Search results for "hydrodynamic"

showing 10 items of 530 documents

Influence of the porosity profile and sets of Ergun constants on the main hydrodynamic parameters in the trickle-bed reactors

2014

Abstract The Eulerian multiphase code has been applied for the comparative simulation of the experimental results obtained for varying flow rates of both fluid phases and for systems of various physicochemical properties used in the laboratory trickle-bed reactor (TBR). Therefore six different radial porosity profiles and three sets of the Ergun constants used in the relations defining the interphase momentum exchange have been implemented into the CFD code. The mean relative error of the pressure drop and of the averaged holdup as well as the standard deviation determined with respect to the experiments have been used as the criterion for the validation of the theoretical model. These valu…

Pressure dropMomentum (technical analysis)Chemistrybusiness.industryGeneral Chemical EngineeringTrickle-bed reactors; CFD; HydrodynamicsEulerian pathGeneral ChemistryMechanicsComputational fluid dynamicsIndustrial and Manufacturing EngineeringStandard deviationVolumetric flow ratesymbols.namesakeApproximation errorsymbolsEnvironmental ChemistryPorositybusinessSimulationChemical Engineering Journal
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The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines

2020

We analyze high-resolution (dv=<10km/s) optical and infrared spectra covering the [OI] 6300 angstrom and [NeII] 12.81 micron lines from a sample of 31 disks in different evolutionary stages. Following work at optical wavelengths, we use Gaussian profiles to fit the [NeII] lines and classify them into HVC (LVC) if the line centroid is more (less) blueshifted than 30 km/s with respect to the stellar radial velocity. Unlike for the [OI] where a HVC is often accompanied by a LVC, all 17 sources with a [NeII] detection have either a HVC or a LVC. [NeII] HVCs are preferentially detected toward high accretors (Macc > 10$^{-8}$ Msun/yr) while LVCs are found in sources with low Macc, low [OI] …

Protoplanetary disks1300010504 meteorology & atmospheric sciencesInfraredFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityStellar accretion disksStellar jets0103 physical sciences1607010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)Earth and Planetary Astrophysics (astro-ph.EP)PhysicsSpectral index1579Astronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesRadial velocityFull width at half maximumWavelengthAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)MagnetohydrodynamicsAstrophysics - Earth and Planetary Astrophysics
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Computational fluid dynamics of the ascending aorta before the onset of type A aortic dissection.

2016

We performed a pre-dissection computational fluid analysis of an ascending aortic aneurysm associated with unicuspid aortic valve. The analysis showed an abnormal helical flow pattern inside the aneurysm and an increased wall stress on the right postero-lateral wall of the ascending aorta. These values were largely higher than the theoretical cut-off for aortic wall dissection, their topographic distribution followed the intimal tear site as subsequently diagnosed by computed tomography scan and confirmed during the operation for dissection repair.

Pulmonary and Respiratory MedicineAdultMalemedicine.medical_specialty0206 medical engineeringBlood Pressure02 engineering and technologyDissection (medical)030204 cardiovascular system & hematologyAortographyComputer03 medical and health sciencesAortic aneurysm0302 clinical medicineAneurysmAneurysm Dissectingmedicine.arteryInternal medicineAscending aortamedicineHumansComputer SimulationAortaAortic dissectionAortabusiness.industryModels CardiovascularSettore ING-IND/34 - Bioingegneria IndustrialeHydrodynamicGeneral Medicinemedicine.disease020601 biomedical engineeringUnicuspid aortic valveAortic wallAortic AneurysmAortic Dissectioncardiovascular systemCardiologyHydrodynamicsSurgeryStress MechanicalCardiology and Cardiovascular MedicinebusinessTomography X-Ray ComputedBlood Flow VelocityHumanEuropean journal of cardio-thoracic surgery : official journal of the European Association for Cardio-thoracic Surgery
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Magnetohydrodynamic simulations of the ejection of a magnetic flux rope

2013

Context. Coronal mass ejections (CME's) are one of the most violent phenomena found on the Sun. One model to explain their occurrence is the flux rope ejection model. In this model, magnetic flux ropes form slowly over time periods of days to weeks. They then lose equilibrium and are ejected from the solar corona over a few hours. The contrasting time scales of formation and ejection pose a serious problem for numerical simulations. Aims: We simulate the whole life span of a flux rope from slow formation to rapid ejection and investigate whether magnetic flux ropes formed from a continuous magnetic field distribution, during a quasi-static evolution, can erupt to produce a CME. Methods: To …

Q ScienceMagnetohydrodynamics (MHD)coronal mass ejections [Sun]010504 meteorology & atmospheric sciencescorona [Sun]FluxAstrophysicsmagnetic fields01 natural sciencesmagnetohydrodynamics (MHD)0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsSun: coronal mass ejectionsSun: coronaQSunAstronomy and AstrophysicsCoronal loopCoronaMagnetic fluxNanoflares13. Climate actionSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsCoronal mass ejectionsCoronaMagnetohydrodynamicsRope
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Thermoelectric magnetohydrodynamic control of melt pool dynamics and microstructure evolution in additive manufacturing.

2020

Large thermal gradients in the melt pool from rapid heating followed by rapid cooling in metal additive manufacturing generate large thermoelectric currents. Applying an external magnetic field to the process introduces fluid flow through thermoelectric magnetohydrodynamics. Convective transport of heat and mass can then modify the melt pool dynamics and alter microstructural evolution. As a novel technique, this shows great promise in controlling the process to improve quality and mitigate defect formation. However, there is very little knowledge within the scientific community on the fundamental principles of this physical phenomenon to support practical implementation. To address this mu…

QA75Materials scienceGeneral MathematicsThermoelectric effectDynamics (mechanics)ThermalGeneral EngineeringGeneral Physics and AstronomyMechanicsMagnetohydrodynamic driveMelt poolMicrostructureMagnetic fieldPhilosophical transactions. Series A, Mathematical, physical, and engineering sciences
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Predictions for multiplicities and flow harmonics in 5.44 TeV Xe+Xe collisions at the CERN Large Hadron Collider

2018

We present the next-to-leading-order event-by-event EKRT model predictions for the centrality dependence of the charged hadron multiplicity in the pseudorapidity interval $|\eta|\le 0.5$, and for the centrality dependence of the charged hadron flow harmonics $v_n\{2\}$ obtained from 2-particle cumulants, in $\sqrt{s_{NN}}=5.44$ TeV Xe+Xe collisions at the CERN Large Hadron Collider. Our prediction for the 0-5 \% central charged multiplicity is $dN_{\rm ch}/d\eta =1218\pm 46$. We also predict $v_n\{2\}$ in Xe+Xe collisions to increase more slowly from central towards peripheral collisions than those in a Pb+Pb system. We find that at $10 \dots 50$\% centralities $v_2\{2\}$ is smaller and $v_…

QuarkParticle physicsNuclear TheoryHadronFOS: Physical scienceshiukkasfysiikka01 natural sciences114 Physical sciencesNuclear physicsENERGYNuclear Theory (nucl-th)GLUON DISTRIBUTION-FUNCTIONSHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBAYESIAN-ANALYSISRapidityNUCLEAR COLLISIONS010306 general physicsNuclear ExperimentPhysicscollective flowta114010308 nuclear & particles physicsparticle and resonance productionHigh Energy Physics::PhenomenologyHIGH-DENSITY QCDQUARKMultiplicity (mathematics)Nuclear matterHigh Energy Physics - PhenomenologyPseudorapidityHigh Energy Physics::ExperimentImpact parameterhydrodynamic modelsCentralityrelativistic heavy-ion collisions
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On a radiating fluid in a general relativistic context

2006

A model for the radiation hydrodynamics in general relativity is analyzed, describing the gravitational collapse and supernovae explosion. As these physical phenomena can be assumed spherically symmetric, the equations of motion for a unique fluid, representing the interaction between matter and radiation, are written in a spherical symmetric space-time with respect to a comoving frame. The system is completed by using the Eddington closure, assuming a local thermodynamical equilibrium for the radiation field. The resulting system is analyzed by the Lie symmetry approach and a reduction to an ODEs system is obtained. Numerical simulations of the solutions are performed, showing a realistic …

Radiation hydrodynamics Lie symmetries Exact solutions
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X-ray emitting MHD accretion shocks in classical T Tauri stars. Case for moderate to high plasma-beta values

2009

AIMS. We investigate the stability and dynamics of accretion shocks in CTTSs, considering the case of beta >= 1 in the post-shock region. In these cases the 1D approximation is not valid and a multi-dimensional MHD approach is necessary. METHODS. We model an accretion stream propagating through the atmosphere of a CTTS and impacting onto its chromosphere, by performing 2D axisymmetric MHD simulations. The model takes into account the stellar magnetic field, the gravity, the radiative cooling, and the thermal conduction (including the effects of heat flux saturation). RESULTS. The dynamics and stability of the accretion shock strongly depends on the plasma beta. In the case of shocks with…

Radiative coolingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesX-rays: starsAstrophysicsstars: pre-main sequenceInstabilitymagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics::Solar and Stellar AstrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)accretion accretion disksStellar magnetic fieldStellar atmosphereAstronomy and Astrophysicsshock wavesAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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A numerical meshless particle method in solving the magnetoencephalography forward problem

2012

In this paper, a numerical meshless particle method is presented in order to solve the magnetoencephalography forward problem for analyzing the complex activation patterns in the human brain. The forward problem is devoted to compute the scalp potential and magnetic field distribution generated by a set of current sources representing the neural activity, and in this paper, it has been approached by means of the smoothed particle hydrodynamics method suitably handled. The Poisson equation generated by the quasi-stationary Maxwell's curl equations, by assuming Neumann boundary conditions has been considered, and the current sources have been simulated by current dipoles. The adopted meshless…

Regularized meshless methodSingular boundary methodComputer Science ApplicationsSmoothed-particle hydrodynamicssymbols.namesakeClassical mechanicsMaxwell's equationsMesh generationModeling and SimulationNeumann boundary conditionsymbolsApplied mathematicsElectrical and Electronic EngineeringPoisson's equationBoundary element methodMathematicsInternational Journal of Numerical Modelling: Electronic Networks, Devices and Fields
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Prediction of river discharges at confluences based on Entropy theory and surface-velocity measurements

2022

Hydrodynamic features of the confluence zone of large rivers are complicated because of their three-dimensional flow structure. The confluence between the Rio Negro and the Rio Solimões, characterised by black and white waters, respectively, ranks among the largest river junctions on Earth. An Entropy-based investigation was carried out to assess the discharge and analyse the 2D structure of velocity distribution for large river flows relying on monitoring of near-surface velocity only. The estimated flow data where compared with in-situ ADCP data gathered across some transects of the Negro and Solimões rivers during both low and relatively high flow conditions. Results are illustrated thro…

RiverVelocity-dipconfluenceEntropy methodentropicpredictionMega riverSecondary currentWater Science and Technologyhydrodynamic
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