Storm and substorm causes and effects at midlatitude location for the St Patrick s 2013 and 2015 events
Authors
Guerrero Ortega, AntonioIdentifiers
Permanent link (URI): http://hdl.handle.net/10017/36326DOI: 10.1002/2017JA024224
ISSN: 2169-9402
Date
2017Funders
Ministerio de Economía y Competitividad
Bibliographic citation
Journal of Geophysical Research: Space Physics, 2017, v. 122, n. , p. 1-18
Keywords
Midlatitude substorm effects
Local geomagnetic disturbances
Interaction of interplanetary structures
Project
info: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/
info:eu-repo/grantAgreement/MINECO//AYA2016-80881-P
info:eu-repo/grantAgreement/MINECO//AYA2013-42614-P
Document type
info:eu-repo/semantics/article
Version
info:eu-repo/semantics/publishedVersion
Rights
Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
© 2017 American Geophysical Union
Access rights
info:eu-repo/semantics/openAccess
Abstract
Midlatitude 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.
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storm_guerrero_JGR_2017.pdf | 7.275Mb |
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