Search results for " EMI"

showing 10 items of 1830 documents

The effect of plasma electrode collar structure on the performance of the JYFL 14GHz electron cyclotron resonance ion source

2013

Abstract The influence of a so-called collar structure on the performance of the JYFL 14 GHz electron cyclotron resonance ion source (ECRIS) has been studied experimentally at the Department of Physics, University of Jyvaskyla (JYFL). The collar is a cylindrical structure extruding inwards from the plasma electrode. The collar length was varied between 5 and 60 mm. For some ion species a moderate performance improvement was achieved in terms of extracted beam current and transverse emittance up to 30 mm collar length. Longer collars resulted in a substantial performance decrease. Different collar materials, i.e. nonmagnetic stainless steel, aluminum and Al 2 O 3 , and a wide range of ion sp…

010302 applied physicsPhysicsNuclear and High Energy Physicsta114Plasma01 natural sciences7. Clean energyElectron cyclotron resonanceIon source010305 fluids & plasmasCollarIon0103 physical sciencesElectrodeThermal emittanceddc:530Atomic physicsInstrumentationBeam (structure)
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Time resolved measurements of hydrogen ion energy distributions in a pulsed 2.45 GHz microwave plasma

2017

A plasma diagnostic study of the Ion Energy Distribution Functions (IEDFs) of H+, H+2H2+, and H+3H3+ ions in a 2.45 GHz hydrogen plasma reactor called TIPS is presented. The measurements are conducted by using a Plasma Ion Mass Spectrometer with an energy sector and a quadrupole detector from HIDEN Analytical Limited in order to select an ion species and to measure its energy distribution. The reactor is operated in the pulsed mode at 100 Hz with a duty cycle of 10% (1 ms pulse width). The IEDFs of H+, H+2H2+, and H+3H3+ are obtained each 5 μs with 1 μs time resolution throughout the entire pulse. The temporal evolution of the plasma potential and ion temperature of H+ is derived from the d…

010302 applied physicsPhysicsRange (particle radiation)plasma sourcesta114plasma diagnosticsPlasmaCondensed Matter PhysicsMass spectrometry01 natural sciences7. Clean energyIon source010305 fluids & plasmasIonplasma dynamicsPhysics::Plasma Physics0103 physical sciencesThermal emittancePlasma diagnosticsionAtomic physicsMicrowaveplasma sheathsPhysics of Plasmas
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Ultrasonic nebulization inductively coupled plasma optical emission spectrometry method for wine analysis

2020

Abstract A methodology was developed to determine mineral elements in wines using Inductively Coupled Plasma Optical Emission Spectrometry combined with ultrasonic nebulization. The concentration of 36 elements (Al, B, Ba, Bi, Ca, Cd, Ce, Co, Cr, Dy, Er, Eu, Fe, Gd, K, La, Lu, Mg, Mn, Mo, Na, Nd, Ni, Pb, Pr, Sb, Sc, Sm, Sr, Tb, Ti, Tm, V, Y, Yb, and Zn) was determined in 59 wine samples and used to distinguish between Brazilian and Spanish wines. The best conditions for the plasma were selected using a two-level factorial design: radiofrequency power 1500 W; plasma gas flow rate 15 L min−1; auxiliary 0.70 L min−1; and nebulizer 0.40 L min−1. An exploratory multivariate analysis by Principal…

010302 applied physicsWineRiver valleyChemistry010401 analytical chemistryAnalytical chemistryMineral composition01 natural sciencesAtomic and Molecular Physics and OpticsUltrasonic nebulization0104 chemical sciencesAnalytical ChemistryInductively coupled plasma atomic emission spectroscopy0103 physical sciencesInductively coupled plasmaOptical emission spectrometryInstrumentationSpectroscopySpectrochimica Acta Part B: Atomic Spectroscopy
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Mechanism of activated chemiluminescence of cyclic peroxides: 1,2-dioxetanes and 1,2-dioxetanones

2017

Almost all chemiluminescent and bioluminescent reactions involve cyclic peroxides. The structure of the peroxide and reaction conditions determine the quantum efficiency of light emission. Oxidizable fluorophores, the so-called activators, react with 1,2-dioxetanones promoting the former to their first singlet excited state. This transformation is inefficient and does not occur with 1,2-dioxetanes; however, they have been used as models for the efficient firefly bioluminescence. In this work, we use the SA-CASSCF/CASPT2 method to investigate the activated chemiexcitation of the parent 1,2-dioxetane and 1,2-dioxetanone. Our findings suggest that ground state decomposition of the peroxide com…

010405 organic chemistryChemistryGeneral Physics and Astronomy010402 general chemistryPhotochemistrySupermolecule01 natural sciencesPeroxideLUCIFERIDAE0104 chemical scienceslaw.inventionchemistry.chemical_compoundlawExcited stateBioluminescenceLight emissionSinglet statePhysical and Theoretical ChemistryGround stateChemiluminescencePhysical Chemistry Chemical Physics
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Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart

2020

We study the impact of gas accretion on the orbital evolution of black-hole binaries initially at large separation in the band of the planned Laser Interferometer Space Antenna (LISA). We focus on two sources: (i)~stellar-origin black-hole binaries~(SOBHBs) that can migrate from the LISA band to the band of ground-based gravitational-wave observatories within weeks/months; and (ii) intermediate-mass black-hole binaries~(IMBHBs) in the LISA band only. Because of the large number of observable gravitational-wave cycles, the phase evolution of these systems needs to be modeled to great accuracy to avoid biasing the estimation of the source parameters. Accretion affects the gravitational-wave p…

010504 meteorology & atmospheric sciencesAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)Observableastro-ph.HE; astro-ph.HE; General Relativity and Quantum Cosmologygas: accretionblack holes gravitational wavesobservatoryInterferometrygravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenainterferometermedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational radiation: direct detectionelectromagnetic field: productionGeneral Relativity and Quantum Cosmologybinary: coalescencestatistical analysisSettore FIS/05 - Astronomia e Astrofisicagravitation: weak field0103 physical sciencesnumerical calculationsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLISAGravitational wavegravitational radiationOrder (ring theory)black hole: accretionAstronomy and Astrophysicsblack holesgravitational radiation detectorRedshiftBlack holeblack hole: binarySpace and Planetary ScienceSkygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray: detectorThe Astrophysical Journal
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Study of a sample of faint Be stars in the exofield of CoRoT

2013

International audience; Context. Be stars are probably the most rapid rotators among stars in the main sequence (MS) and, as such, are excellent candidates to study the incidence of the rotation on the characteristics of their non-radial pulsations, as well as on their internal structure. Pulsations are also thought to be possible mechanisms that help the mass ejection needed to build up the circumstellar disks of Be stars.Aims. The purpose of this paper is to identify a number of faint Be stars observed with the CoRoT satellite and to determine their fundamental parameters, which will enable us to study their pulsation properties as a function of the location in the HR diagram and to searc…

010504 meteorology & atmospheric sciencesBe starHertzsprung–Russell diagramK-type main-sequence starstars: emission-lineAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineBlue stragglersymbols.namesakestars: rotation0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AstronomyBeAstronomy and Astrophysicsstars: early-typeHerbig Ae/Be starT Tauri starStars[SDU]Sciences of the Universe [physics]Space and Planetary Sciencesymbolsstars: fundamental parametersstars: oscillationsAstrophysics::Earth and Planetary Astrophysicsbinaries: spectroscopicAstronomy & Astrophysics
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Developing an indicator-modelling approach to forecast changes in nitrogen critical load exceedance across Europe arising from agricultural reform

2011

International audience; Atmospheric nitrogen (N) deposition above the critical load causes eutrophication with adverse impacts on biodiversity. Average Accumulated critical load Exceedance (AAE) is a measure of the amount of critical load exceedance and the area of habitat which is affected, and has been adopted in Europe as a pressure indicator for biodiversity. In Europe, AAE is calculated by the Coordination Centre for Effects (CCE) of the United Nations Economic Commission for Europe based on modelled nitrogen deposition and country-level reporting of critical load thresholds and ecosystem area. Due to differences in country-level reporting, AAE values for semi-natural habitats may show…

010504 meteorology & atmospheric sciencesBiodiversityGeneral Decision Sciences010501 environmental sciences01 natural sciencesAMMONIA EMISSIONEnvironmental protectionEcosystemEcology Evolution Behavior and Systematics0105 earth and related environmental sciences2. Zero hungerCritical loadNITROGEN DEPOSITIONEcologyEMISSION D'AMONIAQUEbusiness.industry15. Life on landDeposition (aerosol physics)Habitat13. Climate actionAgricultureEUTROPHICATIONSpatial ecologyEnvironmental scienceBIODIVERSITYCAP REFORM[SDE.BE]Environmental Sciences/Biodiversity and EcologyEutrophicationbusiness
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Hydrothermal pressure-temperature control on CO2 emissions and seismicity at Campi Flegrei (Italy)

2021

Fluids supplied by stored magma at depth are causal factors of volcanic unrest, as they can cause pressurization/heating of hydrothermal systems. However, evidence for links between hydrothermal pressurization, CO2 emission and volcano seismicity have remained elusive. Here, we use recent (2010−2020) observations at Campi Flegrei caldera (CFc) to show hydrothermal pressure, gas emission and seismicity at CFc share common source areas and well-matching temporal evolutions. We interpret the recent escalation in seismicity and surface gas emissions as caused by pressure-temperature increase at the top of a vertically elongated (0.3–2 km deep) gas front. Using mass (steam) balance consideration…

010504 meteorology & atmospheric sciencesCampi Flegrei mantle geochemistry CO2 emission Fumarole compositions Hydrothermal systems Volcanic unrest Volcano seismicityInduced seismicity010502 geochemistry & geophysics01 natural sciencesHydrothermal circulationHydrothermal systemsCabin pressurizationGeochemistry and PetrologyCalderaPetrologyFumarole compositions0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryVolcanic unrest; Hydrothermal systems; Campi Flegrei; Fumarole compositions; CO2 emission; Volcano seismicityFront (oceanography)Volcano seismicityGeophysicsVolcanoVolume (thermodynamics)Volcanic unrestCO2 emissionMagmaCampi FlegreiGeology
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Relations between Air Quality and Covid-19 Lockdown Measures in Valencia, Spain

2021

The set of measures to contain the diffusion of COVID-19 instituted by the European governments gave an unparalleled opportunity to improve our understanding of the transport and industrial sectors’ contribution to urban air pollution. The purpose of this study was to assess the impacts of the lockdown measures on air quality and pollutant emissions in Valencia, Spain. For this reason, we determined if there was a significant difference in the concentration levels of different particulate matter (PM) sizes, PM10, PM2.5, and NOx, NO2, NO, and O3, between the period of restrictions in 2020 and the same period in 2019. Our findings indicated that PM pollutant levels during the lockdown period…

010504 meteorology & atmospheric sciencesCoronavirus disease 2019 (COVID-19)Pollutant emissionsHealth Toxicology and Mutagenesisair pollutionAir pollutionlcsh:Medicine010501 environmental sciencesmedicine.disease_cause01 natural sciencesArticleToxicologylockdownmedicineHumansValenciaAir quality index0105 earth and related environmental sciencesPollutantbiologyparticulate matter (pm)Significant differencelcsh:RPublic Health Environmental and Occupational HealthParticulatesbiology.organism_classificationnitrogen oxidesozoneSpainCommunicable Disease ControlEnvironmental scienceParticulate MatterCovid-19Environmental MonitoringInternational Journal of Environmental Research and Public Health
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