CALET measurements with cosmic nuclei: expected performances of tracking and charge identification

dc.contributor.authorBrogi, Paolo
dc.contributor.authorMarrocchesi, Pier Simone
dc.contributor.authorMaestro, Paolo
dc.contributor.authorMori, Nicola
dc.contributor.authorCannady, Nicholas
dc.contributor.authorCALET Collaboration
dc.date.accessioned2023-10-20T18:05:39Z
dc.date.available2023-10-20T18:05:39Z
dc.date.issued2016-08-18
dc.descriptionThe 34th International Cosmic Ray Conference; The Hague, The Netherlands; 30 July- 6 August, 2015en_US
dc.description.abstractCALET is a space mission currently in the final phase of preparation for a launch to the International Space Station (ISS), where it will be installed on the Exposed Facility of the Japanese Experiment Module (JEM-EF). In addition to high precision measurements of the electron spectrum, CALET will also perform long exposure observations of cosmic nuclei from proton to iron and will detect trans-iron elements with a dynamic range up to Z = 40. The energy measurement relies on two calorimeter systems: a fine grained imaging calorimeter (IMC) followed by a total absorption calorimeter (TASC) for a total thickness of 30 X₀ and 1.3 proton interaction length. A dedicated module (a charge detector, CHD), placed at the top of the apparatus, identifies the atomic number Z of the incoming cosmic ray. In this paper, the IMC performances in providing tracking capabilities and a redundant charge measurement by multiple ᵈᴱ/dx samples are studied for the case of proton and He identification with a preliminary version of the analysis. The CALET mission is funded by the Japanese Space Agency (JAXA), the Italian Space Agency (ASI), and NASA.en_US
dc.description.sponsorshipThe CALET mission is funded by the Japanese Space Agency (JAXA), the Italian Space Agency (ASI), and NASA.en_US
dc.description.urihttps://pos.sissa.it/236/595/en_US
dc.format.extent8 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m20juk-8obu
dc.identifier.citationBrogi, Paolo, Pier Simone Marrocchesi, Paolo Maestro, and Nicola Mori. “CALET Measurements with Cosmic Nuclei: Expected Performances of Tracking and Charge Identification.” In Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015), 236:595. SISSA Medialab, 2016. https://doi.org/10.22323/1.236.0595.en_US
dc.identifier.urihttps://doi.org/10.22323/1.236.0595
dc.identifier.urihttp://hdl.handle.net/11603/30316
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 Physics Department
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en_US
dc.rightsAttribution-NonCommercial-ShareAlike 1.0 Generic (CC BY-NC-SA 1.0)*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/1.0/*
dc.titleCALET measurements with cosmic nuclei: expected performances of tracking and charge identificationen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955en_US

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