{"created":"2023-06-20T15:03:56.511860+00:00","id":33144,"links":{},"metadata":{"_buckets":{"deposit":"c9dd6eb8-ced5-4771-adc1-c28daecc6ec6"},"_deposit":{"created_by":1,"id":"33144","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"33144"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00033144","sets":["1887:1890","1896:1898:1899:1912"]},"author_link":["414506","414507","414515","414517","414505","414510","414511","414512","414518","414514","414509","414516","414513","414508"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Balloon-borne Infrared Carbon Explorer : A System Customized for the Survey of the Far-Infrared [CII] Line"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1992-02","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"113","bibliographicPageStart":"83","bibliographicVolumeNumber":"30","bibliographic_titles":[{"bibliographic_title":"宇宙科学研究所報告. 特集: 大気球研究報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"遠赤外線[CII]スペクトル線を広域にわたって効率よく観測することを目的として, 専用の気球搭載観測装置BICE (Balloon-borne Infrared Carbon Explorer) を開発した。気球高度からの天体遠赤外線観測の場合, 最大のノイズとなるのは, 観測機器自身が放射する赤外線(背景放射光)の揺らぎによるものである。我々の観測システムBICEでは, (1)オフセット・オーバーサイズ光学系を採用した超低背景放射望遠鏡, (2)超流動液体ヘリウムで全光学系を冷却したファブリ・ペロー分光器, この両者を採用することにより, 背景放射光を大幅に削減し, [CII]スペクトル線検出能力を大幅に向上させた。一方, 観測に直接関係がない部分については, 簡素化をはかり, システムとしての信頼性を向上させることに留意した。BICEシステムを用いた観測を, 1991年春季に, 米国NSBF (National Scientific Balloon Facility)から行い, 極めて良質の観測データを得ることができた。","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The far-infrared [CII] line is a dominant coolant of neutral clouds and photodissociation regions. In order to make large scale survey observations of the [CII] line, we have built a new balloon-borne observing system called BICE (Balloon-borne Infrared Carbon Explorer). The BICE is a special system customized for the large-scale [CII] observations. Its telescope system consists of a off-set and over-sized optics. Its focal plane instrument is a Fabry-Perot spectrometer whose all optics are cooled with super-fluid liquid Helium. With these devices, the background radiation of the BICE system has been dramatically reduced, and thus the BICE has achieved an excellent sensitivity. We made two successful flights of the BICE in 1991 from Texas, U.S.A. The whole emissivity of the BICE system was measured to as low as 3.2%","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0167028000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙科学研究所"}]},"item_9_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0285-9920","subitem_source_identifier_type":"ISSN"}]},"item_9_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AN00354485","subitem_source_identifier_type":"NCID"}]},"item_9_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"宇宙科学研究所"},{"subitem_text_value":"宇宙科学研究所:東京大学理学部"},{"subitem_text_value":"宇宙科学研究所:東京大学理学部"},{"subitem_text_value":"宇宙科学研究所"},{"subitem_text_value":"宇宙科学研究所"},{"subitem_text_value":"宇宙科学研究所"},{"subitem_text_value":"宇宙科学研究所"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"中川, 貴雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"山下, 由香利"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"土井, 靖生"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"奥田, 治之"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"矢島, 信之"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"芝井, 広"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"成田, 正直"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakagawa, Takao","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yamashita, Jukali","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Doi, Yasuo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Okuda, Haruyuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yajima, Nobuyuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Shibai, Hiroshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Narita, Masanao","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-01-24"}],"displaytype":"detail","filename":"SA0167028.pdf","filesize":[{"value":"1.8 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0167028.pdf","url":"https://jaxa.repo.nii.ac.jp/record/33144/files/SA0167028.pdf"},"version_id":"c9da5d5a-759f-4774-8294-b4e6d79103a4"}]},"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":"遠赤外 [CII] スペクトル線サーベイ望遠鏡 BICE","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"遠赤外 [CII] スペクトル線サーベイ望遠鏡 BICE"}]},"item_type_id":"9","owner":"1","path":["1890","1912"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"33144","relation_version_is_last":true,"title":["遠赤外 [CII] スペクトル線サーベイ望遠鏡 BICE"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:14:30.969891+00:00"}