{"created":"2023-06-20T14:52:22.944647+00:00","id":20524,"links":{},"metadata":{"_buckets":{"deposit":"f9ed1fb3-5b47-4eeb-8e14-55d3078a98dc"},"_deposit":{"created_by":1,"id":"20524","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20524"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020524","sets":["1543:1778:1791","1887:1891"]},"author_link":["195988","195986","195983","195985","195984","195987","195981","195982"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-03","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"36","bibliographicPageStart":"33","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":"Shock-wave heating model is one of the plausible models for chondrule formation, though the generation of shock waves has not been understood clearly. In this study, we have carried out MHD (MagnetoHydroDynamic) simulations of X-ray flares and subsequent expansion of magnetic bubbles and we examine whether the conditions of the shock waves inside of the solar nebula are suitable for chondrule formation. We found that shock waves of about 15 km/s with velocity could be generated at the upper region of the solar nebula at 3 AU from the central star. Such shock conditions at the upper region of the nebula at 3 AU seem to be appropriate for chondrule formation.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063350009","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":"国立天文台"},{"subitem_text_value":"筑波大学 計算科学研究センター"},{"subitem_text_value":"地質調査所"},{"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":"National Astronomical Observatory"},{"subitem_text_language":"en","subitem_text_value":"University of Tsukuba Center for Computational Sciences"},{"subitem_text_language":"en","subitem_text_value":"Geological Survey of Japan"},{"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":"林, 満"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中本, 泰史"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"木多, 紀子"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"橘, 省吾"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hayashi, Mitsuru R.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakamoto, Taishi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kita, Noriko T.","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tachibana, Shogo","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"原始惑星系円盤","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星間塵","subitem_subject_scheme":"Other"},{"subitem_subject":"衝撃波","subitem_subject_scheme":"Other"},{"subitem_subject":"電磁流体力学シミュレーション","subitem_subject_scheme":"Other"},{"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":"衝撃波伝搬","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽星雲","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽フレア","subitem_subject_scheme":"Other"},{"subitem_subject":"おうし座T型星","subitem_subject_scheme":"Other"},{"subitem_subject":"密度分布","subitem_subject_scheme":"Other"},{"subitem_subject":"protoplanetary disk","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"interplanetary dust","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"shock wave","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"magnetohydrodynamic simulation","subitem_subject_language":"en","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":"shock wave propagation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar nebula","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar flare","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"T Tauri star","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"density distribution","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":"Shock-wave heating chondrule formation: MHD simulation of shockwave propagation inside of the disk","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Shock-wave heating chondrule formation: MHD simulation of shockwave propagation inside of the disk","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":"20524","relation_version_is_last":true,"title":["Shock-wave heating chondrule formation: MHD simulation of shockwave propagation inside of the disk"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:49:04.588607+00:00"}