ORCID Profile
0000-0002-1767-8593
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Geology | Earth Sciences Not Elsewhere Classified | Basin Analysis | Geodynamics | Tectonics | Simulation And Modelling | Geophysics | Geochemistry | Artificial Intelligence and Image Processing | Geochronology And Isotope Geochemistry | Inorganic Geochemistry | Exploration Geochemistry | Structural Geology | Geotectonics | Instruments And Techniques | Electrical and Electromagnetic Methods in Geophysics | Inorganic Geochemistry Not Elsewhere Classified | Data Structures | Other Physical Sciences | Simulation and Modelling | Geochemistry Not Elsewhere Classified
Earth sciences | Mineral Exploration not elsewhere classified | Copper Ore Exploration | Information processing services | Application packages | Atmospheric composition | Oil and Gas Exploration | Oil Shale and Tar Sands Exploration | Expanding Knowledge in the Earth Sciences | Titanium Minerals, Zircon, and Rare Earth Metal Ore (e.g. Monazite) Exploration |
Publisher: Elsevier BV
Date: 02-2020
Publisher: Geological Society of America
Date: 05-2009
DOI: 10.1130/G25460A.1
Publisher: Copernicus GmbH
Date: 26-06-2019
Abstract: Abstract. Species distribution and richness ultimately result from complex interactions between biological, physical and environmental factors. It has been recently shown for a static natural landscape that the elevational connectivity, which measures the proximity of a site to others with similar habitats, is a key physical driver of local species richness. Here we examine changes in elevational connectivity during mountain building using a landscape evolution model. We find that under uniform tectonic and variable climatic forcing, connectivity peaks at mid-elevations when the landscape reaches its geomorphic steady-state and that orographic effect on geomorphic evolution tends to favour low connectivity on leeward facing catchments. Statistical comparisons between connectivity distribution and results from a metacommunity model confirm that landscape elevation connectivity explains to the first order species richness in simulated mountainous regions. Our results also predict that low connectivity areas which favour isolation, a driver for in-situ speciation, are distributed across the entire elevational range for simulated orogenic cycles. Rapid adjustments of catchment morphology after cessation of tectonic activity should reduce speciation by decreasing the number of isolated regions.
Publisher: Springer Science and Business Media LLC
Date: 11-09-2020
DOI: 10.1038/S41467-020-18448-Y
Abstract: During extension, the continental lithosphere thins and breaks up, forming either wide or narrow rifts depending on the thermo-mechanical state of the extending lithosphere. Wide continental rifts, which can reach 1,000 km across, have been extensively studied in the North American Cordillera and in the Aegean domain. Yet, the evolutionary process from wide continental rift to continental breakup remains enigmatic due to the lack of seismically resolvable data on the distal passive margin and an absence of onshore natural exposures. Here, we show that Eocene extension across the northern margin of the South China Sea records the transition between a wide continental rift and highly extended ( km) continental margin. On the basis of high-resolution seismic data, we document the presence of dome structures, a corrugated and grooved detachment fault, and subdetachment deformation involving crustal-scale nappe folds and magmatic intrusions, which are coeval with supradetachment basins. The thermal and mechanical weakening of this broad continental domain allowed for the formation of metamorphic core complexes, boudinage of the upper crust and exhumation of middle/lower crust through detachment faulting. The structural architecture of the northern South China Sea continental margin is strikingly similar to the broad continental rifts in the North American Cordillera and in the Aegean domain, and reflects the transition from wide rift to continental breakup.
Publisher: Geological Society of America
Date: 08-12-2018
DOI: 10.1130/G39674.1
Publisher: Elsevier BV
Date: 2021
Publisher: Geological Society of America
Date: 21-12-2013
DOI: 10.1130/B30754.1
Publisher: Wiley
Date: 14-12-2022
DOI: 10.1111/TER.12637
Abstract: Dynamic subsidence and uplift of plates are often explained by the vertical motion of density anomalies in the mantle. Such models predict surface vertical motion rates of less than 100 m Myr −1 at long‐wavelengths with a timespan of tens of Myr. However, during periods of relative sea‐level stability, some of the phases of vertical motion on stable portions of plates have occurred at rates greater than 100 m Myr −1 during episodes that may last only a few Myr. Here, we show that vertical surface motions, with rates greater than 100 m Myr −1 and durations less than a few Myr, can be explained by changes in basal shear stress caused by variation in horizontal motion of a viscous plate relative to the asthenosphere. We apply our physical model to the short‐lived mid‐Eocene immersion of the southern margin of Australia.
Publisher: Informa UK Limited
Date: 04-2013
Publisher: Geological Society of America
Date: 2007
DOI: 10.1130/G23240A.1
Publisher: Mineralogical Society of America
Date: 12-2016
DOI: 10.2138/AM-2016-5868
Publisher: Elsevier BV
Date: 2015
Publisher: Geological Society of London
Date: 2001
Publisher: Geological Society of America
Date: 29-11-2022
Abstract: Additional detail concerning the numerical method, internal and boundary conditions, and numerical parameters, and access to outputs of the entire suite of the numerical experiments.
Publisher: Geological Society of London
Date: 2006
Publisher: Informa UK Limited
Date: 08-1999
Publisher: Geological Society of America
Date: 09-01-2017
DOI: 10.1130/G38595.1
Publisher: Editorial Office of Earth Science
Date: 2020
Publisher: Geological Society of London
Date: 2007
DOI: 10.1144/SP282.18
Publisher: Elsevier BV
Date: 04-1994
Publisher: Elsevier BV
Date: 12-2008
Publisher: Geological Society of America
Date: 1999
Publisher: Elsevier BV
Date: 11-2015
Publisher: Geological Society of America
Date: 03-01-2023
DOI: 10.1130/G50833.1
Abstract: In the context of continental extension, transient compressional episodes (stress inversion) and phases of uplift (depth inversion) are commonly recorded with no corresponding change in plate motion. Changes in gravitational potential energy during the rifting process have been invoked as a possible source of compressional stresses, but their magnitude, timing, and relationship with depth inversions remain unclear. Using high-resolution two-dimensional numerical experiments of the full rifting process, we track the dynamic interplay between the far-field tectonic forces, loading and unloading of the surface via surface processes, and gravitational body forces. Our results show that rift basins tend to localize compressive stresses they record transient phases of compressional stresses as high as 30 MPa and experience a profound depth inversion, 2 km in magnitude, when sediment supply ceases, providing an additional driver for the breakup unconformity, a well-documented phase of regional uplift typically associated with continental breakup.
Publisher: Elsevier BV
Date: 08-2008
Publisher: Geological Society of London
Date: 1997
Publisher: Elsevier BV
Date: 08-2007
Publisher: Springer Science and Business Media LLC
Date: 21-03-2010
DOI: 10.1038/NGEO825
Publisher: Geological Society of America
Date: 12-2011
DOI: 10.1130/G32231.1
Publisher: Informa UK Limited
Date: 04-2019
Publisher: Wiley
Date: 19-02-2020
DOI: 10.1111/JMG.12523
Publisher: Elsevier BV
Date: 06-2014
Publisher: Elsevier BV
Date: 11-2008
Publisher: Springer Science and Business Media LLC
Date: 18-07-2006
Publisher: Geological Society of America
Date: 10-2012
DOI: 10.1130/G33202Y.1
Publisher: Springer Science and Business Media LLC
Date: 23-06-2008
Publisher: American Geophysical Union (AGU)
Date: 19-12-2019
DOI: 10.1029/2019GL084400
Publisher: Wiley
Date: 14-01-2022
DOI: 10.1111/TER.12577
Abstract: Long‐lived high to ultra‐high temperature (HT‐UHT) granulitic terranes formed throughout Earth's history. Yet, the detailed processes involved in their formation remain unresolved and notably the sequence of appearance and duration of migmatisation and granulites conditions in the orogenic cycle. These processes can be evaluated by analytical and numerical models. First, solving the steady‐state heat equation allows underlining the interdependency of the parameters controlling the crustal geotherm at thermal equilibrium. Second, performing two‐dimensional thermo‐mechanical experiments of an orogenic cycle, from shortening to gravitational collapse, allows to consider non‐steady‐state geotherms and understand how deformation velocity may affect the relative timing of migmatite and granulite formation. These numerical experiments with elevated radiogenic heat production and slow shortening rates allow the formation of large volumes of prograde migmatites and granulites going through the sillimanite field as observed in many HT‐UHT terranes. Finally, the interplay between these parameters can explain the difference in predicted pressure‐temperature‐time paths that can be compared with the natural rock archive.
Publisher: Geological Society of America
Date: 29-11-2022
DOI: 10.1130/GEOL.S.21644681.V1
Abstract: Additional detail concerning the numerical method, internal and boundary conditions, and numerical parameters, and access to outputs of the entire suite of the numerical experiments.
Publisher: GeoScienceWorld
Date: 04-02-2023
DOI: 10.2113/2023/8503619
Abstract: Warmer conditions prevalent in the hinterland of orogenic systems facilitate local ductile flow underneath the surface load, making Airy-like local isostasy more prevalent in these domains. In contrast, flexural isostasy better describes the regional response to surface loading of more rigid lithospheres. Here, we explore how the interaction between horizontal tectonic mass transfer and vertical isostatic mass transfer, through either elastic flexure or viscous flow, impacts the overall architecture of fold and thrust belts. We compare numerical models of fold and thrust belts under either an Airy-like ductile isostasy boundary condition or a flexural-like regional isostasy boundary condition. Our experiments suggest that when ductile flow is involved in accommodating isostatic adjustment, subsidence is rather local, larger, and results in narrower, less elevated fold-thrust belts with a complex internal architecture consisting of prominent steeply dipping faults. When isostatic subsidence is controlled by lithospheric flexure, the tilting of the basement on 10 s of km scale facilitates the outward propagation of fold-thrust belts. The internal architecture is simpler and involves prominent basement-parallel décollements. The outcome is wider fold and thrust belts with higher topographies. A change in lithospheric elastic thickness does not significantly affect fold-thrust belt structural styles. Our results are compared to natural ex les from the Subandean zone.
Publisher: Elsevier BV
Date: 06-2009
Publisher: Geological Society of America
Date: 04-2015
Publisher: Geological Society of America
Date: 2008
DOI: 10.1130/G25031A.1;
Publisher: GeoScienceWorld
Date: 10-2010
DOI: 10.1130/L114.1
Publisher: Cambridge University Press (CUP)
Date: 02-04-2012
DOI: 10.1017/S0016756812000131
Abstract: The 3.46 Ga Marble Bar Chert Member of the East Pilbara Craton, Western Australia, is one of the earliest and best-preserved sedimentary successions on Earth. Here, we interpret the finely laminated thin-bedded cherts, mixed conglomeratic beds, chert breccia beds and chert folded beds of the Marble Bar Chert Member as the product of low-density turbidity currents, high-density turbidity currents, mass transport complexes and slumps, respectively. Integrated into a channel-levee depositional model, the Marble Bar Chert Member constitutes the oldest documented deep-sea fan on Earth, with thin-bedded cherts, breccia beds and slumps composing the outer levee facies tracts, and scours and conglomeratic beds representing the channel systems.
Publisher: Geological Society of America
Date: 2007
DOI: 10.1130/G23540A.1
Publisher: Informa UK Limited
Date: 02-2012
Publisher: American Association for the Advancement of Science (AAAS)
Date: 03-03-2023
Abstract: Our capability to reconstruct past landscapes and the processes that shape them underpins our understanding of paleo-Earth. We take advantage of a global-scale landscape evolution model assimilating paleoelevation and paleoclimate reconstructions over the past 100 million years. This model provides continuous quantifications of metrics critical to the understanding of the Earth system, from global physiography to sediment flux and stratigraphic architectures. We reappraise the role played by surface processes in controlling sediment delivery to the oceans and find stable sedimentation rates throughout the Cenozoic with distinct phases of sediment transfer from terrestrial to marine basins. Our simulation provides a tool for identifying inconsistencies in previous interpretations of the geological record as preserved in sedimentary strata, and in available paleoelevation and paleoclimatic reconstructions.
Publisher: Geological Society of America
Date: 12-05-2017
DOI: 10.1130/G39229Y.1
Publisher: Elsevier BV
Date: 02-2018
Publisher: Copernicus GmbH
Date: 28-06-2019
Abstract: Abstract. The sedimentary architecture at continental margins reflects the interplay between the rate of change of accommodation creation (δA) and the rate of change of sediment supply (δS). Stratigraphic interpretation increasingly focuses on understanding the link between deposition patterns and changes in δA∕δS, with an attempt to reconstruct the contributing factors. Here, we use the landscape modelling code pyBadlands to (1) investigate the development of stratigraphic sequences in a source-to-sink context (2) assess the respective performance of two well-established stratigraphic interpretation techniques: the trajectory analysis method and the accommodation succession method and (3) propose quantitative stratigraphic interpretations based on those two techniques. In contrast to most stratigraphic forward models (SFMs), pyBadlands provides self-consistent sediment supply to basin margins as it simulates erosion, sediment transport and deposition in a source-to-sink context. We present a generic case of landscape evolution that takes into account periodic sea level variations and passive margin thermal subsidence over 30 million years, under uniform rainfall. A set of post-processing tools are provided to analyse the predicted stratigraphic architecture. We first reconstruct the temporal evolution of the depositional cycles and identify key stratigraphic surfaces based on observations of stratal geometries and facies relationships, which we use for comparison to stratigraphic interpretations. We then apply both the trajectory analysis and the accommodation succession methods to manually map key stratigraphic surfaces and define sequence units on the final model output. Finally, we calculate shoreline and shelf-edge trajectories, the temporal evolution of changes in relative sea level (proxy for δA) and sedimentation rate (proxy for δS) at the shoreline, and automatically produce stratigraphic interpretations. Our results suggest that the analysis of the presented model is more robust with the accommodation succession method than with the trajectory analysis method. Stratigraphic analysis based on manually extracted shoreline and shelf-edge trajectory requires calibrations of time-dependent processes such as thermal subsidence or additional constraints from stratal terminations to obtain reliable interpretations. The 3-D stratigraphic analysis of the presented model reveals small lateral variations of sequence formations. Our work provides an efficient and flexible quantitative sequence stratigraphic framework to evaluate the main drivers (climate, sea level and tectonics) controlling sedimentary architectures and investigate their respective roles in sedimentary basin development.
Publisher: Geological Society of America
Date: 04-2011
DOI: 10.1130/G31587.1
Publisher: Geological Society of America
Date: 2007
DOI: 10.1130/G24480Y.1
Publisher: Elsevier BV
Date: 12-2001
Publisher: Elsevier BV
Date: 02-2015
Publisher: Elsevier BV
Date: 11-2009
Publisher: Geological Society of America
Date: 17-04-2020
DOI: 10.1130/G47301.1
Abstract: Away from tectonically active regions, the continental crust has an average thickness of 40 ± 1 km. Yet, it shows a remarkable variability from 25 to 65 km, comparable to that of the most tectonically active regions. Here, we consider the problem of the formation and preservation of anomalous deep crustal roots in stable intracontinental regions. Using two-dimensional thermomechanical experiments, we show that the interplay between partial melting, the formation of garnet-pyroxene-bearing rocks, and their strain rate–dependent retrogression result in the preservation of thick and strong crustal roots. We argue that it is the partitioning into narrow regions of strain, retrogression, and weakening coupled into a positive feedback loop that explains why strong high-grade crustal roots remain largely immune to gravitational stresses and are able to persist over hundreds of millions of years.
Publisher: American Geophysical Union (AGU)
Date: 10-03-1994
DOI: 10.1029/93JB03105
Publisher: The Open Journal
Date: 11-04-2019
DOI: 10.21105/JOSS.01136
Publisher: Frontiers Media SA
Date: 20-12-2021
DOI: 10.3389/FEART.2021.696674
Abstract: The lithospheric build-up of the African continent is still to a large extent unexplored. In this contribution, we present a new Moho depth model to discuss the architecture of the three main African cratonic units, which are: West African Craton, Congo Craton, and Kalahari Craton. Our model is based on a two-step gravity inversion approach that allows variable density contrasts across the Moho depth. In the first step, the density contrasts are varied for all non-cratonic units, in the second step for the three cratons in idually. The lateral extension of the tectonic units is defined by a regionalization map, which is calculated from a recent continental seismic tomography model. Our Moho depth is independently constrained by pointwise active seismics and receiver functions. Treating the constraints separately reveals a variable range of density contrasts and different trends in the estimated Moho depth for the three cratons. Some of the estimated density contrasts vary substantially, caused by sparse data coverage of the seismic constraints. With a density contrast of Δ ρ = 200 kg/ m 3 the Congo Craton features a cool and undisturbed lithosphere with smooth density contrasts across the Moho. The estimated Moho depth shows a bimodal pattern with average Moho depth of 39–40 km for the Kalahari and Congo Cratons and 33–34 km for the West African Craton. We link our estimated Moho depth with the cratonic extensions, imaged by seismic tomography, and with topographic patterns. The results indicate that cratonic lithosphere is not necessarily accompanied by thick crust. For the West African Craton, the estimated thin crust, i.e. shallow Moho, contrasts to thick lithosphere. This discrepancy remains enigmatic and requires further studies.
Publisher: Springer Science and Business Media LLC
Date: 09-2014
DOI: 10.1038/NATURE13728
Abstract: Stresses acting on cold, thick and negatively buoyant oceanic lithosphere are thought to be crucial to the initiation of subduction and the operation of plate tectonics, which characterizes the present-day geodynamics of the Earth. Because the Earth's interior was hotter in the Archaean eon, the oceanic crust may have been thicker, thereby making the oceanic lithosphere more buoyant than at present, and whether subduction and plate tectonics occurred during this time is ambiguous, both in the geological record and in geodynamic models. Here we show that because the oceanic crust was thick and buoyant, early continents may have produced intra-lithospheric gravitational stresses large enough to drive their gravitational spreading, to initiate subduction at their margins and to trigger episodes of subduction. Our model predicts the co-occurrence of deep to progressively shallower mafic volcanics and arc magmatism within continents in a self-consistent geodynamic framework, explaining the enigmatic multimodal volcanism and tectonic record of Archaean cratons. Moreover, our model predicts a petrological stratification and tectonic structure of the sub-continental lithospheric mantle, two predictions that are consistent with xenolith and seismic studies, respectively, and consistent with the existence of a mid-lithospheric seismic discontinuity. The slow gravitational collapse of early continents could have kick-started transient episodes of plate tectonics until, as the Earth's interior cooled and oceanic lithosphere became heavier, plate tectonics became self-sustaining.
Publisher: American Geophysical Union (AGU)
Date: 04-1993
DOI: 10.1029/92TC01568
Publisher: Elsevier BV
Date: 12-2004
Publisher: Geological Society of America
Date: 1995
Publisher: Elsevier BV
Date: 05-2013
Publisher: Springer Science and Business Media LLC
Date: 28-09-2022
Publisher: The Open Journal
Date: 25-07-2019
DOI: 10.21105/JOSS.01530
Publisher: Elsevier BV
Date: 11-2003
Publisher: Copernicus GmbH
Date: 20-12-2019
Abstract: Abstract. Much effort is being made to extract the dynamic components of the Earth's topography driven by density heterogeneities in the mantle. Seismically mapped density anomalies have been used as an input into mantle convection models to predict the present-day mantle flow and stresses applied on the Earth's surface, resulting in dynamic topography. However, mantle convection models give dynamic topography litudes generally larger by a factor of ∼2, depending on the flow wavelength, compared to dynamic topography litudes obtained by removing the isostatically compensated topography from the Earth's topography. In this paper, we use 3-D numerical experiments to evaluate the extent to which the dynamic topography depends on mantle rheology. We calculate the litude of instantaneous dynamic topography induced by the motion of a small spherical density anomaly (∼100 km radius) embedded into the mantle. Our experiments show that, at relatively short wavelengths ( km), the litude of dynamic topography, in the case of non-Newtonian mantle rheology, is reduced by a factor of ∼2 compared to isoviscous rheology. This is explained by the formation of a low-viscosity channel beneath the lithosphere and a decrease in thickness of the mechanical lithosphere due to induced local reduction in viscosity. The latter is often neglected in global mantle convection models. Although our results are strictly valid for flow wavelengths less than 1000 km, we note that in non-Newtonian rheology all wavelengths are coupled, and the dynamic topography at long wavelengths will be influenced.
Publisher: Informa UK Limited
Date: 12-2013
Publisher: Elsevier BV
Date: 05-2013
Location: France
Start Date: 2013
End Date: 2018
Funder: Australian Research Council
View Funded ActivityStart Date: 2020
End Date: 2023
Funder: Australian Research Council
View Funded ActivityStart Date: 2003
End Date: 2005
Funder: Australian Research Council
View Funded ActivityStart Date: 2005
End Date: 2006
Funder: Australian Research Council
View Funded ActivityStart Date: 2009
End Date: 2011
Funder: Australian Research Council
View Funded ActivityStart Date: 2006
End Date: 2006
Funder: Australian Research Council
View Funded ActivityStart Date: 10-2005
End Date: 10-2006
Amount: $220,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 02-2003
End Date: 12-2006
Amount: $360,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 02-2009
End Date: 12-2013
Amount: $225,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2015
End Date: 03-2021
Amount: $2,748,358.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2022
End Date: 11-2025
Amount: $490,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2006
End Date: 06-2007
Amount: $133,670.00
Funder: Australian Research Council
View Funded ActivityStart Date: 08-2020
End Date: 08-2024
Amount: $1,055,000.00
Funder: Australian Research Council
View Funded Activity