ORCID Profile
0000-0002-2734-8790
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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.
Geology | Ore Deposit Petrology | Igneous And Metamorphic Petrology | Ore Deposit Petrology | Igneous and Metamorphic Petrology | Separation Science | Chemical Characterisation of Materials | Marine and Estuarine Ecology (incl. Marine Ichthyology) | Geochemistry Not Elsewhere Classified | Exploration Geochemistry | Mineralogy and Crystallography | Geochemistry | Organic Chemical Synthesis | Pharmaceutical Sciences | Vulcanology | Geochronology And Isotope Geochemistry | Biological Oceanography | Mineralogy And Crystallography | Geochronology | Conservation and Biodiversity | Materials Engineering | Metals and Alloy Materials | Environmental Monitoring | Geochemistry not elsewhere classified | Freshwater Ecology | Catalysis and Mechanisms of Reactions | Electromagnetism | Isotope Geochemistry | Plant Cell and Molecular Biology | Neurology and Neuromuscular Diseases | Crop and Pasture Biochemistry and Physiology | Geology not elsewhere classified | Volcanology
Earth sciences | Expanding Knowledge in the Earth Sciences | Mineral Exploration not elsewhere classified | Management of Solid Waste from Mineral Resource Activities | Field crops | Natural Hazards not elsewhere classified | Nervous System and Disorders | Organic Industrial Chemicals (excl. Resins, Rubber and Plastics) | Environmentally Sustainable Manufacturing not elsewhere classified | Biological sciences | Chemical sciences | Concentrating processes of other base metal ores | Integrated (ecosystem) assessment and management | Physical and Chemical Conditions of Water in Fresh, Ground and Surface Water Environments (excl. Urban and Industrial Use) | Marine Flora, Fauna and Biodiversity | Climate Change Mitigation Strategies | Expanding Knowledge in the Medical and Health Sciences | First stage treatment of ores and minerals | Mineral Resources (excl. Energy Resources) not elsewhere classified | Expanding Knowledge in the Physical Sciences | Scientific Instruments | Precious (Noble) Metal Ore Exploration | Titanium Minerals, Zircon, and Rare Earth Metal Ore (e.g. Monazite) Exploration | Copper Ore Exploration |
Publisher: Mineralogical Society of America
Date: 20-12-2012
DOI: 10.2138/AM.2013.4018
Publisher: Elsevier BV
Date: 09-2015
Publisher: Elsevier BV
Date: 09-2014
Publisher: Elsevier BV
Date: 08-2013
Publisher: Geological Society of America
Date: 11-2011
DOI: 10.1130/G32205.1
Publisher: Elsevier BV
Date: 08-2013
Publisher: Elsevier BV
Date: 05-2014
Publisher: Elsevier BV
Date: 06-2007
Publisher: Geological Society of America
Date: 2005
DOI: 10.1130/G21257.1
Publisher: Royal Society of Chemistry (RSC)
Date: 2016
DOI: 10.1039/C6JA00048G
Abstract: U–Pb ages of several apatite reference materials, acquired by LA-ICP-MS over a 3.5 year period using the Otter Lake apatite as a primary standard, show systematic offsets (up to 3%) from reference ages obtained by isotope dilution mass spectrometry.
Publisher: Elsevier BV
Date: 05-2010
Publisher: Elsevier BV
Date: 08-2016
Publisher: Society of Economic Geologists
Date: 09-2017
Publisher: Elsevier BV
Date: 02-2009
Publisher: Elsevier BV
Date: 2003
Publisher: Springer Science and Business Media LLC
Date: 05-2007
DOI: 10.1038/NATURE05759
Abstract: The chemical composition of basaltic magma erupted at the Earth's surface is the end product of a complex series of processes, beginning with partial melting and melt extraction from a mantle source and ending with fractional crystallization and crustal assimilation at lower pressures. It has been proposed that studying inclusions of melt trapped in early crystallizing phenocrysts such as Mg-rich olivine and chromite may help petrologists to see beyond the later-stage processes and back to the origin of the partial melts in the mantle. Melt inclusion suites often span a much greater compositional range than associated erupted lavas, and a significant minority of inclusions carry distinct compositions that have been claimed to s le melts from earlier stages of melt production, preserving separate contributions from mantle heterogeneities. This hypothesis is underpinned by the assumption that melt inclusions, once trapped, remain chemically isolated from the external magma for all elements except those that are compatible in the host minerals. Here we show that the fluxes of rare-earth elements through olivine and chromite by lattice diffusion are sufficiently rapid at magmatic temperatures to re-equilibrate completely the rare-earth-element patterns of trapped melt inclusions in times that are short compared to those estimated for the production and ascent of mantle-derived magma or for magma residence in the crust. Phenocryst-hosted melt inclusions with anomalous trace-element signatures must therefore form shortly before magma eruption and cooling. We conclude that the assumption of chemical isolation of incompatible elements in olivine- and chromite-hosted melt inclusions is not valid, and we call for re-evaluation of the popular interpretation that anomalous melt inclusions represent preserved s les of unmodified mantle melts.
Publisher: Oxford University Press (OUP)
Date: 20-09-2006
Publisher: Elsevier BV
Date: 10-2017
Publisher: Elsevier
Date: 2003
Publisher: Elsevier BV
Date: 07-2016
Publisher: Elsevier BV
Date: 11-2012
Publisher: Geological Society of America
Date: 05-2013
DOI: 10.1130/G34066.1
Publisher: Informa UK Limited
Date: 20-05-2018
Publisher: Pleiades Publishing Ltd
Date: 05-2012
Publisher: Elsevier BV
Date: 12-2001
Publisher: Geological Society of America
Date: 12-2012
DOI: 10.1130/G33265.1
Publisher: Elsevier BV
Date: 06-2015
Publisher: Elsevier BV
Date: 11-2017
Publisher: Elsevier BV
Date: 11-2017
Publisher: MDPI AG
Date: 23-10-2017
DOI: 10.3390/MIN7100202
Publisher: Oxford University Press (OUP)
Date: 28-07-2007
Publisher: Elsevier BV
Date: 02-2018
Publisher: Elsevier BV
Date: 02-2018
Publisher: Oxford University Press (OUP)
Date: 06-2020
DOI: 10.1093/PETROLOGY/EGAA062
Abstract: Olivine is the most abundant phase in kimberlites and is stable throughout most of the crystallization sequence, thus providing an extensive record of kimberlite petrogenesis. To better constrain the composition, evolution, and source of kimberlites we present a detailed petrographic and geochemical study of olivine from multiple dyke, sill, and root zone kimberlites in the Kimberley cluster (South Africa). Olivine grains in these kimberlites are zoned, with a central core, a rim overgrowth, and occasionally an external rind. Additional ‘internal’ and ‘transitional’ zones may occur between the core and rim, and some s les of root zone kimberlites contain a late generation of high-Mg olivine in cross-cutting veins. Olivine records widespread pre-ascent (proto-)kimberlite metasomatism in the mantle including the following features: (1) relatively Fe-rich (Mg# & ) olivine cores interpreted to derive from the disaggregation of kimberlite-related megacrysts (20 % of cores) (2) Mg–Ca-rich olivine cores (Mg# & & ·05 wt% CaO) suggested to be sourced from neoblasts in sheared peridotites (25 % of cores) (3) transitional zones between cores and rims probably formed by partial re-equilibration of xenocrysts (now cores) with a previous pulse of kimberlite melt (i.e. compositionally heterogeneous xenocrysts) (4) olivine from the Wesselton water tunnel sills, internal zones (I), and low-Mg# rims, which crystallized from a kimberlite melt that underwent olivine fractionation and stalled within the shallow lithospheric mantle. Magmatic crystallization begins with internal olivine zones (II), which are common but not ubiquitous in the Kimberley olivine. These zones are euhedral, contain rare inclusions of chromite, and have a higher Mg# (90·0 ± 0·5), NiO, and Cr2O3 contents, but are depleted in CaO compared with the rims. Internal olivine zones (II) are interpreted to crystallize from a primitive kimberlite melt during its ascent and transport of olivine toward the surface. Their compositions suggest assimilation of peridotitic material (particularly orthopyroxene) and potentially sulfides prior to or during crystallization. Comparison of internal zones (II) with liquidus olivine from other mantle-derived carbonate-bearing magmas (i.e. orangeites, ultramafic l rophyres, melilitites) shows that low (100×) Mn/Fe (∼1·2), very low Ca/Fe (∼0·6), and moderate Ni/Mg ratios (∼1·1) appear to be the hallmarks of olivine in melts derived from carbonate-bearing garnet-peridotite sources. Olivine rims display features indicative of magmatic crystallization, which are typical of olivine rims in kimberlites worldwide that is, primary inclusions of chromite, Mg-ilmenite and rutile, homogeneous Mg# (88·8 ± 0·3), decreasing Ni and Cr, and increasing Ca and Mn. Rinds and high-Mg olivine are characterized by extreme Mg–Ca–Mn enrichment and Ni depletion, and textural relationships indicate that these zones represent replacement of pre-existing olivine, with some new crystallization of rinds. These zones probably precipitated from evolved, oxidized, and relatively low-temperature kimberlite fluids after crustal emplacement. In summary, this study demonstrates the utility of combined petrography and olivine geochemistry to trace the evolution of kimberlite magmatic systems from early metasomatism of the lithospheric mantle by (proto-)kimberlite melts, to crystallization at different depths en route to surface, and finally late-stage deuteric or hydrothermal fluid alteration after crustal emplacement.
Publisher: Elsevier BV
Date: 07-2016
Publisher: Elsevier BV
Date: 10-2004
Publisher: Springer Science and Business Media LLC
Date: 11-12-2015
Publisher: Elsevier BV
Date: 08-2013
Publisher: Elsevier BV
Date: 09-2018
Publisher: Mineralogical Society of America
Date: 02-2006
DOI: 10.2138/AM.2006.2107
Publisher: Pleiades Publishing Ltd
Date: 09-2015
Publisher: Elsevier BV
Date: 07-2016
Publisher: Springer Science and Business Media LLC
Date: 08-2015
Publisher: Elsevier BV
Date: 04-2016
Publisher: Elsevier BV
Date: 03-2007
Publisher: Elsevier BV
Date: 04-2018
Publisher: Elsevier BV
Date: 02-2018
Publisher: Elsevier BV
Date: 11-2009
Publisher: Society of Economic Geologists
Date: 17-03-2014
Publisher: Elsevier BV
Date: 07-2009
Publisher: American Association for the Advancement of Science (AAAS)
Date: 04-05-2007
DOI: 10.1126/SCIENCE.
Publisher: Geological Society of America
Date: 23-06-2015
DOI: 10.1130/G36843.1
Publisher: Elsevier BV
Date: 10-1999
Publisher: Elsevier BV
Date: 10-2006
Publisher: Springer Science and Business Media LLC
Date: 1993
DOI: 10.1007/BF01161564
Publisher: Elsevier BV
Date: 11-2009
Publisher: Geological Society of America
Date: 2006
DOI: 10.1130/G22141.1
Publisher: Geological Society of America
Date: 29-06-2012
DOI: 10.1130/G33037.1
Publisher: Elsevier BV
Date: 03-2007
Publisher: Elsevier BV
Date: 03-2007
Publisher: Elsevier BV
Date: 04-2017
Publisher: Informa UK Limited
Date: 30-10-2009
Publisher: Elsevier BV
Date: 2017
Publisher: Springer Science and Business Media LLC
Date: 17-04-2015
DOI: 10.1038/NCOMMS7837
Abstract: Kimberlites and orangeites (previously named Group-II kimberlites) are small-volume igneous rocks occurring in diatremes, sills and dykes. They are the main hosts for diamonds and are of scientific importance because they contain fragments of entrained mantle and crustal rocks, thus providing key information about the subcontinental lithosphere. Orangeites are ultrapotassic, H2O and CO2-rich rocks hosting minerals such as phlogopite, olivine, calcite and apatite. The major, trace element and isotopic compositions of orangeites resemble those of intensely metasomatized mantle of the type represented by MARID (mica- hibole-rutile-ilmenite-diopside) xenoliths. Here we report new data for two MARID xenoliths from the Bultfontein kimberlite (Kimberley, South Africa) and we show that MARID-veined mantle has mineralogical (carbonate-apatite) and geochemical (Sr-Nd-Hf-O isotopes) characteristics compatible with orangeite melt generation from a MARID-rich source. This interpretation is supported by U-Pb zircon ages in MARID xenoliths from the Kimberley kimberlites, which confirm MARID rock formation before orangeite magmatism in the area.
Publisher: Elsevier BV
Date: 04-2012
Publisher: Wiley
Date: 05-2010
DOI: 10.1111/J.1468-8123.2009.00272.X
Abstract: Geofluids (2010) 10 , 293–311 The first occurrence of immiscibility in magmas appears to be most important in the magmatic–hydrothermal transition, and thus studies of magmatic immiscibility should be primarily directed towards recognition of coexisting silicate melt and essentially non‐silicate liquids and fluids (aqueous, carbonic and sulphide). However, immiscible phase separation during decompression, cooling and crystallization of magmas is an inherently fugitive phenomenon. The only remaining evidence of this process and the closest approximation of natural immiscible magmatic liquids and vapours can be provided by melt and fluid inclusions trapped in silicate glasses and magmatic phenocrysts. Such inclusions are often used as a natural experimental laboratory to model the process of exsolution and the compositions of volatile‐rich phases from a wide range of terrestrial magmas. In this paper several ex les from recent research on melt and fluid inclusions are used to demonstrate the significance of naturally occurring immiscibility in understanding some large‐scale magma chamber processes, such as degassing and partitioning of metals.
Publisher: Geological Society of America
Date: 17-08-2017
DOI: 10.1130/G39344.1
Publisher: Elsevier BV
Date: 2015
Publisher: Oxford University Press (OUP)
Date: 07-08-2012
Publisher: Elsevier BV
Date: 11-2004
Publisher: Oxford University Press (OUP)
Date: 28-01-2012
Publisher: Elsevier BV
Date: 05-2017
Publisher: Mineralogical Society of America
Date: 06-2016
DOI: 10.2138/AM-2016-5509
Publisher: Elsevier BV
Date: 04-2016
Publisher: Elsevier BV
Date: 12-2014
Publisher: Elsevier BV
Date: 04-2017
Publisher: Elsevier BV
Date: 09-2014
Publisher: Springer Science and Business Media LLC
Date: 17-12-2013
DOI: 10.1038/NCOMMS3921
Abstract: Kimberlites are a volumetrically minor component of the Earth's volcanic record, but are very important as the major commercial source of diamonds and as the deepest s les of the Earth's mantle. They were predominantly emplaced from ≈2,100 Ma to ≈10 ka ago, into ancient, stable regions of continental crust (cratons), but are also known from continental rifts and mobile belts. Kimberlites have been reported from almost all major cratons on all continents except for Antarctica. Here we report the first bona fide Antarctic kimberlite occurrence, from the northern Prince Charles Mountains, emplaced during the reactivation of the Lambert Graben associated with rifting of India from Australia-Antarctica. The s les are texturally, mineralogically and geochemically typical of Group I kimberlites from more classical localities. Their ≈120 Ma ages overlap with those of many kimberlites from other world-wide localities, extending a vast Cretaceous, Gondwanan kimberlite province, for the first time, into Antarctica.
Publisher: Springer Science and Business Media LLC
Date: 23-07-2013
Publisher: Geological Society of America
Date: 11-2012
DOI: 10.1130/G33221.1
Publisher: Springer Science and Business Media LLC
Date: 10-2004
DOI: 10.1038/NATURE02972
Abstract: A relationship between convergent margin magmas and copper-gold ore mineralization has long been recognized. The nature of the genetic link is controversial, particularly whether the link is due to high-oxygen-fugacity (fO2) melts and fluids released from subducted slabs or to brine exsolution during magmatic evolution. For submarine, subduction-related volcanic glasses from the eastern Manus basin, Papua New Guinea, we here report abrupt decreases in gold and copper abundances, coupled with a switch in the behaviour of titanium and iron from concentration increases to decreases as SiO2 rises. We propose that the abrupt depletion in gold and copper results from concurrent sulphur reduction as a result of fO2 buffering, causing enhanced formation of copper-gold hydrosulphide complexes that become scavenged from crystallizing melts into cogenetic magmatic aqueous fluids. This process is particularly efficient in oxidized arc magmas with substantial sulphate. We infer that subsequent migration and cooling of exsolved aqueous fluids create links between copper-gold mineralization and arc magmatism in the Manus basin, and at convergent margins in general.
Publisher: Geological Society of America
Date: 08-2013
DOI: 10.1130/G34311.1
Publisher: Elsevier BV
Date: 2016
Publisher: Elsevier BV
Date: 03-2002
Publisher: American Geophysical Union (AGU)
Date: 10-05-2007
DOI: 10.1029/2007GL029389
Publisher: Elsevier BV
Date: 10-2011
DOI: 10.1016/J.SAA.2011.01.034
Abstract: Raman spectroscopy has been used for the identification of both common and uncommon minerals in melt inclusions in Group-I kimberlites from Siberia, Canada, SW Greenland and South Africa. The melt inclusions all contained high abundances of alkali-Ca carbonates, with varying proportions of cations, and Na-Ca-Ba sulphates. In accordance with its dry mineralogy, no hydrated carbonates or sulphates were detected in melt inclusions from the Udachnaya-East kimberlite. In contrast, the melt inclusions in kimberlites from Canada, South Africa and SW Greenland were found to contain bassanite, pirssonite, and hydromagnesite suggesting that greater amounts of water were present in their residual magmas. This suggests that enrichment in alkali carbonates and sulphates is widespread across a range of Group-I kimberlites and implies that they commonly have an alkali-, and sulphur-rich residual liquid.
Publisher: Springer Science and Business Media LLC
Date: 27-02-2017
DOI: 10.1038/NGEO2902
Publisher: Pleiades Publishing Ltd
Date: 09-2006
Publisher: Springer Science and Business Media LLC
Date: 03-2003
DOI: 10.1038/NATURE01482
Publisher: Elsevier BV
Date: 03-2002
Publisher: Geological Society of America
Date: 21-11-2016
DOI: 10.1130/G38517.1
Publisher: Springer Science and Business Media LLC
Date: 05-09-2013
Publisher: Wiley
Date: 09-09-2019
DOI: 10.1002/JRS.5701
Publisher: Society of Economic Geologists
Date: 08-2005
Publisher: Elsevier BV
Date: 04-2017
Publisher: Oxford University Press (OUP)
Date: 06-05-2013
Publisher: Mineralogical Association of Canada
Date: 08-2008
Publisher: Mineralogical Society of America
Date: 06-2018
DOI: 10.2138/AM-2018-6352
Publisher: Geological Society of America
Date: 28-08-2015
DOI: 10.1130/G37052.1
Publisher: Elsevier BV
Date: 05-2012
Publisher: Elsevier BV
Date: 08-2014
Publisher: Oxford University Press (OUP)
Date: 08-2014
Publisher: Geological Society of America
Date: 06-2013
DOI: 10.1130/G34119.1
Publisher: Wiley
Date: 26-10-2017
DOI: 10.1111/IAR.12223
Publisher: Oxford University Press (OUP)
Date: 11-03-2014
Publisher: Elsevier BV
Date: 11-2012
Publisher: Geological Society of America
Date: 08-2011
DOI: 10.1130/G31952.1
Publisher: Elsevier BV
Date: 10-2017
Publisher: Springer Science and Business Media LLC
Date: 12-10-2017
Publisher: Geological Society of America
Date: 1999
Publisher: American Association for the Advancement of Science (AAAS)
Date: 19-12-2003
Abstract: At a porphyry copper-gold deposit in Bajo de la Alumbrera, Argentina, silicate-melt inclusions coexist with hypersaline liquid- and vapor-rich inclusions in the earliest magmatic-hydrothermal quartz veins. Copper concentrations of the hypersaline liquid and vapor inclusions reached maxima of 10.0 weight % (wt %) and 4.5 wt %, respectively. These unusually copper-rich inclusions are considered to be the most primitive ore fluid found thus far. Their preservation with coexisting melt allows for the direct quantification of important ore-forming processes, including determination of bulk partition coefficients of metals from magma into ore-forming magmatic volatile phases.
Publisher: Elsevier BV
Date: 03-2002
Publisher: Elsevier BV
Date: 02-2018
Publisher: Oxford University Press (OUP)
Date: 18-06-2018
Publisher: MDPI AG
Date: 26-12-2021
DOI: 10.3390/MIN12010037
Abstract: Sulfur contents in 98.5% of melt inclusions (MI) from calc-alkaline subduction basalts do not exceed 4000 ppm, whereas experimentally established limits of sulfur solubility in basaltic melts with high fO2 (characteristic of subduction zones, e.g., QFM + 2) surpass 14,000 ppm. Here we show that primitive (Mg# 62-64) subduction melts may contain high sulfur, approaching the experimental limit of sulfur solubility. Up to 11,700 ppm S was measured in olivine-hosted MI from primitive arc basalt from the 1941 eruption of the Tolbachik volcano, Kamchatka. These MI often contain magmatic sulfide globules (occasionally enriched in Cu, Ni, and platinum-group elements) and anhydrite enclosed within a brown, oxidized glass. We conclude that the ubiquitous low sulfur contents in MI may originate either from insufficient availability of sulfur in the magma generation zone or early magma degassing prior to inclusion entrapment. Our findings extend the measured range of sulfur concentrations in primitive calc-alkaline basaltic melts and demonstrate that no fundamental limit of 4000 ppm S exists for relatively oxidized subduction basalts, where the maximum sulfur content may approach the solubility limit determined by crystallization of magmatic anhydrite.
Publisher: Informa UK Limited
Date: 06-02-2020
Publisher: Elsevier BV
Date: 03-2012
Publisher: Wiley
Date: 23-12-2010
Publisher: Springer Science and Business Media LLC
Date: 28-09-2004
Publisher: MDPI AG
Date: 29-11-2018
DOI: 10.3390/MIN8120555
Abstract: The emplacement age of the Great Udzha Dyke (northern Siberian Craton) was determined by the U-Pb dating of apatite using laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS). This produced an age of 1386 ± 30 Ma. This dyke along with two other adjacent intrusions, which cross-cut the sedimentary units of the Udzha paleo-rift, were subjected to paleomagnetic investigation. The paleomagnetic poles for the Udzha paleo-rift intrusions are consistent with previous results published for the Chieress dyke in the Anabar shield of the Siberian Craton (1384 ± 2 Ma). Our results suggest that there was a period of intense volcanism in the northern Siberian Craton, as well as allow us to reconstruct the apparent migration of the Siberian Craton during the Mesoproterozoic.
Publisher: Elsevier BV
Date: 07-2008
Publisher: Geological Society of America
Date: 10-2013
DOI: 10.1130/G34638.1
Publisher: Elsevier BV
Date: 09-2008
Publisher: Elsevier BV
Date: 03-2011
Publisher: MDPI AG
Date: 10-01-2020
DOI: 10.3390/MIN10010061
Abstract: Pyrite is the most common sulphide in a wide range of ore deposits and well known to host numerous trace elements, with implications for recovery of valuable metals and for generation of clean concentrates. Trace element signatures of pyrite are also widely used to understand ore-forming processes. Pyrite is an important component of the Olympic Dam Cu–U–Au–Ag orebody, South Australia. Using a multivariate statistical approach applied to a large trace element dataset derived from analysis of random pyrite grains, trace element signatures in Olympic Dam pyrite are assessed. Pyrite is characterised by: (i) a Ag–Bi–Pb signature predicting inclusions of tellurides (as PC1) and (ii) highly variable Co–Ni ratios likely representing an oscillatory zonation pattern in pyrite (as PC2). Pyrite is a major host for As, Co and probably also Ni. These three elements do not correlate well at the grain-scale, indicating high variability in zonation patterns. Arsenic is not, however, a good predictor for invisible Au at Olympic Dam. Most pyrites contain only negligible Au, suggesting that invisible gold in pyrite is not commonplace within the deposit. A minority of pyrite grains analysed do, however, contain Au which correlates with Ag, Bi and Te. The results are interpreted to reflect not only primary patterns but also the effects of multi-stage overprinting, including cycles of partial replacement and recrystallisation. The latter may have caused element release from the pyrite lattice and entrapment as mineral inclusions, as widely observed for other ore and gangue minerals within the deposit. Results also show the critical impact on predictive interpretations made from statistical analysis of large datasets containing a large percentage of left-censored values (i.e., those falling below the minimum limits of detection). The treatment of such values in large datasets is critical as the number of these values impacts on the cluster results. Trimming of datasets to eliminate artefacts introduced by left-censored data should be performed with caution lest bias be unintentionally introduced. The practice may, however, reveal meaningful correlations that might be diluted using the complete dataset.
Publisher: Geological Society of America
Date: 2004
DOI: 10.1130/G20821.1
Publisher: Geological Society of America
Date: 2001
Start Date: 2000
End Date: 2000
Funder: Australian Research Council
View Funded ActivityStart Date: 2000
End Date: 2000
Funder: Monash University
View Funded ActivityStart Date: 2003
End Date: 2003
Funder: Australian Research Council
View Funded ActivityStart Date: 2009
End Date: 2009
Funder: Australian Research Council
View Funded ActivityStart Date: 2010
End Date: 2010
Funder: Australian Research Council
View Funded ActivityStart Date: 2016
End Date: 2016
Funder: Australian Research Council
View Funded ActivityStart Date: 2014
End Date: 2014
Funder: Australian Research Council
View Funded ActivityStart Date: 1999
End Date: 1999
Funder: University of Tasmania
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Australian National University
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Rio Tinto Exploration
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Barrick (Australia Pacific) PTY Limited
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: AngloGold Ashanti Australia Limited
View Funded ActivityStart Date: 2005
End Date: 2009
Funder: Minerals Council of Australia
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: AMIRA International Ltd
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Anglo American Exploration Philippines Inc
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Newcrest Mining Limited
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Newmont Australia Ltd
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: University of Melbourne
View Funded ActivityStart Date: 2005
End Date: 2008
Funder: Zinifex Australia Ltd
View Funded ActivityStart Date: 2010
End Date: 2013
Funder: Oz Minerals Australia Limited
View Funded ActivityStart Date: 2008
End Date: 2013
Funder: St Barbara Limited
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Teck Cominco Limited
View Funded ActivityStart Date: 2008
End Date: 2010
Funder: ARC C of E Industry Partner $ to be allocated
View Funded ActivityStart Date: 2005
End Date: 2009
Funder: Mineral Resources Tasmania
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: University of Queensland
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: BHP Billiton Ltd
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: CSIRO Earth Science & Resource Engineering
View Funded ActivityStart Date: 2013
End Date: 2016
Funder: Australian Research Council
View Funded ActivityStart Date: 2005
End Date: 2013
Funder: Australian Research Council
View Funded ActivityStart Date: 2005
End Date: 12-2009
Amount: $726,825.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2016
End Date: 12-2016
Amount: $600,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 01-2014
End Date: 06-2018
Amount: $193,608.00
Funder: Australian Research Council
View Funded ActivityStart Date: 02-2011
End Date: 12-2011
Amount: $240,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2005
End Date: 06-2014
Amount: $24,450,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 06-2020
End Date: 12-2024
Amount: $497,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2013
End Date: 12-2015
Amount: $154,270.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2010
End Date: 03-2013
Amount: $105,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2002
End Date: 12-2003
Amount: $750,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2010
End Date: 12-2010
Amount: $400,000.00
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: 2013
End Date: 12-2014
Amount: $350,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2009
End Date: 12-2009
Amount: $245,000.00
Funder: Australian Research Council
View Funded Activity