Search results for "physics.plasm-ph"

showing 8 items of 48 documents

Caractérisation du plasma LIBS : réflexions, bonnes pratiques et conséquences analytiques

2022

International audience; La matrice d'un échantillon est définie par l'IUPAC (International Union of Pure and Applied Chemistry) comme les composants de l'échantillon autres que l'analyte. Et l'effet de matrice d'une technique analytique désignent alors l'effet combiné de tous les composants autres que l'analyte sur la mesure de sa quantité. Chose que l'on peut visualiser, par exemple, sur des droites d'étalonnage de pente différente pour différentes matrices. En LIBS, ces effets se traduisent physiquement par une interaction laser-surface et laser-plasma dépendant de la nature du matériau analysé, et induisant des variations de masse ablatée, de température et de densité électroniques d'un …

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][CHIM.ANAL] Chemical Sciences/Analytical chemistry[CHIM.ANAL]Chemical Sciences/Analytical chemistry[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph][PHYS.PHYS.PHYS-PLASM-PH] Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph][PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph][PHYS.PHYS.PHYS-CHEM-PH] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]
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Hyperfine structure of some near-infrared Xe I and Xe II lines

2011

International audience; This work reports on the experimental determination of the hyperfine splitting of the Xe I lines at 828.01 nm and 834.68 nm and the Xe II line at 834.72 nm. Measurements were performed by means of Doppler-free saturation spectroscopy in a low-pressure radio-frequency discharge. The absolute wavelength of all hyperfine components is obtained by way of a high-precision wavemeter backed-up with the absorption spectrum of the NO 2 molecule. We provide an accurate estimate of hyperfine constants for the lower level of the Xe II transition at 834.72 nm. The two Xe I transition outcomes of our experimental study are compared with data available in the literature.

[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Absorption spectroscopyNear-infrared spectroscopychemistry.chemical_element01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasAnalytical ChemistryWavelengthXenonchemistry[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]0103 physical sciencesAtomic physics010306 general physicsSpectroscopyInstrumentationSaturation (magnetic)Hyperfine structureSpectroscopyLine (formation)
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Nitric oxide production rate of pulsed nanosecond and microsecond discharge in atmospheric pressure air

2016

International audience

[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph][PHYS.PHYS.PHYS-PLASM-PH] Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]ComputingMilieux_MISCELLANEOUS
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Nonlinear electrostatic oscillations in a cold magnetized electron-positron plasma

2017

We study the spatio-temporal evolution of the nonlinear electrostatic oscillations in a cold magnetized electron-positron (e-p) plasma using both analytics and simulations. Using a perturbative method we demonstrate that the nonlinear solutions change significantly when a pure electrostatic mode is excited at the linear level instead of a mixed upper-hybrid and zero-frequency mode that is considered in a recent study. The pure electrostatic oscillations undergo phase mixing nonlinearly. However, the presence of the magnetic field significantly delays the phase-mixing compared to that observed in the corresponding unmagnetized plasma. Using 1D PIC simulations we then analyze the damping of t…

[PHYS]Physics [physics]PhysicsFOS: Physical sciencesElectronPlasmaCondensed Matter PhysicsPlasma oscillationLower hybrid oscillation01 natural sciencesPhysics - Plasma Physics010305 fluids & plasmasMagnetic fieldPlasma Physics (physics.plasm-ph)Two-stream instabilityPhysics::Plasma Physics[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Upper hybrid oscillation0103 physical sciencesAstrophysical plasmaAtomic physics010306 general physicsComputingMilieux_MISCELLANEOUSPhysics of Plasmas
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Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection

2020

Predicting the large-scale eruptions from the solar corona and their propagation through interplanetary space remains an outstanding challenge in solar- and helio-physics research. In this article, we describe three dimensional magnetohydrodynamic simulations of the inner heliosphere leading up to and including the extreme interplanetary coronal mass ejection (ICME) of 23 July 2012, developed using the code PLUTO. The simulations are driven using the output of coronal models for Carrington rotations 2125 and 2126 and, given the uncertainties in the initial conditions, are able to reproduce an event of comparable magnitude to the 23 July ICME, with similar velocity and density profiles at 1 …

astro-ph.SRSpace weather010504 meteorology & atmospheric sciencesMHDSolar windSTORMFOS: Physical sciencesMagnitude (mathematics)Context (language use)PROPAGATIONAstronomy & AstrophysicsDisturbancesSpace weatherPROTON01 natural sciencesEVENTSMagnetohydrodynamicsPhysics - Space Physicsphysics.plasm-ph0201 Astronomical and Space Sciences0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologySUNAstronomy and AstrophysicsARRIVALGeophysicsEVOLUTIONSpace Physics (physics.space-ph)Physics - Plasma PhysicsPlasma Physics (physics.plasm-ph)PlutoSolar windAstrophysics - Solar and Stellar Astrophysicsphysics.space-ph13. Climate actionSpace and Planetary ScienceDragPhysical Sciencesastro-ph.EPMagnetohydrodynamicsInterplanetary coronal mass ejectionsHeliosphereAstrophysics - Earth and Planetary AstrophysicsSolar Physics
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A comparative study of the behaviour of silver, copper and nickel submitted to a constant high power flux density

2005

In this paper, we present a numerical simulation of three metal cathode (silver, copper and nickel) submitted to a constant flux power flux density ranging between and . The goal is to compare the interface evolution (vaporization and liquefaction rate, appearance time of liquid and vapour, energetic repartition) to predict the behaviour of the cathodes during an electric arc.

cathodeanodePhysics::Instrumentation and Detectorschemistry.chemical_elementMineralogyFluxarc root01 natural sciences7. Clean energy010305 fluids & plasmaslaw.inventionElectric arclaw[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]0103 physical sciencesVaporizationComposite materialInstrumentation010302 applied physicsLiquefaction[ PHYS.PHYS.PHYS-PLASM-PH ] Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Condensed Matter PhysicsCopperArcCathodeElectronic Optical and Magnetic MaterialsAnodeNickelchemistryPhysics::Accelerator Physics
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Measurement of the energy distribution of electrons escaping minimum-B ECR plasmas

2017

The measurement of the electron energy distribution (EED) of electrons escaping axially from a minimum-B electron cyclotron resonance ion source (ECRIS) is reported. The experimental data were recorded with a room-temperature 14 GHz ECRIS at the JYFL accelerator laboratory. The electrons escaping through the extraction mirror of the ion source were detected with a secondary electron amplifier placed downstream from a dipole magnet serving as an electron spectrometer with 500 eV resolution. It was discovered that the EED in the range of 5–250 keV is strongly non-Maxwellian and exhibits several local maxima below 20 keV energy. It was observed that the most influential ion source operating pa…

electron energy distributionElectron spectrometerFOS: Physical sciencesElectronelektronitresonanssi01 natural sciences7. Clean energyElectron cyclotron resonanceSecondary electrons010305 fluids & plasmasmikroaallot0103 physical sciencesplasma010302 applied physicsPhysicsRange (particle radiation)energiaionitBremsstrahlungPlasmaCondensed Matter PhysicsIon sourcePhysics - Plasma PhysicsPlasma Physics (physics.plasm-ph)electrons escapingAtomic physics
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VUV emission spectroscopy combined with H- density measurements in the ion source Prometheus I

2016

“Prometheus I” is a volume H− negative ion source, driven by a network of dipolar electron cyclotron resonance (ECR; 2.45 GHz) modules. The vacuum-ultraviolet (VUV) emission spectrum of low-temperature hydrogen plasmas may be related to molecular and atomic processes involved directly or indirectly in the production of negative ions. In this work, VUV spectroscopy has been performed in the above source, Prometheus I, both in the ECR zones and the bulk (far from ECR zones and surfaces) plasma. The acquired VUV spectra are correlated with the negative ion densities, as measured by means of laser photodetachment, and the possible mechanisms of negative ion production are considered. The well-e…

plasmatekniikka01 natural sciences7. Clean energySpectral lineElectron cyclotron resonance010305 fluids & plasmasIonPhysics::Plasma Physics[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]0103 physical sciencesPhysics::Atomic and Molecular ClustersultraviolettisäteilyEmission spectrumvacuum-ultraviolet emissionSpectroscopy010302 applied physicsplasma sourcesta114ChemistrysyklotronitPlasmaIon sourceECR ion sourcesExcited stateAtomic physicsemissio (fysiikka)
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