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dc.contributor.author Nava, B.
dc.contributor.author Rodríguez-Zuluaga, J.
dc.contributor.author Alazo-Cuartas, K.
dc.contributor.author Kashcheyev, A.
dc.contributor.author Migoya-Orué, Y.
dc.contributor.author Radicella, S. M.
dc.contributor.author Amory-Mazaudier, C.
dc.contributor.author Fleury, R.
dc.date.accessioned 2018-11-21T12:59:37Z
dc.date.available 2018-11-21T12:59:37Z
dc.date.issued 2016-03-10
dc.identifier.citation Nava, B., Rodríguez-Zuluaga, J., Alazo-Cuartas, K., Kashcheyev, A., Migoya-Orué, Y., Radicella, S. M., ... Fleury, R. (2016). Middle‐ and low‐latitude ionosphere response to 2015 St. Patrick's Day geomagnetic storm.==$Journal of Geophysical Research: Space Physics, 121$==(4), 3421-3438. https://doi.org/10.1002/2015JA022299 es_ES
dc.identifier.uri http://hdl.handle.net/20.500.12816/3768
dc.description.abstract This paper presents a study of the St Patrick's Day storm of 2015, with its ionospheric response at middle and low latitudes. The effects of the storm in each longitudinal sector (Asian, African, American, and Pacific) are characterized using global and regional electron content. At the beginning of the storm, one or two ionospheric positive storm effects are observed depending on the longitudinal zones. After the main phase of the storm, a strong decrease in ionization is observed at all longitudes, lasting several days. The American region exhibits the most remarkable increase in vertical total electron content (vTEC), while in the Asian sector, the largest decrease in vTEC is observed. At low latitudes, using spectral analysis, we were able to separate the effects of the prompt penetration of the magnetospheric convection electric field (PPEF) and of the disturbance dynamo electric field (DDEF) on the basis of ground magnetic data. Concerning the PPEF, Earth's magnetic field oscillations occur simultaneously in the Asian, African, and American sectors, during southward magnetization of the Bz component of the interplanetary magnetic field. Concerning the DDEF, diurnal magnetic oscillations in the horizontal component H of the Earth's magnetic field exhibit a behavior that is opposed to the regular one. These diurnal oscillations are recognized to last several days in all longitudinal sectors. The observational data obtained by all sensors used in the present paper can be interpreted on the basis of existing theoretical models. es_ES
dc.format application/pdf es_ES
dc.language.iso eng es_ES
dc.publisher American Geophysical Union es_ES
dc.relation.ispartof urn:issn:2169-9380
dc.rights info:eu-repo/semantics/restrictedAccess es_ES
dc.subject Geomagnetic storm es_ES
dc.subject Equatorial ionosphere es_ES
dc.subject Prompt penetration of magnetospheric electric field es_ES
dc.subject Ionospheric disturbance dynamo es_ES
dc.subject Global Electron Content es_ES
dc.title Middle‐ and low‐latitude ionosphere response to 2015 St. Patrick's Day geomagnetic storm es_ES
dc.type info:eu-repo/semantics/article es_ES
dc.subject.ocde http://purl.org/pe-repo/ocde/ford#1.05.01 es_ES
dc.identifier.journal Journal of Geophysical Research: Space Physics es_ES
dc.description.peer-review Por pares es_ES
dc.identifier.doi https://doi.org/10.1002/2015JA022299 es_ES

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