Search results for "Auger"

showing 10 items of 144 documents

Initial chemical transport of reducing elements and chemical reactions in oxide cathode base metal

2002

Abstract In the present work, the formation of compounds associated to the diffusion of reducing elements (Mg and Al) to the nickel surface of a one-piece oxide cathode has been studied. Those compounds have been evidenced after the annealing steps at high temperature performed on cathode base metal prior to the emitting coating deposition. Therefore, they form the “initial” interface between the nickel and the coating, in other words, the interface existing at the beginning of cathode life. Extensive analysis to characterize the nickel base prior to coating deposition has been performed by means of scanning electron microscopy (SEM) coupled with energy dispersive X-ray spectroscopy (EDX), …

Auger electron spectroscopyScanning electron microscopeAnalytical chemistryGeneral Physics and Astronomychemistry.chemical_elementSurfaces and InterfacesGeneral Chemistryengineering.materialCondensed Matter PhysicsCathodeSurfaces Coatings and Filmslaw.inventionNickelchemistryCoatinglawTransmission electron microscopyengineeringGrain boundary diffusion coefficientSpectroscopyApplied Surface Science
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Diamond nucleation on iridium: local variations of structure and density within the BEN layer

2009

Abstract The diamond nuclei generated by the bias enhanced nucleation (BEN) on iridium are gathered in well defined areas (“domains”). In atomic force microscopy (AFM) measurements they become manifest in a 1 nm downward step. The fine structure of the carbon layer inside and outside these domains has been studied by small spot Auger electron spectroscopy (AES), high resolution transmission electron microscopy (HRTEM), AFM and lateral force microscopy (LFM). The Auger spectra of the carbon KLL peak taken in an ultra high vacuum setup revealed diamond features inside and more graphitic features outside the domains. The comparison with the intensity of the Auger signal originating from the un…

Auger electron spectroscopybusiness.industryMechanical EngineeringUltra-high vacuumNucleationchemistry.chemical_elementDiamondGeneral Chemistryengineering.materialMolecular physicsElectronic Optical and Magnetic MaterialsAugerOpticschemistryTransmission electron microscopyMaterials ChemistryengineeringElectrical and Electronic EngineeringbusinessHigh-resolution transmission electron microscopyCarbon
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Influence of the passive film properties and residual stresses on the micro-electrochemical behavior of duplex stainless steels

2010

In the present paper, the chemical composition of passive films formed on both phases of two types of duplex stainless steels (UNS S31803 and UNS S32304) is determined at the micro-scale using Auger electron spectroscopy (AES). Samples were either mechanically polished (down to diamond pastes) or electrochemically etched in acidic solutions. The micro-electrochemical behavior of samples was then determined in sodium chloride media by means of the electrochemical micro-cell technique (capillary diameters of 30 μm). The results obtained were analyzed considering the passive film chemical composition. Quantitative relationships between electrochemical parameters and the distribution of chromiu…

AusteniteAuger electron spectroscopyMaterials sciencePassivationGeneral Chemical EngineeringSurface stressMetallurgyOxideCorrosionchemistry.chemical_compoundchemistryResidual stressElectrochemistrySurface layerElectrochimica Acta
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Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory.

2012

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna s…

Ciencias Astronómicas[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomyAstrophysics::High Energy Astrophysical Phenomenashowers: atmosphere | cosmic radiation: UHE | polarization: effect | Auger | radio wave: emission | radio wave: detector | galaxy | background | reflection | noise | detector: networkFOS: Physical sciencesCosmic ray01 natural sciencesSignalKASCADEMHZOpticsSIGNALS0103 physical sciencesTransient responseTime domain010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMathematical Physics[PHYS]Physics [physics]PhysicsPierre Auger ObservatorySPECTRUMLarge detector systems for particle and astroparticle physics010308 nuclear & particles physicsbusiness.industryPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]ATMOSFERA (MONITORAMENTO)Air showerAntennaExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONAntennasFísica nuclearAntenna (radio)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory an…

2014

Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 1019 eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 1019 eV. No significant devia…

Ciencias FísicasAstronomyRaysAstrophysicsAstroparticle physics; Cosmic rays01 natural scienceslaw.inventionPierrelawAnisotropyTelescope010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[PHYS]Physics [physics]Energy[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicRadiación cósmicaAugerCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsCIENCIAS NATURALES Y EXACTASHigh[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raySURFACE DETECTORICECUBETelescopeAIR-SHOWER ARRAYDirectionscosmic rays0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsArraySpectral densitySpherical harmonicsFísicaAstronomy and AstrophysicsASTROFÍSICAUltra[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaDipoleRESOLUTIONSpace and Planetary ScienceExperimental High Energy PhysicsQuadrupoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Clean and ordered surfaces of CeNi 2 Ge 2 layers on W(110)

1997

Investigations of the geometric and electronic properties of ternary Ce-based heavy fermion systems CeT2X2 (T : Ni,Pd,Rh; X : Ge,Si) were carried out by means of electron spectroscopic methods. The main problem for these surface-sensitive techniques is the preparation of well-ordered and atomically clean surfaces. The ternary substance CeNi2Ge2 was grown on a W(110) substrate by MBE with subsequent annealing. A nearly layer-by-layer growth mode was detected using MEED. The annealed layers are ordered, but show small Ni2Ge crystalline islands. The composition was characterised by means of AES in dependence of the substrate as well as the annealing temperature. Electronic properties are inves…

Condensed Matter::Materials ScienceAuger electron spectroscopyCrystallographyX-ray photoelectron spectroscopyChemistryAnnealing (metallurgy)Crystal growthThin filmTernary operationBiochemistryElectron spectroscopyMolecular beam epitaxyFresenius' Journal of Analytical Chemistry
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Properties of Co/sub 2/YZ Heusler compounds

2005

Heusler compounds of Co/sub 2/XY composition (Co/sub 2/Cr/sub 0.6/Fe/sub 0.4/Al, Co/sub 2/FeSi) offer a variety of half-metallic ferromagnetic materials. These were prepared by arc melting and comprehensively characterized by means of X-ray diffraction ( XRD), Mossbauer spectroscopy, magnetic X-ray circular dichroism spectroscopy (MXCD), superconducting quantum interference device (SQUID) magnetometry, electron spectroscopy for chemical analysis (ESCA), extended X-ray absorption fine structure (EXAFS) and Auger electron spectroscopy (AES) depth profiling. Structural disorder phenomena, magnetic hysteresis, magnetic moments, magnetic transition temperatures and Curie temperature were obtaine…

Condensed Matter::Materials ScienceMagnetizationAuger electron spectroscopyMaterials scienceCondensed matter physicsFerromagnetismMagnetic circular dichroismCurie temperatureMagnetic hysteresisSpectroscopyElectron spectroscopyINTERMAG Asia 2005. Digests of the IEEE International Magnetics Conference, 2005.
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Intra-atomic versus interatomic process in resonant Auger spectra at the TiL23edges in rutile

2001

The two components of the Ti ${L}_{23}{M}_{23}V$ Auger transition recorded on a stoichiometric rutile crystal are identified as ${L}_{2}{M}_{23}V$ and ${L}_{3}{M}_{23}V$ contributions. This assignment is evidenced by concordant data relative to resonances of the LMV decay at the Ti ${L}_{23}$ thresholds and to Auger emission recorded in coincidence with the ${2}_{1/2}$ and ${2}_{3/2}$ photoemission at a photon energy far above the Ti ${L}_{23}$ edges. The ${L}_{3}{M}_{23}V$ transition is shown to follow either the direct photoexcitation of a ${2}_{3/2}$ electron or the fast Coster-Kronig decay of a ${2}_{1/2}$ photohole. Although specific LMV contributions related to valence orbitals are id…

CrystalPhysicsValence (chemistry)Atomic orbitalElectronPhoton energyAtomic physicsElectron spectroscopySpectral lineAugerPhysical Review B
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Resonant Photoelectron Diffraction

2013

A layout of a resonant photoelectron diffraction, RESPED, experiment is described from the theoretical basis to the data acquisition and analysis procedures. The theory of the resonance between the directly emitted photoelectron of a selected valence band and the electron emitted by autoionization (Auger) of the same valence band is presented within a formal frame. The critical issue of the angular symmetry and distribution of the resonating electron is discussed in connection with the current computational protocols for photoelectron diffraction, PED, analysis. A few representative applications are presented, where RESPED is shown to overcome some limitations of conventional PED thanks to …

DiffractionMaterials scienceValence (chemistry)AutoionizationPhysics::Atomic and Molecular ClustersValence bandEndohedral fullereneElectronAtomic physicsVolume concentrationAuger
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