Abstract

Over the last two decades, Mineral Resources Tasmania has been developing regional 3D geological and geophysical models for prospective terranes at a range of scales and extents as part of its suite of precompetitive geoscience products. These have evolved in conjunction with developments in 3D modeling technology over that time. Commencing with a jurisdiction-wide 3D model in 2002, subsequent modeling projects have explored a range of approaches to the development of 3D models as a vehicle for the better synthesis and understanding of controls on ore-forming processes and prospectivity. These models are built on high-quality potential field data sets. Assignment of bulk properties derived from previous well-constrained geophysical modeling and an extensive rock property database has enabled the identification of anomalous features that have been targeted for follow-up mineral exploration. An aspect of this effort has been the generation of uncertainty estimates for model features. Our experience is that this process can be hindered by models that are too large or too detailed to be interrogated easily, especially when modeling techniques do not readily permit significant geometric changes. The most effective 3D modeling workflow for insights into mineral exploration is that which facilitates the rapid hypothesis testing of a wide range of scenarios whilst satisfying the constraints of observed data.

Highlights

  • We discuss the outcomes of 3D geological and geophysical modeling in Tasmania, starting with the Statewide 3D geological model released by Mineral Resources Tasmania (MRT) in 2002

  • The Mathinna Supergroup, an Ordovician to Early Devonian turbiditic sequence with cumulative stratigraphic thicknesses exceeding 10 km, is the oldest unit exposed in the Eastern Tasmanian terrane (Figure 2), Cambrian ultramafic rocks are interpreted on geophysical evidence to underlie much of the northern half of the Eastern

  • The potential field contribution from any magnetic/gravity source located beyond the extents of the local model can interfere with this model and be erroneously attributed to its response when the data are inverted

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Summary

Introduction

Publisher’s Note: MDPI stays neutral with regard to jurisdictional claims in published maps and institutional affiliations. Metrics multiple geological models facilitate that satisfy the geophysical [10] These advances allow us to quantify uncertainty (to a degree) of the geometry of geologWe detail and discuss our modeling efforts over the last decade, and present new ical units at depth through statistically generated 3D sensitivity metrics from multiple results using statistically generated 3D sensitivity metrics to address uncertainty. These geological models that satisfy the geophysical observations [10].

Tectonic
Western Tasmanian Terrane
Eastern Tasmanian Terrane
Younger Rock Sequences
Economic Geology
Inversion Methodology and Data
Reference Model Geophysical Validation
Cooperative Inversion and Sensitivity Modeling
Potential Field Data Preparation—Regional-Residual Separation
Data Sources
Rock Physical Properties
Construction
Analysis
Impact
Western Tasmanian Terrane Models
Rosebery Region
Forward and Inverse Modeling
Magnetic Response
Gravity Response
Rosebery–Lyell
11. Three-dimensional schematic illustrating the complexity of the Rosebery–Lyell
Outcomes
14. Forward
Reference Model Magnetic and Gravity Modeling
Cooperative Potential Field Inversion
Tributary Creek Gravity Anomaly
Rosebery North
Heazlewood–Luina–Waratah
18. Carbonate
Northwest Tasmania
Cooperative Geophysical Inversion
Second Phase Implicit Modeling
Alberton–Mathinna
21. Gravity mapgravity draped over
Scamander
Cooperative
23. Discretized model of 3D the model
Inversion Analysis—Great Pyramid Tin and Other Deposits
Findings
Conclusions
Full Text
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