{"created":"2023-06-23T12:14:50.419989+00:00","id":3419,"links":{},"metadata":{"_buckets":{"deposit":"a437b22d-4603-4db7-9a0d-7549c828705c"},"_deposit":{"created_by":20,"id":"3419","owners":[20],"pid":{"revision_id":0,"type":"depid","value":"3419"},"status":"published"},"_oai":{"id":"oai:asahi-u.repo.nii.ac.jp:00003419","sets":["49:133"]},"author_link":["3891","3892","3888"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1991","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"8","bibliographicPageEnd":"689","bibliographicPageStart":"685","bibliographicVolumeNumber":"43","bibliographic_titles":[{"bibliographic_title":"Journal of geomagnetism and geoelectricity"},{"bibliographic_title":"Earth, Planets and Space","bibliographic_titleLang":"en"}]}]},"item_10001_description_12":{"attribute_name":"論文ID（NAID）","attribute_value_mlt":[{"subitem_description":"130003558910","subitem_description_type":"Other"}]},"item_10001_description_19":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"By using data of the ground-level-enhancement (GLE), of solar cosmic rays observed with the neutron and muon monitors in the period 1942-1990, it is shown that the solar proton eruptions producible GLE are forbidden during the transition phase of the heliomagnetic polarity reversal, near the period of the maximum solar activity. It is suggested that the quiescence of GLE is not due to the suppression effect of the proton eruption from the Sun by the strong solar magnetic field, but is due to the deterioration of the proton acceleration efficiency by the structual change of the field during the transition period.","subitem_description_type":"Abstract"}]},"item_10001_description_6":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"By using data of the ground-level-enhancement (GLE), of solar cosmic rays observed with the neutron and muon monitors in the period 1942-1990, it is shown that the solar proton eruptions producible GLE are forbidden during the transition phase of the heliomagnetic polarity reversal, near the period of the maximum solar activity. It is suggested that the quiescence of GLE is not due to the suppression effect of the proton eruption from the Sun by the strong solar magnetic field, but is due to the deterioration of the proton acceleration efficiency by the structual change of the field during the transition period.","subitem_description_type":"Other"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0022-1392","subitem_source_identifier_type":"ISSN"}]},"item_10001_textarea_24":{"attribute_name":"所属","attribute_value_mlt":[{"subitem_textarea_value":"Cosmic-Ray Section, Solar-Terrestrial Environment Laboratory, Nagoya University"},{"subitem_textarea_value":"Cosmic-Ray Section, Solar-Terrestrial Environment Laboratory, Nagoya University"},{"subitem_textarea_value":"Department of Information Management, Asahi University"}]},"item_10001_textarea_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_textarea_value":"Society of Geomagnetism and Earth, Planetary and Space Sciences"}]},"item_10001_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":"Nagashima, Kazuo"}],"nameIdentifiers":[{"nameIdentifier":"3891","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Sakakibara, Shizuko"}],"nameIdentifiers":[{"nameIdentifier":"3892","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Morishita, Isao"}],"nameIdentifiers":[{"nameIdentifier":"3888","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"1000040148200","nameIdentifierScheme":"NRID","nameIdentifierURI":" https://rns.nii.ac.jp/d/nr/1000040148200"},{"nameIdentifier":"40148200","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=40148200"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2015-11-10"}],"displaytype":"detail","filename":"00221392_43_685689_1991.pdf","filesize":[{"value":"469.9 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"00221392_43_685689_1991","url":"https://asahi-u.repo.nii.ac.jp/record/3419/files/00221392_43_685689_1991.pdf"},"version_id":"be512008-fc97-4cdb-a872-afb96ce638d2"}]},"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":"Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period.","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period."},{"subitem_title":"Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period.","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"20","path":["133"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-08-11"},"publish_date":"2015-08-11","publish_status":"0","recid":"3419","relation_version_is_last":true,"title":["Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period."],"weko_creator_id":"20","weko_shared_id":20},"updated":"2023-12-19T06:05:29.664486+00:00"}