Measurements of Heavy Cosmic Ray Nuclei Fluxes with CALET

dc.contributor.authorAkaike, Yosui
dc.contributor.authorCannady, Nicholas
dc.contributor.authorHams, Thomas
dc.contributor.authorKrizmanic, John F.
dc.contributor.authorSakai, Kenichi
dc.contributor.authorCALET Collaboration
dc.contributor.authoret al
dc.date.accessioned2019-10-23T14:48:47Z
dc.date.available2019-10-23T14:48:47Z
dc.date.issued2019-07-24
dc.descriptionCALET Collaboration Authors: O. Adriani, Y. Akaike, K. Asano, Y. Asaoka, 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, A. W. Ficklin, 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, 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, P. Papini, B. F. Rauch, S. B. Ricciarini, K. Sakai, T. Sakamoto, M. Sasaki, Y. Shimizu, A. Shiomi, P. Spillantini, F. Stolzi, S. Sugita, 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, K. Yoshida, and W. V. Zober
dc.description36th International Cosmic Ray Conference -ICRC2019- July 24th – August 1st, 2019, Madison, WI, U.S.A.en
dc.description.abstractThe CALorimetric Electron Telescope (CALET) has been measuring high-energy cosmic rays on the International Space Station since October 2015. One of the scientific objectives is the precise measurements of the boron-to-carbon flux ratio and the energy spectra of nuclei to investigate the cosmic-ray acceleration and propagation in the Galaxy. The instrument has capabilities to identify individual nuclei elements up through Iron with excellent charge resolution and cover the wide energy range from 10 GeV to a PeV. In this paper, we will present the details about the analysis of nuclei measurements and preliminary results of boron-to-carbon flux ratio and energy spectra of heavy nuclei components up to Iron based on three years of operations.en
dc.description.urihttps://pos.sissa.it/358/034/pdfen
dc.format.extent8 pagesen
dc.genreconference papers and proceedingsen
dc.identifierdoi:10.13016/m2ci2u-jpbe
dc.identifier.citation“Measurements of Heavy Cosmic Ray Nuclei Fluxes with CALET,” Y. Akaike for the CALET Collaboration, Proceedings of Science: 36th International Cosmic Ray Conference , (Madison, WI), 034 (2019). https://doi.org/10.22323/1.358.0034en
dc.identifier.urihttp://hdl.handle.net/11603/15959
dc.identifier.urihttps://doi.org/10.22323/1.358.0034
dc.language.isoenen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis 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.
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/*
dc.subjectCALorimetric Electron Telescopeen
dc.subjectboron-to-carbon fluxen
dc.subjectcharge resolutionen
dc.subjectnuclei measurementsen
dc.subjectenergy spectraen
dc.titleMeasurements of Heavy Cosmic Ray Nuclei Fluxes with CALETen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-9489-1515
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955

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