{"created":"2023-05-15T14:36:22.780246+00:00","id":46841,"links":{},"metadata":{"_buckets":{"deposit":"f02dcb40-e0ab-4df3-a218-809ea34816e0"},"_deposit":{"created_by":1,"id":"46841","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"46841"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00046841","sets":["1"]},"author_link":["467268","467267","467265","467264","467269","467266"],"item_8_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2012-10","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"97","bibliographicPageStart":"87","bibliographicVolumeNumber":"689","bibliographic_titles":[{"bibliographic_title":"Nuclear Instruments & Methods in Physics Research Section A"}]}]},"item_8_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The Telescope Array (TA) experiment, located in the western desert of Utah, USA, is designed for the observation of extensive air showers from extremely high energy cosmic rays. The experiment has a surface detector array surrounded by three fluorescence detectors to enable simultaneous detection of shower particles at ground level and fluorescence photons along the shower track. The TA surface detectors and fluorescence detectors started full hybrid observation in March, 2008. In this article we describe the design and technical features of the TA surface detector.","subitem_description_type":"Abstract"}]},"item_8_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Elsevier"}]},"item_8_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"http://www.sciencedirect.com/science/article/pii/S0168900212005931#"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://www.sciencedirect.com/science/article/pii/S0168900212005931#","subitem_relation_type_select":"URI"}}]},"item_8_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0168-9002","subitem_source_identifier_type":"ISSN"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Abu-Zayyad, T."}],"nameIdentifiers":[{"nameIdentifier":"467264","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Nonaka, T."}],"nameIdentifiers":[{"nameIdentifier":"467265","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Uchihori, Y."}],"nameIdentifiers":[{"nameIdentifier":"467266","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"et.al"}],"nameIdentifiers":[{"nameIdentifier":"467267","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"野中 哲生","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"467268","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"内堀 幸夫","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"467269","nameIdentifierScheme":"WEKO"}]}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"The surface detector array of the Telescope Array experiment ","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The surface detector array of the Telescope Array experiment "}]},"item_type_id":"8","owner":"1","path":["1"],"pubdate":{"attribute_name":"公開日","attribute_value":"2014-10-20"},"publish_date":"2014-10-20","publish_status":"0","recid":"46841","relation_version_is_last":true,"title":["The surface detector array of the Telescope Array experiment "],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T23:46:58.415501+00:00"}