Abstract:The intraplate deformation of Iberia during the Cenozoic produced a series of ranges and deformation belts with a wide variety of structural trends. The Spanish‐Portuguese Central System is the most prominent feature crossing over the whole of central Iberia. It is a large thick‐skinned crustal pop‐up with NE‐SW to E‐W thrusts. However, the 500‐km‐long left‐lateral strike‐slip Messejana‐Plasencia fault, also NE‐SW oriented, bends these thrusts to produce NE‐SW local paleostresses close to the fault, which seem… Show more
“…The differences below the CS affect the depth as well as the geometry of the crust-mantle interface. The Moho discontinuity in Diaz et al (2016) presents a rather flat geometry, depicting a little 1 km thick root. The results from gravity inversion, while being closer to our results regarding crustal thickness, are highly influenced by the inclusion of the topography in the inversion procedure.…”
Section: Lower Crustmentioning
confidence: 99%
“…The granites of the western sector correspond to the Avila Batholith, which is a vast association of igneous rocks. The current knowledge of the crustal and lithospheric structure of the Central System comes mainly from geophysical studies such as seismic data (Suriñach and Vegas, 1988;Diaz et al, 2016) and inversion and forward modelling of potential-field data (Tejero et al, 1996;de Vicente et al, 2007;Torne et al, 2015). These studies have found a crustal thickness in the range of 31 to 35 km, showing a thickening underneath the Central System with respect to the surrounding basins.…”
Section: Geological Settingmentioning
confidence: 99%
“…In any case, the structure of the CS suggested by the present dataset is that of an asymmetric orogen. Figure 6 shows a sketch of the interpretation of the CIMDEF GloPSI profile overlapped with the Moho geometry deduced from gravity inversion (Torne et al, 2015) and a compilation of active-source and RF Moho depths (Diaz et al, 2016). Also, the geometry of the inferred imbrication, involving just the lower crust (Fig.…”
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.
“…The differences below the CS affect the depth as well as the geometry of the crust-mantle interface. The Moho discontinuity in Diaz et al (2016) presents a rather flat geometry, depicting a little 1 km thick root. The results from gravity inversion, while being closer to our results regarding crustal thickness, are highly influenced by the inclusion of the topography in the inversion procedure.…”
Section: Lower Crustmentioning
confidence: 99%
“…The granites of the western sector correspond to the Avila Batholith, which is a vast association of igneous rocks. The current knowledge of the crustal and lithospheric structure of the Central System comes mainly from geophysical studies such as seismic data (Suriñach and Vegas, 1988;Diaz et al, 2016) and inversion and forward modelling of potential-field data (Tejero et al, 1996;de Vicente et al, 2007;Torne et al, 2015). These studies have found a crustal thickness in the range of 31 to 35 km, showing a thickening underneath the Central System with respect to the surrounding basins.…”
Section: Geological Settingmentioning
confidence: 99%
“…In any case, the structure of the CS suggested by the present dataset is that of an asymmetric orogen. Figure 6 shows a sketch of the interpretation of the CIMDEF GloPSI profile overlapped with the Moho geometry deduced from gravity inversion (Torne et al, 2015) and a compilation of active-source and RF Moho depths (Diaz et al, 2016). Also, the geometry of the inferred imbrication, involving just the lower crust (Fig.…”
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.
“…Whether these thrust flats reactivate or cut a previous extensional detachment is uncertain (no clear synextensional growth geometries can be identified in their hanging walls and this prevents the characterization of extensional fault geometries at depth; Figure 13a). They outline an imbricate thrust system soled by a décollement in the shallow basement (Figure 8a, basement-involved thin-skinned tectonics, Pfiffner, 2006) that resembles the structural style in the eastern Central System, to the west of the study area (Figure 2;De Vicente et al, 2018). Thickness variations in relation to the Sierra de Arcos thrust (named as Sierra de Arcos Fault in Figure 13a) are in agreement with its role as the northern boundary of the Oliete subbasin (Casas et al, 1997;Soria, 1997) that (i) thinned progressively toward the east (cf.…”
Section: Distribution Of Basement-involved and Cover-detached Structumentioning
Contractional deformation in the transition between the Iberian and Catalan Coastal Ranges (Linking Zone) generated both thin‐skinned structures detached in low‐strength Triassic units and basement‐involved structures. To evaluate their extent and relative contribution to the overall structure, we carried out a study combining structural geology and gravimetry. New gravity data (938 stations) and density determinations (827 samples) were acquired and combined with previous existing databases to obtain Bouguer anomaly and residual Bouguer anomaly maps of the study area. Seven serial and balanced cross sections were built, their depth geometries being constrained through the 2.5‐D gravity modeling and the 3‐D gravity inversion that we accomplished. The residual Bouguer anomaly map shows a good correlation between basement antiforms and gravity highs whereas negative anomalies mostly correspond to (i) Meso‐Cenozoic synclines and (ii) Neogene‐Quaternary basins. Cross sections depict a southern, thick‐skinned domain where extensional, basement faults inherited from Late Jurassic‐Early Cretaceous times were inverted during the Cenozoic. To the north, we interpret the existence of both Triassic‐detached and basement‐involved deformation domains. The two deformation styles are vertically overlapped in the southernmost part of the Catalan Coastal Ranges but relay both across and along strike in the Eastern Iberian Range. These basement and cover relationships and their along‐strike variations are analyzed in terms of the interplay between structural inheritance, its obliquity to the shortening direction, and the continuity and effectiveness of Triassic décollements in the study area.
“…occupy intra-plate positions. Both are the result of plate tectonics in the Mediterranean domain as well as of distributed strain upon Africa-Europe convergence (Dewey et al, 1989;Jolivet et al, 2008;de Vicente et al, 2018).…”
Abstract. Dividing a crystalline basement into tectonostratigraphic units, along with the recognition of the nature of their boundaries (primary vs. tectonic), are essential steps to identify major tectonic slices involved in orogeny. The Neoproterozoic and Paleozoic rocks of the Mérida Massif (SW Iberia) have been grouped into five tectonostratigraphic units according to their structural position, continental or oceanic crust affinity, and equivalent tectonometamorphic evolution. Each unit is separated from the rest ones by either crustal-scale thrusts and/or extensional detachments. The lowermost unit (Magdalena Gneisses; lower plate) has continental crust affinity, and rest below a variably strained and metamorphosed mafic-ultramafic ensemble, referred to as the Mérida Ophiolite (suture zone). The Neoproterozoic Montemolín Formation of the Serie Negra Group constitutes a unit with continental crust affinity (Upper Schist-Metagranitoid Unit; upper plate) located on top of the Mérida Ophiolite. A carbonate-rich succession (Carija Unit) occupies the uppermost structural position. Structural and isotopic data suggest that the suture zone depicted by the Mérida Ophiolite and the tectonic piling and main foliation of the Neoproterozoic and Cambrian units were formed during the Cadomian Orogeny. Superimposed shortening during the late Paleozoic formed a train of upright to NE-verging folds and thrusts that affected the Cadomian suture zone and juxtaposed it onto Ordovician strata (fifth tectonostratigraphic unit) during the Variscan Orogeny. Cenozoic contraction during the Alpine Orogeny formed SW-directed thrusts in an intraplate setting. The Mérida Ophiolite represents a new Cadomian suture zone exposure of the Iberian Massif, but its root zone is yet to be identified. This suture zone exposure seems to share a far-travelled nature with other Cadomian and Variscan suture zone exposures in Iberia, making the latter a piece of continental lithosphere built at the expense of allochthonous terranes transferred inland from peri-Gondwana onto mainland Gondwana, both during the Neoproterozoic-Cambrian and the Devonian-Carboniferous.
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