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P. Schmoldt, PhD - MTNet - DIAS

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10. Data inversion<br />

owing to availability of a state-of-the-art algorithm and high-end computational facilities,<br />

an extensive 3D inversion study was conducted to enhance information about the Tajo<br />

Basin mantle region. The most striking feature therein is the low resistivity region in the<br />

lithospheric-mantle below the centre of the PICASSO Phase I profile, coinciding with a<br />

low velocity region determined in seismic tomography studies by Hoernle et al. [1995],<br />

Bijwaard et al. [1998], Villaseñor et al. [2003], and Amaru [2007]. Low resistivity – low<br />

velocity regions at mantle depth are indicative of increased temperatures, interconnected<br />

partial melt or hydrous phases [e.g. Goes et al., 2000; Nover, 2005; Yoshino, 2010, and<br />

reference therein]. In consideration of the reported extensive HIMU-like 7 reservoir beneath<br />

central and western Europe [Cebriá and Wilson, 1995; Hoernle et al., 1995], partial<br />

melt was concluded as most likely source for the lithospheric-mantle anomaly beneath<br />

the Tajo Basin. An enhancement of the feature’s anomalous seismic velocity and electric<br />

conductivity properties by a hydrous phase is possible, with dehydration processes of<br />

the subducting slab beneath Alboran Domain and Betic Cordillera identified as potential<br />

source for the hydrous phase.<br />

Exceptionally low electric resistivity of the region associated with the lithosphericmantle<br />

beneath the Tajo Basin in the 3D inversion, hence the less distinct contrast in resistivity<br />

between lithosphere and asthenosphere, aggravates estimation of the LAB depth<br />

and its characteristics. Based on forward modelling results it can be concluded that a<br />

conductive uppermost asthenosphere anomaly as well as a uniformly conductive asthenosphere<br />

in the order of 20 Ωm, observed in long-period EM induction studies of other<br />

regions (cf. Sec. 5.2.2), are unlikely for the Tajo Basin subsurface. However, due to the<br />

low signal-to-noise ration of, in particular, long-period data, asthenospheric properties are<br />

not strongly constrained by PICASSO Phase I results.<br />

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