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Multi-observable Thermochemical Tomography: new advances and applications to the Superior and North Australian cratons
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  • Ilya Fomin,
  • Juan Carlos Afonso,
  • Alexei Gorbatov,
  • Farshad Salajegheh,
  • Riddhi Dave,
  • Fiona Ann Darbyshire,
  • Steven Hansen,
  • Babak Hejrani,
  • Marcus W. Haynes,
  • Karol Czarnota
Ilya Fomin
Macquarie University
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Juan Carlos Afonso
University of Twente

Corresponding Author:[email protected]

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Alexei Gorbatov
Geoscience Australia
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Farshad Salajegheh
University of Newcastle Australia
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Riddhi Dave
Geological Survey of Canada
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Fiona Ann Darbyshire
Centre de recherche GEOTOP, Université du Québec à Montréal (UQAM), Canada
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Steven Hansen
Macquarie University
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Babak Hejrani
Australian National University
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Marcus W. Haynes
Australian National University
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Karol Czarnota
Geoscience Australia
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Abstract

Imaging the Earth’s thermochemical structure is crucial for understanding its dynamics and evolution. Moreover, the increased demand for critical minerals and geothermal energy driven by the energy transition has intensified the need for reliable subsurface models. Multi-Observable Thermochemical Tomography (MTT) is a simulation-based, probabilistic inversion platform designed to harness the combined sensitivities of multiple geophysical datasets and thermodynamic modelling. It produces internally-consistent estimates of the Earth’s interior as probability distributions, offering a powerful means for uncertainty quantification. Here, we present an updated MTT formalism and assess its benefits and limitations to image the thermochemical structure of the lithosphere-asthenosphere system. Individual and combined sensitivities of different observables to parameters of interest (e.g. temperature, composition, crustal architecture) are explored using challenging synthetic models. Our findings demonstrate that a judicious combination of observables can retrieve complex thermochemical structures relevant to greenfields exploration. We then apply MTT to study two cratonic regions of geological and economic significance. In the Superior Craton, we jointly invert receiver functions, gravity anomalies, gravity gradients, geoid anomalies, Rayleigh-wave dispersion curves, absolute elevation and surface heat flow. In the North Australian Craton, we incorporate new data from the Ausarray and add teleseismic P- and S-phase travel times to the datasets. The imaged lithospheric architectures provide new insights into the tectonic evolution of these two regions and the physical meaning of geophysical signatures. Additionally, these models offer unique proxies to guide exploration efforts for clean energy and critical minerals and serve as reference models for future high-resolution studies.
10 Jul 2024Submitted to ESS Open Archive
11 Jul 2024Published in ESS Open Archive