WEKO3
アイテム
Fluorescence yields in determination of primary cosmic ray energy
https://doi.org/10.57375/00000954
https://doi.org/10.57375/00000954acd19421-7934-41e1-b06e-5c195f402d76
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
kiyou3948.pdf (4.7 MB)
|
|
| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2009-11-30 | |||||
| タイトル | ||||||
| タイトル | Fluorescence yields in determination of primary cosmic ray energy | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | cosmic | |||||
| 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 | departmental bulletin paper | |||||
| ID登録 | ||||||
| ID登録 | 10.57375/00000954 | |||||
| ID登録タイプ | JaLC | |||||
| 著者 |
Nagano, Motohiko
× Nagano, Motohiko |
|||||
| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | The experiments on the search for the end of the cosmic ray energy spectrum are summarized. In estimation of the primary cosmic ray energy by the fluorescence technique, the determination of fluorescence yields in air is most important. If the preliminary yield at 337nm by AIRFLY measurement is used for Flys' Eye, HiRes and Auger, the di erences of primary spectra among experiments are within experimental errors of each experiment, including su ace detector array experiment AGASA. In order to establish the energy scale, it is most important to determine the absolute fluorescence yield at 337 nm to understand the optical technique further. | |||||
| 書誌情報 | 号 39, p. 352-359, 発行日 2009-08-01 | |||||
| 出版者 | ||||||
| 出版者 | 福井工業大学 | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 18844502 / 18844456 | |||||
| 書誌レコードID | ||||||
| 識別子タイプ | NCID | |||||
| 関連識別子 | TF00009413 | |||||
| 著者版フラグ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
