{"created":"2023-05-15T12:35:24.392144+00:00","id":315,"links":{},"metadata":{"_buckets":{"deposit":"d744da00-5386-49e2-a749-7eb7ad2324ee"},"_deposit":{"created_by":2,"id":"315","owners":[2],"pid":{"revision_id":0,"type":"depid","value":"315"},"status":"published"},"_oai":{"id":"oai:kutarr.kochi-tech.ac.jp:00000315","sets":["5"]},"author_link":["1471","1468","1470","1469"],"item_2_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2016-02","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicPageEnd":"257","bibliographicPageStart":"243","bibliographicVolumeNumber":"41","bibliographic_titles":[{"bibliographic_title":"Experimental Astronomy"}]}]},"item_2_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We present a low cost meteor observation system based on the radio forward scattering and interferometry technique at Kochi University of Technology (KUT). The system can be a suitable model for low budget educational institutes that target practical learning of astronomical objects and upper atmospheric characteristics. The system methodology for the automatic counting of meteor echoes, filtering noise and detecting meteor echo directions is described. Detection of the meteor echo directions, which is the basic element for determining the meteor trajectories and the orbital parameters of parent comets, is based on a software system developed for analysis of phase differences detected by interferometry. Randomly selected observation samples measured by the radio interferometer are compared to simultaneous optical observations by video cameras to verify the system accuracy. Preliminary error analysis revealed that the system accuracy is directly related to the duration of observed meteor echoes. Eighty percent of meteor echo samples with durations longer than 3 s showed agreement in azimuth and elevation angles measurements to within a 10° error range, while meteor echo samples with shorter durations showed lower agreement levels probably due to the low system sampling resolution of 0.1 s. The reasonable agreement level of meteor echoes with duration longer than 3 s demonstrated the applicability of the system methodology. Accurate observation of shorter duration meteor echoes could possibly be achieved by improving the system resolution.","subitem_description_type":"Abstract"}]},"item_2_publisher_35":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Springer Science+Business Media Dordrecht"}]},"item_2_relation_13":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1007/s10686-015-9488-4","subitem_relation_type_select":"DOI"}}]},"item_2_rights_14":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"The final publication is available at link.springer.com"},{"subitem_rights":"Waleed Madkour, Masa-yuki Yamamoto, Yoshihiro Kakinami and Satoshi Mizumoto.: A low cost meteor observation system using radio forward scattering and the interferometry technique. Experimental Astronomy. 41(1), 243-257 (2016)"}]},"item_2_rights_15":{"attribute_name":"権利（URI）","attribute_value_mlt":[{"subitem_rights":"http://dx.doi.org/10.1007/s10686-015-9488-4 | http://dx.doi.org/10.1007/s10686-015-9488-4"}]},"item_2_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0922-6435","subitem_source_identifier_type":"ISSN"}]},"item_2_version_type_18":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_ab4af688f83e57aa","subitem_version_type":"AM"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Madkour, Waleed"}],"nameIdentifiers":[{"nameIdentifier":"1468","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Yamamoto, Masa-yuki"}],"nameIdentifiers":[{"nameIdentifier":"1469","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kakinami, Yoshihiro"}],"nameIdentifiers":[{"nameIdentifier":"1470","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Mizumoto, Satoshi"}],"nameIdentifiers":[{"nameIdentifier":"1471","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":"2019-02-13"}],"displaytype":"detail","filename":"28-51.pdf","filesize":[{"value":"1.6 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"28-51.pdf","url":"https://kutarr.kochi-tech.ac.jp/record/315/files/28-51.pdf"},"version_id":"b599732a-5965-4824-a3a2-8eb392852f15"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Meteors","subitem_subject_scheme":"Other"},{"subitem_subject":"Radar","subitem_subject_scheme":"Other"},{"subitem_subject":"Forward scattering","subitem_subject_scheme":"Other"},{"subitem_subject":"Interferometry","subitem_subject_scheme":"Other"}]},"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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"A low cost meteor observation system using radio forward scattering and the interferometry technique","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"A low cost meteor observation system using radio forward scattering and the interferometry technique"}]},"item_type_id":"2","owner":"2","path":["5"],"pubdate":{"attribute_name":"公開日","attribute_value":"2017-03-24"},"publish_date":"2017-03-24","publish_status":"0","recid":"315","relation_version_is_last":true,"title":["A low cost meteor observation system using radio forward scattering and the interferometry technique"],"weko_creator_id":"2","weko_shared_id":-1},"updated":"2023-05-15T13:38:30.828082+00:00"}