{"created":"2023-06-20T15:16:25.758074+00:00","id":10136,"links":{},"metadata":{"_buckets":{"deposit":"1018fc77-7d2e-4cf1-a350-8c3388987a2b"},"_deposit":{"created_by":3,"id":"10136","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"10136"},"status":"published"},"_oai":{"id":"oai:nifs-repository.repo.nii.ac.jp:00010136","sets":["8:32"]},"author_link":["63341","63343","63342"],"item_5_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1996-09-01","bibliographicIssueDateType":"Issued"},"bibliographic_titles":[{},{"bibliographic_title":"Research Report NIFS-Series","bibliographic_titleLang":"en"}]}]},"item_5_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"\"Interactions of magnetic loops and arcades that are convecting at their photospheric footpoints are investigated by means of a three-dimensional magnetohydrodynamic simulation. The initial magnetic field is given by solving the bipolar potential field emerging from paired conevection holes on the photospheric plane under which magnetic fluxes are supplied. Simulations are performed for single bipolar flux tubes and twin bipolar flux tubes with loop-like and arcade-like shapes. It is found that a prominent energy release can occur only when two flux tubes collide and reconnect with each other. The releasing feature becomes more intensive and narrowly peaked as resistivity becomes smaller, which reflects a nature of driven reconnection. A single loop or arcade does not exhibit any significant energy release, even though it is highly twisted and expanded.\"","subitem_description_type":"Abstract"}]},"item_5_source_id_10":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0915-633X","subitem_source_identifier_type":"ISSN"}]},"item_5_text_8":{"attribute_name":"報告書番号","attribute_value_mlt":[{"subitem_text_value":"NIFS-448"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"\"Ozaki,  M.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Sato,  T.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"The, Complexity Simulation Group\"","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"solar flare","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"coronal magnetic field","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"magnetic reconnection","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"research report","resourceuri":"http://purl.org/coar/resource_type/c_18ws"}]},"item_title":"Interactions of Convecting Magnetic Loops and Arcades","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Interactions of Convecting Magnetic Loops and Arcades","subitem_title_language":"en"}]},"item_type_id":"5","owner":"3","path":["32"],"pubdate":{"attribute_name":"公開日","attribute_value":"2010-02-05"},"publish_date":"2010-02-05","publish_status":"0","recid":"10136","relation_version_is_last":true,"title":["Interactions of Convecting Magnetic Loops and Arcades"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-06-20T20:53:12.048091+00:00"}