{"created":"2023-06-20T15:08:54.071884+00:00","id":38399,"links":{},"metadata":{"_buckets":{"deposit":"115388a5-90de-4a66-8598-47fd9a2ee9c9"},"_deposit":{"created_by":1,"id":"38399","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"38399"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00038399","sets":["1887:1891"]},"author_link":["433185","433187","433188","433186"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1995-12","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"125","bibliographicPageStart":"122","bibliographic_titles":[{"bibliographic_title":"第28回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 28th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We study the fully dynamical mantle convection calculations which include the core-cooling and internal heating. The temporal Nusselt numbers are found to be in proportion to the power of the temporal Rayleigh number, whose exponent is 0.2-0.4 for various choice of the parameters associated with rheology, heat capacity of the mantle and core, and internal heating, unless the bottom thermal boundary disappears. The bottom boundary layer disappears, when the rate of cooling is large. Using the obtained relationship, we calculate the thermal history of the mantle and the core backward in time based on the parameterized convection theory. The results of both models are in good agreement, if the internal heating is small and the thermal boundary layer exists. If the internal heating decays quickly, the results of the dynamical calculation agrees well with those of the parameterized convection theory.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063352032","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"広島大学 理学部　地球惑星システム学科"},{"subitem_text_value":"広島大学 理学部　地球惑星システム学科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Hiroshima University Department of Earth and Planetary Systems Science, Faculty of Science"},{"subitem_text_language":"en","subitem_text_value":"Hiroshima University Department of Earth and Planetary Systems Science, Faculty of Science"}]},"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":"岩瀬, 康行"}],"nameIdentifiers":[{"nameIdentifier":"433185","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"本多, 了"}],"nameIdentifiers":[{"nameIdentifier":"433186","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Iwase, Yasuyuki","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"433187","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Honda, Satoru","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"433188","nameIdentifierScheme":"WEKO"}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"マントル対流","subitem_subject_scheme":"Other"},{"subitem_subject":"地球型惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"冷却","subitem_subject_scheme":"Other"},{"subitem_subject":"Rayleigh数","subitem_subject_scheme":"Other"},{"subitem_subject":"Nusselt数","subitem_subject_scheme":"Other"},{"subitem_subject":"熱容量","subitem_subject_scheme":"Other"},{"subitem_subject":"熱境界層","subitem_subject_scheme":"Other"},{"subitem_subject":"相転移","subitem_subject_scheme":"Other"},{"subitem_subject":"mantle convection","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"terrestrial planet","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"cooling","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Rayleigh number","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Nusselt number","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"heat capacity","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"thermal boundary layer","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"phase transformation","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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"On an applicability of parameterized mantle convection model","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"On an applicability of parameterized mantle convection model","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"38399","relation_version_is_last":true,"title":["On an applicability of parameterized mantle convection model"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T22:41:17.372076+00:00"}