{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004239676151552.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/1538-4357/aae47c"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/869/i=1/a=57/pdf"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/869/i=1/a=57?key=crossref.a81a7ce0e9e0583235a7ddd09a903541"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/aae47c"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/aae47c/pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1811.02786"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Low-latitude Aurorae during the Extreme Space Weather Events in 1859"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>The Carrington storm (1859 September 1/2) is one of the largest magnetic storms ever observed, and it caused global auroral displays in low-latitude areas, together with a series of multiple magnetic storms from 1859 August 28 to September 4. In this study, we revisit contemporary auroral observation records to extract information on their elevation angle, color, and direction to investigate this stormy interval in detail. We first examine the equatorward boundary of the “auroral emission with multiple colors” based on descriptions of elevation angle and color. We find that their locations were 36.°5 ILAT on August 28/29 and 32.°7 ILAT on September 1/2, suggesting that trapped electrons moved to, at least, <jats:italic>L</jats:italic> ∼ 1.55 and <jats:italic>L</jats:italic> ∼ 1.41, respectively. The equatorward boundary of “purely red emission” was likely located at 30.°8 ILAT on September 1/2. If the “purely red emission” was a stable auroral red arc, it would suggest that trapped protons moved to, at least, <jats:italic>L</jats:italic> ∼ 1.36. This reconstruction with observed auroral emission regions provides conservative estimations of magnetic storm intensities. We compare the auroral records with magnetic observations. We confirm that multiple magnetic storms occurred during this stormy interval, and that the equatorward expansion of the auroral oval is consistent with the timing of magnetic disturbances. It is possible that the August 28/29 interplanetary coronal mass ejections (ICMEs) cleared out the interplanetary medium, making the ICME for the Carrington storm on September 1/2 more geoeffective.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004239676151554","@type":"Researcher","foaf:name":[{"@value":"Hisashi Hayakawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1420001326213719936","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"80342616"},{"@type":"NRID","@value":"1000080342616"},{"@type":"ORCID","@value":"0000-0002-2293-1557"},{"@type":"NRID","@value":"9000414093089"},{"@type":"NRID","@value":"9000279889956"},{"@type":"NRID","@value":"9000399770571"},{"@type":"NRID","@value":"9000399535932"},{"@type":"NRID","@value":"9000400195916"},{"@type":"NRID","@value":"9000400187668"},{"@type":"NRID","@value":"9000254739231"},{"@type":"NRID","@value":"9000402481678"},{"@type":"NRID","@value":"9000415306282"},{"@type":"NRID","@value":"9000415306307"},{"@type":"NRID","@value":"9000415083365"},{"@type":"NRID","@value":"9000406032347"},{"@type":"NRID","@value":"9000400195919"},{"@type":"NRID","@value":"9000400195928"},{"@type":"NRID","@value":"9000356514818"},{"@type":"NRID","@value":"9000397828344"},{"@type":"NRID","@value":"9000400195915"},{"@type":"NRID","@value":"9000415306275"},{"@type":"NRID","@value":"9000006128142"},{"@type":"NRID","@value":"9000023592009"},{"@type":"NRID","@value":"9000285477709"},{"@type":"NRID","@value":"9000242547350"},{"@type":"NRID","@value":"9000387919546"},{"@type":"NRID","@value":"9000010295541"},{"@type":"NRID","@value":"9000394956316"},{"@type":"NRID","@value":"9000415306271"},{"@type":"NRID","@value":"9000331467481"},{"@type":"NRID","@value":"9000405868644"},{"@type":"NRID","@value":"9000415306259"},{"@type":"NRID","@value":"9000003005043"},{"@type":"NRID","@value":"9000410485045"},{"@type":"NRID","@value":"9000249538111"},{"@type":"NRID","@value":"9000404664680"},{"@type":"NRID","@value":"9000413742904"},{"@type":"NRID","@value":"9000259864142"},{"@type":"NRID","@value":"9000400195931"},{"@type":"NRID","@value":"9000415306294"},{"@type":"NRID","@value":"9000002249321"},{"@type":"NRID","@value":"9000023868455"},{"@type":"NRID","@value":"9000413694786"},{"@type":"NRID","@value":"9000323844334"},{"@type":"NRID","@value":"9000314389252"},{"@type":"NRID","@value":"9000297476894"},{"@type":"NRID","@value":"9000415306313"},{"@type":"NRID","@value":"9000415306297"},{"@type":"NRID","@value":"9000023975269"},{"@type":"NRID","@value":"9000413501580"},{"@type":"NRID","@value":"9000313628893"},{"@type":"NRID","@value":"9000344802293"},{"@type":"NRID","@value":"9000279889919"},{"@type":"NRID","@value":"9000331448786"},{"@type":"NRID","@value":"9000400195923"},{"@type":"NRID","@value":"9000006566239"},{"@type":"NRID","@value":"9000023578997"},{"@type":"NRID","@value":"9000333209113"},{"@type":"NRID","@value":"9000332222013"},{"@type":"NRID","@value":"9000398156129"},{"@type":"NRID","@value":"9000399010785"},{"@type":"NRID","@value":"9000415306284"},{"@type":"NRID","@value":"9000415306287"},{"@type":"NRID","@value":"9000331467378"},{"@type":"NRID","@value":"9000399262075"},{"@type":"NRID","@value":"9000400195921"},{"@type":"NRID","@value":"9000400195934"},{"@type":"NRID","@value":"9000002259964"},{"@type":"NRID","@value":"9000356514765"},{"@type":"NRID","@value":"9000415306303"},{"@type":"NRID","@value":"9000414093073"},{"@type":"NRID","@value":"9000258442298"},{"@type":"NRID","@value":"9000331429461"},{"@type":"NRID","@value":"9000414093083"},{"@type":"NRID","@value":"9000335567844"},{"@type":"NRID","@value":"9000337100484"},{"@type":"NRID","@value":"9000242547303"},{"@type":"NRID","@value":"9000356514872"},{"@type":"NRID","@value":"9000002635483"},{"@type":"NRID","@value":"9000023589404"},{"@type":"NRID","@value":"9000331467432"},{"@type":"NRID","@value":"9000400195926"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/ebihara_yusuke"}],"foaf:name":[{"@value":"Yusuke Ebihara"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676151298","@type":"Researcher","foaf:name":[{"@value":"David P. Hand"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676151681","@type":"Researcher","foaf:name":[{"@value":"Satoshi Hayakawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676151424","@type":"Researcher","foaf:name":[{"@value":"Sandeep Kumar"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676151299","@type":"Researcher","foaf:name":[{"@value":"Shyamoli Mukherjee"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676151680","@type":"Researcher","foaf:name":[{"@value":"B. Veenadhari"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2018-12-10","prism:volume":"869","prism:number":"1","prism:startingPage":"57"},"reviewed":"false","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"http://stacks.iop.org/0004-637X/869/i=1/a=57/pdf"},{"@id":"http://stacks.iop.org/0004-637X/869/i=1/a=57?key=crossref.a81a7ce0e9e0583235a7ddd09a903541"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/aae47c"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/aae47c/pdf"}],"createdAt":"2018-12-11","modifiedAt":"2024-01-12","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Earth%20and%20Planetary%20Astrophysics%20(astro-ph.EP)","dc:title":"Earth and Planetary Astrophysics (astro-ph.EP)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=Space%20Physics%20(physics.space-ph)","dc:title":"Space Physics (physics.space-ph)"},{"@id":"https://cir.nii.ac.jp/all?q=Geophysics%20(physics.geo-ph)","dc:title":"Geophysics (physics.geo-ph)"},{"@id":"https://cir.nii.ac.jp/all?q=Physics%20-%20Geophysics","dc:title":"Physics - Geophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Physics%20-%20Space%20Physics","dc:title":"Physics - Space Physics"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Solar%20and%20Stellar%20Astrophysics","dc:title":"Astrophysics - Solar and Stellar Astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Solar%20and%20Stellar%20Astrophysics%20(astro-ph.SR)","dc:title":"Solar and Stellar Astrophysics (astro-ph.SR)"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Earth%20and%20Planetary%20Astrophysics","dc:title":"Astrophysics - Earth and Planetary Astrophysics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781833824512","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15H05816"},{"@type":"JGN","@value":"JP15H05816"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-15H05816/"}],"notation":[{"@language":"ja","@value":"太陽周期活動の予測とその地球環境影響の解明"},{"@language":"en","@value":"Prediction of solar cycle activity and investigation of its impact on climate"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781866899328","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15K21709"},{"@type":"JGN","@value":"JP15K21709"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-INTERNATIONAL-15K21709/"}],"notation":[{"@language":"ja","@value":"太陽地球圏環境予測における国際連携研究の推進"},{"@language":"en","@value":"Development of International Collaboration for Solar-Terrestrial Environment 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dynamics"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256938045824","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17J06954"},{"@type":"JGN","@value":"JP17J06954"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17J06954/"}],"notation":[{"@language":"ja","@value":"ポストモンゴル期ユーラシア交通史と自然環境"},{"@language":"en","@value":"Transportation History in Post-Mongolian Eurasia and its Environmental Aspect"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256969268864","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18H01254"},{"@type":"JGN","@value":"JP18H01254"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18H01254/"}],"notation":[{"@language":"ja","@value":"歴史文献を用いた過去の太陽活動の研究"},{"@language":"en","@value":"Study on past solar activity using historical documents"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001335841025920","@type":"Article","resourceType":"学術雑誌論文(journal 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Storms"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292617914527360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observations and theory of the formation of stable auroral red arcs"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292618814749184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Estimation of interplanetary electric field conditions for historical geomagnetic storms"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292618993991168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Anomalous transport produced by kinetic Alfvén wave turbulence"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619538181504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Stable auroral red arcs, sinks for energy of<i>D</i><sub><i>st</i></sub>main 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M. Ngwira, A. Pulkkinen, M. M. Kuznetsova, and A. 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