1995
DOI: 10.1016/0040-1951(95)00025-i
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The 3D crustal structure of the Alps of eastern Switzerland and western Austria interpreted from a network of deep-seismic profiles

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Cited by 18 publications
(12 citation statements)
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“…3), most faults dip steeply close to the surface, particularly in the inner (north‐east) part of the massif where back‐thrust structures are observed (Fry, 1989). Compared with the northern ECM (Ménard, 1988; Guellec et al ., 1990; Hitz and Pfiffner, 1994), it is suggested here that the fault dip progressively decreases at depth below the Argentera, such that the faults would branch into a major shear zone at the top of the lower crust. In our interpretation, the deepest part of the Argentera upper crust is shifted to the NE relative to the topographic crest, consistent with the crustal model calculated by Calais et al .…”
Section: Geological Outline Of the Argentera Massifmentioning
confidence: 77%
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“…3), most faults dip steeply close to the surface, particularly in the inner (north‐east) part of the massif where back‐thrust structures are observed (Fry, 1989). Compared with the northern ECM (Ménard, 1988; Guellec et al ., 1990; Hitz and Pfiffner, 1994), it is suggested here that the fault dip progressively decreases at depth below the Argentera, such that the faults would branch into a major shear zone at the top of the lower crust. In our interpretation, the deepest part of the Argentera upper crust is shifted to the NE relative to the topographic crest, consistent with the crustal model calculated by Calais et al .…”
Section: Geological Outline Of the Argentera Massifmentioning
confidence: 77%
“…Schmid et al ., 1996). From balanced cross‐sections at crustal scale, shortening of the external European upper crust was evaluated at about 30 km and 50 km in the Belledonne and Mont Blanc transects, respectively (Ménard and Thouvenot, 1987; Sommaruga, 1997), while Hitz and Pfiffner (1994) suggest a 25‐km shortening for the Aar massif. In the Argentera case, Lickorish and Ford (1998) provide an estimate of c .…”
Section: Discussionmentioning
confidence: 99%
“…The TALP consists of a stack of subhorizontal to gently south dipping nappe that abruptly steepens and becomes overturned north of the Periadriatic Fault (Figure d). Further north, the only thick‐skinned type of deformation of the nappe stack is a low‐amplitude and large‐wavelength antiform that forms the Engadine Window (Figure d), inferred to accommodate 10–12 km of shortening [ Hitz , ]. Recent investigations suggest that the Subalpine Molasse thrust belt, in the area of the Engadine section, was affected by an Oligocene‐Miocene shortening of ~30 km [ Ortner et al ., ].…”
Section: Cross Sections Exhumation Level and Collisional Shorteningmentioning
confidence: 99%
“…This is due to the wide range of minerals and polymineralic rocks which have not been tested, uncertainty of the conditions in the crust, and processes such as cataclastic flow, frictional sliding behavior, and stress corrosion cracking that are not fully understood. Nevertheless, the general pattern of mechanical layering shown by strength profiles is probably qualitatively correct based on, for example, the correlation of strength profiles with the foci of earthquakes in convergent settings [ Cloetingh and Banda , 1992; Zeyen and Fernández , 1994; Hitz , 1995; Okaya et al , 1996]. For simplicity, wet rheologies are chosen for the entire lithosphere due to the large reduction of plastic yield strength by even trace amounts of water.…”
Section: Mechanical Layering Of the Lithospherementioning
confidence: 99%