{"created":"2023-06-20T14:52:12.360707+00:00","id":20331,"links":{},"metadata":{"_buckets":{"deposit":"b30b48ab-bfa2-419a-8cfb-293374fcf56d"},"_deposit":{"created_by":1,"id":"20331","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20331"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020331","sets":["1543:1778:1786","1887:1891"]},"author_link":["194096","194093","194095","194092","194094"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-08","bibliographicIssueDateType":"Issued"},"bibliographicVolumeNumber":"43","bibliographic_titles":[{"bibliographic_title":"第43回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 43th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_14":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）","attribute_value_mlt":[{"subitem_description":"第43回月・惑星シンポジウム (2010年8月4-6日. 宇宙航空研究開発機構宇宙科学研究所), 相模原市, 神奈川県","subitem_description_type":"Other"}]},"item_5_description_15":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）（英）","attribute_value_mlt":[{"subitem_description":"43rd  ISAS Lunar and Planetary Symposium (August 4-6,  2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Europa, the second Galilean satellites is an interesting object because subsurface ocean is thought to exist. The existence of the ocean has been proposed by researches such as the observation of induced magnetic field and the analysis of topography. However, these are not direct ones nor precise ones. In this report we propose a method for directing the subsurface ocean by using high energy cosmic neutrinos. We performed the simulation on detectability of interaction between the neutrinos and icy shell of Europa and recognized that the number of radiations caused by neutrinos depended on the thickness of the icy layer of Europa. We think that this method will be able to determine the thickness of ice and detect the subsurface ocean directly and accurately.","subitem_description_type":"Other"}]},"item_5_description_18":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"形態: カラー図版あり","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Physical characteristics: Original contains color illustrations","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0065116021","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所 (JAXA)(ISAS)"}]},"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_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA12268968","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学地震研究所"},{"subitem_text_value":"東京大学地震研究所"},{"subitem_text_value":"東京大学地震研究所高エネルギー素粒子地球物理学研究センター"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Earthquake Research Institute, University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Earthquake Research Institute, University of Tokyo"},{"subitem_text_language":"en","subitem_text_value":"Center for High Energy Geophysics Research, Earthquake Research Institute, University of Tokyo"}]},"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":"栗田, 敬"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"田中, 宏幸"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Daigo, Shoji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kurita, Kei","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tanaka, Hiroyuki K. M.","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"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":"A new method for detecting the subsurface ocean of Europa by using high energy neutrinos","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"A new method for detecting the subsurface ocean of Europa by using high energy neutrinos","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1786","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20331","relation_version_is_last":true,"title":["A new method for detecting the subsurface ocean of Europa by using high energy neutrinos"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:51:46.605276+00:00"}