Exploration and evaluation of the Australian geothermal resource
Abstract
A database of 5722 borehole temperatures, AUSTHERM03, has been assembled building
upon the existing work of Somerville et al. (1994) through addition of newly available
commercial open-file data. The application of more rigorous GIS techniques, including the
use of new depth-to-basement and mean annual surface temperature coverages, has resulted in
a more reliable extrapolation of this data to 5km depth. A new Australia-wide map of
estimated temperature at 5km was created from the extrapolated data by interpolation using
geostatistical kriging. The combination of new data and more sophisticated GIS processing
has produced a more realistic map image that is characterised in areas of good data density by
rounded, well constrained temperature anomalies. In most cases, thermal highs were found to
be associated with areas of sedimentary basin cover. Geothermal resource analysis of this
image indicates three major regions of prospectivity beneath the Cooper, McArthur and
Carnarvon Basins.
The use of commercial borehole temperature data in the current AUSTHERM03 temperature
map image means that it is affected by temperature suppression caused by the drilling thermal
anomaly. Data available in AUSTHERM03 from 330 wells in the Cooper Basin of South
Australia provided a unique opportunity to test the reliability of several published models for
bottom of hole temperature (BHT) correction. Incorporated into a new database, the Cooper
Basin Static Temperature or CBST, 61 of these wells proved suitable for use in thermal
modelling. Included within these data were consecutive BHT measurements taken shortly
after drilling was completed. Also available were BHT from cement bond logs (CBL)
recorded a significant time after drilling which provided a good estimate of true formation
temperature and a basis for comparison with model predictions. Four commonly used models
of borehole thermal re-equilibration were tested: the Homer plot derived from Bullard
(1947), the theoretical dual-media, zero-circulation cylindrical model of Cooper & Jones
(1959), the empirical semi-log plot of Pitt (1986) and the exponential model of Nakaya
(1953). On average, most models were found to under-estimate the true formation
temperature. The magnitude of this bias was dependent upon assumptions implicit in each
model. In most cases model prediction accuracy was improved to within around 5% of the
CBL when at least one perturbed BHT was recorded >20 hours after the end of drilling. Of
the models tested, the theoretical Horner plot was found to have the best combination of
accuracy, utility and predictability. Applying this knowledge to perturbed BHT recorded in
AUSTHERM03 enabled correction of a subset of 307 Cooper Basin wells using the Horner
Plot. Two images of temperature distribution at 5km depth were constructed for these wells, one using the perturbed AUSTHERM03 data, the other the corrected values. While the
effects of the drilling temperature suppression were evident on the uncorrected image the
overall anomaly structure was found to be largely undisturbed, confirming the utility of the
AUSTHERM03 image for geothermal exploration.
Located within the Cooper Basin is a strong temperature anomaly that is currently the focus
of Australia's first geothermal resource development, Habanera. A geological and
geochemical study of drill cuttings derived from Habanero 1, the first deep geothermal well
drilled on this site, revealed the presence of a fractured, fractionated 1-type granite body at
depth. Similar in composition to many better known granite bodies around Australia, this
data provides the basis for a geological model of an Australian-style geothermal resource that
compliments the use of temperature mapping as a means of geothermal target generation.
Prospective regions identified using this model include the Murray Basin area of
NSW Nictoria.