{"created":"2024-09-04T03:04:28.786359+00:00","id":2000223,"links":{},"metadata":{"_buckets":{"deposit":"a034a387-f0ac-4db9-aa3d-aa72d0a97398"},"_deposit":{"created_by":11,"id":"2000223","owner":"11","owners":[11],"pid":{"revision_id":0,"type":"depid","value":"2000223"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:02000223","sets":["14:226:1725414013867"]},"author_link":["22320"],"item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2024-09-10","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"57","bibliographicPageStart":"53","bibliographicVolumeNumber":"19","bibliographic_titles":[{"bibliographic_title":"京都産業大学総合学術研究所所報"}]}]},"item_10002_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"雲は惑星の大気循環や表層環境を理解する上で不可欠な要素である。金星には分厚い濃硫酸の雲が全球的に存在し，金星の大気循環や表層環境の理解には雲の内部構造（雲粒の粒径分布と各粒径粒子の数密度の緯度・高度依存性）の形成メカニズムの解明が必要である。そのための手法の一つとして，雲微物理過程と大気運動を高速かつ同時に解ける超水滴法がある。本研究では，超水滴法が金星雲粒の成長過程の考察に対して有効かどうか検証する為に，0次元モデルによる試験的な数値実験を実施した。","subitem_description_type":"Abstract"}]},"item_10002_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"京都産業大学総合学術研究所"}]},"item_10002_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11879037","subitem_source_identifier_type":"NCID"}]},"item_10002_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1348-8465","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":"ANDO, Hiroki","creatorNameLang":"en"},{"creatorName":"安藤, 紘基","creatorNameLang":"ja"},{"creatorName":"アンドウ, ヒロキ","creatorNameLang":"ja-Kana"}],"familyNames":[{"familyName":"ANDO","familyNameLang":"en"},{"familyName":"安藤","familyNameLang":"ja"},{"familyName":"アンドウ","familyNameLang":"ja-Kana"}],"givenNames":[{"givenName":"Hiroki","givenNameLang":"en"},{"givenName":"紘基","givenNameLang":"ja"},{"givenName":"ヒロキ","givenNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"22320","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_access","date":[{"dateType":"Available","dateValue":"2024-09-04"}],"displaytype":"detail","filename":"KSUSGKS_19_53.pdf","filesize":[{"value":"478 KB"}],"format":"application/pdf","licensetype":"license_note","url":{"label":"KSUSGKS_19_53.pdf","url":"https://ksu.repo.nii.ac.jp/record/2000223/files/KSUSGKS_19_53.pdf"},"version_id":"3467980c-90cf-417c-ab9a-284dff6592a9"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"金星","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"雲物理","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"超水滴法","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"0次元モデル","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"硫酸液滴","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"Venus","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Cloud physics","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Super-droplet method","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Box model","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Sulfuric acid droplet","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"超水滴法を用いた金星硫酸雲構造の形成メカニズムの解明","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"超水滴法を用いた金星硫酸雲構造の形成メカニズムの解明","subitem_title_language":"ja"},{"subitem_title":"Formation mechanism of the Venusian cloud structure investigated by Super Droplet Method","subitem_title_language":"en"}]},"item_type_id":"10002","owner":"11","path":["1725414013867"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2024-09-04"},"publish_date":"2024-09-04","publish_status":"0","recid":"2000223","relation_version_is_last":true,"title":["超水滴法を用いた金星硫酸雲構造の形成メカニズムの解明"],"weko_creator_id":"11","weko_shared_id":-1},"updated":"2024-09-04T03:11:59.939599+00:00"}