{"created":"2023-05-15T14:44:14.344681+00:00","id":60489,"links":{},"metadata":{"_buckets":{"deposit":"aee8080c-cae3-409b-aff7-caef26d57e5d"},"_deposit":{"created_by":1,"id":"60489","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"60489"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00060489","sets":["10:29"]},"author_link":["600481","600480"],"item_10005_date_7":{"attribute_name":"発表年月日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2004-07-25","subitem_date_issued_type":"Issued"}]},"item_10005_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We present preliminary results on the spectrum of high energy\ncosmic-ray electrons as the measured in the flight\nof the Polar Patrol Balloon (PPB) which lasted for 13 days,\nin January,2004 with a launch from Syowa Station, Antarctica.\nThe PPB-BETS (Balloon-borne Electron Telescope with Scintillating\nFiber) detector is designed to measure the cosmic-ray electron spectrum\nfrom 10 GeV to 1 TeV during a long balloon flight.\nIt consists of 9 plates of plastic scinlater as a calorimeter\nand a scintillating fiber trackers for cascade showers\ninduced from high energy electrons and protons\nbetween plates of lead with total 9 radiation length thickness.\nIn this paper, we discuss the perfomance of the detector\nand the preliminary results on the spectrum of cosmic-ray electrons.","subitem_description_type":"Abstract"}]},"item_10005_description_6":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）","attribute_value_mlt":[{"subitem_description":"35th COSPAR SCIENTIFIC ASSEMBLY","subitem_description_type":"Other"}]},"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":"Kitamura, Hisashi"}],"nameIdentifiers":[{"nameIdentifier":"600480","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"北村 尚","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"600481","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":"conference object","resourceuri":"http://purl.org/coar/resource_type/c_c94f"}]},"item_title":"Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica"}]},"item_type_id":"10005","owner":"1","path":["29"],"pubdate":{"attribute_name":"公開日","attribute_value":"2004-07-26"},"publish_date":"2004-07-26","publish_status":"0","recid":"60489","relation_version_is_last":true,"title":["Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T21:53:12.528661+00:00"}