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 and the Duero Basin
having 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 the response to (1) the geometry of the Moho discontinuity, (2) an imbricated crustal architecture, and/or (3) the rheological properties of
the lithosphere. Shedding some light on these features is the main
target 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 Central Iberian Massif Deformation (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 (>120∘ 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 relatively
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 time. 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 and 18 s, and probably
related to the Hales discontinuity.