Search results for "Turbulence"

showing 10 items of 378 documents

Experiments and predictions of the transition of the flow pattern with impeller clearance in stirred tanks

2001

In the present work, the double- to single-loop flow pattern transition in a stirred vessel equipped with a Rushton turbine is investigated by Laser Doppler anemometry (LDA). In particular, the clearance at which such transition occurs is assessed by comparing axial velocity profiles underneath the impeller. Computational fluid dynamics (CFD) simulations of the same system are carried out, by employing the 'inner-outer' fully predictive computation strategy. The comparison of predicted results with the experimental data collected shows that the transition is well reproduced by simulations. A good agreement on the mean velocities is also observed but for the impeller discharge stream angle t…

Work (thermodynamics)Materials sciencebusiness.industryTurbulenceInner-outer methodGeneral Chemical EngineeringComputationSettore ING-IND/25 - Impianti ChimiciMechanical engineeringMechanicsComputational fluid dynamicsLaser Doppler velocimetryFlow patternComputer Science ApplicationsRushton turbinePhysics::Fluid DynamicsRushton turbineImpellerComputational fluid dynamicLaser Doppler anemometryControl and Systems EngineeringStirred vesselChemical Engineering (all)Single-double-loop transitionbusiness
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Modelling and simulation of gas-liquid hydrodynamics in mechnically stirred tanks

2007

Abstract Computational fuid dynamics (CFD) is an increasingly important tool for carrying out realistic simulations of process equipment. In the case of multiphase systems the development of CFD models is less advanced than for single-phase systems. In the present work CFD simulations of gas–liquid stirred tanks are reported. An Eulerian–Eulerian multi-fluid approach is used in conjunction with the simplest two-phase extension of the k–ɛ turbulence model. All bubbles are assumed to share the same size. The effect of inter-phase forces on simulation results is separately considered. As concerns drag, it is shown that the sole parameter needed to characterize the dispersed phase behaviour is …

Work (thermodynamics)Terminal velocityGeneral Chemical EngineeringBubbleFLOWSettore ING-IND/25 - Impianti ChimiciBUBBLE-COLUMN REACTORSSINGLE BUBBLESComputational fluid dynamicsPhysics::Fluid DynamicsMomentumsymbols.namesakeControl theorySYSTEMSCFD SIMULATIONSPhysicsTurbulencebusiness.industryNUMERICAL SIMULATIONSGeneral ChemistryMechanicsVELOCITYEuler equationsDragVESSELsymbolsTURBULENCERUSHTON TURBINEbusiness
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Dip Phenomenon in High-Curved Turbulent Flows and Application of Entropy Theory

2018

The estimation of velocity profile in turbulent open channels is a difficult task due to the significant effects of the secondary flow. The present paper investigates the mechanism of the velocity-dip phenomenon, whereby the location of the maximum velocity appears to be below the free surface. Previous studies conducted in straight channels relate the mechanism of the velocity-dip phenomenon to secondary flow induced by anisotropy of turbulence. This work focuses on high-curved channels where the secondary motion, which is also induced by the channel’s curvature, evolves along the bend. The width-to-depth ratio, B/h, is one of the most important parameters that are affecting the secondary …

Work (thermodynamics)lcsh:Hydraulic engineeringAspect ratioriver0208 environmental biotechnologyGeography Planning and Development02 engineering and technologyAquatic ScienceCurvatureBiochemistrySettore ICAR/01 - Idraulicalcsh:Water supply for domestic and industrial purposeslcsh:TC1-978AnisotropyWater Science and TechnologyPhysicslcsh:TD201-500Turbulenceturbulencesecondary motionMechanicspredictionrivers; meanders; turbulence; secondary motion; predictionSecondary flowrivers020801 environmental engineeringFlow velocityFree surfacemeandersmeanderWater; Volume 10; Issue 3; Pages: 306
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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Exploring the Solar Wind from Its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter-Parker Solar Probe Quadrature

2021

This Letter addresses the first Solar Orbiter (SO) -- Parker Solar Probe (PSP) quadrature, occurring on January 18, 2021, to investigate the evolution of solar wind from the extended corona to the inner heliosphere. Assuming ballistic propagation, the same plasma volume observed remotely in corona at altitudes between 3.5 and 6.3 solar radii above the solar limb with the Metis coronagraph on SO can be tracked to PSP, orbiting at 0.1 au, thus allowing the local properties of the solar wind to be linked to the coronal source region from where it originated. Thanks to the close approach of PSP to the Sun and the simultaneous Metis observation of the solar corona, the flow-aligned magnetic fiel…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaSolar windFOS: Physical sciencesSolar radiusSolar coronaAstrophysics01 natural scienceslaw.inventionCurrent sheetOrbiterMagnetohydrodynamicsInterplanetary turbulenceHeliospherePhysics - Space Physics[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]law0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsCoronagraphSolar and Stellar Astrophysics (astro-ph.SR)Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsMagnetohydrodynamics; Space plasmas; Interplanetary turbulence; Solar corona; Heliosphere; Solar windAstronomy and AstrophysicsPlasma[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]CoronaSpace Physics (physics.space-ph)[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]Physics - Plasma PhysicsPlasma Physics (physics.plasm-ph)Solar windAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsSpace plasmasAstrophysics::Earth and Planetary Astrophysics[PHYS.PHYS.PHYS-DATA-AN]Physics [physics]/Physics [physics]/Data Analysis Statistics and Probability [physics.data-an]Heliosphere
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Emergence of rogue waves from optical turbulence

2011

International audience; We provide some general physical insights into the emergence of rogue wave events from optical turbulence by analyzing the long term evolution of the field. Depending on the amount of incoherence in the system (i.e., Hamiltonian), we identify three turbulent regimes that lead to the emergence of specific rogue wave events: (i) persistent and coherent rogue quasi-solitons, (ii) intermittent-like rogue quasi-solitons that appear and disappear erratically, and (iii) sporadic rogue waves events that emerge from turbulent fluctuations as bursts of light or intense flashes.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Nonlinear opticsStatistical opticsField (physics)General Physics and AstronomyStatistical opticsPhysics::OpticsAstrophysics01 natural sciencesPulse propagation and temporal solitons010305 fluids & plasmas010309 opticsPhysics::Fluid Dynamics0103 physical sciencesStatistical physicsRogue wave010306 general physicsDispersion (water waves)Nonlinear Sciences::Pattern Formation and SolitonsPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]TurbulenceTerm (time)Nonlinear Sciences::Chaotic DynamicsClassical mechanicsNonlinear Sciences::Exactly Solvable and Integrable SystemsOptical turbulenceCoherenceOptical turbulenceCoherence (physics)
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Classical wave thermalisation in chaotic multimode optical fibre

2023

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Nonlinear opticsWave condensationChaotic dynamicsThermalisationWave turbulenceMultimode optical fibres[PHYS] Physics [physics]
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Rogue wave description: Rational solitons and wave turbulence theory

2012

We show that rogue waves can emerge from optical turbulence and that their coherent deterministic description provided by the rational solutions is compatible with the statistical description provided by the wave turbulence theory.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Computer simulationTurbulenceWave turbulenceNonlinear opticsTurbulence theory01 natural sciences010305 fluids & plasmasPhysics::Fluid DynamicsClassical mechanics0103 physical sciencesOptical turbulenceRogue wave010306 general physicsDispersion (water waves)ComputingMilieux_MISCELLANEOUS
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Wave turbulence in integrable systems: nonlinear propagation of incoherent optical waves in single-mode fibers.

2011

International audience; We study theoretically, numerically and experimentally the nonlinear propagation of partially incoherent optical waves in single mode optical fibers. We revisit the traditional treatment of the wave turbulence theory to provide a statistical kinetic description of the integrable scalar NLS equation. In spite of the formal reversibility and of the integrability of the NLS equation, the weakly nonlinear dynamics reveals the existence of an irreversible evolution toward a statistically stationary state. The evolution of the power spectrum of the field is characterized by the rapid growth of spectral tails that exhibit damped oscillations, until the whole spectrum ultima…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Integrable systembusiness.industryWave turbulenceSingle-mode optical fiberSpectral densityNonlinear optics01 natural sciencesAtomic and Molecular Physics and Optics010309 opticsNonlinear systemOpticsClassical mechanics0103 physical sciences010306 general physicsbusinessStationary stateCoherence (physics)Optics express
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Self-organization of incoherent optical waves : Condensation, thermalization and repolarization

2019

The subject of this thesis concerns the study of phenomena of self-organization of incoherentoptical waves. This work is essentially theoretical and numerical and relies on different formalisms of waveturbulence theory, the Hamiltonian singularities, and different experiments.The first part of the thesis deals with the irreversible processes of thermalization and condensation ofincoherent waves. The phenomenon of condensation is characterized by the formation of a large scale co-herent structure (condensate) that remains immersed in a sea of small scale fluctuations (uncondensedparticules). In spite of the large propagation lengths required to reach the condensed equilibrium state, wehave i…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Non-Linear opticsWave condensationIncoherent wave thermalizationContrôle de polarisationCondensations d'ondesPolarization controlTurbulence d'ondesWave turbulenceOptique non-LinéaireThermalisation d'ondes incohérentes
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