Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/748
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dc.contributor.authorallMolchanov, O. A.; Schmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.authorallYu. Schekotov, A.; Schmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.authorallFedorov, E.; Schmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.authorallBelyaev, G. G.; Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation (IZMIRAN), Russian Academy of Science, Troitsk (Moscow Region), Russiaen
dc.contributor.authorallSolovieva, M. S.; Schmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.authorallHayakawa, M.; The University of Electro-Communications, Chofugaoka, Chofu, Tokyo, Japanen
dc.date.accessioned2006-02-20T09:27:36Zen
dc.date.available2006-02-20T09:27:36Zen
dc.date.issued2004en
dc.identifier.urihttp://hdl.handle.net/2122/748en
dc.description.abstractWe present the results of ULF magnetic field observation at Karimshino station (Kamchatka, Russia). Using a case study we discovered an effect of suppression of ULF intensity about 2-6 days before rather strong and isolated seismic shocks (magnitude M = 4.6-6.6). It is revealed for nighttime and the horizontal component of ULF field (G) in the frequency range 0.01-0.1 Hz. Then we prove the reliability of the effect by computed correlation between G (or 1/G) and especially calculated seismic indexes Ks for the rather long period of observation from June 2000 to November 2001. Our recent data confirm the validity of the effect. We show here a similar result during a period of frequent strong seismic activity in April-May 2002. It is highly probable that the effect observed is connected with the increase in plasma density perturbations inside the ionosphere, which are induced by preseismic water and gas release at the ground surface and following energy transportation into the ionosphere by atmospheric gravity waves. Two models are discussed and computed: the first is a decrease of penetration coefficient of Alfven waves from the magnetosphere due to a turbulent increase in effective Pedersen conductivity in the ionosphere, and the second is a change in wave number (k) distribution of source ionospheric turbulence. One of the mechanisms or both could be responsible for the observed 2-3 times suppression of ULF magnetic field noise at the ground.en
dc.format.extent1238363 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.publisher.nameINGVen
dc.relation.ispartofAnnals of Geophysicsen
dc.relation.ispartofseries1/47 (2004)en
dc.subjectUltra-Low Frequency emissionen
dc.subjectseismicityen
dc.subjectAlfven wavesen
dc.titlePreseismic ULF effectand possible interpretationen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.subject.INGV04. Solid Earth::04.02. Exploration geophysics::04.02.04. Magnetic and electrical methodsen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorMolchanov, O. A.en
dc.contributor.authorYu. Schekotov, A.en
dc.contributor.authorFedorov, E.en
dc.contributor.authorBelyaev, G. G.en
dc.contributor.authorSolovieva, M. S.en
dc.contributor.authorHayakawa, M.en
dc.contributor.departmentSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.departmentSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.departmentSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.departmentInstitute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation (IZMIRAN), Russian Academy of Science, Troitsk (Moscow Region), Russiaen
dc.contributor.departmentSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russiaen
dc.contributor.departmentThe University of Electro-Communications, Chofugaoka, Chofu, Tokyo, Japanen
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.deptSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia-
crisitem.author.deptInstitute of Earth Physics, Moscow, Russia-
crisitem.author.deptInstitute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation (IZMIRAN), Russian Academy of Science, Troitsk (Moscow Region), Russia-
crisitem.author.deptSchmidt United Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia-
crisitem.author.deptDepartment of Electronic Engineering, The University of Electro-Communications, Chofu, Tokyo, Japan-
crisitem.classification.parent04. Solid Earth-
Appears in Collections:Annals of Geophysics
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