The role of friction in the seismic risk mitigation of freestanding art objects     

Michelina Monaco  Mariateresa Guadagnuolo  Antonio Gesualdo 《Natural Hazards》2014,73(2):389-402

The problem of reducing the seismic risk for art objects, that are the objects generally contained within Museums, is of great interest. The first studies were performed in Japan and were successively organized in a general framework by a research program performed at Southern California University and sponsored by the Getty Museum at Malibu, California. In these papers and in the following Italian studies, the theoretical models for the problem concerning vases and statues are based on the dynamic behavior of rigid blocks and have been deeply developed. Unfortunately, because of the great lack of experimental data, determinant parameters for the problem characterization (like the friction between two superimposed blocks or between the art object and the support plane) are often assumed without reference to real values derived from laboratory tests. This paper presents the results of a research program containing the experimental determination of the friction coefficient between the art object and the support (by means of a testing apparatus on purpose realized) together with dynamic tests performed on simple-shaped objects made of different materials. The dynamic tests were performed using an unidirectional shaking table and different supporting surfaces, so that the influence of different friction coefficients has been analyzed.  相似文献   

Effects of climate change on bioclimatic indices in vineyards along Lake Neuchatel,Switzerland     

Comte  Valentin  Schneider  Léonard  Calanca  Pierluigi  Rebetez  Martine 《Theoretical and Applied Climatology》2022,147(1-2):423-436

Theoretical and Applied Climatology - In this study, we investigated the consequences of climate change on bioclimatic indices in vineyards along the edge of Lake Neuchatel in Switzerland. Like in...  相似文献   

High-order expansion of the solution of preliminary orbit determination problem     

Roberto Armellin  Pierluigi Di Lizia  Michele Lavagna 《Celestial Mechanics and Dynamical Astronomy》2012,112(3):331-352

A method for high-order treatment of uncertainties in preliminary orbit determination is presented. The observations consist in three couples of topocentric right ascensions and declinations at three observation epochs. The goal of preliminary orbit determination is to compute a trajectory that fits with the observations in two-body dynamics. The uncertainties of the observations are usually mapped to the phase space only when additional observations are available and a least squares fitting problem is set up. A method based on Taylor differential algebra for the analytical treatment of observation uncertainties is implemented. Taylor differential algebra allows for the efficient computation of the arbitrary order Taylor expansion of a sufficiently continuous multivariate function. This enables the mapping of the uncertainties from the observation space to the phase space as high-order multivariate Taylor polynomials. These maps can then be propagated forward in time to predict the observable set at successive epochs. This method can be suitably used to recover newly discovered objects when a scarce number of measurements is available. Simulated topocentric observations of asteroids on realistic orbits are used to assess the performances of the method.  相似文献   

Site effects in the Aterno River Valley (L’Aquila,Italy): comparison between empirical and 2D numerical modelling starting from April 6th 2009 Mw 6.3 earthquake     

Iolanda Gaudiosi  Del Monaco Francesco  Milana Giuliano  Tallini Marco 《Bulletin of Earthquake Engineering》2014,12(2):697-716

In this paper, we focused our attention on a cross-section of the Aterno River Valley where a good quality geological and geophysical dataset allowed to reconstruct accurately the geometry and the Vs profiles along all the plane of the section. Its trace is deliberately aligned close to the strong motion stations that recorded the Mw 6.3 (April 6th 2009) L’Aquila earthquake. We analysed strong and weak motion data available at these latter stations as well as at one of the temporary stations installed during the Microzonation activities and located on outcropping bedrock, in proximity of the cross-section. We used the H/V technique to select a reliable reference site and once we found it, we applied the SSR technique to compute amplification functions in correspondence of two strong motion stations. In turn, for both sites we performed a site response numerical modelling with two different 2D codes and we compared simulated versus experimental transfer functions. We found that the cross-section is well constrained based on the very reasonable agreement between results of numerical modelling and earthquake data analysis. We pointed out also a strong amplification of the deposit at the centre of the valley due to the constructive interference of S and surface waves, not predictable by means of 1D numerical modelling. We also compared the H/V as well as the SSR obtained from strong motion data with the ones computed from weak motion finding evidences of non-linearity in soil behaviour.  相似文献   

Active faulting and continental slope instability in the Gulf of Patti (Tyrrhenian side of NE Sicily,Italy): a field,marine and seismological joint analysis     

F. Cultrera  G. Barreca  P. Burrato  L. Ferranti  C. Monaco  S. Passaro  F. Pepe  L. Scarfì 《Natural Hazards》2017,86(2):253-272

The Gulf of Patti and its onshore sector represent one of the most seismically active regions of the Italian Peninsula. Over the period 1984–2014, about 1800 earthquakes with small-to-moderate magnitude and a maximum hypocentral depth of 40 km occurred in this area. Historical catalogues reveal that the same area was affected by several strong earthquakes such as the Mw = 6.1 event in April 1978 and the Mw = 6.2 one in March 1786 which have caused severe damages in the surrounding localities. The main seismotectonic feature affecting this area is represented by a NNW–SSE trending right-lateral strike-slip fault system called “Aeolian–Tindari–Letojanni” (ATLFS) which has been interpreted as a lithospheric transfer zone extending from the Aeolian Islands to the Ionian coast of Sicily. Although the large-scale role of the ATLFS is widely accepted, several issues about its structural architecture (i.e. distribution, attitude and slip of fault segments) and the active deformation pattern are poorly constrained, particularly in the offshore. An integrated analysis of field structural geology with marine geophysical and seismological data has allowed to better understand the structural fabric of the ATLFS which, in the study area, is expressed by two major NW–SE trending, en-echelon arranged fault segments. Minor NNE–SSW oriented extensional structures mainly occur in the overlap region between major faults, forming a dilatational stepover. Most faults display evidence of active deformation and appear to control the main morphobathymetric features. This aspect, together with diffused continental slope instability, must be considered for the revaluation of the seismic and geomorphological hazard of this sector of southern Tyrrhenian Sea.  相似文献   

Holocene relative sea-level changes and vertical movements along the Italian and Istrian coastlines   总被引：2，自引：0，他引：2  

F. Antonioli  L. Ferranti  A. Fontana  A. Amorosi  A. Bondesan  C. Braitenberg  A. Dutton  G. Fontolan  S. Furlani  K. Lambeck  G. Mastronuzzi  C. Monaco  G. Spada  P. Stocchi 《Quaternary International》2009,206(1-2):102

Published and new data exist for relative sea-level change for 105 locations (127 samples) during the late Holocene, along the Italian (and Istrian) coasts. These data, compared with predictions (derived from two different models associated with the last glacial cycle) allowed the calculation of the tectonic vertical movements. They are based on precise measures of geomorphological and archaeological markers between 0.4 and 12.6 ka cal. BP, sampled at elevations between +7 and −51 m. In order to decipher the broad pattern of Holocene tectonic vertical movements along the Italian coastline, these data were compared with predicted sea-level curves using the most recent models published for the Mediterranean sea. Tectonic rates varied from −4.85 mm/a, in a core at Sybaris, to 5 mm/a, in the volcanic areas of Pozzuoli and Pantelleria. New MIS 5.5 (125 ka) data, mostly from the Venetian plain, are reported. In particular the depth of the base of MIS 5.5 paralic deposits found in four cores near Venezia provides a mean subsidence of 0.62 mm/a. New, precise mass spectrometer U-Th analyses on Cladocora layers from the bottom of a long core (named ENEA), indicate older ages (195.7 ± 1.6 and 161.2 ± 1.2 ka, respectively), relative to the published MIS 5.5 ages, which were based on alpha-counting U-Th data.Instrumental data obtained from tide gauges and repeated levelling measurements from the NE Adriatic and Sicily are also considered. These methods have one great advantage with respect to continuous GPS measurements and the satellite altimetric observations, in that a much greater time span is available. Although the altimetric measurements are available for 16 years, and the GPS for less than a decade, repeated levelling lines cover up to 50 years and tide gauge observations in some cases to 100 years or more. The greater time span allows for more stable differential rate estimates. The repeated levelling shows that the plain east of Mestre is subsiding (to −4 mm/a). The Messina tidal gauge demonstrates a total coseismic and post-seismic subsidence of 77 cm associated with the event of 1908, the post-seismic phase lasting for at least 13 years. The Reggio Calabria tidal station points to an uplift of this station relative to Palermo in the order of 1–2 mm/a.  相似文献   

Boundary layer characteristics and turbulent exchange mechanisms in highly complex terrain   总被引：2，自引：0，他引：2  

Mathias W. Rotach  Marco Andretta  Pierluigi Calanca  Andreas P. Weigel  Alexandra Weiss 《Acta Geophysica》2008,56(1):194-219

The Mesoscale Alpine Programme’s Riviera project investigated the turbulence structure and related exchange processes in an Alpine valley by combining a detailed experimental campaign with high-resolution numerical modelling. The present contribution reviews published material on the Riviera Valley’s boundary layer structure and discusses new material on the near-surface turbulence structure. The general conclusion of the project is that despite the large spatial variability of turbulence characteristics and the crucial influence of topography at all scales, the physical processes can accurately be understood and modelled. Nevertheless, many of the “text book characteristics” like the interaction between the valley and slope wind systems or the erosion of the nocturnal valley inversion need reconsideration, at least for small non-ideal valleys like the Riviera Valley. The project has identified new areas of research such as post-processing methods for turbulence variables in complex terrain and new approaches for the surface energy balance when advection is non-negligible. The exchange of moisture and heat between the valley atmosphere and the free troposphere is dominated by local “secondary” circulations due to the curvature of the valley axis. Because many curved valleys exist, and operational models still have rather poor resolution, parameterization of these processes may be required.  相似文献   

A simulation experiment for optimal design hyetograph selection   总被引：1，自引：0，他引：1  

Lorenzo Alfieri  Francesco Laio  Pierluigi Claps 《水文研究》2008,22(6):813-820

The aim of this work is to assess the accuracy of literature design hyetographs for the evaluation of peak discharges during flood events. Five design hyetographs are examined in a set of simulations, based upon the following steps: (i) an ideal river basin is defined, characterized by a Beta distribution shaped unit hydrograph (UH); (ii) 1000 years of synthetic rainfall are artificially generated; (iii) a discharge time‐series is obtained from the convolution of the rainfall time‐series and the UH, and the reference T‐years flood is computed from this series; (iv) for the same return period T, the parameters of the intensity–duration–frequency (IDF) curve are estimated from the 1000 years of synthetic rainfall; (v) five design hyetographs are determined from the IDF curves and are convolved with the discrete UH to find the corresponding design hydrographs; (vi) the hydrograph peaks are compared with the reference T‐years flood and the advantages and drawbacks of each of the five approaches are evaluated. The rainfall and UH parameters are varied, and the whole procedure is repeated to assess the sensitivity of results to the system configuration. We found that all design hyetographs produce flood peak estimates that are consistently biased in most of the climatic and hydrologic conditions considered. In particular, significant underestimation of the design flood results from the adoption of any rectangular hyetograph used in the context of the rational formula. In contrast, the Chicago hyetograph tends to overestimate peak flows. In two cases it is sufficient to multiply the result by a constant scaling factor to obtain robust and nearly unbiased estimates of the design floods. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

Mass function of dormant black holes and the evolution of active galactic nuclei     

Paolo Salucci  Ewa Szuszkiewicz  Pierluigi Monaco  Luigi Danese 《Monthly notices of the Royal Astronomical Society》1999,307(3):637-644

Under the assumption that accretion on to massive black holes (BHs) powers active galactic nuclei (AGNs), the mass function (MF) of the BHs responsible for their past activity is estimated. For this, we take into account not only the activity related to the optically selected AGNs, but also that required to produce the hard X-ray background (HXRB). The MF of the massive dark objects (MDOs) in nearby quiescent galaxies is computed by means of the most recent results on their demography. The two mass functions match well under the assumption that the activity is concentrated in a single significant burst with λ L L _Edd being a weakly increasing function of luminosity. This behaviour may be indicative of some level of recurrence and/or of accretion rates insufficient to maintain the Eddington rates in low-luminosity/low-redshift objects. Our results support the scenario in which the early phase of intense nuclear activity occurred mainly in early-type galaxies (E/S0) during the relatively short period in which they still had an abundant interstellar medium. Only recently, with the decline of the quasi-stellar object (QSO) luminosities, did the activity in late‐type galaxies (Sa/Sab) become statistically significant.  相似文献   

Behaviour of metallic and radioactive elements in lagoonal sediments: the example of the Canet-St Nazaire Pond (Mediterranean coast)     

M. Bernat  G. Cauwet  B. Chassefiere  D. Faguet  F. Gadel  A. Monaco  M. Ouakad  Y. Thommeret 《Estuarine, Coastal and Shelf Science》1984,18(5):557-570

The behaviour of Ca, Mg, Na, K, Fe, Mn, Zn and radionuclides (U, Th, Pb, Ra) was studied in water, suspensions and sediments of an euxinic lagoonal environment of the French Mediterranean coast. The dynamic of these elements at the sediment-water interface is considered particularly in relation to the redox conditions, the nature of inorganic and organic supports and the sedimentation rate.  相似文献