This is a Preprint and has not been peer reviewed. The published version of this Preprint is available: https://doi.org/10.1029/2022GL099871. This is version 1 of this Preprint.
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Abstract
Geological processes in Southern Patagonia are affected by the Patagonian slab window, formed by the subduction of the Chile Ridge and subsequent northward migration of the Chile Triple Junction. Using shear wave splitting analysis, we observe strong splitting of up to 2.5 s with an E-W fast direction just south of the triple junction and the edge of the subducting Nazca slab. This region of strong anisotropy is coincident with low uppermost mantle shear velocities and an absence of mantle lithosphere, indicating that the mantle flow occurs in a warm, low-viscosity, 200-300 km wide shallow mantle channel just to the south of the Nazca slab. The region of flow corresponds to a volcanic gap caused by depleted mantle compositions and absence of slab-derived water. In most of Patagonia to the south of this channel, splitting fast directions trend NE-SW consistent with large-scale asthenospheric flow.
DOI
https://doi.org/10.31223/X5TP95
Subjects
Earth Sciences, Physical Sciences and Mathematics
Keywords
slab window-azimuthal anisotropy-mantle flow-olivine fabrics-volcanic gap-toroidal flow
Dates
Published: 2022-07-08 19:39
Last Updated: 2022-07-09 02:39
License
CC0 1.0 Universal - Public Domain Dedication
Additional Metadata
Data Availability (Reason not available):
Seismic stations information, and shear wave splitting and azimuthal anisotropy results presented in this contribution can be found in the Zenodo repository
Conflict of interest statement:
No conflict of interest
There are no comments or no comments have been made public for this article.