Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11209
DC FieldValueLanguage
dc.date.accessioned2018-03-15T13:22:40Zen
dc.date.available2018-03-15T13:22:40Zen
dc.date.issued2017-03-01en
dc.identifier.urihttp://hdl.handle.net/2122/11209en
dc.description.abstractA large earthquake of 7.8 magnitude occurred on 25 April 2015, 06:26 UTC, with the epicenter in Nepal. Here, taking advantage of measurements provided by the Swarm magnetic satellites, we investigate the possibility to detect some series of pre-earthquake magnetic anomalous signals, likely due to a lithosphere–atmosphere–ionosphere coupling, that can be a potential earthquake precursory pattern. Different techniques have been applied to Swarm data available during two months around earthquake occurrence. From the detected magnetic anomalies series (during night and magnetically quiet times or with an automatic detection algorithm), we show that the cumulative number of anomalies follows the same typical power-law behavior of a critical system approaching its critical time, and hence recovers as the typical recovery phase after a large event. The similarity of this behavior with the one obtained from seismic data analysis and the application of the analyses also to another period without significant seismicity do support a lithospheric-linked origin of the observed magnetic anomalies. We suggest that they might be connected to the preparation phase of the Nepal earthquake.en
dc.language.isoEnglishen
dc.relation.ispartofEarth and planetary science lettersen
dc.relation.ispartofseries/461(2017)en
dc.titlePotential earthquake precursory pattern from space: The 2015 Nepal event as seen by magnetic Swarm satellitesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber119-126en
dc.subject.INGV04.06. Seismologyen
dc.identifier.doi10.1016/j.epsl.2016.12.037en
dc.description.obiettivoSpecifico6T. Variazioni delle caratteristiche crostali e precursorien
dc.description.journalTypeJCR Journalen
dc.contributor.authorDe Santis, Angeloen
dc.contributor.authorBalasis, Georgeen
dc.contributor.authorPavòn-Carrasco, Francisco J.en
dc.contributor.authorCianchini, Gianfrancoen
dc.contributor.authorMandea, Mioaraen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentInstitute for Astronomy, Astrophysics, Space Applications and Remote Sensing, National Observatory of Athens, Athens, Greeceen
dc.contributor.departmentUniversidad Complutense de Madrid, Madrid, Spainen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentCentre National d'Etudes Spatiales, Paris, Franceen
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.deptNational Observatoryof Athens-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptInstitut de Physique du Globe de Paris-IPGP, Université Paris-Diderot & CNRS, 5 rue Thomas Mann,75205 Paris, France-
crisitem.author.orcid0000-0002-3941-656X-
crisitem.author.orcid0000-0001-7342-0557-
crisitem.author.orcid0000-0003-2832-0068-
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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