Search results for "Plasma diagnostics"

showing 10 items of 59 documents

Ultra-fast intensified frame images from an electron cyclotron resonance hydrogen plasma at 2.45 GHz: some space distributions of visible and monochr…

2014

First results from an ultra-fast frame image acquisition diagnostic coupled to a 2.45 GHz microwave hydrogen discharge are presented. The plasma reactor has been modified to include a transparent doubled shielded quartz window allowing to viewing the full plasma volume. Pictures describing the breakdown process at 1μs exposure time have been obtained for integrated visible light signal, Balmer-alpha, Balmer-beta lines, and Fulcher-band. Several different plasma emission distributions are reported. The distribution depends on the magnetic field configuration, incident microwave power, and neutral gas pressure. peerReviewed

Dense plasma focusMaterials scienceta114business.industrymicrowave powerAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaElectron cyclotron resonancemagnetic field configurationPlasma windowOpticsPhysics::Plasma Physicsframe imagesgas pressurePlasma diagnosticsElectromagnetic electron waveAtomic physicsInductively coupled plasmabusinessInstrumentationMicrowaveThe Review of scientific instruments
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Observation of Poincaré-Andronov-Hopf Bifurcation in Cyclotron Maser Emission from a Magnetic Plasma Trap

2018

We report the first experimental evidence of a controlled transition from the generation of periodic bursts of electromagnetic radiation into the continuous-wave regime of a cyclotron maser formed in magnetically confined nonequilibrium plasma. The kinetic cyclotron instability of the extraordinary wave of weakly inhomogeneous magnetized plasma is driven by the anisotropic electron population resulting from electron cyclotron plasma heating in a MHD-stable minimum-B open magnetic trap. peerReviewed

Electromagnetic wavesAstrophysics::High Energy Astrophysical PhenomenasyklotronitPlasma stabilitysähkömagnetismiCyclotronsplasmafysiikkamaseritPlasma diagnosticsMagnetohydrodynamicsPhysics::Plasma PhysicsPhysics::Space PhysicsMasersHopf bifurcationMagnetoplasma
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Stark broadening of the hydrogen Paschen ? transition at electron densities of the order of $ \mathsf {10^{15}}$ cm $ \mathsf {^{-3}}$

2003

Stark broadening measurements and calculations of the Paschen γ spectral line of hydrogen ( λ = 1.094[: MU :] m) are reported. Investigations have been performed at plasma electron densities between 1.4×10 15 cm -3 and 3.7×10 15 cm -3 . As the light source a wall-stabilized arc operated in a helium-hydrogen gas mixture at atmospheric pressure has been applied. The radiation of the plasma emitted from nearly homogeneous plasma layers in end-on direction, was measured with the use of a grating spectrometer equipped with a charge coupled device (CCD) detector. The radiance calibration was carried out against light outputs originating from a tungsten strip radiation standard. The measured FWHM …

Electron densityFull width at half maximumsymbols.namesakeMaterials scienceAtmospheric pressureStark effectsymbolsPlasma diagnosticsElectronPlasmaAtomic physicsAtomic and Molecular Physics and OpticsSpectral lineThe European Physical Journal D - Atomic, Molecular and Optical Physics
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Experimental investigations of two doubly excited NI multiplets

2005

Experimental Stark-broadening studies of two NI multiplets ( 1 D)3s 2 D - ( 1 D)3p 2 D° and ( 1 D)3s 2 D - ( 1 D) 3 p 2 F° are reported. Measurements were performed using a wall-stabilized arc operated at atmospheric pressure in helium with small amounts of nitrogen and hydrogen. The Stark broadening parameters: the electron impact width (w e ) and shift (d e ) have been determined.

Electron densitysymbols.namesakeHydrogenchemistryStark effectExcited statesymbolschemistry.chemical_elementPlasma diagnosticsElectronAtomic physicsElectron ionizationHeliumSPIE Proceedings
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Line Shape Measurement and Modelling for Plasma Diagnostics

2014

In this paper we discuss different methods of narrow spectral line shape measurements for a wide spectral range by means of high-resolution spectrometers such as the Fabry-Perot spectrometer, Zeeman spectrometer and Fourier transform spectrometer as well as a theoretical model for spectral line shape modelling and solving of the inverse task based on Tikhonov's regularization method. Special attention is devoted to the line shape measurements for the optically thin light sources filled with Hg, Ar, Xe, Kr for their use in high precision analysers for detection of heavy metals and benzene.

HistoryZeeman effectSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryChemistryInverseRegularization (mathematics)Computer Science ApplicationsEducationSpectral line shapeTikhonov regularizationsymbols.namesakeOpticssymbolsPlasma diagnosticsNuclear ExperimentbusinessLine (formation)Journal of Physics: Conference Series
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Experimental study of hydrogen plasma breakdown in a 2.45 GHz microwave discharge

2013

Temporal evolution of microwave-plasma coupling, vacuum ultraviolet (VUV) light emission and plasma electron temperature and density is reported for a 2.45GHz microwave hydrogen discharge pulsed at 50Hz. Directional couplers, a VUV spectrometer and a Langmuir probe are used for the diagnostics of the plasma breakdown. A 5‐10 µs transient peak of light emission exceeding the steady-state intensity by a factor of 3.3 is observed in coincidence with an abrupt drop in the microwave electric field. Observed light emission intensities combined with cross section data indicate that the electron temperature during the breakdown transient exceeds the steady-state value of 4‐6eV by a factor 3, which …

HydrogenChemistrybusiness.industrychemistry.chemical_elementAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaCondensed Matter Physicssymbols.namesakeOpticsPhysics::Plasma PhysicsElectric fieldsymbolsElectron temperatureLangmuir probeLight emissionPlasma diagnosticsAtomic physicsbusinessMicrowavePlasma Sources Science and Technology
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Fabry–Pérot lineshape analysis in an optically thick expanding plasma

2007

In this work the authors present Fabry–Perot measurements of Ar atom spectral line profiles originating from the expansion of an Ar–N2 thermal plasma into a low pressure environment. The plasma is characterized by strong density, temperature and velocity gradients and it offers a high degree of light absorption for some gas mixtures. First, it is demonstrated that the Abel inversion method cannot be applied under such conditions even if absorption is absent. Second, two approaches are examined to obtain plasma parameters in the case of an optically thick expanding plasma. It is shown that velocity and temperature development along the jet radius can be inferred from experimental lineshapes …

Jet (fluid)ChemistryPlasma parametersPhysics::Space PhysicsPlasma parameterPlasma diagnosticsRadiusPlasmaAtomic physicsCondensed Matter PhysicsAbsorption (electromagnetic radiation)Spectral linePlasma Sources Science and Technology
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Major results from the first plasma campaign of the Wendelstein 7-X stellarator

2017

After completing the main construction phase of Wendelstein 7-X (W7-X) and successfully commissioning the device, first plasma operation started at the end of 2015. Integral commissioning of plasma start-up and operation using electron cyclotron resonance heating (ECRH) and an extensive set of plasma diagnostics have been completed, allowing initial physics studies during the first operational campaign. Both in helium and hydrogen, plasma breakdown was easily achieved. Gaining experience with plasma vessel conditioning, discharge lengths could be extended gradually. Eventually, discharges lasted up to 6 s, reaching an injected energy of 4 MJ, which is twice the limit originally agreed for t…

Magnetic confinementNuclear and High Energy PhysicsTechnology and EngineeringPlasma heatingCyclotron resonanceCONFINEMENT01 natural sciencesElectron cyclotron resonance010305 fluids & plasmaslaw.inventionPHYSICSNuclear physicsstellaratorcurrent drive; magnetic confinement; plasma heating; stellarator; Nuclear and High Energy Physics; Condensed Matter Physicslaw0103 physical sciencesddc:530010306 general physicstellaratorStellaratorPhysicsmagnetic confinementMagnetic confinement fusionplasma heatingcurrent drive;magnetic confinement;plasma heating;stellaratorPlasma530 PhysikCondensed Matter PhysicsTRANSPORTCurrent drivecurrent driveElectron temperaturePlasma diagnosticsAtomic physicsWendelstein 7-X[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]StellaratorNuclear Fusion
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Hydrogen non-equilibrium ionisation effects in coronal mass ejections

2020

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). D.H.M. would like to thank both the UK STFC and the ERC (Synergy grant: WHOLE SUN, grant Agreement No. 810218) for financial support. D.H.M. and P.P. would like to thank STFC for IAA funding under grant number SMC1-XAS012. This work used the DiRAC@Durham facility man-aged by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk. The equipment was funded by BEIS capital fundin…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesHydrogenSun: coronal mass ejections (CMEs)FOS: Physical scienceschemistry.chemical_elementAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences7. Clean energycoronal mass ejections (CMEs) [un]Ionization0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]Sun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]Sun: coronaAstronomy and Astrophysics3rd-DASPlasmaMagnetic fluxSolar windQC PhysicsAstrophysics - Solar and Stellar AstrophysicschemistrySpace and Planetary SciencePhysics::Space PhysicsPlasma diagnosticsMagnetohydrodynamicsAstronomy & Astrophysics
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Experimental and theoretical studies of Stark profiles of Ar I 696.5 nm spectral line in laser-induced plasma

2019

Abstract We report the results of the Stark profile studies of the 696.543 nm Ar I spectral line in laser-induced plasma generated by a nanosecond Nd:YAG laser radiation at 532 nm in argon at reduced pressure. Plasma diagnostics was performed with the use of the laser Thomson scattering method, free from assumptions about the plasma thermodynamic equilibrium, its composition but also independently of plasma emission spectra. The profiles were investigated in wide range of electron densities and temperatures, from 2.81 · 1022 m − 3 to 5.69 · 1023 m − 3 and from 10 430 K to 73 400 K, respectively. Stark profiles were calculated using a semi-classical method as well as by N-body numerical simu…

Materials science010504 meteorology & atmospheric sciencesStark broadeningThomson scatteringThermodynamic equilibrium01 natural sciencesSpectral linesymbols.namesake[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Physics::Plasma Physicscomputer simulationsLaser-induced plasmaEmission spectrumThomson scatteringComputingMilieux_MISCELLANEOUSSpectroscopy0105 earth and related environmental sciencesRadiationPlasmaAtomic and Molecular Physics and OpticsStark effectlaser-induced plasmasymbolsElectron temperaturePlasma diagnosticsAtomic physicsComputer simulationsJournal of Quantitative Spectroscopy and Radiative Transfer
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