Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/4078
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dc.contributor.authorallFlorindo, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallDe Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPiersanti, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallBoschi, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione AC, Roma, Italiaen
dc.date.accessioned2008-09-24T07:24:39Zen
dc.date.available2008-09-24T07:24:39Zen
dc.date.issued2005-03-22en
dc.identifier.urihttp://hdl.handle.net/2122/4078en
dc.description.abstractThe magnetic field observed at the Earth’s surface is not a stationary feature. It is characterized by time variations ranging from milliseconds (micropulsations) to millions of years (the time interval between field reversals). Time variations with periods of a year or longer are related to Earth’s outer core sources, whereas for shorter timescales an external origin is invoked (i.e., solar activity). One of the most interesting time variations of the geomagnetic field is represented by the “geomagnetic jerk.” It is idealized as a rapid change in the slope of the secular variation, defined as the first derivative of the geomagnetic field. This means that the secular variation roughly appears as a series of straightline segments separated by geomagnetic jerks.en
dc.language.isoEnglishen
dc.publisher.nameAGUen
dc.relation.ispartofEos Trans. AGUen
dc.relation.ispartofseries12 / 86 (2005)en
dc.subjectSumatra Earthquakeen
dc.subjectGeomagnetic Jerken
dc.titleCould the Mw = 9.3 Sumatra Earthquake Trigger a Geomagnetic Jerk?en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber123en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.02. Geomagnetic field variations and reversalsen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.02. Geodynamicsen
dc.relation.referencesAlexandrescu,M.,D.Gibert,G.Hulot,J.-L.Le Mouël,and G.Saracco (1996),Worldwide wavelet analysis of geomagnetic jerks, J.Geophys.Res.,101,21,975–21,994. Alfonsi, L.,A. Piersanti, and G. Spada (1997), Did the 1977 Sumba earthquake excite the Chandler wobble?, Earth Planet. Sci. Lett.,153, 287–292. Bellanger, E., J.-L. Le Mouël, M.Mandea,and S. Labrosse (2001), Chandler wobble and geomagnetic jerks,Phys. Earth Planet. Inter.,124, 95–103. Bloxam, J., S.Zatman, and M.Dumberry (2002),The origin of geomagnetic jerks, Nature,420, 65–68. Chao,B. F. (2005), Did the 26 December 2004 Sumatra, Indonesia, earthquake disrupt the Earth’s rotation as the mass media have said?, Eos Trans.AGU, 86(1), 1–2. Gibert,D.,M.Holschneider, and J.-L. Le Mouël (1998), Wavelet analysis of the Chandler wobble, J.Geophys. Res.,103, 27,069–27,089. Gross, R. S. (2000),The excitation of the Chandler wobble,Geophys. Res. Lett.,27, 2329–2332. Gross, R. S., and B. F.Chao, (1985), Excitation study of the LAGEOS-derived Chandler wobble, J.Geophys. Res.,90, 9369–9380. Malin, S. R. C., and B. M.Hodder (1982),Was the 1970 geomagnetic jerk of internal or external origin?, Nature,296, 726–728. Mandea,M., E. Bellanger, and J.-L. Le Mouël (2000), A geomagnetic jerk for the end of the 20th century?, Earth Planet. Sci. Lett.,183, 369–373. Sabadini, R.,A. Piersanti, and G. Spada (1995), Toroidal/poloidal partitioning of global postseismic deformation,Geophys. Res. Lett.,22, 985–988. Waddington, R.,D.Gubbins, and N.Baber (1995), Geomagnetic field analysis: 5. Determining steady core-surface flows directly from geomagnetic observations,Geophys. J. Int.,122, 326–350.en
dc.description.obiettivoSpecifico3.3. Geodinamica e struttura dell'interno della Terraen
dc.description.obiettivoSpecifico3.4. Geomagnetismoen
dc.description.journalTypeN/A or not JCRen
dc.description.fulltextreserveden
dc.contributor.authorFlorindo, F.en
dc.contributor.authorDe Michelis, P.en
dc.contributor.authorPiersanti, A.en
dc.contributor.authorBoschi, E.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
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione AC, Roma, Italiaen
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 AC, 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 Roma1, Roma, Italia-
crisitem.author.orcid0000-0002-6058-9748-
crisitem.author.orcid0000-0002-2708-0739-
crisitem.author.orcid0000-0002-1814-5721-
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.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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