2006
DOI: 10.1016/j.tecto.2005.10.026
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Reviewing pre-TRANSALP DSS models

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Cited by 27 publications
(15 citation statements)
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“…Moreover, the amplified frequencies obtained by the spectral analyses agree well with both the assumed thickness of sediments reported in Figure 1 (e.g., Cassano et al, 1986;Ambrosetti et al, 1987;Doglioni, 1993) and the crustal model derived for the area through the interpretation of deep seismic soundings (Pieri and Groppi, 1981;Cassinis, 2006). The model provides shear-wave velocities in the first 3 km (maximum depth corresponding to the available stations) which range from 0.6 to 1:2 km=s (see also Vuan et al, 2011).…”
Section: Discussionsupporting
confidence: 82%
See 1 more Smart Citation
“…Moreover, the amplified frequencies obtained by the spectral analyses agree well with both the assumed thickness of sediments reported in Figure 1 (e.g., Cassano et al, 1986;Ambrosetti et al, 1987;Doglioni, 1993) and the crustal model derived for the area through the interpretation of deep seismic soundings (Pieri and Groppi, 1981;Cassinis, 2006). The model provides shear-wave velocities in the first 3 km (maximum depth corresponding to the available stations) which range from 0.6 to 1:2 km=s (see also Vuan et al, 2011).…”
Section: Discussionsupporting
confidence: 82%
“…The global map in the top left inset shows the epicenter of the 11 March 2011 M w 9.0 Tohoku-Oki, Japan, earthquake (gray star) and the position of the investigated area (black rectangle). (b) The contour lines indicate the thickness of the Po Basin sediments (Pieri and Groppi, 1981;Cassinis, 2006). The black dashed lines AA 0 and BB 0 in (a) indicate the transverse sections reported in (c), obtained from Cassano et al (1986) and Livio et al (2009). Parma event (Fig.…”
Section: Target Area: the Po Plainmentioning
confidence: 94%
“…For simplicity, we only consider the shallower crustal root option (~60 km depth), since this is the preferred model by Pedreira et al (2015). Similar Moho-depth values are locally found in several Alpine orogens like Eastern Alps (60 km; Cassinis, 2006), Zagros (56-69 km; Paul et al, 2010), Pyrenees (55-70 km; Chevrot et al, 2015), and Rif (N55 km, Mancilla and Diaz, in this volume). See also Artemieva and Thybo (2013) for a European Moho compilation.…”
Section: Crustal Geometry From Previous Studiesmentioning
confidence: 74%
“…Ebbing et al 2001) and seismic data (Cassinis 2006;Giese and Buness 1992;Waldhauser et al 1998;Waldhauser et al 2002;Ziegler and Dèzes 2007, for compilation) do not point to a significant change of depth of the Moho below the Brenner Fault (Fig. 6).…”
Section: Surface Topography and Geometry Of The Moho Across The Brennmentioning
confidence: 90%
“…c Modified after Waldhauser et al (2002); Ziegler and Dèzes (2007). d Modified from Cassinis (2006) (Kummerow et al 2004;Schmid et al 2004) indicate that the Moho attains almost 50 km below the Tauern Window, suggesting that extension cannot have been very significant.…”
Section: Surface Topography and Geometry Of The Moho Across The Brennmentioning
confidence: 99%