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dc.contributor.authorGuerrero Ortega, Antonio 
dc.contributor.authorPalacios Hernández, Judith 
dc.contributor.authorRodriguez Bouza, M.
dc.contributor.authorRodriguez Bilbao, I.
dc.contributor.authorAran, A.
dc.contributor.authorCid Tortuero, Consuelo 
dc.contributor.authorHerraiz Sarachaga, Miguel
dc.contributor.authorSaiz Villanueva, María Elena 
dc.contributor.authorRodriguez Caderot, G.
dc.contributor.authorCerrato Montalbán, Yolanda 
dc.date.accessioned2019-03-05T10:17:23Z
dc.date.available2019-03-05T10:17:23Z
dc.date.issued2017
dc.identifier.bibliographicCitationJournal of Geophysical Research: Space Physics, 2017, v. 122, n. , p. 1-18en
dc.identifier.issn2169-9402
dc.identifier.urihttp://hdl.handle.net/10017/36326
dc.description.abstractMidlatitude locations are unique regions exposed to both geomagnetic storm and substorm effects, which may be superposed on specific events imposing an extra handicap for the analysis and identification of the sources and triggers. We study space weather effects at the midlatitude location of the Iberian Peninsula for the St. Patrick's day events in 2013 and 2015. We have been able to identify and separate storm and substorm effects on ground magnetometer data from San Pablo-Toledo observatory during storm time revealing important contributions of the Substorm Current Wedge on both events. The analysis of these substorm local signatures have shown to be related to the production of effective geomagnetically induced currents and ionospheric disturbances as measured from Global Navigation Satellite Systems data at MAD2 IGS permanent station and not directly related to the storm main phase. The whole Sun-to-Earth chain has been analyzed in order to identify the solar and interplanetary triggers. In both events a high-speed stream (HSS) and a coronal mass ejections (CME) are involved, though for 2015 event, the HSS has merged with the CME, increasing the storm geoeffectiveness. The enhancement of substorm geoeffectiveness is justified by the effects of the inclined magnetic axes of the Sun and of the Earth during equinox period.en
dc.description.sponsorshipMinisterio de Economía y Competitividades_ES
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.publisherAGU
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)*
dc.rights© 2017 American Geophysical Union
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectMidlatitude substorm effectsen
dc.subjectLocal geomagnetic disturbancesen
dc.subjectInteraction of interplanetary structuresen
dc.titleStorm and substorm causes and effects at midlatitude location for the St Patrick s 2013 and 2015 eventsen
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.updated2019-03-05T10:08:23Z
dc.relation.publisherversionhttps://doi.org/10.1002/2017JA024224
dc.type.versioninfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1002/2017JA024224
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 ACTUAL/es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/MINECO//AYA2016-80881-Pes_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/MINECO//AYA2013-42614-Pes_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessen
dc.identifier.uxxiAR/0000028060
dc.identifier.publicationtitleJournal of Geophysical Research: Space Physicsen
dc.identifier.publicationvolume122
dc.identifier.publicationlastpage18
dc.identifier.publicationfirstpage1


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