{"created":"2023-06-20T14:52:22.749817+00:00","id":20521,"links":{},"metadata":{"_buckets":{"deposit":"e2b9a451-3e5f-4d2c-8cf9-b3f69b807451"},"_deposit":{"created_by":1,"id":"20521","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20521"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020521","sets":["1543:1778:1791","1887:1891"]},"author_link":["195969","195970","195967","195968"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-03","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"24","bibliographicPageStart":"21","bibliographic_titles":[{"bibliographic_title":"第38回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 38th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The existence of chondrules indicates that the flash heating events occurred in the early solar nebula. The shock-wave heating model is a plausible model for chondrule formation. In this model dust particles are heated by the gas frictional heating. So it is naturally expected that the dust particle starts melting from surface to inside and a state where the surface of the particle is liquid and the center is solid is realized (it is called the partial melting state in this study). Kato et al. (2005) and Kadono and Arakawa (2005) show that stripping of the liquid surface by the gas flow may determine the maximal size and size distribution of chondrules assuming that partial melting state is realized in a dust particle. In this study, we examined whether or not the partial melting state is realized in the dust particle by solving a three-dimentional time dependent heat conduction equation. We found that the partial melting state is realized in the shock-wave heating model, and especially for dust particles of 1 mm or larger in radius, it is likely that the partial melting leads to the stripping of the liquid surface.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063350006","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":"筑波大学 計算科学研究センター"},{"subitem_text_value":"筑波大学 計算科学研究センター"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"University of Tsukuba Center for Computational Sciences"},{"subitem_text_language":"en","subitem_text_value":"University of Tsukuba Center for Computational Sciences"}]},"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":"保田, 誠司"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中本, 泰史"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yasuda, Seiji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakamoto, Taishi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"コンドルール","subitem_subject_scheme":"Other"},{"subitem_subject":"衝撃波加熱","subitem_subject_scheme":"Other"},{"subitem_subject":"超高速衝突","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽星雲","subitem_subject_scheme":"Other"},{"subitem_subject":"溶融","subitem_subject_scheme":"Other"},{"subitem_subject":"熱伝導","subitem_subject_scheme":"Other"},{"subitem_subject":"熱伝導度","subitem_subject_scheme":"Other"},{"subitem_subject":"温度分布","subitem_subject_scheme":"Other"},{"subitem_subject":"計算機シミュレーション","subitem_subject_scheme":"Other"},{"subitem_subject":"chondrule","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"shock-wave heating","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"hypervelocity impact","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar nebula","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"melting","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"heat conduction","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"thermal conductivity","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"temperature distribution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"computerized simulation","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":"Is the partial melting condition realized in the chondrule formation in the shock-wave heating model?","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Is the partial melting condition realized in the chondrule formation in the shock-wave heating model?","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1791","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20521","relation_version_is_last":true,"title":["Is the partial melting condition realized in the chondrule formation in the shock-wave heating model?"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:49:07.143719+00:00"}