EGU23-10662
https://doi.org/10.5194/egusphere-egu23-10662
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Probabilistic ambient noise imaging of the Macquarie Ridge Complex using ocean-bottom and land-based seismometers

Thanh-Son Pham1, Hrvoje Tkalcic1, Xiaolong Ma1, Robert Pickle1, Jack Muir1,2, Kenneth Duru3, Tom Winder4, Nicholas Rawlinson4, Caroline Eakin1, Millard Coffin5, Joann Stock6, and the Macquarie Ridge 3D Team*
Thanh-Son Pham et al.
  • 1Australian National University, Research School of Earth Sciences, Canberra, ACT, Australia
  • 2University of Oxford, Department of Earth Sciences, Oxford OX1 3AN, UK
  • 3Australian National University, Mathematical Sciences Institute, Canberra, ACT, Australia
  • 4University of Cambridge, Cambridge, United Kingdom
  • 5University of Tasmania, Institute for Marine and Antarctic Studies, Hobart, TAS, Australia
  • 6California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States
  • *A full list of authors appears at the end of the abstract

The Macquarie Ridge Complex, located at the boundary between Indo-Australian and Pacific plates in the southwest Pacific Ocean, hosts the largest sub-marine earthquakes in the 20th century, not associated with ongoing subduction. We deployed 27 ocean-bottom seismometers, of which 15 have been recovered successfully, to understand the origin of the sub-marine earthquakes and their potential earthquake and tsunami hazards to Australia and New Zealand. Additionally, we deployed five land-based seismometers on Macquarie Island.

We explore state-of-the-art processing methods to analyze the new seismic dataset from the retrieved seismic stations. One of the goals is to image the tectonic settings beneath the MRC. Here, we present a first-order tomographic model and its relevant uncertainty estimate of the region constructed from ambient noise surface waves using a probabilistic inversion framework. The tomographic image will be complemented with receiver-based imaging results such as those from P-wave coda autocorrelations and receiver functions to confirm the existence of possible geometries. The results are expected to supply a fresh understanding of the tectonic settings under the MRC and unpuzzle the origin of the significant underwater earthquakes in the 20th century.

Macquarie Ridge 3D Team:

Sheng Wang, Thuany Costa de Lima, Yun Fann Toh, Haoran Du, Chuan Chuan Lu

How to cite: Pham, T.-S., Tkalcic, H., Ma, X., Pickle, R., Muir, J., Duru, K., Winder, T., Rawlinson, N., Eakin, C., Coffin, M., and Stock, J. and the Macquarie Ridge 3D Team: Probabilistic ambient noise imaging of the Macquarie Ridge Complex using ocean-bottom and land-based seismometers, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-10662, https://doi.org/10.5194/egusphere-egu23-10662, 2023.