Numerical Experiments

Computational experiments
in geodynamics

Thermomechanical numerical models run on supercomputers, simulating millions of years of tectonic evolution to study processes that cannot be directly observed.

01 Thermomechanical

Fold-Thrust Belt — Local Isostasy

When ductile flow accommodates isostatic adjustment beneath a fold-thrust belt, subsidence is local and large, producing a narrower, less elevated belt with steeply dipping faults and a complex internal architecture.

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02 Thermomechanical

Fold-Thrust Belt — Flexural Isostasy

When lithospheric flexure controls isostatic subsidence, basement tilting on tens-of-kilometre scales facilitates outward propagation of the fold-thrust belt, producing a wider, higher belt with simpler architecture and prominent basement-parallel décollements.

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03 Geodynamic

Contractional Gravitational Collapse

Convergent gravitational collapse of a deep intracratonic rift basin. The gravitational potential anomaly relaxes inward, simultaneously driving doming in the extensional domain and nappe emplacement in the contractional domain — linking the Entia Dome and Arltunga Nappe Complex.

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04 Thermomechanical

Narrow Rift — 600°C Moho

Under a colder geotherm representative of modern conditions, extension localises into a narrow rift defined by conjugate normal faults that evolve into listric detachments merging at the brittle-ductile transition.

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05 Thermomechanical

Wide Rift — 800°C Moho

Under a warmer geotherm representative of Proterozoic conditions, extension distributes across a broad zone, forming a wide rift through distributed upper crustal faulting and ductile flow in the underlying lithosphere.

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06 Thermomechanical

Narrow Rift Inversion — 600°C Moho

After 60 Myr of tectonic quiescence, the narrow rift is compressed and inverts into a localised orogenic wedge flanked by foreland basins, largely reactivating the pre-existing rift architecture.

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07 Thermomechanical

Wide Rift Inversion — 800°C Moho

After 60 Myr of quiescence, lithospheric cooling and embrittlement transform the wide rift inversion. Coupling between upper crustal faults and upper mantle shear zones produces a broad, low-relief orogenic plateau with 10–20 km of Moho offset — a framework that may explain distributed shortening in Proterozoic orogens.

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Interactive 3D Models

Structural geometry
from field data

Geometric reconstructions built from field observations and structural mapping in Central Australia. Drag to rotate, pinch to zoom.

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3D Geological Model · Central Australia

Arltunga Nappe Complex

Folded nappes from the Arltunga Nappe Complex, central Australia. The structure records the emplacement of large allochthonous sheets driven by gravitational potential energy during crustal thickening.

The model shows the interference geometry of the nappe system and integrates field structural data with geometric constraints to reconstruct the pre-erosional architecture.

Proterozoic Nappe Complex Gravity-driven Central Australia

3D Cross-Section · Central Australia

Entia Dome

Cross-sectional architecture of the Entia Dome, a gneiss dome with an internal double-dome structure from the Arunta Region, central Australia. The model shows the structural relationships between the core gneisses and surrounding metasedimentary sequences.

Gneiss domes of this type form by gravity-driven flow in thickened orogenic crust, where buoyant lower-crustal material rises through denser overlying rocks to produce the dome-and-keel geometry.

Gneiss Dome Double-Dome Entia Dome Cross-Section