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Three-dimensional numerical simulation of ambient seismic noise for arbitrary surface source distributions: application to the study of horizontal-to-vertical spectral ratios and their variability
Seismologists have been exploiting ambient seismic noise for decades to investigate subsurface properties. Among the earliest methods developed, the analysis of H/V spectral ratios, introduced in the early 1970s by Japanese researchers, is now widely used to identify the frequencies at which ground motion may be amplified during an earthquake. Despite its widespread use, the interpretation of H/V measurements still raises many questions, particularly when they exhibit significant temporal variations.
This is precisely what was observed at the Volvi site, in the Mygdonia Basin in northern Greece, where the frequency of the main H/V peak can shift from 1 Hz to 2 Hz within a single day.
To better understand this striking variation, we conducted an in-depth numerical investigation of the sensitivity of H/V measurements to the spatial distribution of noise sources and to the presence of strong lateral structural contrasts. The Volvi site is indeed characterized by a particular geological setting, with a so-called "blind fault", buried beneath the surface, separating two parts of the basin with different properties.
We investigated not only H/V amplitude but also its polarization, that is, the presence of preferred directions in horizontal ground motion. This approach makes it possible to explore how source-related and structural effects can combine or even mask one another.
This work contributes to a better understanding of the information contained in ambient seismic noise measurements and of the precautions required when interpreting them. It also highlights the potential of H/V polarization, an observable that remains relatively underexplored, for characterizing complex geological structures.
To better understand this striking variation, we conducted an in-depth numerical investigation of the sensitivity of H/V measurements to the spatial distribution of noise sources and to the presence of strong lateral structural contrasts. The Volvi site is indeed characterized by a particular geological setting, with a so-called "blind fault", buried beneath the surface, separating two parts of the basin with different properties.
We investigated not only H/V amplitude but also its polarization, that is, the presence of preferred directions in horizontal ground motion. This approach makes it possible to explore how source-related and structural effects can combine or even mask one another.
This work contributes to a better understanding of the information contained in ambient seismic noise measurements and of the precautions required when interpreting them. It also highlights the potential of H/V polarization, an observable that remains relatively underexplored, for characterizing complex geological structures.
Figure 1. Numerical model of the Volvi basin showing the distribution of noise sources and receivers on either side of a blind fault. The results illustrate variations in the frequency of the H/V spectral peak depending on receiver location, as well as the differences observed between the shallow and deep parts of the basin.
The full study is published in: Geophysical Journal International
References :
Gregor, D., Chaljub, E., Wathelet, M., Hollender, F., Perron, V., & De Martin, F. (2026). Three-dimensional numerical simulation of ambient seismic noise for arbitrary surface source distributions: application to the study of horizontal-to-vertical spectral ratios and their variability. Geophys. J. Int., 247(2), ggag348.
Scietific contacts:
- David Gregor – ISTerre, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, Univ. Gustave Eiffel, Grenoble, France
- Emmanuel Chaljub – ISTerre, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, Univ. Gustave Eiffel, Grenoble, France
- Marc Wathelet – ISTerre, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, Univ. Gustave Eiffel, Grenoble, France
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