{"created":"2023-06-20T15:02:46.304269+00:00","id":31854,"links":{},"metadata":{"_buckets":{"deposit":"d22746cf-2c04-40ce-a4df-b7034a223e78"},"_deposit":{"created_by":1,"id":"31854","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"31854"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00031854","sets":["1887:1890","1896:1898:1899:1910"]},"author_link":["406527","406526"],"item_9_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Possible Lunar X-Rays Excited by Terrestrial Electrons"}]},"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1966-07","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"3_A","bibliographicPageEnd":"942","bibliographicPageStart":"940","bibliographicVolumeNumber":"2","bibliographic_titles":[{"bibliographic_title":"東京大学宇宙航空研究所報告"}]}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Energetic electrons found in the tail of the magnetosphere are able to excite X-rays on the lunar surface, when they hit the moon. The flux of such electrons with energies of several KeV is observed as high as 10^8cm^<-2>sec^<-1>, and the bremsstrahlung X-rays of energy k in &lrtri;k excited thereby is as strong as 4 X10^3 (&lrtri;k/K) cmcm^<-2>sec^<-1> at the lunar surface. The intensity of K X-rays, for example, of silicon is about 5KeV//&lrtri;k times the bremsstrahlung intensity at the same energy. It is, therefore, suggested that the observation of such lunar X-rays provides information on the electrons in the magnetosphere as well as on the chemical composition of the moon.","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA0124911000","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_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0563-8100","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":"AN00161914","subitem_source_identifier_type":"NCID"}]},"item_9_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"名古屋大学理学部"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"早川, 幸男"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"HAYAKAWA, Sachio","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":"SA0124911.pdf","filesize":[{"value":"192.8 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA0124911.pdf","url":"https://jaxa.repo.nii.ac.jp/record/31854/files/SA0124911.pdf"},"version_id":"c1878df1-bf8b-4abc-8d5b-6d96e883447f"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"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":"地球磁場に伴う電子で励起される月のX線","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"地球磁場に伴う電子で励起される月のX線"}]},"item_type_id":"9","owner":"1","path":["1890","1910"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"31854","relation_version_is_last":true,"title":["地球磁場に伴う電子で励起される月のX線"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T00:48:31.120737+00:00"}