CALET measurements with cosmic nuclei: expected performances of tracking and charge identification
dc.contributor.author | Brogi, Paolo | |
dc.contributor.author | Marrocchesi, Pier Simone | |
dc.contributor.author | Maestro, Paolo | |
dc.contributor.author | Mori, Nicola | |
dc.contributor.author | Cannady, Nicholas | |
dc.contributor.author | CALET Collaboration | |
dc.date.accessioned | 2023-10-20T18:05:39Z | |
dc.date.available | 2023-10-20T18:05:39Z | |
dc.date.issued | 2016-08-18 | |
dc.description | The 34th International Cosmic Ray Conference; The Hague, The Netherlands; 30 July- 6 August, 2015 | en_US |
dc.description.abstract | CALET 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.sponsorship | The CALET mission is funded by the Japanese Space Agency (JAXA), the Italian Space Agency (ASI), and NASA. | en_US |
dc.description.uri | https://pos.sissa.it/236/595/ | en_US |
dc.format.extent | 8 pages | en_US |
dc.genre | conference papers and proceedings | en_US |
dc.identifier | doi:10.13016/m20juk-8obu | |
dc.identifier.citation | Brogi, 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.uri | https://doi.org/10.22323/1.236.0595 | |
dc.identifier.uri | http://hdl.handle.net/11603/30316 | |
dc.language.iso | en_US | en_US |
dc.publisher | Proceedings of Science | 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 Physics Department | |
dc.rights | This 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.rights | Attribution-NonCommercial-ShareAlike 1.0 Generic (CC BY-NC-SA 1.0) | * |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-sa/1.0/ | * |
dc.title | CALET measurements with cosmic nuclei: expected performances of tracking and charge identification | en_US |
dc.type | Text | en_US |
dcterms.creator | https://orcid.org/0000-0003-2916-6955 | en_US |