Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10867
DC FieldValueLanguage
dc.date.accessioned2018-02-28T08:50:41Zen
dc.date.available2018-02-28T08:50:41Zen
dc.date.issued2017-10-15en
dc.identifier.urihttp://hdl.handle.net/2122/10867en
dc.description.abstractWe provide insights about how the Total Electron Content (TEC), derived by a network of Global Navigation Satellite System (GNSS) receivers over the European longitudinal sector, reacts to a Sudden Impulse (SI). In particular, we investigate how the different components of the TEC variability relates with the ionospheric currents, derived by ground magnetometers and the Piersanti and Villante (2016) model, during the 2015 Saint Patrick’s Day storm. To identify the different TEC components, we apply the Ensemble Empirical Mode Decomposition (EEMD) analysis to vertical TEC (vTEC) time series to isolate its SI-related variations over co-located GNSS receiver-magnetometer couples. With such an approach, we were able to identify for the first time a peculiar vTEC mode (WstarHT, T 45 min) switching on during the SI and propagating southward with a velocity of ∼1.5 km/s. We also found a linear relationship between the estimated ionospheric current and the temporal fluctuations of WstarHT for both the Preliminary Impulse (PI) and the Main Impulse (MI). The slope has been found to depend only on the electron charge, on the magnetic permeability and on the altitude of the ionospheric E-layer, as expected from first principles equations and as discussed in details.en
dc.language.isoEnglishen
dc.relation.ispartofAdvances in Space Researchen
dc.relation.ispartofseries/60 (2017)en
dc.titleDoes TEC react to a sudden impulse as a whole? The 2015 Saint Patrick’s day storm eventen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1807-1816en
dc.identifier.URLhttps://www.sciencedirect.com/science/article/pii/S0273117717300510en
dc.identifier.doi10.1016/j.asr.2017.01.021en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.contributor.authorPiersanti, M.en
dc.contributor.authorCesaroni, Claudioen
dc.contributor.authorSpogli, Lucaen
dc.contributor.authorAlberti, T.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0001-5207-2944-
crisitem.author.orcid0000-0003-2268-4389-
crisitem.author.orcid0000-0003-2310-0306-
crisitem.author.orcid0000-0001-6096-0220-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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