{"created":"2023-06-20T15:08:53.503352+00:00","id":38388,"links":{},"metadata":{"_buckets":{"deposit":"5868379b-1ee2-47c0-84da-1e5b790a1da6"},"_deposit":{"created_by":1,"id":"38388","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"38388"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00038388","sets":["1887:1891"]},"author_link":["433132","433129","433131","433130"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1995-12","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"84","bibliographicPageStart":"81","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 investigate shocks occurred in the solar nebula in a framework of a local one-dimensional gas dynamics problem in order to clarify the possibility of chondrule formation through shock processes. We consider nonsteady shock case which is raised by gas clumps infalling on the disk nebula and found ranges of clump mass and size which can make the disk temperature rise to the dust evaporation temperature (about 1,500 K) and corresponding gas heating time. From our obtained relation between clumpy clouds and shock strength, the clumps estimated by some observations seems difficult to rise the nebular temperature high enough for dust evaporation.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063352021","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":"東京工業大学 理学部　地球惑星科学科"},{"subitem_text_value":"神戸大学 理学部　地球惑星科学科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Tokyo Institute of Technology Department of Earth and Planetary Sciences, Faculty of Science"},{"subitem_text_language":"en","subitem_text_value":"Kobe University Department of Earth and Planetary Sciences, 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":"北神, 今日子"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中川, 義次"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kitakami, Kyoko","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakagawa, Yoshitsugu","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"衝撃波","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽星雲","subitem_subject_scheme":"Other"},{"subitem_subject":"降着円盤","subitem_subject_scheme":"Other"},{"subitem_subject":"ガスダイナミクス","subitem_subject_scheme":"Other"},{"subitem_subject":"コンドルール","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星進化","subitem_subject_scheme":"Other"},{"subitem_subject":"隕石","subitem_subject_scheme":"Other"},{"subitem_subject":"隕石組成","subitem_subject_scheme":"Other"},{"subitem_subject":"shock wave","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar nebula","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"accretion disk","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"gas dynamics","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"chondrule","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar system","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"meteorite","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"meteoritic 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":"Clumpy cloud accretion on the disk and the chondrule formation","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Clumpy cloud accretion on the disk and the chondrule formation","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":"38388","relation_version_is_last":true,"title":["Clumpy cloud accretion on the disk and the chondrule formation"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T22:41:26.431919+00:00"}