Search results for " Simulation"

showing 10 items of 4034 documents

Comparison between observation and simulation of sodium LGS return flux with a 20W CW laser on Tenerife

2016

We report on the comparison between observations and simulations of a completed 12-month field observation campaign at Observatorio del Teide, Tenerife, using ESO's transportable 20 watt CW Wendelstein laser guide star system. This mission has provided sodium photon return flux measurements of unprecedented detail regarding variation of laser power, polarization and sodium D2b repumping. The Raman fiber laser and projector technology are very similar to that employed in the 4LGSF/AOF laser facility, recently installed and commissioned at the VLT in Paranal. The simulations are based on the open source LGSBloch density matrix simulation package and we find good overall agreement with experim…

PhysicsPhoton010504 meteorology & atmospheric sciencesComputer simulationbusiness.industryPolarization (waves)Laser01 natural scienceslaw.inventionsymbols.namesakeLaser guide starOpticslawFiber laser0103 physical sciencessymbolsLaser power scalingbusinessRaman spectroscopy010303 astronomy & astrophysics0105 earth and related environmental sciencesAdaptive Optics Systems V
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Acoustic Wave Properties in Footpoints of Coronal Loops in 3D MHD Simulations

2021

Acoustic waves excited in the photosphere and below might play an integral part in the heating of the solar chromosphere and corona. However, it is yet not fully clear how much of the initially acoustic wave flux reaches the corona and in what form. We investigate the wave propagation, damping, transmission, and conversion in the lower layers of the solar atmosphere using 3D numerical MHD simulations. A model of a gravitationally stratified expanding straight coronal loop, stretching from photosphere to photosphere, is perturbed at one footpoint by an acoustic driver with a period of 370 seconds. For this period acoustic cutoff regions are present below the transition region (TR). About 2% …

PhysicsPhotosphere010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaSolar physics Solar atmosphere Solar oscillations Solar coronal waves Solar chromosphere Solar coronal loops Magnetohydrodynamical simulations MagnetohydrodynamicsFOS: Physical sciencesAstronomy and AstrophysicsAcoustic waveCoronal loop01 natural sciencesCoronaComputational physicsStanding waveAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Science0103 physical sciencesCutoffAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesThe Astrophysical Journal
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Turbulence structure and budgets in curved pipes

2013

Abstract Turbulent flow in curved pipes was investigated by Direct Numerical Simulation. Three curvatures δ (pipe radius a /curvature radius c ) were examined: δ  = 0 (straight pipe), simulated for validation and comparison purposes; δ  = 0.1; and δ  = 0.3. The friction velocity Reynolds number (based on the pipe radius a ) was 500 in all cases, yielding bulk Reynolds numbers of ∼17,000, ∼15,000 and ∼12,000 for δ  = 0, 0.1 and 0.3, respectively. The computational domain was ten pipe radii in length and was resolved by up to 20 × 10 6 hexahedral finite volumes. The time step was chosen equal to a wall time unit; 1 Large Eddy TurnOver Time (LETOT) was thus resolved by 500 time steps and simul…

PhysicsPlug flowGeneral Computer ScienceTurbulenceDirect Numerical SimulationGeneral EngineeringDirect numerical simulationCurved pipeReynolds numberLaminar flowMechanicsCurved pipe;Direct Numerical Simulation;Turbulence budget;Turbulent flowCurvatureVortexTurbulent flowPhysics::Fluid Dynamicssymbols.namesakeClassical mechanicsTurbulence budgetsymbolsShear velocitySettore ING-IND/19 - Impianti Nucleari
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Noise delayed decay of unstable states: theory versus numerical simulations

2004

We study the noise delayed decay of unstable nonequilibrium states in nonlinear dynamical systems within the framework of the overdamped Brownian motion model. We give the exact expressions for the decay times of unstable states for polynomial potential profiles and obtain nonmonotonic behavior of the decay times as a function of the noise intensity for the unstable nonequilibrium states. The analytical results are compared with numerical simulations.

PhysicsPolynomialStatistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesGeneral Physics and AstronomyNoise intensityNon-equilibrium thermodynamicsStatistical and Nonlinear PhysicsFunction (mathematics)Nonlinear dynamical systemsnumerical simulationsBrownian motion modelStatistical physicsCondensed Matter - Statistical MechanicsMathematical PhysicsNoise (radio)
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Adiabatic quantum simulation with a segmented ion trap: Application to long-distance entanglement in quantum spin systems

2013

We investigate theoretically systems of ions in segmented linear Paul traps for the quantum simulation of quantum spin models with tunable interactions. The scheme is entirely general and can be applied to the realization of arbitrary spin-spin interactions. As a specific application we discuss in detail the quantum simulation of models that exhibit long-distance entanglement in the ground state. We show how tailoring of the axial trapping potential allows for generating spin-spin coupling patterns that are suitable to create long-distance entanglement. We discuss how suitable sequences of microwave pulses can implement Trotter expansions and realize various kinds of effective spin-spin int…

PhysicsQuantum PhysicsQuantum discordCondensed Matter - Mesoscale and Nanoscale PhysicsQuantum sensorFOS: Physical sciencesQuantum simulatorQuantum entanglementQuantum imaging01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmas3. Good healthQuantum mechanicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesQuantum metrologyQuantum algorithmQuantum Physics (quant-ph)010306 general physicsAmplitude damping channelquantum simulationPhysical Review A
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Scale-free relaxation of a wave packet in a quantum well with power-law tails

2013

We propose a setup for which a power-law decay is predicted to be observable for generic and realistic conditions. The system we study is very simple: A quantum wave packet initially prepared in a potential well with (i) tails asymptotically decaying like ~ x^{-2} and (ii) an eigenvalues spectrum that shows a continuous part attached to the ground or equilibrium state. We analytically derive the asymptotic decay law from the spectral properties for generic, confined initial states. Our findings are supported by realistic numerical simulations for state-of-the-art expansion experiments with cold atoms.

PhysicsQuantum PhysicsStatistical Mechanics (cond-mat.stat-mech)Thermodynamic equilibriumWave packetFOS: Physical sciencesGeneral Physics and AstronomyObservableQuantum mechanicPower lawSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)03.65.Ge Solutions of wave equations: bound states 02.60.Cb Numerical simulationtunnelingpower law distributionRelaxation (physics)Statistical physicssolution of equations 03.65.Xp Tunneling traversal time quantum Zeno dynamics 02.10.Ud Linear algebra03.65.Fd Algebraic methodsQuantum Physics (quant-ph)QuantumCondensed Matter - Statistical MechanicsEigenvalues and eigenvectorsQuantum well
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KINETICS OF CRYSTAL GROWTH LIMITED BY RANDOM VELOCITY FIELDS

2008

A spherical growth process controlled by velocity fluctuations of particles of a saturated solution is investigated. Velocity fluctuations are modeled by a Gaussian random field. The interface evolution is determined by a Langevin-type equation with a multiplicative random field, which in the case of the quasi-homogeneous random Gaussian field is equivalent to Fokker–Planck dynamics. We analyze numerically the Fokker–Planck equation and compare growth kinetics in the case of noisy (i.e. space-independent) fluctuations. It is shown that for a large class of spatially correlated velocity fluctuations, the growth kinetics is universal, i.e. it does not depend on the details of statistics of f…

PhysicsRandom fieldField (physics)Applied MathematicsGaussianKineticsDynamics (mechanics)Multiplicative functionGaussian random fieldsymbols.namesakeFlow velocityModeling and SimulationsymbolsStatistical physicsEngineering (miscellaneous)International Journal of Bifurcation and Chaos
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Energy loss measurement of protons in liquid water

2011

The proton stopping power of liquid water was, for the first time, measured in the energy range 4.7-15.2 MeV. The proton energies were determined by the time-of-flight transmission technique with the microchannel plate detectors, which were especially developed for timing applications. The results are compared to the literature values (from ICRU Report 49 (1993) and Janni's tabulation (1982 At. Data Nucl. Data Tables 27 147-339)) which are based on Bethe's formula and an agreement is found within the experimental uncertainty of 4.6%. Thus, earlier reported discrepancy between the experimental and literature stopping power values at lower energies was not observed at the energies considered …

PhysicsRange (particle radiation)Energy lossTime FactorsRadiological and Ultrasound TechnologyProtonLiquid waterDetectorWaterNuclear physicsExperimental uncertainty analysisSolventsStopping power (particle radiation)Computer SimulationLinear Energy TransferRadiology Nuclear Medicine and imagingMicrochannel plate detectorProtonsAtomic physicsRadiometryPhysics in Medicine and Biology
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Dosimetric characteristics of backscattered electrons in lead.

2000

In electron beam therapy, tissue overdose due to electrons backscattered from lead has been profusely studied. To quantify this dose enhancement effect, an electron backscatter factor (EBF) was defined as the ratio of dose at the tissue-inhomogeneity interface with and without the scatterer present. The dependence of the EBF on energy at the scatterer surface is not well known for energies lower than 3 MeV which is the most frequent clinical situation. In this work, we have done Monte Carlo calculations with the GEANT code to study EBF in lead at this energy range. The applicability of this code and the developed procedure for dose estimation has been experimentally verified. The dependence…

PhysicsRange (particle radiation)Radiological and Ultrasound Technologybusiness.industryRadiotherapy Planning Computer-AssistedPhysics::Medical PhysicsMonte Carlo methodDose-Response Relationship RadiationElectronsElectronRadiationComputational physicsOpticsLeadCathode rayElectron Beam TherapyDosimetryRadiology Nuclear Medicine and imagingComputer SimulationbusinessRadiometryMonte Carlo MethodBeam (structure)AlgorithmsSoftwarePhysics in medicine and biology
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Instabilities of concentration stripe patterns in ferrocolloids

1999

Equations describing the kinetics of the phase separation in ferrocolloids in a Hele-Shaw cell under the action of a rotating magnetic field are proposed. Numerical simulation on the basis of a pseudospectral technique demonstrates that upon the action of a rotating field on a magnetic colloid which undergoes the phase separation a periodical system of stripes parallel to the plane of a rotating magnetic field stripes is created. The period of a structure found numerically satisfactorily corresponds to the one calculated on the basis of the energy minimum. Thus, the undulation instability leading to the formation of chevron structures takes place if the tangential component of a rotating ma…

PhysicsRotating magnetic fieldClassical mechanicsComputer simulationField (physics)Condensed matter physicsPlane (geometry)Orientation (geometry)Tangential and normal componentsInstabilityAction (physics)Physical Review E
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