Search results for " emission"

showing 10 items of 1496 documents

β-decay of 35Ca

1999

Abstract The β-decay of the T z =− 5 2 nucleus 35 Ca was studied at the LISE3 spectrometer at GANIL. The 35 Ca decay scheme was deduced from its β-delayed proton emission into the ground and excited states of 34 Ar and from its β-delayed two-proton emission. The 35 Ca half-life was determined to be 25.7±0.2 ms. The measured transition strength function B(GT) is compared to results obtained from large-scale sd-shell model calculations.

PhysicsNuclear and High Energy PhysicsDecay schemeSpectrometer010308 nuclear & particles physics01 natural sciences7. Clean energymedicine.anatomical_structureTransition strengthExcited state0103 physical sciencesmedicineProton emissionAtomic physics010306 general physicsNucleusPhysics Letters B
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Defect Luminescence of LiBaF3 Perovskites

2000

Blue and red luminescence of undoped LiBaF3 crystals was studied. A broad, isotropic photoluminescence band centered at 410 nm can be excited by 210 nm — 275 nm light in as grown crystals. After X-irradiation at RT a new narrower, anisotropic luminescence band appears at 425 mn which has an additional excitation band at 290 nm. The X-irradiation also creates the F- type centres and anisotropic centres with an absorption band at 630 nm and a luminescence band at 700 nm. No F- centre luminescence is observed. All the other centres mentioned act as radiative recombination centers as well. It is speculated that the origin of the blue luminescence is due to oxygen defects and that the red lumine…

PhotoluminescenceMaterials scienceImpurityAbsorption bandExcited stateSpontaneous emissionLuminescenceAnisotropyMolecular physicsExcitation
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Photoluminescence of Ga-face AlGaN/GaN single heterostructures

2001

Abstract The radiative recombination in Ga-face Al 0.30 Ga 0.70 N/GaN single heterostructures (SHs) was studied by photoluminescence (PL) measurements. An energy shift of the excitonic transitions toward higher energies was observed, indicating the presence of residual compressive strain in the GaN layer. In addition to these exciton lines, a broad band energetically localized between the exciton lines and the LO-phonon replica was noticed in the undoped SH. From its energy position, excitation power dependence, as well as temperature behaviour, we have attributed this luminescence to the H -band (HB), which is representative of the two-dimensional electron gas (2DEG) recombination.

PhotoluminescenceMaterials scienceCondensed matter physicsCondensed Matter::OtherMechanical EngineeringExcitonHeterojunctionCondensed Matter::Mesoscopic Systems and Quantum Hall EffectCondensed Matter PhysicsCondensed Matter::Materials ScienceMechanics of MaterialsGeneral Materials ScienceSpontaneous emissionFermi gasLuminescenceExcitationRecombinationMaterials Science and Engineering: B
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Parametric assessment of myocardial perfusion by densitometric evaluation of digital subtraction coronary angiograms: a comparison with tomographic T…

2002

Densitometric results about local myocardial perfusion are compared with those derived from a quantitative analysis of TL-201 single photon emission computer tomograms (TL-201 SPECT). Ten patients underwent conventional TL-201 SPECT at rest and after maximum bicycle stress and dipyridamole infusion the day prior to the investigation. SPECT was applied to provide improved spatial resolution for the detection of perfusion abnormalities. During the catheterization procedure four digital subtraction coronary angiograms were performed, two of the left and two of the right coronary artery both before and after pharmacologically induced hyperemia by intracoronary papaverine. The densitometric para…

medicine.medical_specialtymedicine.diagnostic_testbusiness.industrySubtractionSingle-photon emission computed tomographyScintigraphyDipyridamoleCatheterization procedureRight coronary arterymedicine.arteryAngiographymedicineRadiologybusinessNuclear medicinePerfusionmedicine.drug[1990] Proceedings Computers in Cardiology
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Unconventional Reducing Gases Monitoring in Everyday Places

2017

Abstract Air pollution, be it indoors or outdoors, is a major environmental health concern as it can lead to serious health effects, such as respiratory diseases, including asthma and lung cancer. Much progress has been made in Europe in improving outdoor air quality and limit values have been set for several pollutants. However, indoor air quality also requires attention because this is where we spend most of our time. Measurements at appropriate spatial and temporal scales are essential for understanding and monitoring heterogeneous environments with complex and highly variable emission sources, such as in urban areas. However, the costs and complexity of conventional air quality measurem…

Engineering010504 meteorology & atmospheric sciencesAir pollutionhuman exposure010402 general chemistrymedicine.disease_cause01 natural sciencesIndoor air qualitymedicineunconventional environmentsTemporal scalesEnvironmental planningAir quality index0105 earth and related environmental sciencesPollutantGovernmentair quality reducing gas low-cost and portable sensor unconventional environments human exposureWaste managementbusiness.industryOutdoor air qualityair quality0104 chemical scienceslow-cost and portable sensorreducing gasFugitive emissionsbusinessEnergy Procedia
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
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Characterisation of the magmatic signature in gas emissions from Turrialba Volcano, Costa Rica

2014

The equilibrium composition of volcanic gases with their magma is often overprinted by interaction with a shallow hydrothermal system. Identifying the magmatic signature of volcanic gases is critical to relate their composition to properties of the magma (temperature, fO2, gas-melt segregation depth). We report measurements of the chemical composition and flux of the major gas species emitted from Turrialba Volcano during March 2013. Measurements were made of two vents in the summit region, one of which opened in 2010 and the other in 2012. We determined an average SO2 flux of 5.2 ± 1.9 kg s-1 using scanning ultraviolet spectroscopy, and molar proportions of H2O, CO2, SO2, HCl, CO and H2 ga…

010504 meteorology & atmospheric sciencesStratigraphyChemical compositionContinuous emissionSoil ScienceMineralogyVolcanoe010502 geochemistry & geophysics01 natural sciencesHydrothermal circulationVolcanic GasesHydrothermal systemFlux (metallurgy)lcsh:StratigraphyMagmatic signaturesGeochemistry and PetrologyUltraviolet spectroscopyeventGas compositionFourier transform infrared spectroscopyChemical compositionlcsh:QE640-6990105 earth and related environmental sciencesEarth-Surface Processesevent.disaster_typegeographygeography.geographical_feature_categorylcsh:QE1-996.5Fourier transform infrared spectrometryPaleontologyFourier transform infrared spectroscopyGeologyChemical signatureGas-sensing systemlcsh:GeologyGeophysicsVolcanoCarbon dioxideSulfur dioxide13. Climate actionEquilibrium compositionMagmaCarbon dioxide; Fourier transform infrared spectroscopy; Sulfur dioxide; Ultraviolet spectroscopy; Volcanoes; Chemical compositions; Chemical signatures; Continuous emission; Equilibrium compositions; Fourier transform infrared spectrometry; Gas-sensing systems; Hydrothermal system; Magmatic signaturesGeology
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Plasma diagnostic tools for ECR ion sources : What can we learn from these experiments for the next generation sources

2019

International audience; The order-of-magnitude performance leaps of ECR ion sources over the past decades result from improvements to the magnetic plasma confinement, increases in the microwave heating frequency, and techniques to stabilize the plasma at high densities. Parallel to the technical development of the ion sources themselves, significant effort has been directed into the development of their plasma diagnostic tools. We review the recent results of Electron Cyclotron Resonance Ion Source (ECRIS) plasma diagnostics highlighting a number of selected examples of plasma density, electron energy distribution, and ion confinement time measurements, obtained mostly with the second-gener…

[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Solenoidmagnetic fieldshiukkaskiihdyttimetplasmafysiikka7. Clean energy01 natural sciencesbremsstrahlungElectron cyclotron resonance010305 fluids & plasmasIonoptical emission spectroscopySuperposition principleion sourcesPhysics::Plasma Physics0103 physical sciencesInstrumentation010302 applied physicsPhysics[PHYS]Physics [physics]plasma confinementplasma properties and parametersplasma diagnosticssyklotronitplasma heatingPlasmaIon sourceComputational physicsMagnetic fieldPlasma diagnostics
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Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave

2017

Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity. We investigate the correlation between the optical emission and the X-ray activity to predict the occurrence of new X-ray outbursts from the inferred state of the circumstellar disc. We have performed a multiwavelength study of H 1145-619 from 1973 to 2017 and present here a global analysis of its variability over the last 40 years. We have used optical spectra from the SAAO, SMARTS and SALT telescopes and optical photometry from INTEGRAL/OMC and ASAS. We also used X-ray observations from INTEGRAL/…

BrightnessBe starAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectX-ray binarystars: emission-lineFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineDensity wave theoryPhotometry (optics)X-rays: binariesstars: neutrontechniques: photometric0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsBeAstronomy and AstrophysicsLight curvestars: emission-line BeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSkyAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenatechniques: spectroscopicAstronomy & Astrophysics
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A tandem-flow assembly for the chemiluminometric determination of hydroquinone

2003

A direct chemiluminescent procedure for determination of hydroquinone based on the emergent flow methodology known as multicommutation or tandem-flow is presented for first time. The manifold was based on a set of three channels and three solenoid valves; and, the determination was performed at 60degreesC and at flow-rate of 7.5 ml min(-1). The complete cycle lasted 35 s, which resulted in a sample flow trough of 103 h(-1). The chemical process was the hydroquinone oxidation with the system sulphuric acid-potassium permanganate; and the light emission was clearly enhanced by the presence of quinine sulphate and benzalkonium chloride reaching a detection limit of 30 Rg l(-1). The dynamic int…

Detection limitChemiluminescenceChromatographyHydroquinoneHydroquinonePermanganateAnalytical chemistrySulfuric acidAnalytical Chemistrylaw.inventionchemistry.chemical_compoundBenzalkonium chloridePotassium permanganatechemistryEnvironmental sampleslawTandem-flowQUIMICA ANALITICAmedicinePharmaceuticalsLight emissionChemiluminescencemedicine.drugTalanta
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