Feasibility of Using a 300 GHz Radar to Detect Fractures and Lithological Changes in Rocks

Author:

Sanjuan Federico1ORCID,Fauquet Frédéric2,Fasentieux Bertrand3,Mounaix Patrick2ORCID,Guillet Jean-Paul2ORCID

Affiliation:

1. E2S UPPA, CNRS, TotalEnergies, LFCR, Université de Pau et des Pays de l’Adour, 64013 Pau, France

2. UMR 5218, CNRS 351 Cours de la Libération, IMS Laboratory, University of Bordeaux, 33405 Talence, France

3. Géosciences, Collège STEE, Université de Pau et des Pays de l’Adour, 64013 Pau, France

Abstract

The detection and quantification of fractures in rocks, as well as the detection of lithological changes, are of particular interest in scientific fields, such as construction materials, geotechnics, reservoirs and the diagnostics of dielectric composite materials and cultural heritage objects. Therefore, different methods and techniques have been developed and improved over the years to provide solutions, e.g., seismic, ground-penetrating radar and X-ray microtomography. However, there are always trade-offs, such as spatial resolution, investigated volume and rock penetration depth. At present, high-frequency radars (>60 GHz) are available on the market, which are compact in size and capable of imaging large areas in short periods of time. However, the few rock applications that have been carried out have not provided any information on whether these radars would be useful for detecting fractures and lithological changes in rocks. Therefore, in this work, we performed different experiments on construction and reservoir rocks using a frequency-modulated continuous wave radar working at 300 GHz to evaluate its viability in this type of application. The results showed that the radar quantified millimeter fractures at a 1 cm rock penetration depth with a sensitivity of 500 μm. Furthermore, lithological changes were identified, even when detecting interfaces generated by the artificial union of two samples from the same rock.

Funder

I-site E2S UPPA

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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