Lithospheric image of the Central Iberian Zone (Iberian Massif) using Global-Phase Seismic Interferometry

Author:

Andrés JuvenalORCID,Draganov DeyanORCID,Schimmel MartinORCID,Ayarza PuyORCID,Palomeras ImmaORCID,Ruiz MarioORCID,Carbonell RamonORCID

Abstract

Abstract. The Spanish Central System is an intraplate mountain range that divides the Iberian Inner Plateau in two sectors – the northern Duero Basin and the Tajo Basin to the south. The topography of the area is highly variable with the Tajo Basin having an average altitude of 450–500 m while the Duero Basin presents a higher average altitude of 750–800 m. The Spanish Central System is characterized by a thick-skin pop-up and pop-down configuration formed by the reactivation of Variscan structures during the Alpine Orogeny. The high topography is, most probably, the response of a tectonically thickened crust that should be also identified by 1) the geometry of the Moho discontinuity 2) an imbricated crustal architecture and/or 3) the rheological properties of the lithosphere. Shedding some light about these features are the main targets of the current investigation. In this work, we present the lithospheric-scale model across this part of the Iberian Massif. We have used data from the CIMDEF project, which consists of recordings of an almost-linear array of 69 short-period seismic stations, which define a 320 km long transect. We have applied the so-called Global-Phase Seismic Interferometry. The technique uses continuous recordings of global-earthquakes (> 120º epicentral distance) to extract global phases and their reverberations within the lithosphere. The processing provides an approximation of the zero-offset reflection response of a single station to a vertical source, sending (near) vertical seismic energy. Results indeed reveal a clear thickening of the crust below the Central System resulting, most probably, from an imbrication of the lower crust. Accordingly, the crust-mantle boundary is mapped as a relative flat interface at approximately 10 s two-way travel time except in the Central System, where this feature deepens towards the NW reaching more than 12 s. The boundary between the upper and lower crust is well defined and is found at 5 s two-way travel. The upper crust has a very distinctive signature depending on the region. Reflectivity at upper-mantle depths is scattered throughout the profile, located between 13–18 s, and probably related with the Hales discontinuity.

Funder

Generalitat de Catalunya

Publisher

Copernicus GmbH

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