Probabilistic Seismic Hazard Curves and Maps for Italian Slopes

The seismic performance of an earth slope is commonly evaluated through the permanent displacements developed at the end of an earthquake. In this paper a probabilistic approach is adopted to assess the displacement of the slope for a given hazard level using an updated database of ground motions rec-orded during the earthquakes occurred in Italy. The results are presented in terms of hazard curves, showing the annual rate of exceedance of permanent slope displacement evaluated using ground motion data provided by a standard probabilistic hazard analysis and a series of semi-empirical relationships linking the permanent displacements of slopes to one or more ground motion parame-ters. The probabilistic approach permits to take into account synthetically the characteristics of the slope through the yield seismic coefficient, the aleatory variability of the ground motions and the different subsoil classes of the record-ing stations. Finally, the procedure has been extended on a regional scale to produce seismic landslide hazard maps for Irpinia, one of the most seismically active regions in Italy. Seismic landslide hazard maps are very attractive for practitioners and government agencies for a screening level analysis to identify, monitor and minimise damages in zones that are potentially susceptible to earthquake-induced slope instability

Influence of the displacement predictive relationships on the probabilistic seismic analysis of slopes

Seismically induced landslides can often cause severe human and economic losses. Therefore, it is worth assessing the seismic performance of slopes through a reliable quantification of the permanent displacements induced by seismic loading. This paper presents a new semiempirical relationship linking the permanent earthquake-induced displacements of slopes to one or two synthetic ground motion parameters developed considering the Italian seismicity, and a comparison with existing simplified displacement models is illustrated. Once combined with a fully probabilistic approach, these relationships provide a useful tool for practicing engineers and national agencies for a preliminary estimate of the seismic performance of a slope. In this perspective, the predictive capability of different semiempirical relationships is analyzed with reference to the permanent displacements evaluated for the Italian seismicity assimilating the slope to a rigid body and adopting the Newmark integration approach. The consequences of the adoption of these relationships on the results of the probabilistic approach are illustrated in terms of displacement hazard curves and hazard maps for different slope scenarios

Evaluation of Seismic Landslide Hazard Based on a New Displacement Semi-empirical Relationship

This paper presents a new semi-empirical relationship that links the permanent earthquake-induced displacements of slopes to the synthetic ground motion parameter PGA or to the couple PGA and PGV. The displacements are evaluated under the hypothesis of a rigid sliding block performing Newmark’s integrations for all the acceleration time histories of the updated Italian seismic database. The relationship reproduces well the displacements for any values of yield seismic coefficient in the whole range of peak ground acceleration. The two parameters expression is more reliable for the study of Italian slopes under seismic loading than that based on the single PGA parameter as characterised by a lower standard deviation. The proposed relationship is also combined with a fully probabilistic approach to produce displacement hazard curves and hazard maps for different sites and regions of Italy that represent a useful tool for practicing engineers and national agencies for a preliminary estimate of the seismic performance of a slope

Energy-Efficiency Evaluation of FPGAs for Floating-Point Intensive Workloads

In this work we describe a method to measure the computing performance and energy-efficiency to be expected of an FPGA device. The motivation of this work is given by their possible usage as accelerators in the context of floating-point intensive HPC workloads. In fact, FPGA devices in the past were not considered an efficient option to address floating-point intensive computations, but more recently, with the advent of dedicated DSP units and the increased amount of resources in each chip, the interest towards these devices raised. Another obstacle to a wide adoption of FPGAs in the HPC field has been the low level hardware knowledge commonly required to program them, using Hardware Description Languages (HDLs). Also this issue has been recently mitigated by the introduction of higher level programming framework, adopting so called High Level Synthesis approaches, reducing the development time and shortening the gap between the skills required to program FPGAs wrt the skills commonly owned by HPC software developers. In this work we apply the proposed method to estimate the maximum floating-point performance and energy-efficiency of the FPGA embedded in a Xilinx Zynq Ultrascale+ MPSoC hosted on a Trenz board

Porting a Lattice Boltzmann Simulation to FPGAs Using OmpSs

Reconfigurable computing, exploiting Field Programmable Gate Arrays (FPGA), has become of great interest for both academia and industry research thanks to the possibility to greatly accelerate a variety of applications. The interest has been further boosted by recent developments of FPGA programming frameworks which allows to design applications at a higher-level of abstraction, for example using directive based approaches. In this work we describe our first experiences in porting to FPGAs an HPC application, used to simulate Rayleigh-Taylor instability of fluids with different density and temperature using Lattice Boltzmann Methods. This activity is done in the context of the FET HPC H2020 EuroEXA project which is developing an energyefficient HPC system, at exa-scale level, based on Arm processors and FPGAs. In this work we use the OmpSs directive based programming model, one of the models available within the EuroEXA project. OmpSs is developed by the Barcelona Supercomputing Center (BSC) and allows to target FPGA devices as accelerators, but also commodity CPUs and GPUs, enabling code portability across different architectures. In particular, we describe the initial porting of this application, evaluating the programming efforts required, and assessing the preliminary performances on a Trenz development board hosting a Xilinx Zynq UltraScale+ MPSoC embedding a 16nm FinFET+ programmable logic and a multi-core Arm CPU

Dark Matter Halos within Clusters

We examine the properties of dark matter halos within a rich galaxy cluster using a high resolution simulation that captures the cosmological context of a cold dark matter universe. The mass and force resolution permit the resolution of 150 halos with circular velocities larger than 80 kms within the cluster's virial radius of 2 Mpc. This enables an unprecedented study of the statistical properties of a large sample of dark matter halos evolving in a dense environment. The cumulative fraction of mass attached to these halos varies from 0% at 200 kpc, to 13% at the virial radius. Even at this resolution the overmerging problem persists; halos that pass within 200 kpc of the cluster center are tidally disrupted. Additional substructure is lost at earlier epochs within the massive progenitor halos. The median ratio of apocentric to pericentric radii is 6:1; the orbital distribution is close to isotropic, circular orbits are rare, radial orbits are common. The orbits of halos are unbiased with respect to both position within the cluster and with the orbits of the smooth dark matter background and no velocity bias is detected. The tidal radii of surviving halos are generally well-fit using the simple analytic prediction applied to their orbital pericenters. Halos within clusters have higher concentrations than those in the field. Within the cluster, halo density profiles can be modified by tidal forces and individual encounters with other halos that cause significant mass loss - ``galaxy harassment''. Mergers between halos do not occur inside the clusters virial radius.Comment: LaTeX MN style, 20 pages, 30 figures included + 1 colour plo

A 65-nm CMOS Temperature-Compensated Mobility-Based Frequency reference for wireless sensor networks

For the first time, a temperature-compensated CMOS frequency reference based on the electron mobility in a MOS transistor is presented. Over the temperature range from -55°C to 125 °C, its frequency spread is less than ±0.5% after a two-point trim and less than ±2.7% after a one-point trim. These results make it suitable for use in Wireless Sensor Network nodes. Fabricated in a baseline 65-nm CMOS process, the 150 kHz frequency reference occupies 0.2 mm2 and draws 42.6 μA from a 1.2-V supply at room temperature.\ud \u