Search results for "RADIATION"

showing 10 items of 5298 documents

Study of the reactive dynamics of nanometric metallic multilayers using Molecular Dynamics: the Al−Ni system

2012

A molecular dynamics study of a layered Ni-Al-Ni system is developed using an embedded atom method potential. The specific geometry is designed to model a Ni-Al nanometric metallic multilayer. The system is initially thermalized at the fixed temperature of 600 K. We first observe the interdiffusion of Ni and Al at the interfaces, which is followed by the spontaneous phase formation of B2-NiAl in the Al layer. The solid-state reaction is associated with a rapid system's heating which further enhances the diffusion processes. NiAl phase is organized in small regions separated by grain boundaries. This study confirms the hypothesis of a layer-by-layer development of the new phase. For longer t…

Exothermic reactionNialMaterials scienceDiffusionmultilayersIntermetallicnanometric metallic multilayersNanotechnology02 engineering and technology01 natural sciencesinterfacesMolecular dynamicsPhase (matter)0103 physical sciencesGeneral Materials Scienceintermetallics010306 general physicscomputer.programming_languageRadiationnanoscale effects[CHIM.MATE]Chemical Sciences/Material chemistry021001 nanoscience & nanotechnologyCondensed Matter PhysicsMicrostructuremolecular dynamics[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Chemical physics[ CHIM.MATE ] Chemical Sciences/Material chemistryGrain boundary[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]0210 nano-technologycomputer
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Protocols for UV camera volcanic SO2 measurements

2010

Abstract Ultraviolet camera technology offers considerable promise for enabling 1 Hz timescale acquisitions of volcanic degassing phenomena, providing two orders of magnitude improvements on sampling frequencies from conventionally applied scanning spectrometer systems. This could, for instance enable unprecedented insights into rapid processes, such as strombolian explosions, and non-aliased corroboration with volcano geophysical data. The uptake of this technology has involved disparate methodological approaches, hitherto. As a means of expediting the further proliferation of such systems, we here study these diverse protocols, with the aim of suggesting those we consider optimal. In part…

ExpeditingVignettingSpectrometerSampling (statistics)Settore GEO/08 - Geochimica E Vulcanologiaultraviolet camera; volcanic SO2 monitoring; volcanic gas geochemistryvolcanic SO2 monitoringGeophysicsNarrowbandGeochemistry and PetrologyCalibrationultraviolet cameraAbsorption (electromagnetic radiation)volcanic gas geochemistryOrder of magnitudeGeologyRemote sensingJournal of Volcanology and Geothermal Research
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Light-component spectrum of the primary cosmic rays in the multi-TeV region measured by the ARGO-YBJ experiment

2012

The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-coverage detector which is in stable data taking in its full configuration since November 2007 at the YBJ International Cosmic Ray Observatory (4300 m a.s.l., Tibet, People's Republic of China). In this paper the measurement of the light-component spectrum of primary cosmic rays in the energy region $(5\textdiv{}200)\text{ }\text{ }\mathrm{TeV}$ is reported. The method exploited to analyze the experimental data is based on a Bayesian procedure. The measured intensities of the light component are consistent with the recent CREAM results and higher than that obtained adding the proton and helium sp…

Extended Air Showers Cosmic Rays Gamma Ray sourcesNuclear and High Energy PhysicsProtonTIBETAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerchemistry.chemical_elementCosmic rayHELIUM SPECTRAAstrophysicsPROTONBayesian methodCASCADESSpectral lineSettore FIS/05 - Astronomia E AstrofisicaNuclear magnetic resonanceCosmic-ray observatoryHeliumPhysicsRange (particle radiation)ENERGY-RANGEBALLOON EXPERIMENTNUCLEISettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for Astrophysicslight component spectrumchemistryEnergy (signal processing)SYSTEM
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The fate of silver ions in the photochemical synthesis of gold nanorods: an Extended X-ray Absorption Fine Structure analysis

2009

Water-soluble gold nanorods (Au NRs) were synthesized using a silver-ion mediated photochemical route under UV irradiation. Extended X-ray Absorption Fine Structure (EXAFS) measurements on the Ag K-edge were performed on samples obtained at different Ag/Au ratios and at increasing irradiation times in order to investigate the fate of silver ions during the growth of Au NRs. EXAFS measurements allowed to probe the chemical state and the local environment of silver in the final product. Experimental data suggest that Ag atoms are placed on top of the Au particles as metallic Ag(0), while no significant contribution to the EXAFS spectra comes from AgBr or other Ag(+) based species. The reporte…

Extended X-ray absorption fine structureChemistryAnalytical chemistryNanoparticleEXAFS gold nanoparticle TEMPhotochemistryIonInorganic ChemistryMetalChemical statevisual_artvisual_art.visual_art_mediumNanorodIrradiationAbsorption (chemistry)
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Extended X-Ray Absorption Fine Structure Spectroscopy of Perovskite-Type Compounds

2000

Application of the extended x-ray absorption fine structure (EXAFS) spectroscopy to a study of the local atomic structure in perovskitetype materials is discussed on the example of several compounds (m-WO3, NaxWO3, ReO3 and FeF3). The sensitivity of the EXAFS to the out-of-center and rotational distortions is discussed in details.

Extended X-ray absorption fine structureChemistrySurface-extended X-ray absorption fine structureAnalytical chemistrySpectroscopyAbsorption (electromagnetic radiation)Perovskite (structure)X-ray absorption fine structure
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Extension of the MIRS computer package for the modeling of molecular spectra : from effective to full ab initio ro-vibrational hamiltonians in irredu…

2012

The MIRS software for the modeling of ro-vibrational spectra of polyatomic molecules was considerably extended and improved. The original version (Nikitin, et al. JQSRT, 2003, pp. 239--249) was especially designed for separate or simultaneous treatments of complex band systems of polyatomic molecules. It was set up in the frame of effective polyad models by using algorithms based on advanced group theory algebra to take full account of symmetry properties. It has been successfully used for predictions and data fitting (positions and intensities) of numerous spectra of symmetric and spherical top molecules within the vibration extrapolation scheme. The new version offers more advanced possib…

ExtrapolationAb initioFOS: Physical sciences02 engineering and technologyPoint group01 natural scienceshigh-resolution infrared spectroscopyTheoretical physicsAb initio quantum chemistry methodsPhysics - Chemical PhysicsQuantum mechanics0103 physical sciencesMolecular symmetrypolyadsSpectroscopycomputational spectroscopyChemical Physics (physics.chem-ph)Physics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation010304 chemical physicsab initio calculationseffective hamiltoniansRotational–vibrational spectroscopy021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Opticsmolecular symmetryPhysics - Atmospheric and Oceanic Physicsvibration-rotation spectroscopy[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Atmospheric and Oceanic Physics (physics.ao-ph)Curve fittingirreducible tensors0210 nano-technologyGroup theory
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Gain, detuning, and radiation patterns of nanoparticle optical antennas

2008

International audience; For their capability to localize and redirect electromagnetic field, metal nanoparticles have been recently viewed as efficient nanoantenna operating in the optical regime. In this article, we experimentally investigated the optical responses of coupled gold antenna pairs and measured the critical parameters defining antenna characteristics: resonant frequencies and bandwidths, detuning and gains, and radiation patterns.

FAR-FIELDElectromagnetic fieldPLASMONIC NANOPARTICLEPhysics::OpticsNanoparticle02 engineering and technologySILVER NANOPARTICLESRadiation01 natural sciencesNANOANTENNASOptics[ PHYS.COND.CM-MSQHE ] Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall]0103 physical sciencesSCATTERING[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics010306 general physicsMetal nanoparticles[PHYS.COND.CM-MSQHE]Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryRESONANCE021001 nanoscience & nanotechnologyCondensed Matter PhysicsDIMERSElectronic Optical and Magnetic MaterialsSINGLE[SPI.OPTI]Engineering Sciences [physics]/Optics / PhotonicQuasiparticleOptoelectronics[ SPI.NANO ] Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics[ SPI.OPTI ] Engineering Sciences [physics]/Optics / PhotonicAntenna (radio)EMISSION0210 nano-technologybusinessNEAR-FIELDPhysical Review B
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Direct validation of FVC, LAI and FAPAR VEGETATION/SPOT derived products using LSA SAF methodology

2007

The aim of this work is to perform a direct validation of fraction of vegetation cover (FVC), leaf area index (LAI) and fraction of absorbed photosynthetically active radiation (FAPAR) resulting products from applying the LSA SAF methodology to VEGETATION BRDF data. LSA SAF adapted algorithms were tested in adequate test sites comprising different continental biomes covering a wide range of FVC, LAI and FAPAR values. Results seem to indicate the competitiveness of LSA SAF proposed methodology to retrieve remotely sensed biophysical parameters. A noticeable good agreement regarding the ground measurements was found. The overall accuracy (RAISE) is around 20% for FVC and FAPAR and around 15% …

FEV1/FVC ratioPhotosynthetically active radiationBiomeEnvironmental scienceEnhanced vegetation indexVegetationBidirectional reflectance distribution functionLeaf area indexVegetation coverRemote sensing2007 IEEE International Geoscience and Remote Sensing Symposium
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

2016

We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles ra…

FLUORESCENCE YIELDAstronomymagnetic monopolemagnetic fieldAstrophysics7. Clean energy01 natural sciencesObservatoryUHE Cosmic Raysair-showerMonte Carlo010303 astronomy & astrophysicsMagnetic Monopolesmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicscritical phenomenaFLUORESCENCE YIELD; ENERGY LOSS; DETECTORAugerMagnetic fieldobservatoryLorentz factorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical Phenomenaspatial distribution [showers]LorentzENERGY LOSSatmosphere [showers]energyFLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]airmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Magnetic monopoleFOS: Physical sciencesCosmic rayNuclear physicssymbols.namesakecosmic rays0103 physical sciencesddc:530High Energy PhysicsDETECTORCiencias Exactasfluorescence [detector]Pierre Auger Observatorybackground010308 nuclear & particles physicsFísicaASTROFÍSICAUniversefluxultrarelativistic magnetic monopolesAir shower13. Climate actionExperimental High Energy PhysicsrelativisticgalaxyENERGY-LOSS
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Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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