AusLAMP - Illuminating Australia's deep earth

About AusLAMP

The Australian Lithospheric Architecture Magnetotelluric Project (AusLAMP) is a collaborative, national survey that acquires long-period magnetotelluric (MT) data at approximately 3000 sites across the Australian continent. It is being conducted over multiple years to create a new national MT dataset. This dataset will be used to map electrical conductivity structures in the crust and upper mantle to improve our understanding of the geology and tectonic evolution of the Australian plate. The results will provide new information for identifying regions with mineral and energy resource potential. The AusLAMP dataset is an essential input to the Exploring for the Future program.

AusLAMP assists with

  • understanding the geological make up of Australia
  • understanding how geological processes work
  • geological hazard mapping such as earthquake risk
  • analysing risks to Australia's electricity infrastructure
  • helping to identify mineral and energy resource potential at a broad regional scale, not at a local property scale.

This visionary project can only be achieved with the involvement of many government and research organisations. AusLAMP is led by Geoscience Australia in conjunction with the State and Northern Territory geological surveys, universities, and other research organisations. The long-period MT instruments used in the project are from two equipment pools, one co-funded by AuScope and accessed through ANSIR Research Facilities For Earth Sounding, the other managed by Geoscience Australia. AuScope is funded by the Australian Government under the National Collaborative Research Infrastructure Strategy (NCRIS). The field data are acquired by these portable instruments on a half-degree grid spacing (approximately 55 km) during deployments of 4‑6 weeks. This records sufficient data to image to the base of the lithosphere (the rigid upper plate of the Earth). The acquisition phase of AusLAMP is expected to take more than 15 years to complete.

AusLAMP progress

AusLAMP was launched in November 2013. To date, data have been acquired at about 1300 stations, which is approximately 40% of the national coverage. In Victoria, data acquisition was undertaken by the Geological Survey of Victoria and Geoscience Australia in 2014 and 2017. In Tasmania, data were acquired by the University of Tasmania, the Tasmanian Government, and Geoscience Australia in 2016. Data acquisition in South Australia was completed through a collaboration between the Geological Survey of South Australia, the University of Adelaide, and Geoscience Australia between 2014 and 2017.

Further data acquisition is ongoing. The Geological Survey of New South Wales and Geoscience Australia have essentially completed acquisition in New South Wales. As part of the Exploring for the Future program, Geoscience Australia has acquired, or plans to acquire, AusLAMP data in the Northern Territory in collaboration with the Northern Territory Geological Survey, in Queensland with the Geological Survey of Queensland, and in Western Australia with the Geological Survey of Western Australia.

Data accessibility

Time-series data, processed data, inversion products, and reports will be released progressively throughout the project. The data and associated products are freely available to the public, scientific research organisations, and industry. Figure 2 is an example of a recently released AusLAMP model, showing the electrical conductivity structure at a depth of about 36 km in the Northern Territory and western Queensland (Duan et al., 2021; Jiang and Duan, 2020; Doublier, 2020).

AusLAMP land access

AusLAMP requires Geoscience Australia staff, its collaborators and contractors to access sites on various landholdings, including farms, national parks and Indigenous lands. Prior agreement to access these sites is always sought through consultation with landowners, traditional owners and other relevant stakeholders.

AusLAMP partners

AusLAMP in detail

AusLAMP is a long-period MT survey that images the electrical conductivity structure of the Australian continental lithosphere in three dimensions (3D) and aims to identify and characterise major geological structures in the crust and upper mantle. The survey results provide new insight and valuable information for the Australian continental lithosphere framework and address fundamental questions, such as how the current geological structure was established, the nature of the geological processes, and how large-scale crustal and lithospheric structures control mineral deposition and hydrocarbon basin formation. The survey results can be integrated with other national datasets, such as aeromagnetic, gravity, seismic tomography, geochemical, and geological datasets. The integration of these multidisciplinary datasets will help to develop a better scientific understanding of the lithospheric architecture and evolution of the Australian continent, highlighting prospective areas for mineral and energy resources at a regional scale, as well as to assess geoelectric and other geological hazards.

Magnetotelluric method

Magnetotellurics is a passive geophysical technique that measures variations of the Earth's naturally occurring magnetic and electric fields to derive the electrical resistivity distribution of the subsurface. Different types of MT instruments – audio, broadband and long-period – acquire data in different frequency ranges, giving an overall investigation depth of tens of meters to hundreds of kilometres. MT source fields are generated by worldwide thunderstorm activity (mainly lightning discharges at a frequency above 1 Hz) and the interactions between the solar wind and the Earth's magnetic field in the magnetosphere and ionosphere (at a frequency less than 1 Hz). These sources provide a rich spectrum of magnetic-field variations in the band 10-5 to 104 Hz, which are suited for crust and upper mantle studies. These signals vary in strength over hours, days, weeks and over the solar cycle.

The time-series measurements of the magnetic and electric fields are converted to a set of frequency responses through Fourier transformation – the lower the frequency the deeper the source of the Earth response. In order to image the deep crust and upper mantle it is necessary to measure very low frequencies to achieve sensitivity to the base of the lithosphere. Using these data, a 3D Earth electrical conductivity model can be generated by sophisticated mathematical inversion algorithms on high performance computers.

The MT method is widely used for mineral, petroleum and geothermal exploration, and in studies of the crust and mantle. The main strengths of the method are that it allows a broader range of investigation depths than other geophysical techniques, and it has a greater level of sensitivity to lateral and vertical electrical conductivity variations. It is useful for distinguishing different rock types and helping to understand geological structures and tectonic evolution.

AusLAMP data acquisition

An AusLAMP survey collects long-period MT data using portable instruments on a grid of approximately 55 km (half-degree geodetic). AusLAMP instruments include a three-component fluxgate magnetometer and dipoles with electrodes to record continuous magnetic and electric signals in the field. AusLAMP surveys target signals in the range 10 s–20,000 s, which is an investigation depth from a few kilometres to hundreds of kilometres. To ensure the MT measurement captures sufficient natural signals at longer periods, data is collected for 4‑6 weeks at each site. Multiple stations are recorded simultaneously for the purposes of remote reference processing that improves the quality of processed data.

AusLAMP acquisition box and solar panels.

A typical MT station is shown above. Deployment sites are in open areas approximately 100 x 100 m in size, away from human-made noise sources such as houses, electric fences, power lines and major roads.

The deployed instruments comprise:

  • an acquisition box containing a data recording unit, GPS and 12 volt battery
  • four electrodes buried 50 cm deep and spaced 100 m apart on a north, south, east and west axis – the electrodes are connected to the acquisition box with a cable and, where required, the cable is buried
  • three magnetic sensors (within a single magnetometer) buried 50 cm deep and connected to the acquisition box by a 20 m cable, which is also buried
  • a small solar panel mounted close to the acquisition box to charge the battery.

Further information

For further information, contact Geoscience Australia via email