ERT data collected at the Corona volcano (Lanzarote, Canary Islands) during the European Space Agency (ESA) testing campaign PANGAEA-X 2017
Creators
- 1. Università di Pavia, Dipartimento di Scienze della Terra e dell'Ambiente
- 2. Università di Padova
- 3. Jacobs University Bremen, Physics and Earth Sciences
- 4. Università di Bologna
- 5. Julius-Maximilians-Universität Würzburg
Description
This dataset contains the ERT (Electrical Resistivity Tomography) data collected between 22 and 23 November 2017 at the Corona volcano (Lanzarote, Canary Islands, Fig. 1) for the detection of lava tubes and the stratigraphic investigation of planetary volcanic analogues. This geophysical survey was carried out within the European Space Agency (ESA) testing campaign PANGAEA-X 2017 (Bessone et al., 2018), aimed at integrating astronaut training-data collection, documentation, analogue field geology procedures with remote sensing and in situ geophysical methods.
Two ERT profiles were acquired in NE-SW and NNE-SSW orientations (Fig. 1). These were located roughly orthogonal to the Corona lava tube system and as far as possible on top of the main lava tube axes. The longer profile, profile D, is 470 m in length and was obtained using 48 electrodes spaced 10 m apart. The profile orientation is from SW to NE (electrode 1 to 48). The profile was acquired to detect lava tubes in test site D (sub-area south) where the exact location of a lava tube was known thanks to a LiDAR TLS (Terrestrial Laser Scan) subsurface survey (Santagata et al., 2018). A shorter profile, profile E, is 235 m long and was obtained using 48 electrodes 5 m apart. The profile orientation is from SSW to NNE (electrode 1 to 48). This profile was acquired in test site E (sub-area north) to provide a more detailed investigation of the potential existence of inaccessible sections of the tube whose location could be indicated by the evidence of closely-spaced aligned collapse structures.
Each profile was collected using measure sequences compounded by 276 Wenner-Schlumberger array quadrupoles which ensure high vertical resolution and signal amplitude and 328 dipole-dipole array quadrupoles which provide enhanced lateral resolution. A fully automatic multi-electrode resistivity meter SYSCAL Jr Switch-48 by IRIS Instruments (400 V max output voltage, 1200 mA max output current, 100 W max output power, http://www.iris-instruments.com/syscal-juniorsw.html), was used for data collection.
At most of the measurement points, it was necessary to drill the basalt using a hand drilling machine in order to place the tips of the electrodes into the ground at a depth of approximately 40 cm. The electrodes also needed to kept moist to reduce contact resistance between the electrode and the ground. A large amount of water (up to 2 liters per point) was needed for profile D, situated in an area above the lava tubes with very porous dry soil cover.
The dataset is presented as a spreadsheet format which has the "space" as separator and the ".txt" extension. The structure of such a file is the following one:
#, El array, Spa1/4, Rho, Dev, M, Sp, Vp, In, Time, Spa5/12, M1/20
- #: Data point number
- El array: Electrode array
- Spa. 1/4: four spacing parameters (corresponding to the electrode array – in m)
- Rho: resistivity value (in Ohm.m)
- Dev: standard deviation (quality factor, in %)
- M: global chargeability value (induced polarization parameter (in mV/V – "=0" if only-resistivity data))
- Sp: spontaneous polarization (measured just before the injection, in mV)
- Vp: measured primary voltage (in mV)
- In: injected current intensity (in mA)
- Time: injection time (pulse duration, in s)
- Spa. 5/8: other spacing parameters (in m)
- Spa. 9/12: electrode elevation (in m)
- M1/M20: partial chargeability values (induced polarization window (in mV/V – "=0" if only-resistivity data))
Acknowledgements
The authors are grateful to ESA and all PANGAEA-X 2017 staff, particularly Loredana Bessone, Matthias Maurer, Herve Stevenin and Igor Drozdovskiy for their participation in data collection during some of the experiments and to the MilesBeyond Team, particularly Francesco Maria Sauro for his logistical support. Regional and local remote sensing data were obtained by the Spanish Instituto Geográfico Nacional (https://www.ign.es) and Gobierno de Canarias (https://www.grafcan.es, https://opendata.sitcan.es).
References
Bessone, L., et al., 2018, Testing technologies and operational concepts for field geology exploration of the Moon and beyond: the ESA PANGAEA-X campaign, Geophysical Research Abstract, #EGU2018-4013.
Santagata, T., Sauro, F., Massironi, M., Pozzobon, R., Del Vecchio, U., Lazzaroni, M., Damiano, N., Tonello, M., Tomasi, I., Martínez-Frìas, J. and Mateo Medero, E., 2018. Subsurface laser scanning and photogrammetry in the Corona Lava Tube System, Lanzarote, Spain, EGU General Assembly 2018, pp. EGU2018-5290.
Notes
Files
Fig. 1.pdf
Files
(1.1 MB)
Name | Size | Download all |
---|---|---|
md5:3c7400246c43cf4e7dc031695d0079db
|
652.6 kB | Preview Download |
md5:17533a587153ffee824a680f9b8d6994
|
121.5 kB | Preview Download |
md5:a5db0a66547ca02cea299fb178921417
|
101.3 kB | Preview Download |
md5:58837400c4affe8a95cacc375545326f
|
119.3 kB | Preview Download |
md5:97ab4226bfac75deb74f733b3eedafb4
|
99.3 kB | Preview Download |