2005
Type of resources
Keywords
Publication year
Scale
Topics
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A1/F4; Characteristics of mineralised faults; Annual Review Meeting Perth, November 2003.
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Mt Isa PDT Meeting, Mt Isa, March 2005
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Cleverley J.S. & Olver N.H.S., 2005. JCU/EGRU/CRC Masters Program at JCU. Geochemical Modelling
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Fisher, L., 2005. Fluid inclusion compositions and conditions at Osborne; preliminary results.
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Mustard, R., Mark, G., Ulrich, T., Foster, D., and Gillen, D., 2005. Geochemsitry of magmatic fluids from intrusions in the Williams-Naraku batholith, Cloncurry district, NW Queensland: preliminary results from laser ablation ICPMS analysis.
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H4 - Yilgarn delivery workshop Nov 2005
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H4 - Mt Isa Workshop
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Revised geodynamic history Delamarian/Lachlan
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This web-enabled system allows researchers to retrieve fluid inclusion data from anywhere in the world. The concept is to build a free and widely available web-based library of fluid properties for a range of geological fluids. The database is being developed as an "open" project, which intends to bring together researchers interested in the properties of geological fluids or fluid inclusions.
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AUSGeoid98 data files contain a 2 minute grid of AUSGeoid98 data covering the Australian region, which you can use to interpolate geoid-ellipsoid separations for the positions required.You can use your own interpolation software, or you can use Geoscience Australia's Windows Interpolation software (Winter). The data files are text files in a standard format that cover the same area as standard topographic map areas. Files covering both 1:250,000 (approximately 100 x 150 km) and 1:1,000,000 (approximately 400 x 600 km) map areas are available. There is a 4 minute overlap on all sides of each area. Data format: AUSGeoid98 data files have a header record at the start of each file, to distinguish them from the superseded AUSGeoid93 data files. AUSGeoid98 data files show the geoid-ellipsoid separation to 3 decimal places, while the superseded AUSGeoid93 data files showed only 2 decimal places. AUSGeoid98 deflections of the vertical were computed from the geoid-ellipsoid separation surface, while the AUSGeoid93 deflections of the vertical were computed from OSU91A.