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Mantle transition zone shear velocity gradients beneath USArray

Schmandt, Brandon (2012) Mantle transition zone shear velocity gradients beneath USArray. Earth and Planetary Science Letters, 355 . pp. 119-130. ISSN 0012-821X. http://resolver.caltech.edu/CaltechAUTHORS:20130222-102744260

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Abstract

Broadband P-to-s scattering isolated by teleseismic receiver function analysis is used to investigate shear velocity (V_S) gradients in the mantle transition zone beneath USArray. Receiver functions from 2244 stations were filtered in multiple frequency bands and migrated to depth through P and S tomography models. The depth-migrated receiver functions were stacked along their local 410 and 660 km discontinuity depths to reduce stack incoherence and more accurately recover the frequency-dependent amplitudes of P410s and P660s. The stacked waveforms were inverted for one-dimensional V_S between 320 and 840 km depth. First, a gradient-based inversion was used to find a least-squares solution and a subsequent Monte Carlo search about that solution constrained the range of V_S profiles that provide an acceptable fit to the receiver function stacks. Relative to standard references models, all the acceptable models have diminished V_S gradients surrounding the 410, a local V_S gradient maximum at 490–500 km depth, and an enhanced V_S gradient above the 660. The total 410 V_S increase of 6.3% is greater than in reference models, and it occurs over a thickness of 20 km. However, 60% of this V_S increase occurs over only 6 km. The 20 km total thickness of the 410 and diminished V_S gradients surrounding the 410 are potential indications of high water content in the regional transition zone. An enhanced V_S gradient overlying the 660 likely results from remnants of subduction lingering at the base of the transition zone. Cool temperatures from slabs subducted since the late Cretaceous and longer-term accumulation of former ocean crust both may contribute to the high gradient above the 660. The shallow depth of the 520 km discontinuity, 490–500 km, implies that the regional mean temperature in the transition zone is 110–160 K cooler than the global mean. A concentrated V_s gradient maximum centered near 660 km depth and a low V_S gradient below 675 km confirms that the ringwoodite to perovskite+magnesiowüstite reaction is the dominant cause of the 660 in the region.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/j.epsl.2012.08.031DOIUNSPECIFIED
http://www.sciencedirect.com/science/article/pii/S0012821X12004591PublisherUNSPECIFIED
Additional Information:© 2012 Elsevier B.V. Received 13 May 2012. Received in revised form 23 August 2012. Accepted 25 August 2012. Editor: Dr. P. Shearer. Available online 10 October 2012. Seismic wave form data for the preceding receiver function study were acquired from the IRIS DMC. Discussions with Ken Dueker, Don Helmberger, Jennifer Jackson, and Rob Clayton are appreciated. Huaiyu Yuan provided his version of the reflectivity code. Two reviewers and the editor are thanked for their constructive feedback. This research was supported by the Gordon and Betty Moore Foundation through the Tectonics Observatory at Caltech.
Group:Caltech Tectonics Observatory
Funders:
Funding AgencyGrant Number
Gordon and Betty Moore FoundationUNSPECIFIED
Subject Keywords:mantle transition zone, 520 km discontinuity, 410 km discontinuity, 660 km discontinuity, subduction
Record Number:CaltechAUTHORS:20130222-102744260
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20130222-102744260
Official Citation:Brandon Schmandt, Mantle transition zone shear velocity gradients beneath USArray, Earth and Planetary Science Letters, Volumes 355–356, 15 November 2012, Pages 119-130, ISSN 0012-821X, 10.1016/j.epsl.2012.08.031. (http://www.sciencedirect.com/science/article/pii/S0012821X12004591)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:37075
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:22 Feb 2013 19:00
Last Modified:22 Feb 2013 19:00

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