{"created":"2021-03-01T06:30:27.424395+00:00","id":22673,"links":{},"metadata":{"_buckets":{"deposit":"a1903711-4c5e-4c8d-b6c8-e0a15e95be6d"},"_deposit":{"id":"22673","owners":[],"pid":{"revision_id":0,"type":"depid","value":"22673"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00022673","sets":["879:880:881"]},"author_link":["66788","66789","66790","66791","66792"],"item_10_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2016-08","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"L41","bibliographicPageStart":"L41","bibliographicVolumeNumber":"827","bibliographic_titles":[{"bibliographic_title":"The Astrophysical Journal Letters","bibliographic_titleLang":"en"}]}]},"item_10_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We developed an automated prediction technique for coronal holes using potential magnetic field extrapolation in the solar corona to construct a database of coronal holes appearing from 1975 February to 2015 July (Carrington rotations from 1625 to 2165). Coronal holes are labeled with the location, size, and average magnetic field of each coronal hole on the photosphere and source surface. As a result, we identified 3335 coronal holes and found that the long-term distribution of coronal holes shows a similar pattern known as the magnetic butterfly diagram, and polar/low-latitude coronal holes tend to decrease/increase in the last solar minimum relative to the previous two minima.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_10_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"DOI","subitem_identifier_uri":"http://dx.doi.org/10.3847/2041-8205/827/2/L41"},{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/24822"}]},"item_10_publisher_32":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"IOP publishing","subitem_publisher_language":"en"}]},"item_10_relation_11":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.3847/2041-8205/827/2/L41","subitem_relation_type_select":"DOI"}}]},"item_10_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2016. The American Astronomical Society","subitem_rights_language":"en"}]},"item_10_select_15":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_select_item":"publisher"}]},"item_10_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"2041-8205","subitem_source_identifier_type":"PISSN"}]},"item_1615787544753":{"attribute_name":"出版タイプ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"open access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_abf2"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Fujiki, K.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"66788","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Tokumaru, M.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"66789","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hayashi, K.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"66790","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Satonaka, D.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"66791","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hakamada, K.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"66792","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":"2018-02-22"}],"displaytype":"detail","filename":"apjl_827_2_L41.pdf","filesize":[{"value":"1.1 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"apjl_827_2_L41.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/22673/files/apjl_827_2_L41.pdf"},"version_id":"164d33b4-d3c6-4cbf-a125-b4fdda3cd81b"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Sun: activity","subitem_subject_scheme":"Other"},{"subitem_subject":"Sun: general","subitem_subject_scheme":"Other"},{"subitem_subject":"Sun: magnetic fields","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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"LONG-TERM TREND OF SOLAR CORONAL HOLE DISTRIBUTION FROM 1975 TO 2014","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"LONG-TERM TREND OF SOLAR CORONAL HOLE DISTRIBUTION FROM 1975 TO 2014","subitem_title_language":"en"}]},"item_type_id":"10","owner":"1","path":["881"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2016-09-14"},"publish_date":"2016-09-14","publish_status":"0","recid":"22673","relation_version_is_last":true,"title":["LONG-TERM TREND OF SOLAR CORONAL HOLE DISTRIBUTION FROM 1975 TO 2014"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T04:45:34.156081+00:00"}