Abstract
We evaluate four mantle convection models that use tectonic reconstructions to specify kinematic boundary conditions to explore the development of the lower mantle large low shear velocity provinces (LLSVP) structures and their relationship with mantle plumes. Evolution of mantle plumes in our spherical models is broadly consistent with observations including the number of plumes generated and their physical properties, trajectories, and timings. Broad modeled anomalously dense structures (MADS) form at the base of the mantle in similar locations to the African and Pacific LLSVPs and the Perm Anomaly in all models, with boundaries deforming at mean rates of 8–12km Myr−1. The western and southern walls of the African LLSVP remain relatively stable over time in our models—these edges are associated with the majority of kimberlites previously interpreted as evidence for African LLSVP stability. Our models highlight that these slow moving LLSVP edges are not representative of their overall stability and that edges proximal to subduction zones are significantly more prone to migration.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.