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IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />

(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />

Interior<br />

JSS011 Oral Presentation 2113<br />

Temperature and composition of the upper mantle as inferred from long<br />

period seismic waveforms<br />

Dr. Fabio Cammarano<br />

Earth and Planetary Science UC Berkeley <strong>IASPEI</strong><br />

Using long period seismic waveforms and a novel inversion approach which includes constraints from<br />

mineral physics, we find that lateral variations of temperature can explain a large part of the data in the<br />

upper mantle. The additional compositional signature of cratons emerges in the global model as well.<br />

Above 300 km, we obtain seismic geotherms that span the range of expected temperatures in various<br />

tectonic regions. Below 300 km, average velocities and gradients with depth are well constrained by the<br />

long period data used, except near the mantle discontinuities. We find that seismic data globally require<br />

a slower transition zone and an overall faster shallow upper mantle than reference pyrolitic models.<br />

Despite the large uncertainties in mineral physics data, the observations are not compatible with a<br />

thermal interpretation assuming dry pyrolite. A gradual enrichment in a garnet-rich component<br />

throughout the upper mantle may help reconcile the observed discrepancies. A hydrated transition<br />

would help to lower the transition zone shear velocities, as required, but the high velocities and<br />

gradients we found above the wadsleyite stability field are not consistent with this hypothesis. Exploiting<br />

the different ways in which thermal and compositional variations affect the phase and amplitude of<br />

seismic waveforms, we are now proceeding to include in our inversion the amplitude effects and invert<br />

simultaneously for temperature and composition.<br />

Keywords: mantle, seismology, mineral physics

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