{"created":"2023-06-20T15:03:41.874008+00:00","id":32913,"links":{},"metadata":{"_buckets":{"deposit":"d46abc6f-5df2-4ee4-8b9f-e5ed09e9dffc"},"_deposit":{"created_by":1,"id":"32913","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"32913"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00032913","sets":["1887:1890","1896:1898:1899:1912"]},"author_link":["412647","412648","412646","412649"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Variation of Ion Tail of a Comet at the Time of its Crossing through the Heliospheric Neutral Sheet : Comet Halley in 1910 and Others"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1986-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"101","bibliographicPageStart":"89","bibliographicVolumeNumber":"15","bibliographic_titles":[{"bibliographic_title":"宇宙科学研究所報告. 特集: 太陽風と彗星の相互作用研究報告"}]}]},"item_9_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"HALLEY彗星は前回1910年に回帰したが, その時の写真26枚がSURVEYされ, 中でもION TAILが際だって特異な様相を示したのが5月13日EVENTであることが確認された。そのKINK状様相を太陽風構造との関連で調べるために, 先づ1910年は太陽圏がEXCURSION PHASEにあったことを突きとめた。次に地磁気活動度の27日回帰性から, 太陽圏中性面の傾きと位置が求められた。そして地球と彗星の三次元的軌道位置を重ね合わせた結果, HALLY彗星はちょうどこの日に中性面を横切っていたことが判明した。太陽風向の中性面付近でこの変化に関する観測結果を適用して次のような結論を得た。1910年5月13日にHALLEY彗星のION TAILに特異なKINKが生じたのは, ちょうどこの日に, 太陽風向風速分布が急に変る太陽圏中性面を, 彗星が横切ったためである。他の2∿3の彗星ION TAILに見られたKINKについても, 同様な解析を行ない, 結論の正しさを傍証した。","subitem_description_type":"Abstract"}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Surveying 26 plates of Comet Halley during the last apparition in 1910,the ion tail with a distinct kink on May 13 is concluded to be the most specific throughout the 1910 apparition. The heliosphere was deduced from the analysis of its solar cycle variation to be in excursion phase. From the analysis of 27-day recurrence time pattern of geomagnetic activity index C 9 during 1909-1911,the inclination and the position of the heliospheric neutral sheet on the day is obtained and expressed on the two-hemisphere diagram. Superposition of the positions of the earth and the comet on the day on the diagram revealed that the comet was just on the neutral sheet on 13 May 1910. Considering the recent observation on the deflection of the solar wind near the neutral sheet, it is concluded that the kind of the ion tail was caused by a sector boundary crossing.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0166722000","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":"東北大学理学部"},{"subitem_text_value":"法政大学"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"斎藤, 尚生"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"斎藤, 馨児"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SAITO, Takao","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SAITO, Keiji","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":"SA0166722.pdf","filesize":[{"value":"1.0 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0166722.pdf","url":"https://jaxa.repo.nii.ac.jp/record/32913/files/SA0166722.pdf"},"version_id":"3ceac600-545d-4c81-9c00-5fa94d2bd08c"}]},"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":"彗星が太陽磁気圏中性面を通過する際の尾の変化 : 1910年出現時のハレー彗星その他","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"彗星が太陽磁気圏中性面を通過する際の尾の変化 : 1910年出現時のハレー彗星その他"}]},"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":"32913","relation_version_is_last":true,"title":["彗星が太陽磁気圏中性面を通過する際の尾の変化 : 1910年出現時のハレー彗星その他"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:20:43.270822+00:00"}