{"created":"2023-06-19T09:36:13.038331+00:00","id":809,"links":{},"metadata":{"_buckets":{"deposit":"d4308851-49ba-4847-aa8f-db8b3b6dc856"},"_deposit":{"created_by":16,"id":"809","owners":[16],"pid":{"revision_id":0,"type":"depid","value":"809"},"status":"published"},"_oai":{"id":"oai:mue.repo.nii.ac.jp:00000809","sets":["1:3:83"]},"author_link":["1756","1754","1760","1757","1420","1758","1252","1755","685","1753","1761","1759"],"item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2019-01-31","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"192","bibliographicPageStart":"183","bibliographicVolumeNumber":"53","bibliographic_titles":[{"bibliographic_title":"宮城教育大学紀要"},{"bibliographic_title":"Bulletin of Miyagi University of Education","bibliographic_titleLang":"en"}]}]},"item_10002_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"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","subitem_description_type":"Abstract"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"FUKUDA, Yoshiyuki"}],"nameIdentifiers":[{"nameIdentifier":"685","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000006334744","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000006334744"}]},{"creatorNames":[{"creatorName":"ANZAI, Daisuke"}],"nameIdentifiers":[{"nameIdentifier":"1753","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000399252642","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000399252642"}]},{"creatorNames":[{"creatorName":"KAMEI, Yuto"}],"nameIdentifiers":[{"nameIdentifier":"1754","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000020107031","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000020107031"}]},{"creatorNames":[{"creatorName":"Narengerile"}],"nameIdentifiers":[{"nameIdentifier":"1252","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000383211291","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000383211291"}]},{"creatorNames":[{"creatorName":"OBATA, Akira"}],"nameIdentifiers":[{"nameIdentifier":"1755","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000383211292","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000383211292"}]},{"creatorNames":[{"creatorName":"MORIYAMA, Shigetaka"}],"nameIdentifiers":[{"nameIdentifier":"1756","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000242354735","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000242354735"}]},{"creatorNames":[{"creatorName":"HIRAIDE, Katsuki"}],"nameIdentifiers":[{"nameIdentifier":"1757","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000399807192","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000399807192"}]},{"creatorNames":[{"creatorName":"OGAWA, Izumi"}],"nameIdentifiers":[{"nameIdentifier":"1420","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000242354736","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000242354736"}]},{"creatorNames":[{"creatorName":"GUNJI, Takahiro"}],"nameIdentifiers":[{"nameIdentifier":"1758","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000000796441","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000000796441"}]},{"creatorNames":[{"creatorName":"HAYAMI, Ryohei"}],"nameIdentifiers":[{"nameIdentifier":"1759","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000383211296","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000383211296"}]},{"creatorNames":[{"creatorName":"TSUKADA, Satoru"}],"nameIdentifiers":[{"nameIdentifier":"1760","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000263068282","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000263068282"}]},{"creatorNames":[{"creatorName":"KUROSAWA, Shunsuke"}],"nameIdentifiers":[{"nameIdentifier":"1761","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000256907093","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000256907093"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2019-02-22"}],"displaytype":"detail","filename":"Direct measurement of spectral shape of Cherenkov light using cosmic muons.pdf","filesize":[{"value":"6.1 MB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"Direct measurement of spectral shape of Cherenkov light using cosmic muons","url":"https://mue.repo.nii.ac.jp/record/809/files/Direct measurement of spectral shape of Cherenkov light using cosmic muons.pdf"},"version_id":"474263a6-6601-4fff-9217-646450f53413"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Direct measurement of spectral shape of Cherenkov light using cosmic muons","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Direct measurement of spectral shape of Cherenkov light using cosmic muons"}]},"item_type_id":"10002","owner":"16","path":["83"],"pubdate":{"attribute_name":"公開日","attribute_value":"2019-02-22"},"publish_date":"2019-02-22","publish_status":"0","recid":"809","relation_version_is_last":true,"title":["Direct measurement of spectral shape of Cherenkov light using cosmic muons"],"weko_creator_id":"16","weko_shared_id":-1},"updated":"2023-06-19T09:59:27.378573+00:00"}