{"created":"2021-12-06T05:38:13.301993+00:00","id":2001671,"links":{},"metadata":{"_buckets":{"deposit":"aeafabcc-1187-484f-be84-619f5d7d34f9"},"_deposit":{"created_by":17,"id":"2001671","owner":"17","owners":[17],"owners_ext":{"displayname":"\u56f3\u66f8\u60c5\u5831\u4fc2","username":"repository"},"pid":{"revision_id":0,"type":"depid","value":"2001671"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:02001671","sets":[]},"author_link":[],"control_number":"2001671","item_1615768549627":{"attribute_name":"\u51fa\u7248\u30bf\u30a4\u30d7","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_1629683748249":{"attribute_name":"\u65e5\u4ed8","attribute_value_mlt":[{"subitem_date_issued_datetime":"2021-12-06","subitem_date_issued_type":"Available"}]},"item_9_biblio_info_6":{"attribute_name":"\u66f8\u8a8c\u60c5\u5831","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2021-04","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"4","bibliographicPageStart":"e2020JA029081","bibliographicVolumeNumber":"126","bibliographic_titles":[{"bibliographic_title":"Journal of Geophysical Research: Space Physics","bibliographic_titleLang":"en"}]}]},"item_9_description_4":{"attribute_name":"\u5185\u5bb9\u8a18\u8ff0","attribute_value_mlt":[{"subitem_description":"Stable auroral red (SAR) arcs are optical events with dominant 630.0-nm emission caused by low-energy electron heat flux into the topside ionosphere from the inner magnetosphere. SAR arcs are observed at subauroral latitudes and often occur during the recovery phase of magnetic storms and substorms. Past studies concluded that these low-energy electrons were generated in the spatial overlap region between the outer plasmasphere and ring-current ions and suggested that Coulomb collisions between plasmaspheric electrons and ring-current ions are more feasible for the SAR-arc generation mechanism rather than Landau damping by electromagnetic ion cyclotron waves or kinetic Alfv\u00e9n waves. This work studies three separate SAR-arc events with conjunctions, using all-sky imagers and inner magnetospheric satellites (Arase and Radiation Belt Storm Probes [RBSP]) during non-storm-time substorms on December 19, 2012 (event 1), January 17, 2015 (event 2), and November 4, 2019 (event 3). We evaluated for the first time the heat flux via Coulomb collision using full-energy-range ion data obtained by the satellites. The electron heat fluxes due to Coulomb collisions reached \u223c109 eV/cm2/s for events 1 and 2, indicating that Coulomb collisions could have caused the SAR arcs. RBSP-A also observed local enhancements of 7\u201320-mHz electromagnetic wave power above the SAR arc in event 2. The heat flux for the freshly detached SAR arc in event 3 reached \u223c108 eV/cm2/s, which is insufficient to have caused the SAR arc. In event 3, local flux enhancement of electrons (<200 eV) and various electromagnetic waves were observed, these are likely to have caused the freshly detached SAR arc.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_9_publisher_32":{"attribute_name":"\u51fa\u7248\u8005","attribute_value_mlt":[{"subitem_publisher":"Wiley","subitem_publisher_language":"en"}]},"item_9_relation_43":{"attribute_name":"\u95a2\u9023\u60c5\u5831","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1029/2020JA029081","subitem_relation_type_select":"DOI"}}]},"item_9_rights_12":{"attribute_name":"\u6a29\u5229","attribute_value_mlt":[{"subitem_rights":"\u00a9 2021 American Geophysical Union","subitem_rights_language":"en"}]},"item_9_source_id_7":{"attribute_name":"\u53ce\u9332\u7269\u8b58\u5225\u5b50","attribute_value_mlt":[{"subitem_source_identifier":"2169-9380","subitem_source_identifier_type":"PISSN"}]},"item_access_right":{"attribute_name":"\u30a2\u30af\u30bb\u30b9\u6a29","attribute_value_mlt":[{"subitem_access_right":"open access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_abf2"}]},"item_creator":{"attribute_name":"\u8457\u8005","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Inaba, Yudai","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Shiokawa, Kazuo","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Oyama, Shin\u2010ichiro","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Otsuka, Yuichi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Connors, Martin","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Schofield, Ian","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Miyoshi, Yoshizumi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Imajo, Shun","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Shinbori, Atsuki","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Gololobov, Artem Yu","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Kazama, Yoichi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Wang, Shiang\u2010Yu","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Tam, Sunny W. Y.","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Chang, Tzu\u2010Fang","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Wang, Bo\u2010Jhou","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Asamura, Kazushi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Yokota, Shoichiro","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Kasahara, Satoshi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Keika, Kunihiro","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Hori, Tomoaki","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Matsuoka, Ayako","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Kasahara, Yoshiya","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Kumamoto, Atsushi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Matsuda, Shoya","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Kasaba, Yasumasa","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Tsuchiya, Fuminori","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Shoji, Masafumi","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Kitahara, Masahiro","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Nakamura, Satoko","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Shinohara, Iku","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Spence, Harlan E.","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Reeves, Geoff D.","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Macdowall, Robert J.","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Smith, Charles W.","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Wygant, John R.","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Bonnell, John W.","creatorNameLang":"en"}]}]},"item_files":{"attribute_name":"\u30d5\u30a1\u30a4\u30eb\u60c5\u5831","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_access","date":[{"dateType":"Available","dateValue":"2021-12-06"}],"displaytype":"detail","filename":"2020JA029081.pdf","filesize":[{"value":"13.1 MB"}],"format":"application/pdf","mimetype":"application/pdf","url":{"objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/2001671/files/2020JA029081.pdf"},"version_id":"3fdd29d6-078d-490f-bf44-f8148cfd3645"}]},"item_language":{"attribute_name":"\u8a00\u8a9e","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"\u8cc7\u6e90\u30bf\u30a4\u30d7","attribute_value_mlt":[{"resourcetype":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Multi\u2010Event Analysis of Plasma and Field Variations in Source of Stable Auroral Red (SAR) Arcs in Inner Magnetosphere During Non\u2010Storm\u2010Time Substorms","item_titles":{"attribute_name":"\u30bf\u30a4\u30c8\u30eb","attribute_value_mlt":[{"subitem_title":"Multi\u2010Event Analysis of Plasma and Field Variations in Source of Stable Auroral Red (SAR) Arcs in Inner Magnetosphere During Non\u2010Storm\u2010Time Substorms","subitem_title_language":"en"}]},"item_type_id":"40001","owner":"17","path":["879/880/881"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2021-12-06"},"publish_date":"2021-12-06","publish_status":"0","recid":"2001671","relation_version_is_last":true,"title":["Multi\u2010Event Analysis of Plasma and Field Variations in Source of Stable Auroral Red (SAR) Arcs in Inner Magnetosphere During Non\u2010Storm\u2010Time Substorms"],"weko_creator_id":"17","weko_shared_id":-1},"updated":"2021-12-06T05:53:51.184439+00:00"}