Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/7791
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dc.contributor.authorallPrattes, G.en
dc.contributor.authorallSchwingenschuh, K.en
dc.contributor.authorallEichelberger, H. U.en
dc.contributor.authorallMagnes, W.en
dc.contributor.authorallBoudjada, M.en
dc.contributor.authorallStachel, M.en
dc.contributor.authorallVellante, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallVillante, U.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallWesztergom, V.en
dc.contributor.authorallNenovski, P.en
dc.date.accessioned2012-02-22T13:36:06Zen
dc.date.available2012-02-22T13:36:06Zen
dc.date.issued2011en
dc.identifier.urihttp://hdl.handle.net/2122/7791en
dc.description.abstractThis work presents ground based Ultra Low Fre- quency (ULF) magnetic field measurements in the frequency range from 10–15mHz from 1 January 2008 to 14 April 2009. In this time period a strong earthquake series hit the Italian Abruzzo region around L’Aquila with the main stroke of magnitude M = 6.3 on 6 April 2009. In the frame of the South European Geomagnetic Array (SEGMA), a European collaboration runs ULF fluxgate instruments providing con- tinuously magnetic field data recorded in mid- and south Eu- rope. The main scientific objective is the investigation of signal variations due to seismic activity and the discrimi- nation between other natural and human influences. The SEGMA station closest to the L’Aquila earthquake epicen- ter is L’Aquila observatory located in the epicenter region. For the scientific analysis we extract the nighttime period from 22:00–02:00 UT and determine the power spectral den- sity (PSD) of the horizontal (H) and vertical (Z) magnetic field components and the standardized polarization ratio (Z) over (H). To discriminate local emissions from global ge- omagnetic effects, data from three SEGMA stations in dis- tances up to 630 km from the epicenter region are analyzed and further compared to the independent global geomagnetic 􏰎Kp index. Apart from indirect ionospheric effects, elec- tromagnetic noise could be originated in the lithosphere due to tectonic mechanisms in the earthquake focus. To estimate the amplitude of assumed lithospheric electromagnetic noise emissions causing anomalies in the PSD of the (Z) compo- nent, we consider magnetotelluric calculations of the electric crust conductivity in the L’Aquila region. Results found at L’Aquila observatory are interpreted with respect to the litho- sphere electrical conductivity in the local observatory region, the 􏰎Kp index, and further in a multi station analysis. Pos- sible seismic related ULF anomalies occur ∼2 weeks before the main stroke.en
dc.language.isoEnglishen
dc.relation.ispartofNatural Hazards and Earth System Sciences (NHESS)en
dc.relation.ispartofseries/11(2011)en
dc.subjectmagnetic field analysisen
dc.titleUltra Low Frequency (ULF) European multi station magnetic field analysis before and during the 2009 earthquake at L'Aquila regarding regional geotechnical informationen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1959-1968en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.99. General or miscellaneousen
dc.identifier.doi10.5194/nhess-11-1959-2011en
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.relation.issn1561-8633en
dc.relation.eissn1684-9981en
dc.contributor.authorPrattes, G.en
dc.contributor.authorSchwingenschuh, K.en
dc.contributor.authorEichelberger, H. U.en
dc.contributor.authorMagnes, W.en
dc.contributor.authorBoudjada, M.en
dc.contributor.authorStachel, M.en
dc.contributor.authorVellante, M.en
dc.contributor.authorVillante, U.en
dc.contributor.authorWesztergom, V.en
dc.contributor.authorNenovski, P.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
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 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.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-3630-7958-
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.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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