Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/617
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dc.contributor.authorallCammarano, F.; Berkeley Seismological Laboratory, University of California Berkeley, CA, USen
dc.contributor.authorallRomanowicz, B.; Berkeley Seismological Laboratory, University of California Berkeley, CA, USen
dc.contributor.authorallStixrude, L.; Department of Geological Sciences, University of Michigan, MI, USen
dc.contributor.authorallLithgow-Bertelloni, C.; Department of Geological Sciences, University of Michigan, MI, USen
dc.date.accessioned2006-01-18T19:25:38Zen
dc.date.available2006-01-18T19:25:38Zen
dc.date.issued2005-12-06en
dc.identifier.urihttp://hdl.handle.net/2122/617en
dc.description.abstractB: Unraveling the physical state of the upper mantle, including the transition zone, is one of the key factors for understanding the Earth's mantle dynamics. Knowledge of mantle temperature and composition is mainly based on the interpretation of seismological observations based on insights from mineral physics. Despite the progress made to image the 3-D seismic structure of the upper mantle, its interpretation in terms of physical parameters is still challenging and it requires a truly interdisciplinary approach. Due to the better knowledge of the elastic and anelastic properties of mantle minerals at high temperatures and pressures, such an approach is now becoming feasible. We propose a new waveform inversion procedure, based on a formalism previously developed at Berkeley for global elastic and anelastic tomography, and using our existing collection of long-period fundamental and higher mode surface waveforms. Here, we incorporate mineral physics data at an early stage of the process to directly map lateral variations in temperature and composition, using recent estimates of the temperature and composition derivatives of seismic velocities (∂lnV/∂lnT,C). Anelasticity introduces a non-linear dependence of the seismic velocities with temperature throughout the upper mantle, and phase-transitions confer a non-linear character to the compositional derivatives as well, therefore the kernels should be re-computed after each iteration of the inversion. We discuss ways to address the non-linearities, as well as uncertainties in the partial derivatives. In addition to constraining the lateral variations in temperature or composition, the models can have implications on the average structure of the upper mantle. The most-common accepted physical 1-D structure had problems to satisfactorily fit seismic travel time data, requiring a slower TZ to improve the fit. However, these data do not have sufficient coverage (and resolution) in the TZ. A complementary outcome of our models will be to shed light on whether the seismic data require a modification of the physical structure in the transition zone and if the three-dimensional heterogeneity introduces a significant shift of the average physical structure away from adiabatic pyrolite.en
dc.format.extent5932792 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.publisher.nameAGUen
dc.relation.ispartofAGU 2005en
dc.subjectmantle temperaturesen
dc.subjectseismologyen
dc.titleTowards Inverting Seismic Waveform Data for Temperature and Composition in the Earth's Upper Mantleen
dc.typePoster sessionen
dc.description.statusPublisheden
dc.identifier.URLhttp://seismo.berkeley.edu/~fabioen
dc.subject.INGV04. Solid Earth::04.01. Earth Interior::04.01.01. Composition and stateen
dc.description.ConferenceLocationSan Franciscoen
dc.description.fulltextopenen
dc.contributor.authorCammarano, F.en
dc.contributor.authorRomanowicz, B.en
dc.contributor.authorStixrude, L.en
dc.contributor.authorLithgow-Bertelloni, C.en
dc.contributor.departmentBerkeley Seismological Laboratory, University of California Berkeley, CA, USen
dc.contributor.departmentBerkeley Seismological Laboratory, University of California Berkeley, CA, USen
dc.contributor.departmentDepartment of Geological Sciences, University of Michigan, MI, USen
dc.contributor.departmentDepartment of Geological Sciences, University of Michigan, MI, USen
item.openairetypePoster session-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDepartment of Geoscience, Università Roma Tre, Rome, Italy-
crisitem.author.deptSeismological Laboratory, University of California, Berkeley-
crisitem.author.deptDepartment of Geological Sciences, University of Michigan, MI, US-
crisitem.author.deptDepartment of Geological Sciences, University of Michigan, MI, US-
crisitem.author.orcid0000-0003-3475-9448-
crisitem.classification.parent04. Solid Earth-
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