Fernández-Viejo Gabriela

Dr. Fernández-Viejo Gabriela

orcid

Research Focus & Metrics

Academic Career Length

31Years (1996-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 October 1996 in Tectonophysics
Verified
Journal Article
Closed access
JPJ.A. Pulgar
J.A. Pulgar
JGJ. Gallart
J. Gallart
FGFernández-Viejo Gabriela
Fernández-Viejo Gabriela
APA. Pérez-Estaún
A. Pérez-Estaún
JÁJ. Álvarez-Marrón
J. Álvarez-Marrón

1 July 2010 in Near Surface Geophysics
Verified
Journal Article
Closed access
PDF file
JOJavier Olona
Javier Olona
JPJavier A. Pulgar
Javier A. Pulgar
FGFernández-Viejo Gabriela
Fernández-Viejo Gabriela
CLCarlos López-Fernández
Carlos López-Fernández
JGJuan M. González‐Cortina
Juan M. González‐Cortina

1 December 1998 in Geophysical Research Letters
Verified
Journal Article
Closed access
PDF file
FGFernández-Viejo Gabriela
Fernández-Viejo Gabriela
JGJ. Gallart
J. Gallart
JPJ. A. Pulgar
J. A. Pulgar
JGJ. Gallastegui
J. Gallastegui
JDJ. J. Dañobeitia
J. J. Dañobeitia
DCD. Córdoba
D. Córdoba

10 February 2000 in Journal of Geophysical Research
Verified
Journal Article
Closed access
PDF file
FGFernández-Viejo Gabriela
Fernández-Viejo Gabriela
JGJosep Gallart
Josep Gallart
JPJavier A. Pulgar
Javier A. Pulgar
DCDiego Córdoba
Diego Córdoba
DADañobeitia
Dañobeitia
JJJuan José
Juan José


1 June 2005 in Canadian Journal of Earth Sciences
Verified
Journal Article
Closed access
RCRon M Clowes
Ron M Clowes
PHPhilip Tc Hammer
Philip Tc Hammer
FGFernández-Viejo Gabriela
Fernández-Viejo Gabriela
JWJ. Kim Welford
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.