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The Telescope Array Experiment: An Overview aand Physics Aims
https://repo.qst.go.jp/records/53274
https://repo.qst.go.jp/records/53274bea00360-d104-4190-ae37-3a4bf2a258a3
| Item type | 会議発表論文 / Conference Paper(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2004-01-07 | |||||
| タイトル | ||||||
| タイトル | The Telescope Array Experiment: An Overview aand Physics Aims | |||||
| 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_5794 | |||||
| 資源タイプ | conference paper | |||||
| 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 |
Arai, Yasuo
× Arai, Yasuo× Fukushima, Masaki× Uchihori, Yukio× Yasuda, Nakahiro× et.al× 内堀 幸夫× 安田 仲宏 |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | The Telescope Array (TA) experiment plans to deploy an array of 10 telescope stations in the west desert of Utah, USA and observes extremely high energy cosmic rays (EHECRs) by the atmospheric fluorescence. Its purpose is to study super-GZK (E > 10^20 eV) cosmic rays discovered by AGASA. In order to identify the origin of super-GZK events, TA has ~30 times larger aperture than AGASA and provides a particle identification by the shower profile measurement. The first step of construction will start as a hybrid detector with an AGASA/10 ground array and a part of fluorescence telescopes, which will unambiguously establish the existence of super-GZK and cluster events with much improved statistics and systematics. This paper describes the physics of TA and its overall planning. | |||||
| 書誌情報 |
Proceedings of International Cosmic Ray Conference p. 1025-1028, 発行日 2003-06 |
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