Scientific teams analyze earthquake hazards of the cascadia subduction zone
[No abstract available]
Eos, Transactions, American Geophysical Union↗
Geology topics
Nina Kukowski
Publications and source records attributed to Nina Kukowski.
Thermo-hydraulics of the Peruvian accretionary complex at 12°S
Coupled heat and fluid transport at the Peruvian convergent margin at 12°S wasstudied with finite element modelling. Structural information was available from two seismicreflection lines. Heat production in the oceanic plate, the metamorphic basement, and sedimentswas estimated from literature. Porosity, permeability, and thermal conductivity for the modelswere partly available from Ocean Drilling Program (ODP) Leg 112; otherwise we used empiricalrelations. Our models accounted for a possible permeability anisotropy. The decollement was bestmodelled as a highly permeable zone (10 −13 m 2 ). Permeabilities of thePeruvian accretionary wedge adopted from the model calculations fall within the range of 2 to7×10 −16 m 2 at the ocean bottom to a few 10 −18 m 2 at the base and need to be anisotropic. Fluid expulsion at the sea floor decreases graduallywith distance from the deformation front and is structure controlled. Small scale variations of heatflux reflected by fluctuations of BSR depths across major faults could be modelled assuming highpermeability in the faults which allow for efficient advective transport along those faults. The models were constrained by the thermal gradient obtained from the depth of bottomsimulating reflectors (BSRs) at the lower slope and some conventional measurements. We foundthat significant frictional heating is required to explain the observed strong landward increase ofheat flux. This is consistent with results from sandbox modelling which predict strong basalfriction at this margin. A significantly higher heat source is needed to match the observed thermalgradient in the southern line.
Journal of Geodynamics↗
New seismic images of the cascadia subduction zone from cruise SO 108-ORWELL
In April and May 1996, a geophysical study of the Cascadia continental margin off Oregon and Washington was conducted aboard the German R/V Sonne. This cooperative experiment by GEOMAR and the USGS acquired wide-angle reflection and refraction seismic data, using ocean-bottom seismometers (OBS) and hydrophones (OBH), and multichannel seismic reflection (MCS) data. The main goal of this experiment was to investigate the internal structure and associated earthquake hazard of the Cascadia subduction zone and to image the downgoing plate. Coincident MCS and wide-angle profiles along two tracks are presented here. The plate boundary has been imaged precisely beneath the wide accretionary wedge close to shore at c13km depth. Thus, the downgoing plate dips more shallowly than previously assumed. The dip of the plate changes from 2?? to 4?? at the eastern boundary of the wedge on the northern profile, whereas approximately 3km of sediment is entering the subduction zone. On the southern profile, where the incoming sedimentary section is about 2.2km thick, the plate dips about 0.5?? to 1.5?? near the deformation front and increases to 3.5?? further landwards. On both profiles, the deformation of the accretionary wedge has produced six ridges on the seafloor, three of which represent active faulting, as indicated by growth folding. The ridges are bordered by landward verging faults which reach as deep as the top of the oceanic basement. Thus, the entire incoming sediment package is being accreted. At least two phases of accretion are evident, and the rocks of the older accretionary phase(s) forms the backstop for the younger phase, which started around 1.5 Ma ago. This documents that the 30 to 50km wide frontal part of the accretionary wedge, which is characterized by landward vergent thrusts, is a Pleistocene feature which was formed in response to the high input of sediment building the fans during glacial periods. Velocities increase quite rapidly within the wedge, both landward and downward. At the toe of the deformation front, velocities are higher than 4.0 km/s, indicating extensive dewatering of deep, oceanic sediment. Further landward, considerable velocity variation is found, which indicates major breaks throughout the accretionary history.
British Columbia, California, Idaho, Nevada, Orego↗