Measurement of iron cosmic-ray primaries below 10 GeV/n by use of the geomagnetic effect with CALET

dc.contributor.authorIchimura, M.
dc.contributor.authorKasahara, K.
dc.contributor.authorCannady, Nicholas
dc.contributor.authorHams, T.
dc.contributor.authorSakai, K.
dc.contributor.authorCALET Collaboration
dc.contributor.authoret al.
dc.date.accessioned2023-08-18T17:48:18Z
dc.date.available2023-08-18T17:48:18Z
dc.date.issued2023-07-25
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, N. Cannady, G. Castellini, C. Checchia, M.L. Cherry, G. Collazuol, G.A. de Nolfo, 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, S. Okuno, J.F. Ormes, 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. Zoberen_US
dc.description38th International Cosmic Ray Conference (ICRC2023), Nagoya, Japan, 26 July - 3 August, 2023
dc.description.abstractThe CALET Calorimeter on the International Space Station(ISS) has previously measured the flux and spectrum of iron cosmic-ray nuclei above 10 GeV/n. In order to extend the measurement to the region below 10 GeV/n, we carry out an analysis to utilize the geomagnetic effect. Cutoff rigidities of cosmic-ray nuclei are calculated for all directions for each observation point in the ISS orbit. The integral spectrum of observed rigidities is then obtained by counting the number of iron nuclei in each bin of cutoff rigidity. The absolute flux and differential spectrum are then calculated by taking the detection efficiencies into account. Here we present the details of the analysis procedure and the iron spectrum below 10 GeV/n. en_US
dc.description.sponsorshipWe gratefully acknowledge JAXA’s contributions to the development of CALET and to the operations onboard the International Space Station. The CALET effort in Italy is supported by ASI under Agreement No. 2013- 018-R.0 and its amendments. The CALET effort in the United States is supported by NASA through Grants No. 80NSSC20K0397, No. 80NSSC20K0399, and No. NNH18ZDA001N-APRA18-0004. This work is supported in part by JSPS Grant-in-Aid for Scientific Research (S) Grant No. 19H05608 and (C) Grant No. 20K03982 in Japan.en_US
dc.description.urihttps://pos.sissa.it/444/057en_US
dc.format.extent9 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2fhhv-swcf
dc.identifier.citationIchimura, M., et al. "Measurement of iron cosmic-ray primaries below 10 GeV/n by use of the geomagnetic effect with CALET." Paper presented at 38th International Cosmic Ray Conference (ICRC2023) 26 July - 3 August, 2023 instrument Nagoya, Japan. https://doi.org/10.22323/1.444.0057.en_US
dc.identifier.urihttps://doi.org/10.22323/1.444.0057
dc.identifier.urihttp://hdl.handle.net/11603/29280
dc.language.isoen_USen_US
dc.publisherProceedings of Scienceen_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.||Public Domain en_US
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleMeasurement of iron cosmic-ray primaries below 10 GeV/n by use of the geomagnetic effect with CALETen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955en_US

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