Development and Testing of Down-the-Hole Deployabe X-Ray Florescence Spectrometer
Access Status
Authors
Date
2010Type
Metadata
Show full item recordCitation
Source Title
Source Conference
ISBN
School
Remarks
Carter, Geoffrey A. and Golovanevskiy, Vladimir A. 2010. Development and Testing of Down-the-Hole Deployabe X-Ray Florescence Spectrometer, 10th International Multidisciplinary Scientific Geoconference - SGEM 2010, Jun 20 2010, pp. 407-413. Sofia, Bulgaria: STEF92 Technology Ltd. DOI: 10.5593/sgem2010.1.3.S1.816
The official site of the International Multidisciplinary Scientific GeoConference (SGEM) can be found at: http://www.sgem.org
Collection
Abstract
To allow a truly in-situ elemental analysis, an Australian resource company commissioned the development and building of a down-the-hole deployable ED-XRF sensor. The instrument was designed to be deployable up to a depth of 30 m for drill holes of varying diameters as well as being run in a bench-top mode. Following the development and upon commissioning, the ED-XRF system was investigated in the laboratory for its suitability for use in the Iron Ore industry by using well characterised crushed iron ore samples, standards made from analytical reagents and large iron ore rocks that had been sectioned to provide a curved surface for presentation to the XRF. The effects of operating conditions and other parameters were studied using the standards made from the analytical reagents. It was found that the system could be used to determine the elemental Fe content with reasonable accuracy when used on crushed powder samples. The curved surfaces of the sectioned rocks increased the variability of the amount of Fe detected. Two trace elements, Al and Si were also investigated using the same methodology. It was found that the ED-XRF system was not suitable for distinguishing the Al and Si. This paper outlines the ED-XRF system used, the testing methodology employed and the results of the laboratory testing.
Related items
Showing items related by title, author, creator and subject.
-
Gallo, E.; Miller-Jones, James; Russell, D.; Jonker, P.; Homan, J.; Plotkin, R.; Markoff, S.; Miller, B.; Corbel, S.; Fender, R. (2014)We report on deep, coordinated radio and X-ray observations of the black hole X-ray binary XTE J1118+480 in quiescence. The source was observed with the Karl G. Jansky Very Large Array for a total of 17.5 h at 5.3 GHz, ...
-
Motch, C.; Pakull, M.; Soria, Roberto; Grisé, F.; Pietrzynski, G. (2014)Most ultraluminous X-ray sources have a typical set of properties not seen in Galactic stellar-mass black holes. They have luminosities of more than 3 × 10 39 ergs per second, unusually soft X-ray components (with a typical ...
-
Corbel, S.; Miller-Jones, James; Fender, R.; Gallo, E.; Maccarone, T.; O'brien, T.; Paragi, Z.; Rupen, M.; Rushton, A.; Sabatini, S.; Sivakoff, G.; Strader, J.; Woudt, P. (2014)The universal link between the processes of accretion and ejection leads to the formation of jets and outflows around accreting compact objects. Incoherent synchrotron emission from these outflows can be observed from a ...