ORCID Profile
0000-0002-3953-7783
Current Organisation
University of South Australia
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In Research Link Australia (RLA), "Research Topics" refer to ANZSRC FOR and SEO codes. These topics are either sourced from ANZSRC FOR and SEO codes listed in researchers' related grants or generated by a large language model (LLM) based on their publications.
Geochemistry | Isotope Geochemistry | Marine and Estuarine Ecology (incl. Marine Ichthyology) | Geology | Exploration Geochemistry | Ore Deposit Petrology | Proteomics and Intermolecular Interactions (excl. Medical Proteomics) | Environmental Chemistry (incl. Atmospheric Chemistry) | Environmental Monitoring | Basin Analysis | Igneous and Metamorphic Petrology | Geochronology | Tectonics
Mineral Exploration not elsewhere classified | Physical and Chemical Conditions of Water in Fresh, Ground and Surface Water Environments (excl. Urban and Industrial Use) | Expanding Knowledge in the Earth Sciences | Copper Ore Exploration | Oil and Gas Exploration | Precious (Noble) Metal Ore Exploration | Cancer and Related Disorders | Marine Flora, Fauna and Biodiversity | Ecosystem Assessment and Management of Marine Environments |
Publisher: American Association for the Advancement of Science (AAAS)
Date: 10-05-2019
Abstract: Vertebrates are typically thought to have a consistent system for processing light, in which multiple cone opsins permit color vision during the day, but a single rod opsin provides only monochrome vision in the dark. Musilova et al. analyzed more than 100 deep-sea fish genomes and found a previously unknown proliferation of rod opsin genes that generate rod opsin photopigments that are tuned to different wavelengths of light. These receptors may allow the fish to perceive bioluminescent signals that pervade their deep-sea environment. These results reveal a previously undescribed visual system that allows for color vision in the dark. Science , this issue p. 588
Publisher: Proceedings of the National Academy of Sciences
Date: 29-12-2014
Abstract: Gene and whole-genome duplications are important evolutionary forces promoting organismal ersification. Teleost fishes, for ex le, possess many gene duplicates responsible for photoreception (opsins), which emerged through gene duplication and allow fishes to adapt to the various light conditions of the aquatic environment. Here, we reevaluate the evolutionary history of the violet-blue–sensitive opsins [short wavelength-sensitive 2 (SWS2)] in modern teleosts using next generation genome sequencing. We uncover a gene duplication event specific to the most erse lineage of vertebrates (the percomorphs) and show that SWS2 evolution was highly dynamic and involved gene loss, pseudogenization, and gene conversion. We, thus, clarify previous discrepancies regarding opsin annotations. Our study highlights the importance of integrative approaches to help us understand how species adapt and ersify.
Publisher: Informa UK Limited
Date: 12-2007
Publisher: Elsevier BV
Date: 2011
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 07-2015
Publisher: Elsevier BV
Date: 08-2011
Publisher: Elsevier BV
Date: 03-2022
Publisher: Elsevier BV
Date: 02-2015
Publisher: Elsevier BV
Date: 08-2014
Publisher: MDPI AG
Date: 29-08-2017
Publisher: Geological Society of America
Date: 27-02-2014
DOI: 10.1130/B30977.1
Publisher: American Geophysical Union (AGU)
Date: 03-2021
DOI: 10.1029/2020TC006498
Publisher: Informa UK Limited
Date: 11-06-2018
Publisher: Geological Society of America
Date: 30-07-2014
DOI: 10.1130/B30842.1
Publisher: Elsevier BV
Date: 06-2017
Publisher: Springer Science and Business Media LLC
Date: 16-03-2017
Publisher: Public Library of Science (PLoS)
Date: 30-08-2016
Publisher: Cambridge University Press (CUP)
Date: 23-12-2020
DOI: 10.1017/S0016756820001223
Abstract: The c. 1.5–1.3 Ga Wilton package, the upper succession of the greater McArthur Basin, preserves detailed tectono-sedimentary evidence for the Mesoproterozoic evolution of the North Australian Craton (NAC). In addition, it is a valuable global sedimentary repository for the poorly explored Mesoproterozoic. New detrital zircon U–Pb age and Lu–Hf isotope data, collected from multiple, geographically separated, basins that make up the Wilton package, are compiled with previously published data to illuminate the basin evolution. The spatial and temporal variation in sedimentary provenance illustrates two major geographic changes that correspond to continent-scale tectonic convulsions of the NAC during the Mesoproterozoic. The first is shown by the influx of sediment sourced from east and southeast terranes. This is linked to rifting between Proterozoic Australia and Laurentia at c . 1.45 Ga, resulting in the uplift of the eastern margin of the NAC–SAC (South Australian Craton). The second basin geographic change is illustrated by a flux of southerly-sourced detritus that is interpreted to be tectonically driven by the uplift of the southern NAC, during the subduction/closure of the Mirning Ocean at c. 1.32 Ga. Spatially, sediment in the Wilton package is separated into two depositional systems: sedimentary rocks within the Birrindudu Basin, the western component of the Wilton package, have different detrital signatures relative to other Wilton package successions found east of the Daly Waters Fault Zone, in the Beetaloo Sub-basin, the McArthur Basin and the South Nicholson Basin. The Daly Waters Fault Zone is interpreted as an ancient bathymetric high, blocking sediment transport. Although they differ in sources, rocks in both the Birrindudu Basin and the eastern Wilton package record coeval shifts of basin provenance to southern sources. The coherent evolution of basin provenance indicates a consistent tectono-sedimentation history, and links the Birrindudu Basin and the other Wilton successions in a tectonic framework.
Publisher: Elsevier BV
Date: 05-2017
Publisher: Geological Society of America
Date: 03-2014
DOI: 10.1130/G35112.1
Publisher: Elsevier BV
Date: 12-2015
Publisher: Elsevier BV
Date: 08-2006
Publisher: Geological Society of London
Date: 09-05-2019
DOI: 10.1144/JGS2018-159
Publisher: Elsevier BV
Date: 04-2016
Publisher: Wiley
Date: 12-08-2020
Publisher: Informa UK Limited
Date: 08-2011
Publisher: Elsevier BV
Date: 03-2010
Publisher: Elsevier BV
Date: 08-2016
Publisher: Wiley
Date: 06-08-2013
DOI: 10.1002/ECE3.708
Publisher: Elsevier BV
Date: 08-2021
Publisher: Elsevier BV
Date: 11-2017
Publisher: Elsevier BV
Date: 03-2022
Publisher: Elsevier BV
Date: 09-2018
Publisher: Elsevier BV
Date: 03-2016
Publisher: Elsevier BV
Date: 12-2014
Publisher: Elsevier BV
Date: 11-2015
Publisher: Geological Society of America
Date: 05-2012
DOI: 10.1130/G32854.1
Publisher: Geological Society of America
Date: 2013
DOI: 10.1130/G33422.1
Publisher: Geological Society of America
Date: 09-2009
DOI: 10.1130/G30175A.1
Publisher: Geological Society of London
Date: 22-11-2019
DOI: 10.1144/JGS2018-125
Publisher: American Geophysical Union (AGU)
Date: 06-2019
DOI: 10.1029/2018TC005384
Publisher: Elsevier BV
Date: 12-2011
Publisher: Elsevier BV
Date: 11-2015
Publisher: Royal Society of Chemistry (RSC)
Date: 2013
DOI: 10.1039/C3JA50090J
Publisher: Society of Economic Geologists
Date: 05-2022
DOI: 10.5382/ECONGEO.4886
Abstract: Extrusive and intrusive felsic magmas occur throughout the evolution of silicic-dominated large igneous province magmatism that is temporally related to numerous economically significant iron oxide copper-gold (IOCG) deposits in southern Australia. We investigate zircon trace element signatures of the felsic magmas to assess whether zircon composition can be related to fertility of the volcanic and intrusive suites within IOCG-hosted mineral provinces. Consistent with zircon forming in oxidizing magmatic conditions, the rare earth element (REE) patterns of zircon sourced from both extrusive and intrusive magmatic rocks are characterized by light REE depletions and a range of positive Ce and negative Eu anomalies. The timing of the major phase of IOCG mineralization overlaps with the early part of the first phase of Lower Gawler Range Volcanics magmatism (1593.6–1590.4 Ma) and older intrusive magmatism of the Hiltaba Suite (1593.06–1590.50 Ma). Zircon in these mineralization-related intrusives and extrusives is distinguished from zircon in younger, mineralization-absent rocks by higher Eu/Eu*, Ce/Ce*, and Ti values and separate magma evolution paths with respect to Hf. These zircon characteristics correspond to lower degrees of fractionation and/or crustal assimilation, more oxidizing magmatic conditions, and higher magmatic temperatures, respectively, in magmas coeval with mineralization. In this respect, we consider higher oxidation state, lower degrees of fractionation, and higher magmatic temperatures to be features of fertile magmas in southern Australian IOCG terrains. Similar zircon REE characteristics are shared between magmas associated with southern Australian IOCG and iron oxide-apatite (IOA) rhyolites from the St. Francois Mountains, Missouri, namely high Ce/Ce* and high Dy/Yb, indicative of oxidized and dry magmas, respectively. The dry and more fractionated nature of the IOCG- and IOA-associated magmas contrasts with the hydrous and unfractionated nature of fertile porphyry Cu deposit magmas. As indicated by high Ce/Ce* ratios, the oxidized nature is considered a key element in magma fertility in IOCG-IOA terrains. In both IOCG and IOA terrains, the trace element compositions of zircon are able to broadly differentiate fertile from nonfertile magmatic rocks.
Publisher: Elsevier BV
Date: 2019
Publisher: Elsevier BV
Date: 04-2020
Publisher: Elsevier BV
Date: 11-2019
Publisher: Geological Society of London
Date: 2011
Publisher: Elsevier BV
Date: 11-2019
Publisher: Elsevier BV
Date: 11-2017
Publisher: Informa UK Limited
Date: 07-2008
Publisher: American Geophysical Union (AGU)
Date: 09-2023
DOI: 10.1029/2023GC011019
Publisher: Elsevier BV
Date: 09-2019
Publisher: Elsevier BV
Date: 11-2014
Publisher: Elsevier BV
Date: 09-2017
Publisher: Oxford University Press (OUP)
Date: 16-08-2019
DOI: 10.1093/GJI/GGZ376
Abstract: Thermal conductivity is a physical parameter crucial to accurately estimating temperature and modelling thermally related processes within the lithosphere. Direct measurements are often impractical due to the high cost of comprehensive s ling or inaccessibility and thereby require indirect estimates. In this study, we report 340 new thermal conductivity measurements on igneous rocks spanning a wide range of compositions using an optical thermal conductivity scanning device. These are supplemented by a further 122 measurements from the literature. Using major element geochemistry and modal mineralogy, we produce broadly applicable empirical relationships between composition and thermal conductivity. Predictive models for thermal conductivity are developed using (in order of decreasing accuracy) major oxide composition, CIPW normative mineralogy and estimated modal mineralogy. Four common mixing relationships (arithmetic, geometric, square-root and harmonic) are tested and, while results are similar, the geometric model consistently produces the best fit. For our preferred model, $k_{\\text{eff}} = \\exp ( 1.72 \\, C_{\\text{SiO}_2} + 1.018 \\, C_{\\text{MgO}} - 3.652 \\, C_{\\text{Na}_2\\text{O}} - 1.791 \\, C_{\\text{K}_2\\text{O}})$, we find that SiO2 is the primary control on thermal conductivity with an RMS of 0.28 W m−1 K−1or ∼10 per cent. Estimates from normative mineralogy work to a similar degree but require a greater number of parameters, while forward and inverse modelling using estimated modal mineralogy produces less than satisfactory results owing to a number of complications. Using our model, we relate thermal conductivity to both P-wave velocity and density, revealing systematic trends across the compositional range. We determine that thermal conductivity can be calculated from P-wave velocity in the range 6–8 km s−1 to within 0.31 W m−1 K−1 using $k({V_p}) = 0.5822 \\, V_p^2 - 8.263 \\, V_p + 31.62$. This empirical model can be used to estimate thermal conductivity within the crust where direct s ling is impractical or simply not possible (e.g. at great depths). Our model represents an improved method for estimating lithospheric conductivity than present formulas which exist only for a limited range of compositions or are limited by infrequently measured parameters.
Publisher: Cambridge University Press (CUP)
Date: 07-03-2018
DOI: 10.1017/S0016756817000061
Abstract: The Omani basement is located spatially distant from the dominantly juvenile Arabian–Nubian Shield (ANS) to its west, and its relationship to the amalgamation of those arc terranes has yet to be properly constrained. The Jebel Ja'alan (NE Oman) basement inlier provides an excellent opportunity to better understand the Neoproterozoic tectonic geography of Oman and its relationship to the ANS. To understand the origin of this basement inlier, we present new radiogenic isotopic data from igneous bodies in Jebel Ja'alan. U–Pb and 40 Ar/ 39 Ar geochronological data are used to constrain the timing of magmatism and metamorphism in the jebel. Positive εHf and εNd values indicate a juvenile origin for the igneous lithologies. Phase equilibria modelling is used to constrain the metamorphic conditions recorded by basement. Pressure–temperature ( P – T ) pseudosections show that basement schists followed a clockwise P–T path, reaching peak metamorphic conditions of c. 650–700°C at 4–7.5 kbar, corresponding to a thermal gradient of c. 90–160°C/kbar. From the calculated thermal gradient, in conjunction with collected trace-element data, we interpret that the Jebel Ja'alan basement formed in an arc environment. Geochronological data indicate that this juvenile arc formed during Tonian time and is older than basement further west in Oman. We argue that the difference in timing is related to westwards arc accretion and migration, which implies that the Omani basement represents its own tectonic domain separate to the ANS and may be the leading edge of the Neoproterozoic accretionary margin of India.
Publisher: Informa UK Limited
Date: 25-09-2020
Publisher: Elsevier BV
Date: 07-2021
Publisher: Geological Society of London
Date: 31-07-2018
DOI: 10.1144/JGS2017-028
Publisher: Geological Society of London
Date: 2009
DOI: 10.1144/SP323.16
Publisher: Elsevier BV
Date: 05-2018
Start Date: 2016
End Date: 2018
Funder: Australian Research Council
View Funded ActivityStart Date: 2014
End Date: 2014
Funder: Australian Research Council
View Funded ActivityStart Date: 2014
End Date: 12-2014
Amount: $360,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 04-2017
End Date: 06-2022
Amount: $490,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2021
End Date: 09-2022
Amount: $715,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2022
End Date: 12-2022
Amount: $389,526.00
Funder: Australian Research Council
View Funded ActivityStart Date: 11-2016
End Date: 11-2020
Amount: $225,000.00
Funder: Australian Research Council
View Funded Activity