Search results for "optical spectra"

showing 7 items of 7 documents

Correlations between density distributions, optical spectra, and ion species in a hydrogen plasma (invited)

2016

An experimental study of plasma distributions in a 2.45 GHz hydrogen discharge operated at 100 Hz repetition rate is presented. Ultrafast photography, time integrated visible light emission spectra, time resolved Balmer-alpha emission, time resolved Fulcher Band emission, ion species mass spectra, and time resolved ion species fraction measurements have been implemented as diagnostic tools in a broad range of plasma conditions. Results of plasma distributions and optical emissions correlated with H + , H + 2 , and H + 3 ion currents by using a Wien filter system with optical observation capability are reported. The magnetic field distribution and strength is found as the most critical facto…

010302 applied physicsMaterials scienceWien filterta114Hydrogenchemistry.chemical_elemention speciesPlasma01 natural sciences010305 fluids & plasmasIonchemistryPhysics::Plasma Physics0103 physical scienceshydrogen plasmaMass spectrumPlasma diagnosticsEmission spectrumAtomic physicsdensity distributionsoptical spectraInstrumentationVisible spectrumReview of Scientific Instruments
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Optical and Vibrational Spectra of CsCl-Enriched GeS2-Ga2S3 Glasses

2016

Optical and FTIR spectroscopy was employed to study the properties of 80GeS2-20Ga2S3-CsCl chalcohalide glasses with CsCl additives in a temperature range of 77–293 K. It is shown that CsCl content results in the shift of fundamental absorption edge in the visible region. Vibrational bands in FTIR spectra of (80GeS2-20Ga2S3)100 − х (СsCl) x (x = 5, 10, and 15) are identified near 2500 cm−1, 3700 cm−1,, around 1580 cm−1, and a feature at 1100 cm−1. Low energy shifts of vibrational frequencies in glasses with a higher amount of CsCl can be caused by possible thermal expansion of the lattice and nanovoid agglomeration formed by CsCl additives in the inner structure of the Ge-Ga-S glass.

Materials scienceChalcohalide glassChalcogenideAnalytical chemistryNanochemistry02 engineering and technologyModification01 natural sciencesThermal expansionVibrational propertieschemistry.chemical_compound78.70.BjMaterials Science(all)Lattice (order)0103 physical sciencesGeneral Materials ScienceFourier transform infrared spectroscopy010302 applied physicsNano ExpressChalcogenide61.43.Fs71.23.CqAtmospheric temperature rangeOptical spectra021001 nanoscience & nanotechnologyCondensed Matter Physics81.70PgchemistryAbsorption edge82.56Ub0210 nano-technologyVibrational spectraNanoscale Research Letters
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Optical Spectra and Direct Optical Transitions in Amorphous and Crystalline ZnO Thin Films and Powders

2010

Comparative studies of ZnO crystalline and amorphous thin films and nanocrystalline powders are reported. The UV-visible optical spectra were analyzed with special attention paid to the direct optical bandgap. Atmospheric radio-frequency barrier torch discharge and pulsed hollow cathode sputtering techniques for the film fabrication were used. For the crystalline films, similar values of the direct optical bandgap were found independent of the growth method used. The analysis of the amorphous films and powders revealed a pronounced Urbach-like exponential absorption tail approaching the bandedge. For the powders, the bandgap energies were larger than those for the crystalline and amorphous …

Materials scienceFabricationRenewable Energy Sustainability and the EnvironmentBand gapbusiness.industryNanotechnologyCondensed Matter PhysicsNanocrystalline materialOptical spectraSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsAmorphous solidMaterials ChemistryElectrochemistryOptoelectronicsParticle sizeThin filmAbsorption (electromagnetic radiation)businessJournal of The Electrochemical Society
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Photonic crystals based on two-layer opaline heterostructures

2002

AbstractOptical properties of several heterostructures representing two-layer opaline photonic crystals have been examined. Two separate stop-bands have been observed both in transmission and emission spectra. The effect of the interface disorder on the optical spectra was not observed, probably, due to the insufficient degree of order of the opaline layers.

Materials sciencebusiness.industryTwo layerPhysics::OpticsOptoelectronicsDegree of orderHeterojunctionEmission spectrumbusinessOptical spectraPhotonic crystal
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Controlling the oxidation processes of Zn nanoparticles produced by pulsed laser ablation in aqueous solution

2016

We used online UV-VIS optical absorption and photoluminescence spectra, acquired during and after pulsed laser ablation of a Zinc plate in aqueous solution, to investigate the effect of the laser repetition rate and liquid environment on the oxidation processes of the produced nanoparticles. A transient Zn/ZnO core-shell structure was revealed by the coexistence of an absorption peak around 5.0 eV due to Zn surface plasmon resonance and of an edge at 3.4 eV coming from wurtzite ZnO. The growth kinetics of ZnO at the various repetition rates, selectively probed by the excitonic emission at 3.3 eV, began immediately at the onset of laser ablation and was largely independent of the repetition …

PhotoluminescenceAqueous solutionMaterials scienceLaser ablationAnalytical chemistryGeneral Physics and AstronomyNanoparticlechemistry.chemical_element02 engineering and technologyZinc010402 general chemistry021001 nanoscience & nanotechnologyLaserPhotochemistry01 natural sciences0104 chemical scienceslaw.inventionchemistrylawZnO nanoparticles laser ablation oxidation Photoluminescence Surface plasmon resonance In situ optical spectra Defects excitons0210 nano-technologyAbsorption (electromagnetic radiation)Wurtzite crystal structureJournal of Applied Physics
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APOGEE Data Releases 13 and 14: Stellar Parameter and Abundance Comparisons with Independent Analyses

2018

Data from the SDSS-IV / Apache Point Observatory Galactic Evolution Experiment (APOGEE-2) have been released as part of SDSS Data Releases 13 (DR13) and 14 (DR14). These include high resolution H-band spectra, radial velocities, and derived stellar parameters and abundances. DR13, released in August 2016, contained APOGEE data for roughly 150,000 stars, and DR14, released in August 2017, added about 110,000 more. Stellar parameters and abundances have been derived with an automated pipeline, the APOGEE Stellar Parameter and Chemical Abundance Pipeline (ASPCAP). We evaluate the performance of this pipeline by comparing the derived stellar parameters and abundances to those inferred from opti…

Physics010308 nuclear & particles physicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencesStandard deviationSpectral lineOptical spectraStarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceObservatoryAbundance (ecology)Astrophysics of Galaxies (astro-ph.GA)0103 physical sciencesThick disk[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)ComputingMilieux_MISCELLANEOUS
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Non-linear optical spectra of excitons in polydiacetylene

1992

Abstract Adding long-range Coulomb interactions to the Su-Schrieffer-Heeger model makes it possible to investigate excitonic states in conjugated polymers. Various characteristic features due to these states as well as due to the electron-hole continuum can be found in the calculated non-linear optical susceptibilities. In particular the electroabsorption spectrum and the third harmonic generation intensity and its dependence on the system size are examined. Using only moderate interaction strength, various experiments in polydiacetylene can be interpreted in a consistent way.

chemistry.chemical_classificationbusiness.industryChemistryExcitonBiophysicsInteraction strengthGeneral ChemistryPolymerConjugated systemCondensed Matter PhysicsBiochemistryMolecular physicsAtomic and Molecular Physics and OpticsOptical spectraNonlinear systemCoulombOptoelectronicsThird harmonicbusinessJournal of Luminescence
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