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  • 1
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    PANGAEA
    In:  Supplement to: Cordell, Darcy; Unsworth, Martyn J; Diaz, Daniel; Reyes-Wagner, Valentina; Currie, Claire A; Hicks, Stephen P (2019): Fluid and Melt Pathways in the Central Chilean Subduction Zone Near the 2010 Maule Earthquake (35–36°S) as Inferred From Magnetotelluric Data. Geochemistry, Geophysics, Geosystems, 20(4), 1818-1835, https://doi.org/10.1029/2018GC008167
    Publication Date: 2024-02-05
    Description: The subduction zone of central Chile (36° S) has produced some of the world's largest earthquakes and significant volcanic eruptions. Understanding the fluid fluxes and structure of the subducting slab and over-riding plate can provide insight into the tectonic processes responsible for both seismicity and magmatism. Magnetotellurics (MT) is a geophysical method which is sensitive to conductive anomalies (e.g. partial melt and brines) in the subsurface. This dataset includes MT EDI data files for 38 sites collected along a profile in central Chile and western Argentina in 2016 and 2017. It includes 19 long period (10 s to 10000 s) MT stations and 19 broadband (0.001 s to 1000 s) MT stations. Four of the broadband MT sites were collected by Alterra Power Corp (now Innergex Renewable Energy Inc.) labelled MU-002, MU-003, MU-011, and MU-019 (Hickson et al., 2011). Four of the long period sites in Argentina are taken from Burd et al. (2014). This dataset also includes two geo-referenced 2-D resistivity models and the inversion parameters used to produce the model. The nonlinear conjugate gradient algorithm of Rodi and Mackie (2001) was used to produce this model. The first is the unconstrained case where no slab tear was imposed (MODEL_UNCONSTRAINED). In this folder is the geo-referenced model (longitude, latitude, depth (km b.s.l.), resistivity) as well as a folder containing the inversion input files. The second is the constrained case where a slab tear was imposed (MODEL_CONSTRAINED). This also includes a geo-referenced model (longitude latitude depth resistivity) text file and a folder containing the inversion input files.
    Keywords: Central_Chile; Chile; File format; File name; File size; geophysics; magnetotellurics; maule; MULT; Multiple investigations; subduction zone; Uniform resource locator/link to file
    Type: Dataset
    Format: text/tab-separated-values, 12 data points
    Location Call Number Limitation Availability
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  • 2
    Publication Date: 2022-05-25
    Description: Author Posting. © American Geophysical Union, 2014. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geochemistry, Geophysics, Geosystems 15 (2014): 4230–4253, doi:10.1002/2014GC005509.
    Description: Five magnetotelluric (MT) profiles have been acquired across the Cascadia subduction system and transformed using 2-D and 3-D nonlinear inversion to yield electrical resistivity cross sections to depths of ∼200 km. Distinct changes in plate coupling, subduction fluid evolution, and modes of arc magmatism along the length of Cascadia are clearly expressed in the resistivity structure. Relatively high resistivities under the coasts of northern and southern Cascadia correlate with elevated degrees of inferred plate locking, and suggest fluid- and sediment-deficient conditions. In contrast, the north-central Oregon coastal structure is quite conductive from the plate interface to shallow depths offshore, correlating with poor plate locking and the possible presence of subducted sediments. Low-resistivity fluidized zones develop at slab depths of 35–40 km starting ∼100 km west of the arc on all profiles, and are interpreted to represent prograde metamorphic fluid release from the subducting slab. The fluids rise to forearc Moho levels, and sometimes shallower, as the arc is approached. The zones begin close to clusters of low-frequency earthquakes, suggesting fluid controls on the transition to steady sliding. Under the northern and southern Cascadia arc segments, low upper mantle resistivities are consistent with flux melting above the slab plus possible deep convective backarc upwelling toward the arc. In central Cascadia, extensional deformation is interpreted to segregate upper mantle melts leading to underplating and low resistivities at Moho to lower crustal levels below the arc and nearby backarc. The low- to high-temperature mantle wedge transition lies slightly trenchward of the arc.
    Description: Phil Wannamaker and Virginie Maris gratefully acknowledge funding by the U.S. National Science Foundation under grants EAR08–43725 and EAR08–38043 through the Earthscope and Geophysics programs. The 2D inversion capability received development support under U.S. Department of Energy contract DE-PS36-04GO94001. Rob Evans was supported through Earthscope grant EAR08–44041 and Shane McGary through a National Defense Science and Engineering Graduate (NDSEG) fellowship. Fieldwork in Canada was made possible by an NSERC Discovery Grant and a Canadian Foundation for Innovation award to Martyn Unsworth.
    Description: 2015-05-11
    Keywords: Cascadia ; Electrical resistivity ; Magnetotellurics ; Plate coupling ; Episodic tremor and slip ; Arc magmatism
    Repository Name: Woods Hole Open Access Server
    Type: Article
    Format: application/pdf
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  • 3
    Publication Date: 2011-08-01
    Description: As the continental crust thickens during mountain building, it can become hot enough to start melting, leading to a profound reduction in its strength. Melt-weakened crust can flow outward or upward in response to the pressure gradients associated with mountain building, and may be transported hundreds of kilometres laterally as mid-crustal channels. In the Himalayan-Tibetan system, melting began about 30 million years ago, and widespread granite intrusion began at 20-23 Ma. Geophysical data indicate that melt is present beneath the Tibetan plateau today, and deeply eroded mountain belts preserve evidence for melt-enhanced ductile flow in the past. Flow of partially molten crust may limit the thickness and elevation of mountain belts and has influenced the deep structure of continents.
    Print ISSN: 1811-5209
    Electronic ISSN: 1811-5217
    Topics: Geosciences
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