Observation of the Energy Spectra of Cosmic Ray Nuclei 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.accessioned2022-08-11T20:17:14Z
dc.date.available2022-08-11T20:17:14Z
dc.date.issued2020-04-18
dc.descriptionAPS April Meeting 2020, Saturday–Tuesday, April 18–21, 2020; Washington D.C.en_US
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.description.abstractObservation of the Energy Spectra of Cosmic Ray Nuclei with CALET YOSUI AKAIKE, NASA/GSFC/CRESST/UMBC, CALET COLLABORATION — The Calorimetric Electron Telescope, CALET, onboard the International Space Station has been collecting scientific data since October 2015. CALET is performing a precise measurement of the cosmic ray electron spectrum in the TeV region as well as measuring nuclear spectra from protons to iron in the range from a few tens of GeV to the PeV scale. These allow for the investigation of the details of their acceleration and propagation mechanisms in the Galaxy. The features of the CALET instrument include excellent charge resolution of 0.18e for carbon and 0.30e for iron based on the segmented scintillator paddles and scintillating fibers and energy resolution of 30 - 40 % for hadrons provided by its 30Xo thick calorimeter. The details about the analysis procedure of nuclei measurements, comparison with our Monte Carlo simulations and preliminary results of the energy spectra for nuclei up to 100 TeV with four years of operations will be presented.en_US
dc.description.sponsorshipThis effort is supported by NASA in the United States, by JAXA in Japan and ASI in Italy.en_US
dc.description.urihttps://meetings.aps.org/Meeting/APR20/Session/B09.9en_US
dc.format.extent13 pagesen_US
dc.genrepresentations (communicative events)en_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2xfby-yjpd
dc.identifier.urihttp://hdl.handle.net/11603/25365
dc.language.isoen_USen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
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.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.subjectCALorimetric Electron Telescope (CALET)en_US
dc.subjectCosmic ray Nucleien_US
dc.subjectmeasurement of the cosmic ray electron spectrum in the TeV
dc.subjectInternational Space Station
dc.titleObservation of the Energy Spectra of Cosmic Ray Nuclei with CALETen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-9489-1515en_US
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955en_US

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