{"created":"2023-06-20T15:03:16.820725+00:00","id":32444,"links":{},"metadata":{"_buckets":{"deposit":"9479a8f9-93aa-489f-b12c-9e50ee1629f0"},"_deposit":{"created_by":1,"id":"32444","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"32444"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00032444","sets":["1887:1890","1896:1898:1899:1910"]},"author_link":["409156","409158","409154","409151","409157","409153","409152","409155"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"The Solar Hydrogen Lyman-alpha Observation by the TAIYO Satellite (TAIYO SXU)"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1978-12","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"4_B","bibliographicPageEnd":"1157","bibliographicPageStart":"1141","bibliographicVolumeNumber":"14","bibliographic_titles":[{"bibliographic_title":"東京大学宇宙航空研究所報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"\"たいよう\"衛星における本観測の目的は,狭帯域イオン箱を用いて,太陽全面からの太陽水素ライマンα線(H Ly-α:1216 Å)の絶対放射照度とその変動を連続観測することである.装置はイオン箱,アクセサリー,エレクトロニクスより成る.イオン箱はMgF_2窓,NOガス入りで,H Ly-α線を含む狭帯域のものである.イオン箱前面に\"2段三角おおい\"を取りつけて,±30°の角度にわたって約1%の誤差内で,イオン箱の指向特性の平坦化を行った.太陽H Ly-α線の絶対放射照度は,打ち上げ時(1975年2月24日)のとき,3.2×10^<11>ケ/cm^2 sec(1 A.U.)の値を得た1975年3月10日から同年9月30日までは平均3.5×10^<11>ケ/cm^2 secで±5%以内でほぼ一定値であった.H Ly-α線と他のインデックス(F_<10.7>,カルシウムプラージュ,フレアー)との相関はあまり見られなかった.地球大気中性水素原子の密度分布を高度約800 kmから3000 kmで得た.地球大気の酸素分子によるH Ly-α線の吸収のプロファイルが観測され,CIRA'72 Mean AtmophereのO_2分布を使い,シミュレーションにより求めた値と比較して,よい一致を得た.","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The absolute intensity of hydrogen Lyman-alpha (H Ly-α:1216 Å) from the total solar disk is currently monitored by an ion chamber as a part of the satellite mission TAIYO. The apparatus consists of an ion chamber with a special mask and associated electronics. The ion chamber with an MgF_2 window and filled with NO gas is sensitive to a narrow spectral band including the H Ly-α line. The special mask serves to keep the angular response of the detector constant at the elevation angle of the sun relative to the plane perpendicular to the spinning axis of the satellite within an error of the order of 1%, when the angle is within ±30°. From the currently observed data, the absolute intensity of the solar H Ly-α was estimated as 3.2×10^<11> photons/cm^2 sec at 1A.U. and constant within ±4.2% during the period from 24 February to 30 September, 1975. No remarkable correlations with other indices such as F_<10.7> and Calcium plage indices were observed. The density distribution of hydrogen atoms in the altitude range from about 800 km to 3000 km was obtained. The observed absorption profiles by oxygen molecules agreed with the simulation curves calculated by referring to the CIRA '72 Mean Atmosphere.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0125697000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"東京大学宇宙航空研究所"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0563-8100","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":"AN00161914","subitem_source_identifier_type":"NCID"}]},"item_9_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"大阪市立大学工学部"},{"subitem_text_value":"大阪市立大学工学部"},{"subitem_text_value":"大阪市立大学原子力基礎研究所"},{"subitem_text_value":"大阪市立大学原子力基礎研究所"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"渡辺, 紀彦"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"東野, 一郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小塩, 高文"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"増岡, 俊夫"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"WATANABE, Norihiko","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"HIGASHINO, Ichiro","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"OSHIO, Takanori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MASUOKA, Toshio","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":"SA0125697.pdf","filesize":[{"value":"737.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0125697.pdf","url":"https://jaxa.repo.nii.ac.jp/record/32444/files/SA0125697.pdf"},"version_id":"f33b2232-55ea-49a7-a9be-43dba4c5d6ad"}]},"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":"<論文>\"たいよう\"衛星による太陽水素ライマンα線の観測(TAIYO SXU)","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"<論文>\"たいよう\"衛星による太陽水素ライマンα線の観測(TAIYO SXU)"}]},"item_type_id":"9","owner":"1","path":["1890","1910"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"32444","relation_version_is_last":true,"title":["<論文>\"たいよう\"衛星による太陽水素ライマンα線の観測(TAIYO SXU)"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:32:14.573028+00:00"}