TY - JOUR
T1 - Unsupervised machine learning and depth clusters of Euler deconvolution of magnetic data
T2 - a new approach to imaging geological structures
AU - Chukwu, Chibuzo
AU - Betts, Peter
AU - Moore, David
AU - Munukutla, Radhakrishna
AU - Armit, Robin
AU - McLean, Mark
AU - Grose, Lachlan
N1 - Funding Information:
The authors thank Geoscience Australia and Geological Survey Victoria for providing and maintaining publicly available high-resolution magnetic data. This study was supported by the Australian Society of Exploration Geophysics Foundation Grant (RF21P01) and Monash-IITB scholarship awarded to Chukwu. We also thank the editor, Mark Lackie, the associate editor, Sam Matthews, and three additional anonymous reviewers for their constructive comments that have helped improved the manuscript.
Publisher Copyright:
© 2024 Australian Society of Exploration Geophysicists.
PY - 2024
Y1 - 2024
N2 - We present a novel approach that determines the location and dip of geologic structures by clustering Euler deconvolution depth solutions using Density-Based Spatial Clustering Applications with Noise (DBSCAN). This method and workflow rely on the association of changes in the location and relationships between Euler depth clusters and cluster boundaries with changes in rock susceptibility. We applied our method to global magnetic and high-resolution aeromagnetic datasets over Phanerozoic-Precambrian zone-bounding faults in west and central Victoria. The architecture of these structures at different scales from this imaging technique is comparable to interpreted 2D seismic reflection data. The results from the global magnetic data resolved the architecture of these structures below 5 km, while the aeromagnetic data used were limited to structural information of faults above 2 km depth. Therefore, this method shows the structural relationship of the west-dipping Avoca Fault that soles into the east-dipping Moyston Fault at a depth of ∼22 km in central Victoria and at a shallower depth of ∼15 km southward beneath the Quaternary basaltic rocks of the Newer Volcanic Province. In the vicinity of the Heathcote Zone, the method resolves the location, dip, and overprinting relationship between faults and extrusive rocks, such as the relationship between the Heathcote and Mount William Faults and the granitic Cobaw Batholith. We show how combining magnetic data at various scales can track faults from the near-surface to deeper roots while avoiding possible over-interpretation. We demonstrate how to optimise the DBSCAN parameters and a sensitivity analysis of how to determine clusters and cluster boundaries that are geologically relevant in the absence of geological constraints. Our technique provides an effective and rapid tool for imaging structures and can supplement complex and expensive imaging techniques to resolve the architecture of structures in complex geologic terrains.
AB - We present a novel approach that determines the location and dip of geologic structures by clustering Euler deconvolution depth solutions using Density-Based Spatial Clustering Applications with Noise (DBSCAN). This method and workflow rely on the association of changes in the location and relationships between Euler depth clusters and cluster boundaries with changes in rock susceptibility. We applied our method to global magnetic and high-resolution aeromagnetic datasets over Phanerozoic-Precambrian zone-bounding faults in west and central Victoria. The architecture of these structures at different scales from this imaging technique is comparable to interpreted 2D seismic reflection data. The results from the global magnetic data resolved the architecture of these structures below 5 km, while the aeromagnetic data used were limited to structural information of faults above 2 km depth. Therefore, this method shows the structural relationship of the west-dipping Avoca Fault that soles into the east-dipping Moyston Fault at a depth of ∼22 km in central Victoria and at a shallower depth of ∼15 km southward beneath the Quaternary basaltic rocks of the Newer Volcanic Province. In the vicinity of the Heathcote Zone, the method resolves the location, dip, and overprinting relationship between faults and extrusive rocks, such as the relationship between the Heathcote and Mount William Faults and the granitic Cobaw Batholith. We show how combining magnetic data at various scales can track faults from the near-surface to deeper roots while avoiding possible over-interpretation. We demonstrate how to optimise the DBSCAN parameters and a sensitivity analysis of how to determine clusters and cluster boundaries that are geologically relevant in the absence of geological constraints. Our technique provides an effective and rapid tool for imaging structures and can supplement complex and expensive imaging techniques to resolve the architecture of structures in complex geologic terrains.
KW - Euler deconvolution
KW - Fault architecture
KW - magnetic data
KW - unsupervised machine learning
UR - http://www.scopus.com/inward/record.url?scp=85181466738&partnerID=8YFLogxK
U2 - 10.1080/08123985.2023.2299475
DO - 10.1080/08123985.2023.2299475
M3 - Article
AN - SCOPUS:85181466738
SN - 0812-3985
VL - 55
SP - 223
EP - 245
JO - Exploration Geophysics
JF - Exploration Geophysics
IS - 3
ER -