{"created":"2023-06-20T15:03:31.019918+00:00","id":32732,"links":{},"metadata":{"_buckets":{"deposit":"876e2445-892d-4dc0-be2d-ccb211924f27"},"_deposit":{"created_by":1,"id":"32732","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"32732"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00032732","sets":["1887:1890","1896:1898:1899:1911"]},"author_link":["411248","411245","411246","411247"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Spectroscopic Observation of the Middle Ultraviolet Earth Albedo by S-520-4 Rocket and Mesospheric Ozone Density Profile"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1982-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"12","bibliographicPageStart":"1","bibliographicVolumeNumber":"8","bibliographic_titles":[{"bibliographic_title":"宇宙科学研究所報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"中間紫外域に存在するオゾンハートレー吸収帯を利用したオゾンの定量はロケット・衛星観測で広く行なわれている。我国においても1965年以来, この波長域の太陽光のオゾンによる吸収をロケットに搭載した光電受光器で観測している。一方1984年打ち上げが予定されている EXOS-C に分光器を搭載して, この波長域の地球大気散乱光を分光観測することが計画されている。1981年9月5日 S-520-4 号機により, 衛星搭載用の分光器試験を行なった。この装置で2500A∿3300Aの太陽紫外光の地球大気による散乱光と4030Aの可視散乱光を測定した。分光器は凹面回折格子を用い, 波長分解能は約10Aである。検出器には C_s-Te光電面の光電子増倍管を用いた。一方可視散乱光は干渉フィルターと光電管を用いて測定した。得られた紫外光のスペクトルとモデル計算による値を比較し, オゾン密度の定量を行なった。今回得られた散乱光の強度から推定されるオゾン密度分布は高度30km以上で, 従来内之浦で行なわれた光電受光器による観測結果とほぼ一致した。スペクトル強度について, 2600A以下3100A以上で実測値と計算値に違いが見られた。これはミー散乱及び紫外光の迷光の影響と考えると説明できる。今回の実験で飛翔時における分光器及び検出器の性能が確認できた。","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The ozone Hartey basorption band in the middle ultra-violet range is commonly adopted for the ozone measurement by rocket and satellite observations. In Japan, since 1965 the ozone absorption in the solar ultraviolet radiation has been observed by rocket-borne uv photometers. On the other hand the spectroscopic measurements of the scattered solar ultraviolet radiation from the terrestrial atmosphere will be performed by the EXOS-C satellite which will be launched in 1984. We tested the spectrometer for this satellite experiment by S-520-4 rocket launched on 5 September 1981. This instrument observed the scattered radiation of 2500A∿3300A and the visible earth albedo of 4030 A. The spectrometer is consisted of a concave grating and has about 10A wavelength resolution. A photomultiplier having a Cs-Te photocathode is used as a uv detector. The visible albedo is measured by a photometer consisting of an interference filter and a phototube. We estimated the atmospheric ozone profile, comparing the uv spectrum obtained by this experiment with the model calculations. The estimated ozone density profile higher than 30km altitude has good agreement with the profile obtained by the previous uv photometer experiments at Uchinoura. There are differences between the observed spectrum and the calculated one in ≲ 2600A and ≳ 3100A We can explain them by the effect of Mie scattering and the uv stray light. In the present experiment we could successfully test the functions of the instrument in the space. rocket, spectrometer, solar ultraviolet radiation, earth albedo, ozone","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0166378000","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_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0285-2853","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":"AN00354474","subitem_source_identifier_type":"NCID"}]},"item_9_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学理学部地球物理研究施設"},{"subitem_text_value":"宇宙科学研究所惑星研究系客員部門助教授"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"鈴木, 勝久"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小川, 利紘"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SUZUKI, Katsuhisa","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"OGAWA, Toshihiro","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":"SA0166378.pdf","filesize":[{"value":"780.5 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0166378.pdf","url":"https://jaxa.repo.nii.ac.jp/record/32732/files/SA0166378.pdf"},"version_id":"cbd07bbc-88a6-4472-8861-08bfa9963fc2"}]},"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":"S-520-4 号機による中間紫外大気散乱光観測とオゾン密度","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"S-520-4 号機による中間紫外大気散乱光観測とオゾン密度"}]},"item_type_id":"9","owner":"1","path":["1890","1911"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"32732","relation_version_is_last":true,"title":["S-520-4 号機による中間紫外大気散乱光観測とオゾン密度"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:25:31.357674+00:00"}