Search results for " Hydrodynamic"

showing 10 items of 121 documents

Overionization in X-ray spectra: a new paradigm for Mixed-Morphology SNRs

2011

Mixed-morphology SNRs are characterized by a shell-like radio emission, a centrally peaked X-ray morphology, and by interaction with molecular clouds. Many models have been proposed to explain these peculiar remnants, but their physical origin is still unclear. The recent discovery of over-ionized (i. e. recombining) ejecta in 3 mixed-morphology SNRs has dramatically challenged all the previous models and opened up new, unexpected scenarios. I review the main properties of these remnants and their peculiar X-ray spectral properties. I also discuss the hydrodynamic model developed to explain the presence of over-ionized ejecta in W49B and present a list of open issues that still need to be c…

High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaMixed-morphology SNRs are characterized by a shell-like radio emission a centrally peaked X-ray morphology and by interaction with molecular clouds. Many models have been proposed to explain these peculiar remnants but their physical origin is still unclear. The recent discovery of overionized (i. e. recombining) ejecta in 3 mixed-morphology SNRs has dramatically challenged all the previous models and opened up new unexpected scenarios. I review the main properties of these remnants and their peculiar X-ray spectral properties. I also discuss the hydrodynamic model developed to explain the presence of overionized ejecta in W49B and present a list of open issues that still need to be clarified.Astrophysics::Galaxy Astrophysics
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On the observability of T Tauri accretion shocks in the X-ray band

2010

Context. High resolution X-ray observations of classical T Tauri stars (CTTSs) show a soft X-ray excess due to high density plasma (n_e=10^11-10^13 cm^-3). This emission has been attributed to shock-heated accreting material impacting onto the stellar surface. Aims. We investigate the observability of the shock-heated accreting material in the X-ray band as a function of the accretion stream properties (velocity, density, and metal abundance) in the case of plasma-beta<<1 in the post-shock zone. Methods. We use a 1-D hydrodynamic model describing the impact of an accretion stream onto the chromosphere, including the effects of radiative cooling, gravity and thermal conduction. We expl…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRadiative coolingAstrophysics::High Energy Astrophysical Phenomenaaccretion accretion disks hydrodynamics shock waves stars: pre-main sequence X-rays: starsFOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaAstrophysicsThermal conductionAccretion (astrophysics)T Tauri starSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceThermalAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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The jets and disc of SS 433 at super-Eddington luminosities

2009

We examine the jets and the disc of SS 433 at super-Eddington luminosities with 600 times Eddington critical accretion rate by time-dependent two-dimensional radiation hydrodynamical calculations, assuming alpha-model for the viscosity. One-dimensional supercritical accretion disc models with mass loss or advection are used as the initial configurations of the disc. As a result, from the initial advective disc models with alpha =0.001 and 0.1, we obtain the total luminosities 2.5x10^{40} and 2.0x10^{40} erg/s. The total mass-outflow rates are 4x10^{-5} and 10^{-4} solar-mass/yr and the rates of the relativistic axial outflows in a small half opening angle of 1 degree are about 10^{-6} solar…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion discs black hole physics hydrodynamics radiation mechanisms: thermal X-rays: individual: SS 433Jet (fluid)Plane (geometry)AdvectionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadiationLuminosityViscositySettore FIS/05 - Astronomia E AstrofisicaAmplitudeSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsOutflowAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Periodic massloss from viscous accretion flows around black holes

2014

We investigate the behaviour of low angular momentum viscous accretion flows around black holes using Smooth Particle Hydrodynamics (SPH) method. Earlier, it has been observed that in a significant part of the energy and angular momentum parameter space, rotating transonic accretion flow undergoes shock transition before entering in to the black hole and a part of the post-shock matter is ejected as bipolar outflows, which are supposed to be the precursor of relativistic jets. In this work, we simulate accretion flows having injection parameters from the inviscid shock parameter space, and study the response of viscosity on them. With the increase of viscosity, shock becomes time dependent …

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsAngular momentumShock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsMechanicsAccretion (astrophysics)Physics::Fluid DynamicsSmoothed-particle hydrodynamicsViscosityAstrophysical jetSpace and Planetary ScienceInviscid flowAstrophysics::Solar and Stellar AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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Modélisation numérique d’impacts à hautes vitesses par la méthode sans maillage Smoothed Particles Hydrodynamics. Application aux micro-impacts dans …

2021

Investigations on the ballistic behaviours of soft tissue materials are significant research in a medical and pharmaceutical framework. They mainly focus on particles penetrating or traveling into the soft materials. For instance, in the needle-free drug delivery, the micro-scale particles as drug powders are injected into skin with high velocity, and several factors should be considered such as the particle diameters, trajectories, and momentum or velocities of projectile in this process. There have been investigated by some experiments, but there is still no study from the numerical insights.The numerical methods are suitable to study these kinds of processes. Although grid-based methods …

High-Velocity impact[SPI.OTHER]Engineering Sciences [physics]/OtherMicro-Impacts[SPI.OTHER] Engineering Sciences [physics]/OtherTissus mousImpact à hautes vitesseSoft tissuesSmoothed Particles HydrodynamicsPénétrations à micro-Échelle
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Wind- and tide-induced currents in the Stagnone Lagoon (Sicily)

2011

The hydrodynamic circulation is analyzed in the coastal lagoon of Stagnone di Marsala, a natural reserve located in the north-western part of Sicily, using both experimental measurements and numerical simulations. Field measurements of velocities and water levels, carried out using an ultrasound sensor (3D), are used to validate the numerical model. A 3D finite-volume model is used to solve the Reynolds-averaged momentum and mass balance differential equations on a curvilinear structured grid, employing the k– $${\varepsilon}$$ turbulence model for the Reynolds stresses. The numerical analysis allows to identify the relative contribution of the forces affecting the hydrodynamic circulation …

HydrogeologySeicheMeteorologyTurbulenceFlow (psychology)Wind stressReynolds stressMechanicsSettore ICAR/01 - IdraulicaWaves and shallow waterCirculation (fluid dynamics)Coastal lagoon. Tidal hydrodynamics. Shallow-water. Seiche. Wind-driven flowEnvironmental ChemistryPhysics::Atmospheric and Oceanic PhysicsGeologyWater Science and Technology
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The Poisson problem: A comparison between two approaches based on SPH method

2012

Abstract In this paper two approaches to solve the Poisson problem are presented and compared. The computational schemes are based on Smoothed Particle Hydrodynamics method which is able to perform an integral representation by means of a smoothing kernel function by involving domain particles in the discrete formulation. The first approach is derived by means of the variational formulation of the Poisson problem, while the second one is a direct differential method. Numerical examples on different domain geometries are implemented to verify and compare the proposed approaches; the computational efficiency of the developed methods is also studied.

Integral representationApplied MathematicsMathematical analysisFunction (mathematics)Domain (software engineering)Smoothed-particle hydrodynamicsSettore MAT/08 - Analisi NumericaComputational MathematicsVariational principleApplied mathematicsPoisson problem Meshless method Smoothed Particle Hydrodynamics Consistency restoring Variational principle Differential methodSmoothing kernelPoisson problemDifferential methodMathematicsApplied Mathematics and Computation
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The smoothed particle hydrodynamics method via residual iteration

2019

Abstract In this paper we propose for the first time an iterative approach of the Smoothed Particle Hydrodynamics (SPH) method. The method is widespread in many areas of science and engineering and despite its extensive application it suffers from several drawbacks due to inaccurate approximation at boundaries and at irregular interior regions. The presented iterative process improves the accuracy of the standard method by updating the initial estimates iterating on the residuals. It is appealing preserving the matrix-free nature of the method and avoiding to modify the kernel function . Moreover the process refines the SPH estimates and it is not affected by disordered data distribution. W…

Iterative and incremental developmentComputer scienceMechanical EngineeringComputational MechanicsProcess (computing)General Physics and Astronomy010103 numerical & computational mathematicsBivariate analysisIterated residualResidual01 natural sciencesComputer Science Applications010101 applied mathematicsSmoothed-particle hydrodynamicsSettore MAT/08 - Analisi NumericaDistribution (mathematics)Smoothed particle hydrodynamicMechanics of MaterialsConvergence (routing)Test functions for optimization0101 mathematicsConvergenceAlgorithmAccuracyKernel based method
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Experimental and numerical investigation of the leading edge sweep angle effect on the performance of a delta blades hydrokinetic turbine

2020

Abstract In the last decades, an increase of energy consumption has been noted around the world. Hence, the excessive use of fossil fuels can lead to serious environmental concerns. Indeed, the use of renewable energy sources is needed to reduce the greenhouse gas effects and the CO2 emissions in the atmosphere. Small-scale hydropower could be an interesting and renewable alternative solution. The cross-flow turbines present several advantages compared to the axial-flow turbines. Therefore, increasing efforts are taken to enhance the efficiency and extend the applicability of the cross-flow turbines. In this paper, experimental investigation was carried out to evaluate the performance of a …

Leading edge060102 archaeologyRenewable Energy Sustainability and the Environmentbusiness.industry020209 energyFlow (psychology)06 humanities and the arts02 engineering and technologyEnergy consumptionComputational fluid dynamicsTurbineRenewable energySettore ICAR/01 - IdraulicaDelta Blades Leading Edge Sweep Angle CFD Rotor Efficiency Hydrodynamic Characteristic0202 electrical engineering electronic engineering information engineeringSwept wingEnvironmental science0601 history and archaeologybusinessHydropowerMarine engineering
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Numerical investigation of rain droplet impact on offshore wind turbine blades under different rainfall conditions: A parametric study

2020

The leading edge of a fiber composite wind turbine blade (WTB) is prone to erosion damages due to repeated rain droplet impact during its service life. Such damages are critical to the blade's aerodynamic as well as structural performance, ultimately resulting in substantial repair costs. An effective design of a coating material for WTB is necessary and its analysis must include variables associated with erosive rain droplets such as (1) droplet diameter, (2) impact velocity, and (3) droplet impact angle. The present paper develops and validates a coupled fluid structure interaction (FSI) computational model for simulating rain droplet impact on WTBs, where the structure domain is modelled…

Leading edgeOffshore wind turbine bladeTurbine blade02 engineering and technologyAerodynamicsMechanics021001 nanoscience & nanotechnologySmooth particle hydrodynamics (SPH)Finite element methodlaw.inventionSmoothed-particle hydrodynamicsOffshore wind powerVDP::Teknologi: 500020303 mechanical engineering & transports0203 mechanical engineeringCoating materiallawFluid–structure interactionCeramics and CompositesErosionOperation and maintenanceEnvironmental science0210 nano-technologyCivil and Structural EngineeringLeading edge erosion
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