Seismics of the Rio Grande Rift


Seismic Reflection Study of North Western Espanola Basin at Abiquiu

    This model is a combination of seismic reflection, seismic refraction and gravity from the western boundary of the Rio Grande Rift. It is located in the Abiquiu embayment in the Espanola Basin in the Northern Rio Grande Rift. This data was taken along a 16 km long line during the 1990 and 1991 SAGE field seasons.
    The rift in this area is bounded by northeast striking faults that offset the Paleozoic/Mesozoic rocks of the Colorado Plateau from the rift sediments. Go to Stratigraphic section.
    The above figure represents the interpretive geologic cross section at Abiquiu. In B, the cross section has been restored to reset faults to make the Madera Formation smooth. The amount of horizontal extension has been calculated to be about 1.1 km and the vertical displacement is about 0.6 km.
(Figure from Baldridge et al 1994)

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Velocity Model for Rio Grande Rift

       The low velocity zone is representative of the transition zone and not the rift graben trend. The pattern that results seems consistent with a clockwise rotation of the Colorado Plateau. The low velocity zone that strikes NNE to NE currently, is roughly perpendicular to the WNW-ESE current regional extension trend. This suggests that the lithosphere could be extending due to modern regional stress, thus the surface indication of stress at the surface.
        Vertically averaged variations of velocity were contoured at an interval of 1%. It was assumed that the velcity variation under the stable Great Plains, is zero. The velocity map is overlaid on a tectonic map of the Rio Grande Rift.
(Figure from Slack et al 1996)
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SKS Splitting Beneath the Rio Grande Rift

        SKS splitting is caused by an anisotropic upper mantle. Anisotropy in the upper mantle is caused by the LPO (Lattice Preferred Orientation) of olivine and other ellastically anisotropic minerals in the upper mantle (orthopyroxene). With strain the LPO of olivine (a-axis) aligns perpendicular with the maximum compressional direction ( uniaxial compression), perpendicular to shortening direction (simple shear), or aligns to flow direction (simple shear) (Gao et al 1997).
        Passive rifting is expected to have a LPO to align with the direction of extension. Active rifting involves asthenospheric upwelling and any fabric that would develop the LPO would depend on the convection (Gao et al 1997).
        SKS Splitting results show a fast direction in the north-northeast direction, perpendicular to the regional stress field and parallel to subparallel to the rift trend. Splits ranged from 0.9 to 1.5 seconds. The interpretation of the rift-parallel fast polarization direction is consistent with a rift-parallel flow in a convection cell within the mantle. The Rio Grande Rift is above a low velocity upper mantle that has been determined from teleseismic tomography (Gao et al 1997).
        Another possible model involves the SKS splitting to be from fossil anisotropy from past tectonic disturbances (Laramide deformation). Though it is unlikely that any anisotropy could be preserved with high heat flow associated from upwelling asthenosphere. Tomography suggests that the 9000C isotherm is about 50 km beneath rift zones (Gao et al 1997).
(Figure from Gao et al 1997)
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