{"created":"2021-03-01T06:27:13.875012+00:00","id":19715,"links":{},"metadata":{"_buckets":{"deposit":"6356d79f-e44f-4515-a67c-4df919f27375"},"_deposit":{"id":"19715","owners":[],"pid":{"revision_id":0,"type":"depid","value":"19715"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00019715","sets":["879:1183:1689:1717"]},"author_link":["57624","57625","57626","57627"],"control_number":"19715","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":"ECLIPSE OBSERVATIONS OF MTCROWAVE RADIO SOURCES ON THE SOLAR DISK ON 19 APRIL 1958","subitem_alternative_title_language":"en"}]},"item_9_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1959-03-25","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1-2","bibliographicPageEnd":"41","bibliographicPageStart":"39","bibliographicVolumeNumber":"9","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 partial and annular eclipse on 19 April 1958 was observed at Toyokawa and Hachijojima at four frequencies, i.e. 9400, 3750, 2000 and 1000 Mc/s. Brightness distribution over the solar disk at these frequencies is derived with the aid of interferometric observations at 4000 Mc/s in full course of the eclipse. The maximum brightness was, from 9400 to 1000 Mc/s, of the order of 10^5, 10^6, 2X10^6 and 3x10^6°K respectively. It is very remarkable that the source of polarization is strictly confined in a small area over the sunspot, about 1' in diameter. Thus, two sources of polarization of different sense exist over each pole of a bipolar sunspot. The polarization seems to be determined at a lower altitude than what has been considered. Most of the sources have the sense of extraordinary wave, though some have an opposite sense at 9400 Mc/s. The degree of polarization increases with frequency: the value for the most active spot amounts to more than 60% at 9400 Mc/s, while at 1000 Mc/s, it is subject to nothing.","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/2237/21761"}]},"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":"田中, 春夫","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"57624","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"柿沼, 隆清","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"57625","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"TANAKA, Haruo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"57626","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KAKINUMA, Takakiyo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"57627","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_9_1-2_39.pdf","filesize":[{"value":"532.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"bulria_9_1-2_39.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/19715/files/bulria_9_1-2_39.pdf"},"version_id":"ab7f505e-06e2-4ed2-b48c-1a8d96a4bd16"}]},"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":"1958年4月19日の日食観測の結果について","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"1958年4月19日の日食観測の結果について","subitem_title_language":"ja"}]},"item_type_id":"9","owner":"1","path":["1717"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2015-04-30"},"publish_date":"2015-04-30","publish_status":"0","recid":"19715","relation_version_is_last":true,"title":["1958年4月19日の日食観測の結果について"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-11-17T04:54:09.048762+00:00"}