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  • 1
    Publication Date: 2021-01-04
    Description: We investigated whether the joint inversion of geodetic and stress direction data can constrain long‐term fault slip rates in the central Apennines, and ultimately how extension is partitioned among fault slip and bulk lithosphere permanent strain. Geodetic velocities are collected in the fault interseismic stage with steady secular deformation; thus, long‐term estimates can be derived with a model of elastically unloading seismogenic faults within a viscously deforming lithosphere. As the average spacing of permanent Global Navigation Satellite Systems (GNSS) stations is similar to the average length of seismogenic faults (25–35 km), if not larger, we decided to merge permanent and temporary GNSS measurements, resulting in a denser geodetic data set. Given that most normal faults in the Apennines have slip rates around or below 1 mm/a, and most campaign GNSS velocities carry similar uncertainties, simple local back slip models cannot be applied. More sophisticated modeling is required to extract reasonable bulk deformation rates and long‐term fault slip rates at signal‐to‐noise ratio of order unity. Given the spatial distribution of the GNSS network, we estimated the long‐term slip rate of seven major fault systems that are in satisfactory agreement with available geological slip rates. The resulting spatial distribution of bulk deformation rates locally fits short‐term transients; in other cases, they represent the currently unclear signature of tectonic processes like upper‐crustal viscoplastic deformation and aseismic slip, or indicate missing faults in the adopted database. We conclude that the time is ripe for determining fault slip rates using geodetic and stress direction data, particularly where fault activity rates are hard to determine geologically.
    Description: Published
    Description: e2019JB018956
    Description: 2T. Deformazione crostale attiva
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 2
    Publication Date: 2020-02-19
    Description: An edited version of this paper was published by AGU. Copyright (2019) American Geophysical Union
    Description: The 2016 central Apennines earthquake sequence was caused by slip on an extensional fault system and resulted in sizable coseismic surface deformation. The most evident effects occurred along the western slope of Mount Vettore, a geologically and morphologically complex mountain ridge. Steep topography and rheological contrasts are known to have strongly controlled the coseismic deformation pattern during a number of different earthquakes that occurred in mountainous areas worldwide. Nevertheless, so far the role of seismically induced slope failures has not been taken into account in the interpretation of the surface fractures caused by the 2016 earthquake sequence. We modeled the static and dynamic slope stability along the western flank of Mount Vettore and in the underlying Piano Grande plain. Combining the slope stability analysis with geomorphic and geological analyses, we show that the coseismic fractures are distributed along the most unstable areas of the western flank of Mount Vettore and can be partly explained by shaking‐induced mechanisms such as gravity‐driven displacement, compaction, and secondary ground failure. Conversely, in the Piano Grande plain the fracture pattern is not affected by topography or rheology contrasts, suggesting that it is positively caused by tectonic faulting. Different processes, such as gravitational and erosional‐depositional phenomena, may contribute to the exposure of fault scarps during both the coseismic and interseismic periods. Attributing the surface deformation entirely to tectonic faulting, especially in complex mountainous terrains such as the Apennines, may lead to an incorrect assessment of fault displacement and fault slip rate and hence of seismic hazard.
    Description: Published
    Description: 994-1017
    Description: 2T. Deformazione crostale attiva
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 3
    Publication Date: 2019-02-25
    Description: Following the Mw 6.3 earthquake that hit the city of L'Aquila (Central Italy) on the 6th April 2009, a scientific project was proposed with the aim of investigating the Abruzzo area by means of different disciplinary approaches including geological, seismic, and physical studies. Electromagnetic field monitoring in the 0.01–500 mHz frequency band was implemented for the investigation of electromagnetic signals in the Earth's crust. Three measurement stations were installed in a tectonically active area with a radius of about 10 km. Each site was equipped with a fluxgate magnetometer with a 1 Hz sampling rate. This paper describes a long term geomagnetic deep sounding analysis for each site, aimed at investigating the dimensionality of the electrical structure of the subsurface in the area involved in the survey. According to a very simplified RL circuit model, some electrical properties of subsurface are also deduced.
    Description: Published
    Description: 32-37
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: JCR Journal
    Keywords: Electromagnetic inductionConductivity ; Tipper arrow ; Geoelectric strike
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2017-04-04
    Description: Il terremoto di L’Aquila del 2009 ci ha resi consapevoli che occorre fare un salto qualitativo nella osservazione dei campi magnetici naturali se vogliamo estendere le nostre indagini ai fenomeni elettromagnetici che accompagnano in generale i processi geodinamici (Palangio et al., 2008). Questo terremoto è l’unico nella storia che si sia verificato praticamente sotto un osservatorio geomagnetico con 50 anni di storia. La disponibilità di un così esteso archivio dati ci consente di monitorare tutta la fase preparatoria finale del terremoto. Stando alla letteratura corrente avremmo dovuto osservare effetti cosismici molto intensi, invece i segnali osservati lambiscono appena la superficie del mare di noise in cui sono immersi (Palangio et al., 2007) soltanto in alcune bande di frequenza i segnali ipogeici emergono nettamente dal rumore di fondo (Di Lorenzo et.al., 2011). Da questa esperienza del terremoto di L’Aquila è emersa la necessità di progettare un sistema osservativo che consenta di rilevare “l’impronta” del terremoto nei segnali elettromagnetici misurati sulla superficie terrestre. Questa impronta dovrebbe fornire la prova del legame tra il fenomeno tettonico e il campo magnetico osservato. Lo studio dei segnali magnetici prima e durante la fase sismica di L’Aquila ha messo in luce alcuni aspetti interessanti che riguardano il rumore di fondo e le finestre spettrali e temporali di osservabilità degli eventuali segnali magnetici di origine interna alla terra legati al terremoto.
    Description: Published
    Description: Potenza
    Description: 7A. Geofisica di esplorazione
    Description: open
    Keywords: interferometria, anomalie magnetiche ; 04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Conference paper
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  • 5
    Publication Date: 2017-04-04
    Description: Nei fondali marini in cui sono presenti discontinuità nelle proprietà fisico-chimiche quali ad esempio giacimenti minerari o di combustibili naturali [1] oppure discontinuità tettoniche si possono generare correnti elettriche che si chiudono in parte attraverso l'acqua del mare elettricamente molto conduttiva e in parte nel sottosuolo marino. Inoltre sono presenti anche correnti elettriche indotte dalle variazioni del campo magnetico e correnti generate per effetto MHD dal moto dell'acqua. In generale il campo magnetico misurato al di fuori del sistema di correnti che lo generano gode di due fondamentali proprietà: è indivergente e irrotazionale [5]. All'interno delle sorgenti il rotore del campo magnetico è legato alle correnti e quindi al campo elettrico, mentre la divergenza è legata alla presenza di pozzi o sorgenti di corrente o a gradienti non lineari del campo magnetico. In questo lavoro si propone il rilevamento del campo magnetico e delle correnti nei fondali marini mediante misure dirette della divergenza e del rotore del campo magnetico locale.
    Description: Published
    Description: Trieste
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: open
    Keywords: anomalie magnetiche, gradiometria tensoriale ; 03. Hydrosphere::03.01. General::03.01.08. Instruments and techniques
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Conference paper
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  • 6
    Publication Date: 2022-03-16
    Description: Several methods such as paleoseismic trenching, mapping of offset geomorphic markers, and dating of scarp profiles have been used to determine slip rates of normal faults in the central Apennines. Combining measurements obtained with different methods remains challenging because non-tectonic processes can introduce noise or spurious signals that are elusive to quantify, and these influence slip rate estimates. To this end, we meta-analyzed throw measurements with associated ages collected in the central Apennines with several methods to quantify such erratic fluctuations and method-related variances. We show that throw rates are overdispersed with respect to nominal uncertainties in throw and age; therefore, they are commonly affected by unmodeled noise processes. After comparing throw rate distributions sampling the same faults with different techniques, no clear spatiotemporal patterns appear, but only quasi-random noise. Assuming that field investigators sampled real tectonic features (i.e., fault scarps), we find that such erratic throw rates indicate total uncertainties are two to three times greater than the stated observation uncertainties. In this situation, a simple and robust null hypothesis is appropriate. We propose that most faults should be assumed to have uniform throw rate along their traces, except for possible tapering near unconnected ends. We also propose that models in which throw rates are time-dependent (within the last 25 ka) are not yet justified. Then, relying on the estimated total uncertainties, we determine the most probable long-term fault throw rate for each active fault by combining different throw-rate probability density functions.
    Description: Published
    Description: e2021JB023252
    Description: 2T. Deformazione crostale attiva
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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