Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9858
DC FieldValueLanguage
dc.contributor.authorallNenovski, P. I.en
dc.contributor.authorallPezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallCiraolo, L.en
dc.contributor.authorallVellante, M.en
dc.contributor.authorallVillante, U.en
dc.contributor.authorallDe Lauretis, M.en
dc.date.accessioned2015-06-11T06:38:31Zen
dc.date.available2015-06-11T06:38:31Zen
dc.date.issued2015-01-01en
dc.identifier.urihttp://hdl.handle.net/2122/9858en
dc.description.abstractIonospheric TEC (total electron content) variations derived from GPS measurements recorded at 7 GPS stations in Northern, Central and Southern Italy before and after the 2009 Abruzzo earthquake (EQ) of magnitude Mw6.3 were processed and analyzed. The analysis included interpolated and non-interpolated TEC data. Variations in the TEC of both regional and local characteristics were revealed. Several regional changes were observed in the studied period: 1 January–21 April 2009. After analyzing non-interpolated TEC data of 5 GPS stations in Central Italy (Unpg (Perugia), Untr (Terni), Aqui (Aquila), M0se (Rome) and Paca (Palma Campania, (Naples)), a local disturbance of TEC was also found. This local TEC disturbance arises preparatory to the EQ main shock occurred at 01:32 UT on 06 April 2009, maximizes its amplitude of ~0.8 TECu after the shock moment and disappears after it. The local TEC disturbance was confined at heights below 160 km, i.e. in the lower ionosphere.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofAdvances in space researchen
dc.relation.ispartofseries1/55(2015)en
dc.subjectGPS measurementsen
dc.subjectTotal electron content (TEC)en
dc.subjectTEC disturbanceen
dc.subjectLower ionosphereen
dc.subjectEarthquake shocken
dc.titleLocal changes in the total electron content immediately before the 2009 Abruzzo earthquakeen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber243–258en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.02. Dynamicsen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.05. Wave propagationen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.99. General or miscellaneousen
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.10. Instruments and techniquesen
dc.identifier.doi10.1016/j.asr.2014.09.029en
dc.description.obiettivoSpecifico4T. Fisica dei terremoti e scenari cosismicien
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.relation.issn0273-1177en
dc.relation.eissn1879-1948en
dc.contributor.authorNenovski, P. I.en
dc.contributor.authorPezzopane, M.en
dc.contributor.authorCiraolo, L.en
dc.contributor.authorVellante, M.en
dc.contributor.authorVillante, U.en
dc.contributor.authorDe Lauretis, M.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
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 di Ricerche Sulle Onde Elettromagnetiche, Firenze, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptDipartimento di Fisica, Università dell'Aquila, Italy-
crisitem.author.orcid0000-0001-5800-2322-
crisitem.author.orcid0000-0002-3630-7958-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
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