{"created":"2023-06-20T14:52:19.887481+00:00","id":20464,"links":{},"metadata":{"_buckets":{"deposit":"43f9ab58-1d66-402b-8013-76c269984fed"},"_deposit":{"created_by":1,"id":"20464","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20464"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020464","sets":["1543:1778:1790","1887:1891"]},"author_link":["195478","195477","195480","195479","195481","195482"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-08-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"8","bibliographicPageStart":"5","bibliographic_titles":[{"bibliographic_title":"第39回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 39th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We previously developed a model to analyze chemical zoning in olivine on the basis of Fe-Mg interdiffusion during olivine crystal growth and to obtain the cooling rate (or burial depth) of parent rock. We verified this model by using Fe-Mg zoning in olivine produced by dynamic crystallization experiments for bulk chemical compositions like a Martian meteorite (Yamato 980459) and a lunar meteorite (LAP 02205). The calculated zoning profiles are in good agreement with the experimentally produced profiles and the calculated cooling rates are also in good agreement with the experimental cooling rates. These results mean that our model is valid for calculating the cooling rate on the basis of Fe-Mg zoning considering the crystal growth and that the Fe-Mg interdiffusion coefficient used is relatively accurate.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063505002","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":"東京大学 大学院理学系研究科"},{"subitem_text_value":"東京大学 大学院理学系研究科"},{"subitem_text_value":"東京大学 大学院理学系研究科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"University of Tokyo Graduate School of Science"},{"subitem_text_language":"en","subitem_text_value":"University of Tokyo Graduate School of Science"},{"subitem_text_language":"en","subitem_text_value":"University of Tokyo Graduate School 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":"宮本, 正道"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小泉, 英祐"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"三河内, 岳"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Miyamoto, Masamichi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Koizumi, Eisuke","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Mikochi, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"隕石母天体","subitem_subject_scheme":"Other"},{"subitem_subject":"火星隕石","subitem_subject_scheme":"Other"},{"subitem_subject":"隕石組成","subitem_subject_scheme":"Other"},{"subitem_subject":"冷却速度","subitem_subject_scheme":"Other"},{"subitem_subject":"カンラン石","subitem_subject_scheme":"Other"},{"subitem_subject":"結晶成長","subitem_subject_scheme":"Other"},{"subitem_subject":"結晶化","subitem_subject_scheme":"Other"},{"subitem_subject":"拡散","subitem_subject_scheme":"Other"},{"subitem_subject":"化学的ゾーニング","subitem_subject_scheme":"Other"},{"subitem_subject":"月隕石","subitem_subject_scheme":"Other"},{"subitem_subject":"化学組成","subitem_subject_scheme":"Other"},{"subitem_subject":"meteorite parent body","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Martian meteorite","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"meteoritic composition","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"cooling rate","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"olivine","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"crystal growth","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"crystallization","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"diffusion","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"chemical zoning","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"lunar meteorite","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"chemical composition","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":"Calculation of the cooling rate for olivine by consideration of Fe-Mg diffusion and olivine crystal growth: Verification by Martian and lunar meteorite composition","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Calculation of the cooling rate for olivine by consideration of Fe-Mg diffusion and olivine crystal growth: Verification by Martian and lunar meteorite composition","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1790","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20464","relation_version_is_last":true,"title":["Calculation of the cooling rate for olivine by consideration of Fe-Mg diffusion and olivine crystal growth: Verification by Martian and lunar meteorite composition"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:49:53.148983+00:00"}