Search results for " Hydrodynamics"

showing 10 items of 93 documents

A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method

2021

We have demonstrated that the Transition Region Adaptive Conduction (TRAC) method permits fast and accurate numerical solutions of the field-aligned hydrodynamic equations, successfully removing the influence of numerical resolution on the coronal density response to impulsive heating. This is achieved by adjusting the parallel thermal conductivity, radiative loss, and heating rates to broaden the transition region (TR), below a global cutoff temperature, so that the steep gradients are spatially resolved even when using coarse numerical grids. Implementing the original 1D formulation of TRAC in multi-dimensional magnetohydrodynamic (MHD) models would require tracing a large number of magne…

Sun: flaresMagnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]Field lineNDASFOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencestransition region [Sun]0103 physical sciencesRadiative transferQB AstronomyMagnetohydrodynamic driveflares hydrodynamics [Sun]Sun: transition region010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencescomputer.programming_languageQBPhysicsSun: coronaSun: chromosphereAstronomy and AstrophysicsTRACCoronal loopThermal conductionComputational physicsMagnetic fieldQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHydrodynamicsMagnetohydrodynamicscomputerSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo Circumterrestre
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A mesoscopic mechanical model of the surface tension and some simulation results

2019

Abstract Drops of mercury do not spread on a surface. A metal paper clip can float on water. These phenomena are macroscopic manifestations of molecular interactions and can be explained in terms of surface tension. In this study, we discuss a simple mesoscopic mechanical model of the surface tension and the results of numerical fluid dynamics simulations implemented on the basis of it. We study the droplet formation without and with gravity when it can drop from a narrow hole like a trickling tap and finally the behaviour of free surface liquid in a vessel. Teachers and students can be able to study the surface tension by using the computer simulation as a “tool” for analysing and discussi…

Surface tensionHistoryMesoscopic physicsMaterials scienceMechanicsFluid dynamics. Surface tension. Modelling. Simulation. Smoothed particles hydrodynamics.Computer Science ApplicationsEducationJournal of Physics: Conference Series
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Computer simulations to approach surface tension by means of a simple mesoscopic mechanical model

2019

A small insect can stand or walk on water surface, drops of mercury do not spread on a solid surface, and a meniscus is formed at the free surface of a liquid contained in a thin vessel. These phenomena can be seen as macroscopic manifestations of molecular interactions and can be explained macroscopically in terms of surface tension. In this study, we deal with an approach to surface tension from a mechanical point of view, presenting a simple mesoscopic mechanical model of surface tension and the results of its implementation in numerical fluid dynamics simulations. Particularly, phenomena like droplet formation without gravity and with gravity when it can drop from a narrow hole like a t…

Surface tensionSmoothed-particle hydrodynamicsMesoscopic physicsMaterials scienceGeneral Computer ScienceSimple (abstract algebra)Settore FIS/08 - Didattica E Storia Della Fisicacomputer simulation mesoscopic model smoothed‐particle hydrodynamics surface tensionGeneral EngineeringMechanicsEducation
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A computational framework for coating fatigue analysis of wind turbine blades due to rain erosion

2021

Author's accepted manuscript The rain-induced fatigue damage in the wind turbine blade coating has attracted increasing attention owing to significant repair and maintenance costs. The present paper develops an improved computational framework for analyzing the wind turbine blade coating fatigue induced by rain erosion. The paper first presents an extended stochastic rain field simulation model that considers different raindrop shapes (spherical, flat, and spindle), raindrop sizes, impact angles, and impact speeds. The influence of these raindrop characteristics on the impact stress of the blade coating is investigated by a smoothed particle hydrodynamics approach. To address the expensive …

Turbine blade020209 energyRain erosionSmoothed particle hydrodynamicsFatigue damage02 engineering and technologyengineering.materialRaindrop impactlaw.inventionSmoothed-particle hydrodynamicsStress (mechanics)Coatinglaw0202 electrical engineering electronic engineering information engineering0601 history and archaeology060102 archaeologyCrack propagationRenewable Energy Sustainability and the Environmentbusiness.industryFracture mechanics06 humanities and the artsStructural engineeringFatigue analysisWind turbine bladeVDP::Teknologi: 500ErosionengineeringEnvironmental sciencebusinessInterpolationRenewable Energy
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Modeling an X-ray Flare on Proxima Centauri: evidence of two flaring loop components and of two heating mechanisms at work

2003

We model in detail a flare observed on Proxima Centauri with the EPIC-PN on board XMM-Newton at high statistics and high time resolution and coverage. Time-dependent hydrodynamic loop modeling is used to describe the rise and peak of the light curve, and a large fraction of the decay, including its change of slope and a secondary maximum, over a duration of more than 2 hours. The light curve, the emission measure and the temperature derived from the data allow us to constrain the loop morphology and the heating function and to show that this flare can be described with two components: a major one triggered by an intense heat pulse injected in a single flaring loop with half-length ~1.0 10^{…

Work (thermodynamics)010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics01 natural scienceslaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsLoop modelingstars: flare stars: coronae X-rays: stars hydrodynamics010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsLight curveCoronaPulse (physics)Loop (topology)13. Climate actionSpace and Planetary ScienceEvent (particle physics)Flare
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The dawning of the theory of equilibrium figures: a brief historical account from the 16th through the 20th century

2014

A very brief historical survey of the theory of equilibrium figures is outlined, from the early origins, dating back to the late 1500s, until up the latest 20th century developments. A seen toward physical applications, ranging from relativistic astrophysics through nuclear physics, is also provided.

celestial bodieatomic nucleiSelf-gravitanting fluid; hydrodynamics; celestial bodies; atomic nucleiSelf-gravitanting fluidhydrodynamic
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Use of stable isotopes to investigate dispersal of waste from fish farm as a function of hydrodynamics.

2006

Stable isotopes were used to examine differential effects of fish farm waste on the water column and sediments. To achieve this objective, we chose 3 marine fish farms located along the coast of Sicily (Mediterranean Sea) as point-source disturbances, and a control area. The hypothesis that carbon and nitrogen isotope composition of particulate (POM) and sedimentary (SOM) organic matter varied with increasing distance (from cages to 1000 m) was tested at 3 levels of hydrodynam- ics: low (mean velocity of current (MVC) ~12 cm s -1 ), intermediate (MVC ~22 cm s -1 ), and high (MVC ~40 cm s -1 ). Different isotopic signals from allochthonous (fish waste) over natural (phytoplankton, terrigenou…

chemistry.chemical_classificationSettore BIO/07 - EcologiaEcologybusiness.industryTerrigenous sedimentStable isotope ratioFish farmingstable isotope aquaculture sedimentsAquatic ScienceIsotopes of nitrogenOceanographyWater columnMediterranean seachemistryAquacultureEnvironmental scienceOrganic matterFish farming Impact Water column Sediment Stable isotopes Hydrodynamics MediterraneanbusinessEcology Evolution Behavior and Systematics
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Towards an efficient meshfree solver

2016

In this paper we focus on the enhancement in accuracy approximating a function and its derivatives via smoothed particle hydrodynamics. We discuss about improvements in the solution by reformulating the original method by means of the Taylor series expansion and by projecting with the kernel function and its derivatives. The accuracy of a function and its derivatives, up to a fixed order, can be simultaneously improved by assuming them as unknowns of a linear system. The improved formulation has been assessed with gridded and scattered data points distribution and the convergence has been analyzed referring to a case study in a 2D domain.

convergenceaccuracyLinear systemFunction (mathematics)SolverSmoothed-particle hydrodynamicssymbols.namesakeSettore MAT/08 - Analisi NumericaSettore ING-IND/31 - ElettrotecnicaData pointConvergence (routing)Taylor seriessymbolsmeshless methodFocus (optics)AlgorithmMathematics
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A CUDA-based implementation of an improved SPH method on GPU

2021

We present a CUDA-based parallel implementation on GPU architecture of a modified version of the Smoothed Particle Hydrodynamics (SPH) method. This modified formulation exploits a strategy based on the Taylor series expansion, which simultaneously improves the approximation of a function and its derivatives with respect to the standard formulation. The improvement in accuracy comes at the cost of an additional computational effort. The computational demand becomes increasingly crucial as problem size increases but can be addressed by employing fast summations in a parallel computational scheme. The experimental analysis showed that our parallel implementation significantly reduces the runti…

fast gauss transformScheme (programming language)0209 industrial biotechnologyComputer scienceApplied Mathematics020206 networking & telecommunications02 engineering and technologyFunction (mathematics)Computational scienceSmoothed-particle hydrodynamicsComputational MathematicsCUDAsymbols.namesakeSettore MAT/08 - Analisi Numerica020901 industrial engineering & automationgraphic processing unit0202 electrical engineering electronic engineering information engineeringTaylor seriessymbolsSmoothed Particle Hydrodynamics Fast Gauss Transform Graphics Processing Unit.Central processing unitsmoothed particle hydorodinamicscomputercomputer.programming_language
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Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution

2018

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity, gas mass, X-ray temperature, and $Y_{X}$. Three sets of simulations are performed with an improved version of the smoothed particle hydrodynamics GADGET-3 code. These consider the following: non-radiative gas, star formation and stellar feedback, and the addition of feedback by active galactic nuclei (AGN). We select clusters with $M_{500} > 10^{14} M_{\odot} E(z)^{-1}$, mimicking the typical selection of Sunyaev-Zeldovich samples. This permits to have a mass range large enough to enable robust fitting of the r…

galaxies: clusters: intracluster mediumCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusNUMERICAL [METHODS]Ciencias FísicasFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsnumerical galaxies: clusters: general galaxies: clusters: intracluster medium X-rays: galaxies: clusters [methods]01 natural sciencesmethods: numericalLuminosity//purl.org/becyt/ford/1 [https]GALAXIES: CLUSTERS [X-RAYS]Smoothed-particle hydrodynamics0103 physical sciences010303 astronomy & astrophysicsScalingAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysicsmethods: numerical galaxies: clusters: general galaxies: clusters: intracluster medium X-rays: galaxies: clustersSettore FIS/05010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsObservable//purl.org/becyt/ford/1.3 [https]RedshiftAstronomíamethods: numerical; galaxies: clusters: general; galaxies: clusters: intracluster medium; X-rays: galaxies: clusters; Astrophysics - Cosmology and Nongalactic Astrophysicsgalaxies: clusters: generalSpace and Planetary ScienceX-rays: galaxies: clustersCLUSTERS: INTRACLUSTER MEDIUM [GALAXIES]CLUSTERS: GENERAL [GALAXIES]CIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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