scholarly journals The Hatton Bank continental margin-III. Structure from wide-angle OBS and multichannel seismic refraction profiles

1989 ◽  
Vol 98 (2) ◽  
pp. 367-384 ◽  
Author(s):  
J. V. Morgan ◽  
P. J. Barton ◽  
R. S. White
2017 ◽  
Vol 717 ◽  
pp. 65-82 ◽  
Author(s):  
M. Ruiz ◽  
J. Díaz ◽  
D. Pedreira ◽  
J. Gallart ◽  
J.A. Pulgar

Author(s):  
C. Ravaut ◽  
A. Chabert ◽  
P. W. Readman ◽  
B. M. O‘Reilly ◽  
P. M. Shannon ◽  
...  

2005 ◽  
Vol 42 (6) ◽  
pp. 1277-1293 ◽  
Author(s):  
Ron M Clowes ◽  
Philip TC Hammer ◽  
Gabriela Fernández-Viejo ◽  
J Kim Welford

The SNORCLE refraction – wide-angle reflection (R/WAR) experiment, SNORE'97, included four individual lines along the three transect corridors. A combination of SNORE'97 results with those from earlier studies permits generation of a 2000 km long lithospheric velocity model that extends from the Archean Slave craton to the present Pacific basin. Using this model and coincident near-vertical incidence (NVI) reflection data and geological information, an interpreted cross section that exemplifies 4 Ga of lithospheric development is generated. The velocity structural models correlate well with the reflection sections and provide additional structural, compositional, and thermal constraints. Geological structures and some faults are defined in the upper crust. At a larger scale, the seismic data identify a variety of orogenic styles ranging from thin- to thick-skinned accretion in the Cordillera and crustal-scale tectonic wedging associated with both Paleoproterozoic and Mesozoic collisions. Models of Poisson's ratio support the NVI interpretation that a thick wedge of cratonic metasediments underlies the eastern accreted Cordilleran terranes. Despite the variety of ages, orogenic styles, and tectono-magmatic deformations that are spanned by the seismic corridors, the Moho remains remarkably flat and shallow (33–36 km) across the majority of the transect. Significant variations only occur at major tectonic boundaries. Laterally variable crustal velocities are consistently slower beneath the Cordillera than beneath the cratonic crust. This is consistent with the high temperatures (800–900 °C) required by the slow upper mantle velocities (7.8–7.9 km/s) observed beneath much of the Cordillera. Heterogeneity of the lithospheric mantle is indicated by wide-angle reflections below the Precambrian domains and the western Cordillera.


2013 ◽  
Vol 599 ◽  
pp. 170-196 ◽  
Author(s):  
Volker Thor Leinweber ◽  
Frauke Klingelhoefer ◽  
Sönke Neben ◽  
Christian Reichert ◽  
Daniel Aslanian ◽  
...  

2001 ◽  
Vol 28 (12) ◽  
pp. 2329-2332 ◽  
Author(s):  
Takaya Iwasaki ◽  
Wataru Kato ◽  
Takeo Moriya ◽  
Akiko Hasemi ◽  
Norihito Umino ◽  
...  

2007 ◽  
Vol 110 (2-3) ◽  
pp. 407-418 ◽  
Author(s):  
J. Stankiewicz ◽  
T. Ryberg ◽  
A. Schulze ◽  
A. Lindeque ◽  
M.H. Weber ◽  
...  

2004 ◽  
Vol 159 (1) ◽  
pp. 117-128 ◽  
Author(s):  
I. Contrucci ◽  
F. Klingelhöfer ◽  
J. Perrot ◽  
R. Bartolome ◽  
M.-A. Gutscher ◽  
...  

1993 ◽  
Vol 30 (7) ◽  
pp. 1440-1452 ◽  
Author(s):  
J. A. Hole ◽  
R. M. Clowes ◽  
R. M. Ellis

As part of a multidisciplinary investigation of the structure and tectonics of the Queen Charlotte Basin and underlying crust, deep multichannel seismic reflection and coincident crustal refraction data were collected in 1988. Energy from the reflection air-gun array source was recorded at land sites at offsets appropriate to record crustal refraction and wide-angle reflection data. Refraction data recorded in a broadside geometry provide good three-dimensional coverage of western Hecate Strait. These data are modelled using tomographic inversion techniques to determine the three-dimensional velocity structure of the crust in this region. The one-dimensional average velocity increases rapidly with depth to 6.5 km/s at 7 km depth. Velocities from 7 to at least 12 km depth remain approximately constant and are associated with rocks of the Wrangellia terrane. Significant lateral velocity variations, including large differences in near-surface velocities attributable to surface features, relatively low velocities representing interbedded Tertiary sediments and volcanics, and a deep high-velocity anomaly that may represent the root of an igneous intrusion, are mapped. Wide-angle reflections from the Moho are used to determine the thickness of the crust. The Moho is at 29 km depth beneath the east coast of the Queen Charlotte Islands. This is deeper than the Moho observed below Queen Charlotte Sound and as deep as, or deeper than, that below Hecate Strait. Crustal thinning during Tertiary extension was thus greatest beneath the surface expression of the Queen Charlotte Basin, leaving the crust under the islands considerably thicker than under the basin. In an alternate or additional explanation, compression at the continental margin during the last 4 Ma may have been taken up by thickening or underplating of the continental crust beneath the islands. If the Pacific plate is subducting beneath the islands, the Moho observations constrain the slab to dip greater than 20–26°.


2009 ◽  
Vol 475 (3-4) ◽  
pp. 423-437 ◽  
Author(s):  
Zhongjie Zhang ◽  
Zhiming Bai ◽  
Walter Mooney ◽  
Chunyong Wang ◽  
Xuebo Chen ◽  
...  

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