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dc.contributor.authorCid Tortuero, Consuelo 
dc.contributor.authorSaiz Villanueva, María Elena 
dc.contributor.authorGuerrero Ortega, Antonio 
dc.contributor.authorPalacios Hernández, Judith 
dc.contributor.authorCerrato Montalbán, Yolanda 
dc.date.accessioned2017-04-27T13:40:35Z
dc.date.available2017-04-27T13:40:35Z
dc.date.issued2015-05-21
dc.identifier.bibliographicCitationJournal of Space Weather and Space Climate, 2015, v. A16, n. 5, p. 1-6
dc.identifier.issn2115-7251
dc.identifier.urihttp://hdl.handle.net/10017/29324
dc.description.abstractIn September 1859 the Colaba observatory measured the most extreme geomagnetic disturbance ever recorded at low latitudes related to solar activity: the Carrington storm. This paper describes a geomagnetic disturbance case with a profile extraordinarily similar to the disturbance of the Carrington event at Colaba: the event on 29 October 2003 at Tihany magnetic observatory in Hungary. The analysis of the H-field at different locations during the ''Carrington-like'' event leads to a re-interpretation of the 1859 event. The major conclusions of the paper are the following: (a) the global Dst or SYM-H, as indices based on averaging, missed the largest geomagnetic disturbance in the 29 October 2003 event and might have missed the 1859 disturbance, since the large spike in the horizontal component (H) of terrestrial magnetic field depends strongly on magnetic local time (MLT); (b) the main cause of the large drop in H recorded at Colaba during the Carrington storm was not the ring current but field-aligned currents (FACs); and (c) the very local signatures of the H-spike imply that a Carrington-like event can occur more often than expected.en
dc.description.sponsorshipMinisterio de Economía, Industria y Competitividades_ES
dc.description.sponsorshipJunta de Comunidades de Castilla-La Manchaes_ES
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.rightsAttribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)*
dc.rights© EDP Sciences, 2015
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/*
dc.subjectGeomagnetics stormsen
dc.subjectSpace Physicsen
dc.subjectSolar and Stellar Astrophysicsen
dc.titleA Carrington-like geomagnetic storm observed in the 21st centuryen
dc.typeinfo:eu-repo/semantics/articleen
dc.subject.ecienciaFísicaes_ES
dc.subject.ecienciaPhysicsen
dc.subject.ecienciaAstronomíaes_ES
dc.subject.ecienciaAstronomyen
dc.contributor.affiliationUniversidad de Alcalá. Departamento de Física y Matemáticases_ES
dc.date.updated2017-04-27T13:37:53Z
dc.relation.publisherversionhttp:/7dx.doi.org/10.1051/swsc/2015017
dc.type.versioninfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1051/swsc/2015017
dc.relation.projectIDinfo:eu-repo/grantAgreement/MINECO//AYA2013-47735-P/ES/NUEVOS RETOS EN LA CIENCIA DE LA INTERACCION SOL-TIERRA ANTE LAS NECESIDADES TECNOLOGICAS DE LA SOCIEDAD ACTUALes_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/JCCM//PPII10-0183-7802/ESes_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessen
dc.identifier.uxxiAR/0000021726
dc.identifier.publicationtitleJournal of Space Weather and Space Climateen
dc.identifier.publicationlastpage6
dc.identifier.publicationissue5
dc.identifier.publicationfirstpage1


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