Search results for "Plasma parameters"

showing 10 items of 20 documents

Plasma heating power dissipation in low temperature hydrogen plasmas

2015

A theoretical framework for power dissipation in low temperature plasmas in corona equilibrium is developed. The framework is based on fundamental conservation laws and reaction cross sections and is only weakly sensitive to plasma parameters, e.g., electron temperature and density. The theory is applied to low temperature atomic and molecular hydrogen laboratory plasmas for which the plasma heating power dissipation to photon emission, ionization, and chemical potential is calculated. The calculated photon emission is compared to recent experimental results.

PhysicsElectron densityHydrogenta114Plasma parameterslow temperature plasmaspower dissipationchemistry.chemical_elementFOS: Physical sciencesPlasmaDissipationCondensed Matter PhysicsCoronaPhysics - Plasma PhysicsPlasma Physics (physics.plasm-ph)chemistryPhysics::Plasma PhysicsIonizationPhysics::Space Physicshydrogen plasmasElectron temperatureAtomic physicsPhysics of Plasmas
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Fine-structure infrared lines from the Cassiopeia A knots

2008

Aims: Archival observations of infrared fine-structure lines of the young Galactic supernova remnant Cassiopeia A allow us to test existing models and determine the physical parameters of various regions of the fast-moving knots (FMKs), which are metal-dominated clouds of material ejected by the supernova explosion. Methods: The fluxes of the far-infrared [O i] and [O iii] lines are extracted from the previously unpublished archival ISO data. The archival Spitzer data are used to determine the fluxes of the O, Ne, Si, S, Ar and Fe ion fine-structure lines originating in the FMKs. The ratios of these line fluxes are used for the plasma diagnostics. We also determine the infrared line flux ra…

PhysicsInfraredPlasma parametersAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Doubly ionized oxygenFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCassiopeia ASupernovaSpace and Planetary SciencePlasma diagnosticsSupernova remnantSpectral line ratiosAstrophysics::Galaxy Astrophysics
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Detailed diagnostics of an X-ray flare in the single giant HR 9024

2007

We analyze a 96 ks Chandra/HETGS observation of the single G-type giant HR 9024. The high flux allows us to examine spectral line and continuum diagnostics at high temporal resolution, to derive plasma parameters. A time-dependent 1D hydrodynamic model of a loop with half-length $L = 5 \times 10^{11}$ cm ($\sim R_{\star}/2$), cross-section radius $r = 4.3 \times 10^{10}$ cm, with a heat pulse of 15 ks and $2 \times 10^{11}$~erg cm$^{-2}$ s$^{-1}$ deposited at the loop footpoints, satisfactorily reproduces the observed evolution of temperature and emission measure, derived from the analysis of the strong continuum emission. For the first time we can compare predictions from the hydrodynamic …

PhysicsPlasma parametersAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Spectral propertiesX-rayFOS: Physical sciencesAstronomy and Astrophysicshydrodynamics plasmas stars: activityPlasmaAstrophysicsAstrophysicsSpectral linelaw.inventionHigh fluxSpace and Planetary SciencelawHigh temporal resolutionFlare
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Method for estimating charge breeder ECR ion source plasma parameters with short pulse 1+ injection of metal ions

2020

Abstract A new method for determining plasma parameters from beam current transients resulting from short pulse 1+ injection of metal ions into a charge breeder electron cyclotron resonance ion source has been developed. The proposed method relies on few assumptions, and yields local values for the ionisation times 1 / n e σ v q → q + 1 inz , charge exchange times 1 / n 0 σ v q → q − 1 cx , the ion confinement times τ q , as well as estimates for the minimum plasma energy contents n e E e and the plasma triple products n e E e τ q . The method is based on fitting the current balance equation on the extracted beam currents of high charge state ions, and using the fitting coefficients to dete…

PhysicsPlasma parameterssyklotronitCharge (physics)PlasmahiukkaskiihdyttimetplasmafysiikkaCondensed Matter Physics01 natural sciencesElectron cyclotron resonanceIon source010305 fluids & plasmasIonIonization0103 physical sciencesContent (measure theory)Atomic physics010306 general physicsPlasma Sources Science and Technology
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Even harmonics generation of high frequency radiation in current-carrying plasmas

2005

Generation of high frequency radiation harmonics in a current-carrying plasma is studied. The physical mechanism responsible for harmonics generation is provided by electron-ion collisions. The current in the plasma is sustained by a constant electric field. It is shown that the electron distribution function anisotropy due to the static field yields generation of even harmonics. As a result, the radiation spectrum emitted by the current-carrying plasma contains both even and odd harmonics, the latter being attributed to currentless plasma. For a broad range of plasma and high frequency radiation parameters, a detailed analysis of the even harmonics properties is reported.

PhysicsTwo-stream instabilityDense plasma focusPhysics::Plasma PhysicsWaves in plasmasPlasma parametersHarmonicsHigh harmonic generationElectromagnetic electron wavePlasmaAtomic physicsCondensed Matter PhysicsPhysics of Plasmas
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Energy and frequency dependence of the alpha particle redistribution produced by internal kink modes

2014

International audience; The redistribution of alpha particles due to internal kink modes is studied. The exact particle trajectories in the total fields, equilibrium plus perturbation, are calculated. The equilibrium has circular cross section and the plasma parameters are similar to those expected in ITER. The alpha particles are initially distributed according to a slowing down distribution function and have energies between 18 keV and 3.5 MeV. The (1, 1), (2, 2), and (2, 1) modes are included and the effect of changing their amplitude and frequency is studied. When only the (1, 1) mode is included, the spreading of high energy ( E≳1  MeV) alpha particles increases slowly with the energy …

Physics[PHYS]Physics [physics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Plasma parameters[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Perturbation (astronomy)Alpha particlePlasmaKink instabilityCondensed Matter PhysicsAmplitudeDistribution function13. Climate action[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Redistribution (chemistry)Atomic physics
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Overview of diagnostic performance and results for the first operation phase in Wendelstein 7-X (invited)

2016

Wendelstein 7-X, a superconducting optimized stellarator built in Greifswald/Germany, started its first plasmas with the last closed flux surface (LCFS) defined by 5 uncooled graphite limiters in December 2015. At the end of the 10 weeks long experimental campaign (OP1.1) more than 20 independent diagnostic systems were in operation, allowing detailed studies of many interesting plasma phenomena. For example, fast neutral gas manometers supported by video cameras (including one fast-frame camera with frame rates of tens of kHz) as well as visible cameras with different interference filters, with field of views covering all ten half-modules of the stellarator, discovered a MARFE-like radiati…

Physicsbusiness.industryPlasma parametersInstrumentationPlasma01 natural sciencesRadiation zone010305 fluids & plasmaslaw.inventionOpticslaw0103 physical sciencesLimiterddc:530Plasma diagnosticsWendelstein 7-X010306 general physicsbusinessInstrumentationStellaratorReview of Scientific Instruments
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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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Confirmation of the topology of the Wendelstein 7-X magnetic field to better than 1:100,000

2016

Fusion energy research has in the past 40 years focused primarily on the tokamak concept, but recent advances in plasma theory and computational power have led to renewed interest in stellarators. The largest and most sophisticated stellarator in the world, Wendelstein 7-X (W7-X), has just started operation, with the aim to show that the earlier weaknesses of this concept have been addressed successfully, and that the intrinsic advantages of the concept persist, also at plasma parameters approaching those of a future fusion power plant. Here we show the first physics results, obtained before plasma operation: that the carefully tailored topology of nested magnetic surfaces needed for good c…

TokamakPlasma parametersScienceGeneral Physics and AstronomyTopology (electrical circuits)Topology7. Clean energy01 natural sciencesArticleGeneral Biochemistry Genetics and Molecular Biology010305 fluids & plasmaslaw.inventionlaw0103 physical sciences010306 general physicsPhysicsFusion Wendelstein7-X StellaratorMultidisciplinaryta114QGeneral ChemistryPlasmaFusion powerMagnetic fieldErratumWendelstein 7-XStellarator
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Dust environment of an airless object: A phase space study with kinetic models

2016

Abstract The study of dust above the lunar surface is important for both science and technology. Dust particles are electrically charged due to impact of the solar radiation and the solar wind plasma and, therefore, they affect the plasma above the lunar surface. Dust is also a health hazard for crewed missions because micron and sub-micron sized dust particles can be toxic and harmful to the human body. Dust also causes malfunctions in mechanical devices and is therefore a risk for spacecraft and instruments on the lunar surface. Properties of dust particles above the lunar surface are not fully known. However, it can be stated that their large surface area to volume ratio due to their irr…

asteroidsDusty plasma010504 meteorology & atmospheric sciencesPlasma parametersta221ta1171plasma–surface interactionPlasma-surface interactionElectronAstrophysics01 natural sciences7. Clean energyInterplanetary dust cloud0103 physical scienceskinetic particle simulationsta216Moon010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsta115ta213ta114Astronomy and AstrophysicsPlasmaComputational physicsspace plasmaSolar windSurface-area-to-volume ratio13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysical plasmadustAstrophysics::Earth and Planetary AstrophysicsPlanetary and Space Science
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