{"created":"2021-03-01T06:35:58.609969+00:00","id":18571,"links":{},"metadata":{"_buckets":{"deposit":"b8a06e65-61ab-4241-a476-7c5c306bec7b"},"_deposit":{"id":"18571","owners":[],"pid":{"revision_id":0,"type":"depid","value":"18571"},"status":"published"},"_oai":{"id":"oai:repository.dl.itc.u-tokyo.ac.jp:00018571","sets":["171:1108:1244:1266","9:504:1111:1246:1267"]},"item_4_alternative_title_1":{"attribute_name":"その他のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"Large-Scale Magnetic Fields in Spiral Galaxies"}]},"item_4_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1995-02","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"106","bibliographicPageStart":"99","bibliographicVolumeNumber":"47","bibliographic_titles":[{"bibliographic_title":"生産研究"}]}]},"item_4_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"銀河あるいは星間空間のプラズマとしての性質が概観され, 磁場および速度場の基本的な観測方法およびその結果が示される. 平均の回転運動がある系では, 磁場と速度場の相関であるクロス･ヘリシティが磁場の生成に重要な役割を果たす. さまざまな銀河磁場の強さと回転速度との関係からクロス･ヘリシティについての重要な情報が導かれる. 銀河面に関して非対称な密度･速度場を仮定するとクロス･ヘリシティ･ダイナモによって銀河の代表的な大規模磁場配位であるBSS磁場が再現できる.","subitem_description_type":"Abstract"}]},"item_4_description_6":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"特集 乱流の数値シミュレーション(NST)その11","subitem_description_type":"Other"}]},"item_4_full_name_3":{"attribute_name":"著者別名","attribute_value_mlt":[{"nameIdentifiers":[{"nameIdentifier":"32385","nameIdentifierScheme":"WEKO"}],"names":[{"name":"Yokoi, Nobumitsu"}]}]},"item_4_publisher_20":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"東京大学生産技術研究所"}]},"item_4_source_id_10":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AN00127075","subitem_source_identifier_type":"NCID"}]},"item_4_source_id_8":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0037105X","subitem_source_identifier_type":"ISSN"}]},"item_4_subject_15":{"attribute_name":"日本十進分類法","attribute_value_mlt":[{"subitem_subject":"440","subitem_subject_scheme":"NDC"}]},"item_4_text_21":{"attribute_name":"出版者別名","attribute_value_mlt":[{"subitem_text_value":"Institute of Industrial Science, the University of Tokyo"}]},"item_4_text_4":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学生産技術研究所第1部 物理学"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"横井, 喜充"}],"nameIdentifiers":[{"nameIdentifier":"32384","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2017-06-08"}],"displaytype":"detail","filename":"sk047002004.pdf","filesize":[{"value":"6.6 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"sk047002004.pdf","url":"https://repository.dl.itc.u-tokyo.ac.jp/record/18571/files/sk047002004.pdf"},"version_id":"ec081328-873c-4989-ae70-d2c2c2386926"}]},"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":"特集4 : 研究解説 : 渦状銀河の磁場","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"特集4 : 研究解説 : 渦状銀河の磁場"}]},"item_type_id":"4","owner":"1","path":["1266","1267"],"pubdate":{"attribute_name":"公開日","attribute_value":"2012-11-13"},"publish_date":"2012-11-13","publish_status":"0","recid":"18571","relation_version_is_last":true,"title":["特集4 : 研究解説 : 渦状銀河の磁場"],"weko_creator_id":"1","weko_shared_id":null},"updated":"2022-12-19T03:57:20.314520+00:00"}