EGU25-18914, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-18914
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 29 Apr, 14:00–15:45 (CEST), Display time Tuesday, 29 Apr, 14:00–18:00
 
Hall X2, X2.112
Field examples regarding Horizontal-to-Vertical Spectral Ratio measurements as a tool for shallow faulting investigation
Federica Davani1, Iolanda Gaudiosi1, Maurizio Simionato1, Grazia Maria Caielli1, Graziano Boniolo1, Attilio Porchia1, Giuseppe Tortorici1, Jessica Bellanova2, Giuseppe Calamita2, Angela Perrone2, Sabatino Piscitelli2, Luca Maria Puzzilli4, Vincenzo Di Fiore3, Marco Mancini1, Edoardo Peronace1, Stefano Catalano5, Antonio Torrisi6, and Roberto De Franco1
Federica Davani et al.
  • 1CNR-IGAG, DSSTTA, Roma, Italy
  • 2CNR-IMAA, DSSTTA, Tito Scalo (PZ), Italy
  • 3ISPC, DSU, Napoli, Italy
  • 4ISPRA, Roma, Italy
  • 5Università di Catania, DSBGA, Catania, Italy
  • 6Protezione Civile Regione Siciliana, Nicolosi (CT), Italy

In this study, we present the results of 76 Horizontal-to-Vertical Spectral Ratio (HVSR) measurements carried out near three active fault lineaments on the eastern flank of Mt. Etna (Santa Tecla-Linera, Fiandaca and Trecastagni). In this area, earthquakes are very shallow (within 2 km of depth) and produce surface fracturing and deformations around the identified emerging fault zones, even for moderate magnitude (Mw > 3.5), leading to widespread damage to  buildings. Therefore, accurately identifying the zones affected by surface faulting is fundamental for improving territorial management.

The dataset was processed using HVSR technique to obtain the HVSR curves and the related spectra, as well as to extrapolate information on the directional effects of the signals as a function of both frequency and azimuth. In the literature, the HVSR method has been successfully used to detect polarization effects across fault zones: previous studies have shown that horizontal polarization in Mt. Etna is often strong and tends to be perpendicular to the predominant fracture field or has high-angle polarization from the fault strike (Rigano et al. 2008; Di Giulio et al., 2009). We thus applied the wavefield polarization analysis to the ambient noise measurements to investigate the areal pattern of horizontal polarization and to identify any existing spatial variations. Moreover, the polarization angles were also estimated by using the Matlab code POLARGUI (Huailiang Li et al., 2021). This method allowed us to map the polar histograms and display the distributions of polarization azimuths in different frequency bands. The code is based on the decomposition of the eigenvectors and eigenvalues of the covariance matrix of the three ground motion components of Jurkevics (1988).

Lastly, since fault zones may produce fault-zone trapped waves, which may consist primarily of Love-type waves with particle motion parallel to the fault strike (e.g. Lewis & Ben-Zion 2010) or may include Rayleigh-type components with different polarization angles (e.g Ellsworth & Malin 2011), we computed the ellipticity curves obtained with the RayDec method (Hobiger et al., 2009) to isolate the contribution of Rayleigh waves alone.

The ellipticity of the Rayleigh waves was analyzed for all the measurements to identify any differences that might indicate the presence of a surface faulting zone. To emphasize the deviation between the HVSR curves and the ellipticity curves, a residuals analysis was performed based on the Root Mean Squared Error (RMSE).

These results enabled the identification and proposal a new indicator as proxy for the presence of the fault system and/or any associated fracture field, to be integrated with other types of geophysical measurements.

Acknowledgements: The measurements are part of the geophysical acquisitions for the ETNA-FAC project, signed by CNR IGAG with the Regional Department of Sicilian Civil Protection. The project involved: CNR IGAG, INGV, University of Catania, OGS, ISPRA, CNR ISPC and CNR IMAA.

How to cite: Davani, F., Gaudiosi, I., Simionato, M., Caielli, G. M., Boniolo, G., Porchia, A., Tortorici, G., Bellanova, J., Calamita, G., Perrone, A., Piscitelli, S., Puzzilli, L. M., Di Fiore, V., Mancini, M., Peronace, E., Catalano, S., Torrisi, A., and De Franco, R.: Field examples regarding Horizontal-to-Vertical Spectral Ratio measurements as a tool for shallow faulting investigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18914, https://doi.org/10.5194/egusphere-egu25-18914, 2025.