Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8671
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dc.contributor.authorallDudkin, F.; Lviv Centre of Institute for Space Research, Ukraineen
dc.contributor.authorallKorepanov, V.; Lviv Centre of Institute for Space Research, Ukraineen
dc.contributor.authorallHayakawa, M.; University of Electro-Communications, Japanen
dc.contributor.authorallDe Santis, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2013-04-23T13:39:03Zen
dc.date.available2013-04-23T13:39:03Zen
dc.date.issued2013-01en
dc.identifier.isbn978-960-89704-1-0en
dc.identifier.urihttp://hdl.handle.net/2122/8671en
dc.description.abstractFew days before many earthquakes a general change in the ratio of vertical to horizontal magnetic field components in the ULF band, often called “polarization”, has been observed that can be considered as a magnetic precursor of the subsequent earthquake. To explain such a specific behavior, we propose a simple model based on a linear current approximation depending on some assumption on the signal to noise ratio. This model is confirmed through a comparison that has been carried out between the experimental magnetic field data at Matsushiro (Japan, 1998.06.30, M=4.7) and Simeiz (Crimea, Ukraine, 1998.10.16, M=4.3 and 1998.10.18, M=4.3) earthquakes. About 1 – 2 days before these events we had recorded the anomalous decrease of the ratio of vertical to horizontal magnetic field components in Pc4 – Pc3 band. The NE-SW direction of the corresponding current linear model well agrees with the main tectonic feature of both seismogenic events. Additionally we also estimate the signal to noise ratio limits for the detection of ULF magnetic field components in Corralitos and Stanford campus for Loma Prieta (MS 7.1, 1989) earthquake.en
dc.language.isoEnglishen
dc.subjectelectromagnetismen
dc.subjectseismic forecastingen
dc.subjectseismic source modelen
dc.titlePossible model of electromagnetic signals before earthquakesen
dc.typebook chapteren
dc.description.statusPublisheden
dc.description.pagenumber159-170en
dc.subject.INGV04. Solid Earth::04.02. Exploration geophysics::04.02.04. Magnetic and electrical methodsen
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.03. Earthquake source and dynamicsen
dc.description.obiettivoSpecifico1.8. Osservazioni di geofisica ambientaleen
dc.description.obiettivoSpecifico2.6. TTC - Laboratorio di gravimetria, magnetismo ed elettromagnetismo in aree attiveen
dc.description.obiettivoSpecifico3.1. Fisica dei terremotien
dc.description.fulltextrestricteden
dc.contributor.authorDudkin, F.en
dc.contributor.authorKorepanov, V.en
dc.contributor.authorHayakawa, M.en
dc.contributor.authorDe Santis, A.en
dc.contributor.departmentLviv Centre of Institute for Space Research, Ukraineen
dc.contributor.departmentLviv Centre of Institute for Space Research, Ukraineen
dc.contributor.departmentUniversity of Electro-Communications, Japanen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypebook chapter-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptLviv Centre of Institute for Space Research, Ukraine-
crisitem.author.deptLviv Centre of Institute for Space Research, Ukraine-
crisitem.author.deptDepartment of Electronic Engineering, The University of Electro-Communications, Chofu, Tokyo, Japan-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-3941-656X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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