{"created":"2023-06-20T15:02:46.207800+00:00","id":31852,"links":{},"metadata":{"_buckets":{"deposit":"8713b76e-60bf-40c8-974d-7db48fae9a1c"},"_deposit":{"created_by":1,"id":"31852","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"31852"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00031852","sets":["1887:1890","1896:1898:1899:1910"]},"author_link":["406513","406517","406512","406515","406516","406514"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Rocket Measurements of the 6300Å and 3914Å Dayglow Features"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1966-07","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"3_A","bibliographicPageEnd":"927","bibliographicPageStart":"918","bibliographicVolumeNumber":"2","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":"K9M-9ロケットによる昼間大気光,酸素原子6300Å線およびN_2^+イオンの3914Å帯の測定結果とその理論的解釈.測定は高度78kmないし335kmの間でおこなわれた.6300Å線の全輝度は13KRであったが,そのうと5.5KRは太陽紫外によるO_2シューマンルンゲ解離により,0.55KRはO_2^+およびNO^+イオンと常子の解離再結合によりまた,0.03KRはO原子の電子による熱励起により発輝されたものとおもわれる.このほか280kmより高処に別の6300入線の放射源があるようである.一方O(^1D))のO_2(X^3-Σ_0^-)の非活性化の大きさは200km以下の高度ではいちぢるしく大きく,その反応速変係数は2×10^<-10>cm^3/secと推定された.3914Å帯の全輝度は6.5KRであったが,330kmで3.2KRまで減少した.この発輝機構を太陽放射のN_2^+イオンによる螢光散乱として,N_2^+の密度の高度分布を求めた.またN_2^+イオンの電離層内での消失機構について論じた.","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Rocket results are presented on the OI 6300Å line and on the N_2^+ 3914Å band in the dayglow. An altitude range of 78-335 km is covered. Theoretical interpreta tions are given, using results of simultaneous measurements of electron density and electron temperature. The apparent brightness of the 6300Å line at the base of the emitting region is found to be 13kR, of which 5. 5kR are ascribed to excitation through the SchumannRunge dissociation of O_2 by the solar UV radiations, 0. 55KR to the dissociative recombination of O_2^+and NO^+ ions, and 0. 03KR to the excitation of O by thermal electrons. An additional source of excitation above 280km is suggested. The deactivation of O^D) by O_2(X^3Σ_0^-) is found to be appreciable below 200km, and its rate coefficient is estimated to be 2X10^10cm^3/sec. The apparent brightness of the 3914Å band at the base of the emitting region is found to be 6. 5KR, decreasing to 3. 2KR at 330km. Assuming that fluorescent scattering of solar radiation is the mechanism involved the distribution of N_2 ions is calculated. The rate coefficients for the loss of these ions are hence calculated.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0124909000","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":"東大理学部附属地球物理研究施設:宇宙高級研究所"},{"subitem_text_value":"東大理学部附属地球物理研究施設"},{"subitem_text_value":"東大理学部地球物理学教室"}]},"item_9_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Geophysics Research Laboratory. Faculty of Science. University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Geophysics Research Laboratory. Faculty of Science. University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Geophysics Research Laboratory. Faculty of Science. University of Tokyo"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"永田, 武"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"等松, 隆夫"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小川, 利紘"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"NAGATA, Takesi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"TOHMATSU, Takao","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":"SA0124909.pdf","filesize":[{"value":"686.3 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0124909.pdf","url":"https://jaxa.repo.nii.ac.jp/record/31852/files/SA0124909.pdf"},"version_id":"9c59318c-d6c8-4382-be93-a9546973ed33"}]},"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":"昼間大気光6300Åおよび3914Å放射のロケット観測","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"昼間大気光6300Åおよび3914Å放射のロケット観測"}]},"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":"31852","relation_version_is_last":true,"title":["昼間大気光6300Åおよび3914Å放射のロケット観測"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:48:40.393626+00:00"}