{"created":"2023-06-20T15:05:10.619402+00:00","id":34437,"links":{},"metadata":{"_buckets":{"deposit":"a7ec1221-838d-4798-ac63-4a6016906932"},"_deposit":{"created_by":1,"id":"34437","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"34437"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00034437","sets":["1887:1890","1896:1898:1899:1992"]},"author_link":["419599","419601","419600"],"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1970-12","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"16","bibliographicPageEnd":"522","bibliographicPageStart":"513","bibliographicVolumeNumber":"35","bibliographic_titles":[{},{"bibliographic_title":"ISAS report/Institute of Space and Aeronautical Science,University of Tokyo","bibliographic_titleLang":"en"}]}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The electric field generated by the interaction of solar wind with planetary bodies is discussed by the laboratory simulation. It is inferred from this experiment that an upper limit of the electric field behind Moon would be in the order of 10^<-2>V/m, and almost zero behind Venus. The mechanisms generating the electric and the magnetic field by the solar wind interaction are also discussed, and they would respectively be due to charge separation and pressure gradient drift.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA2400787000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"東京大学宇宙航空研究所"}]},"item_9_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Aeronautical Science,University of Tokyo"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0372-1418","subitem_source_identifier_type":"ISSN"}]},"item_9_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00675986","subitem_source_identifier_type":"NCID"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"KUBO, Haruya","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"ITOH, Tomizo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"YAMORI, Akira","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-01-24"}],"displaytype":"detail","filename":"SA2400787.pdf","filesize":[{"value":"559.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA2400787.pdf","url":"https://jaxa.repo.nii.ac.jp/record/34437/files/SA2400787.pdf"},"version_id":"4b3ca6b1-c0cf-43aa-a3f7-8eabeb77d46e"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Laboratory Experiment on the Solar Wind Interaction with Planetary Bodies","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Laboratory Experiment on the Solar Wind Interaction with Planetary Bodies","subitem_title_language":"en"}]},"item_type_id":"9","owner":"1","path":["1890","1992"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"34437","relation_version_is_last":true,"title":["Laboratory Experiment on the Solar Wind Interaction with Planetary Bodies"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T23:42:05.882624+00:00"}