EGU24-13498, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-13498
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Real-time Ambient Seismic Noise Tomography of the Hillside IOCG Deposit

Tim Jones1, Gerrit Olivier1, Bronwyn Murphy1, Martin Gal1, Nick Smith1, Brooke North1, Darren Burrows1, Lachlan Cole2, Craig Went2, and Steven Olsen2
Tim Jones et al.
  • 1Fleet Space Technologies, Australia
  • 2Rex Minerals, Australia

We use ambient noise tomography (ANT) to image the Hillside Iron-Ore-Copper-Gold (IOCG) deposit at prospect-scale, leveraging Fleet's direct-to-satellite technology for real-time data analysis. Our results capture aspects of the deposit's known geology, including depth of cover, structures linked to mineralisation, and the mineralised host rock, and identifies several new features, including the behavior of key structures down to 1 km depth and lithological variation that underlies the Hillside deposit. Results are compared to existing magnetic, gravity, induced-polarization and drilling data. An analysis of model convergence rates with respect to environmental noise conditions (signal-to-noise ratio) shows that real-time analysis can reduce data collection at the site to within 50% of traditional deployment times. We conclude by commenting on the efficacy of ANT for IOCG exploration more broadly.

How to cite: Jones, T., Olivier, G., Murphy, B., Gal, M., Smith, N., North, B., Burrows, D., Cole, L., Went, C., and Olsen, S.: Real-time Ambient Seismic Noise Tomography of the Hillside IOCG Deposit, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13498, https://doi.org/10.5194/egusphere-egu24-13498, 2024.