{"created":"2023-06-20T15:03:47.996723+00:00","id":33004,"links":{},"metadata":{"_buckets":{"deposit":"ae49c9df-17d2-41c4-b1f7-3d3b81907408"},"_deposit":{"created_by":1,"id":"33004","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"33004"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00033004","sets":["1887:1890","1896:1898:1899:1912"]},"author_link":["413244","413243","413249","413247","413250","413248","413251","413252","413246","413245"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"27-Day Recurrence-Associated Phenomena Observed by Sakigake in the Heliosphere"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1988-03","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"73","bibliographicPageStart":"61","bibliographicVolumeNumber":"21","bibliographic_titles":[{"bibliographic_title":"宇宙科学研究所報告. 特集: 宇宙観測研究報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"「さきがけ」に搭載された太陽風(SOW), プラズマ波動(PWP), 及び惑星間空間磁場(IMF)観測装置で計測した27日回帰性諸現象の相関解析から, 1985年4月から1986年8月までの太陽磁気圏は黄道面に対して傾いたイクスカーションの過渡状態であり, その後から1987年7月まではニュートラルシートが黄道面と平行になるアラインド状態であった事が明らかになった。又, 高分解能データ解析から, 数R_Eのニュートラル(カレント)シート近傍に≳100R_E(∿7×10^5km)程度の厚さを持つイオン密度・温度の高い\"プラズマシート\"が存在していることが発見された。","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"27-day recurrence-associated phenomena of the solar wind (SOW), the plasma wave (PWP), and the interplanetary magnetic field (IMF) were detected by the Sakigake spacecraft. The heliospheric structures, having a neutral (current) sheet of ∿2×10^4km thickness and a \"plasmasheet\" of ≳7×10^5km thickness, during April, 1985-August, 1986 and September, 1986-July, 1987,were in the excursion and aligned phases, respectively. In the neutral sheet the IMF direction usually reverses in a minute. Using high time-resolution data, the average ion density and temperature in the heliospheric plasma sheet are also found to be ≳60/cc and ∿20×10^4K, respectively.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0166843000","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_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0285-9920","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":"AN00354485","subitem_source_identifier_type":"NCID"}]},"item_9_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"「さきがけ」観測研究グループ"},{"subitem_text_value":"「さきがけ」観測研究グループ"},{"subitem_text_value":"東北大理"},{"subitem_text_value":"電波研"},{"subitem_text_value":"「さきがけ」観測研究グループ"},{"subitem_text_value":"宇宙研"},{"subitem_text_value":"東海大工"},{"subitem_text_value":"「さきがけ」観測研究グループ"},{"subitem_text_value":"「さきがけ」観測研究グループ"},{"subitem_text_value":"東北大理"}]},"item_9_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Sakigake Research Group for Plasma Wave and Structure in the Solar Wind"},{"subitem_text_language":"en","subitem_text_value":"Sakigake Research Group for Plasma Wave and Structure in the Solar Wind"},{"subitem_text_language":"en","subitem_text_value":"Sakigake Research Group for Plasma Wave and Structure in the Solar Wind"},{"subitem_text_language":"en","subitem_text_value":"Sakigake Research Group for Plasma Wave and Structure in the Solar Wind"},{"subitem_text_language":"en","subitem_text_value":"Sakigake Research Group for Plasma Wave and Structure in the Solar Wind"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"大家, 寛"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"森岡, 昭"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小林, 敬生"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"三宅, 亘"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小山, 孝一郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"阿部, 琢美"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"平尾, 邦雄"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"斎藤, 尚生"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"湯元, 清文"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"鈴木, 裕見子"}],"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":"SA0166843.pdf","filesize":[{"value":"825.8 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0166843.pdf","url":"https://jaxa.repo.nii.ac.jp/record/33004/files/SA0166843.pdf"},"version_id":"7184171b-f940-4d4a-9b1a-cc269b086487"}]},"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":"「さきがけ」による 27 日回帰性太陽磁気圏構造に関わる諸現象","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"「さきがけ」による 27 日回帰性太陽磁気圏構造に関わる諸現象"}]},"item_type_id":"9","owner":"1","path":["1890","1912"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"33004","relation_version_is_last":true,"title":["「さきがけ」による 27 日回帰性太陽磁気圏構造に関わる諸現象"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:18:21.640184+00:00"}