Search results for "design [electronics]"

showing 10 items of 505 documents

Il Rilievo MMS di tracciati autostradali

2009

Già da alcuni anni alcuni autori hanno messo in risalto come, anche in ambito autostradale, la geometria d’asse intesa come il complesso plano-altimetrico degli elementi di tracciato, eserciti un ruolo non marginale sulla condotta di guida dell’utente. Grazie alle metodologie di verifica della coerenza della linea d’asse di tracciato (Design Consistency), si accerta o meno che esista un’armonica correlazione tra parametri geometrici significativi e la velocità, di progetto od operativa, del tronco considerato. L’espressione grafica di tale correlazione è il cosiddetto diagramma delle velocità, dalla cui analisi, secondo criteri invero peculiari di infrastrutture viarie non autostradali, è p…

GPS velocità operativaDesign ConsistencySettore ICAR/04 - Strade Ferrovie Ed AeroportiSettore ICAR/06 - Topografia E Cartografia
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Simulation as a game design tool

2009

In this paper we suggest using gameplay simulations on a logical event level as a design tool already in the early stages of the development process. The approach is centred on abstracting all unnecessary details of the gameplay to produce a highly simplified model of the game system. Compared to other kinds of intermediate design representations, such as sketches and prototypes, the simulations can reveal problems and opportunities in the longer term dynamics of possible gameplay. As an example we describe an implementation of a simulation model for the game Tower Bloxx using a simulation software package called DisCo.

Game testingGame designGame programmingGame design documentHuman–computer interactionComputer scienceDesign toolComputingMilieux_PERSONALCOMPUTINGGame development toolcomputer.software_genrecomputerFirst playable demoSimulation softwareProceedings of the International Conference on Advances in Computer Entertainment Technology
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Government Architecture: Concepts, Use and Impact

2013

Part 3: Service Design and Improvement; International audience; Government architecture (GA) is a relatively young discipline in which concepts are slowly emerging. Often terms and concepts are used in various ways and there is no uniform agreement on these concepts. Further, the relationship between GA, benefits and public value creation is unclear. In this paper we unravel and define GA concepts that are often used by governments. Although GA is used in different ways there are common concepts. GA practice in two different countries, the Netherlands and Norway, indicates that although the Netherlands clearly has more experience with GA than Norway, both countries employ similar concepts. …

GovernmentKnowledge managementManagement sciencebusiness.industryEnterprise architecture[SHS.INFO]Humanities and Social Sciences/Library and information sciencesdesigngovernmentConceptual model (computer science)Enterprise architecturegovernment architecturedesign science governancemedicine[INFO]Computer Science [cs]BusinessPublic valuepublic valuemedicine.symptomArchitectureConfusion
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Assessing Effects of eGovernment Initiatives Based on a Public Value Framework

2012

Published version of a chapter in the book: Electronic Government. Also available from the publisher at: http://dx.doi.org/10.1007/978-3-642-33489-4_21 Assessing effects of eGovernment initiatives is considered an important but challenging endeavor. Assessments are, among other things, important to justify e-government investments. They are challenging because they are complex, often based on locally defined indicators, many times over-emphasizing financial effects, imprecise, faced with a number of contingencies and very seldom validated. Consequently, effect assessments can be seen as imprecise and difficult to compare across different initiatives. This paper addresses some of the challen…

GovernmentKnowledge managementaction design researchE-Governmentbusiness.industryeGEP measurement framework[SHS.INFO]Humanities and Social Sciences/Library and information sciencesDesign elements and principlesperformance indicatorsAction (philosophy)Risk analysis (engineering)Design studyAgency (sociology)[INFO]Computer Science [cs]Public valuePerformance indicatorVDP::Social science: 200::Library and information science: 320::Information and communication systems: 321public valuebusinesse-governmentinterpretive evaluation of IS
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Multi-objective optimisations for a superscalar architecture with selective value prediction

2012

This work extends an earlier manual design space ex ploration of our developed Selective Load Value Pre diction based superscalar architecture to the L2 unified cache. A fter that we perform an automatic design space expl oration using a special developed software tool by varying several architectural parameters. Our goal is to find optim al configurations in terms of CPI (Cycles per Instruction) and energy consumption. By varying 19 architectural parameter s, as we proposed, the design space is over 2.5 millions of billions configurations which obviously means that only heuristic search can be considered. Therefore, we propose dif ferent methods of automatic design space exploratio n based…

Hardware and ArchitectureComputer scienceCycles per instructionSuperscalarValue (computer science)Parallel computingCacheEnergy consumptionElectrical and Electronic EngineeringDesign spaceSoftwareSpace explorationSign (mathematics)IET Computers & Digital Techniques
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A Comparison of Multi-objective Algorithms for the Automatic Design Space Exploration of a Superscalar System

2013

In today’s computer architectures the design spaces are huge, thus making it very difficult to find optimal configurations. One way to cope with this problem is to use Automatic Design Space Exploration (ADSE) techniques. We developed the Framework for Automatic Design Space Exploration (FADSE) which is focused on microarchitectural optimizations. This framework includes several state-of-the art heuristic algorithms.

Heuristic (computer science)Design space explorationComputer scienceSuperscalarParticle swarm optimizationAlgorithm
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Spectral analysis of the low-mass X-ray pulsar 4U 1822-371: Reflection component in a high-inclination system

2021

Context. The X-ray source 4U 1822-371 is an eclipsing low-mass X-ray binary and X-ray pulsar, hosting a NS that shows periodic pulsations in the X-ray band with a period of 0.59 s. The inclination angle of the system is so high (80–85°) that in principle, it should be hard to observe both the direct thermal emission of the central object and the reflection component of the spectrum because they are hidden by the outer edge of the accretion disc. Despite the number of studies carried out on this source, many aspects such as the geometry of the system, its luminosity, and its spectral features are still debated. Aims. Assuming that the source accretes at the Eddington limit, the analysis perf…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysics01 natural sciencesaccretion accretion disks stars: neutron stars: individual: 4U 1822-371 X-rays: binaries X-rays: general eclipsesLuminositysymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary Science0103 physical sciencesEddington luminosityReflection (physics)symbolsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsX-ray pulsarEclipse
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Magneto-elastic oscillations of neutron stars: exploring different magnetic field configurations

2012

We study magneto-elastic oscillations of highly magnetized neutron stars (magnetars) which have been proposed as an explanation for the quasi-periodic oscillations (QPOs) appearing in the decaying tail of the giant flares of soft gamma-ray repeaters (SGRs). We extend previous studies by investigating various magnetic field configurations, computing the Alfv��n spectrum in each case and performing magneto-elastic simulations for a selected number of models. By identifying the observed frequencies of 28 Hz (SGR 1900+14) and 30 Hz (SGR 1806-20) with the fundamental Alfv��n QPOs, we estimate the required surface magnetic field strength. For the magnetic field configurations investigated (dipole…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsField lineAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsMagnetar01 natural sciencesAsteroseismologyGeneral Relativity and Quantum CosmologyMagnetic fieldDipoleNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamics010306 general physicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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Radio emission of SN1993J. The complete picture: II. Simultaneous fit of expansion and radio light curves

2010

We report on a simultaneous modelling of the expansion and radio light curves of SN1993J. We have developed a simulation code capable of generating synthetic expansion and radio light curves of supernovae by taking into consideration the evolution of the expanding shock, magnetic fields, and relativistic electrons, as well as the finite sensitivity of the interferometric arrays used in the observations. Our software successfully fits all the available radio data of SN 1993J with an standard emission model for supernovae extended with some physical considerations, as an evolution in the opacity of the ejecta material, a radial drop of the magnetic fields inside the radiating region, and a ch…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOpacityAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveGalaxyMagnetic fieldParticle accelerationSupernovaSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsEjectaAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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Testing Rate Dependent corrections on timing mode EPIC-pn spectra of the accreting Neutron Star GX 13+1

2014

When the EPIC-pn instrument on board XMM-Newton is operated in Timing mode, high count rates (>100 cts/s) of bright sources may affect the calibration of the energy scale, resulting in a modification of the real spectral shape. The corrections related to this effect are then strongly important in the study of the spectral properties. Tests of these calibrations are more suitable in sources which spectra are characterised by a large number of discrete features. Therefore, in this work, we carried out a spectral analysis of the accreting Neutron Star GX 13+1, which is a dipping source with several narrow absorption lines and a broad emission line in its spectrum. We tested two different co…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion discs line: identification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1)Spectral shape analysisAccretion (meteorology)Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesSpectral lineNeutron starAmplitudeidentification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1) [accretion accretion discs line]Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Emission spectrumAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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