EGU2020-10835
https://doi.org/10.5194/egusphere-egu2020-10835
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Linking thermomechanical models with geodetic observations to evaluate the 2018 eruption of Sierra Negra Volcano, Galápagos

Patricia Gregg1, Yan Zhan1, Falk Amelung2, Jack Albright1, Dennis Geist3, Patricia Mothes4, Zhang Yunjun5, and Seid Koric6
Patricia Gregg et al.
  • 1University of Illinois at Urbana-Champaign, Department of Geology, Urbana, United States of America (pgregg@illinois.edu)
  • 2Department of Marine Geosciences, Rosenstiel School of Marine and Atmospheric Sciences, University of Miami, FL, USA
  • 3Division of Earth Sciences, National Science Foundation, Alexandria, VA, USA
  • 4Instituto Geofísico, Escuela Politécnica Nacional, Quito, Ecuador
  • 5Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
  • 6Mechanical Science and Engineering, University of Illinois, Urbana, IL, USA

Ensemble based data assimilation approaches, such as the Ensemble Kalman Filter (EnKF), have been widely and successfully implemented to combine observations with dynamic models to investigate the evolution of a system’s state. Such inversions are powerful tools for providing forecasts as well as “hindcasting” events such as volcanic eruptions to investigate source parameters and triggering mechanisms. In this study, a high performance computing (HPC) adaptation of the EnKF is used to assimilate ground deformation observations from interferometric synthetic-aperture radar (InSAR) into high-fidelity, multiphysics finite element models to evaluate the prolonged unrest and June 26, 2018 eruption of Sierra Negra volcano, Galápagos. The stability of the Sierra Negra magma system is evaluated at each time step by estimating variations in reservoir overpressure, Mohr-Coulomb failure in the host rock, and tensile stress and failure along the reservoir boundary. The deformation of Sierra Negra is tracked over a decade, during which almost 5 meters of surface uplift has been recorded. The EnKF reveals that the evolution of the stress state in the host rock surrounding the Sierra Negra magma reservoir likely controlled the timing of the eruption. While increases in magma reservoir overpressure remained modest (< 10 MPa) throughout the data assimilation time period, significant Mohr-Coulomb failure is indicated in the lead up to the eruption coincident with increased seismicity along both trapdoor faults within Sierra Negra’s caldera and along the caldera’s ring faults. During the final stages of pre-eruptive unrest, the EnKF models indicate limited tensile failure, with no tensile failure along the northern portion of the magma system where the eruption commenced. Most strikingly, model calculations of significant through-going Mohr-Coulomb failure correspond in space and time with a Mw 5.4 earthquake recorded in the hours preceding the 2018 eruption. Subsequent stress modeling implicates the Mw 5.4 earthquake along the southern intra-caldera trapdoor fault as the potential catalyst for tensile failure and dike initiation along the reservoir to the north. In conclusion, the volcano EnKF approach successfully tracked the evolving stability of Sierra Negra, indicating great potential for future forecasting efforts.

How to cite: Gregg, P., Zhan, Y., Amelung, F., Albright, J., Geist, D., Mothes, P., Yunjun, Z., and Koric, S.: Linking thermomechanical models with geodetic observations to evaluate the 2018 eruption of Sierra Negra Volcano, Galápagos, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-10835, https://doi.org/10.5194/egusphere-egu2020-10835, 2020

This abstract will not be presented.