{"created":"2021-03-01T06:27:49.385456+00:00","id":20258,"links":{},"metadata":{"_buckets":{"deposit":"9d0f39dc-a766-4215-8100-c74631ac0f88"},"_deposit":{"id":"20258","owners":[],"pid":{"revision_id":0,"type":"depid","value":"20258"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00020258","sets":["879:1183:1640:1749"]},"author_link":["59129","59130","59131","59132","59133","59134"],"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_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1971-03-30","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"71","bibliographicPageStart":"59","bibliographicVolumeNumber":"18","bibliographic_titles":[{"bibliographic_title":"Proceedings of the Research Institute of Atmospherics, Nagoya University","bibliographic_titleLang":"en"}]}]},"item_9_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Observations of interplanetary scintillation of radio sources for studying the solar wind have been carried out at two stations, Toyokawa and Fujigane, since June, 1970. The aerial is a square array containing 256 half-wave dipoles. A phase-switching receiver and a recording system which assure the simultaneity of the records taken at the two stations are used. The observational data are analysed by the statistical method. The velocity enhancements of the solar wind which correspond to the Forbush decrease and the geomagnetic storm have been detected by the observation of 3C 48 about 3 days after the solar flare. There is a tendency for the scale of the diffraction pattern to increase with increasing velocity, as pointed out by Vitkevich and Vlasov. The average scale of the diffraction pattern is about 300 km and it appears that the scale of the pattern or the size of the density fluctuations in the solar wind increases with increasing solar activity.","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/2237/22176"}]},"item_9_publisher_32":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"The Research Institute of Atmospherics, Nagoya University","subitem_publisher_language":"en"}]},"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":"0077-264X","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":"WATANABE, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"59129","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"WASHIMI, Haruichi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"59130","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KAKINUMA, Takakiyo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"59131","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KOJIMA, Masayoshi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"59132","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MARUYAMA, Kazuo","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"59133","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"ISHIDA, Yoshio","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"59134","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":"proria_18_59.pdf","filesize":[{"value":"1.9 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"proria_18_59.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/20258/files/proria_18_59.pdf"},"version_id":"b07710cb-fe99-4199-a462-3e18030ec469"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"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":"PRELIMINARY OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 69.3 MHz","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"PRELIMINARY OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 69.3 MHz","subitem_title_language":"en"}]},"item_type_id":"9","owner":"1","path":["1749"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2015-06-01"},"publish_date":"2015-06-01","publish_status":"0","recid":"20258","relation_version_is_last":true,"title":["PRELIMINARY OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 69.3 MHz"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-26T02:57:56.548767+00:00"}