{"created":"2023-06-20T15:03:49.656390+00:00","id":33029,"links":{},"metadata":{"_buckets":{"deposit":"8fef3a0b-71fb-4f57-80e4-192b85dfad2e"},"_deposit":{"created_by":1,"id":"33029","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"33029"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00033029","sets":["1887:1890","1896:1898:1899:1912"]},"author_link":["413481","413475","413479","413487","413491","413484","413483","413477","413478","413494","413488","413493","413490","413486","413485","413482","413495","413476","413480","413492","413489"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Far-Infrared Spectroscopic Observations by Balloon"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1989-03","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"76","bibliographicPageStart":"69","bibliographicVolumeNumber":"23","bibliographic_titles":[{"bibliographic_title":"宇宙科学研究所報告. 特集: 宇宙観測研究報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"われわれは口径50cmの気球搭載赤外線望遠鏡(BIRT)に超流動ヘリウム冷却ファブリ・ペロー分光器を搭載して, 星間空間の比較的暖かい領域から放射される, 遠赤外スペクトル線([CII]158μm, [OI]63μm)の観測に成功した。われわれの観測装置は広がった放射成分の検出に特に威力を発揮し, これらのスペクトル線の放射領域(光解離領域と考えられている)が星生成領域に限られず, 周辺の低温分子ガス中にも広く存在すること, さらに銀河系全体にわたって広く一般的にみられることを明らかにした。また[CII]線の放射エネルギーは全放射エネルギーの0.1∿0.5%にも達し, 星間ガス雲の支配的冷却源であることが証明された。","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Far-infrared spectroscopic observations have been made using a 50cm balloon-borne infrared telescope, a superfluid helium cooled Fabry-Perot spectrometer, and a frequency switching method, which is a newly developped observational technique. Remarkable two-dimensional [CII] line intensity maps constructed from the data show us that the [CII] 158μm line is strongly emitted not only from the photodissociation regions but also from their surrounding regions and from general region of the Galactic Plane. This fact indicates singly ionized carbon ions and carbon ioinizing UV photons should be abundantly distributed in interstellar clouds of the Galactic Plane. Since the energy emitted in form of the [CII] 158μm line can reach up to 0.5% of the total energy output of the clouds, the [CII] line must be one of the dominant coolants of the interstellar cloud.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0166878000","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":"京都大学理学部"},{"subitem_text_value":"京都大学理学部"},{"subitem_text_value":"アリゾナ大学スチュワード天文台"},{"subitem_text_value":"アリゾナ大学スチュワード天文台"},{"subitem_text_value":"東京大学理学部"},{"subitem_text_value":"国立天文台"},{"subitem_text_value":"郵政省通信総合研究所"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"芝井, 広"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"奥田, 治之"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中川, 貴雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松原, 英雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"舞原, 俊憲"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"水谷, 耕平"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"西村, 徹郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小林, 行泰"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"高見, 英樹"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"広本, 宣久"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SHIBAI, Hiroshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"OKUDA, H.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"NAKAGAWA, Takao","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MATSUHARA, Hideo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MAIHARA, T.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MIZUTANI, K.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Low, F.J.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"NISHIMURA, T.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"KOBAYASHI, Y.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"TAKAMI, H.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"HIROMOTO, N.","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":"SA0166878.pdf","filesize":[{"value":"584.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0166878.pdf","url":"https://jaxa.repo.nii.ac.jp/record/33029/files/SA0166878.pdf"},"version_id":"b817c11c-0621-435d-804c-78c57f6a7b5c"}]},"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":"気球による天体遠赤外分光観測","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"気球による天体遠赤外分光観測"}]},"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":"33029","relation_version_is_last":true,"title":["気球による天体遠赤外分光観測"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:17:40.329930+00:00"}