
NSF Org: |
EAR Division Of Earth Sciences |
Recipient: |
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Initial Amendment Date: | May 20, 2012 |
Latest Amendment Date: | May 20, 2012 |
Award Number: | 1161038 |
Award Instrument: | Standard Grant |
Program Manager: |
Robin Reichlin
EAR Division Of Earth Sciences GEO Directorate for Geosciences |
Start Date: | May 15, 2012 |
End Date: | April 30, 2015 (Estimated) |
Total Intended Award Amount: | $220,326.00 |
Total Awarded Amount to Date: | $220,326.00 |
Funds Obligated to Date: |
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History of Investigator: |
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Recipient Sponsored Research Office: |
660 S MILL AVENUE STE 204 TEMPE AZ US 85281-3670 (480)965-5479 |
Sponsor Congressional District: |
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Primary Place of Performance: |
AZ US 85287-1404 |
Primary Place of
Performance Congressional District: |
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Unique Entity Identifier (UEI): |
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Parent UEI: |
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NSF Program(s): | STUDIES OF THE EARTHS DEEP INT |
Primary Program Source: |
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Program Reference Code(s): | |
Program Element Code(s): |
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Award Agency Code: | 4900 |
Fund Agency Code: | 4900 |
Assistance Listing Number(s): | 47.050 |
ABSTRACT
This two-year proposal focuses on seismological imaging of lower mantle heterogeneity beneath the Pacific Ocean, and numerical convection simulations to put the seismic imaging into a dynamically consistent framework. Our approach is multidisciplinary, and combines seismological analyses by PI Garnero with geodynamical convection simulations by PI McNamara. Recent seismological work has added great detail to deep mantle structure beneath the Pacific, with evidence for large low shear velocity provinces (LLSVPs) that are denser than and chemically distinct from the surrounding mantle. Smaller scale structure includes ultra-low velocity zones (ULVZs) that may preferentially reside at LLSVP margins. Our high resolution seismological experiments aim to better resolve sharp LLSVP edges that appear to extend well up off the core-mantle boundary (CMB), and associated phenomena that depend strongly on LLSVP and mantle properties, including: ULVZ location and structure, CMB topography in vicinity of LLSVP edge, strong heterogeneity within the LLSVP, and relationship to plume upwelling off the LLSVP top. We are focusing on seismic data from southwest Pacific subduction zones recorded in North American, since they densely sample the LLSVP beneath the Pacific Ocean, especially beneath Hawaii. This is a focus area of the proposed work. The seismic findings will inform and be informed by geodynamic simulations that include LLSVP structures. Particular attention will be given to LLSVP morphology and internal structure in the dynamical calculations, as these features will be seismically imaged. Better imaging and modeling LLSVPs will help move us forward in understanding Earth's thermal and mass transport mechanisms, and hence the driving forces in convection that shape the deep structures. Better understanding the nature of convective flow in Earth's deep mantle, how that flow shapes plausible deep and dense compositional reservoirs, and return flow mass transfer that includes plumes is an underlying motivation in this work.
This work is important for understanding the structure and dynamics of Earth's deep interior. The nature of convective flow in Earth?s deep mantle, how that flow shapes plausible deep and dense compositional reservoirs, and return flow mass transfer that includes plumes is of interest to the vast spectrum of Earth and planetary scientists. The funding is for a geodynamics graduate student who will be trained on an interdisciplinary research project, and a postdoctoral researcher focused on seismic imaging and geodynamics computations. The PIs are experienced at co-mentoring students and postdocs in a cross-disciplinary fashion.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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PROJECT OUTCOMES REPORT
Disclaimer
This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.
This research was a multidisciplinary study of the imaging and dynamics of Earth's deep mantle. Seismic imaging has identified heterogeneous structure in the deep mantle, but the nature of the anomalous heterogeneity remains unknown. This grant funded seismological (imaging) and numerical convection (predictions of convective motion over long time scales) studies of these features. Our main findings argue that the heterogeneities are compositionally distinct from the rest of the deep mantle rock. This has important consequences for a number of phenomena, including how hot plumes of mantle rock bring heat and unique chemistry to Earth's surface, to manifest as volcanic eruptions. To carry out this research, we developed a number of computer algorithms to (a) study, analyze, process and measure seismic data, which revealed that the two large deep mantle low seismic wave speed provinces are likely chemically distinct from the surrounding mantle, and (b) predict the convective motions of mantle rock over many millions of years, considering likely sources of heterogeneity, such as the oceanic basaltic crust which sinks into the interior as a part of subduction (the plate tectonic process of the oceanic tectonic plates going into the planetary interior). Our multidisciplinary work focused on the chemical evolution of the large lower mantle chemically distinct piles from the input of the former oceanic crust, as well as the nature of plumes that come off of these piles of dense basal material, which can retain a chemical and thermal signature from the piles. The deep mantle imagine and dynamics is seen to be clearly linked to whole mantle convective flow over millions of years, and thus is linked to the motion of the tectonic plates at the surface, which ride on top of the flowing mantle.
Last Modified: 06/02/2015
Modified by: Edward J Garnero
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