{"created":"2023-05-15T14:41:38.427212+00:00","id":1582,"links":{},"metadata":{"_buckets":{"deposit":"7f9582d8-e123-4523-9830-118d0a15b87e"},"_deposit":{"created_by":3,"id":"1582","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"1582"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:00001582","sets":["14:13:60"]},"author_link":["9253"],"control_number":"1582","item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2005-03","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"229","bibliographicPageStart":"212","bibliographicVolumeNumber":"34","bibliographic_titles":[{"bibliographic_title":"京都産業大学論集. 自然科学系列"}]}]},"item_10002_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Comparatively, recurrent type geomagnetic storms are weaker than SSC type geomagnetic storms. Therefore, during sunspot maximum, it is difficult to find recurrent type geomagnetic storms in the magnetogram due to the masking effect of the large disturbance. However, in the graphs of the geomagnetic activity index Kp as the basis, a small number of these storms (three) were detected in the magnetogram in 2000. Examinations of these storms were made by using geomagnetic data, mainly from the Kakioka geomagnetic observatory. Also, the present paper displays data about space plasma, and space magnetic field and the location of the artificial satellite Wind were shown.","subitem_description_type":"Abstract"}]},"item_10002_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"京都産業大学"}]},"item_10002_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11923897","subitem_source_identifier_type":"NCID"}]},"item_10002_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1348-3323","subitem_source_identifier_type":"PISSN"}]},"item_10002_version_type_20":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"山本, 実","creatorNameLang":"ja"},{"creatorName":"YAMAMOTO, Minoru","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"9253","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":"2017-09-30"}],"displaytype":"detail","filename":"AHSUSK_NSS_34_212.pdf","filesize":[{"value":"354.7 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AHSUSK_NSS_34_212.pdf","url":"https://ksu.repo.nii.ac.jp/record/1582/files/AHSUSK_NSS_34_212.pdf"},"version_id":"da15284a-35d3-4319-b245-baf8b649151b"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"地磁気嵐","subitem_subject_scheme":"Other"},{"subitem_subject":"回帰性","subitem_subject_scheme":"Other"},{"subitem_subject":"SSC型","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽活動極大期","subitem_subject_scheme":"Other"},{"subitem_subject":"人工衛星Wind","subitem_subject_scheme":"Other"},{"subitem_subject":"geomagnetic storm","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"recurrence","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"SSC-type","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"sunspot maximum","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"NASA satellite Wind","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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"太陽活動極大期の回帰性地磁気嵐に関する予備的報告","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"太陽活動極大期の回帰性地磁気嵐に関する予備的報告","subitem_title_language":"ja"},{"subitem_title":"A Preliminary Report on Recurrent Type Geomagnetic Storms During the Sunspot Maximum","subitem_title_language":"en"}]},"item_type_id":"10002","owner":"3","path":["60"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2017-09-30"},"publish_date":"2017-09-30","publish_status":"0","recid":"1582","relation_version_is_last":true,"title":["太陽活動極大期の回帰性地磁気嵐に関する予備的報告"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-08-22T01:45:23.461671+00:00"}