{"created":"2021-03-01T06:27:13.423602+00:00","id":19708,"links":{},"metadata":{"_buckets":{"deposit":"cd922bc6-6531-4d6b-9b8b-41a05788d0a1"},"_deposit":{"id":"19708","owners":[],"pid":{"revision_id":0,"type":"depid","value":"19708"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00019708","sets":["879:1183:1689:1716"]},"author_link":["57598","57599"],"item_1615768549627":{"attribute_name":"出版タイプ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_9_alternative_title_19":{"attribute_name":"その他のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES. I.","subitem_alternative_title_language":"en"}]},"item_9_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1958-03-20","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1-2","bibliographicPageEnd":"66","bibliographicPageStart":"60","bibliographicVolumeNumber":"8","bibliographic_titles":[{"bibliographic_title":"空電研究所報告","bibliographic_titleLang":"ja"}]}]},"item_9_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The intensity and polarization of solar radio bursts have been observed at 9400, 3750, 2000 and 1000 Mc/s since July 1957. In this paper the results of observations during 6 months are described. In most bursts at microwave frequencies, the difference in the intensity of two circularly polarized components is observed. At 3750 Mc/s, the bursts of small degree of polarization (less than 10%) are predominant, compared with other frequencies. At 2000 and 1000 Mc/s the circularly polarized bursts were occasionally observed, but not at 9400 and 3750 Mc/s. In most bursts observed at four frequencies, the sense of polarization reverses near 3750 or 2000 Mc/s and the degree of polarization is generally small at 3750 Mc/s. At 9400 Mc/s, it seems that the sense of polarization correlates with the position of the source on the solar disk. Further observations will be continued to investigate the relation between them.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_9_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/21754"}]},"item_9_publisher_32":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"名古屋大学空電研究所","subitem_publisher_language":"ja"}]},"item_9_select_15":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_select_item":"publisher"}]},"item_9_source_id_7":{"attribute_name":"ISSN（print）","attribute_value_mlt":[{"subitem_source_identifier":"0465-7756","subitem_source_identifier_type":"PISSN"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"open access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_abf2"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"柿沼, 隆清","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"57598","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KAKINUMA, Takakiyo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"57599","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":"2018-02-21"}],"displaytype":"detail","filename":"bulria_8_1-2_60.pdf","filesize":[{"value":"1.2 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"bulria_8_1-2_60.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/19708/files/bulria_8_1-2_60.pdf"},"version_id":"d05ba789-5eab-4581-8324-1095d090a76b"}]},"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":"マイクロ波帯における太陽電波バーストの偏波について I","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"マイクロ波帯における太陽電波バーストの偏波について I","subitem_title_language":"ja"}]},"item_type_id":"9","owner":"1","path":["1716"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2015-04-28"},"publish_date":"2015-04-28","publish_status":"0","recid":"19708","relation_version_is_last":true,"title":["マイクロ波帯における太陽電波バーストの偏波について I"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-26T06:49:42.640521+00:00"}