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The S reflector and Rifting Processes: Galicia Bank Basin and Iberia Abyssal Plain

Rice University Investigators : Dale S. Sawyer and Colin Zelt

Collaborators:
James Austin, Yosio Nakamura, Gail Christeson, Univ. of Texas Inst for Geophys
Tim Reston, GEOMAR, Kiel, Germany
JuanJo Danobeitia, Inst. of Earth Sciences, Barcelona, Spain
Diego Cordoba, Univ. of Madrid, Spain

Graduate students working with data from our cruise:
Mike Unger, Rice MS student
Tyler Knoll, Rice MS student
Phil Pappano, Rice PhD student
Allison Henning, Rice PhD student
Stephen Clark, UT MS student
Marta Perez Gussinye, GEOMAR PhD student
Rafael Bartolome, U. Madrid, Spain, PhD student
Francisco Teixiera, U. Aveiro, Portugal, PhD student

Funding Source: NSF Marine Geology and Geophysics


Interpreted seismic depth sections across the outer Galicia Bank margin. Normal oceanic crust is on the left part of the section and the continental crust of the Iberia Peninsula is frar to the right of the section. The extended continental crust (pink) was highly faulted during continental breakup. Line 4 crosses a teature known as the Peridotite Ridge, where upper mantle rocks (green) penetrate the crust and once outcropped at the seafloor. Line 15 crosses two peridotite ridge features, indicating an overlapping or en echelon character for the ridge.

Abstract

During July and August of 1997, we used the RV Maurice Ewing to acquire multichannel seismic (MCS) reflection profiles, ocean bottom seismograph/hydrophone (OBS/OBH) refraction/reflection profiles, bathymetry, and magnetic observations in the Atlantic Ocean offshore of Portugal and Spain. The experiment consisted of MCS profiling using the 160 channel digital streamer and 8400 cu. in. airgun array of the R/V Maurice Ewing, long-offset marine seismic acquisition using 11 OBS's and 14 OBH's. Approximately 4000 km of MCS data, and 55 OBS/OBH datasets were acquired. The experiment took place on the Galicia Bank, the Galicia Interior Basin, and the transition from the Galicia margin to the Iberia Abyssal Plain margin to the south. This work was conducted in cooperation with scientists at the University of Texas at Austin, the GEOMAR Marine Laboratory in Kiel Germany, the University of Aberdeen, Scotland, the University of Madrid and the Center for Earth Sciences of Barcelona Spain, and the University of Aveiro in Portugal.

We acquired data to address each of our three main research objectives:

1. Describing the character of the S reflector in the lower crust or upper mantle of the Galicia Bank margin segment. We show that the S reflector is the boundary between rocks of velocity 6.9 km/s above and 7.8 km/s below. This suggests that S forms the Moho in this area and that continental crustal rocks have been emplaced by faulting over rocks of the upper mantle.

2. Mapping the variation in crust thickness and amount of extension across the entire continental margin from unambiguous oceanic crust to unrifted continental crust. We show the crustal thickness and velocity structure across the entire rifted margin at 4 locations. The rifting in the Galicia Interior basin seems to have reached a peak extension of beta 3.0. Extension of the crust forming the Galicia Bank shows extension by beta 2.0.

3. Mapping the variation along-strike of the rifting process from the Iberia Abyssal Plain to the south to the Galicia Bank in the north. We have 9 crossings of the transitional zone of the Galicia Bank and iberia rifted margin segments. They show greater variation along strike than we had envisionesd. We are now working to understand those differences.

We have processed all the MCS data through post-stack f-k time migration. These sections are quite good and certainly allow first level interpretation and synthesis as well as allowing us to choose profile segments that will benefit from more extensive processing

The OBS/OBH are generally of excellent quality. The MCS data however are unable to constrain the velocity structure of the crust and uppermost mantle, or the position of the Moho, except where it appears to be synonymous with the S reflector. Therefore, the main role of the wide-angle data is to constrain the sub-sedimentary velocity structure to uppermost mantle depth. By utilizing zero-offset reflection times picked from the MCS data with the wide-angle data in the velocity and interface inversion, the degree of velocity-depth ambiguity associated with the sediment structure and above the S reflector is reduced in comparison to the constraint provided by the wide-angle data alone.



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Last updated 7 November, 2000 by dale@rice.edu