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Direct measurement of spectral shape of Cherenkov light using cosmic muons
https://mue.repo.nii.ac.jp/records/809
https://mue.repo.nii.ac.jp/records/80952c6f24b-dd02-4fac-86b0-e4c80df8c3f7
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
Direct measurement of spectral shape of Cherenkov light using cosmic muons (6.1 MB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2019-02-22 | |||||
| タイトル | ||||||
| タイトル | Direct measurement of spectral shape of Cherenkov light using cosmic muons | |||||
| 言語 | ||||||
| 言語 | jpn | |||||
| 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 | |||||
| 著者 |
FUKUDA, Yoshiyuki
× FUKUDA, Yoshiyuki× ANZAI, Daisuke× KAMEI, Yuto× Narengerile× OBATA, Akira× MORIYAMA, Shigetaka× HIRAIDE, Katsuki× OGAWA, Izumi× GUNJI, Takahiro× HAYAMI, Ryohei× TSUKADA, Satoru× KUROSAWA, Shunsuke |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | The spectral pulse shape of Cherenkov lights was directly measured by using cosmic muons. The observed decay times for early and late timing were 5.0 and 5.2ns, respectively. They were actually shorter than the time of scintillation lights which were also measured as 9.3ns and 9.2ns, respectively. However we could not see the difference of the rise time between scintillation and Cherenkov lights. This was due to the slow response of our DAQ equipment, photomultiplier and FADC digitizer | |||||
| 書誌情報 |
宮城教育大学紀要 en : Bulletin of Miyagi University of Education 巻 53, p. 183-192, 発行日 2019-01-31 |
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