Accepted Manuscript Using laterally compatible cross sections to infer fault growth and linkage models in foreland thrust belts Hannah Watkins, Robert W.H. Butler, Clare E. Bond PII:
S0191-8141(17)30019-6
DOI:
10.1016/j.jsg.2017.01.010
Reference:
SG 3440
To appear in:
Journal of Structural Geology
Received Date: 31 August 2016 Revised Date:
20 January 2017
Accepted Date: 26 January 2017
Please cite this article as: Watkins, H., Butler, R.W.H., Bond, C.E., Using laterally compatible cross sections to infer fault growth and linkage models in foreland thrust belts, Journal of Structural Geology (2017), doi: 10.1016/j.jsg.2017.01.010. This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.
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Using laterally compatible cross sections to infer fault growth and linkage models in
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foreland thrust belts
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[email protected]
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Robert W. H. BUTLER¹
[email protected]
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Clare E. BOND¹
[email protected]
+44 (0) 1224 273879
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Hannah WATKINS¹*
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¹ School of Geosciences, Meston Building, University of Aberdeen, Aberdeen. AB24 3UE,
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SCOTLAND.
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Keywords: fold-thrust; laterally compatible cross-section; thrust growth; thrust linkage;
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displacement transfer; French Alps
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ACCEPTED MANUSCRIPT Abstract
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We investigate changes in shortening, displacement and fold geometry to understand the
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detailed along-strike structural variation within fold-thrust belts, and infer thrust growth and
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linkage mechanisms. Field observations from the Vercors in SE France are used to
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characterise deformation style in the region. Parallel cross sections are constructed, analysed
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and used to create shortening and thrust displacement profiles from the northern to southern
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Vercors. Sections show changes in structural style and shortening accommodation from
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thrust-dominated in the north to fold-dominated in the south. The total shortening distance in
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the Vercors does not change significantly along strike (3400-4650 m), however
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displacements along individual thrust zones do vary significantly and displacement profiles
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show a range in displacement gradients (16-107 m/km). Despite relatively simple shortening
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patterns in the Vercors, sections show a more complex 3D internal structure of the fold-thrust
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belt. Thrust displacements and geometries suggest both large-scale thrust zones and small-
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scale thrusts are soft linked, transferring displacement along strike through transfer zones.
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Short, soft-linked thrust segments indicate an intermediate stage of thrust growth and linkage,
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well documented for normal fault systems, which form prior to the formation of thrust
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branches and hard-linked displacement transfer.
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INSERT GRAPHICAL ABSTRACT HERE
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1. Introduction
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Dahlstrom (1969) presented a theoretical construction of gradual structural change in the
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along strike-geometry and displacement of thrust systems. In this he envisaged thrusts
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relaying displacement through an array (Figure 1a). Individual thrusts lost displacement and
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died out laterally in a predicable fashion – giving rise to the so-called “bow and arrow rule”
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(e.g. Elliott 1976) where the ratio of thrust map-half-length and maximum displacement is
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ACCEPTED MANUSCRIPT about 10:1. Since then there have been various attempts to quantify the amount of shortening
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in thrust belts and its along strike variations (e.g. Alvarez-Marron, 1995; Fermor, 1999;
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Apotria & Wilkerson, 2002; Torres Carbonell et al., 2013). These variations in shortening
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effect structural style, fold geometry, internal strain, thrust displacement, and other geometric
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and kinematic aspects of fold-thrust belts (e.g. Pérez-Estaún et al., 1997; Cooley et al., 2011;
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Torres Carbonell et al., 2013; Qayyum et al., 2015). The underlying causes of along strike
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variation in fold-thrust belt structure have been attributed to pre-existing basement and basin
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structure, changes in stratigraphy causing variation in rheological properties and variation in
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shortening closer to the hinterland in the internal zones (Woodward, 1988; Pérez-Estaún et
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al., 1997; Cooley et al., 2011; Qayyum et al., 2015; Rocha & Cristallini, 2015; Bhattacharyya
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& Ahmed, 2016; Cain et al., 2016). Here we develop studies of lateral variation in thrust belt
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structure using the notion of lateral compatibility to develop an array of mutually-compatible
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cross-sections and use these to examine lateral changes in displacement.
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INSERT FIGURE 1 HERE
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Despite decades of research on thrust systems, there are few systematic descriptions of
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variations in shortening and displacement through thrust arrays. This contrasts with research
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on normal fault systems where there is a well-established fault growth and linkage model
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(Childs et al., 1995). This model suggests that small faults initiate and, as they grow, the
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stress perturbations produced by the propagation of their process zones and their strain fields
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interact so they become soft linked. As displacements increase, fault splays may form,
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transferring displacement between established fault segments that become hard linked (Figure
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1b; Childs et al., 1995; Davis et al., 2005; Fossen, 2010). Based on this model developed for
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extensional faults, it would also be expected that displacement on a large fault is made up of
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slip on multiple hard-linked smaller fault segments that have branched to form a major fault
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zone (Figure 1c). However, in contrast with this understanding from normal faults, much of
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ACCEPTED MANUSCRIPT the early work on the three dimensional structure of thrust systems treated them as fully
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connected (hard-linked). In this fashion displacement has been interpreted to have transferred
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simply across branch lines (e.g. Diegel, 1986; Hossack, 1983). While these studies of finite
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fault patterns show predicable map patterns in restored state (e.g. Butler, 1985; Fermor,
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1999), they give little information on how the thrust array developed.
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The aim of this paper is to examine a thrust system that shows rather low displacements –
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focussing on the Vercors segment of the Sub-Alpine thrust belt of SE France. The intention is
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to establish whether systematic variations of displacement exist through the thrust array that
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might inform the growth of the system. Field data are used to highlight large-scale structural
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variation along strike in the fold-thrust belt. Cross sections are used to investigate how
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shortening varies along strike, and how fold geometry changes within a fold-thrust belt.
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Thrust zone displacements are also analysed to determine the detailed nature of how
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shortening may be distributed, how this may vary along strike, and how displacement is
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transferred within and between fault zones.
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2. Vercors field area
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The Vercors is a fold-thrust belt forming part of the Sub-Alpine Chains of France, which,
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along with the Jura, represent the most westward regional-scale deformation structure
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deformation associated with the Alps. The French Sub-Alpine Chains run for over 200 km
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from Chamonix in the NE to south of Grenoble in the SW (Figure 2a) and include the Haute-
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Giffre, Bornes, Bauges, Chartreuse and Vercors subdivisions (Moss, 1992a; Bellahsen et al.,
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2014). Thrusting and folding in the Vercors is thought to have occurred in the middle-late
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Miocene (Roberts, 1994; Bellahsen et al., 2014), between 10-6 Ma (Butler, 1987), and
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represents one of the youngest phases of Alpine deformation. Prior to Alpine mountain
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occurred during the mid-late Jurassic and regional subsidence occurred during the Cretaceous
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(Lemoine et al., 1986; Rudkiewicz, 1988; Butler, 1989). Although many associated normal
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faults are present in the Jurassic-Cretaceous succession, they are not thought to have been
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inverted during Alpine compression (e.g. Butler, 1989).
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INSERT FIGURE 2 HERE
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The Vercors forms a plateau elevated 1000-2300 metres above its foreland (regional) level,
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some 15-20 km across. At outcrop it is dominated by the “Urgonian” limestone (Hauterivian-
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Barremian) that is the youngest carbonate platform that built out from this part of the
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European continent towards the Tethyan ocean. The Urgonian is c 250-300m thick. It is
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underlain by older Cretaceous and Jurassic strata. These strata comprise of marls, shales,
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mudstones and competent limestones (Ramsay, 1963; Lemoine et al., 1986; Arnaud-Vanneau
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& Arnaud, 1990). The Mesozoic strata within the thrust belt form a marked mechanical
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multilayer, which is likely to have a significant control on present-day fold and thrust
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geometries. Collectively the stratigraphy achieves thicknesses in excess of 6 km in the east of
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the Vercors. However, well-data (see Butler 1987) for the foreland show the equivalent
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stratigraphy to be less than 3 km thick and dominated by carbonates. Thus the Mesozoic
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strata formed a broad westward-tapering wedge. During the Miocene this wedge was pushed
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westwards, along a basal detachment established in Triassic evaporites (Bayer et al., 1987;
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Mugnier et al., 1987; Roberts, 1991) and lower Jurassic shales, forming a high plateau offset
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by internal thrusts. The front of the Vercors appears to be pinned by pre-existing normal
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faults (so-called “faille de l’Isere” Butler, 1987, 1989).
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This study builds upon previous analyses of the Vercors. Butler (1987) presents a single
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balanced cross-section through the Vercors that established that plateau uplift and its internal
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being accommodated on a large backthrust that emerges to the east of the Drac Valley.
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Deville & Sassi (2005) presented a cross section through the Vercors, as part of a larger study
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on structural variation and thermal evolution of the Sub-Alpine Chains. As part of their
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regional study of the Subalps, Gratier et al. (1989) presented four cross-sections through the
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Vercors and demonstrated the southward decline in net displacement across the system. This
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is in contrast to the much higher displacements interpreted further north in the external
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Alpine thrust belt, where hard-linked interpretations have been applied (Butler, 1985; Deville
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et al., 1994; Affolter et al., 2008; Bellahsen et al., 2012; Bellahsen et al., 2014). The position
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of the Vercors, at the southern end of this declining chain, is ideal for testing the thrust
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linkage model proposed by Dahlstrom (1969), and the fault growth and linkage model
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originally established for normal fault systems (Figure 1b, Childs et al., 1995).
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3. Field observations
Field observations, photographs, sketches and bedding orientation data were collected in the
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field. We now describe some field relationships and fold geometries from different structural
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zones throughout the fold-thrust belt, which have been influential in regional cross section
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construction. The Vercors was divided into four main structural zones (see Figure 2b), which
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were chosen based on the positions of major thrusts, well-developed fold forelimbs marking
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the edge of large fold structures, or topographical features.
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3.1.Pont-en-Royans: thrust zone splays, backthrusts and disharmonic folding (structural zone 2)
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ACCEPTED MANUSCRIPT The frontal thrust of structural zone 2 (see Figure 2b) can be observed in the village of Pont-
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en-Royans where, instead of a single thrust surface, several thrust splays can be seen cutting
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up through folded Upper Cretaceous units (Figure 3a), defining a distributed thrust zone.
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From the outcrop, it is unclear how these thrusts link at depth. The fold geometry at Pont-en-
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Royans is also of particular interest due to its very short wavelength. Figure 3b shows a very
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tight fold to the east of the village; we have interpreted this as being caused by backthrusts
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branching off the main foreland-directed thrust at depth. Backthrusts can be seen elsewhere
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throughout the Vercors at a range of scales. The presence of backthrusts, particularly in fold
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forelimbs, have a significant control on resulting fold geometry and potentially damage
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distribution.
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INSERT FIGURE 3 HERE
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The tight fold geometry at Pont-en-Royans is associated with high density fracturing in the
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Urgonian Limestone, and small-scale, disharmonic folding in the Hauterivian shales below
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(Figure 3c). Disharmony in weak underlying layers (Hauterivian shales) appears to have
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allowed the Urgonian limestone to fold tightly, resulting in the geometry seen on Figure 3c.
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This difference in deformation style between more competent units such as the Urgonian and
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Upper Valanginian, and more incompetent units such as the Lower Valanginian and
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Hauterivian can be seen throughout the Vercors at a range of structural positions. The Pont-
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en-Royans structure is a good example of the relationship between deformation distribution
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in strong versus weak units in the Vercors, caused by rheological differences. The competent
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Urgonian Limestone defines the large-scale fold geometry, and much smaller scale folds
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form in the incompetent Hauterivian below in response to compression in the fold core.
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3.2.Petits Goulets: pre-existing structure in fold forelimbs (structural zone 2)
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ACCEPTED MANUSCRIPT The forelimb structure at Petits Goulets (see Figure 2b for location) is another example of the
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importance of backthrusts in fold-thrust belts. This forelimb exposure has a very different
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geometry to at Pont-en-Royans, despite being located just 1.5 km along strike to the south. In
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this example a prominent fault can be seen in cross section in the forelimb of the fold (Figure
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4a). We have interpreted this as a westward dipping backthrust that pre-dates the main
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folding and thrusting phase, based on the fold geometry and steep fault angle observed in the
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field. However Butler (1987) suggests the backthrust formed late and offsets the main
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eastward-dipping thrust. Initially the dip of this feature would have been much shallower, but
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it has since been rotated within the forelimb of a larger fold-thrust structure (see inset Figure
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4a). The presence of this backthrust has created small-scale folding within the fold forelimb,
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which causes structural complexity and could potentially affect the strain distribution within
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this region.
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3.3.Rencurel Thrust (structural zone 3)
The Rencurel Thrust zone marks the western edge of structural zone 3 (Figure 2b). Above the
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thrust is a well-developed forelimb of the Rencurel structure. It is best exposed in the Gorges
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de la Bourne (Figure 2b) where a gently westward-dipping forelimb can be seen in the
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Urgonian (Figure 4b). Minor backthrusting, associated with the Rencurel Thrust appears to
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have developed at this locality, but in this case the backthrust displacement is minimal
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meaning it does not have a significant impact on the fold geometry, unlike at Pont-en-Royans
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(Figure 3b).
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3.4.Plateau de Sornin (structural zone 3) 8
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is exposed in the Isere Valley, to the Plateau de Sornin, 1300 m above (see Figure 2b for
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location). The Urgonian flattens on the plateau before being cut by the Rencurel Thrust Zone
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5.5 km further west (Figure 5a). This geometry is quite different from anything seen further
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south in the Vercors and suggests a more complex thrust geometry at depth. Unlike further
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south where exposure of Urgonian Limestone suggest smooth, curved fold profiles, the
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Urgonian above Sassenage appears to have a kinked geometry with distinct hinge zones.
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3.5.Urgonian plateau and the Drac Valley (structural zones 3 and 4) The eastern edge of the Vercors is marked by the Urgonian plateau and ridge that runs
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continuously for over 50 km from St-Nizier-du-Moucherotte in the north to Chatillon-en-
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Diois at the southern edge of the Vercors (Figure 2). Urgonian bedding on the ridge dips
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moderately to the west, probably due to the presence of an underlying backthrust. The
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presence of such a continuous, high-elevation ridge suggests this backthrust must be a
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continuous feature, with relatively high displacement. The Drac Valley to the east of the ridge
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exposes multiple ridges of Jurassic sediments (Figure 5b, all dipping to the west. These ridges
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are also likely to have formed due to eastward vergent backthrusts. The backthrusts forming
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the Drac Valley structures and the Urgonian ridge probably splay off the large-displacement
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backthrust bounding the eastern edge of the Drac Valley, suggested by Butler (1989).
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4. Cross sections through the Vercors
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were constructed through the Vercors, from the Bas Dauphine in the west to the Drac Valley
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in the east (see Figure 2b). The orientations of the cross sections are ESE-WNW (110-290°).
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This orientation was chosen by calculating the average dip direction of surface bedding data
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(see Figure 2d), which is parallel to the thrust transport direction (Philippe et al., 1998). The
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six cross section lines were chosen in locations where exposure is good enough to analyse
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fold geometry in cross section, for example along WNW-ESE oriented gorges. The bedding
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data used to construct the cross sections was made up of our own field data, along with data
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from published geological maps of the Vercors (B.R.G.M. map sheets 1967, 1968, 1975,
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1978, 1983). Lithological unit boundaries and fault positions on the published maps
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(B.R.G.M. map sheets 1967, 1968, 1975, 1978, 1983) were also used for cross section
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construction. Bedding data was projected from between 1500-2000 m either side of each
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section line; the projection distance was chosen to ensure high enough data density on each
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cross section.
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Field observations have shown the variation in deformation style in different units must be
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taken into account when constructing a regional-scale cross section. In weaker units, such as
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the Hauterivian, the bedding orientation may relate either to large scale fold geometry, and
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therefore parallel stronger unit horizons, or to much smaller scale folds which are not
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representative of regional scale structure (e.g. Figure 3c). For this reason, where
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discrepancies between bedding data in competent and incompetent units are found, the data
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from the more competent unit is assumed to be more representative of larger scale structure,
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and
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Aptian/Maastrichtian) were restored using line-length restoration with a fixed pin at the
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WNW end of each cross section (e.g. Dahlstrom, 1969) to ensure they balanced and had
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realistic fault geometries.
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is
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Horizons
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4.1.Barbieres cross section (Figure 6) The Barbieres cross section is the most southerly section presented here. It runs through the
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south-central Vercors, across the wide Urgonian plateaus. The cross section features two
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high-displacement thrusts, both of which are towards the western end of the section (thrust
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zones 1 & 2, Figure 2b). Backthrusts splaying off eastward-dipping thrusts are also a key
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feature of this section; some are emergent and some have been interpreted at depth due to
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asymmetric folding at the surface. Structural zone 3 is bounded by the Rencurel Thrust Zone
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(thrust zone 3) which, in this section, is non emergent and instead is inferred at depth due to
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the presence of a well-developed, steeply dipping forelimb at the surface. The section also
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includes a large number of out-of-zone thrusts (i.e. thrusts located outside of the main thrust
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zones 1-3).
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INSERT FIGURE 6 HERE
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4.2.Beauregard-Baret cross section (Figure 7)
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The Beauregard-Baret section is 5.8 km north, along strike of the Barbieres section. It also
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features the two high-displacement thrusts at the western end, bounding structural zones 1
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and 2, as well as the well-developed forelimb above the non-emergent Rencurel thrust at the
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western edge of structural zone 3. Thrusting in this section is mainly foreland-directed, but
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there are some minor backthrust splays inferred in structural zone 1. The section contains a
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few out-of-zone thrusts, as well as minor folding in larger-scale fold backlimbs.
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4.3.Ste-Eulalie-en-Royans cross section (Figure 8) The Ste-Eulalie-en-Royans section is located 10 km north, along strike of the Beauregard-
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Baret section. There is no surface evidence for the main thrust controlling the development of
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the frontal structure (zone 1) seen on the Barbieres and Beauregard-Baret sections therefore it
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is assumed that displacement has decreased and this structure no longer exists as far north as
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the Ste-Eulalie-en-Royans line. The most striking feature of this section is the complication in
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the forelimb of the frontal structure (zone 2). This is the oversteepened backthrust described
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at Petits Goulets in section 3.2 (Figure 4a); based on the steep thrust dip this is interpreted as
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an older thrust with an eastward transport direction that has later been oversteepened by the
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formation of a larger forelimb. The presence of this backthrust structure has been attributed to
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a buttressing effect (as suggested by Butler, 1987) due to the presence of a basement-
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involved normal fault at the level of the regional detachment. The buttressing effect has been
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described by Welbon (1988) and Butler (1989), where a rigid obstacle at depth (i.e. the
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basement fault scarp) acts as a buffer, inhibiting propagation of a regional detachment layer
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towards the foreland. In response to this a hinterland-directed thrust is inferred to have
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propagated up from this buffering obstacle at depth. Alternatively this feature could be a
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‘rabbit-ear’ structure, in which the hinterland-dipping thrust and the backthrust are coeval;
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the backthrust ramps out of a bedding slip surface, forming asymmetrical fault-propagations
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folds within the foreland-dipping fold forelimb (Neely & Erslev, 2008). Since the major
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eastward-dipping thrust is not exposed it is not possible to distinguish between the two
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interpretations. The Ste-Eulalie section also reflects the tight fold geometry above thrust zone
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2 seen at Pont-en-Royans (Figure 3b). The other key feature of the St-Eulalie section is the
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Rencurel Thrust zone which marks the western end of structural zone 3. On this section it is
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an emergent feature with several major thrust splays and no significant fold forelimb
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development.
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INSERT FIGURE 8 HERE
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4.4. St-Romans cross section (Figure 9) 6.7 km north along strike from the Ste-Eulalie-en-Royans section line is the St-Romans cross
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section. There is little field evidence for backthrusting in the forelimb of the frontal structure,
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as seen on the Ste-Eulalie-en-Royans section; instead a simpler, steeply dipping forelimb is
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seen on the St-Romans section. The Rencurel Thrust zone (thrust zone 3) on the western edge
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of structural zone 3 is again emergent on this cross section, with both foreland and hinterland
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directed thrust splays. A major feature of this cross section is a high-displacement, westward-
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dipping backthrust at the eastern end of the section. This thrust is probably associated with
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the westward dip of bedding on the Urgonian Plateau.
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INSERT FIGURE 9 HERE
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4.5.Cognin-les-Gorges cross section (Figure 10) The Cognin-les-Gorges cross section lies 7.8 km north, along strike from the St-Romans
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section. This cross section features rotated and steepened backthrusts in the forelimb of the
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frontal structure, similar to that seen at Petits Goulets (Figure 4a) and on the St-Eulalie cross
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section (Figure 8). The deep structure of this feature has been interpreted in the same way as
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further south, initiating at a basement fault scarp at depth. The Rencurel thrust zone (thrust
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zone 3) in this cross section is represented as a single structure rather than fault splays, unlike
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further south. The eastern edge of the Vercors is again marked by a high-displacement,
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westward-dipping backthrust below the Urgonian Plateau, presumably associated with
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backthrusting in the Drac Valley (structural zone 4).
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INSERT FIGURE 10 HERE
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4.6.Sassenage cross section (Figure 11) The Sassenage cross section is the most northerly of the six regional sections presented, and
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is located 11 km along strike, to the north of the Cognin-les-Gorges section. It runs through
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the narrow northern tip of the Vercors, and is therefore a relatively short section. The most
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prominent feature of the Sassenage section is the large displacement Rencurel thrust zone
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(thrust zone 3) that emplaces the Hauterivian and Valanginian on top of Miocene rocks.
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Another distinctive feature of this cross section has already been described in section 3.4; the
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Urgonian limestone of Plateau de Sornin, which rises sharply from the Valley bottom (Figure
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5a). This geometry has been interpreted in the cross section as being associated with a flat-
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ramp-flat thrust geometry at depth. Further east towards the hinterland a series of closely
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spaced thrusts that splay off a major thrust at depth can be seen. These low displacement
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thrusts are associated with well-developed forelimbs, unlike the large-displacement thrust
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further west, which has no significant fold forelimb developed.
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INSERT FIGURE 11 HERE
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4.7.Deep structure, the Drac Valley and pre-existing, Mesozoic normal faults
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On each of the cross sections presented (Figures 6-11), a large scale (>1 km displacement)
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normal fault is shown to offset the top basement horizon; this is the Faille de L’Isere fault.
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Butler (1987, 1989) interpreted this fault as the main control on the position of the frontal
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thrust, suggesting that the lower detachment of the fold-thrust belt was unable to propagate
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westwards from the Triassic evaporites in the Faille de L’Isere hangingwall through to the
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ACCEPTED MANUSCRIPT much stronger basement in the footwall. Instead the detachment deflected upwards over the
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basement fault scarp of the Faille de L’Isere and emerged as the frontal thrust at the surface,
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on the western margin of the Vercors. This interpretation has been used in this paper to infer
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a simple model for the deep structure. Pre-existing literature has also been used to infer the
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structure to the east of the cross sections; beyond the main field area. Bedding data from the
340
Urgonian limestone to the west of the Drac Valley shows a moderate dip to the west,
341
suggesting a backthrust may be present at depth.
342
In the Drac Valley a series of westward-dipping dip panels in Jurassic units can be seen
343
(Figure 5b), also indicating westward dipping backthrusts at depth. These are probably linked
344
to the large displacement backthrust suggested by Butler (1987). Backthrusting in the Drac
345
Valley has been represented as a single, large fault on the Sassenage cross section (Figure 11)
346
although in reality the structure is probably more complex, with multiple thrust splays.
347
The other main structural feature of the cross sections is normal faults. Each of the cross
348
sections contains several eastward or westward-dipping normal faults, most of which are
349
thought to pre-date thrusting and probably relate to Mesozoic rifting during opening of the
350
Tethys Ocean. The normal faults on the cross section are shown to be offset by younger
351
thrusts, and none are shown to have been reactivated or inverted. This is because there is little
352
field evidence along the lines of section to suggest the pre-existing normal faults significantly
353
influence fold-thrust structure; instead they appear to have behaved passively during
354
thrusting. Other authors report localised interaction between pre-existing normal faults and
355
younger thrusts in the Vercors, for example Butler (1987, 1989) shows an example where a
356
normal fault has juxtaposed the strong, competent Urgonian limestone alongside weaker,
357
incompetent Hauterivian shales. This horizontal change in lithology meant that a thrust could
358
not easily propagate from the weak shales into the strong limestones, so instead, intense,
359
localised folding occurred, with potential reactivation of the normal fault in the hangingwall
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of the newly formed thrust, a phenomenon termed buttressing (Welbon, 1988). Although
361
evidence for buttressing is seen in Mesozoic rocks in the Vercors, it appears to be quite rare
362
and is therefore not represented on the cross sections.
364
5. Along strike variation
365
5.1.Shortening and total thrust displacement
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Regional cross sections were analysed to determine changes in fold geometry, thrust
368
displacement and shortening. Displacements on each thrust were measured at the top
369
Urgonian horizon for the six regional cross sections (Figures 6-11), along with total
370
shortening distance and shortening percentage. Figure 12 shows how these estimates for
371
shortening, along with the total thrust displacement for each cross section, varies along strike.
372
The graph patterns for total thrust displacement and shortening distance are quite similar
373
(Figure 12a), indicating that, overall, the majority of shortening is accommodated by
374
thrusting and brittle deformation rather than folding. Both the total thrust displacement and
375
shortening distance increase from Sassenage to St-Romans, before decreasing in the Ste-
376
Eulalie-en-Royans section and increasing again to the Barbieres section. On the southern two
377
cross sections (Beauregard-Baret and Barbieres) the shortening distance becomes larger than
378
the total thrust displacement, probably due to the presence of well-developed folds on lower
379
displacement thrusts (Figures 10 &11).
380
INSERT FIGURE 12 HERE
381
The shortening percentage has also been calculated for each cross section and plotted on
382
Figure 12b. This value is commonly used to compare the amount of compression and strain in
383
thrust belts. Figure 12b shows the shortening percentage trend along strike is different to that
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ACCEPTED MANUSCRIPT of shortening distance (Figure 12a). The three northern sections (Sassenage, Cognin-les-
385
Gorges and St-Romans, Figures 6-8) have the highest shortening values (11-14%) and the
386
three southern sections (Ste-Eulalie-en-Royans, Beauregard-Baret and Barbieres, Figures 9-
387
11) have the lowest shortening values (5-10%). Shortening percentages suggest the two most
388
southerly sections underwent less shortening that the two most northerly sections, however
389
the shortening distance values suggest the opposite (Figure 12a). The reason for this
390
discrepancy is that the two southerly cross sections are much longer than the northern
391
sections. If you compare two cross sections with the same shortening distance but different
392
lengths, the shorter section will appear to have higher shortening percentage than the longer
393
section. Clearly when analysing thrust belt shortening using cross sections of different
394
lengths it is important to use the actual shortening distance value rather than shortening
395
percentage, for the reason shown above.
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5.2.Thrust zone displacement
Three main thrust zones were identified in the study area; zone 1 is the frontal thrust zone in
399
front of the Beauregard-Baret structure (structural zone 1). It can be traced along the
400
mountain front in the southern Vercors. Zone 2 is the thrust zone beneath the Pont-en-Royans
401
structure (structural zone 2), and zone 3 is the Rencurel Thrust zone (bounding structural
402
zone 3) that merges with the Voreppe Thrust in the southern Chartreuse (Figure 2). Total
403
displacements for each thrust zone were calculated at the top Urgonian horizon for each cross
404
section to determine whether shortening variations along strike occur along a single thrust
405
zone or are due to consistent changes in displacement within all three main thrust zones.
406
Displacement variations along strike on individual thrusts were not analysed because at the
407
surface thrusts are relatively short and usually do not intersect more than one cross section.
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ACCEPTED MANUSCRIPT INSERT FIGURE 13 HERE
409
Figure 13 shows how thrust zone displacements vary along strike, as well as on out-of-zone
410
thrust in between major thrust zones. Thrust zone 1 only appears on the two most southerly
411
sections, where its displacement is 900-1100 m. This sudden increase in displacement
412
between the Ste-Eulalie-en-Royans and Beauregard-Baret sections is reflected in the fold
413
geometry; on the northern banks of the Isère river no fold is present and topography is
414
relatively flat; 3km to the south of this a large fold with a well-developed, steeply dipping
415
forelimb rising 500 m above the river in the Urgonian. Thrust zone 2 is not present on the
416
Sassenage section; its displacement gradually increases from the Cognin-les-Gorges section
417
to the south at a much steadier rate than thrust zone 1. Thrust zone 2 remains a relatively low
418
displacement zone throughout the region. Displacement on thrust zone 3 is high in the north,
419
and decreases gradually to the south where it is interpreted to have zero displacement in the
420
Urgonian; the thrust is still present at depth in the Jurassic succession. On the southern two
421
cross sections thrust zone 3 is represented at the surface as a well-developed fold with a
422
steeply dipping forelimb. This fold geometry contrasts with sections further north along
423
thrust zone 3, where thrust displacement in the Urgonian is much higher, but folds are less
424
well developed and have only shallowly dipping forelimbs. Out-of-zone displacement in
425
between thrust zones 1, 2 and 3 is relatively low in the north, increasing significantly to the
426
south.
427
The patterns of thrust displacement variation in the three thrust zones and out-of-zone are a
428
good example of how displacement may be transferred along strike in a fold-thrust belt. In
429
the north thrust zone 3 is clearly the dominant one, accommodating the majority of
430
shortening in the Vercors. As displacement within thrust zone 3 decreases to the south, both
431
the out-of-zone and thrust zone 1 displacement gradually increase to accommodate
432
displacement loss from zone 3. Displacement in thrust zone 2 remains low throughout the
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ACCEPTED MANUSCRIPT Vercors, indicating that it has little influence on along strike shortening variation (Figure 13).
434
Data presented on Figure 13 shows that variation in shortening along strike is accommodated
435
along certain zones rather than being due to consistent changes in displacement on all thrusts.
436
Figure 13 also shows that displacement in all three thrust zones, as well as out-of-zone
437
displacement is low on the Ste Eulalie section, causing a low shortening distance on Figure
438
12a.
439
6. Discussion
441
6.1 Shortening and structural style of the Vercors
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The six cross sections presented in section 4 suggest shortening in the Vercors is up to 5 km;
443
this is in contrast to other authors who estimate more shortening such as Butler (1989) and
444
Philippe et al. (1998) who both calculate 10 km of shortening and Bellahsen et al. (2014) who
445
suggests that the value is around 28 km. The reason for the differences in shortening
446
estimates is because the cross sections of Butler (1989) and Bellahsen et al. (2014) extend
447
much further east than our own. In this paper we focus mainly on the deformation in the
448
central Vercors (i.e. structural zones 1-3, see Figure 2b), however Butler’s (1989) estimate
449
includes large-scale backthrusting present in the Drac Valley to the east of our sections.
450
Figure 5b showed west-dipping ridges of Jurassic units which are probably the backlimbs of
451
folds formed above backthrusts. The topographic relief of these features is quite high, which
452
might indicate high thrust displacement and significant shortening on these structures, which
453
could accommodate any ‘missing’ shortening distance.
454
Total thrust displacement curves (Figure 12a) suggest a gradual increase in displacement to
455
the south from the Sassenage section to the St-Romans section, before decreasing on the Ste-
456
Eulalie-en-Royans section and increasing again in the Beauregard-Baret and Barbieres
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19
ACCEPTED MANUSCRIPT sections. This rather complicated pattern can be explained simply by the presence of
458
backthrusts at the eastern end the Cognin-les-Gorges and St-Romans sections (Figures 9 &
459
10); if the displacements of these two thrusts were removed from the thrust displacement
460
graph (Figure 12a), there would be little change in total thrust displacement along strike, with
461
the exception of the Ste-Eulalie-en-Royans section, indicating relatively consistent
462
deformation along the length of the Vercors.
463
The Ste-Eulalie-en-Royans section (Figure 8) is anomalous to the overall shortening patterns;
464
the total thrust displacement and total shortening distance (Figure 12a) are much lower than
465
on adjacent sections. If shortening did decrease suddenly around the Ste-Eulalie-en-Royans
466
section line we might expect to see localised faults and folds forming oblique to the main
467
thrusts zones, deviations in the orientation of these thrust zones, and more intense
468
deformation in this region. These features would be required to accommodate the sudden
469
change
470
The map patterns of thrust zones 1-3 show continuous, parallel features that do not show any
471
significant changes around the Ste-Eulalie-en-Royans section line. This would suggest that
472
the total shortening distance along the thrust belt is relatively consistent with no sudden
473
changes. This suggests that a significant amount of shortening (c. 2500-3000 m) is absent
474
from the Ste-Eulalie-en-Royans cross section (Figure 8). Displacements on individual thrusts
475
on this section line are well constrained by map patterns and field observations so the
476
‘missing’ shortening suggests at least one major compressional feature is absent from this
477
section. The absence of this feature was inferred by analysing and comparing cross sections
478
along strike; when observed in isolation this cross section balances when restored (Figure 8)
479
and appears as a structurally valid interpretation. Along strike cross section analysis is not
480
only important for determining large scale structural trends, but can also be used as a tool to
481
validate structural interpretation.
shortening
distance.
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ACCEPTED MANUSCRIPT The patterns for total thrust displacement and shortening distance on Figure 12a also indicate
483
a change in the nature of deformation along strike; in the north thrust displacement and
484
shortening are similar, whereas in the south shortening distance is considerably higher than
485
thrust displacement. This relationship reflects a change in structural style, as exemplified by
486
the Rencurel thrust zone (thrust zone 3). In the north brittle deformation dominates; thrust
487
displacement is high but folds are poorly developed. In the south, around the Beauregard-
488
Baret and Barbieres sections, the thrust has zero displacement at the surface but folds are well
489
developed. A similar amount of shortening is accommodated along strike but structural
490
geometries are very different.
491
There are several reasons behind this change in fold geometry, including variation in burial
492
depth and deformation conditions; rate of deformation; variation in lithology; change in thrust
493
kinematic mechanism, variation in detachment characteristics and proximity to the thrust tip.
494
The change from thrust-dominated shortening in the north to fold-dominated shortening in
495
the south could be explained by deeper burial depths, and therefore warmer deformation
496
conditions in the south. Investigations into the organic maturation and tectonic loading by
497
Moss (1992a, 1992b) suggest the southern Sub-Alpine chains (Vercors and Chartreuse) have
498
undergone shallower burial than the northern chains (Haute-Giffre and Aravis massifs),
499
however data was not collected south of the Gorges de la Bourne in the Vercors (Figure 2b),
500
meaning little is known about deformation conditions in the southern Vercors, around the
501
Beauregard-Baret and Barbieres sections.
502
Variation in the rate of deformation may also cause changes in structural style; slower rates
503
might allow well-developed folding without brittle failure to occur in the south, whereas
504
faster rates might be the cause of brittle thrusting and poorly developed folds in the north.
505
Although variation in deformation rate could be behind the observed structural variation,
506
there is no other evidence for it so it is an unlikely cause. A major change in lithology would
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ACCEPTED MANUSCRIPT lead to changes in the rheological behaviour of the deforming rocks, and therefore alter the
508
structural style. However, once again there is little evidence for significant changes in
509
lithology in the Vercors that might cause these changes in structural style.
510
It is probable that the variation in fold geometry could be caused by changes in kinematic
511
thrusting mechanism along strike and proximity to the thrust tip. The change from a high
512
displacement thrust in the north to a non-emergent thrust in the south suggests the Rencurel
513
Thrust (thrust zone 3) probably dies out south of the cross sections so the folds on the
514
Beauregard-Baret and Barbieres sections (Figures 10 & 11) are likely to be much closer to
515
the thrust tip than the northern sections. The sections also show a difference in thrust
516
propagation from north to south. In the northern sections (Figures 6-9) the Rencurel Thrust is
517
shown to have propagated all the way through the Upper Cretaceous whereas on the southern
518
two sections (Figures 10 & 11) the thrust tip is in the Jurassic or Lower Cretaceous. The
519
difference in structural geometry might relate to the thrust propagation rate: for the same
520
amount of shortening the thrust in the south may have had a slower thrust propagation rate,
521
giving time for the fold to develop in the hangingwall in front of the thrust tip, as in the
522
trishear mechanism (Erslev, 1991). The thrust in the north may have propagated up section
523
much faster, giving little time for folding in the hangingwall, as in the fault-parallel flow or
524
fault-bend-fold mechanisms (Suppe, 1983; Egan et al., 1997; Kane et al., 1997). It has also
525
been suggested (e.g. by Philippe et al., 1998) that the nature of the lower detachment to the
526
fold-thrust belt changes along strike; in the northern Vercors the detachment is thought to be
527
in marls and shales, whereas in the south thrusts are thought to detach in a salt horizon
528
(Philippe et al., 1998). The lithology of a detachment has been found to control the structural
529
style of a fold-thrust belt; frictional detachments create thrusts with asymmetric folds whereas
530
viscous detachments (such as salt) create more symmetric structures with less faulting (e.g.
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ACCEPTED MANUSCRIPT 531
Ruh et al., 2012). The variation in detachment lithology could therefore influence structural
532
style variations in the Vercors.
533
6.2 Thrust linkage and growth Analysing displacements in individual thrust zones has shown variations from north to south.
535
Thrust zone displacement curves (Figure 13) show evidence for displacement transfer along
536
strike; zone 3 dominates in the north and decreases to the south, whereas displacement in
537
zone 1 and on out-of-zone thrusts increases to the north. Displacement in thrust zone 2
538
appears not to change significantly along strike. These patterns can be compared with the
539
model of Dahlstrom (1969) showing thrusts relaying displacements through an array (Figure
540
1a). In the model the total shortening is equal on all sections, suggesting that thrust belt
541
structure is relatively simple on a large scale. However, displacement on individual thrusts
542
varies significantly, which creates structural complexity within the thrust belt. Dahlstrom’s
543
model has been reconstructed for the Vercors (Figure 14), showing that displacement loss in
544
thrust zone 3 to the south is accommodated by displacement gain in thrust zone 1. Thrust
545
zones are not isolated systems, but instead these large features are soft linked. Displacement
546
is transferred between thrusts zones to maintain a relatively constant shortening distance
547
along strike. Although thrusting in the Vercors occurs on a much smaller scale to the
548
Canadian Rockies, on which Dahlstrom’s (1969) thrust transfer zone model was based, we
549
can see the same mechanisms for large-scale thrust linkage.
550
INSERT FIGURE 14 HERE
551
The relatively low thrust displacements in the Vercors has allowed us to analyse the
552
mechanisms of thrust growth and linkage. Map patterns within thrust zones show them to be
553
made up of multiple short thrust segments rather than single, long thrust structures. These
554
short thrust segments within individual thrusts zones do not branch off one-another and
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ACCEPTED MANUSCRIPT appear isolated on the geological map (Figure 2b). These patterns suggests that thrust zones
556
must be made of short, soft linked thrusts, which transfer displacement along strike and
557
contribute towards the total thrust zone displacement. These observations suggest the
558
established model for normal fault growth and linkage (Childs et al., 1995, Figure 1b-c) could
559
also be applied to thrust systems. The soft linked thrusts observed in the Vercors are an
560
under-reported thrusting style, which may represent the early stages of thrust development. In
561
other thrust belt examples (e.g. Diegel, 1986; Hossack, 1983) high displacement thrusts are
562
shown to transfer displacement across branch lines (i.e. they are hard-linked). If the fault
563
growth model (Childs et al., 1995) for extensional systems can be applied to thrust belts, then
564
we have might expected thrust branches to have formed within the Vercors thrust zones, had
565
displacements increased, leading to hard linked, through-going thrust zones.
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7. Conclusions
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567
Analysis of parallel cross sections constructed through the Vercors fold-thrust belt has shown
569
the total shortening distance is relatively consistent, however the internal structure is more
570
complex. Cross sections show changes in structural style along strike and significant
571
variation in individual thrust zone displacement with displacement gradients varying
572
significantly from 16-107 m/km. Large-scale thrust zone displacement patterns suggest they
573
are soft linked; as displacement decreases in one zone, it increases in another to maintain a
574
constant total shortening within the fold-thrust belt. Individual thrust zones are comprised of
575
short, soft-linked thrust segments. They probably represent an intermediate stage in thrust
576
development at low displacements (up to 2000 m in the Vercors), where thrust splays have
577
not yet formed to create larger, through-going thrust structures, as seen in other global thrust
578
belt examples, such as the Rockies, where thrust displacements are much higher (over 10 km,
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ACCEPTED MANUSCRIPT 579
Price, 1981). The question is are the thrust displacement gradients and linkage patterns in the
580
Vercors applicable to carbonate thrust belts in general or are they dependent on the specific
581
nature of the deforming multiplayer?
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Acknowledgements
584
This research is partially funded by a CGG-financed pathfinder project, and formed part of a
585
study by the Fold-Thrust Research Group at the University of Aberdeen, co-funded by
586
InterOil, Oil Search and Santos. We also thank Nicolas Bellahsen and Stefano Tavani for
587
constructive reviews.
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ACCEPTED MANUSCRIPT Fermor, P., 1999. Aspects of the three-dimensional structure of the Alberta Foothills and
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Front Ranges. GSA Bulletin, 111, 3, 317-346.
674
Fossen, H., 2010. Structural Geology. Cambridge University Press.
675
Gratier, J-P., Ménard, G. & Arpin, R., 1989. Strain-displacement compatibility and
676
restoration of the Chaines Subalpines of the western Alps. In: Alpine Tectonics edited by
677
Coward, M. P., Dietrich, D. & Park, R. G. Geological Society, London, Special Publications,
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45, 65-81.
679
Hossack, J. R., 1983. A cross-section through the Scandinavian Caledonides constructed with
680
the aid of branch-line maps. Journal of Structural Geology, 5, 2, 103-111.
681
Kane, S. J., Williams, G. D., Buddin, T. S., Egan, S. S., and Hodgetts, D., 1997, Flexural-
682
slip based restoration in 3D, a new approach. AAPG Annual Convention Official
683
Program, A58.
684
Lemoine, M., Bas, T., Arnaud-Vanneau, A., Arnaud, H., Dumont, T., Gidon, M., De
685
Graciansky, P. C., Rudkiewicz, J. L., Megard-Galli, J. & Tricart, P. 1986. The continental
686
margin of the Mesozoic Tethys in the western Alps. Marine Petroleum Geology, 3, 179-199.
687
Moss, S., 1992a. Organic maturation in the French Subalpine Chains: regional differences in
688
burial
689
history and the size of tectonic loads. Journal of the Geological Society, London, 149, 503-
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515.
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Moss, S. J., 1992b. Burial diagenesis, organic maturation and tectonic loading in the French
692
subalpine chains, S.E. France, Durham theses, Durham University.
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Mugnier, J. L., Arpin, R. & Thouvenot, F., 1987. Coupes Equilibrees a travers le massif sub
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alpine de la Chartreuse. Geodinamica Acta, Paris, 1, 125-137.
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ACCEPTED MANUSCRIPT Neely, T. G. & Erslev, E. A., 2008. The interplay of fold mechanisms and basement
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weaknesses at the transition between Laramide basement-involved arches, north-central
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Wyoming, USA. Journal of Structural Geology, 31, 1012-1027.
698
Qayyum, M., Spratt, D. A., Dixon, J. M. & Lawrence, R. D., 2015. Displacement transfer
699
from fault-bend to fault-propagation fold geometry: An example from the Himalayan thrust
700
front. Journal of Structural Geology, 77, 260-276.
701
Pérez-Estaún, A., Alvarez-Marrón, J., Brown, D., Puchkov, V., Gorozhanina, Y. & Baryshev,
702
V., 1997. Along-strike structural variations in the foreland thrust and fold belt of the southern
703
Urals. Tectonophysics, 276, 265-280.
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Philippe, Y., Deville, E. & Mascle, A., 1998. Thin-skinned inversion tectonics at oblique
705
basin margins: example of the western Vercors and Chartreuse Subalpine massifs (SE
706
France). In: Cenozoic Foreland Basins of Western Europe edited by Mascle, A.,
707
Puigdefàbregas, C., Luterbacher, H. P. & Fernàndez, M. Geological Society of London,
708
Special Publications, 134, 239-262.
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Price, R. A., 1981. The Cordilleran foreland thrust and fold belt in the southern Canadian
710
Rocky Mountains. In: Thrust and Nappe Tectonics edited by McClay, K.R. & Price, N.J.
711
Geological Society, London, Special Publications, 9, 427-448.
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Ramsay, J. G., 1963. Stratigraphy, Structure and Metamorphism in the Western Alps.
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Proceedings of the Geological Association, 74, 3, 357-391.
714
Roberts, G., 1991. Structural controls on fluid migration through the Rencurel thrust zone,
715
Vercors, French Sub-Alpine Chains. In: Petroleum Migration edited by England, W. A. &
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Fleet, A. J. Geological Society, London, Special Publications, 59, 245-262.
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Roberts, G. P., 1994. Displacement localization and palaeo-seismicity of the Rencurel Thrust
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Zone, French Sub-Alpine Chains. Journal of Structural Geology, 16, 5, 633-646.
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ACCEPTED MANUSCRIPT Rocha, E. & Cristallini, E. O., 2015. Controls on structural styles along the deformation front
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of the Subandean zone of southern Bolivia. Journal of Structural Geology, 73, 83-96.
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Suppe, J., 1983. Geometry and kinematics of fault-bend folding. American Journal of
722
Science, 283, 684-721.
723
Rudkiewicz, J. L., 1988. Quantitative subsidence and thermal structure of the European
724
continental margin of the Tethys during Early and Middle Jurassic times in the Western Alps
725
(Grenoble-Briancon transect). Bulletin de la Société Géologique de France, 4, 4, 623-632.
726
Ruh, J. B., Kaus, B. J. P. & Burg, J-P., 2012. Numerical investigation of deformation
727
mechanics in fold-thrust belts: Influence of rheology of single and multiple décollements.
728
Tectonics, 31, TC3005.
729
Torres Carbonell, P. J., Dimieri, L. V. & Olivero, E. B., 2013. Evaluation of strain and
730
structural style variations along the strike of the Fuegian thrust-fold belt front, Argentina.
731
Andean Geology, 40, 3, 438-457.
732
Welbon, A., 1988. The influence of intrabasinal faults on the development of a linked thrust
733
system. Geologische Rundschau, 77, 1-11.
734
Woodward, N. D., 1988. Primary and secondary basement controls on thrust sheet
735
geometries. Geological Society of America Memoirs, 171, 353-366.
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Figure captions
739
Figure 1: a) Dahlstroms (1969) model for soft-linked thrusts; as displacement on one thrust
740
decreases, it must increase on another to maintain a constant shortening distance along the
741
fold-thrust belt. In this case displacement on thrust A increases towards the top, displacement
742
on thrust C decreases towards the top and the maximum displacement on thrust B is on the
31
ACCEPTED MANUSCRIPT central section. b) Fault growth and linkage model. At stage 1 the stress and strain fields of
744
two small faults do not interact; the faults are unlinked. At stage 2 the faults have grown and
745
their dispalcements increased; their stress and strain field begin to interact so they are soft
746
linked. By stage 3 the thrust displacement has increased and a thrust splay has formed,
747
linking the two faults; the faults are now hard linked. b) High displacement thrust fault zones
748
may be expected to be made up of multiple, smaller fault segments. Total thrust zone
749
displacement (dashed line) is made up of slip on individual small fault segments or series of
750
linked fault segments (adapted from Fossen, 2010).
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Figure 2: a) Location map and simplified geological map of the French Sub-Alpine Chains in
753
SE France. Adapted from Moss, 1992a. b) Geological map of the Vercors showing the
754
boundaries of major structural zones (dashed lines) and cross section traces, adapted from
755
B.R.G.M. map sheets 1967, 1968, 1975, 1978, 1983. c) Key to geological map and cross
756
sections (Figures 6-11). d) Equal area stereonet showing contoured poles to bedding for the
757
Jurassic-Cretaceous succession (using a 0.75 % contour interval). The orientation of the best
758
fit section plane is derived by calculating the average bedding dip direction using Move
759
software.
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Figure 3: a) Looking north onto eastward dipping thrust splays in the forelimb of the fold at
762
Pont-en-Royans. b) Looking NNE from Ste-Eulalie-en-Royans to the tight Urgonian fold at
763
Pont-en-Royans, possibly caused by the presence of west-dipping backthrusts causing a pop-
764
up structure. c) Looking north into the fold core at Pont-en-Royans. Small-scale folding in the
765
Hauterivian is probably caused by compression within the fold core. See Figure 2 for
766
locations.
767
32
ACCEPTED MANUSCRIPT Figure 4: a) Looking north from Petits Goulets; a steep, west-dipping backthrust probably
769
formed early during Vercors deformation, and was later rotated as the larger fold forelimb
770
developed. Inset: suggested evolution of the Petits Goulets structure: stage 1: backthrusting
771
followed by rotation of the resultant fold due to folding above a larger, eastward-dipping
772
thrust at depth; stage 2: eastward-dipping thrust offsets the older backthrust . b) The Urgonian
773
fold forelimb above the Rencurel Thrust in the Gorges de la Bourne; backthrusts are seen
774
cutting through the fold but they do not alter fold geometry significantly. See Figure 2 for
775
location.
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Figure 5: a) Looking south from the southern Chartreuse onto the northern Vercors. The
778
Urgonian shows a clear kinked geometry as it rises from the Valley bottom to the Plateau de
779
Sornin, possible due to a kinked thrust geometry at depth. b) Looking SE from Pic St-Michel
780
to the Drac Valley. Forested ridges represent the dip panels of Jurassic folds, probably caused
781
by west-dipping backthrusts at depth. See Figure 2 for locations.
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Figure 6: Top: Barbieres cross section running WNW-ESE from the Bas Dauphine (BD) to
784
the Drac Valley (zone 4). F: Faille de L’Isere fault. See Figure 2b for section trace line.
785
Bottom: cross section following line-length restoration. Line length restoration has been
786
applied only to the top Jurassic-Cretaceous horizons; the internal structure of the Jurassic and
787
basement is not restored.
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Figure 7: Top: Beauregard-Baret cross section running WNW-ESE from the Bas Dauphine
790
(BD) to the Drac Valley (zone 4). F: Faille de L’Isere fault. See Figure 2b for section trace
791
line. Bottom: cross section following line-length restoration. Line length restoration has been
33
ACCEPTED MANUSCRIPT 792
applied only to the top Jurassic-Cretaceous horizons; the internal structure of the Jurassic and
793
basement is not restored.
794
Figure 8: Top: Ste-Eulalie-en-Royans cross section running WNW-ESE from the Bas
796
Dauphine (BD) to the Drac Valley (zone 4). F: Faille de L’Isere fault. See Figure 2b for
797
section trace line. Bottom: cross section following line-length restoration. Line length
798
restoration has been applied only to the top Jurassic-Cretaceous horizons; the internal
799
structure of the Jurassic and basement is not restored.
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Figure 9: Top: St-Romans cross section running WNW-ESE from the Bas Dauphine (BD) to
802
the Drac Valley (zone 4). F: Faille de L’Isere fault. See Figure 2b for section trace line.
803
Bottom: cross section following line-length restoration. Line length restoration has been
804
applied only to the top Jurassic-Cretaceous horizons; the internal structure of the Jurassic and
805
basement is not restored.
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Figure 10: Top: Cognin-les-Gorges cross section running WNW-ESE from the Bas Dauphine
808
(BD) to the Drac Valley (zone 4). F: Faille de L’Isere fault. See Figure 2b for section trace
809
line. Bottom: cross section following line-length restoration. Line length restoration has been
810
applied only to the top Jurassic-Cretaceous horizons; the internal structure of the Jurassic and
811
basement is not restored.
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Figure 11: Top: Sassenage cross section running WNW-ESE from the Bas Dauphine (BD) to
814
the Drac Valley (zone 4). F: Faille de L’Isere fault. See Figure 2b for section trace line.
815
Bottom: cross section following line-length restoration. Line length restoration has been
34
ACCEPTED MANUSCRIPT 816
applied only to the top Jurassic-Cretaceous horizons; the internal structure of the Jurassic and
817
basement is not restored.
818
Figure 12: a) Shortening distance and total thrust displacement profiles showing along strike
820
variations from north to south. A good correlation between the two lines in the north shows
821
thrusting accommodates the majority of shortening; in the south shortening distance is higher
822
than thrust displacement indicating more folding is accommodating shortening. b) Shortening
823
percentage profile suggesting a general decrease in shortening from north to south. S:
824
Sassenage section; C: Cognin-les-Gorges section; SR: St-Romans sections; SE: Ste-Eulalie-
825
en-Royans section; BB: Beauregard-Baret section; B: Barbieres section. Shortening
826
percentages have been calculated by measuring the difference in line length between the
827
present day and restored cross sections (Figures 6-11) for the top Urgonian horizon, dividing
828
by the original (restored) length and multiplying by 100.
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Figure 13: Thrust zone displacement profiles for thrust zones 1-3 and out-of-zone
831
displacement. Out-of-zone displacement refers to displacement on thrusts that are located
832
within structural zones 1-3 (see Figure 2b) but not within thrust zones 1-3. A decrease in
833
thrust zone 3 displacement coincides with increases in thrust zone 1 and out-of-zone
834
displacement, indicating displacement transfer between thrust zones. S: Sassenage section; C:
835
Cognin-les-Gorges section; SR: St-Romans sections; SE: Ste-Eulalie-en-Royans section; BB:
836
Beauregard-Baret section; B: Barbieres section.
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837 838
Figure 14: Model for thrust zone displacement transfer along strike in the Vercors.
839
Displacement in thrust zone 3 gradually decreases to the south, which is accommodated by a
35
ACCEPTED MANUSCRIPT gradual increase in thrust zone 1 displacement to maintain constant fold-thrust belt
841
shortening. Displacement in thrust zone 2 varies very little along strike.
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36
ACCEPTED MANUSCRIPT FIGURE 1 A
a A
B
B C
C
C
B
A
C
B
A
b
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3
2
1
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Displacement
Displacement
Horizontal distance along faults
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Horizontal distance along faults
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Horizontal distance along faults
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stress/strain field
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Displacement
fault
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Horizontal distance along fault zone
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FIGURE 2 a Ge
B.
RT
SR
C: Chamonix
Gr: Grenoble A: Annecy au
PeR
sD
PG SE on
e2
Chartr.: Chartreuse DR: Drome River
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thr u
st
zo
ne
1
B
Hauterivian Valanginian Berrasian Jurassic (& Triassic) Basement Structural zone boundary
Fault
Zone 2
St-R
d best fit section plane
om
ans
Ste Roy Eulalie ans -en -
Bea u Bar regard et Bar
bie
Zone 3
Cog les- ninGor ges
n = 781
UR
CR
Zone 1
Barremian (non platform carbonate)
age
G
SNi
GG CL
thrust zone 3
thr
BB
TE D
ine
SN
Ba
H.-G.: Hautes-Giffre
Urgonian
PM
GB ph
Ch: Chatillon-en-Diois
Aptian-Maastrichtian
RI PT
e nn
C
Cr: Crest
Ge: Geneva
Sas
M AN U
Cr Dr
Palaeocene-Miocene
sen
N
M. B.: Mont Blanc
S
PS
Brianconnais Internal Zone
Internal Zones
50 km
Key to geological map of the Vercors and cross sections N
External Zone Massifs
do
Ba
Ch
SQ
Dauphinois Mesozoic
ust z
b
c 10 km
Jurassian Mesozoic
lle Be
Ch art r.
C
Ve rco rs
Gr
H.-
G.
Tertiary
M.
es Bo rne s ug
A
Bas Dauphine
b Geological map of the Vercors
SC
Jura
res
Zone 4: Drac Valley
B. Barbieres BB. Beauregard-Baret C. Cognin-les-Gorges CL. Combe Laval CR. Col de Rousset G. Grenoble GB. Gorges de la Bourne GG. Grands Goulets PeR. Pont-en-Royans PG. Petits Goulets PM. Pic St-Michel PS. Plateau de Sornin
S. Sassenage SE. Ste-Eulalie-enRoyans SN. St-Nazaire-enRoyans SNi. St-Nizier-duMoucherotte SQ. St-Quentin-surIsère SR. St-Romans RT. Rencurel Thrust UR. Urgonian Ridge
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N
b
offset thrust: flexural slip?
ESE WNW tight fold
thrust splays
c
N
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Urgonian Hauterivian
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bedding
800
SC
thrust trace
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10 m
bedding
backthrust
m
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photo W WNW
E
ESE ESE
WNW
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b
260 m
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backthrusts
FIGURE 4
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2
SC
a
ACCEPTED MANUSCRIPT FIGURE 5 a
WNW
ESE fold hinges
Plateau de Sornin
Rencurel Thrust
inian
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Urgonia
5 km Jurassic ridges
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Jura
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E
Jurassic bedding
17 km
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g Valan Upper
Vercors
Urgonian ridge (W-dipping)
W
ACCEPTED MANUSCRIPT
Barbieres zone 3
zone 2
zone 1 thrust zone 2
thrust zone 1
thrust zone 3 topography
Internal structure not shown
SC
F
M AN U
5000 m WNW
zone 4 (Drac Valley)
RI PT
BD
Internal structure not restored
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FIGURE 6
ESE
ACCEPTED MANUSCRIPT
Beauregard-Baret zone 1 thrust zone 1
zone 2
zone 4 (Drac Valley)
zone 3
thrust zone 2
thrust zone 3
RI PT
BD
topography
SC
Internal structure not shown
5000 m F
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FIGURE 7
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WNW
ESE
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ACCEPTED MANUSCRIPT Ste-Eulalie-en-Royans BD
zone 4 (Drac Valley)
zone 3
zone 2 thrust zone 3
Internal structure not shown
5000 m
ESE
F
SC
WNW
topography
RI PT
thrust zone 2
M AN U
Internal structure not restored
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FIGURE 8
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BD
zone 2
thrust zone 3
RI PT
St-Romans zone 3
topography
SC
thrust zone 2
zone 4 (Drac Valley)
Internal structure not shown
WNW
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5000 m F
EP AC C
FIGURE 9
TE D
Internal structure not restored
ESE
ACCEPTED MANUSCRIPT
Cognin-les-Gorges zone 3
zone 2
BD
zone 4 (Drac Valley)
thrust zone 3 thrust zone 2
Internal structure not shown
5000 m F
ESE
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topography
Internal structure not restored
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FIGURE 10
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Sassenage BD
zone 4 (Drac Valley)
zone 3
thrust zone 3
RI PT
topography
5000 m
SC
F
ESE
M AN U
WNW
Drac Valley backthrusting (simplified)
Internal structure not shown
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FIGURE 11
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ACCEPTED MANUSCRIPT a.
Shortening distance/total thrust displacement
Shortening distance
4000 3000
Total thrust displacement (top Urgonian horizon)
2000 1000 0 North S
C
SR
SE
BB
B South
b.
SC
cross section
Shortening percentage
8 4 0 North S
C
SR
SE
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FIGURE 12
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shortening (%)
16 12
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shortening/displacement (m)
5000
B South
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Thrust zone displacement
1500 Zone 1
RI PT
displacement (m)
2000
Zone 2
1000
Zone 3
Out-of-zone
0 North
S
C
SR
SE
BB
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cross section
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500
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FIGURE 13
B
South
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FIGURE 14
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1
3 2
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ACCEPTED MANUSCRIPT Using laterally compatible cross sections to infer fault growth and linkage models in foreland thrust belts Highlights
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We construct parallel cross sections through the Vercors foreland thrust belt Cross sections are analysed to ensure lateral continuity Displacement profiles show displacement transfer between thrust zones Fault properties suggest thrusts evolve through soft-linked and hard-linked stages
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• • • •