Riccardo Lanari

Mr. Riccardo Lanari

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Research Focus & Metrics

Academic Career Length

25Years (2002-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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14 December 2004 in Geophysical Research Letters
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RLRiccardo Lanari
Riccardo Lanari
PLPaul Lundgren
Paul Lundgren
MMMariarosaria Manzo
Mariarosaria Manzo
FCFrancesco Casu
Francesco Casu

15 July 2017 in Geophysical Research Letters
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Daniele CheloniDaniele Cheloni
Daniele Cheloni
VNVincenzo De Novellis
Vincenzo De Novellis
Matteo AlbanoMatteo Albano
Matteo Albano
AAA. Antonioli
A. Antonioli
Marco AnzideiMarco Anzidei
Marco Anzidei
CDCarlo Doglioni
Carlo Doglioni
We investigate a large geodetic data set of interferometric synthetic aperture radar (InSAR) and GPS measurements to determine the source parameters for the three main shocks of the 2016 Central Italy earthquake sequence on 24 August and 26 and 30 October (Mw 6.1, 5.9, and 6.5, respectively). Our preferred model is consistent with the activation of four main coseismic asperities belonging to the SW dipping normal fault system associated with the Mount Gorzano‐Mount Vettore‐Mount Bove alignment. Additional slip, equivalent to a Mw ~ 6.1–6.2 earthquake, on a secondary (1) NE dipping antithetic fault and/or (2) on a WNW dipping low‐angle fault in the hanging wall of the main system is required to better reproduce the complex deformation pattern associated with the greatest seismic event (the Mw 6.5 earthquake). The recognition of ancillary faults involved in the sequence suggests a complex interaction in the activated crustal volume between the main normal faults and the secondary structures and a partitioning of strain release.

24 May 2019 in IEEE Transactions on Geoscience and Remote Sensing
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MMMichele Manunta
Michele Manunta
CLClaudio De Luca
Claudio De Luca
IZIvana Zinno
Ivana Zinno
FCFrancesco Casu
Francesco Casu
MMMariarosaria Manzo
Mariarosaria Manzo
RLRiccardo Lanari
Riccardo Lanari
We present an advanced differential synthetic aperture radar (SAR) interferometry (DInSAR) processing chain, based on the Parallel Small BAseline Subset (P-SBAS) technique, for the efficient generation of deformation time series from Sentinel-1 (S-1) interferometric wide (IW) swath SAR data sets. We first discuss an effective solution for the generation of high-quality interferograms, which properly accounts for the peculiarities of the terrain observation with progressive scans (TOPS) acquisition mode used to collect S-1 IW SAR data. These data characteristics are also properly accounted within the developed processing chain, taking full advantage from the burst partitioning. Indeed, such data structure represents a key element in the proposed P-SBAS implementation of the S-1 IW processing chain, whose migration into a cloud computing (CC) environment is also envisaged. An extensive experimental analysis, which allows us to assess the quality of the obtained interferometric products, is presented. To do this, we apply the developed S-1 IW P-SBAS processing chain to the overall archive acquired from descending orbits during the March 2015-April 2017 time span over the whole Italian territory, consisting in 2740 S-1 slices. In particular, the quality of the final results is assessed through a large-scale comparison with the GPS measurements relevant to nearly 500 stations. The mean standard deviation value of the differences between the DInSAR and the GPS time series (projected in the radar line of sight) is less than 0.5 cm, thus confirming the effectiveness of the implemented solution. Finally, a discussion about the performance achieved by migrating the developed processing chain within the Amazon Web Services CC environment is addressed, highlighting that a two-year data set relevant to a standard S-1 IW slice can be reliably processed in about 30 h.The presented results demonstrate the capability of the implemented P-SBAS approach to efficiently and effectively process large S-1 IW data sets relevant to extended portions of the earth surface, paving the way to the systematic generation of advanced DInSAR products to monitor ground displacements at a very wide spatial scale.

26 December 2016 in Geophysical Research Letters
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GLG. Lavecchia
G. Lavecchia
Raffaele CastaldoRaffaele Castaldo
Raffaele Castaldo
RNR. de Nardis
R. de Nardis
VNVincenzo De Novellis
Vincenzo De Novellis
FFFederica Ferrarini
Federica Ferrarini
PTPietro Tizzani
Pietro Tizzani
We investigate the ground deformation and source geometry of the 2016 Amatrice earthquake (Central Italy) by exploiting ALOS2 and Sentinel‐1 coseismic differential interferometric synthetic aperture radar (DInSAR) measurements. They reveal two NNW‐SSE striking surface deformation lobes, which could be the effect of two distinct faults or the rupture propagation of a single fault. We examine both cases through a single and a double dislocation planar source. Subsequently, we extend our analysis by applying a 3‐D finite elements approach jointly exploiting DInSAR measurements and an independent, structurally constrained, 3‐D fault model. This model is based on a double fault system including the two northern Gorzano and Redentore‐Vettoretto faults (NGF and RVF) which merge into a single WSW dipping fault surface at the hypocentral depth (8 km). The retrieved best fit coseismic surface deformation pattern well supports the exploited structural model. The maximum displacements occur at 5–7 km depth, reaching 90 cm on the RVF footwall and 80 cm on the NGF hanging wall. The von Mises stress field confirms the retrieved seismogenic scenario.

28 January 2009 in Geophysical Research Letters
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Marco NeriMarco Neri
Marco Neri
FCFrancesco Casu
Francesco Casu
VAValerio Acocella
Valerio Acocella
Giuseppe SolaroGiuseppe Solaro
Giuseppe Solaro
SPSusi Pepe
Susi Pepe
RLRiccardo Lanari
Riccardo Lanari

7 June 2019 in Geophysical Research Letters
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VNVincenzo De Novellis
Vincenzo De Novellis
SASimone Atzori
Simone Atzori
CLClaudio De luca
Claudio De luca
MMMariarosaria Manzo
Mariarosaria Manzo
EVE. Valerio
E. Valerio
FCFrancesco Casu
Francesco Casu
We investigate the 24–27 December 2018 eruption of Mount Etna occurred from fissures located on the volcano eastern flank and accompanied by a seismic swarm, which was triggered by the magma intrusion and continued for weeks after the end of the eruption. Moreover, this swarm involved some of the shallow volcano‐tectonic structures located on the Mount Etna flanks and culminated on 26 December with the strongest event (ML 4.8), occurred along the Fiandaca Fault. In this work, we analyze seismological data and Sentinel‐1 Differential Interferometric Synthetic Aperture Radar (DInSAR) measurements, the latter inverted through analytical modeling. Our results suggest that a dike source intruded, promoting the opening of the eruptive fissures fed by a shallower dike. Moreover, our findings indicate that the activation of faults in different sectors of the volcano may be considered as a response to accommodate the deformations induced by the magma volumes injection.