{"created":"2023-06-20T13:42:53.979031+00:00","id":494,"links":{},"metadata":{"_buckets":{"deposit":"1ef450e4-2fc7-41dc-9ed6-c6acf1e7058d"},"_deposit":{"created_by":2,"id":"494","owners":[2],"pid":{"revision_id":0,"type":"depid","value":"494"},"status":"published"},"_oai":{"id":"oai:fut.repo.nii.ac.jp:00000494","sets":["1"]},"author_link":["10157","10154","10155","10156"],"item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2003-03-20","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"33","bibliographicPageEnd":"342","bibliographicPageStart":"335","bibliographic_titles":[{"bibliographic_title":"福井工業大学研究紀要. 第一部"}]}]},"item_10002_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Many of split-band Type II solar radio bursts are characterized by the simultaneous intensity variation between two split band emissions suggesting that the origin of the two split bands is located in the same place associated with the shock waves propagating through the solar coronal plasma. We propose here the emission mechanism of the split band Type II solar radio bursts in terms of the nonlinear wave particle interactions of cyclotron resonance type shown by ω_H-ω_P-(K_H-K_P)・V=nω.(n=1, 2, 3...) where ω_H, ω_P and ω_C are frequency of higher frequency component of split bands, plasma frequency and cyclotron frequency, respectively. The present hypothesis can be confirmed by studying high resolution spectra in decametric wave length range obtained by Tsukidate radio spectrograph and wide band dynamic spectra given by HiRAS (Hiraiso radio spectrograph). And the image processing technique for the radio spectrograph is also referred.","subitem_description_type":"Abstract"}]},"item_10002_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.57375/00000488","subitem_identifier_reg_type":"JaLC"}]},"item_10002_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"福井工業大学"}]},"item_10002_relation_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"TF00008947","subitem_relation_type_select":"NCID"}}]},"item_10002_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"2868571","subitem_source_identifier_type":"ISSN"}]},"item_10002_version_type_20":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"青山, 隆司"}],"nameIdentifiers":[{"nameIdentifier":"10154","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"大家, 寛"}],"nameIdentifiers":[{"nameIdentifier":"10155","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Aoyama, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"10156","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Oya, Hiroshi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"10157","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":"2023-04-12"}],"displaytype":"detail","filename":"KJ00004279720.pdf","filesize":[{"value":"567.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00004279720.pdf","url":"https://fut.repo.nii.ac.jp/record/494/files/KJ00004279720.pdf"},"version_id":"4322c89f-2a71-4d00-bf95-fb55a889b9d9"}]},"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":"スプリット型太陽電波の発生機構","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"スプリット型太陽電波の発生機構"},{"subitem_title":"Generation Mechanism of Split Band Solar Radio Bursts","subitem_title_language":"en"}]},"item_type_id":"10002","owner":"2","path":["1"],"pubdate":{"attribute_name":"公開日","attribute_value":"2009-04-04"},"publish_date":"2009-04-04","publish_status":"0","recid":"494","relation_version_is_last":true,"title":["スプリット型太陽電波の発生機構"],"weko_creator_id":"2","weko_shared_id":-1},"updated":"2023-06-20T14:31:18.613744+00:00"}