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Research

The seismic landscape of Earth's deep mantle

The mantle is full of weird and wonderful phenomena. As tectonic plates sink into the mantle at subduction zones and hot material upwells to erupt at mid-ocean ridges and hot-spot volcanoes, the mantle is churned into a marble cake of thermal and chemical heterogeneity. At the core-mantle boundary, where the solid rocky mantle meets the liquid metal outer core, the differences in physical properties are so extreme (even more so than between the crust and the atmosphere!) that a menagerie of complex and variable structures have collected there over billions of years of dynamic processes.

 

By resolving these structures in seismic models and reconciling our observations with geodynamic simulations and compositional constraints from mineral physics experiments, we ultimately build a more holistic understanding of Earth's compositional and dynamic evolution. Current seismic models of the deep mantle most notable reveal two giant piles of thermochemically distinct material that sit on opposite sides of the core, reaching over 1,000 km up into the overlying mantle and extending laterally up to ~10,000 km. Seismologists model these structures as regions where seismic waves travel at slightly lower speeds than expected, and so they are referred to most commonly as Large Low-Velocity Provinces (LLVPs). Models also show much smaller features of even more extreme wave-speed reductions, called Ultra Low-Velocity Zones (ULVZs), which may collect at the edges of LLVPs and constitute the roots of very hot plumes, some of which traverse the entire mantle and erupt at the surface (e.g., Hawai'i, Iceland, Samoa, Kerguelen).​​ I have the great good fortune to study these structures, which together constitute the seismic landscape of Earth's deep mantle, as part of Ed Garnero's research group.

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SITRUS: updating global models

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​​Currently, my primary research involves the development of a method and software to update global, whole-mantle tomography models in a flexible and efficient forward modeling framework to better explain observed seismic travel times. This method, the Seismic Iterative Tomography Update Scheme (SITRUS), migrates input tomography models toward versions that reduce the misfit between predicted and observed travel time residuals. The software allows the user to experiment with many different input parameters related to the model setup and input dataset to produce various solution models. The software is openly available on GitHub. SITRUS was developed in collaboration with Ed Garnero, with support from Samantha Hansen, Jeroen Ritsema, and Steve Grand.​​​​​​​​​​​

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An example of the model GLAD-M25 (Lei et al., 2020) updated using SITRUS.

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EMPRESS: optimized event selection

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In addition to SITRUS and global, whole-mantle models, I also work on methods to bridge the gap between theoretical and observational seismology. Advanced theoretical modeling frameworks are computationally expensive and thus well-suited to regional applications, however models are limited by the number of events that can be incorporated. Therefore, careful event selection is imperative for producing optimized models of mantle structure. To address this, I developed the Earth Modeling PRioritized Event Selection Scheme (EMPRESS), to assist in choosing events with abundant high-quality data that provide good regional coverage. EMPRESS is also openly available and designed with a flexible, user-friendly Jupyter interface. EMPRESS was developed in collaboration with Ed Garnero and Ebru Bozdag.

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website_empress_example.png

 

An example of 100 prioritized events selected by EMPRESS for a potential regional model of the Pacific LLVP.

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Arizona contains 22 Native American tribal nations. The School of Earth and Space Exploration at ASU is located on the ancestral homelands of the Akimel O'odham (Pima) and Pee Posh (Maricopa) peoples.

clairerichardson@asu.edu

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website last updated December 2024

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