Search results for "PLASMA"

showing 10 items of 4043 documents

Energy-loss straggling of 2-10 MeV/u Kr ions in gases

2013

Measurements have been performed on a time-of-flight setup at the Jyväskylä K130 cyclotron, aiming at energy-loss straggling of heavy ions in gases. Theoretical predictions based on recently developed theory as well as an empirical interpolation formula predict that straggling can be more than ten times higher than Bohr straggling in the MeV/u regime. Our measurements with up to 9.3 MeV/u Kr ions on He, N2, Ne and Kr targets confirm this feature. Our calculations show the relative contributions of linear straggling, bunching including packing, and charge exchange. Our results for stopping cross sections are compatible with values from the literature. Funding Agencies|EU||Academy of Finland …

PhysicsEnergy lossCyclotronPhysics::Medical Physics7. Clean energy01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmaslaw.inventionIonBohr modelNuclear physicssymbols.namesakelawAtomic and Molecular CollisionsTeknik och teknologier0103 physical sciencessymbolsEngineering and TechnologyAtomic physics010306 general physicsAtomien ja molekyylien törmäyksetCharge exchange
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Beyond the Vegard's law: solid mixing excess volume and thermodynamic potentials prediction, from end-members

2020

Abstract A method has been developed, herein presented, to model binary solid solutions' volume, enthalpy and Gibbs energy using the energy state functions, E ( V , S ) , of the end-members only. The E ( V , S ) s are expanded around an unknown mixing volume, V Mix , and the fundamental equilibrium equation − ( ∂ E / ∂ V ) S = P is used to determine V Mix . V Mix allows us to model enthalpy, straightforwardly. The same argument holds using Helmholtz energy, F ( V , T ) , in place of E ( V , S ) , and the equilibrium equation becomes − ( ∂ F / ∂ V ) T = P . One can readily determine the Gibbs free energy, too. The method presented remarkably simplifies computing of solid mixings' thermodynam…

PhysicsEnthalpyGeneral Physics and AstronomyThermodynamicsComputer simulation01 natural sciences010305 fluids & plasmasThermodynamic potentialGibbs free energysymbols.namesakeVolume (thermodynamics)Vegard's lawNitride materialHelmholtz free energy0103 physical sciencessymbols010306 general physicsMetals and alloyThermodynamic modelingMixing (physics)Solid solution
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A generalization of the Carnahan–Starling approach with applications to four- and five-dimensional hard spheres

2018

Abstract Development of good equations of state for hard spheres is an important task in the study of real fluids. In a way consistent with other theoretical results, we generalize the famous Carnahan–Starling approach for arbitrary dimensions and apply it to four- and five-dimensional hard spheres. We obtain simple and integer representations for virial coefficients of lower orders and accurate equations of state. Since theoretically and practically validated, these results improve understanding of hard sphere fluids.

PhysicsEquation of stateGeneralizationGeneral Physics and AstronomyHard spheres01 natural sciences010305 fluids & plasmasVirial coefficientSimple (abstract algebra)0103 physical sciencesDevelopment (differential geometry)Statistical physics010306 general physicsInteger (computer science)Physics Letters A
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The screened cluster equation of state for hydrogen-helium mixtures: Atomic, molecular, and ionic contributions from first principles

2018

International audience

PhysicsEquation of stateHydrogenIonic bondingThermodynamicschemistry.chemical_elementCondensed Matter Physics01 natural sciences010305 fluids & plasmasVirial coefficientchemistry0103 physical sciencesBound stateCluster (physics)010306 general physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HeliumComputingMilieux_MISCELLANEOUS
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Comment on "Direct linear term in the equation of state of plasmas"

2015

In a recent paper [Phys. Rev. E 91, 013108 (2015)], Kraeft et al. criticize known exact results on the equation of state of quantum plasmas, which have been obtained independently by several authors. They argue about a difference in the definition of the direct two-body function Q(x), which appears in virial expansions of thermodynamical quantities, but Q(x) is not a measurable quantity in itself. Differences in definitions of intermediate quantities are irrelevant, and only differences in physical quantities are meaningful. Beyond Kraeft et al.'s broad statement that there is no agreement at order ρ(5/2) in the virial equation for the pressure, we show that their published results for this…

PhysicsEquation of stateLinear termQuantum mechanicsOrder (group theory)PlasmaFunction (mathematics)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]QuantumVirial theoremComputingMilieux_MISCELLANEOUSPhysical quantityMathematical physics
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Lifetime Studies in Traps

2009

A knowledge of the radiative lifetimes of excited atomic states is of wide interest, not only in the detailed understanding of intrinsic atomic structure and dynamics but also in the fields of plasma diagnostics and astrophysics. The transition rates of intercombination and electric-dipole forbidden lines are of particular importance, since their low transition probability gives them long optical depths in plasmas and astrophysical environments.

PhysicsExcited stateMetastabilityRadiative transferPlasma diagnosticsPhysics::Atomic PhysicsPlasmaIon trapAtomic physics
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A multispacecraft analysis of a small-scale transient entrained by solar wind streams

2009

The images taken by the Heliospheric Imagers (HIs), part of the SECCHI imaging package onboard the pair of STEREO spacecraft, provide information on the radial and latitudinal evolution of the plasma compressed inside corotating interaction regions (CIRs). A plasma density wave imaged by the HI instrument onboard STEREO-B was found to propagate towards STEREO-A, enabling a comparison between simultaneous remote-sensing and in situ observations of its structure to be performed. In situ measurements made by STEREO-A show that the plasma density wave is associated with the passage of a CIR. The magnetic field compressed after the CIR stream interface (SI) is found to have a planar distribution…

PhysicsExtraterrestrial Physics Space SciencesOrbital planecoronal mass ejection [Interplanetary medium]PhysicsStellar magnetic fieldAstronomyFluxAstronomy and AstrophysicsPlasmaAstrophysicsMagnetic fieldComputational physicsMeteorology/ClimatologySolar windSpace and Planetary SciencePhysics::Space Physicsmagnetic field [Sun]Astrophysics::Solar and Stellar AstrophysicsHeliospheric current sheetMagnetic cloudAstrophysics::Earth and Planetary Astrophysicscorotating interaction regions [Sun]
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HINODE /EIS SPECTROSCOPIC VALIDATION OF VERY HOT PLASMA IMAGED WITH THE SOLAR DYNAMICS OBSERVATORY IN NON-FLARING ACTIVE REGION CORES

2012

We use coronal imaging observations with SDO/AIA, and Hinode/EIS spectral data, to explore the potential of narrow band EUV imaging data for diagnosing the presence of hot (T >~5MK) coronal plasma in active regions. We analyze observations of two active regions (AR 11281, AR 11289) with simultaneous AIA imaging, and EIS spectral data, including the CaXVII line (at 192.8A) which is one of the few lines in the EIS spectral bands sensitive to hot coronal plasma even outside flares. After careful coalignment of the imaging and spectral data, we compare the morphology in a 3 color image combining the 171, 335, and 94A AIA spectral bands, with the image obtained for CaXVII emission from the an…

PhysicsExtreme ultraviolet lithographyImaging spectrometerGamma rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaSpectral bandsSpectral lineSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceTemporal resolutionSolar and Stellar Astrophysics (astro-ph.SR)Sun: activity Sun: corona Sun: UV radiation Sun: X-rays gamma rays techniques: imaging spectroscopyLine (formation)The Astrophysical Journal
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On the Measurements of Numerical Viscosity and Resistivity in Eulerian MHD Codes

2016

We propose a simple ansatz for estimating the value of the numerical resistivity and the numerical viscosity of any Eulerian MHD code. We test this ansatz with the help of simulations of the propagation of (magneto)sonic waves, Alfven waves, and the tearing mode instability using the MHD code Aenus. By comparing the simu- lation results with analytical solutions of the resistive-viscous MHD equations and an empirical ansatz for the growth rate of tearing modes we measure the numerical viscosity and resistivity of Aenus. The comparison shows that the fast-magnetosonic speed and wavelength are the characteristic velocity and length, respectively, of the aforementioned (relatively simple) syst…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsEulerian pathMechanicsCharacteristic velocity01 natural sciencesNumerical resistivityRiemann solver010305 fluids & plasmassymbols.namesakeViscosityAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetorotational instability0103 physical sciencessymbolsMagnetohydrodynamicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)AnsatzThe Astrophysical Journal Supplement Series
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Influence of electromagnetic boundary conditions onto the onset of dynamo action in laboratory experiments

2009

We study the onset of dynamo action of the Riga and Karlsruhe experiments with the addition of an external wall, the electro-magnetic properties of which being different from those of the fluid in motion. We consider a wall of different thickness, conductivity and permeability. We also consider the case of a ferro-fluid in motion.

PhysicsFerrofluid[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Mechanics of the fluids [physics.class-ph][SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Fluid Dynamics (physics.flu-dyn)FOS: Physical sciences[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Physics - Fluid DynamicsConductivity01 natural sciences010305 fluids & plasmas[SPI.MECA.MEFL]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph]Physics::GeophysicsGeophysics (physics.geo-ph)Physics - GeophysicsPhysics::Fluid DynamicsClassical mechanicsPermeability (electromagnetism)0103 physical sciencesBoundary value problem[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph]010306 general physicsDynamo
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