Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/752
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dc.contributor.authorallGuglielmi, A. V.; Schmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.authorallPotapov, A. S.; Institute of Solar-Terrestrial Physics, Siberian Branch of the Russian Academy of Sciences, Irkutsk, Russiaen
dc.contributor.authorallTsegmed, B.; Astronomy and Geophysics Research Center, Mongolian Academy of Sciences, Ulaanbaatar, Mongoliaen
dc.date.accessioned2006-02-20T09:38:39Zen
dc.date.available2006-02-20T09:38:39Zen
dc.date.issued2004en
dc.identifier.urihttp://hdl.handle.net/2122/752en
dc.description.abstractThe polarization method for recognition of seismomagnetic waves against a noise background is presented. The method is applied to detection of magnetic oscillations accompanying the propagation of surface Love wave after a strong earthquake. A specific property of the Love waves is that theoretically the Tolman-Stewart effect is alone responsible for the magnetic field that penetrates into the Earth's surface. Data from the Mondy Magnetic Observatory and the Talaya Seismic Station suggest that the arrival time, duration, period,and polarization of magnetic signals conform with the idea of generation of alternating electric currents due to fluid vibrations in pores and fractures of rocks under the action of the inertial force associated with the Love wave propagation.en
dc.format.extent555996 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.publisher.nameINGVen
dc.relation.ispartofAnnals of Geophysicsen
dc.relation.ispartofseries1/47 (2004)en
dc.subjectEarth crusten
dc.subjectTolman-Stewart effecten
dc.titleOn the excitation of magnetic signals by Love wavesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.09. Waves and wave analysisen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorGuglielmi, A. V.en
dc.contributor.authorPotapov, A. S.en
dc.contributor.authorTsegmed, B.en
dc.contributor.departmentSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.departmentInstitute of Solar-Terrestrial Physics, Siberian Branch of the Russian Academy of Sciences, Irkutsk, Russiaen
dc.contributor.departmentAstronomy and Geophysics Research Center, Mongolian Academy of Sciences, Ulaanbaatar, Mongoliaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia-
crisitem.author.deptInstitute of Solar-Terrestrial Physics, Siberian Branch of the Russian Academy of Sciences, Irkutsk, Russia-
crisitem.author.deptAstronomy and Geophysics Research Center, Mongolian Academy of Sciences, Ulaanbaatar, Mongolia-
crisitem.classification.parent04. Solid Earth-
Appears in Collections:Annals of Geophysics
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