Measurement of High-energy Cosmic-Ray Proton Spectrum from the ISS-CREAM Experiment

Author:

Choi G. H.,Seo E. S.,Aggarwal S.,Amare Y.,Angelaszek D.,Bowman D. P.,Chen Y. C.,Copley M.,Derome L.,Eraud L.,Falana C.,Gerrety A.,Han J. H.,Huh H. G.,Haque A.,Hwang Y. S.,Hyun H. J.,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.,Lu L.ORCID,Lundquist J. P.,Lutz L.,Menchaca-Rocha A.,Ofoha O.,Park H.,Park I. H.ORCID,Park J. M.,Picot-Clemente N.,Scrandis R.,Smith J. R.,Takeishi R.,Vedenkin N.,Walpole P.,Weinmann R. P.,Wu H.,Wu J.,Yin Z.,Yoon Y. S.,Zhang H. G.

Abstract

Abstract The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) experiment successfully recorded data for 539 days from 2017 August to 2019 February. We report the energy spectrum of cosmic-ray protons from the ISS-CREAM experiment at energies from 1.60 × 103 to 6.55 × 105 GeV. The measured spectrum deviates from a single power law. A smoothly broken power-law fit to the data, including statistical and systematic uncertainties, shows the spectral index change at 9.0 × 103 GeV from 2.57 ± 0.03 to 2.82 ± 0.02 with a significance of greater than 3σ. This bump-like structure is consistent with a spectral softening recently reported by the balloon-borne CREAM, DAMPE, and NUCLEON, but ISS-CREAM extends measurements to higher energies.

Funder

National Aeronautics and Space Administration

National Research Foundation of Korea

CNRS ∣ Institut National de Physique Nucléaire et de Physique des Particules

Centre National d’Etudes Spatiales

UNAM ∣ Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México

MSIT ∣ Institute for Information and Communications Technology Promotion

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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