{"created":"2023-05-15T14:36:38.748662+00:00","id":47204,"links":{},"metadata":{"_buckets":{"deposit":"250c79da-31df-4405-b3c8-f02e36bf0d27"},"_deposit":{"created_by":1,"id":"47204","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"47204"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00047204","sets":["1"]},"author_link":["471758","471757","471755","471756","471754"],"item_8_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2014-12","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"10","bibliographicPageEnd":"2121","bibliographicPageStart":"2114","bibliographicVolumeNumber":"54","bibliographic_titles":[{"bibliographic_title":"Advances in Space Research"}]}]},"item_8_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Depth dependency of neutrons produced by cosmic rays (CRs) in the lunar subsurface was estimated using the three-dimensional\nMonte Carlo particle and heavy ion transport simulation code, PHITS, incorporating the latest high energy nuclear data, JENDL/\nHE-2007. The PHITS simulations of equilibrium neutron density profiles in the lunar subsurface were compared with the measurement\nby Apollo 17 Lunar Neutron Probe Experiment (LNPE). Our calculations reproduced the LNPE data except for the 350–400 mg/cm2\nregion under the improved condition using the CR spectra model based on the latest observations, well-tested nuclear interaction models\nwith systematic cross section data, and JENDL/HE-2007.","subitem_description_type":"Abstract"}]},"item_8_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Elsevier"}]},"item_8_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0273-1177","subitem_source_identifier_type":"ISSN"}]},"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":"Ota, S."}],"nameIdentifiers":[{"nameIdentifier":"471754","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Sihver, L."}],"nameIdentifiers":[{"nameIdentifier":"471755","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"小林, 進悟"}],"nameIdentifiers":[{"nameIdentifier":"471756","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hasebe, N."}],"nameIdentifiers":[{"nameIdentifier":"471757","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"小林 進悟","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"471758","nameIdentifierScheme":"WEKO"}]}]},"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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Depth dependency of neutron density produced by cosmic rays in the lunar subsurface","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Depth dependency of neutron density produced by cosmic rays in the lunar subsurface"}]},"item_type_id":"8","owner":"1","path":["1"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-08-06"},"publish_date":"2015-08-06","publish_status":"0","recid":"47204","relation_version_is_last":true,"title":["Depth dependency of neutron density produced by cosmic rays in the lunar subsurface"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T23:42:40.450963+00:00"}