Search results for "Absorption"

showing 10 items of 2701 documents

Determination of Kerr and two-photon absorption coefficients of indandione derivatives

2017

This material is based upon work supported by the ERDF 1.1.1.1 activity project Nr. 1.1.1.1/16/A/046 “Application assessment of novel organic materials by prototyping of photonic devices” as well as by National Research Program “Multifunctional Materials and Composites, Photonics and Nanotechnology” (IMIS2) project “Photonics and materials for photonics”.

Z-scanMaterials scienceKerr effectPhotonHyperpolarizability02 engineering and technology01 natural sciences7. Clean energyTwo-photon absorptionlaw.invention010309 opticsOpticsKerr effectlaw0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]two-photon absorptionZ-scan techniqueAbsorption (electromagnetic radiation)business.industrynonlinear opticsNonlinear optics021001 nanoscience & nanotechnologyLaser3. Good healthorganic materialsAtomic physics0210 nano-technologybusiness
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Optical diagnostic method for benzene detection in air

2014

In this paper we show our first results of research for creation a detector for benzene vapor and possibly other volatile organic compounds detection in air based on Zeeman atomic absorption technique. First the detailed study of benzene absorption spectra with high resolution spectrometer Jobin-Yvon 1000M was done. The absorption spectra of benzene were registered in the spectral range from 200-900 nm. More detailed analysis was done for the 240 – 260 nm spectral range to test a possibility to detect benzene by means of emission line of 254 nm of mercury.

Zeeman effectAbsorption spectroscopySpectrometerDetectorAnalytical chemistrychemistry.chemical_elementlaw.inventionMercury (element)chemistry.chemical_compoundsymbols.namesakechemistrylawsymbolsEmission spectrumAtomic absorption spectroscopyBenzeneSPIE Proceedings
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Critical review of the atomic spectrometric analysis of arsenic in foods

1994

The literature on the determination of arsenic in foods by atomic spectroscopy involving hydride generation, platform furnace Zeeman and inductively coupled plasma has been critically reviewed. Hydride generation has been largely displaced as a powerful tool by platform furnace Zeeman, using the STPF (stabilized temperature platform furnace) concept for the control of interferences. Inductively coupled plasma with conventional pneumatic nebulization has been little used. An alternative is to employ hydride generation-ICP with extraction of the arsenic in an organic phase. This technique permits proper control of interferences together with an increase in sensitivity. Depending on the conten…

Zeeman effectChemistryHydrideExtraction (chemistry)Analytical chemistrychemistry.chemical_elementAtomic spectroscopyBiochemistryAnalytical Chemistrylaw.inventionsymbols.namesakelawsymbolsInductively coupled plasmaSpectroscopyAtomic absorption spectroscopyArsenicFresenius' Journal of Analytical Chemistry
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<title>Deconvolution of the mercury 253.7 nm spectral line shape for the use in absorption spectroscopy</title>

2008

In this work we present measurement and results of the deconvolution of the Hg 253.7 nm spectral line shapes, emitted from the mercury isotope high-frequency electrodeless discharge lamps, made at the Institute of Atomic Physics and Spectroscopy for the use in Zeeman Atomic Absorption Spectrometry. The emission line profiles of 254 nm Hg resonance line have been measured by means of a Zeeman scanning spectrometer at the mercury cold spot temperature value at 20 C. Then the deconvolution procedure or solving of this ill-posed inverse problem by means of the Tikhonov's regularization method [1] was performed to obtain the real spectral line shape.© (2008) COPYRIGHT SPIE--The International Soc…

Zeeman effectSpectrometerAbsorption spectroscopybusiness.industryChemistrySpectral lineSpectral line shapesymbols.namesakeOpticssymbolsPhysics::Atomic PhysicsDeconvolutionEmission spectrumbusinessSpectroscopySPIE Proceedings
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<title>Advanced light sources for atomic absorption analysis</title>

2003

High-frequency electrodeless light sources (HF EDLS) are widely used as bright radiators of narrow and intensive atomic and ionic spectral lines, covering the spectrum from VUV to IR. Main characteristics of HF EDLS are high emitted spectral line intensity, long service life, and in general, narrow spectral line shapes because of low-pressure of filling elements. In this work we give a short overview of the use of HF EDLS, containing Hg, Te, Se, Zn, Pb, As, Sb, Bi, Tl, In, Cd, Sn, in Zeeman Atomic absorption devices for assaying natural, drinking, waste and technical water as well as air, soil, food products and biological samples. The first steps are made for optimization of Ge, Ga, P, S, …

Zeeman effectSpectrometerbusiness.industryAnalytical chemistrychemistry.chemical_elementCathodeSpectral linelaw.inventionHafniumsymbols.namesakechemistryAntimonylawsymbolsOptoelectronicsbusinessAbsorption (electromagnetic radiation)Atomic absorption spectroscopySPIE Proceedings
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Correction parameters in X-ray fluorescence analysis applying the limit dilution method (LDM)

1992

This paper is a study of the interelemental effect and its correction based on the mathematical model used to develop LDM in XRF analysis. A “compensation coefficient” is defined which is obtained from the quotient of the mass absorption coefficients of the problem and the standard (μs*/μp*). This coefficient compensates the effects produced by interactions between the analyt and the interferences and therefore acts as a correction factor for the interelemental effect within this theoretical model. The model itself establishes a simple relation of the “compensation coefficient” and the Y/H correction parameters for the unknown and the standard. An algorithm is proposed for calculating the “…

ZirconiumMass absorptionChemistryMathematical analysisAnalytical chemistrychemistry.chemical_elementX-ray fluorescenceBiochemistryAnalytical ChemistryCompensation (engineering)DilutionFluorescence intensityLimit (mathematics)QuotientFresenius' Journal of Analytical Chemistry
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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The 30 Year Search for the Compact Object in SN 1987A

2018

Despite more than 30 years of searches, the compact object in Supernova (SN) 1987A has not yet been detected. We present new limits on the compact object in SN 1987A using millimeter, near-infrared, optical, ultraviolet, and X-ray observations from ALMA, VLT, HST, and Chandra. The limits are approximately 0.1 mJy ($0.1\times 10^{-26}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) at 213 GHz, 1 Lsun ($6\times 10^{-29}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) in optical if our line-of-sight is free of ejecta dust, and $10^{36}$ erg s$^{-1}$ ($2\times 10^{-30}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) in 2-10 keV X-rays. Our X-ray limits are an order of magnitude less constraining than previous limits because we use a…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstrophysicsPhysical Chemistry01 natural sciences7. Clean energyAtomicLuminosityParticle and Plasma PhysicsQB460Astrophysics::Solar and Stellar AstrophysicsAbsorption (logic)10. No inequality010303 astronomy & astrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)SUPERNOVA REMNANT 1987ASupernovaAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesPhysical Chemistry (incl. Structural)NEUTRON-STARSCIRCUMSTELLAR RINGX-RAYSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBLUE SUPERGIANTSAstrophysics::Cosmology and Extragalactic AstrophysicsCompact starAstronomy & Astrophysicsstars: neutronneutron [stars]Pulsarindividual [supernovae]0103 physical sciencesblack holes [stars]NuclearINTEGRAL FIELD SPECTROSCOPY010306 general physicsUNDERGROUND SCINTILLATION TELESCOPEsupernovae: individualAstrophysics::Galaxy AstrophysicsOrganic ChemistryMolecularAstronomy and AstrophysicsHUBBLE-SPACE-TELESCOPEEffective temperatureNeutron starRAY EMISSION-LINESPhysics and Astronomyindividual (SN 1987A) [supernovae]13. Climate actionSpace and Planetary ScienceLARGE-MAGELLANIC-CLOUD[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]stars: black holes
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Prise en eau par composites carbone/époxy et leur effet sur le comportement mécanique : application aux réparations de structures en composite par co…

2013

Le travail présenté dans ce mémoire avait pour objectif d’étudier le processus de la pénétration d'eau dans les composites en carbone/époxyde dans un premier temps, et dans un deuxième temps, d’étudier l’effet de la prise en eau par ces matériaux sur les performances mécaniques des composites et leur joints collés. L'intégration de ces phénomènes physiques dans la modélisation numérique est d'une grande importance dans la prédiction de la durabilité d’une structure en composite subissant un vieillissement hygrothermique. Par conséquent, ce travail consiste non seulement en des observations expérimentales, mais aussi en des simulations numériques. Des corrélations entre les résultats obtenus…

[ SPI.OTHER ] Engineering Sciences [physics]/Other[SPI.OTHER] Engineering Sciences [physics]/OtherCarbon/epoxy compositesMechanical performanceTwo-phase diffusion modelResidual Property ModeWater uptake behaviourLinear-exponential traction separation lawComportement d'absorption d'eauModèle de diffusion à deux-phasesModèle RPMJoints collésComposites carbone/époxydeNumerical simulationsLoi de traction-séparation linéaire-exponentielAdhesive bonded jointsPerformances mécaniquesSimulations numériques
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All-optical extinction-ratio enhancement of a 160 GHz pulse train by a saturable-absorber vertical microcavity

2006

International audience; A vertical-access passive all-optical gate has been used to improve the extinction ratio of a 160 GHz pico-second pulse train at 1555 nm. An extinction ratio enhancement of 6 dB is observed within an 8 nm bandwidth. Such a device is a promising candidate for low-cost all optical reamplication and reshaping (211) regeneration at 160 Gbits/s.

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Materials scienceExtinction ratiobusiness.industryNonlinear opticsSaturable absorption02 engineering and technology01 natural sciencesPulse shapingAtomic and Molecular Physics and Optics[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]010309 optics020210 optoelectronics & photonicsOptics[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]0103 physical sciences0202 electrical engineering electronic engineering information engineeringPulse wavePhotonicsbusinessUltrashort pulseQuantum well
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