{"created":"2021-03-01T06:27:12.834491+00:00","id":19699,"links":{},"metadata":{"_buckets":{"deposit":"382268a6-3a3d-4c98-924b-ccf91573f8e3"},"_deposit":{"id":"19699","owners":[],"pid":{"revision_id":0,"type":"depid","value":"19699"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00019699","sets":["879:1183:1689:1715"]},"author_link":["57553","57554","57555","57556","57557","57558"],"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":"DATA ON SOLAR RADIO EMISSION WITH SOME NOTES","subitem_alternative_title_language":"en"}]},"item_9_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1957-05-25","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1-2","bibliographicPageEnd":"99","bibliographicPageStart":"66","bibliographicVolumeNumber":"7","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 results of observations by 3750 and 9400 Mc/s radiometers are tabulated. The daily flux density at both frequencies has a correlation coefficient of 0.95, and the S-component at 9400 Mc/s is 0.8 times as large as that at 3750 Mc/s. The sense of polarization at both frequencies is similar. The percentage polarization referring to the S-component of an isolated radio spot occasionally exceeds 30 percent at 9400 Mc/s, which is much larger than that at 3750 Mc/s. Some bursts show yet a remarkable structure of frequency spectrum at these super-high-frequencies. The observations with an 8-element interferometer have been made for five hours every day for locating sources of outstanding occurrences. A burst occasionally occurs in an emissive region where no intense radiation is usually observed.","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/2237/21745"}]},"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":"57553","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"高柳, 利男","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"57554","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"太陽電波研究室一同","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"57555","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kakinuma, Takakiyo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"57556","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Takayanagi, Toshio","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"57557","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"other members of Radio Astronomy Section","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"57558","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_7_1-2_66.pdf","filesize":[{"value":"5.1 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"bulria_7_1-2_66.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/19699/files/bulria_7_1-2_66.pdf"},"version_id":"69280138-8eca-4a7b-877c-f7231dae0045"}]},"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":"太陽電波の観測と二三の考察","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"太陽電波の観測と二三の考察","subitem_title_language":"ja"}]},"item_type_id":"9","owner":"1","path":["1715"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2015-04-28"},"publish_date":"2015-04-28","publish_status":"0","recid":"19699","relation_version_is_last":true,"title":["太陽電波の観測と二三の考察"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-26T06:44:18.431437+00:00"}