EGU26-6444, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-6444
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 14:00–15:45 (CEST), Display time Monday, 04 May, 14:00–18:00
 
Hall X3, X3.22
Assessing the feasibility of DInSAR for detecting coseismic deformation in small-magnitude earthquakes: the 2023 ML 4.4 Umbertide earthquake (Central Italy)
Riccardo Gaspari1, Martina Occhipinti2,3, Claudio De Luca2, Fernando Monterroso2, Federica Riva4,5, Ioannis Doukakos6, Shaila Amorini6, Giacomo Cenci1, Massimiliano Rinaldo Barchi1,3,4, and Massimiliano Porreca1,3
Riccardo Gaspari et al.
  • 1Department of Physics and Geology, University of Perugia, Perugia, Italy
  • 2National Research Council (CNR), Istituto per il Rilevamento Elettromagnetico dell’Ambiente (IREA), Naples, Italy
  • 3CRUST, Interuniversity Centre for 3D Seismotectonics with Territorial Applications, Chieti, Italy
  • 4Istituto Nazionale di Geofisica e Vulcanologia (INGV), Osservatorio Nazionale Terremoti, Italy
  • 5International School of Advanced Studies, Camerino, Italy
  • 6EagleProjects S.p.A., Perugia, Italy

Differential Interferometric Synthetic Aperture Radar (DInSAR) techniques are largely used to detect coseismic deformation patterns associated with large-to-moderate magnitude earthquakes. In contrast, small earthquakes (M<5), although far more frequent and potentially crucial for understanding regional stress regimes and active faulting, generally produce weak surface deformation that is difficult to detect using remote sensing approaches.

In this work, we integrate relocated seismicity, observed DInSAR deformation, and the Okada elastic dislocation model to infer insights into the geometry and mechanics of the causative fault of the 2023 ML 4.4 Umbertide extensional earthquake in Central Italy. The seismicity was relocated using the Non-Linear Earthquake Location Algorithm in combination with the three-dimensional velocity model developed specifically for the area.

We benefited of Sentinel-1 Line Of Sight (LOS) displacement maps generated over ascending and descending orbits through the EPOSAR service of the European Plate Observing System (EPOS) Research Infrastructure. These data were exploited to derive the vertical and east-west deformation components using a recently developed open-source Python tool capable of combining multiple LOS displacement maps. The results reveal up to ~2 cm of subsidence and ~1.5 cm of eastward motion in the epicentral area, suggesting the activation of a NE-dipping normal fault, consistent with the relocated seismicity distribution.

The focal mechanism parameters of this plane were adopted for the Okada modeling. According to the maximum-likelihood solution of the ML 4.4 mainshock relocation, the source was modeled at 3.5 km of depth. The best-fitting solution between the modeled and observed deformation is a rectangular planar fault measuring 2.3 × 2.7 km (L × W), with a maximum slip of 20 cm.

Despite the earthquake’s limited magnitude and the surface deformation signal being partially affected by atmospheric disturbances, properly applied DInSAR techniques can provide a detailed estimation of surface displacement. The results demonstrate DInSAR’s ability to detect deformation induced by small-magnitude earthquakes in a seismically active region, with the potential to improve active fault mapping and seismic hazard assessment.

How to cite: Gaspari, R., Occhipinti, M., De Luca, C., Monterroso, F., Riva, F., Doukakos, I., Amorini, S., Cenci, G., Barchi, M. R., and Porreca, M.: Assessing the feasibility of DInSAR for detecting coseismic deformation in small-magnitude earthquakes: the 2023 ML 4.4 Umbertide earthquake (Central Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6444, https://doi.org/10.5194/egusphere-egu26-6444, 2026.