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2D Seismic velocity structure of the Iberia margin

Investigator : Colin Zelt, Dale Sawyer, Mike Unger, Tyler Knoll

Outside Collaborators: James Austin, Jr., Yosio Nakamura, Gail Christeson (Institute for Geophysics, University of Texas at Austin)

Funding Source: NSF, Marine Geology and Geophysics


Velocity model derived by simultaneous traveltime inversion of wide-angle and reflection seismic data. The unconstrained portion of the model is omitted. The ocean bottom receiver locations are indicated along the seafloor as yellow dots. The PmP reflection points are indicated by black dots along the Moho (thick white line). The black contour is the sediment-basement boundary. The range of P-wave velocities in the three sediment layers is indicated along with representative velocities along the top and bottom of the crust and beneath the Moho. Large red dots are reflection points of picks of the S reflector from the MCS data that were inverted simultaneously with the wide-angle data as reflections from the Moho. Small pink dots are reflection points of picks from the MCS data modeled as "floating" reflectors, i.e., reflectors not associated with a layer velocity discontinuity. The yellow contours labeled 7.0 and 7.6 are isovelocity contours (km/s) from a minimum-structure model derived by tomographic inversion of the first-arrival traveltimes. The coast line is indicated by the arrow at the top of the model. OC - oceanic crust; PR - Peridotite Ridge; GB - Galicia Bank; GIB - Galicia Interior Basin.


Abstract

We have analyzed wide-angle and MCS data from the Iberia margin along a 335 km dip profile over the Galicia Interior Basin (GIB), Galicia Bank (GB), S reflector, and Peridotite Ridge. The MCS data provide a detailed image of the margin sediments and basement. The wide-angle data constrain the sub-sedimentary velocity structure. Zero-offset reflection times from the sediments, basement and S reflector were inverted simultaneously with the deeper refraction/wide-angle phases to account for the complex shallow structure on the deeper raypaths. A minimum-parameter, preferred final model satisfying all the data was obtained which includes subjective features considered geologically reasonable. The S reflector appears to be the Moho just 3-5 km beneath the seafloor and its seaward dip suggests it is a detachment fault. To objectively assess this model, the first arrival and Moho reflection data were inverted using a minimum-structure tomographic approach. The isovelocity contours representing the Moho in the final tomographic model obtained from the first arrivals agree well with the Moho in the preferred final model. The flattest and smoothest Moho obtained from a tomographic inversion of the zero-offset S reflector and wide-angle reflections also agrees well with the Moho in the preferred final model. Landward of the S reflector, the correlation between crustal thickness, water depth and sediment thickness is typical for a rifted margin. Crustal thickness variations suggest the margin extended in two phases spatially separated by about 100 km, with stretching factors of 2.5-3 and nearly infinite implied for the early and late (preceding seafloor spreading) stages of rifting beneath the GIB and GB basin. A checkerboard resolution test using first arrival tomography shows that lateral velocity resolution is 5-15 km in the sediments and basement to ~8 km depth, and resolution is about 40-50 km at the Moho landward of the S reflector.


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Last updated 15 October, 2000 by dale@rice.edu