Multitemporal UAV surveys for landslide mapping and characterization   总被引：1，自引：0，他引：1  

Guglielmo Rossi  Luca Tanteri  Veronica Tofani  Pietro Vannocci  Sandro Moretti  Nicola Casagli 《Landslides》2018,15(5):1045-1052

This paper presents the preliminary results of the IPL project 196 “Development and applications of a multi-sensor drone for geohazards monitoring and mapping.” The objective of the project is to test the applicability of a multi-sensor drone for the mapping and monitoring of different types of geohazards. The Department of Earth Sciences of the University of Florence has developed a new type of drone airframe. Several survey campaigns were performed in the village of Ricasoli, in the Upper Arno river Valley (Tuscany, Italy) with the drone equipped with an optical camera to understand the possibility of this rising technology to map and characterize landslides. The aerial images were combined and analyzed using Structure-from-Motion (SfM) software. The collected data allowed an accurate reconstruction and mapping of the detected landslides. Comparative analysis of the obtained DTMs also permitted the detection of some slope portions being prone to failure and to evaluate the area and volume of the involved mass.  相似文献   

Integration of rainfall thresholds and susceptibility maps in the Emilia Romagna (Italy) regional-scale landslide warning system   总被引：2，自引：2，他引：0  

Samuele Segoni  Daniela Lagomarsino  Riccardo Fanti  Sandro Moretti  Nicola Casagli 《Landslides》2015,12(4):773-785

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Numerical modeling of space-time wave extremes using WAVEWATCH III     

Francesco Barbariol  Jose-Henrique G. M. Alves  Alvise Benetazzo  Filippo Bergamasco  Luciana Bertotti  Sandro Carniel  Luigi Cavaleri  Yung Y. Chao  Arun Chawla  Antonio Ricchi  Mauro Sclavo  Hendrik Tolman 《Ocean Dynamics》2017,67(3-4):535-549

A novel implementation of parameters estimating the space-time wave extremes within the spectral wave model WAVEWATCH III (WW3) is presented. The new output parameters, available in WW3 version 5.16, rely on the theoretical model of Fedele (J Phys Oceanogr 42(9):1601-1615, 2012) extended by Benetazzo et al. (J Phys Oceanogr 45(9):2261–2275, 2015) to estimate the maximum second-order nonlinear crest height over a given space-time region. In order to assess the wave height associated to the maximum crest height and the maximum wave height (generally different in a broad-band stormy sea state), the linear quasi-determinism theory of Boccotti (2000) is considered. The new WW3 implementation is tested by simulating sea states and space-time extremes over the Mediterranean Sea (forced by the wind fields produced by the COSMO-ME atmospheric model). Model simulations are compared to space-time wave maxima observed on March 10th, 2014, in the northern Adriatic Sea (Italy), by a stereo camera system installed on-board the “Acqua Alta” oceanographic tower. Results show that modeled space-time extremes are in general agreement with observations. Differences are mostly ascribed to the accuracy of the wind forcing and, to a lesser extent, to the approximations introduced in the space-time extremes parameterizations. Model estimates are expected to be even more accurate over areas larger than the mean wavelength (for instance, the model grid size).  相似文献   

Seismic response of bridge piers on pile groups for different soil damping models and lumped parameter representations of the foundation     

Francisco González  Luis A. Padrón  Sandro Carbonari  Michele Morici  Juan J. Aznárez  Francesca Dezi  Graziano Leoni 《地震工程与结构动力学》2019,48(3):306-327

This paper presents a wide parametric study aimed at elucidating the influence, on the computed seismic response of bridge piers, of two related aspects of the model: (1) the adoption of the classical hysteretic or the causal Biot's damping models for the soil and (2) the use of two different lumped parameter models of different complexity and accuracy to approximate the impedances of the pile foundation. A total of 2072 cases, including different superstructures, pile foundations, soil deposits, and seismic input signals, are studied. The results are presented so that the influence of the different parameters involved in the analysis can be assessed. From an engineering point of view, both lumped parameter models provide, in general, sufficiently low errors. The choice of the most adequate model for each case will depend not only on the configuration of the structure and the soil-foundation system but also on the assumed soil damping model, whose influence on the computed seismic responses is relevant in many cases. The nonphysical behaviour provided by the classical hysteretic damping model for the soil at zero frequency generates issues in the process of fitting the impedance functions. It is also found that larger deck displacements are predicted by Biot's model due to the higher damping at low frequencies provided by the classical hysteretic damping model.  相似文献   

Investigating the impact of surface wave breaking on modeling the trajectories of drifters in the northern Adriatic Sea during a wind-storm event   总被引：4，自引：0，他引：4  

Sandro Carniel  John C. Warner  Jacopo Chiggiato  Mauro Sclavo 《Ocean Modelling》2009,30(2-3):225-239

An accurate numerical prediction of the oceanic upper layer velocity is a demanding requirement for many applications at sea and is a function of several near-surface processes that need to be incorporated in a numerical model. Among them, we assess the effects of vertical resolution, different vertical mixing parameterization (the so-called Generic Length Scale –GLS– set of k–ε, k–ω, gen, and the Mellor–Yamada), and surface roughness values on turbulent kinetic energy (k) injection from breaking waves.First, we modified the GLS turbulence closure formulation in the Regional Ocean Modeling System (ROMS) to incorporate the surface flux of turbulent kinetic energy due to wave breaking. Then, we applied the model to idealized test cases, exploring the sensitivity to the above mentioned factors. Last, the model was applied to a realistic situation in the Adriatic Sea driven by numerical meteorological forcings and river discharges. In this case, numerical drifters were released during an intense episode of Bora winds that occurred in mid-February 2003, and their trajectories compared to the displacement of satellite-tracked drifters deployed during the ADRIA02-03 sea-truth campaign.Results indicted that the inclusion of the wave breaking process helps improve the accuracy of the numerical simulations, subject to an increase in the typical value of the surface roughness z₀. Specifically, the best performance was obtained using α_CH = 56,000 in the Charnok formula, the wave breaking parameterization activated, k–ε as the turbulence closure model. With these options, the relative error with respect to the average distance of the drifter was about 25% (5.5 km/day). The most sensitive factors in the model were found to be the value of α_CH enhanced with respect to a standard value, followed by the adoption of wave breaking parameterization and the particular turbulence closure model selected.  相似文献   

The Radio and X-ray Mode-Switching Pulsar PSR B0943+10     

Sandro Mereghetti  Michela Rigoselli 《Journal of Astrophysics and Astronomy》2017,38(3):54

Observations obtained in the last years challenged the widespread notion that rotation-powered neutron stars are steady X-ray emitters. Besides a few allegedly rotation-powered neutron stars that showed ‘magnetar-like’ variability, a particularly interesting case is that of PSR B0943+10. Recent observations have shown that this pulsar, well studied in the radio band where it alternates between a bright and a quiescent mode, displays significant X-ray variations, anticorrelated in flux with the radio emission. The study of such synchronous radio/X-ray mode switching opens a new window to investigate the processes responsible for the pulsar radio and high-energy emission. Here we review the main X-ray properties of PSR B0943+10 derived from recent coordinated X-ray and radio observations.  相似文献   

An atmosphere–ocean regional climate model for the Mediterranean area: assessment of a present climate simulation     

Vincenzo Artale  Sandro Calmanti  Adriana Carillo  Alessandro Dell’Aquila  Marine Herrmann  Giovanna Pisacane  Paolo M. Ruti  Gianmaria Sannino  Maria Vittoria Struglia  Filippo Giorgi  Xunqiang Bi  Jeremy S. Pal  Sara Rauscher 《Climate Dynamics》2010,35(5):721-740

We present an atmosphere–ocean regional climate model for the Mediterranean basin, called the PROTHEUS system, composed by the regional climate model RegCM3 as the atmospheric component and by a regional configuration of the MITgcm model as the oceanic component. The model is applied to an area encompassing the Mediterranean Sea and compared to a stand-alone version of its atmospheric component. An assessment of the model performances is done by using available observational datasets. Despite a persistent bias, the PROTHEUS system is able to capture the inter-annual variability of seasonal sea surface temperature (SST) and also the fine scale spatio-temporal evolution of observed SST anomalies, with spatial correlation as high as 0.7 during summer. The close inspection of a 10-day strong wind event during the summer of 2000 proves the capability of the PROTHEUS system to correctly describe the daily evolution of SST under strong air–sea interaction conditions. As a consequence of the model’s skill in reproducing observed SST and wind fields, we expect a reliable estimation of air–sea fluxes. The model skill in reproducing climatological land surface fields is in line with that of state of the art regional climate models.  相似文献   

Future projections of the surface heat and water budgets of the Mediterranean Sea in an ensemble of coupled atmosphere–ocean regional climate models     

C. Dubois  S. Somot  S. Calmanti  A. Carillo  M. Déqué  A. Dell’Aquilla  A. Elizalde  S. Gualdi  D. Jacob  B. L’Hévéder  L. Li  P. Oddo  G. Sannino  E. Scoccimarro  F. Sevault 《Climate Dynamics》2012,39(7-8):1859-1884

Within the CIRCE project “Climate change and Impact Research: the Mediterranean Environment”, an ensemble of high resolution coupled atmosphere–ocean regional climate models (AORCMs) are used to simulate the Mediterranean climate for the period 1950–2050. For the first time, realistic net surface air-sea fluxes are obtained. The sea surface temperature (SST) variability is consistent with the atmospheric forcing above it and oceanic constraints. The surface fluxes respond to external forcing under a warming climate and show an equivalent trend in all models. This study focuses on the present day and on the evolution of the heat and water budget over the Mediterranean Sea under the SRES-A1B scenario. On the contrary to previous studies, the net total heat budget is negative over the present period in all AORCMs and satisfies the heat closure budget controlled by a net positive heat gain at the strait of Gibraltar in the present climate. Under climate change scenario, some models predict a warming of the Mediterranean Sea from the ocean surface (positive net heat flux) in addition to the positive flux at the strait of Gibraltar for the 2021–2050 period. The shortwave and latent flux are increasing and the longwave and sensible fluxes are decreasing compared to the 1961–1990 period due to a reduction of the cloud cover and an increase in greenhouse gases (GHGs) and SSTs over the 2021–2050 period. The AORCMs provide a good estimates of the water budget with a drying of the region during the twenty-first century. For the ensemble mean, he decrease in precipitation and runoff is about 10 and 15% respectively and the increase in evaporation is much weaker, about 2% compared to the 1961–1990 period which confirm results obtained in recent studies. Despite a clear consistency in the trends and results between the models, this study also underlines important differences in the model set-ups, methodology and choices of some physical parameters inducing some difference in the various air-sea fluxes. An evaluation of the uncertainty sources and possible improvement for future generation of AORCMs highlights the importance of the parameterisation of the ocean albedo, rivers and cloud cover.  相似文献   

Lithium speciation in aqueous fluids at high P and T studied by ab initio molecular dynamics and consequences for Li-isotope fractionation between minerals and fluids     

Sandro Jahn  Bernd Wunder 《Geochimica et cosmochimica acta》2009,73(18):2797-6123

Ab initio molecular dynamics simulations are performed to study the speciation changes in lithium bearing aqueous fluids at high temperature (T = 1000 K) and high pressures, P, between about 0.3 and 6.0 GPa. The simulations show a linear increase in Li coordination with fluid density, from 3.2 to about five in the considered pressure range. Towards low densities, associated LiF complexes are becoming increasingly stable, which is quantified by evaluating the dynamic behavior of the respective species. In the high-density region, HF complexes are observed. The differences in speciation may be related to structural changes of the solvent under compression. At a fluid density of 1.2 g/cm³, kinks in the pressure dependences of the oxygen–oxygen nearest neighbor distance and the oxygen–oxygen coordination are observed, which indicates a change in compaction mechanism. Assuming that the Li coordination difference between crystal and fluid is a major determinant for the isotopic fractionation between minerals and fluids, we expect only a small pressure dependence of the Li isotopic fractionation between Li bearing fluids and minerals. Our simulation results are consistent with experimental data that show reverse fractionation of ⁷Li between fluid and mineral, when Li is in tetrahedral instead of octahedral coordination in the crystal.  相似文献   

The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars     

Sandro Mereghetti 《Astronomy and Astrophysics Review》2008,15(4):225-287

Two classes of X-ray pulsars, the anomalous X-ray pulsars and the soft gamma-ray repeaters, have been recognized in the last decade as the most promising candidates for being magnetars: isolated neutron stars powered by magnetic energy. I review the observational properties of these objects, focussing on the most recent results, and their interpretation in the magnetar model. Alternative explanations, in particular those based on accretion from residual disks, are also considered. The possible relations between these sources and other classes of neutron stars and astrophysical objects are also discussed.  相似文献