Search results for "plasmas"

showing 10 items of 1475 documents

Properties of the Binary Neutron Star Merger GW170817

2019

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data. We extend the range of gravitational-wave frequencies considered down to 23 Hz, compared to 30 Hz in the initial analysis. We also compare results inferred using several signal models, which ar…

AstrofísicaGravitacióneutron star: binaryAstronomyGeneral Physics and AstronomyBinary numberAstrophysicsELECTROMAGNETIC COUNTERPARTspin01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESlocalization010305 fluids & plasmasGravitational wave detectorsEQUATIONenergy: densityLIGOGEO600QCastro-ph.HESettore FIS/01PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSSettore FIS/05PhysicsEquations of stateGravitational effectsGravitational-wave signalsDeformability parameterAmplitudePhysical SciencesPhysical effectsINSPIRALING COMPACT BINARIES[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Spectral energy densityAstrophysics - High Energy Astrophysical PhenomenaPARAMETER-ESTIMATIONBinary neutron starsdata analysis methodgr-qcQC1-999Physics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesBayesianGravimeterselectromagnetic field: productionPhysics and Astronomy (all)galaxy: binary0103 physical sciencesddc:530SDG 7 - Affordable and Clean Energy010306 general physicsgravitational radiation: frequencySTFCAstrophysics::Galaxy Astrophysicsequation of stateLIGHT CURVESEquation of stateScience & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energySpinsgravitational radiationRCUKSpectral densityKILONOVATRANSIENTSbinary: compactStarsGEO600GalaxyLIGOgravitational radiation detectorNeutron starVIRGOPhysics and Astronomygravitational radiation: emissionRADIATIONBayesian AnalysisDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Efficient generation of energetic ions in multi-ion plasmas by radio-frequency heating

2017

We describe a new technique for the efficient generation of high-energy ions with electromagnetic ion cyclotron waves in multi-ion plasmas. The discussed ‘three-ion’ scenarios are especially suited for strong wave absorption by a very low number of resonant ions. To observe this effect, the plasma composition has to be properly adjusted, as prescribed by theory. We demonstrate the potential of the method on the world-largest plasma magnetic confinement device, JET (Joint European Torus, Culham, UK), and the high-magnetic-field tokamak Alcator C-Mod (Cambridge, USA). The obtained results demonstrate efficient acceleration of 3He ions to high energies in dedicated hydrogen–deuterium mixtures.…

Astrophysical plasmasTokamakradio-frequency heatingCyclotronJoint European TorusPlasma heatingGeneral Physics and AstronomyFREQUENCY114 Physical sciences01 natural sciences7. Clean energyMagnetically confined plasmas010305 fluids & plasmaslaw.inventionIonPHYSICSPhysics and Astronomy (all)FUSIONMODE CONVERSIONlawPhysics::Plasma Physics0103 physical sciencesDielectric heating010306 general physicsPhysics[PHYS]Physics [physics]ta114Solar flare:Física [Àrees temàtiques de la UPC]Plasma dynamicsmulti-ion plasmasSettore FIS/01 - Fisica SperimentaleMagnetic confinement fusionPlasmaHE-3-RICH SOLAR-FLARESTècniques de plasmaJETCYCLOTRON RANGETOKAMAKPhysics::Space PhysicsAtomic physicsHE-3-RICH SOLAR-FLARES; MODE CONVERSION; CYCLOTRON RANGE; FUSION; JET; FREQUENCY; TOKAMAK; PHYSICS
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Observation of Poincaré-Andronov-Hopf Bifurcation in Cyclotron Maser Emission from a Magnetic Plasma Trap.

2018

We report the first experimental evidence of a controlled transition from the generation of periodic bursts of electromagnetic radiation into the continuous-wave regime of a cyclotron maser formed in magnetically confined nonequilibrium plasma. The kinetic cyclotron instability of the extraordinary wave of weakly inhomogeneous magnetized plasma is driven by the anisotropic electron population resulting from electron cyclotron plasma heating in a MHD-stable minimum-$B$ open magnetic trap.

Astrophysics::High Energy Astrophysical PhenomenaCyclotronGeneral Physics and AstronomyElectronplasmafysiikka01 natural sciences7. Clean energyInstabilityElectromagnetic radiation010305 fluids & plasmaslaw.inventionsymbols.namesakePhysics::Plasma PhysicslawMagnetic trap0103 physical sciencesMaser010306 general physicsPhysicsHopf bifurcationta114plasma physicssyklotronitPlasmaPhysics::Space PhysicssymbolsAtomic physicscyclotronsPhysical review letters
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Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars

2013

(abridged) AIMS. We investigate the dynamics and stability of post-shock plasma streaming along nonuniform stellar magnetic fields at the impact region of accretion columns. We study how the magnetic field configuration and strength determine the structure, geometry, and location of the shock-heated plasma. METHODS. We model the impact of an accretion stream onto the chromosphere of a CTTS by 2D axisymmetric magnetohydrodynamic simulations. Our model takes into account the gravity, the radiative cooling, and the magnetic-field-oriented thermal conduction. RESULTS. The structure, stability, and location of the shocked plasma strongly depend on the configuration and strength of the magnetic f…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField strengthX-rays: starsAstrophysicsstars: pre-main sequence01 natural sciencesmagnetohydrodynamics (MHD)pre-main sequence X-rays: stars [accretion accretion disks instabilities magnetohydrodynamics (MHD) shock waves stars]010305 fluids & plasmasSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsaccretion disksAstronomy and AstrophysicsPlasmashock wavesAccretion (astrophysics)Magnetic fieldT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesPhysics::Space PhysicsOblique shockAstrophysics::Earth and Planetary Astrophysicsaccretion accretion disks instabilities magnetohydrodynamics (MHD) shock waves stars: pre-main sequence X-rays: stars[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Analysis of a jet stream induced gravity wave associated with an observed ice cloud over Greenland

2004

International audience; A polar stratospheric ice cloud (PSC type II) was observed by airborne lidar above Greenland on 14 January 2000. It was the unique observation of an ice cloud over Greenland during the SOLVE/THESEO 2000 campaign. Mesoscale simulations with the hydrostatic HRM model are presented which, in contrast to global analyses, are capable to produce a vertically propagating gravity wave that induces the low temperatures at the level of the PSC afforded for the ice formation. The simulated minimum temperature is ~8 K below the driving analyses and ~4.5 K below the frost point, exactly coinciding with the location of the observed ice cloud. Despite the high elevations of the Gre…

Atmospheric Science010504 meteorology & atmospheric sciences010502 geochemistry & geophysicsAtmospheric sciences01 natural sciences010305 fluids & plasmaslaw.inventionPhysics::Geophysicslcsh:Chemistrylaw0103 physical sciencesGravity wavePhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereJet (fluid)Ice cloud[SDU.OCEAN] Sciences of the Universe [physics]/Ocean AtmosphereOrographyJet streamlcsh:QC1-999lcsh:QD1-99913. Climate actionHydrostatic equilibriumTropopauselcsh:PhysicsGeologyGeostrophic wind
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What Flow Conditions are Conducive to Banner Cloud Formation?

2016

Abstract Banner clouds are clouds that are attached to the leeward slope of a steep mountain. Their formation is essentially due to strong Lagrangian uplift of air in the lee of the mountain. However, little is known about the flow regime in which banner clouds can be expected to occur. The present study addresses this question through numerical simulations of flow past idealized orography. Systematic sets of simulations are carried out exploring the parameter space spanned by two dimensionless numbers, which represent the aspect ratio of the mountain and the stratification of the flow. The simulations include both two-dimensional flow past two-dimensional orography and three-dimensional fl…

Atmospheric Science010504 meteorology & atmospheric sciencesAtmospheric circulationStratification (water)OrographyMechanicsParameter spaceAtmospheric sciences01 natural sciences010305 fluids & plasmasBoundary layerFlow separationFlow conditions0103 physical sciencesGeology0105 earth and related environmental sciencesDimensionless quantityJournal of the Atmospheric Sciences
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Mountain waves modulate the water vapor distribution in the UTLS

2017

Abstract. The water vapor distribution in the upper troposphere–lower stratosphere (UTLS) region has a strong impact on the atmospheric radiation budget. Transport and mixing processes on different scales mainly determine the water vapor concentration in the UTLS. Here, we investigate the effect of mountain waves on the vertical transport and mixing of water vapor. For this purpose we analyze measurements of water vapor and meteorological parameters recorded by the DLR Falcon and NSF/NCAR Gulfstream V research aircraft taken during the Deep Propagating Gravity Wave Experiment (DEEPWAVE) in New Zealand. By combining different methods, we develop a new approach to quantify location, direction…

Atmospheric Science010504 meteorology & atmospheric sciencesTransportmountain wavesAtmospheric sciences01 natural sciences010305 fluids & plasmaslcsh:ChemistryTroposphere0103 physical sciencesUTLSGravity waveWolkenphysikDropsondeStratosphere0105 earth and related environmental sciencesVerkehrsmeteorologieRadiative forcinglcsh:QC1-999water vapourWavelengthlcsh:QD1-999ClimatologyEnvironmental scienceTropopauselcsh:PhysicsWater vapor
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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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Assessing the predictability of Medicanes in ECMWF ensemble forecasts using an object-based approach

2018

The predictability of eight southern European tropical-like cyclones, seven of which Medicanes, is studied evaluating ECMWF operational ensemble forecasts against operational analysis data. Forecast cyclone trajectories are compared to the cyclone trajectory in the analysis by means of a dynamic time warping technique, which allows to find a match in terms of their overall spatio-temporal similarity. Each storm is treated as an object and its forecasts are analysed using metrics that describe intensity, symmetry, compactness, and upper-level thermal structure. This object-based approach allows to focus on specific storm features, while tolerating their shifts in time and space to some exten…

Atmospheric ScienceDynamic time warping010504 meteorology & atmospheric sciencesMeteorologyFOS: Physical sciencesStorm01 natural sciences010305 fluids & plasmasPhysics - Atmospheric and Oceanic Physics0103 physical sciencesAtmospheric and Oceanic Physics (physics.ao-ph)Data analysisTrajectoryJumpCycloneEnvironmental sciencePredictabilityLead timePhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciences
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