Search results for "turbulence"

showing 10 items of 378 documents

Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

2015

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15∘. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with …

AstrofísicaPhysics and Astronomy (miscellaneous)Raycosmic radiation anisotropy cosmic radiation propagation cosmic radiation deflectionAstronomymagnetic fieldpAstrophysicsanisotropy [cosmic radiation]01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareAugerPierre//purl.org/becyt/ford/1 [https]ObservatoryJetsQuantum Chromodynamicscosmic radiation: VHEenergy: correlationPatternsMonte Carlo010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicscosmic radiation: propagationEnergyCOSMIC cancer databaseAngular distance[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleSearchAstrophysics::Instrumentation and Methods for Astrophysicscosmic radiation anisotropyPierre Auger Observatorycosmic radiation: deflectionRadiación cósmicaAugerSurface Detector ArrayCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaPrincipal axis theorem[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Regular Article - Experimental PhysicsAstrophysics::High Energy Astrophysical PhenomenaPhysics and Astronomy (miscellaneous) Engineering (miscellaneous).FOS: Physical sciencesCosmic ray530cosmic radiation: anisotropyParticle detectorSettore FIS/05 - Astronomia e AstrofisicaVHE [cosmic radiation]statistical analysisSpectrum0103 physical sciencesthrustddc:530Engineering (miscellaneous)AstrophysiqueCiencias ExactasPierre Auger Observatoryair: showerscosmic radiation propagationPhysics and Astronomy (miscellaneous); Engineering (miscellaneous)010308 nuclear & particles physicsturbulence[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstroparticles//purl.org/becyt/ford/1.3 [https]ASTROFÍSICAGalactic Magnetic-fieldcorrelation [energy]DirectionExperimental High Energy Physicscosmic radiation deflectionpropagation [cosmic radiation]direct detectiongalaxyObservatory[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]deflection [cosmic radiation]showers [air]Model
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Simulations of stellar/pulsar wind interaction along one full orbit

2012

The winds from a non-accreting pulsar and a massive star in a binary system collide forming a bow-shaped shock structure. The Coriolis force induced by orbital motion deflects the shocked flows, strongly affecting their dynamics. We study the evolution of the shocked stellar and pulsar winds on scales in which the orbital motion is important. Potential sites of non-thermal activity are investigated. Relativistic hydrodynamical simulations in two dimensions, performed with the code PLUTO and using the adaptive mesh refinement technique, are used to model interacting stellar and pulsar winds on scales ~80 times the distance between the stars. The hydrodynamical results suggest the suitable lo…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencessymbols.namesakePulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAdaptive mesh refinementTurbulenceAstronomy and AstrophysicsParticle accelerationPlutoStarsLorentz factor13. Climate actionSpace and Planetary ScienceOrbital motionsymbolsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts

2002

We consider the transverse structure and stability properties of relativistic jets formed in the course of the collapse of a massive progenitor. Our numerical simulations show the presence of a strong shear in the bulk velocity of such jets. This shear can be responsible for a very rapid shear--driven instability that arises for any velocity profile. This conclusion has been confirmed both by numerical simulations and theoretical analysis. The instability leads to rapid fluctuations of the main hydrodynamical parameters (density, pressure, Lorentz factor, etc.). However, the perturbations of the density are effectively decoupled from those of the pressure because the beam of the jet is radi…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies jetsAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAInstabilitysymbols.namesakeAstrophysical jetISM jets and outflowsPhysicsBurstsGamma ray theoryTurbulenceAstrophysics (astro-ph)Magnetohydradynamics (MHD) : Gamma rays ; Bursts ; Gamma ray theory ; ISM jets and outflows ; galaxies jetsAstronomy and AstrophysicsMechanicsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Transverse planeLorentz factorSpace and Planetary SciencesymbolsGamma rays [Magnetohydradynamics (MHD)]OutflowUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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The Effect of Turbulence on the Accretional Growth of Graupel

2019

Abstract Wind tunnel experiments were carried out to investigate the influence of turbulence on the collection kernel of graupel. The collection kernel defines the growth rate of a graupel accreting supercooled droplets as it falls through a cloud. The ambient conditions were similar to those occurring typically in the mixed-phase zone of convective clouds, that is, at temperatures between −7° and −16°C and with liquid water contents from 0.5 to 1.3 g m−3. Tethered spherical collectors with radii between 220 and 340 μm were exposed in a flow carrying supercooled droplets with a mean volume radius of 10 μm. The vertical root-mean-square fluctuation velocity, the dissipation rate, and the Tay…

Atmospheric Science010504 meteorology & atmospheric sciencesTurbulence01 natural sciences010305 fluids & plasmasPhysics::Fluid DynamicsKernel (statistics)0103 physical sciencesGrowth ratePrecipitationStatistical physicsGraupel0105 earth and related environmental sciencesMathematicsJournal of the Atmospheric Sciences
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The evolution of microphysical and optical properties of an A380 contrail in the vortex phase

2012

A contrail from a large-body A380 aircraft at cruise in the humid upper troposphere has been probed with in-situ instruments onboard the DLR research aircraft Falcon. The contrail was sampled during 700 s measurement time at contrail ages of about 1–4 min. The contrail was in the vortex regime during which the primary wake vortices were sinking 270 m below the A380 flight level while the secondary wake remained above. Contrail properties were sampled separately in the primary wake at 90 and 115 s contrail age and nearly continously in the secondary wake at contrail ages from 70 s to 220 s. The scattering phase functions of the contrail particles were measured with a polar nephelometer. The …

Atmospheric Science010504 meteorology & atmospheric sciencesWakeAtmospheric sciences01 natural sciences010305 fluids & plasmaslcsh:ChemistryTroposphere0103 physical sciencesclimate impactWake turbulence0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereInstitut für Physik der AtmosphäreNephelometerIce crystalsAtmosphärische SpurenstoffeRadiative forcinglcsh:QC1-999FalconVortexlcsh:QD1-99913. Climate actionEnvironmental sciencePolarlcsh:Physics
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Reply to a comment by R. Brown on ‘a numerical model of the cloud‐topped planetary boundary‐layer: Radiation, turbulence and spectral microphysics in…

1997

Atmospheric ScienceCloud microphysicsMarine boundary layerMeteorologyMicrophysicsTurbulencePlanetary boundary layerbusiness.industryCloud computingRadiationAtmospheric sciencesbusinessGeologyQuarterly Journal of the Royal Meteorological Society
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A Wind Tunnel Study of Turbulence Effects on the Scavenging of Aerosol Particles by Water Drops

2001

Abstract Laboratory experiments are described where the effects of turbulence on the impaction scavenging of aerosol particles by water drops were investigated. During the experiments the drops were freely suspended at their terminal velocities in the Mainz vertical wind tunnel. Turbulence in the tunnel airstream was produced by placing a needle obstruction upstream of the floating drop. The energy dissipation rates e were between 0.03 and 0.5 m2 s−3. The power spectrum covered a range of k values between 102 and 3 × 103 m−1, agreeing with atmospheric observations within this range. Collector drops of 346-μm, 1.68-mm, and 2.88-mm radius were exposed to indium acetylacetonate aerosol particl…

Atmospheric ScienceMaterials scienceTurbulencebusiness.industryDrop (liquid)Laminar flowRadiusMechanicsAerosolchemistry.chemical_compoundOpticschemistryIndium acetylacetonatebusinessScavengingWind tunnelJournal of the Atmospheric Sciences
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A numerical model of the cloud-topped planetary boundary-layer: Radiation, turbulence and spectral microphysics in marine stratus

1996

A numerical model of the cloud-topped planetary boundary-layer is presented. The model is one-dimensional with special emphasis on a detailed description of cloud microphysical processes. Aerosols and cloud droplets are treated in a two-dimensional particle-distribution whereby the activation of aerosols is calculated explicitly by solving the droplet-growth equation at all relative humidities. Atmospheric radiation is determined with a δ-two-stream radiation scheme. Turbulent fluxes are parametrized as a function of the turbulent kinetic energy. Numerical results are presented which are obtained by utilizing measurements made over the North Sea. The interaction between radiation, turbulenc…

Atmospheric ScienceMicrophysicsComputer simulationMeteorologyPlanetary boundary layerTurbulencebusiness.industryCloud computingRadiationComputational physicsTurbulence kinetic energyEnvironmental sciencebusinessNorth seaPhysics::Atmospheric and Oceanic PhysicsQuarterly Journal of the Royal Meteorological Society
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The importance of stratospheric–tropospheric transport in affecting surface ozone concentrations in the western and northern tier of the United States

2011

Stratospheric–tropospheric exchange (STE) processes contribute at both high and low-elevation monitoring sites to background ozone (O3) concentrations. This study addresses the importance of stratospheric intrusions contributing to enhanced hourly average surface O3 concentrations (i.e., ≥50 ppb) at 12 O3 monitoring stations in the western and northern tier of the US for 2006, 2007, and 2008. The Lagrangian Analysis Tool (LAGRANTO) trajectory model identified specific days when stratosphere-to-troposphere transport was optimal to elevate surface O3 levels. The coincidences between the number of days with a daily maximum hourly average O3 concentration ≥ 50 ppb and stratosphere-to-tropospher…

Atmospheric ScienceOzoneAdvectionBoundary layer turbulenceMesoscale meteorologyElevationAtmospheric sciencesTropospherechemistry.chemical_compoundSurface ozonechemistryClimatologyEnvironmental scienceGeneral Environmental ScienceAtmospheric Environment
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Coexistence of single-mode and multi-longitudinal mode emission in the ring laser model

2005

A homogeneously broadened unidirectonal ring laser can emit in several longitudinal modes for large enough pump and cavity length because of Rabi splitting induced gain. This is the so called Risken-Nummedal-Graham-Haken (RNGH) instability. We investigate numerically the properties of the multi-mode solution. We show that this solution can coexist with the single-mode one, and its stability domain can extend to pump values smaller than the critical pump of the RNGH instability. Morevoer, we show that the multi-mode solution for large pump values is affected by two different instabilities: a pitchfork bifurcation, which preserves phase-locking, and a Hopf bifurcation, which destroys it.

BistabilityFOS: Physical sciencesPhysics::OpticsRing laserInstabilityOptical bistabilityLongitudinal modesymbols.namesakeINSTABILITIESOpticsElectrical and Electronic EngineeringPhysical and Theoretical ChemistryHopf bifurcationPhysicsbusiness.industrySingle-mode optical fiberNonlinear Sciences - Chaotic DynamicsAtomic and Molecular Physics and OpticsPULSESElectronic Optical and Magnetic MaterialsPitchfork bifurcationsymbolsTURBULENCEChaotic Dynamics (nlin.CD)businessOptics (physics.optics)Physics - Optics
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