kim, Hongfang Zhang, Jon Paul Lundquist, Y. Amare, Arvind Bagga, A. Menchaca-Rocha, K. C. Kim, R. Weinmann, Alifa Bintha Haque, Zachary Michael Dorris, Jingzhu Wu, S. Aggarwal, J. H. Han, S. C. Kang, M. Copley, S. Pandey, D. P. Bowman, S. Jeong, H.G. Huh, N. Picot-Clémente
article en

Abstract

The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) payload was developed to measure the elemental spectra for a charge range of Z = 1 to 26, with an energy range from ∼10^12 to ∼10^15eV. Launched in August 2017, the ISS-CREAM payload successfully collected data for 539 days until February 2019. The ISS-CREAM instrument consists of several particle detectors: a Silicon Charge Detector (SCD) for charge measurements and a calorimeter (CAL) with carbon targets for energy measurements. It also includes a top counting detector (TCD), a bottom counting detector (BCD), and a boronated scintillator detector (BSD) to help separate electrons from protons. For this analysis, SCD and CAL were used for the charge and energy measurement, respectively, while TCD/BCD and CAL were used for the trigger. The ISS-CREAM proton spectrum has been reported in the energy range of 1.6 − 655 TeV. This proton spectrum deviates from a single power-law, softening at ∼ 9 TeV. This study presents the preliminary helium spectrum from the ISS-CREAM experiment in the energy range of 6 TeV to ∼ 1.1 PeV.

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Solar and Space Plasma Dynamics
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