Geodynamics and Basin Studies Reseach Group, Institutt for Geovitenskap, UiB, Bergen
Project: Paleogene Basin Development on the Vøring and Møre Margins | PALMAR.
PI: Prof. Ritske Huismans
I am a postdoctoral research associate at Universitetet i Bergen (UiB), where I explore the evolution of the North Atlantic volcanic rifted margins through numerical modelling. This research seeks to better understand the spatial and temporal variations in magmatism during rifting. I am particularly interested in lithosphere-mantle interactions and the feedback between the two domains to drive tectonic systems.
This builds on my previous research at Cardiff University, focussing on the interactions between mantle geodynamics and tectonic processes throughout the supercontinent cycle. Much of this work involved developing and using the 3D mantle convection code TERRA to simulate Earth's long-term evolution. My current research integrates these interests with the skills gained during my Masters studies at the University of Leeds, where my dissertation combined 2D models (using the ASPECT code) with seismic data to investigate the effect of extension rate on magmatism at rifted margins. I am always keen to collaborate and share ideas—please feel free to get in touch!
Email me at: abigail.plimmer@uib.no
My current research investigates the spatial and temporal controls on magmatism across the North Atlantic rifted margins using 2D and 3D numerical models. This work will build on my previous studies and contribute to a more comprehensive picture of mantle–lithosphere coupling in tectonically active regions.
Previously, I have approached this at a global scale, exploring how mantle dynamics are coupled with the lithosphere throughout the supercontinent cycle. Using 3D global mantle circulation model, I investigated the dynamics of mantle downwellings and the influence of plate motions on slab sinking in the deep mantle; the coupling between deep mantle structures and surface tectonics; and the ways in which lithospheric structure impacts mantle flow from supercontinent assembly to breakup.
Geodynamics and Basin Studies Reseach Group, Institutt for Geovitenskap, UiB, Bergen
Project: Paleogene Basin Development on the Vøring and Møre Margins | PALMAR.
PI: Prof. Ritske Huismans
Tectonics & Geophysics Research Group, School of Earth & Environmental Sciences, Cardiff University, Cardiff, UK
Project: Mantle Circulation Constrained (MC2): A multidisciplinary 4D Earth framework for understanding mantle upwellings.
PI: Prof. J. Huw Davies
Tectonics & Geophysics Research Group, School of Earth & Environmental Sciences, Cardiff University, Cardiff, UK
PhD Thesis: Constraining the relationship between mantle circulation and supercontinent cycles.
Supervisors: Prof. J. Huw Davies, Prof. James Wookey, Dr James Panton
School of Earth & Environment, University of Leeds, Leeds, UK
MSc Dissertation: Assessing the role of extension velocity and magmatic additions as controls on magmatic budget during rifting and rifted margin formation.
Supervisors: Dr Mohamed Gouiza, Dr Tim Craig
Awarded: Distinction
Department of Earth, Ocean, and Environmental Sciences, University of Liverpool, Liverpool, UK
BSc Dissertation: The Geological History of the Camaret-Sur-Mer Region of the Crozon Peninsula.
Supervisors: Dr Paul Wallace, Prof Peter Burgess
Awarded: 1st Class
Abstract: The relationship between the lithosphere and the mantle during the supercontinent cycle is complex and poorly constrained. The processes which drive dispersal are often simplified to two end members: slab pull and plume push. We aim to explore how lithosphere thickness and viscosity during supercontinent assembly may affect the interaction of deep mantle structures throughout the supercontinent cycle. We consider supercontinental lithosphere structure as one of many potential processes which may affect the evolution of upwellings and downwellings and therefore systematically vary the properties of continental and cratonic lithosphere, respectively within our 3D spherical simulations. The viscosity and thickness of the lithosphere alters the dip and trajectory of downwelling material beneath the supercontinent as it assembles. Focusing on Pangea, we observe that plumes evolve and are swept beneath the center of the supercontinent by circum-continental subduction. The proximity of these upwelling and downwelling structures beneath the supercontinent interior varies with lithosphere thickness and viscosity. Where slabs impinge on the top of an evolving plume head (when continental and cratonic lithosphere are thick and viscous in our simulations), the cold slabs can reduce the magnitude of an evolving plume. Conversely, when the continental lithosphere is thin and weak in our simulations, slab dips shallow in the upper mantle and descend adjacent to the evolving plume, sweeping it laterally near the core-mantle boundary. These contrasting evolutions alter the magnitude of the thermal anomaly and the degree to which the plume can thin the lithosphere prior to breakup.
Abstract: Mantle circulation in the Earth acts to remove heat from its interior and is thus a critical driver of our planet’s internal and surface evolution. Numerical mantle circulation models (MCMs) driven by plate motion history allow us to model relevant physical and chemical processes and help answer questions related to mantle properties and circulation. Predictions from MCMs can be tested using a variety of observations. Here, we illustrate how the combination of many disparate observations leads to constraints on mantle circulation across space and time. We present this approach by first describing the set-up of the example test MCM, including the parameterization of melting, and the methodology used to obtain elastic Earth models. We subsequently describe different constraints, that either provide information about present-day mantle (e.g. seismic velocity structure and surface deflection) or its temporal evolution (e.g. geomagnetic reversal frequency, geochemical isotope ratios and temperature of upper mantle sampled by lavas). We illustrate the information that each observation provides by applying it to a single MCM. In future work, we shall apply these observational constraints to a large number of MCMs, which will allow us to address questions related to Earth-like mantle circulation.
Abstract: We use a multidisciplinary approach to investigate how the parameter space of mantle convection affects present-day mantle composition. We compare 22 forward geodynamical mantle circulation model simulations against 24 variants of a geochemical inversion model of the global radiogenic isotope data set of mantle-derived lavas. Both models are fully independent but able to output compositional parameters for the lower mantle sampled by upwelling mantle plumes and for the upper mantle sampled by mid-oceanic ridges. Geodynamical model results suggest an excess degree of peridotite melt-depletion ΔFd = +0.4% ± 0.4% and an excess amount of recycled crust ΔfRC = +2.7% ± 3.1% in plumes compared to ridges, while the geochemical inversion returns ΔFd = +0.4% ± 1.2% and ΔfRC = +1.5% ± 0.6%. Models are thus in quantitative agreement but with opposite sensitivities, allowing to restrict their respective parameter space. Geodynamical runs show best fits with the narrow geochemical ΔfRC for core-mantle boundary (CMB) temperatures of 3,400–3,800 K and a recycled crust buoyancy number of 0.44–0.66. A dense primordial layer at the CMB also leads to a better fit. Variants of our geochemical model show a best fit with the narrow geodynamical ΔFd value when early mantle differentiation occurs in the garnet stability field. We also find that the formation of early compositional heterogeneities is needed to fully explain the isotope range of mantle melts. Our work emphasizes the need to correct isotopic data for the effects of non-magmatic processes in a quantitative geochemical model before extracting the parameters relevant to a comparison with geodynamical model results.
Plimmer, A., Davies, J.H. The Superpile Cycle: the mobility of LLSVPs in response to plate tectonics. Submitted to Nature Geoscience.
Throughout my time at Cardiff University I have facilitated teaching on a range of undergraduate modules. I am committed to creating an inclusive and supportive learning environment which encourages students to become independent learners, and have explored this through my participation in the AdvanceHE-accredited Cardiff University Education Associate Fellow Programme.
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