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Surface detectors of the TAx4 experiment
https://repo.qst.go.jp/records/85645
https://repo.qst.go.jp/records/8564533d1989b-aed7-4076-aa99-be6e1fdbb23b
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2022-02-16 | |||||
タイトル | ||||||
タイトル | Surface detectors of the TAx4 experiment | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Telescope Array Collaboration, The
× Telescope Array Collaboration, The× Yukio, Uchihori× Yukio, Uchihori |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Telescope Array (TA) is the largest ultrahigh energy cosmic-ray (UHECR) observatory in the Northern Hemisphere. It explores the origin of UHECRs by measuring their energy spectrum, arrival-direction distribution, and mass composition using a surface detector (SD) array covering approximately 700 km and fluorescence detector (FD) stations. TA has found evidence for a cluster of cosmic rays with energies greater than 57 EeV. In order to confirm this evidence with more data, it is necessary to increase the data collection rate. We have begun building an expansion of TA that we call TAx4. In this paper, we explain the motivation, design, technical features, and expected performance of the TAx4 SD. We also present TAx4’s current status and examples of the data that have already been collected. | |||||
書誌情報 |
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 巻 1019, p. 165726, 発行日 2021-12 |
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出版者 | ||||||
出版者 | Elsevier | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0168-9002 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1016/j.nima.2021.165726 | |||||
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識別子タイプ | URI | |||||
関連識別子 | https://www.sciencedirect.com/science/article/pii/S0168900221007117#! |