The value of full-range spectrometers for petrology.
“Petrology is the study of rocks – describing their characteristics such as composition, texture, structure, occurrence and distribution; and determining the conditions and processes that formed them.” [5]
The ASD TerraSpec spectrometers are portable with optimal signal-to-noise design for faster measurements, and wide spectral coverage of 350-2500 nm for determining a variety of important geological parameters.
We offer different instrument configurations and many accessory options for a variety of set-up and sampling approaches for the most convenient and productive measurement scenarios.
ASD instruments offer a practical solution for applications in Petrology.
The TerraSpec 4 Mineral Analyzer can be used in the field or the lab; accurately measures a wide variety of geologic samples, including clays and other alteration minerals. The high signal-to-noise ratio of this spectrometer allows for accurate measurement of even dark rocks containing an abundance of iron silicate minerals.
The TerraSpec Halo Mineral Identifier is an all-in-one full-range spectrometer (350-2500 nm) including the visible and short-wave infrared regions. Halo includes an onboard GPS producing GIS compatible information, audio recorder and internal wavelength standard to allow for easy operation, and efficient instrument status monitoring. It also features ASD’s proprietary, state-of-the-art mineral identification software for one click mineral-identification of up to seven minerals contained in a natural sample in the field or the lab.
Figure 1. Real-time mineral identification with the TerraSpec Halo in Death Valley, California (US). [2]
Halo Manager, the desktop computer-based software, allows for the configuration of the TerraSpec Halo instrument, display of Halo spectra and mineral identification results, and exporting of the data to third-party software programs like The Spectral Geologist (TSG®) Pro mineral analysis software by AusSpec
Ideal for Petrology applications:
1. Duke, E.F., and Lewis, R.S. (2010). Near infrared spectra of white mica in the Belt Supergroup and implications for metamorphism. American Mineralogist, 95, 908-920. doi: 10.2138/am.2010.3281
2. Duke, E.F. (2016). NIR, Metamorphic Petrology & Remote Sensing [Video Webinar]. Retrieved from http://www.asdi.com/learn/resources/videos/nir-metamorphicpetrology- and-remote-sensing.
3. Gazis, P., Newsom, H.E., & Stoker, C. (2001). Geological characterization of remote field sites using visible and infrared spectroscopy. Journal of geophysical research, 106(E4), 7683-7711.
4. Hubbard, M. (2003, November). Application of VIS/NIR spectral reflectance in sourcing and recognition of heat-treatment in cherts. In 2003 Seattle Annual Meeting.
5. Memorial University of Newfoundland (MUN). (2014, September 2). Petrology and Mineralogy. Retrieved from http://www.mun.ca/earthsciences/Research/Areas_of_Research/Petrology.php.
6. Pilorget, C., Fernando, J., Ehlmann, B. L., Schmidt, F., & Hiroi, T. (2016). Wavelength dependence of scattering properties in the VIS–NIR and links with grain-scale physical and compositional properties. Icarus, 267, 296-314.
7. Qiu, J.T., Li, P.J., Yu, Z.F., & Li, P. (2015). Petrology and Spectroscopy Studies on Danxia Geoheritage in Southeast Sichuan Area, China: Implications for Danxia Surveying and Monitoring. Geoheritage, 7(4), 307-318.