TS6.1 | Dynamics and structural evolution of fold-and-thrust belts and accretionary prisms: an interdisciplinary approach
EDI
Dynamics and structural evolution of fold-and-thrust belts and accretionary prisms: an interdisciplinary approach
Convener: Esther Izquierdo Llavall | Co-conveners: Jonas B. Ruh, Sandra Borderie, Olivier Lacombe, Christoph von Hagke
Orals
| Tue, 25 Apr, 14:00–18:00 (CEST)
 
Room K1
Posters on site
| Attendance Wed, 26 Apr, 10:45–12:30 (CEST)
 
Hall X2
Orals |
Tue, 14:00
Wed, 10:45
Fold-and-thrust belts and accretionary prisms are key geological features occurring all around the globe. They mostly develop along convergent plate boundaries although they may also form along passive margins or other super-critical slopes by a gravitationally driven stress field. Fold-and-thrust belts can display a varied range of scales, may involve the whole continental lithosphere or just the uppermost sedimentary cover and can differ in their spatial extent, longevity of their formation and the rock types involved. Their geometry and kinematic evolution strongly depend on an ample variety of parameters (rheology, temperature, surface processes, structural inheritance, mechanical stratigraphy…), the understanding of their effects being fundamental for the comparison of different fold-and-thrust belts and the development of common predictive models.
Fold-and-thrust belts have been intensely investigated, aiming to decipher their short- and long-term evolution. However, there are important questions that remain not fully understood: i) What is the effect of structural inheritance, décollements, syn-tectonic sedimentation and the interplay between them on mountain building processes? ii) How are transient and long-term rheological/mechanical characteristics and processes affecting the evolution of fold-and-thrust belts? iii) How can we better define deep orogenic geometries and better reconstruct the burial, thermal and kinematic evolution of orogens?
The here proposed session tackles these questions by considering a multidisciplinary approach. We look forward to receiving abstracts focusing on the short- and long-term dynamics and the geometry and structural evolution of fold-and-thrust belts by means of different methodological approaches, including (but not limited to) field structural geology, cross-section construction and balancing, 3D structural modelling, seismics and seismology, analogue and numerical modelling, rock mechanics, geomorphology, thermochronology and geophysics.

Orals: Tue, 25 Apr | Room K1

Chairpersons: Esther Izquierdo Llavall, Christoph von Hagke
14:00–14:05
Deformation mechanisms and strain distribution in folded and faulted rocks
14:05–14:15
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EGU23-12156
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On-site presentation
Inga Boianju, Carly Faber, and Christie Rowe

Fold and thrust belts are frequent structures that form under a compressive regime. They record a variety of deformation that guides earthquake ruptures and controls seismic hazard. The Naukluft mountains of Namibia with their extraordinary exposure, present a unique opportunity to study carbonate fault rocks. Through linked field investigations and microstructural analysis, we aim to map how changes in fault strength contributed to larger scale architectural evolution of a fold and thrust belt. Mineralogical assemblage of the stacked nappes show units of carbonate and shale in the lower to upper greenschist facies, correlating to the seismological depth for carbonate rocks. Cross cutting relations prove that the Naukluft Nappe Complex (NNC), previously thought to form through gravity sliding, is a foreword-propagating fold and thrust belt, stacking Neo Proterozoic sedimentary nappes on top of each other, and on top of the cambrian Nama fore-rift group. Most thrusts separating the stacked nappes are made of 20-150 meters of calc mylonites, except for the youngest two brittle thrust faults, including the basal thrust. Brittle deformation is recorded by localized brecciation and the development of discrete faults. The brittle faults follow the same orientation as the overall transport direction of the nappe complex. Ductile shearing is facilitated by crystal plastic deformation, leading to grain size reduction, and grain boundary sliding. Both ductile mylonite units and the younger brittle faults are also overprinted by later brittle faults, and between the ductile and brittle behavior, we map a unit of a block-in-matrix. We found no clear correlation between the temporal evolution of the nappe complex and the thickness of ductile shear zones. We show evidence for embrittlement through exhumation of a carbonate terrane, and suggest that it may be important to consider the effects of deeper ductile behavior in “Coulomb wedge” descriptions of thin-skinned thrust belts.

How to cite: Boianju, I., Faber, C., and Rowe, C.: Deformation in carbonates and its contribution to fold & thrust belt architecture, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-12156, https://doi.org/10.5194/egusphere-egu23-12156, 2023.

14:15–14:25
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EGU23-14083
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ECS
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On-site presentation
Piotr Strzelecki and Anna Świerczewska

Deformation in sandstones often takes the form of tabular strain localization structures known as deformation bands. To date, only a few localities have been documented with naturally occurring deformation bands that primarily localize compactant failure i.e. pure compaction bands (PCBs).

The PCBs are found in the Oligocene flysch sequence of the (Lower) Krosno beds within the Otryt sandstones of the Silesian Nappe, the Outer Carpathians (SE Poland). The PCBs are perpendicular to the bedding planes and occur within the folded strata. The PCBs were formed in very fine-grained to very coarse-grained sandstones of moderate or poor sorting. The spacing of PCBs is on average 7 mm and the average thickness of a band is 0.7 mm. The PCBs’ microstructures originated due to a range of mechanisms which include pore collapse resulting in compact grain packing and disaggregation, including kinking and cataclasis. The type of resultant microstructure shows a strong relationship with the textural parameters of the host rock. The frequency of cataclasis increases with grain size, whereas kinking is related to the moderate sorting of the host rock. The structural restoration of beds to the primary horizontal position indicates that the PCBs formed prior to the folding and recorded the SW-NE directed shortening which is consistent with the subsequent folding. The results of the mechanical modelling and stratigraphic constraints suggest that the PCBs formed under shallow burial depths <1 km.

The occurrence of hydrocarbons and calcite veins within some fractured PCBs shows that the PCBs might have played an important role in fluid transport during the subsequent evolution of the fold-and-thrust belt of the Outer Carpathians.

Acknowledgements: This research was funded by National Science Centre, Poland (grant number: 2018/31/N/ST10/02486).

How to cite: Strzelecki, P. and Świerczewska, A.: Pure compaction bands in the naturally deformed flysch sandstones of the Silesian Nappe (SE Poland): early markers of tectonic shortening, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-14083, https://doi.org/10.5194/egusphere-egu23-14083, 2023.

14:25–14:35
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EGU23-13457
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On-site presentation
Saskia Köhler, Daniel Koehn, Harald Stollhofen, Hamed Fazlikhani, Tobias Stephan, and Florian Duschl

We investigated Mesozoic sequences of the Franconian Platform (SE Germany) according to their deformation history. Based on field observations we performed fault-slip and stylolite stress inversion. We could distinguish two stress cycles in an intraplate compressional setting starting with (i) normal faulting, (ii) thrusting and the development of folds and tectonic stylolites (iii) and strike-slip regimes. The first cycle is caused by the Europe-Iberia-Africa collision in the Cretaceous, while the second cycle is induced by the Cenozoic Alpine orogeny. We can zoom into the transition between the thrusting and strike-slip regime of the first cycle by the preservation of a stress field with none principal stress being in the vertical axis. The combination of field and microscopic observations shows a rather complex chronology of this relatively short time span with alternating sedimentary and tectonic stylolites.

With our work we contribute to the understanding of stress development in intraplate compressional settings.

How to cite: Köhler, S., Koehn, D., Stollhofen, H., Fazlikhani, H., Stephan, T., and Duschl, F.: Zooming into the transition between thrusting and strike-slip in an intra-continental compressional setting, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-13457, https://doi.org/10.5194/egusphere-egu23-13457, 2023.

14:35–14:45
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EGU23-13527
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ECS
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On-site presentation
Phoebe Sleath, Rob Butler, and Clare Bond

In most idealised models of thrust fault formation thrusts form along a weaker basal detachment and then propagate upwards through strata, producing a hang-wall anticline and developing in a piggy-back sequence. This idealised thrust fault geometry commonly fails to match actual outcrop structures. Conversely, in a stiff layer thrusting model, the thrust originates and localises in mechanically competent beams as ramps and the thrust tip propagates both up and down slowly to create a linked fault system. This model has had few tests at outcrop level and the lack of field examples has hindered adoption of this model. 

In the UK, thrust structures in the Old Red Sandstone are ideal test outcrops as they contain a multilayer stratigraphy of competent sandstone beds encased in cleaved mudrocks. Field and photogrammetric mapping has been applied to the St Brides Haven outcrop on the west coast of Pembrokeshire in SW Wales, the 10m high outcrop exposes an open fold pair cut by thrusts typical of Variscan deformation. The outcrop has an abrupt rheological change within the multilayer with a 1m thick sandstone bed within mudstones. Thrust faults are confined to the strong sandstone beam, with a fault spacing along the competent beam, with cleavage development in the mudstone above and below. The structural style is controlled by variations in the multi-layer rheology, and fault localisation in the competent sandstone beams appears to be balanced by distributed deformation in the form of cleavage development in the mudstones. The outcrop matches key features of the stiff layer thrusting model.

Observations from this outcrop show that the observed thrust fault geometry evolved from soft to hard linked across the multilayer. Drag faults have developed in both the hanging and footwalls, showing thrusts initiate in the stiff layers. Cleavage developed in the mudstones and along rheological boundaries the cleavage and thrust trajectories connect. The outcrop matches key features of the stiff layer thrusting model. This work contributes to a series of studies on fold-thrust outcrops to expand the range of widely used models and avoid bias in interpretation of fold-thrust belts when basing work on theoretical models.

How to cite: Sleath, P., Butler, R., and Bond, C.: Strata-dependent thrust localisation in multilayers, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-13527, https://doi.org/10.5194/egusphere-egu23-13527, 2023.

14:45–14:55
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EGU23-9905
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Highlight
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On-site presentation
Clare Bond, Francisca Robledo, and Robert Butler

The Jura, on the outer margin of the NW Alps, is classically interpreted as a “thin-skinned” fold-thrust belt, detached along Triassic evaporites. It includes the Opalinus Clay (Toarcian-Aalenian), the designated host formation for a radioactive waste repository in Switzerland. We develop a case study to illustrate how methods and approaches in cross-section balancing and restoration, based on seismic imagery, can be applied to assess risks and uncertainties for the integrity of the Opalinus Clay. We focus on the Nördlich Lägern area, announced in 2022 as the preferred site for nuclear waste disposal in Switzerland.  Between northern and southern fold-thrust structures, 3D seismic mapping defines a largely unfaulted domain within which there is no seismic indication of deformation in the Opalinus Clay. It is however seismically transparent. Bounded to the north and south by domains of strongly-faulted Mesozoic strata the low-strain zone has been translated tectonically and is underlain by a seismically resolved Permo-Carboniferous basin.

 

Here we consider multiple interpretations of key section lines with varying degrees of structural linkage and several conceptual models for the timing of the contractional deformation structures. By exploring multiple interpretations, we consider the key uncertainties in structural understanding and risks that might compromise the structural integrity of the waste repository site. Key questions include: were the thin-skinned thrust structures influenced by deep basement structures (that might reactivate in the future)? Has the Opalinus acted as an intraformational detachment that connects kinematically the northern and southern fold-thrust structures? Section balancing and restoration are used to assess whether strain in the two deformation domains can be matched on both sides of the Opalinus Clay. If not, then there is an increased risk of the Opalinus having acted as a detachment passing through the low strain domain, the candidate repository site. A combination of line-length and formation area balancing have been applied to the adjacent, upper and lower, units to the Opalinus Clay, evoking different interpretations of fault trajectories in the bounding fold-thrust domains. In all these interpretations, a balance in tectonic contraction can be achieved without involving distributed strain or requiring detachment within the Opalinus. On this basis, the structural integrity of the prospective repository site is not compromised; an inference consistent with borehole evidence. No significant layer-parallel fault zones have been identified in the four borehole penetrations in the Nördlich Lägern area. 

The work highlights the importance of structural interpretation and restoration techniques in assessing risks for energy and waste storage projects in contractional settings, even when searching for low strain zones.

How to cite: Bond, C., Robledo, F., and Butler, R.: The Jura Fold-Thrust Belt, Switzerland – a contractional deformation setting for nuclear waste disposal, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-9905, https://doi.org/10.5194/egusphere-egu23-9905, 2023.

Interaction between tectonics and sedimentation
14:55–15:05
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EGU23-2766
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On-site presentation
Nicolas Pinet, Mathieu J. Duchesne, and Virginia Brake

The Beaufort-Mackenzie fold and thrust belt in Arctic Canada corresponds to the offshore part of the Cordilleran orogen in Yukon and Alaska. The main folds are associated with thrusts that root in a basal décollement at depths of ca. 12-15 km. Deformation mainly occurred prior to the deposition of the Richards sequence (late Eocene) and subsequent folding that progressed basinward and continued episodically to the present accounts for < 10% of the total shortening. In the shelf region, normal faults dipping either seaward or landward are located on the apex of anticlines. Detailed analysis on seismic sections of the variations of throw (T) and expansion index (Ei) with depth (z) indicates that despite the clear spatial relationship with anticlines, normal faults initiated after fold development. Normal faulting migrated seaward during the Oligocene to Pliocene (and possibly later) along with the shelf edge that resulted from the progradation of thick sedimentary wedges of clastic sediments. This strongly suggests that normal faulting is not related to tectonics (i.e., linked with the building of the Cordillera), but to gravity spreading due to high sedimentary loading in the Mackenzie delta; i.e. main depocenter for sediments originating from the northeastern Cordillera since the latest Cretaceous. The superimposition of extensional structures on an existing fold and thrust belt shows the complex interplay in time and space between far-field stresses linked with plate-dynamics and stresses associated with sedimentary loading in a delta setting.

 

How to cite: Pinet, N., Duchesne, M. J., and Brake, V.: Cenozoic tectonic evolution of the Beaufort-Mackenzie fold and thrust belt (Arctic Canada): from orogenic shortening to gravity spreading, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-2766, https://doi.org/10.5194/egusphere-egu23-2766, 2023.

15:05–15:15
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EGU23-5404
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ECS
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On-site presentation
Romain Hemelsdaël, Olivier Averbuch, Laurent Beccaletto, Alain Izart, Laure Capar, Stéphane Marc, and Raymond Michels

A new structural model is presented for the Permo-Carboniferous Lorraine Basin (NE France), a major intramountain basin that developed during the latest stages of the Variscan orogeny (ca 315–270 Ma). This basin is buried in NE France below the Paris Basin but outcrops in southern Germany (Saar-Nahe Basin). Digitalized well logs and reprocessed seismic data were used to decipher the kinematic evolution of this basin located along the Rhenohercynian orogenic suture zone. The basin initiated during the late collision stage (Late Namurian-Westphalian) in a wedge- top position upon the Saxothüringian retrowedge. The syn-orogenic sequences are delimited to the north by the major SE-directed Metz Thrust, which is part of the backthrust system that propagated during Late Westphalian times. Seismic data provide evidence of negative tectonic inversion, allowing the formation of syn-rift depocenters (Stephanian-Early Permian) above the former anticlines. Erosion of these anticlines results in a major unconformity (base of Stephanian) marking the onset of post-orogenic collapse stage. The late Early Permian shortening (Saalian phase) reactivated former thrusts and normal faults, thus generating uplift of the basin. The post- orogenic phase is complex and diachronous at basin scale, and both compression and extension can be recorded in the same area over a short period (<10 Ma). The Late Carboniferous negative tectonic inversion along the Rhenohercynian suture zone is proposed to result from the lithospheric delamination of the Variscan orogenic roots. The associated upwelling of asthenospheric material is recorded by intense magmatic activity, and can be, in turn, considered as the main trigger for the subsequent thermal subsidence of the Paris basin.

How to cite: Hemelsdaël, R., Averbuch, O., Beccaletto, L., Izart, A., Capar, L., Marc, S., and Michels, R.: A deformed wedge-top basin inverted during the collapse of the Variscan belt: the Permo-Carboniferous Lorraine Basin (NE France), EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-5404, https://doi.org/10.5194/egusphere-egu23-5404, 2023.

15:15–15:25
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EGU23-14064
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ECS
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On-site presentation
Lionel Menzer, Cédric Bonnel, Guilhem Hoareau, Charles Aubourg, and Jean-Paul Callot

Foreland fold and thrust belts (FFTB) are the locus of strong interactions between tectonics and sedimentation during both mountain building then dismantling processes. Especially, the nature and rheology of decollement layers within the basin pre and/or syn-orogenic sequence are susceptible to influence the kinematic evolution and geometry of FFTBs as well as the growth of orogenic wedges.

In the South Pyrenean Zone, the Jaca basin forms the main pro-foreland basin filled by marine to continental siliciclastic sediments during Eocene and Lower Oligocene times. From Bartonian until Rupelian at least, several alluvial fans were successively deposited from east to west along its northern margin in the footwall of emergent thrusts, where they were accompanied by the syn-sedimentary growth of shale-cored anticlines downstream.

Field surveys and “bed-to-bed” mapping of syn-orogenic formations using high-resolution DEMs were used with re-interpreted published seismic lines to build two cross-sections that highlight the structural style and evolution of the Gavarnie-Jaca FFTB. This illustrates the tectono-sedimentary evolution of a transitional, shallow-marine to alluvial foreland margin.

The Eocene-Oligocene syn-orogenic deposits are folded as a wide synclinorium that is thrusted southward over the Ebro foreland along to the Triassic detachment level. In the northern limb, the late Eocene Orosia-Cancias conglomerates exhibit a short-wavelength and small-scale fold detached within the late Middle Eocene shallow marine marls. Beneath this decoupling level, the Lower and Middle Eocene turbidites form a gently foreland ward-dipping imbricate composed of several small-scales thrust-sheets detached at the base of Upper Cretaceous. During end-Bartonian and early Priabonian, the deposition of the Orosia alluvial fan was coeval with the early growth of the Basa anticline downstream. From Priabonian, the anticline was subsequently welded and forward-tilted coevally with the development of the turbidite imbricate beneath, in response to the Gavarnie thrust-sheet emplacement. At this time, the second Cancias conglomerate unit was deposited as a large fluvial fan that progressively filled the foreland basin northern margin.

The tectono-sedimentary evolution of the north-eastern Jaca foreland margin illustrate the interactions between the regional convergence, syn-orogenic shales tectonics and alluvial sedimentation within a foreland fold and thrust belt. The South Pyrenean foreland documents a first example of a gliding alluvial fan on gravity-driven mobile shales in a convergent margin setting.

How to cite: Menzer, L., Bonnel, C., Hoareau, G., Aubourg, C., and Callot, J.-P.: Role of syn-orogenic sedimentation in the evolution of a foreland fold and thrust belt: an example from the Jaca basin, South Pyrenean Zone, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-14064, https://doi.org/10.5194/egusphere-egu23-14064, 2023.

Structural style and kinematics in fold-and-thrust belts
15:25–15:35
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EGU23-6425
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ECS
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solicited
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On-site presentation
Alexandra Tamas, Dan Mircea Tamas, Bianca Copot, Ioana Silvia Mihaela Tocariu, Daria Dohan, Zsolt Schléder, and Csaba Krézsek

Fold and thrust belts are a notoriously challenging environment when it comes to providing structural models for the subsurface, and the Romanian Carpathians are no exception. Hosting the largest onshore oil fields in Romania, this is a highly mature hydrocarbon area, with most of the fields producing since the late nineteenth century.

The structural style of this fold and thrust belt is influenced by a number of parameters which includes multiple detachments (including salt), combined with multiphase tectonic event and reactivation of basement structures which adds to the complexity and variability of the structural style.

As a consequence, the reservoirs, especially the Oligocene - lower Miocene (sub-salt), thought very prolific are structurally complex, heterogeneous, and compartmentalized. It is a constant struggle for geologists to create structural maps of these reservoirs due to complex deformation, and insufficient or ambiguous geological/geophysical data. Some of the most significant issues are related to scattering dip data and the overall difficulties in correlating well logs. In some cases, even the logs of the side-track well do not correlate with the initial log.

Single-method approaches (e.g. only seismic interpretation) often lead to uncertainties or contrasting models regarding the structural style. In this study, we adopted a multiscale/multimethod approach such as forward-modeled regional cross-sections that rely on seismic reflection and well data, UAV-based digital outcrop models, fieldwork, microstructure analysis, and scaled analogue modelling.

This holistic approach enhanced our understanding of fold and thrust belts and provided better constraints on the subsurface structural style in the Romanian Carpathians, as well as explaining complexities that have hitherto been ignored. These new models can reduce subsurface uncertainties regarding structural style, and unlock the full potential of the area which will significantly enhance future exploration programs.

How to cite: Tamas, A., Tamas, D. M., Copot, B., Tocariu, I. S. M., Dohan, D., Schléder, Z., and Krézsek, C.: Challenges in the subsurface interpretation of a fold and thrust belt and how to get the best insights: examples from the Romanian Carpathians, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-6425, https://doi.org/10.5194/egusphere-egu23-6425, 2023.

15:35–15:45
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EGU23-324
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ECS
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On-site presentation
Rafael Guerra Roel, Daniel Pastor Galán, Gabriel Chávez Cabello, César Francisco Ramírez-Peña, José Jorge Aranda Gómez, Gerardo Patiño Méndez, Alejandro Rodríguez-Parra, Eduer Giovanny Nova Rodríguez, and Roberto Stanley Molina Garza

The Mexican Fold-and-Trust Belt is a winding belt that formed after a series of protracted tectonic events, which began with the onset of sedimentation in the basins formed during the break-up of Pangea and during the roll-back of the oceanic Kula plate in Jurassic times. Later, the continued subduction of Kula-Farallon constituent plates at the western margin of Mexico triggered arc formation, thrusting, basin inversion, and folding. The kinematics of the fold-and-thrust belt curvature at regional and local scales is still debated. Different hypotheses have been explored to explain the trace of the orogen: 1) curvature is mainly and primarily controlled by the basin architecture; 2) Curvature is progressive and was at least partially acquired during deformation being controlled by the basement geometry, lithologic heterogeneities, and/or the shortening direction, and 3) The curvature is, at least partially, postdating the main orogenic deformation structures being formed as the youngest of the deformation phases. Several regional-scale studies have been performed (Eguiluz et al., 2010; Fitz-Diaz et al., 2017). But most of the previous paleomagnetic studies were focused on studying the configuration of the desegregated fragments of Pangea (Molina-Garza et al., 1992). In this study, we investigate the nature of the curvature in the north and central-eastern part of the Mexican Fold and Trust Belt using paleomagnetic data obtained from the Jurassic rocks of the Nazas Formation, this formation is composed of a volcanic and volcano-sedimentary succession of andesites and dacite flows interbedded with tuff deposited in an intra-arc or back-arc setting. Our results show remagnetizations, some potential primary magnetizations, and significant counterclockwise rotations. This implies a potential oroclinal bending origin for at least part of the Mexican fold-and-thrust-belt curvature. This contribution will discuss the potential mechanisms causing the curvature and the implications for the kinematics, tectonic and geodynamic evolution of the central-western Pacific subduction during the Mesozoic-Paleogene in northeastern Mexico. This work is a posthumous contribution of Dr. Roberto Stanley Molina-Garza and a tribute to his huge contribution to the understanding of the tectonic history of Mexico.

Keywords: Paleomagnetism; Mexican Fold and Trust Belt; Anticlockwise rotation; Remagnetization; Jurassic; Nazas Arc.

How to cite: Guerra Roel, R., Pastor Galán, D., Chávez Cabello, G., Ramírez-Peña, C. F., Aranda Gómez, J. J., Patiño Méndez, G., Rodríguez-Parra, A., Nova Rodríguez, E. G., and Molina Garza, R. S.: Another bend in the orogen? Kinematics of the winding Mexican Fold-and-Trust Belt: Paleomagnetism of the Nazas arc., EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-324, https://doi.org/10.5194/egusphere-egu23-324, 2023.

Coffee break
Chairpersons: Jonas B. Ruh, Olivier Lacombe
16:15–16:25
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EGU23-1487
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ECS
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On-site presentation
Matteo Basilici, Stefano Mazzoli, Vincenzo Spina, Pietro Paolo Pierantoni, and Emanuele Tondi

Seismic interpretation, cross-section balancing and sequential restoration unravel how inherited (rifted continental margin-related) and syn-kinematic stratigraphy, structural features and rheology played different roles at various times and locations along the fold and thrust belt to produce major changes in structural style in the outer Albanides. Different processes appear to have concurred to slowdown and/or arrest detachment-dominated thrusting of the sedimentary cover during a late-stage (<5 Ma) switch from thin-skinned to thick-skinned thrusting. In the northern outer Albanides, the limited thickness of Triassic evaporites inhibited thrust belt propagation within the Ionian basin succession, favoring further advancement of the detached carbonate platform (Kruja) units in its hanging wall. The rapid accumulation of an up to 10 km thick succession of syn-tectonic strata in the Peri-Adriatic Depression likely had a twofold effect of: (i) stopping detachment-dominated thrust belt propagation into the foredeep strata; and (ii) providing a burial that substantially contributed to thermal weakening of the crust. On the other hand, in the southern outer Albanides the Ionian basin carbonate succession, here overlying thick Triassic evaporites, was intensely shortened. Folding and detachment-dominated thrusting proceeded efficiently up to the western margin of the basin. There, normal faults controlling the platform-to-basin transition and the reduced thickness of the Triassic evaporites at the base of the Sazani (Apulia) carbonate platform succession hindered thrust belt propagation into the thick shallow-water carbonate succession. The latter was later broadly folded and significantly uplifted above regional by deformation associated with the crustal thrust ramp controlling the present-day blind thrust front in this southern sector of the belt. In this region, tectonic burial – produced by the imbricated and thickened sedimentary cover – rather than sedimentary burial likely contributed to thermal weakening of the crust. 3D structural modelling effectively shows the role of major, inherited transverse structures in compartmentalizing fold and thrust belt architecture and tectonic evolution.

How to cite: Basilici, M., Mazzoli, S., Spina, V., Pierantoni, P. P., and Tondi, E.: Along-strike variations of fold and thrust belt architecture and tectonic evolution revealed by 3D structural modelling of the outer Albanides, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-1487, https://doi.org/10.5194/egusphere-egu23-1487, 2023.

16:25–16:35
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EGU23-16544
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ECS
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On-site presentation
Marco Snidero, Josep Anton Muñoz De La Fuente, Pablo Santolaria Otin, Pablo Martinez Granado, and Nikolaos Likakis

The Hellenides of Western Greece is a salt detached fold and thrust belt which resulted from the inversion of the previous southern Neo-Tethys margin. Before the Paleogene and Neogene contractional deformation, the Ionian basin was formed during the Triassic to early Jurassic rifting, bounded by the Apulian and Gabrovo platforms to the west and to the east respectively. The structural style of Western Greece is largely controlled by the presence of Triassic evaporites flooring the sedimentary succession of the Ionian basin, while previous models invoked the existence of extensional faults affecting the Triassic to Jurassic succession as one of the main structural controls. Understanding the present contractional structure mainly depends on unraveling the geometry of the Mesozoic extensional system, the distribution of the salt horizon and the presence and geometry of salt structures preceding the contractional deformation. Based on an extensive field study carried out along the Ionian fold and thrust belt, we present several regional and local balanced cross-sections and define several characteristic structural templates resulting from of this area.

Despite inversion tectonics and reactivated salt structures are common features in many salt-detached fold and thrust belts but no evidence for the presence of inherited (and inverted) Jurassic extensional faults was found. However, the deformational style was strongly controlled by significant changes in thicknesses involving the pre-contractional stratigraphic package, and suggesting the presence of pre-existing salt structures. The pre-shortening configuration was dominated by salt pillows and salt plateaus formed during the Triassic to early Jurassic rifting. As a result, we observe a significative change in the deformation style, from remarkable detachment folds, box-folds or inclined folds, to more wide and far-travelled thrust sheets formed in the areas with a thicker stratigraphy. Despite the stratigraphic thickness is reduced to few hundreds of meters in some cases,  diapirism is just related with the contractional stage, as a result of the squeezing of former salt pillows, and no evidence of precursor passive diapirs has been found.

How to cite: Snidero, M., Muñoz De La Fuente, J. A., Santolaria Otin, P., Martinez Granado, P., and Likakis, N.: Structural style variations along the Ionian fold and thrust belt, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-16544, https://doi.org/10.5194/egusphere-egu23-16544, 2023.

16:35–16:45
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EGU23-8370
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solicited
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On-site presentation
Pablo Santolaria, Pablo Granado, Josep Anton Muñoz, Oriol Ferrer, Elizabeth P. Wilson, Marco De Matteis, Marco Snidero, Oscar Gratacós, and Eduard Roca

In this work, we experimentally explore the role played by salt in contractional systems: from simple layer-cake, salt-floored settings to inverted salt-bearing rifted-margins, the inherent low-strength rheology of salt and its distribution determine particular structural styles and kinematics. Salt-detached contractional systems exhibit low taper angles, with no dominant structural vergence, and are comparatively wider in cross section than their non-salt-involved equivalents. The salt-sediment thickness controls structural spacing while the presence of pre-existing isolated salt bodies breaks the mechanical homogeneity. If salt bodies are connected through a framework of salt walls, contractional deformation concentrates in them and structural trends are no longer perpendicular to shortening but determined by the inherited orientation of salt bodies.

Finally, we assess the inversion of a salt-bearing rifted margin, where late syn-rift to early post-rift salt undergoes differential loading and gravity gliding leading to a salt-sediment architecture consisting of a salt wall-minibasin province, and a distal raft system. Upon shortening, inherited salt bodies localize contractional deformation and the salt-sediment architecture determines the structural configuration of the contractional system. In the experiments, a large-transport thrust detached along allochthonous salt accumulated in the distal raft system, and the squeezing of salt walls together with the tilting of minibasins, accounted for most of the shortening in the salt wall-minibasin province. During shortening, about 75% of the original salt evacuates and is eroded. Due to the low salt-sediment ratio found in fold-and-thrust belts, the role played by salt tectonics could be underestimated. So, the best practice approach for understanding structural style and kinematics of salt-influenced fold-and-thrust belt resides in the rifted margin stratigraphy involved, and not in the salt itself, since salt is generally poorly preserved and strongly deformed.

How to cite: Santolaria, P., Granado, P., Muñoz, J. A., Ferrer, O., Wilson, E. P., De Matteis, M., Snidero, M., Gratacós, O., and Roca, E.: Salt-influenced fold-and-thrust belts: insights from experimental analog models, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-8370, https://doi.org/10.5194/egusphere-egu23-8370, 2023.

16:45–16:55
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EGU23-16650
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On-site presentation
Gianluca Vignaroli, Manuel Curzi, Costantino Zuccari, Luca Aldega, Andrea Billi, Eugenio Carminati, Roelant Van der Lelij, Andrew Kylander-Clark, and Giulio Viola

Constraining the timing of tectonic events is of prime importance for the in-depth understanding of the complex evolution of orogenic deformation, particularly in the case of fold-and-thrust belts. In this work, we combined U-Pb dating of tectonic carbonates and K-Ar dating of fault gouges of selected key outcrops along two main thrusts of the Paleogene-Neogene Eastern Southern Alps (ESA), Italy. The ESA are the south-verging fold-and-thrust retrobelt of the Alpine orogen, offering spectacular exposures to study the details of past tectonic processes. However, despite a few published papers regarding the deformation mechanisms of a major thrust in the ESA (the Belluno Thrust), modern, multiscale structural and radiometric studies of fault zones in the ESA are missing, such that detailed reconstructions of the local and regional tectonic evolution through space and time remain only loosely constrained. We focused on the (i) Valsugana Thrust, which is a first-order thrust separating the Dolomites s.s. to the north from the Venetian Pre-Alps to the south, and (ii) the more external Belluno Thrust. We coupled U-Pb dating of tectonic carbonates and X-ray diffraction and K-Ar dating of clay minerals in fault gouges with structural analysis and microtextural characterization. We show that the Valsugana Thrust represents an inherited pre-Alpine structure that (i) registered far field deformation during the Early Cretaceous (K-Ar gouge age of 140 ± 32 Ma), (ii) strongly influenced the geometry and kinematics associated with deformation structures during the Alpine orogenesis and (iii) recorded multiple reactivations in Late Cretaceous (K-Ar age of 79.2 ± 8.4 Ma and 76.2 ± 1.4 Ma), late Miocene (U-Pb age of 9.1 ± 0.8 Ma), and Miocene-Pliocene (U-Pb age of 5.3 ± 1.6 Ma) times. Radiometric constraints from the Valsugana Thrust attest to remarkable out-of-sequence compressional movements in the inner ESA after the orogenic wave had progressed farther south to the more external Belluno Thrust, whose activity is constrained to the Oligocene by a 30.6 ± 5.8 Ma K-Ar gouge age and a 23 ± 14 Ma U-Pb syn-tectonic vein age.

How to cite: Vignaroli, G., Curzi, M., Zuccari, C., Aldega, L., Billi, A., Carminati, E., Van der Lelij, R., Kylander-Clark, A., and Viola, G.: Long-term tectonic evolution of the Eastern Southern Alps (Italy): a reappraisal from new structural and radiometric constraints, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-16650, https://doi.org/10.5194/egusphere-egu23-16650, 2023.

16:55–17:05
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EGU23-16083
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On-site presentation
Bianca Heberer, Salcher Bernhard, Dunkl István, Sachsenhofer Reinhard, Gabor Tari, Michael Wagreich, Christoph von Hagke, and Godfrid Wessely

Thermochronology has seen widespread application in the Eastern Alps. Tracking upper crustal cooling has focused mainly on the Tauern Window, the core of the collisional orogen, where exhumation has been most prominent. Further to the east, mostly fission track work is concentrated along fault zones and thermochronometers with lower closure temperatures, such as apatite (U-Th)/He dating, have hardly been applied to higher elements of the nappe pile. Due to the scarcity of the dataset and preferential application of fission track dating uppermost crustal cooling below ca. 80 °C remains undetected.

In this contribution, we present new low-T thermochronological ages from the easternmost Eastern Alps from the vicinity of the Vienna basin. We carried out apatite (U-Th)/He dating on clastic units, i.e. Gosau Group, Rhenodanubian Flysch and Lunz Formation sandstone. Additional apatite fission track analysis was performed on a smaller subset of these samples. A compilation of existing as well as new vitrinite reflectance data was used for estimating burial paleotemperatures. These served as criteria for sample selection, as sites with temperatures sufficient to reset at least the apatite (U-Th)/He system (> ca. 80 °C) and potentially the apatite fission track system (> ca. 110 °C) were preferentially targeted.

We find reset AHe and subordinately reset AFT ages, that monitor a so far un(der)appreciated phase of prominent cooling between ca. 18 to 25 Ma. For flysch sandstones from the Wienerwald both thermochronometers yield similar ages, implying an exhumation phase, which removed 4-6 km of overburden. Similar results were found for Lunz sandstone samples from the area around Lilienfeld. Apatite (U-Th)/He ages from Gosau sandstones along the western border of the Vienna basin were mostly reset with single grain ages clustering around 20 Ma.

Our new results are difficult to reconcile with geodynamic models that imply tectonic quiescence during large-scale subsidence and widespread deposition of Augenstein clastics. Interestingly, the sedimentary archive of the eastern part of the Molasse basin records a change in the sedimentation pattern and onset of rapid basin infill at ca. 19 Ma, too.

We discuss our findings in the light of postcollisional thrust wedge evolution and potential impact of margin architecture and the Bohemian Spur. This promontory acted as a buttress for foreland-propagating thrusting, intensifying exhumation above it. Slab detachment beneath the Eastern Alps has recently been proposed based on results from the AlpArray initiative. We discuss, to what extent the newly detected cooling pulse may constitute the surficial expression of this slab break-off.

How to cite: Heberer, B., Bernhard, S., István, D., Reinhard, S., Tari, G., Wagreich, M., von Hagke, C., and Wessely, G.: Rapid Oligocene to Miocene cooling in the easternmost Alps driven by thrusting onto the Bohemian promontory and/or deep mantle processes, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-16083, https://doi.org/10.5194/egusphere-egu23-16083, 2023.

Inheritance and basement architecture
17:05–17:15
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EGU23-13479
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On-site presentation
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Hannah Pomella, Thomas Klotz, Anna-Katharina Sieberer, Hugo Ortner, Alexandra Wzietek, István Dunkl, and Ernst Willingshofer

The Dolomites Indenter represents the eastern front segment of the Neogene to ongoing N(W)-directed continental indentation of Adria into Europe. Concomitant shortening is accommodated within a south-vergent thrust belt, situated between the Periadriatic Fault system and the South-Alpine front. A combination of low temperature thermochronological analyses, focussed mapping and analogue modelling is used for unravelling the Neoalpine history of the crustal and lithospheric scale tectonic processes during indentation.

In our analogue models, extensional platform-basin geometries, formed at passive continental margins, are subject to subsequent shortening and orogenesis. Parallel to oblique (10 to 20 degrees with respect to the basin axes) contraction has been applied leading to the inversion of the pre-orogenic basins. The experiments show that the simple presence of an inherited platform-basin configuration controls the overall style of compressional deformation, no matter of including frictional or viscous basal décollements, of varying the rheology of the basin fill, or of changing platform-basin thickness ratios. Orientations of thrust faults change laterally across inherited platform-basin transitions throughout all experiments. New fault slip data and shortening directions from fold axes along the western segment of the Belluno thrust of the Valsugana fault system support variations of thrust fault orientation and a lateral change in shortening direction (from SSW to SSE along strike) along one single fault. Based on our modelling results, we infer that this variability of shortening directions depends on inherited structures and do not necessarily reflect different deformation phases.

Our low-temperature thermochronological dataset (zircon and apatite (U-Th)/He, and apatite fission track analyses) focuses on the Dolomites Indenter and spans from the Periadriatic Fault System (Pustertal-Gailtal fault) in the north to the footwall of the Bassano thrust in the south. The results argue against an only in-sequence fault activity within the dominantly WSW – ENE striking thrust belt but indicate a more complex fault system development, including backstepping fault activity. This is locally supported by field observations of fault cross-cutting relationships (e.g., at the Moschesin fault near Agordo). Remarkable that west of the Transalp Corridor Mesozoic apatite fission track ages are preserved within fault delimited areas while further to east all apatite fission track data show Cenozoic ages indicating younger exhumation in the eastern part of the study area.

How to cite: Pomella, H., Klotz, T., Sieberer, A.-K., Ortner, H., Wzietek, A., Dunkl, I., and Willingshofer, E.: The evolution of a thrust belt within a continental indenter: investigating the internal deformation of the Dolomites Indenter, eastern Southern Alps, in a combined low-temperature thermochronology, field and analogue modelling study, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-13479, https://doi.org/10.5194/egusphere-egu23-13479, 2023.

17:15–17:25
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EGU23-6654
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ECS
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On-site presentation
Patricia Cadenas Martínez, J. Kim Welford, João C. Duarte, Gabriela Fernández-Viejo, and Luis Somoza

The structure of Iberian Atlantic margins resulted from multiple Mesozoic rift events and subsequent contractional deformation occurring from the Upper Cretaceous to Cenozoic during the Alpine Orogeny. Along the southern Bay of Biscay, the North Iberian margin shows various styles of contractional deformation, ranging from mild reactivation of pre-existing extensional structures, halokynetic-related processes, to wedging and underthrusting. The Biscay accretionary wedge developed as the major structure at the base of the continental slope in the central and western parts of the North Iberian margin, which are part of the western branch of the Pyrenean-Cantabrian Orogen, together with the Cantabrian Mountains onshore. The wedge is interpreted to continue from the western North Iberian margin, where incipient subduction has been proposed, to the Galicia Margin further to the southwest. Along the West Iberian margin, thrusting and related folding and halokynetic-related processes focused contractional deformation.

In this work, we describe the seismo-stratigraphy, and we map contractional structures along the North Iberian and West Iberian margins based on the interpretation of 2D seismic reflection profiles. We identify and describe structural domains along the extinct subduction zone along the North Iberian margin, describe the structure of the fossil Biscay accretionary wedge, and identify and map different styles of Alpine contractional deformation along the North Iberian and West Iberian margins. We also describe the pre-existing Mesozoic rift structure in order to analyse the overprint between different rift architectures and contractional styles of deformation. The overall goal is to define different styles and stages of Alpine contractional deformation along Iberian Atlantic margins during the first phases of the convergent cycle preceding or leading to subduction.

 

How to cite: Cadenas Martínez, P., Welford, J. K., C. Duarte, J., Fernández-Viejo, G., and Somoza, L.: Alpine subduction and intraplate deformation along the Iberian Atlantic margins, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-6654, https://doi.org/10.5194/egusphere-egu23-6654, 2023.

17:25–17:35
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EGU23-4943
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On-site presentation
Ahmed Abdelmaksoud, Mohammed Ali, Meixia Geng, and Michael Searle

The subsurface structural geometries of the United Arab Emirates (UAE) fold-and-thrust belt (FTB) and foreland basins are interpreted from seismic, well data, and gravity and magnetic data, integrated with surface geology. We also determined the basement depths, as well as the relation between shallow sedimentary structures and deep basement features. Miocene to Lower Jurassic sequences were interpreted and mapped. Additionally, we outlined subsurface extent of Sumeini and Hawasina allochthonous nappes. The tectonic subsidence curves suggest that the final major passive margin rifting event occurred in the early Aalenian and lasted till Oxfordian. Loading of the Semail ophiolite thrust sheet and accompanying allochthonous thrust sheets resulted in uplift at ca. 95 Ma and rapid subsidence at ca. 83 Ma, indicating the transition of the Arabian margin from a rifted passive margin to a foreland basin. The region witnessed an accelerated subsidence during the late Oligocene-Miocene, attributed to the initial collision of the Central Iran and Arabian plates. The Permian-Jurassic NW-SE oriented rift faults were reactivated as thrust faults during the Late Cretaceous ophiolite obduction and late Oligocene-Miocene continental collision. Two different tectonic regimes are identified in the FTB. Based on the seismic reflection profiles and derivative maps of gravity and magnetic data, the northern regime has NNW–SSE striking thrusts, backthrusts and folds. It is characterized by major inversion of the rift faults with up to 3,700 m thrusting throw. Four major west-verging and east-dipping thrusts, which cross the northern area, form fault-propagation folds and dissect the entire stratigraphy. Whereas the southern regime around Jabal Hafit is dominated by the Tarabat backthrust, which cuts across the Upper Cretaceous and Cenozoic successions. Moreover, the Mesozoic platform carbonates are dissected by inverted faults (pop-up structure) in this regime. The Hawasina décollement, together with the inverted basement structures formed the Jabal Hafit anticline as a backthrust structure. On the other hand, results of the 3D gravity inversion indicate that the basement depths range from 11.5 km along uplifted areas of the FTB to 18.8 km within the deeper parts of the foreland basin. Significant northward increases in both basement depth and the thickness of the late Oligocene-early Miocene successions indicate a northward increase in the severity of thrusting and crustal loading along the main Khusub thrust. The basement uplifts are found to be correlated with shallower anticlinal features, indicating a direct relationship between basement uplifts and shallow sedimentary structures and hence indicating reactivation of basement structures during the Zagros collision.

How to cite: Abdelmaksoud, A., Ali, M., Geng, M., and Searle, M.: Fold-and-thrust belt and foreland basin of the United Arab Emirates: Sedimentary structures, basement morphology, and tectono-stratigraphic evolution, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-4943, https://doi.org/10.5194/egusphere-egu23-4943, 2023.

17:35–17:45
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EGU23-9481
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On-site presentation
Patrick A Meere and Chloe R Parker

Determining the sequencing of different deformation mechanisms and styles is crucial to understanding how the Earth’s crust responds to tectonic stress.  The sequence of near surface compressional deformation in peripheral orogenic forelands typically starts with an early stage of bulk homogenous shortening, i.e. layer parallel shortening (LPS) followed by folding and contractional faulting. The temporal and spatial distribution of strain is also very much influenced by the inherited basement structure and pre-collisional basin architecture in such foreland settings, in particular inherited extensional fault systems. Tectonic contraction in such settings tends to promote the positive inversion of basins through LPS, folding and reverse faulting by the exploitation of pre-existing bounding structures and facilitated by the lower bulk density and strength of sedimentary fill sequences when compared to the surrounding basement.

This study will combine conventional structural field studies from the Variscides of SW Ireland with the spatial characterisation of finite strain using clast shape analysis and anisotropy of magnetic susceptibility (AMS) studies on deformed sandstones as a means of elucidating the temporal and spatial evolution of deformation in an orogenic foreland that is heavily influenced by pre-existing basement architecture and structures. AMS is increasingly seen to be a particularly sensitive proxy for tectonic strain signals in low to medium strain settings on the periphery of orogens.

The Variscan of SW Ireland offers an excellent opportunity to investigate the full foreland strain cycle from early bedding parallel oblate fabrics to more prolate intermediate fabrics and finally cleavage parallel oblate fabrics in an overall setting that incorporates marked basement control of the spatial distribution of finite strain. The adopted multi-technique approach will also allow for insights into the relative timing of deformation events.  

How to cite: Meere, P. A. and Parker, C. R.: The role of basement architecture in the spatial and temporal development of tectonic deformation in an orogenic foreland – An example from the Variscides of SW Ireland., EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-9481, https://doi.org/10.5194/egusphere-egu23-9481, 2023.

17:45–17:55
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EGU23-6785
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ECS
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On-site presentation
Yating Zhong, Timothy Kusky, Lu Wang, and Kurt Stüwe

     We report studies of an ancient, ~10 km wide fold/thrust nappe belt developed as one zone of a 150 km wide, Archean collisional orogen in the North China Craton. Principles of cross-section construction and balancing were utilized to derive the first-reported, detailed map and crustal-scale profile of the Archean fold/thrust nappe belt. Combined with stratigraphy and geometric restoration, we demonstrate that the fold/thrust nappe pile consists of four major 2.69-2.52 Ga sub-horizontal nappes stacked upon each other, and ductile shear zones below each of them, emplaced onto a 2.56-2.51 Ga passive margin-like shallow marine platformal para-autochthon at 2.51-2.50 Ga. Four individual nappes were derived from different tectonic belts of an ancient paleo-ocean before they were emplaced. They are characterized by distinctive kinematic and thermal evolution.

    Geometric, statistical analysis of structural-fabrics and kinematic indicators illustrate that the fold/thrust nappes of forearc and oceanic floor sequences have been reworked by folding and thrusting with stratigraphic repetition during three kinematic phases, and the final emplacement was accomplished by a combination of rigid body translation along shear zones between nappes and the para-authochthon as well as internal strain by ductile deformation. The para-autochthon only records the predominant D2 event, related to the fold/thrust nappes emplacement, but lacks the records of oldest kinematic phase.

    Thermal characteristic inferred by metamorphic studies reveal an inverted thermal structure in the fold/thrust nappes, indicated by the observation of a decrease in metamorphic grade from amphibolite facies in the nappes to greenschist facies in the underlying schistes lustrés forming the basal décollement; but it shows a downward temperature-increase in the metamorphic field gradient in the passive margin para-authochthon with relatively stable pressure records.

    This work explicitly unravels the first-order geometry and the tectono-structural evolution of the 2.5 Ga fold/thrust nappe belt by constraints on the scale, structural sequence, and metamorphic grade of the different tectonic units. This provides a quantitative basis for drawing analogies between Archean and present lithospheric deformation and discussing the style of tectonism during Archean orogenesis.

How to cite: Zhong, Y., Kusky, T., Wang, L., and Stüwe, K.: Structural and thermal evolution of an Archean fold/thrust nappe belt based on quantitative structural profile, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-6785, https://doi.org/10.5194/egusphere-egu23-6785, 2023.

17:55–18:00

Posters on site: Wed, 26 Apr, 10:45–12:30 | Hall X2

Chairpersons: Jonas B. Ruh, Esther Izquierdo Llavall
Analogue and numerical modelling
X2.209
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EGU23-3827
Atsushi Noda, Fabien Graveleau, Cesar Witt, Frank Chanier, and Bruno Vendeville

Deformation process and strength evolution in accretionary wedges are important factors that affect kinematics and dynamics at subduction zones. However, it is still challenging to understand the relationship between the short-term geodetic observations (coupling ratios or earthquakes) and the long-term geological structures (patterns of imbricated thrust sheets or fault networks) in natural systems. In this study, we performed 2-D, large-shortening (1 m) analog sandbox experiments to examine how the wedge deformation is affected by different décollement conditions including heterogeneities and numbers of weak layers in the incoming sediment. Four different settings (Types 1–4) of the incoming sediment layers were examined in this study. Serial side-view digital photographs were quantitatively analyzed with an open-source DIC software to characterize the accretion cycles, underthrusting/underplating, and reactivation of pre-existing thrusts (out-of-sequence thrusts).

The reference models with single décollement (Type1) were dominated by periodic cycles of frontal accretion with landward propagation of strain, uplift, and reactivation of the pre-existing thrusts, which progressively increased in strength and then approached the critical state. Each cycle was composed of preparation (Phase 0), initiation (Phase 1), accretion (Phase 2), and reactivation (Phase 3). Through frontal accretion, the wedge accumulated the strain internally with landward migration of the basal coupled area along the plate interface, which caused uplift and reactivation of the landward preexisting thrusts in the wedge (hardening). When a new frontal thrust emerged at the deformation front (Phase 1), the basal coupling was suddenly lost (softening). Through this cycle, the entire accretionary wedge progressively increased in strength while experiencing hardening and softening and approached the critical state. The double décollement models (Type 2) showed a similar accretion cycle to Type 1 models, but it consisted of a combination of shallow-rooted and deep-rooted frontal thrusts, meaning that the décollement stepped up and down between the interbedded and basal weak layers. This promoted sediment underthrusting at the frontal part of the wedge during the early phase of the accretion cycle and favored the connection of pre-existing deep-rooted thrusts with shallow-rooted thrusts. A frictional interruption in the basal décollement (Type 3 or 4 models) produced a combination of a steep-taper inner wedge and a gentle-taper outer wedge, and disturbed the wavelengths of the accretion cycle. The single décollement models (Type 3) were dominated by high-angle out-of-sequence thrusts, while underplating was significantly promoted in the double décollement model (Type 4) where the interbedded décollement acted as a low-angle, smooth-surface megathrust.

These results shed light on the impact of properties and homogeneity of the incoming sediment and the plate interface on the spatial and temporal evolution of internal structure and thrust activity in accretionary wedges through multiple accretion cycles. Comparisons of our results with natural subduction zones will contribute to understanding the mechanisms and dynamics of deformation process and strength evolution in natural subduction zones.

How to cite: Noda, A., Graveleau, F., Witt, C., Chanier, F., and Vendeville, B.: Analog modeling of accretionary wedges with various décollement settings: Quantitative analysis of deformation process and strength evolution, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-3827, https://doi.org/10.5194/egusphere-egu23-3827, 2023.

X2.210
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EGU23-10608
Yi Long, Fabien Graveleau, Bruno C. Vendeville, Hanlin Chen, Xiaogan Cheng, and Xiubin Lin

Structural deformation of fold-and-thrust belts is influenced by the properties of décollements (number, rheology, thickness, etc.), the presence of inherited structures in the basement as well as the amount of syntectonic sedimentation, among others. Although the effect of each of these parameters has been well constrained with a series of numerical and experimental works in the literature, few sandbox models comprehensively consider all these parameters together, and particularly investigate the effect of their lateral variation. In this context, we carried out several 3-D sandbox models to investigate the effect of increasing syntectonic sedimentation rate on kinematic evolution of fold‐and‐thrust systems which contain a basal brittle detachment layer and a shallow detachment layer that changed from a brittle to a viscous domain along the mountain strike. The influence of different basement width structures, affecting the kinematics and geometry of the interbedded viscous décollement, has been also tested.
Results indicate that the rate of syntectonic sedimentation exerts a first-order control on the kinematic evolution of fold‐and‐thrust belts since increasing syntectonic sedimentation rate stops (in the brittle domain) or delays (in the viscous domain) the propagation of deformation towards the foreland. Moreover, syntectonic sedimentation prohibits the propagation of deformation in the deep décollement level due to the modification of the taper angle. Structural evolution of the transfer zone in between the brittle and viscous domain is also affected since if becomes narrower and more orthogonal to the mountain front at higher sedimentation rates. Specifically, in the brittle domain, the fault dip angle increases with the increase in syn-sedimentation rate and its cross-sectional geometry becomes straighter. In the viscous domain, syntectonic sedimentation affects the partitioning of deformation with development of long-lived and complex 3-D salt structures near the hinterland (such as squeezed diapirs, salt welds and salt tongue), whereas frontal structure becomes more cylindrical. Toward the hinterland, syntectonic sedimentation increases backthrust activity, which becomes increasingly different between the brittle and viscous domain. For instance, the increase in backthrust displacement in the ductile domain is greater than the one in the brittle domain. About the basement high, our study reveals that it has a strong controlling effect on the viscous domain, dominating the development of structural belt on the top of the basement high and promoting the propagation of deformation front to the pinch-out of the salt layer. Besides, syntectonic sedimentation simplifies the structural style between the basement high and the hinterland. It strengthens the structural influence of the transfer zone, which localizes into a single strike-slip transfer fault which increases the frontal fault displacement.
Our experimental results are compared with structures in the Wushi-Kuqa fold-and-thrust belts in Southern Tianshan (Central Asia) and help better understanding interaction between syntectonic sedimentation, décollement properties and basement configuration.

How to cite: Long, Y., Graveleau, F., Vendeville, B. C., Chen, H., Cheng, X., and Lin, X.: Influence of syntectonic sedimentation on kinematic evolution of fold‐and‐thrust belts with lateral changes in shallow décollement properties and basement inherited structures: insights from analogue modeling, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-10608, https://doi.org/10.5194/egusphere-egu23-10608, 2023.

X2.211
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EGU23-4618
Ayumu Miyakawa, Atsushi Noda, and Hiroaki Koge

We propose a conceptual geological model for the collision of multiple basement topographic highs (BTHs; e.g., seamounts, ridges, and horsts) with a forearc accretionary wedge. Even though there are many BTHs on an oceanic plate, there are few examples of modeling the collision of multiple BTHs. We conducted numerical simulations using the discrete element method to examine the effects of three BTH collisions with forearcs. The typical geological structure associated with a BTH collision was reproduced during the collision of the first BTH, and multiple BTH collisions create a cycle of formation of BTH collisional structures. Each BTH forces the basal décollement to move up to the roof décollement, and the roof décollement becomes inactive after the passage of the BTH, and then the décollement moves down to the base. As the active décollement position changes, the sequences of underthrust sediments and uplifted imbricate thrusts are sandwiched between the décollements and incorporated into the wedge. The distinctive structural features observed in our model are comparable to the large faults in the Kumano transect of the Nankai Trough, Japan, where a splay fault branches from the plate boundary and there are old and active décollements. 

How to cite: Miyakawa, A., Noda, A., and Koge, H.: Evolution of the geological structure due to the collision of multiple basement topographic highs in a forearc accretionary wedge: insights from numerical simulations, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-4618, https://doi.org/10.5194/egusphere-egu23-4618, 2023.

X2.212
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EGU23-12099
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ECS
Marc Guardia, Albert Griera, Boris Kaus, Andrea Piccolo, Norbert Caldera, and Antonio Teixell

Fold nappes and thrust nappes are found either in the internal or the external parts of orogenic belts worldwide and are geometrically and kinematically well constrained after more than a century of studies. However, the mechanics favouring one vs. the other remain incompletely understood due to the uncertainty and variability of pre-contractional configurations.

Recent numerical modelling of the Helvetic nappes of the Alps highlighted the relevance of the competence contrast between stiff and weak layers in controlling the deformation style. Similarly, the Eaux-Chaudes fold nappe of the French Pyrenees (Caldera et al. 2021) appears governed by the mechanical stratigraphy. However, the ductile extrusion of a half graben with which the Helvetic nappes have been modelled cannot be invoked for the Pyrenean example, which appears formed by shearing of a stiff carbonate layer between two weak decoupling units and a backstop. The occurrence of the two structural styles in the Eaux-Chaudes region highlights the need to find out under which conditions or pre-orogenic configurations one or the other nappe style are favoured.

We employed the thermomechanical staggered finite difference code LaMEM (Kaus et al., 2016) to perform 2D parametric simulations to address changes between thrust nappes (plastic/brittle-localisation) and recumbent fold nappes (viscous/ductile-distributed). The simulations were carried out using a linear viscoelastoplastic rheology with the Drucker-Prager criterion for plasticity. We measured the hinge migration during folding by implementing passive tracer elements tracking the position of markers through time. Based on the Eaux-Chaudes fold nappe as a reference natural example, we tested the pre-orogenic geometry but also the intrinsic mechanical properties of the stiff key layer and the adjacent units. Our results demonstrate a strong control of the configuration of weak and strong units on the deformation style.

In all cases a backstop causing stress concentration in the stiff layer (an underlying granite massif in the Eaux-Chaudes case) was necessary to induce either recumbent folding or thrusting. The absence of a backstop causes detachment buckle folds in the stiff layers, hindering nappe development. Deep burial and the combination of a thick upper decoupling unit and a lower detachment level are essential features favouring viscous behaviour and spatially distributed deformation, enabling the formation of fold nappes by progressive fold hinge migration (material particles are travelling from the normal to the reverse limb of the nappe). On the other hand, shallower conditions, shorter lengths of the stiff layer and lower friction angles of the key layer reduces hinge migration, enhancing instead reverse limb stretching and shearing, which eventually results in strain localisation and thrusting. Our results may be applicable to other orogenic belts and also to other parts of the Axial Zone of the Pyrenees where the Mesozoic cover is eroded and the Alpine deformation is obscure.

Caldera, N., Teixell, A., Griera, A., Labaume, P. and Lahfid, A. (2021): https://doi.org/10.1111/ter.12517

Kaus, B.J.P., Popov, A., Baumann, T, Püsök, A., Bauville, A., Fernandez, N. and Collignon, M. (2016): Forward and Inverse Modelling of Lithospheric Deformation on Geological Timescales, NIC Symposium 2016–Proceedings, Germany, NIC Series, 48, 299-307.

How to cite: Guardia, M., Griera, A., Kaus, B., Piccolo, A., Caldera, N., and Teixell, A.: Conditions favouring fold vs. thrust nappes: insights from the modelling of a Pyrenean example and implications on hinge migration vs. limb stretching mechanisms, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-12099, https://doi.org/10.5194/egusphere-egu23-12099, 2023.

X2.213
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EGU23-16710
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ECS
|
Florian Duschl, Antonia Schätz, and Michael Drews

Weak detachments below active thrust fronts of subaerial orogenic wedges are mostly controlled by wedge taper geometry. A common method to investigate wedge properties is critical taper analysis. According to critical taper theory fault strength in a mechanically homogeneous wedge can be constrained from surface slope angle α and the angle of inclination of the basal detachment β. However, the influence of fluid overpressure on fault strength is often underestimated. Here, we present a simplified 3D wedge taper model of the North Alpine Thrust Front (SE Germany) between Lake Constance and the Inn Valley which is used for critical taper analysis. Different scenarios with varying input parameters are considered with special emphasis on fluid overpressure ratios.

Critical taper analysis shows that frictional sliding resistance within the wedge varies both, laterally and longitudinally. Small fault strength values are predominant in the inner wedge, whereas the outer wedge is characterized by a higher fault strength due to a steepening detachment. Frictional sliding resistance in general decreases towards the hinterland likely resulting from lower surface slope values. For the western part of the North Alpine Thrust Front, our model shows low fault strength which is probably controlled by pore fluid overpressure and a flat detachment angle. Comparatively high fault strength in the eastern part however might be controlled by a steeper basal detachment, which is problay caused by underplating and a more complex structural framework. Finally, we use acquired data to discuss the influence of laterally varying sliding friction within the basal detachment on observed pore fluid overpressure in adjacent tectonic units, i.e. the Subalpine Molasse and the Foreland Molasse in Bavaria.

How to cite: Duschl, F., Schätz, A., and Drews, M.: Critical taper analysis of the North Alpine Thrust Front, SE Germany – Influence of fluid overpressure on fault strength in a subaerial orogenic wedge, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-16710, https://doi.org/10.5194/egusphere-egu23-16710, 2023.

Interaction between tectonics and sedimentation
X2.214
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EGU23-14129
Cédric Bonnel, Lionel Menzer, Charles Aubourg, Jean-Paul Callot, and Guilhem Hoareau

The nature and rate of syn-orogenic sedimentation play an important role in the tectono-stratigraphic evolution of foreland basins. Recent works have shown syn orogenic evaporites at the transition between underfilled and overfilled conditions in the Sivas basin (Turkey) have strongly influenced the subsequent structural and sedimentary evolution of the foreland fold and thrust belt (Legeay et al., 2020).

In the western South Pyrenean Zone, the Jaca basin exhibits the classical stratigraphic succession of a pro-foreland basin systems. This was filled during Eocene-Oligocene with siliciclastic sediments derived from the erosion of the Pyrenees and deposited in a marine to continental environment. During Bartonian, a derivation in the sediment routing system and decreasing subsidence rate resulted in the deposition of a km-thick shale unit forming the transition between marine and continental conditions.

The “bed-to-bed” mapping of the syn-orogenic units at the basin-scale using high-resolution DEM together with the reinterpreted seismic lines were used to build three cross-sections that highlight the structural style of the western South Pyrenean Zone. These illustrate the tectono-sedimentary evolution of a transitional shallow-marine to continental foreland basin.

From end-Bartonian, the deposition of the Orosia-Cancias conglomerates in the north-eastern basin margin is coeval with the onset of the folding of the Basa anticline forward. During Priabonian, this were subsequently welded and forward-tilted coevally with the development of an imbricate in Hecho turbidites beneath, that can be linked to the emplacement of the Gavarnie thrust-sheet. At this time, the Orel alluvial fan was deposited westward at the termination of the Basa anticline and was associated with the growth of the second, shale-cored Atarès anticline folding ahead. This was in turn welded during Rupelian at the time of deposition of the San Juan conglomerates at its western termination, coevally to the Botaya anticline folding downstream.

The tectono-sedimentary evolution of the Jaca fold-and-thrust belt is thus resulting from complex interactions between the deformation of mobile shale and syn-orogenic alluvial sedimentation both at local and regional scale. This example highlights the influence of the syn-orogenic sedimentation and especially the deposition of a decoupling layer at the transition between marine and continental conditions during the evolution of foreland fold and thrust belts as well as thein mountain building processes.

How to cite: Bonnel, C., Menzer, L., Aubourg, C., Callot, J.-P., and Hoareau, G.: A model of forced folding controlled by syn-orogenic clastic deposits in a foreland fold and thrust belt. The case of the Jaca Basin, South Pyrenean Zone., EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-14129, https://doi.org/10.5194/egusphere-egu23-14129, 2023.

X2.215
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EGU23-3797
Andréa Peuzin, Marianne Saillard, Nicolas Espurt, François Michaud, Cédric Bulois, Marc Régnier, and Ysabel Calderon

Understanding the dynamics of forearc basins is a challenge to improve knowledge of their influence on subduction zone earthquakes and tsunamis. The structural architecture of the Tumbes and Guayaquil forearc depocenters in the Northern Andes is revealed by subsurface data and the construction of serial cross-sections. Seismic reflection profiles and well data reveal that the overall forearc depocenters by widespread gravitational raft tectonics instabilities. These instabilities occurred principally during the Late Neogene to Quaternary period. We emphasize kilometric-scale upper listric normal fault dip regionally basinward paired with downdip thrust wedge. These structures branch downward on a regional décollement level developed in the upper Oligocene ductile shales above subduction zone. The development of this tectonic style appears to be significantly controlled by the coeval of tectonics, high sedimentation rate in the basin and pore pressures processes. Our findings are original enough as these kinds of instabilities are much more often observed in passive margins. Finally, the large active movements of sedimentary masses could also be triggered by seismicity and could generate potential tsunamis that could reach the neighboring coastal zone, including the Guayaquil city.

How to cite: Peuzin, A., Saillard, M., Espurt, N., Michaud, F., Bulois, C., Régnier, M., and Calderon, Y.: Gravitational raft tectonics in the Tumbes-Guayaquil forearc basin, Northern Andes (North Peru-South Ecuador), EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-3797, https://doi.org/10.5194/egusphere-egu23-3797, 2023.

X2.216
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EGU23-4732
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ECS
Yirang Jang, Sanghoon Kwon, and Vinod O. Samuel

Detrital zircon geochronology and isotope analysis can be used for inferring the provenance of detrital sedimentary sources in general, and can provide useful information to establish the tectonic evolution of a sedimentary basin. In this respect, analyzed detrital zircon SHRIMP U-Pb ages and LA–(MC)–ICP MS Lu-Hf isotopes from the Paleozoic metasedimentary successions in the Okcheon fold-thrust belt (FTB), providing new insights into their provenance and evolution during the Phanerozoic orogenesis.

The Okcheon FTB has been considered a prominent belt between the two basements (viz. Gyeonggi and Yeongnam massifs) in the southern part of the Korean Peninsula, and subdivided the Okcheon Zone to the west and the Taebaeksan Zone to the east. The Taebaeksan Zone consists predominantly of the Paleozoic metasedimentary rocks comprising Early Paleozoic Joseon and the Late Paleozoic Pyeongan supergroups with Middle Paleozoic hiatus locally. On the contrary, the Okcheon Zone exposed the post-Devonian to Permian clastic wedge on top of the Neoproterozoic bimodal volcanic rocks related to the intracontinental rifted settings.

Our results show that all Paleozoic strata commonly have Paleoproterozoic and Paleozoic zircon ages with rare Meso- to Neoproterozoic ones. Each zircon population shows the following notable results, allowing estimation of their sedimentary sources: (1) The Paleoproterozoic zircons (ca. 1.85 and 2.50 Ga) with similar ranges of εHf(t) values are most common in the basement rocks of the Korean Peninsula, thus can be sourced from both the Gyeonggi and Yeongnam massifs. (2) The Meso- to Neoproterozoic zircons, only preserved in the late Middle to Late Cambrian strata, probably reflected abrupt changes in source areas. (3) The youngest Paleozoic zircons of each formation, almost coincident with its deposition ages, suggest the presence of syndepositional magmatism. This means that detritus was supplied from proximal magmatic sources during the deposition (4) The Cambrian-Ordovician zircons from the Lower Paleozoic sequences, but rarely not included in the successive Upper Paleozoic sequences, suggest a provenance change after the hiatus between the two sedimentary successions. (5) The Permian zircons showing different εHf(t) values in each locality within the study area indicate that detrital sources were varied and localized.  

These integrated results of the detrital zircon U-Pb ages and Hf isotope data from the Paleozoic successions together with the existence of a post-Devonian to Permian clastic wedge in the Okcheon Zone might possibly be related to the subduction in relation to Okcheon Orogeny similar to the Allegany orogenic time span in Appalachian. The entire sedimentary sequences within the Okcheon Belt experienced deformation and metamorphism related to the subsequent (Permo-) Triassic collisional orogeny (viz. Songrim Orogeny) along the Korean collision belt, forming regional fold-dominated mountains of the Okcheon FTB. This suggests that the Okcheon FTB records important information for Paleozoic provenance changes linked to the tectonic evolution of the Korean Peninsula, which will further help to understand the spatial and temporal evolution of orogenic belts during the Phanerozoic along the East Asian continental margin.

How to cite: Jang, Y., Kwon, S., and Samuel, V. O.: Provenances of the Paleozoic successions in the Okcheon FTB, Korea with implications for the Phanerozoic tectonic evolution of the Korean Peninsula along the East Asian continental margin, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-4732, https://doi.org/10.5194/egusphere-egu23-4732, 2023.

Structural style and kinematics in fold-and-thrust belts
X2.217
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EGU23-15525
Maryline Le Béon, Jhih-Wei Shih, Chang-Chih Chen, Wen-Jeng Huang, Ya-Chu Tseng, Yi-Wei Chiu, Yen-Chiu Liu, Meng-Long Hsieh, Chih-Heng Lu, and Erwan Pathier

In the classical evolution of a fold-and-thrust belt, the deformation front progressively propagates basin-ward and the activity of the newly developed structures modifies the geometry and, likely, the kinematics of the existing structures located on their hanging wall. The Taiwan mountain belt sits at the convergence boundary between the Luzon volcanic arc and the Chinese continental margin. The 8-cm/yr westward shortening across the island is partly accommodated at the western piedmont of the orogen by a series of folds and thrusts trending about N30˚E. This study investigates the Holocene activity of a geological structure located within the foothills of southwestern Taiwan. At this latitude, GPS observations indicate about 2 cm/yr of westward shortening across a 20-km-wide zone. The targeted geological structure is located about 12 km east of the deformation front. It includes, from west to east, a tight upright anticline, the Wushantou anticline, with early Pleistocene mudstone at the anticline axis, a significant thrust fault with a steep dip to the east, the Lunhou fault, that brought early Pliocene strata against Pleistocene strata, and an active west-dipping backthrust with limited total offset, the Kouhsiaoli fault. These structures are crossed over by the Tsengwen River. A flight of 11 Holocene river terraces was dated from 10 ka to 2 ka using radiocarbon dating. The highest terrace locates near the anticline fold axis and lies 140 m above the modern river. We determined bedrock incision rates across the investigated structure and accounted for sedimentation rates in the Holocene foreland basin to determine uplift rates that evolve from 5-7 mm/yr west of the anticline to 15-20 mm/yr from the anticline axis to the Kouhsiaoli backthrust, and decreasing to 5-7 mm/yr east of the backthrust. Present deformation observed by InSAR indicates a similar deformation pattern. These suggest that the backthrust and anticline are the main active structures at least since the early Holocene and that the major geological thrust has likely been inactive during this time period. On-going works are focused on the deep geometry of these geological and active structures, on the partition of shortening between the anticline and the backthrust and on how the entire structure may have evolved as deformation propagated westward.

How to cite: Le Béon, M., Shih, J.-W., Chen, C.-C., Huang, W.-J., Tseng, Y.-C., Chiu, Y.-W., Liu, Y.-C., Hsieh, M.-L., Lu, C.-H., and Pathier, E.: Active anticline and backthrust override a geological thrust: evidence from present and Holocene deformation rates within the foothills of southwestern Taiwan, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-15525, https://doi.org/10.5194/egusphere-egu23-15525, 2023.

X2.218
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EGU23-5320
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ECS
Zhenyu Peng, Xin Wang, Bruno Vendeville, Fabien Graveleau, and Alan Nunns

In central Asia, the Tianshan mountains have undergone a series of subduction-collision-accretion processes during Paleozoic times that resulted in forming basement structures later reactivated during the Cenozoic rejuvenation of the range. In the northern Tianshan-South Junggar foreland basin, en échelon W-E / WNW-ESE folds constitute the large-scale fold-and-thrust belt (FTB). Using recent industrial 2-D and 3-D seismic surveys carried out in the western area of the FTB, we have analyzed outcropping structures (Dushanzi and Xihu anticlines) and buried structures (Gaoquan, Kadong, Kayindike, and Dunan anticlines). Observing that the strike of these structures changes from W-E in the east to NW-SE in the west, we investigated the parameters that controlled this lateral variation along the FTB. We particularly analyzed the structural and kinematic relationships between deep Mesozoic and shallow Neogene-Quaternary structures. We support our investigation by using seismic interpretation and balanced restoration.

Our results provide new insights into the structural and kinematical history of the Mesozoic-Cenozoic tectonic evolution of the northern Tianshan foreland basin, and into the record of deformation propagation. We first demonstrated that the tectonic and sedimentary evolution during the Triassic and Jurassic is characterized by NW-SE and NNW-SSE strike-slip faults that controlled the development of pull-apart and restraining bend systems. These features were partially reactivated during the Neogene-Quaternary contractional deformation, depending on their position relative to the mountain front. Second, we quantified that about 7 km of total S-N shortening has been accommodated across the western area of the FTB. We also quantified the displacement rate accommodated on every single structure. It is ~0.13-0.2 mm/yr in the Gaoquan anticline since Quaternary, ~0.19-0.30 mm/yr in the Dunan anticline since Quaternary, ~0.36 mm/yr in Dushanzi anticline since Pliocene and ~0.30-1.2 mm/yr in the Xihu, Kadong and Kayindike anticlines during Quaternary times. Additionally, the rate of thrusting above the reactivated strike-slip faults in the Gaoquan anticline is 3 to 6 times lower than that of thrusting above the inactive strike-slip faults of the Kadong and Kayindike anticlines. This suggests that the reactivation of the basement strike-slip fault zone partitioned the contractional strain during Quaternary times. Finally, we integrate our results in a 3-D model of the western area of the FTB that illustrates the spatial pattern of structures at depth. Notably, it emphasizes how deep Mesozoic structures exerted a primary control on the growth of Cenozoic thrust-related folds by localizing the nucleation of thrust ramps during compression. This pattern of deep vs. shallow deformation interaction might be applied in some other areas of the Tianshan foreland basin.

How to cite: Peng, Z., Wang, X., Vendeville, B., Graveleau, F., and Nunns, A.: Geometry and kinematics of Mesozoic and Cenozoic structures in northern Tianshan foreland basin: insights from quantitative structural analysis of 2-D and 3-D seismic reflections and balanced restoration, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-5320, https://doi.org/10.5194/egusphere-egu23-5320, 2023.

X2.219
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EGU23-21
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ECS
|
Anzor Giorgadze, Victor Alania, Benjamin Busch, Onise Enukidze, Dennis Quandt, Paolo Pace, Alexander Razmadze, and Tamar Shikhashvili

The Rioni foreland fold-and-thrust belt which is part of the western Greater Caucasus pro-wedge is located between the Lesser Caucasus and the Greater Caucasus orogens and is one of the most important examples of the collision-driven far-field deformation of the Arabia-Eurasia convergence zone (Alania et al., 2022). The Rioni foreland fold-and-thrust belt sedimentary infill consists of pre-and syn-orogenic sequences. Moreover, recent GPS and earthquake data indicate that the Rioni foreland fold-and-thrust belt is still tectonically active and the earthquakes’ focal mechanisms are mainly thrust faults (e.g., Tibaldi et al., 2017; Tsereteli et al., 2016).

Fault-related folding and wedge thrust folding theories were used to interpret 2D depth-migrated seismic reflection profiles and to construct the regional balanced and restored cross-sections across Rioni foreland fold-and-thrust belt. The balanced cross-section is approximately parallel to the trust transport direction and has a total length of 64 km. On the other hand, the amount of shortening obtained for this part of the regional balanced cross-section is 40% (-42.78km).

The main style of the deformation within the thin-skinned Rioni foreland fold-and-thrust belt is represented by a set of growth fault-propagation folds, duplexes, triangle zone, and a series of thrust-top basins. The evolution of the trust-top basins was mainly controlled by the kinematics of thrust sequences and competing growth fault-propagation folds and building compressional structures of the Rioni foreland fold-and-thrust belt was governed by the Greater Caucasus basement crustal-scale duplexes propagation along detachment horizons within the cover-generating thin-skinned structures.

Acknowledgment: This work was supported by Shota Rustaveli National Science Foundation (SRNSF) [Structural model of the Rioni foreland fold-and-thrust belt and the Southern Slope of the Greater Caucasus (The Tekhuri river gorge area) Grant #: PHDF-21-087]

References:

Alania, V., et al. (2022). Deformation structural style of the Rioni foreland fold-and-thrust belt, western Greater Caucasus: Insight from the balanced cross-section. Frontiers in Earth Science, 10:968386.

Tibaldi, A., et al. (2017). Active inversion tectonics, simple shear folding and back-thrusting at Rioni Basin, Georgia. Journal of Structural Geology 96, 35-53.

Tsereteli, N., et al. (2016). Active tectonics of central-western Caucasus, Georgia. Tectonophysics 691, 328-344.

How to cite: Giorgadze, A., Alania, V., Busch, B., Enukidze, O., Quandt, D., Pace, P., Razmadze, A., and Shikhashvili, T.: Structural architecture of the western Greater Caucasus pro-wedge: A case study from the Rioni foreland fold-and-thrust belt, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-21, https://doi.org/10.5194/egusphere-egu23-21, 2023.

X2.220
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EGU23-267
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ECS
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Augusto Maresca, Pablo Granado, Josep A. Muñoz, Gianreto Manatschal, Kei Ogata, and Stefano Tavani

The Apennines fold-and-thrust belt, forming part of the Africa-Eurasia plate boundary, developed due to the Neogene subduction of the Alpine Tethys underneath Europe and to the subsequent involvement of the Adria rifted margin into the collisional process. Since the Miocene, E-ward retreat of the slab caused extensional deformation to affect the thrust pile, which eventually led to the opening of the Tyrrhenian back-arc basin at the rear of the belt. Multiple schools of thought exist about the structural style of the Apennines, which propose irreconcilable models. The amount of shortening, the involvement of the crystalline basement, the architecture of the inherited rifted system and its degree of reactivation during convergence, and the role played by compressive inheritance during back-arc extension, are still highly debated.

In this contribution we focus on the Central Apennines. We integrate publicly available geological maps, interpretation of vintage seismic sections, borehole data, recent seismicity studies, previously published surficial geological cross-sections, and the latest thermochronological insights to build a balanced cross-section across the inner portion of the belt. Our aim is to critically evaluate previous models and to better define its deeper part. Our results suggest a dominantly thin-skinned style, in which inherited Mesozoic extensional faults developed during Adria rifting have been partly reactivated during thrusting. The major thrusts of the area are characterized by large displacements, ranging between 10 and >20 km, and sole into a basal décollement located at the base of the post-Variscan sedimentary sequence. Post-thrusting back-arc extension is accommodated by faults that either displace the compressional décollement levels or reactivate them with opposite kinematics.

How to cite: Maresca, A., Granado, P., Muñoz, J. A., Manatschal, G., Ogata, K., and Tavani, S.: A new crustal balanced cross-section through the Central Apennines (Italy), EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-267, https://doi.org/10.5194/egusphere-egu23-267, 2023.

X2.221
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EGU23-8509
Pablo Santolaria Otín, Concepción Ayala, Pilar Clariana, Ruth Soto, Josep Anton Muñoz, Félix M. Rubio, Juliana Martín-León, and Emilio L. Pueyo

Upon shortening, salt distribution determines the formation of salients and reentrants in fold-and-thrust belts. Such distribution is controlled by the original sedimentary architecture of the salt basin and subsequent post-sedimentary salt tectonics. In the Southern Pyrenees, the South Pyrenean Central Salient detaches on Triassic evaporites (the regional décollement of the Pyrenees) and stands as a prominent feature bounded, to the north and to the south, by diapiric provinces. Despite its subsurface geometry has been characterized by 2D reflection seismic profiles and exploration wells, an accurate image of the distribution at depth of the Triassic evaporites remains unsolved. In this work, we present an updated observed residual gravity anomaly map of the South Pyrenean Central Salient together with three gravity-validated cross-sections that give structural meaning to gravity anomalies and therefore yields a further interpretation of them helping to interpret those areas lacking seismic images. Middle-Upper Triassic salt accumulations dominate in the western half of the South Pyrenean Central Salient. To the northwest, a prominent accumulation of Triassic evaporites is likely associated with an inherited accumulation predating the Pyrenean orogeny and associated with extensional to gravity-driven salt tectonics during the rift and post-rift stages. To the South, Triassic rocks core salt-detached anticlines. Along the southernmost (and youngest) thrust sheet of the salient, diapirs and evaporite accumulations are associated to an inflated area resulting from the north-coming migration of evaporites during the middle to late stages of the Pyrenean orogeny.

How to cite: Santolaria Otín, P., Ayala, C., Clariana, P., Soto, R., Muñoz, J. A., Rubio, F. M., Martín-León, J., and Pueyo, E. L.: Gravity-constraint salt distribution and migration model in the South Pyrenean Central Salient, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-8509, https://doi.org/10.5194/egusphere-egu23-8509, 2023.

X2.222
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EGU23-11654
Ferdinando Musso Piantelli, Lukas Nibourel, Alfons Berger, and Marco Herwegh

Inversion and exhumation of crystalline basement units of passive margins is a critical stage of mountain-building processes. With a multi-methodological approach that combines 3D geological modelling and cross-section restoration at different time steps, we unravel the 4D geodynamic evolution of the Aar Massif (central Alps, Switzerland) during the late-stage Alpine orogeny (22 to 0 Ma). Our results demonstrate how a portion of the crystalline basement units of the European continental margin was exhumed in a non-cylindrical framework with an alternation of vertical and horizontal-dominated tectonics. Rapid exhumation (22 to 12 Ma), with deformation along steep reverse/normal faults, alternated with northwest-directed thrusting of the previously exhumed basement units (16 to 0 Ma). We pay special attention to how shear/fault zone patterns change laterally and temporarily to accommodate the non-cylindrical deformation in dome-like basement rises. Published thermochronometric and metamorphic peak temperature data provide additional insights into the temporal sequence of reverse and thrust faulting perpendicular and parallel to the strike of the orogen. Such variations in the fault geometries and associated offsets were constrained by the detailed reconstruction of the shear zone pattern in 3D. In this study, we show how the basement-involved uplift and shortening controlled the late-stage collisional overprint and mechanics of the northern rim of the central Alps.

How to cite: Musso Piantelli, F., Nibourel, L., Berger, A., and Herwegh, M.: 4D reconstruction of the Aar Massif during the late-stage continent-continent collision in the European Alps, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-11654, https://doi.org/10.5194/egusphere-egu23-11654, 2023.

X2.223
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EGU23-15666
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ECS
Julia Rudmann, David Colin Tanner, Michael Stipp, and Hannah Pomella

The Tauern Window in the European Alps has a high tectonic complexity. It is a key area to understand a number of important orogenic processes, including nappe stacking, exhumation, indentation as well as escape tectonics. The polyphase Alpine deformation history of the Tauern Window began with subduction and accretion of the Penninic realm beneath the northern margin of Adria (Austroalpine) in the Cretaceous. Ongoing convergence led to collision between Europe (Subpenninic) and the Adria margin and to the formation of the Penninic and Subpenninic nappe stack in the southward dipping orogenic wedge from Eocene to early Oligocene. The W-E trending Periadriatic Fault System (PFS) located within the Adriatic units south of the Tauern Window was active as dextral strike-slip fault at this time, as indicated by the deformation of the Eocene and Oligocene Periadriatic intrusions [1]. Indentation of the Dolomites Indenter (Eastern Southalpine) bent the primarily PFS and finally caused this fault system to be sinistrally offset by the NNE-SSW striking Giudicarie fault system in the Miocene. This last deformation stage (D5 after [2]) caused strong N-S shortening (~65 km) of the western Tauern Window in front of the Dolomites Indenter, accompanied by lateral extrusion towards the east of at least ~100 km involving major strike-slip faults (e.g., Inntal Fault, PFS, SEMP). W-E extension further led to the formation of the Katschberg and Brenner Normal Fault (on the eastern and western borders of the Tauern Window, respectively). The latter, perhaps in combination with slab break-off and mantle upwelling, led to rapid exhumation of the Tauern Window.

Balancing a cross-section is an excellent tool to analyze the kinematic evolution of mountain belts. Therefore, we collected a structural dataset along a N-S trending cross-section through the western Tauern Window based on the Brenner Base Tunnel profile [3]. Before balancing, however, basic assumptions have to be typically considered: (1) Whether plane-strain deformation is applicable, which means that no material should move lateral into or out of the cross-section plane (2) Conservation of the area (or volume), and (3) line-length should be preserved. Hence, such a balancing is not simply possible in the western Tauern Window because of the last deformation stage (D5 after [2]), when contemporaneous N-S shortening, W-E extension, and vertical uplift led to penetrative deformation and non-plane strain conditions, respectively. We focus on the restoration of the last deformation stage; first with plane-strain and second with non-plane, oblate strain. The results reveal the effect of the W-E extension on the nappe geometry in the footwall of the Brenner Normal Fault – a topic that is controversially discussed. This is the basis for further backward restoration that needs to incorporate all the tectonic movements out of the cross-section plane, and will be carried out as balancing in 3-D at a later stage of the project.

 

 

References

[1] Pomella, H. et al. (2011). International Journal of Earth Sciences, 100(8), 1827-1850.

[2] Schmid, S. M. et al. (2013). Swiss Journal of Geosciences, 106(1), 1-32.

[3] Brandner, R. et al. (2008). Geo Alp, 5, 165-174.

How to cite: Rudmann, J., Tanner, D. C., Stipp, M., and Pomella, H.: Balancing a cross-section through the western Tauern Window using non-plane strain, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-15666, https://doi.org/10.5194/egusphere-egu23-15666, 2023.