Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10 GeV/n to 2.2 TeV/n with the Calorimetric Electron Telescope on the International Space Station
dc.contributor.author | Adriani, O. | |
dc.contributor.author | Akaike, Y. | |
dc.contributor.author | Asano, K. | |
dc.contributor.author | Asaoka, Y. | |
dc.contributor.author | Cannady, Nicholas | |
dc.contributor.author | Hams, Thomas | |
dc.contributor.author | Krizmanic, John F. | |
dc.contributor.author | Link, J. | |
dc.contributor.author | Sakai, Kenichi | |
dc.contributor.author | CALET Collaboration | |
dc.contributor.author | et al | |
dc.date.accessioned | 2022-08-09T18:01:16Z | |
dc.date.available | 2022-08-09T18:01:16Z | |
dc.date.issued | 2020-12-18 | |
dc.description | Authors: O. Adriani, Y. Akaike, K. Asano, Y. Asaoka, M. G. Bagliesi, E. Berti, G. Bigongiari, W. R. Binns, M. Bongi, P. Brogi, A. Bruno, J. H. Buckley, N. Cannady, G. Castellini, C. Checchia, M. L. Cherry, G. Collazuol, K. Ebisawa, H. Fuke, S. Gonzi, T. G. Guzik, T. Hams, K. Hibino, M. Ichimura, K. Ioka, W. Ishizaki, M. H. Israel, K. Kasahara, J. Kataoka, R. Kataoka, Y. Katayose, C. Kato, N. Kawanaka, Y. Kawakubo, K. Kobayashi, K. Kohri, H. S. Krawczynski, J. F. Krizmanic, J. Link, P. Maestro, P. S. Marrocchesi, A. M. Messineo, J. W. Mitchell, S. Miyake, A. A. Moiseev, M. Mori, N. Mori, H. M. Motz, K. Munakata, S. Nakahira, J. Nishimura, G. A. de Nolfo, S. Okuno, J. F. Ormes, N. Ospina, S. Ozawa, L. Pacini, F. Palma, P. Papini, B. F. Rauch, S. B. Ricciarini, K. Sakai, T. Sakamoto, M. Sasaki, Y. Shimizu, A. Shiomi, R. Sparvoli, P. Spillantini, F. Stolzi, S. Sugita, J. E. Suh, A. Sulaj, M. Takita, T. Tamura, T. Terasawa, S. Torii, Y. Tsunesada, Y. Uchihori, E. Vannuccini, J. P. Wefel, K. Yamaoka, S. Yanagita, A. Yoshida, and K. Yoshida | en_US |
dc.description.abstract | In this paper, we present the measurement of the energy spectra of carbon and oxygen in cosmic rays based on observations with the Calorimetric Electron Telescope on the International Space Station from October 2015 to October 2019. Analysis, including the detailed assessment of systematic uncertainties, and results are reported. The energy spectra are measured in kinetic energy per nucleon from 10 GeV / n to 2.2 TeV / n with an all-calorimetric instrument with a total thickness corresponding to 1.3 nuclear interaction length. The observed carbon and oxygen fluxes show a spectral index change of ∼0.15 around 200 GeV / n established with a significance > 3σ. They have the same energy dependence with a constant C/O flux ratio 0.911±0.006 above 25 GeV / n. The spectral hardening is consistent with that measured by AMS-02, but the absolute normalization of the flux is about 27% lower, though in agreement with observations from previous experiments including the PAMELA spectrometer and the calorimetric balloon-borne experiment CREAM. | en_US |
dc.description.sponsorship | We gratefully acknowledge JAXA’s contributions to the development of CALET and to the operations onboard the International Space Station. We also wish to express our sincere gratitude to Agenzia Spaziale Italiana (ASI) and NASA for their support of the CALET project. This work was supported in part by JSPS Grant-in-Aid for Scientific Research (S) No. 26220708 and No. 19H05608, JSPS Grant-in-Aid for Scientific Research (B) No. 17H02901, and by the MEXT-Supported Program for the Strategic Research Foundation at Private Universities (2011-2015) (No. S1101021) at Waseda University. The CALET effort in Italy is supported by ASI under agreement 2013-018-R.0 and its amendments. The CALET effort in the United States is supported by NASA through Grants No. NNX16AB99G, No. NNX16AC02G, and No. NNH14ZDA001N-APRA0075. | en_US |
dc.description.uri | https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.125.251102 | en_US |
dc.format.extent | 7 pages | en_US |
dc.genre | journal articles | en_US |
dc.identifier | doi:10.13016/m2aabs-qphx | |
dc.identifier.citation | Adriani, O. et al. "Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10 GeV/n to 2.2 TeV/n with the Calorimetric Electron Telescope on the International Space Station." Phys. Rev. Lett. 125, no. 25 (18 December 2020). https://doi.org/10.1103/PhysRevLett.125.251102 | en_US |
dc.identifier.uri | https://doi.org/10.1103/PhysRevLett.125.251102 | |
dc.identifier.uri | http://hdl.handle.net/11603/25325 | |
dc.language.iso | en_US | en_US |
dc.publisher | APS | en_US |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
dc.relation.ispartof | UMBC Faculty Collection | |
dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | en_US |
dc.rights | Public Domain Mark 1.0 | * |
dc.rights.uri | http://creativecommons.org/publicdomain/mark/1.0/ | * |
dc.title | Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10 GeV/n to 2.2 TeV/n with the Calorimetric Electron Telescope on the International Space Station | en_US |
dc.type | Text | en_US |
dcterms.creator | https://orcid.org/0000-0003-2916-6955 | en_US |
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