{"created":"2023-07-25T11:04:54.720955+00:00","id":8113,"links":{},"metadata":{"_buckets":{"deposit":"3a36d810-71ea-4b05-ab67-70a4af256960"},"_deposit":{"created_by":4,"id":"8113","owners":[4],"pid":{"revision_id":0,"type":"depid","value":"8113"},"status":"published"},"_oai":{"id":"oai:nipr.repo.nii.ac.jp:00008113","sets":["1259:906:974"]},"author_link":["13512","13915","13508","5874"],"item_1_alternative_title_5":{"attribute_name":"論文名よみ","attribute_value_mlt":[{"subitem_alternative_title":"セイシ エイセイ キドウ ニオケル コウエネルギー リュウシ ノ カンソク a. ニュウシャ リュウシ ト オーロラ ダイ2カイ キョクイキ ニオケル デンリケン ジキケン ソウゴウ カンソク シンポジウム PART 1"}]},"item_1_biblio_info_14":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1980-02","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"34","bibliographicPageStart":"23","bibliographicVolumeNumber":"68","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":"長井, 嗣信"},{"creatorName":"ナガイ, ツグノブ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"河野, 毅"},{"creatorName":"コウノ, ツヨシ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]}]},"item_1_creator_8":{"attribute_name":"著者名(英)","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"NAGAI, Tsugunobu","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"KOHNO, Tsuyoshi","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_11":{"attribute_name":"抄録(日)","attribute_value_mlt":[{"subitem_description":"本論文では,磁気圏嵐時の静止衛星軌道における高エネルギー粒子のフラックス変動について報告する.3つの静止衛星の同時観測により,夕方側で粒子の減少がみえる時に,真夜中から朝側にかけては,粒子の増加がみられることを明確に示した.また,地磁気じょう乱が引き続いて起きている時には,比較的大きなしかも孤立して起きた磁気圏嵐の時とやや異なる粒子フラックスの変動がみられることを2日間の例を使い示した.","subitem_description_type":"Other"}]},"item_1_description_12":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"This article reports the results of studying the behavior of the energetic particle flux obtained at synchronous orbit during substorms. The multi-satellite study has clearly showed that the evening particle flux decrease contrasts with the behavior in the midnight-morning side, where the energetic particle flux increases at the substorm expansion onset. Two-days' examples indicate that the flux behavior during the periods of the continued geomagnetic activities seems to be somewhat different from that for the relatively large and isolated events.","subitem_description_type":"Other"}]},"item_1_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.15094/00008113","subitem_identifier_reg_type":"JaLC"}]},"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":"Magnetic Observatory"},{"subitem_text_language":"en","subitem_text_value":"The Institute of Physical and Chemical Research"}]},"item_1_text_9":{"attribute_name":"著者所属(日)","attribute_value_mlt":[{"subitem_text_value":"気象庁地磁気観測所"},{"subitem_text_value":"理化学研究所"}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"1980-02-01"}],"displaytype":"detail","filename":"KJ00002477173.pdf","filesize":[{"value":"2.1 MB"}],"format":"application/pdf","licensetype":"license_6","mimetype":"application/pdf","url":{"label":"KJ00002477173","url":"https://nipr.repo.nii.ac.jp/record/8113/files/KJ00002477173.pdf"},"version_id":"8c70047d-88ea-44ac-8fda-a910e67af8ee"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"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":"静止衛星軌道における高エネルギー粒子の観測(a.入射粒子とオーロラ)(第2回極域における電離圏磁気圏総合観測シンポジウム : Part I)","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"静止衛星軌道における高エネルギー粒子の観測(a.入射粒子とオーロラ)(第2回極域における電離圏磁気圏総合観測シンポジウム : Part I)"},{"subitem_title":"Energetic Particle Observations at Synchronous Orbit : Multiple-Satellite Study for Flux Variation by GOES-2, GOES-3 and GMS and Nightside Flux Depression for Continuous Geomagnetic Activity by GMS (a. Precipitating Particles and Auroras) (Proceedings of the Second Symposium on Coordinated Observations of the Ionosphere and Magnetosphere in the Polar Regions : Part I)","subitem_title_language":"en"}]},"item_type_id":"1","owner":"4","path":["974"],"pubdate":{"attribute_name":"公開日","attribute_value":"1980-02-01"},"publish_date":"1980-02-01","publish_status":"0","recid":"8113","relation_version_is_last":true,"title":["静止衛星軌道における高エネルギー粒子の観測(a.入射粒子とオーロラ)(第2回極域における電離圏磁気圏総合観測シンポジウム : Part I)"],"weko_creator_id":"4","weko_shared_id":4},"updated":"2023-07-25T13:27:43.284574+00:00"}