Search results for "Asma"

showing 10 items of 4204 documents

RadioAstron reveals a spine-sheath jet structure in 3C 273

2021

We present Space-VLBI RadioAstron observations at 1.6 GHz and 4.8 GHz of the flat spectrum radio quasar 3C 273, with detections on baselines up to 4.5 and 3.3 Earth Diameters, respectively. Achieving the best angular resolution at 1.6 GHz to date, we have imaged limb-brightening in the jet, not previously detected in this source. In contrast, at 4.8 GHz, we detected emission from a central stream of plasma, with a spatial distribution complementary to the limb-brightened emission, indicating an origin in the spine of the jet. While a stratification across the jet width in the flow density, internal energy, magnetic field, or bulk flow velocity are usually invoked to explain the limb-brighte…

Astrophysics::High Energy Astrophysical PhenomenaStratification (water)FOS: Physical sciencesJets [Galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesQuasars: individual: 3C 2730103 physical sciencesAngular resolution010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsJet (fluid)Internal energy010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarPlasmaGalaxies: activeAstrophysics - Astrophysics of GalaxiesActive [Galaxies]Magnetic fieldFlow velocitySpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsIndividual: 3C 273 [Quasars]
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YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission

2013

Context. Theoretical arguments and numerical simulations of radiative shocks produced by the impact of the accreting gas onto young stars predict quasi-periodic oscillations in the emitted radiation. However, observational data do not show evidence of such periodicity. Aims. We investigate whether physically plausible perturbations in the accretion column or in the chromosphere could disrupt the shock structure influencing the observability of the oscillatory behavior. Methods. We performed local 2D magneto-hydrodynamical simulations of an accretion shock impacting a chromosphere, taking optically thin radiation losses and thermal conduction into account. We investigated the effects of seve…

Astrophysics::High Energy Astrophysical Phenomenaaccretion accretion disks magnetohydrodynamics (MHD) radiative transfer shock waves instabilitiesFOS: Physical sciencesPerturbation (astronomy)Astrophysics01 natural sciencesmagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsaccretion disksAstronomy and AstrophysicsObservablePlasmashock wavesThermal conductionMagnetic fieldAmplitudeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Scienceradiative transferinstabilities[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Measurement of the Groomed Jet Radius and Momentum Splitting Fraction in pp and Pb-Pb Collisions at √sNN = 5.02 TeV

2022

This article presents groomed jet substructure measurements in pp and Pb−Pb collisions at √sNN = 5.02 TeV with the ALICE detector. The soft drop grooming algorithm provides access to the hard parton splittings inside a jet by removing soft wide-angle radiation. We report the groomed jet momentum splitting fraction, zg, and the (scaled) groomed jet radius, θg. Charged-particle jets are reconstructed at midrapidity using the anti-kT algorithm with resolution parameters R=0.2 and R=0.4. In heavy-ion collisions, the large underlying event poses a challenge for the reconstruction of groomed jet observables, since fluctuations in the background can cause groomed parton splittings to be misidentif…

Astrophysics::High Energy Astrophysical Phenomenakvarkki-gluoniplasmaHigh Energy Physics::ExperimenthiukkasfysiikkaNuclear Experiment
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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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Intermittent release of transients in the slow solar wind: 1. Remote sensing observations

2010

[1] The Heliospheric Imager (HI) instruments on board the STEREO spacecraft are used to analyze the solar wind during August and September 2007. We show how HI can be used to image the streamer belt and, in particular, the variability of the slow solar wind which originates inside and in the vicinity of the streamer belt. Intermittent mass flows are observed in HI difference images, streaming out along the extension of helmet streamers. These flows can appear very differently in images: plasma distributed on twisted flux ropes, V-shaped structures, or “blobs.” The variety of these transient features may highlight the richness of phenomena that could occur near helmet streamers: emergence of…

Atmospheric ScienceAstrophysics::High Energy Astrophysical PhenomenaSoil ScienceFluxInterplanetary mediumAquatic ScienceOceanographyPhysics::Plasma PhysicsGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Astrophysics::Solar and Stellar AstrophysicsInterplanetary magnetic fieldEjectaEarth-Surface ProcessesWater Science and TechnologyPhysicsEcologyPaleontologyAstronomyForestryHelmet streamerCoronaSolar windGeophysicsSpace and Planetary SciencePhysics::Space PhysicsOutflowAstrophysics::Earth and Planetary AstrophysicsJournal of Geophysical Research: Space 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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