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  • 04. Solid Earth::04.03. Geodesy::04.03.06. Measurements and monitoring  (25)
  • 04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolution  (7)
  • 04. Solid Earth::04.06. Seismology::04.06.04. Ground motion
  • Astronomy
  • E31
  • E52
  • J24
  • 2015-2019  (35)
  • 1
    Publication Date: 2019-07-13
    Description: We report the design of a new application-specific integrated circuit (ASIC) for use in radio telescope correlators. It supports the construction of correlators for an arbitrarily large number of signals. The ASIC uses an intrinsically low-power architecture along with design techniques and a process that together result in unprecedentedly low power consumption. The design is flexible in that it can support telescopes with almost any number of antennas N. It is intended for use in an "FX" correlator, where a uniform filter bank breaks each signal into separate frequency channels prior to correlation.
    Keywords: Astronomy
    Type: United States National Committee of URSI National Radio Science Meeting (USNC-URSI NRSM); Jan 06, 2016 - Jan 09, 2016; Boulder, CO; United States
    Format: text
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  • 2
    Publication Date: 2019-08-26
    Description: Radio telescopes that employ arrays of many antennas are in operation, and ever larger ones are being designed and proposed. Signals from the antennas are combined by cross-correlation. While the cost of most components of the telescope is proportional to the number of antennas N, the cost and power consumption of cross-correlationare proportional to N2 and dominate at sufficiently large N. Here we report the design of an integrated circuit (IC) that performs digital cross-correlations for arbitrarily many antennas in a power-efficient way. It uses an intrinsically low-power architecture in which the movement of data between devices is minimized. In a large system, each IC performs correlations for all pairs of antennas but for a portion of the telescope's bandwidth (the so-called "FX" structure). In our design, the correlations are performed in an array of 4096 complex multiply-accumulate (CMAC) units. This is sufficient to perform all correlations in parallel for 64 signals (N=32 antennas with 2 opposite-polarization signals per antenna). When N is larger, the input data are buffered in an on-chipmemory and the CMACs are re-used as many times as needed to compute all correlations. The design has been synthesized and simulated so as to obtain accurate estimates of the IC's size and power consumption. It isintended for fabrication in a 32 nm silicon-on-insulator process, where it will require less than 12mm2 of silicon area and achieve an energy efficiency of 1.76 to 3.3 pJ per CMAC operation, depending on the number of antennas. Operation has been analyzed in detail up to N = 4096. The system-level energy efficiency, including board-levelI/O, power supplies, and controls, is expected to be 5 to 7 pJ per CMAC operation. Existing correlators for the JVLA (N = 32) and ALMA (N = 64) telescopes achieve about 5000 pJ and 1000 pJ respectively usingapplication-specific ICs in older technologies. To our knowledge, the largest-N existing correlator is LEDA atN = 256; it uses GPUs built in 28 nm technology and achieves about 1000 pJ. Correlators being designed for the SKA telescopes (N = 128 and N = 512) using FPGAs in 16nm technology are predicted to achieve about 100 pJ.
    Keywords: Astronomy
    Type: Journal of Astronomical Instrumentation; 5; 2; 1650002
    Format: text
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  • 3
    Publication Date: 2021-03-02
    Description: This study presents new geological and seismological data that are used to assess the seismic hazard of a sector of the Po Plain (northern Italy), a large alluvial basin hit by two strong earthquakes on May 20 (Mw 6.1) and May 29 (Mw 6.0), 2012. The proposed interpretation is based on high-quality relocation of 5,369 earthquakes ( 'Emilia sequence‘) and a dense grid of seismic profiles and exploration wells. The analysed seismicity was recorded by 44 seismic stations, and initially used to calibrate new one-dimensional and three- dimensional local Vp and Vs velocity models for the area. Considering these new models, the initial sparse hypocenters were then relocated in absolute mode and adjusted using the double-difference relative location algorithm. These data define a seismicity that is elongated in the W-NW to E-SE directions. The aftershocks of the May 20 mainshock appear to be distributed on a rupture surface that dips ~45° SSW, and the surface projection indicates an area ~10 km wide and 23 km long. The aftershocks of the May 29 mainshock followed a steep rupture surface that is well constrained within the investigated volume, whereby the surface projection of the blind source indicates an area ~6 km wide and 33 km long. Multichannel seismic profiles highlight the presence of relevant lateral variations in the structural style of the Ferrara folds that developed during the Pliocene and Pleistocene. There is also evidence of a Mesozoic extensional fault system in the Ferrara arc, with faults that in places have been seismically reactivated. These geological and seismological observations suggest that the 2012 Emilia earthquakes were related to ruptures along blind fault surfaces that are not part of the Pliocene-Pleistocene structural system, but are instead related to a deeper system that is itself closely related to re-activation of a Mesozoic extensional fault system.
    Description: Published
    Description: 107–123
    Description: 5T. Sorveglianza sismica e operatività post-terremoto
    Description: JCR Journal
    Description: restricted
    Keywords: velocity model ; relocated hypocenters ; double-difference locations ; Po Plain ; May 2012 Emilia earthquakes ; reactivated extensional faults ; 04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolution
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2021-03-01
    Description: Seismic hazard studies have been undertaken at Etna volcano in the last years with the aim of estimating the potential of local fault’s activity in generating destructive earthquakes. The target is the mid-term assessment (30, 20, 10 and 5 yrs), as the identification of zones that are exposed to the recurrent seismic shaking may be important for land planning at a local scale, and it represents a valuable complement to establish priority criteria for seismic risk reduction action. The methodologies applied at Mt. Etna area include probabilistic approaches based on the use of historical macroseismic data (the “site approach” by the software code SASHA, see Azzaro et al., 2008) and fault-based time-dependent models in which occurrence probabilities of major earthquakes are estimated through the Brownian Passage Time (BPT) function and the time lapsed since the last event (Azzaro et al., 2012b, 2013b). Mean return period of major earthquakes - strong to destructive events with epicentral intensity I0 ≥ VIII EMS, considered as “proxies” of “characteristic” earthquakes – have been obtained by the fault seismic histories, i.e. the associations “earthquake-seismogenic fault” derived from the historical catalogue of Etnean earthquakes (CMTE Working Group, 2014). Inter-time statistics of major earthquakes have been applied to the Timpe tectonic system, considered as a homogeneous seismotectonic domain (Azzaro et al., 2013b), obtaining a mean recurrence time (Tmean) of 71.3 years, and an aperiodicity factor α (σTmean/Tmean) = 0.42, typical of semi-periodic processes. In the present study we present the preliminary results of an analysis aimed at verifying the variability of the mean occurrence times of major earthquakes generated by the main tectonic systems at Etna (Pernicana and Timpe faults) by using a geological approach based on geometrickinematic parameters (3D dimensions, slip-rates etc) representative of fault activity. Method and input data.
    Description: Published
    Description: Bologna, Italy
    Description: 3T. Pericolosità sismica e contributo alla definizione del rischio
    Description: open
    Keywords: Seismic rate, faults ; 04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolution
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Extended abstract
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  • 5
    Publication Date: 2017-04-04
    Description: Durante il IV semestre di attività, l’Unità di Ricerca “Analisi delle sorgenti sismogenetiche” (OR2), ha ampliato ulteriormente il numero di scenari di scuotimento prodotti per il sito dimostratore di Cosenza (vedi precedente rapporto tecnico), eseguendo nuove modellazioni a sorgente estesa anche per la classe di magnitudo 5.0. Al fine di validare l’affidabilità degli scenari di scuotimento si eseguirà il confronto tra le distribuzioni statistiche dei parametri di strong motion simulati (e.g. PGA e PGV) con quelle predette dalle più recenti GMPEs europee (Bindi et al., 2014). Il range di validità di suddette relazioni empiriche predittive del moto del suolo è compatibile, in termini di magnitudo e distanza, con quello degli eventi di scenario modellati per il sito di Cosenza. Per l’analisi di dettaglio dei risultati acquisiti si rimanda al rapporto tecnico del prossimo semestre di attività.
    Description: PON 01/02710 MASSIMO - Monitoraggio in Area Sismica di SIstemi MOnumentali
    Description: Unpublished
    Description: 2T. Tettonica attiva
    Description: 3T. Pericolosità sismica e contributo alla definizione del rischio
    Description: reserved
    Keywords: Calabria ; Faglie sismogeniche ; Scenari di scuotimento ; Sismogrammi sintetici ; 04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolution ; 04. Solid Earth::04.06. Seismology::04.06.04. Ground motion
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: report
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  • 6
    Publication Date: 2017-04-04
    Description: Durante il V semestre di attività, l’Unità di Ricerca “Analisi delle sorgenti sismogenetiche” (OR2), ha prodotto gli scenari di scuotimento per il sito dimostratore di Reggio Calabria, eseguendo n. 31 modellazioni a sorgente estesa per le classi di Mw 5.0, 6.0 e 7.0 e adottando il medesimo work flow proposto per il sito di Cosenza, per la cui descrizione si rimanda al report del III semestre di attività. Nella fase di aggiornamento dei dati geologici in Calabria meridionale è stata di fondamentale importanza la collaborazione con la UR Rilievi Aeromagnetici.
    Description: PON 01/02710 MASSIMO - Monitoraggio in Area Sismica di SIstemi Monumentali
    Description: Unpublished
    Description: 2T. Tettonica attiva
    Description: 3T. Pericolosità sismica e contributo alla definizione del rischio
    Description: reserved
    Keywords: Calabria ; Faglie sismogeniche ; Scenari di scuotimento ; Sismogrammi sintetici ; 04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolution ; 04. Solid Earth::04.06. Seismology::04.06.04. Ground motion
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: report
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  • 7
    Publication Date: 2020-02-24
    Description: The Sybaris archaeological site, founded by the Greeks in 720 B.C., is located within the Sibari Plain near the Crati River mouth (Ionian northern Calabria, southern Italy), in an almost flat and low-lying area (Fig. 1). The plain is bounded by the Pollino chain to the north and by the Sila massif and the northern Crati basin to the south and west. From a seismotectonic point of view, Sybaris is located inferences the northeastern Calabrian arc, the tectonic evolution of which is controlled by slow north-northwest/south-southeast convergence between the Eurasian and African–Adriatic continental plates (e.g., Gvirtzmann and Nur, 1999; Argnani, 2000; Jolivet and Faccenna, 2000). Throughout the Calabrian arc, complex dynamics associated with subduction and rollback have produced back-arc extension, widespread uplift, and relative subsidence in the major tectonic basins, including Sibari, where mainly normal seismogenic faults accommodate internal deformation. The interior of the Sibari Plain has a high seismogenic potential, and recently, on July 2010, theMt. Pollino chain area experienced a three-year seismic sequence with magnitudes up to 5.2 (Fig. 1), following 30 years of seismic quiescence. In contrast, low to moderate seismicity characterizes the eastern half of the plain closer to the Ionian Sea, where the archaeological site of Sybaris is located (Fig. 1). Although not well constrained, there is evidence for active compression in this portion of northern Calabria and the Ionian Sea, where mostly strike-slip faults aremapped (e.g., Frepoli and Amato, 2000; Galadini et al., 2001; Pondrelli et al., 2006; Scognamiglio et al., 2009; Comerci et al., 2013; Fig. 1), but significant uncertainty exists on locations, geometry, and age of these faults. The 2700-year long record of history stored in the archaeological site of Sybaris may have recorded the traces of earthquakes that occurred in the area by sealing their effects in the sediments and in the archaeological remains. An archaeoseismic study of the site constitutes a unique means to deepenour knowledge of the seismotectonic of the area. The recognition and characterization of the coseismic deformation affecting the structures of the Sybaris archaeological site is the objective of the present study. To identify past seismic deformation events at Sybaris, we proceeded with (1) a systematic survey of the deformed structures, (2) an analysis of the tectonic deformation, (3) the formulation of a hypothesis for tectonics and earthquakes inferences, and (4) constraints on the timing of the deformation based on archaeological stratigraphy and absolute dating.
    Description: Published
    Description: 245-254
    Description: 2T. Tettonica attiva
    Description: JCR Journal
    Description: restricted
    Keywords: Archaeo-seismology ; Active tectonics ; 04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolution
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 8
    Publication Date: 2017-04-04
    Description: INGV - Sezione di Napoli Osservatorio Vesuviano
    Description: Unpublished
    Description: 5V. Sorveglianza vulcanica ed emergenze
    Description: 1IT. Reti di monitoraggio e Osservazioni
    Description: open
    Keywords: Campi Flegrei ; Gravity changes ; Volcano monitoring ; 04. Solid Earth::04.02. Exploration geophysics::04.02.02. Gravity methods ; 04. Solid Earth::04.03. Geodesy::04.03.05. Gravity variations ; 04. Solid Earth::04.03. Geodesy::04.03.06. Measurements and monitoring ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: report
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  • 9
    Publication Date: 2017-04-04
    Description: INGV - Sezione di Napoli Osservatorio Vesuviano
    Description: Unpublished
    Description: 5V. Sorveglianza vulcanica ed emergenze
    Description: 1IT. Reti di monitoraggio e Osservazioni
    Description: open
    Keywords: Vesuvio ; Gravity changes ; Volcano monitoring ; 04. Solid Earth::04.02. Exploration geophysics::04.02.02. Gravity methods ; 04. Solid Earth::04.03. Geodesy::04.03.05. Gravity variations ; 04. Solid Earth::04.03. Geodesy::04.03.06. Measurements and monitoring ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: report
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  • 10
    Publication Date: 2017-04-04
    Description: As well known, measurements of the time-space changes of the gravity field are a powerful approach to detect the masses change/redistribution in the underground, such as those at volcanoes. The most common approach to detect gravity precursory signals is the use of repeated relative measurements at benchmarks on networks. This is very good, but has some and significant limits: 1) the networks must be linked to a reference station stable over long time and if possible external to the active area. This is quite simply for land volcanoes, but is generally difficult for volcanoes on islands, particularly when far from the terra firma; 2) to reach high precision, measurements require special operative procedure implying long time surveys; 3) relative gravity changes can be affected over the long-time by changes of instrumental sensitivity and loss of vacuum in the air-tight sealing system, therefore the instruments must be subject to continuous check. Measurements on network have the advantage to permit to define the position and the geometry of the masses change/redistribution, even if they suffer from the lack of information about the rate and/or quick changes, since variations are assumed linearly changing over the time between two consecutive surveys, usually spaced out some months or years. This is a fundamental information in the prediction of the volcanic activity changes and/or of volcanic eruptions and leads to conclude that measurements on networks cannot be excluded from a monitoring program, but moving toward absolute methodologies is advisable. Nowadays, and since some years, this is possible due to the commercially availability of a portable field absolute gravimeter (Micro-g_LaCoste A10), which we acquired at the end of 2014. The main advantages of the absolute measurements on networks are: i) they are independent from any reference and the field operation are faster and easier, permitting much frequent measurements and reducing the lack of information between two consecutive surveys; ii) they are directly linked to standards of time and length therefore fairly independent from instrumental references and drift, avoiding loss of long-term information; iii) the measured value can be used without loop reductions, post processing and benchmark links. This can be translated into large advantages, such as saving of human resources, survey’s time and costs. Before to start field surveys, we carried out several measurements to test the performances of the instrument and mainly to verify the repeatability of the measured value. The test was performed at the Old Building of the Osservatorio Vesuviano, on Mount Vesuvio, that is a very low noised and good logistic site; it is one of the absolute stations installed in 80’s in the Neapolitan area which value has been measured several time till 2010. In June 2015, starting from Campi Flegrei, we set the first absolute gravity networks on the Neapolitan volcanoes, formed by stations coinciding or close to the benchmarks of the already existing relative networks. Here we present and discuss the data collected during the test and the field surveys; we also will describe the new absolute networks.
    Description: Unpublished
    Description: Naples (Italy)
    Description: 5V. Sorveglianza vulcanica ed emergenze
    Description: 1IT. Reti di monitoraggio e Osservazioni
    Description: open
    Keywords: Absolute gravimetry ; Neapolitan Volcanoes ; 04. Solid Earth::04.02. Exploration geophysics::04.02.02. Gravity methods ; 04. Solid Earth::04.03. Geodesy::04.03.05. Gravity variations ; 04. Solid Earth::04.03. Geodesy::04.03.06. Measurements and monitoring ; 04. Solid Earth::04.03. Geodesy::04.03.09. Instruments and techniques ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Poster session
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