{"created":"2023-07-25T11:04:18.187320+00:00","id":7388,"links":{},"metadata":{"_buckets":{"deposit":"ae73f81b-c41e-4886-a33c-80278d8f4589"},"_deposit":{"created_by":4,"id":"7388","owners":[4],"pid":{"revision_id":0,"type":"depid","value":"7388"},"status":"published"},"_oai":{"id":"oai:nipr.repo.nii.ac.jp:00007388","sets":["1259:906:931"]},"author_link":["12644","11442","12015","11441","11826","11433","11430","11440","11444","11443"],"item_1_alternative_title_5":{"attribute_name":"論文名よみ","attribute_value_mlt":[{"subitem_alternative_title":"1961ネン ノ エットウ カンソク カラ ミタ ショウワ キチ ニオケル デンリソウ キョクコウ オヨビ チジキ ヘンカ ノ ソウゴ カンケイ"}]},"item_1_biblio_info_14":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1965-10","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"2023","bibliographicPageStart":"1993","bibliographicVolumeNumber":"25","bibliographic_titles":[{"bibliographic_title":"南極資料"}]}]},"item_1_creator_6":{"attribute_name":"著者名(日)","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"川尻, 矗大"},{"creatorName":"カワジリ, ノブヒロ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"若井, 登"},{"creatorName":"ワカイ, ノボル","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中村, 純二"},{"creatorName":"ナカムラ, ジュンジ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中村, 強"},{"creatorName":"ナカムラ, ツヨシ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"長谷川, 貞雄"},{"creatorName":"ハセガワ, サダオ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]}]},"item_1_creator_8":{"attribute_name":"著者名(英)","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"KAWAJIRI, Nobuhiro","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"WAKAI, Noboru","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"NAKAMURA, Junji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"NAKAMURA, Tsuyoshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"HASEGAWA, Sadao","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_1_description_1":{"attribute_name":"ページ属性","attribute_value_mlt":[{"subitem_description":"P(論文)","subitem_description_type":"Other"}]},"item_1_description_12":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"Ionospheric, auroral and geomagnetic observations were made simultaneously at Syowa Station during the fifth wintering of the Japanese Antarctic Research Expedition in 1961 The ionospheric soundings at vertical incidence were carried out every fifteen minutes. Auroras were measured by photometric technique for the three lines, λ5577A (OI (S-D) line), λ6300A (OI (D-P) line and λ4278A (N G of N_2^+ (0-1) band), and the magnetogram from which the magnetic Qindices were reduced, was obtained by a magnetometer of pen-recording type Based on these data obtained during the winter months, the expressions for the relation between auroral luminosity (J in kR) and electron density (N in electrons/cm^3) in the E region were calculated in the following two ways. 1) When the exponent b of maximum electron density in the expression J=aN^b_<max> is calculated by the method of least squares, it is about 1 6 for λ5577A line and about 1 3 for λ4278A band for the case of E_n (night E layer) or E_<sr> (retadation type of E_s). 2) In case it is assumed beforehand that the auroral luminosity is proportional to the square of maximum electron density in the E-region, the expression becomes J (4278)=1 2×10^<-11>N^2_<max> for the case of the correlation of the 4278 band with E_<sr> layers. In general, type of the sporadic E layer seems to change in the order from E_n to E_<sr>, E_<sa> (auroral type of E_s) and E_<sf> (flat type of E_s, as the geomagnetic disturbance of negative bay type progresses There is a kind of the sporadic E layer which is not accompanied by auroral and geomagnetic disturbances Such E_s layers are apt to take a shape of flat type, and may be, so to speak, of mid-latitudinal type The relations between auroral intensities of λ5577A line and λ6300A line and between auroral luminosity and geomagnetic variation of H component are also discussed","subitem_description_type":"Other"}]},"item_1_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.15094/00007388","subitem_identifier_reg_type":"JaLC"}]},"item_1_publisher_22":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"国立極地研究所"}]},"item_1_source_id_13":{"attribute_name":"雑誌書誌ID","attribute_value_mlt":[{"subitem_source_identifier":"AN00181831","subitem_source_identifier_type":"NCID"}]},"item_1_source_id_20":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00857289","subitem_source_identifier_type":"ISSN"}]},"item_1_subject_21":{"attribute_name":"国際十進分類法","attribute_value_mlt":[{"subitem_subject":"551.510.535/.537","subitem_subject_scheme":"UDC"}]},"item_1_text_10":{"attribute_name":"著者所属(英)","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"The Radio Research Laboratories"},{"subitem_text_language":"en","subitem_text_value":"The Radio Research Laboratories"},{"subitem_text_language":"en","subitem_text_value":"Institute of Physics, College of General Education, the University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Tokyo Astronomical Observatory, the University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"The Radio Research Laboratories"}]},"item_1_text_9":{"attribute_name":"著者所属(日)","attribute_value_mlt":[{"subitem_text_value":"電波研究所"},{"subitem_text_value":"電波研究所"},{"subitem_text_value":"東京大学教養学部物理学教室"},{"subitem_text_value":"東京天文台"},{"subitem_text_value":"電波研究所"}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"1965-10-01"}],"displaytype":"detail","filename":"KJ00002476310.pdf","filesize":[{"value":"19.0 MB"}],"format":"application/pdf","licensetype":"license_6","mimetype":"application/pdf","url":{"label":"KJ00002476310","url":"https://nipr.repo.nii.ac.jp/record/7388/files/KJ00002476310.pdf"},"version_id":"b2174f84-89ae-45a1-96f5-fcde3cbbc1c3"}]},"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":"1961年の越冬観測から見た昭和基地における電離層,極光および地磁気変化の相互関係","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"1961年の越冬観測から見た昭和基地における電離層,極光および地磁気変化の相互関係"},{"subitem_title":"RESULTS OF SIMULTANEOUS OBSERVATIONS OF IONOSPHERE, AURORA AND GEOMAGNETISM AT SYOWA STATION DURING THE 1961 WINTERING","subitem_title_language":"en"}]},"item_type_id":"1","owner":"4","path":["931"],"pubdate":{"attribute_name":"公開日","attribute_value":"1965-10-01"},"publish_date":"1965-10-01","publish_status":"0","recid":"7388","relation_version_is_last":true,"title":["1961年の越冬観測から見た昭和基地における電離層,極光および地磁気変化の相互関係"],"weko_creator_id":"4","weko_shared_id":4},"updated":"2023-07-25T11:56:33.030130+00:00"}