DI009-06
Magma transport beneath mid-ocean ridges

Wednesday, 9 December 2020: 10:50
Virtual
Shi Joyce Sim, Georgia Institute of Technology Main Campus, Atlanta, GA, United States, Marc W Spiegelman, Columbia University, New York, NY, United States, Dave R Stegman, University of California San Diego, La Jolla, CA, United States, Cian R Wilson, Lamont -Doherty Earth Observatory, Palisades, NY, United States, Ross Parnell-Turner, Scripps Institution of Oceanography, La Jolla, United States and Jean-Arthur L Olive, WHOI, Woods Hole, MA, United States; Ecole Normale Supérieure Paris/CNRS, Laboratoire de géologie, Paris, France
Abstract:
Melt transport beneath the lithosphere is elusive. With a distinct viscosity and density from the surrounding mantle, magmatic melt moves on a different time scale as the surrounding mantle. To resolve the temporal scale necessary to accurately capture melt transport in the mantle, the model simulations become numerically expensive quickly. Recent computational advances make possible two-phase numerical explorations to understand magma transport in the mantle. We briefly review results from a suite of two-phase models applied to the mid-ocean ridges, where we varied half-spreading rate and intrinsic mantle permeability using new openly available models, with the goal of understanding melt focusing beneath mid-ocean ridges and its relevance to the lithosphere-asthenosphere boundary (LAB). Here, we highlight the importance of viscosities for the melt focusing mechanisms. In addition, Magmatic porosity waves that are a natural consequence of these two-phase flow formulations. We show that these waves could explain long-period temporal variations in the seafloor bathymetry at the Southeast Indian Ridge. We conclude by comparing how the one-way coupled models are more numerically efficient than the fully coupled equations.