Search results for "PLASMA"

showing 10 items of 4043 documents

Laboratory evidence for proton energization by collisionless shock surfing

2021

Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite increasing efforts in the characterization of these shocks from satellite measurements at Earth’s bow shock as well as powerful numerical simulations, the underlying acceleration mechanism or a combination thereof is still widely debated. Here we show that astrophysically relevant super-critical quasi-perpendicular magnetized collisionless shocks can be produced and characterized in the laboratory. We observe the characteristics of super-criticali…

Shock waveProtonAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesAccelerationSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBow shock (aerodynamics)010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsMechanicsplasmasPhysics - Plasma PhysicsCharged particleComputer Science::Computers and Society[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Magnetic fieldShock (mechanics)Plasma Physics (physics.plasm-ph)Supernova13. Climate actionPhysics::Space PhysicsPhysics::Accelerator Physics
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Hydrodynamic Modeling of Accretion Impacts in Classical T Tauri Stars: Radiative Heating of the Pre-shock Plasma

2016

Context. It is generally accepted that, in classical T Tauri stars, the plasma from the circumstellar disc accretes onto the stellar surface with free-fall velocity and the impact generates a shock. The impact region is expected to contribute to emission in different spectral bands; many studies have confirmed that the X-rays arise from the post-shock plasma but, otherwise, there are no studies in the literature investigating the origin of the observed UV emission which is apparently correlated to accretion. Aims: We investigated the effect of radiative heating of the infalling material by the post-shock plasma at the base of the accretion stream, with the aim to identify in which region a …

Shock waveRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAccretion accretion diskSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsX-rays: starIrradiationEmission spectrum010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsHydrodynamicPlasmaAstronomy and AstrophysicThermal conductionAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsShock waveSpace and Planetary ScienceStars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysics
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Metastable oxygen atom velocity and temperature in supersonic CO2plasma expansions

2008

Radial and axial velocity distribution functions of metastable oxygen atoms were obtained by way of resonant laser induced fluorescence spectroscopy at 777.19 nm in rarefied supersonic plasma jets produced from pure CO2 and CO2–N2 gas mixtures. The N2 seeded fraction is 3% in volume in order to mimic the Martian atmosphere composition. The measured lineshapes allow computation of the mean radial velocity and the perpendicular temperature, with respect to the jet axis, as well as the mean axial velocity and the parallel temperature. With an arcjet plasma source input power of 6.5 kW, the metastable O(5S) atom axial velocity is around 4500 m s−1 and the atom perpendicular temperature reaches …

Shock waveThermal equilibriumJet (fluid)Acoustics and UltrasonicsChemistryPlasmaCondensed Matter PhysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsRadial velocityDistribution functionAtomSupersonic speedAtomic physicsJournal of Physics D: Applied Physics
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Spectral long-range interaction of temporal incoherent solitons.

2014

We study the interaction of temporal incoherent solitons sustained by a highly noninstantaneous (Raman-like) nonlinear response. The incoherent solitons exhibit a nonmutual interaction, which can be either attractive or repulsive depending on their relative initial distance. The analysis reveals that incoherent solitons exhibit a long-range interaction in frequency space, which is in contrast with the expected spectral short-range interaction described by the usual approach based on the Raman-like spectral gain curve. Both phenomena of anomalous interaction and spectral long-range behavior of incoherent solitons are described in detail by a long-range Vlasov equation.

Shock waveWave propagationIncoherent scatter01 natural sciences010305 fluids & plasmassymbols.namesakeOptics[ MATH.MATH-AP ] Mathematics [math]/Analysis of PDEs [math.AP][NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Quantum mechanics0103 physical sciences[MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP][ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]010306 general physicsDispersion (water waves)ComputingMilieux_MISCELLANEOUSPhysicsbusiness.industrystatistical opticsVlasov equationAtomic and Molecular Physics and Optics[MATH.MATH-PR]Mathematics [math]/Probability [math.PR]Nonlinear systemsymbolsbusiness[ MATH.MATH-PR ] Mathematics [math]/Probability [math.PR]Raman scatteringCoherence (physics)Optics letters
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High-order regularization in lattice-Boltzmann equations

2017

A lattice-Boltzmann equation (LBE) is the discrete counterpart of a continuous kinetic model. It can be derived using a Hermite polynomial expansion for the velocity distribution function. Since LBEs are characterized by discrete, finite representations of the microscopic velocity space, the expansion must be truncated and the appropriate order of truncation depends on the hydrodynamic problem under investigation. Here we consider a particular truncation where the non-equilibrium distribution is expanded on a par with the equilibrium distribution, except that the diffusive parts of high-order nonequilibrium moments are filtered, i.e., only the corresponding advective parts are retained afte…

Shock waverecurrence relationspolynomialsComputational MechanicsLattice Boltzmann methods114 Physical sciences01 natural sciences010305 fluids & plasmassubspaces0103 physical sciences010306 general physicsFluid Flow and Transfer ProcessesPhysicstensor methods: shock tubesHermite polynomialsRecurrence relationta114AdvectionMechanical EngineeringpolynomitMathematical analysisCondensed Matter PhysicsDistribution functionMechanics of MaterialsRegularization (physics)shock tubes [tensor methods]Shear flowPhysics of Fluids
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Impact of self-steepening on incoherent dispersive spectral shocks and collapse-like spectral singularities

2014

International audience; Incoherent dispersive shock waves and collapselike singularities have been recently predicted to occur in the spectral evolution of an incoherent optical wave that propagates in a noninstantaneous nonlinear medium. Here we extend this work by considering the generalized nonlinear Schrödinger equation. We show that self-steepening significantly affects these incoherent spectral singularities: (i) It leads to a delay in the development of incoherent dispersive shocks, and (ii) it arrests the incoherent collapse singularity. Furthermore, we show that the spectral collapselike behavior can be exploited to achieve a significant enhancement (by two orders of magnitudes) of…

Shock wavespecklesIncoherent scatterDegree of coherencespeckles steepening shock waves01 natural sciencesNO010305 fluids & plasmasSingularity[ MATH.MATH-AP ] Mathematics [math]/Analysis of PDEs [math.AP][NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Quantum mechanicsNonlinear medium0103 physical sciences[MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP][ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]010306 general physicsPhysicsstatistical opticsshock wavesAtomic and Molecular Physics and Optics[MATH.MATH-PR]Mathematics [math]/Probability [math.PR]Nonlinear systemQuantum electrodynamicsGravitational singularitysteepening[ MATH.MATH-PR ] Mathematics [math]/Probability [math.PR]Coherence (physics)
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Laboratory evidence for asymmetric accretion structure upon slanted matter impact in young stars

2020

Aims. Investigating the process of matter accretion onto forming stars through scaled experiments in the laboratory is important in order to better understand star and planetary system formation and evolution. Such experiments can indeed complement observations by providing access to the processes with spatial and temporal resolution. A previous investigation revealed the existence of a two-component stream: a hot shell surrounding a cooler inner stream. The shell was formed by matter laterally ejected upon impact and refocused by the local magnetic field. That laboratory investigation was limited to normal incidence impacts. However, in young stellar objects, the complex structure of magne…

Shock wavestarsAccretionMagnetohydrodynamics (MHD)Young stellar objectFOS: Physical sciencesX-rays: starsAstrophysics01 natural sciencesShock wavesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsEjecta010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicspre-main sequence -X-raysAstronomy and AstrophysicsPlasmaPlanetary system[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]accretion disks -instabilities -magnetohydrodynamics (MHD) -shock waves -starsAccretion (astrophysics)StarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceInstabilitiesAccretion disksStars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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INVESTIGATIONS ON ‘CANDIDATUS PHYTOPLASMA SOLANI’ IN WESTERN SICILY, SOUTHERN ITALY

2016

‘Candidatus Phytoplasma solani’, belonging to the 16SrXII-A subgroup, is associated with grapevine Bois Noir (BN). It is usually transmitted by Hyalesthes obsoletus from a wide range of weeds to grapevine, which is considered a dead-end host. Moreover, other alternative vectors can play a role in the epidemiology of the disease. In Sicily, the presence of BN was reported in 1996, both on typical and on newly introduced cultivars. Furthermore, high BN incidence was observed on native grape cultivars grown close to ‘Chardonnay’ vineyards. In summer 2014 and 2015, the spread and the severity of BN were recorded in a 10 year-old vineyard located in San Giuseppe Jato (PA, Western Sicily), grown …

Sicily Vitis vinifera Candidatus Phytoplasma SolaniSettore AGR/12 - Patologia Vegetale
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The classical two-dimensional Heisenberg model revisited: An $SU(2)$-symmetric tensor network study

2021

The classical Heisenberg model in two spatial dimensions constitutes one of the most paradigmatic spin models, taking an important role in statistical and condensed matter physics to understand magnetism. Still, despite its paradigmatic character and the widely accepted ban of a (continuous) spontaneous symmetry breaking, controversies remain whether the model exhibits a phase transition at finite temperature. Importantly, the model can be interpreted as a lattice discretization of the $O(3)$ non-linear sigma model in $1+1$ dimensions, one of the simplest quantum field theories encompassing crucial features of celebrated higher-dimensional ones (like quantum chromodynamics in $3+1$ dimensio…

Sigma modelSpontaneous symmetry breakingQC1-999Lattice (group)General Physics and AstronomyFOS: Physical sciencesClassical Heisenberg modelQuantum Materials53001 natural sciences010305 fluids & plasmasTheoretical physicsHigh Energy Physics - Lattice0103 physical sciencesSymmetric tensorTensorQuantum field theory010306 general physicsclassical Heisenberg modelCondensed Matter - Statistical MechanicsPhysicsQuantum PhysicsStatistical Mechanics (cond-mat.stat-mech)Heisenberg modelPhysics500 Naturwissenschaften und Mathematik::530 Physik::530 PhysikHigh Energy Physics - Lattice (hep-lat)magnetismstatistical and condensed matter physicsQuantum Physics (quant-ph)
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Radial properties of high-frequency electrodeless lamps in argon–mercury mixtures

2005

Radial emission properties of high-frequency electrodeless discharge lamps (HFEDLs) in argon–mercury mixtures are investigated both numerically and experimentally. The radial profile of the intensities of the mercury triplet lines 404.7, 435.8 and 546.1 nm are measured for two different values of the high frequency generator power. A model describing physical processes in an HFEDL, including the calculation of radial plasma parameters, is developed. Radial intensity dependences of the lines 404.7, 435.8 and 546.1 nm are calculated and are found to be in good agreement with the experimental measurements.

Signal generatorArgonGas-discharge lampAcoustics and UltrasonicsPlasma parametersAnalytical chemistrychemistry.chemical_elementCondensed Matter PhysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialslaw.inventionMercury (element)chemistrylawAtomic physicsJournal of Physics D: Applied Physics
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