{"created":"2023-06-20T15:03:17.192009+00:00","id":32452,"links":{},"metadata":{"_buckets":{"deposit":"cd17a6c6-b29e-4612-b8d9-b8c0230147f4"},"_deposit":{"created_by":1,"id":"32452","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"32452"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00032452","sets":["1887:1890","1896:1898:1899:1910"]},"author_link":["409194","409193"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Geomagnetic Conjugacy of Auroral X-rays and Energetic Electrons Observed at the Geostationary Satellite"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1978-12","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"4_B","bibliographicPageEnd":"1265","bibliographicPageStart":"1245","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":"1975年4月9日UTにThompsonで行われた気球観測による15～85keVのオーロラX線と,赤道面静止衛星ATS-6による28～50 keVの電子との相関関係について調べた.magnetosphereの各モデルについて磁力線群を描き,磁力線の根元の地表上地磁気緯度λ_<mag>を,地磁気共役性の解析の新しいパラメーターとして用いた.適当なmagnetosphereのモデルを用いれば,極光帯でのオーロラX線と赤道面静止衛星ATS-6位置での高エネルギー電子の相関が良い時,地磁気共役性が成立していることが見出された.これは,赤道面での高エネルギー電子のピッチ角の大小にかかわらず成立している.プラズマ粒子による反磁性的効果についても検討された.地磁気擾乱の大きい時,最夜中子午面付近のATS-6位置(6.62R_E)で磁場の方向が赤道面に平行な方向に寄っていることは,magnetsphereのtailの磁気中性線を説明するのに都合がよい.","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"A correlation between auroral X-rays (15～85 keV) observed with the balloon (April 9,1975 UT, Thompson) and electrons (28～50 keV) at geostationary satellite ATS-6, has been researched. Geomagnetic filed configurations by some models of the magnetosphere were pictured, then a geomagnetic latitude λ_<mag> on the earth surface traced back along a field line has been used as a new parameter for analysis of geomagnetic conjugacy. When the correlation between auroral X-ray counts in auroral zone and high energy electron counts at the geosynchronous orbit is good, geomagnetic conjugacy realizes, if an appropriate model of the magnetosphere is adopted. This realization of geomagnetic conjugacy is not dependent on sizes of electron pitch angles. An effect of diamagnetism by plasma particles has been discussed. It is convenient for explanation of a neutral line in the tail of the magnetosphere, that direction of field line at the midnight ATS-6 position (6.62 R_E) approaches equatorward in the time of large geomagnetic disturbance.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0125705000","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":"立教大学理学部"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"平島, 洋"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"HIRASIMA, Yo","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":"SA0125705.pdf","filesize":[{"value":"989.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0125705.pdf","url":"https://jaxa.repo.nii.ac.jp/record/32452/files/SA0125705.pdf"},"version_id":"696d5cd2-4ebd-4af3-90c6-dd0b2de3a88e"}]},"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>極光帯オーロラX線と静止衛星位置高エネルギー電子の地磁気共役性","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"<論文>極光帯オーロラX線と静止衛星位置高エネルギー電子の地磁気共役性"}]},"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":"32452","relation_version_is_last":true,"title":["<論文>極光帯オーロラX線と静止衛星位置高エネルギー電子の地磁気共役性"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:32:00.248096+00:00"}