{"created":"2023-06-23T12:14:49.942472+00:00","id":3406,"links":{},"metadata":{"_buckets":{"deposit":"92c8333a-0b2b-4cbb-9f9f-336bc4b6b7d8"},"_deposit":{"created_by":20,"id":"3406","owners":[20],"pid":{"revision_id":0,"type":"depid","value":"3406"},"status":"published"},"_oai":{"id":"oai:asahi-u.repo.nii.ac.jp:00003406","sets":["49:133"]},"author_link":["3857","3859","3855","3858","3856","3817"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2012-07-01","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"7","bibliographicPageEnd":"639","bibliographicPageStart":"613","bibliographicVolumeNumber":"64","bibliographic_titles":[{"bibliographic_title":"Earth, planets and space"}]}]},"item_10001_description_12":{"attribute_name":"論文ID（NAID）","attribute_value_mlt":[{"subitem_description":"10031015636","subitem_description_type":"Other"}]},"item_10001_description_19":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_10001_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"出版社版"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://www.terrapub.co.jp/journals/EPS/pdf/2012/6407/64070613.pdf","subitem_relation_type_select":"URI"}}]},"item_10001_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11211921","subitem_source_identifier_type":"NCID"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"13438832","subitem_source_identifier_type":"ISSN"}]},"item_10001_textarea_24":{"attribute_name":"所属","attribute_value_mlt":[{"subitem_textarea_value":"Solar-Terrestrial Environment Laboratory, Nagoya University"},{"subitem_textarea_value":"Department of Information Management, Asahi University"},{"subitem_textarea_value":"Solar-Terrestrial Environment Laboratory, Nagoya University"},{"subitem_textarea_value":"Physics Department, Shinshu University"},{"subitem_textarea_value":"Institute for Cosmic Ray Research, University of Tokyo"},{"subitem_textarea_value":"Antarctic Division, Department of Science and Technology"}]},"item_10001_version_type_20":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_ab4af688f83e57aa","subitem_version_type":"AM"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"NAGASHIMA, K."}],"nameIdentifiers":[{"nameIdentifier":"3855","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MORISHITA, I"}],"nameIdentifiers":[{"nameIdentifier":"3817","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"9000018753133","nameIdentifierScheme":"CiNii ID","nameIdentifierURI":"http://ci.nii.ac.jp/nrid/9000018753133"}]},{"creatorNames":[{"creatorName":"FUJII, Z."}],"nameIdentifiers":[{"nameIdentifier":"3856","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MORI, S."}],"nameIdentifiers":[{"nameIdentifier":"3857","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KONDO, I."}],"nameIdentifiers":[{"nameIdentifier":"3858","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"JACKLYN, R. M."}],"nameIdentifiers":[{"nameIdentifier":"3859","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2015-06-19"}],"displaytype":"detail","filename":"13438832_64_613639_2012.pdf","filesize":[{"value":"2.0 MB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"13438832_64_613639_2012","url":"https://asahi-u.repo.nii.ac.jp/record/3406/files/13438832_64_613639_2012.pdf"},"version_id":"41bf7a89-b171-4912-9657-7feabce293a1"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Cosmic rays (CR)","subitem_subject_scheme":"Other"},{"subitem_subject":"sidereal anisotropy","subitem_subject_scheme":"Other"},{"subitem_subject":"heliomagnetosphere (HMS)","subitem_subject_scheme":"Other"},{"subitem_subject":"interstellar matter (ISM)","subitem_subject_scheme":"Other"},{"subitem_subject":"Compton-Getting effect","subitem_subject_scheme":"Other"},{"subitem_subject":"motion of the HMS","subitem_subject_scheme":"Other"},{"subitem_subject":"motion of ISM","subitem_subject_scheme":"Other"},{"subitem_subject":"acceleration of CRs","subitem_subject_scheme":"Other"},{"subitem_subject":"cosmic ray lens effect","subitem_subject_scheme":"Other"},{"subitem_subject":"Cosmic rays (CR)","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"sidereal anisotropy","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"heliomagnetosphere (HMS)","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"interstellar matter (ISM)","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Compton-Getting effect","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"motion of the HMS","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"motion of ISM","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"acceleration of CRs","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"cosmic ray lens effect","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 10^4 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 10^4 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field"},{"subitem_title":"The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 10^4 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"20","path":["133"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-06-19"},"publish_date":"2015-06-19","publish_status":"0","recid":"3406","relation_version_is_last":true,"title":["The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 10^4 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field"],"weko_creator_id":"20","weko_shared_id":-1},"updated":"2023-12-19T06:05:38.288087+00:00"}