Search results for "Instrumentation"

showing 10 items of 4914 documents

Oxygen K-edge XANES investigation of NicMg1−cO solid solutions

2005

A series of Ni(c)Mg(1-c)O solid solutions are characterized by means of synchrotron radiation X-ray diffraction and X-ray absorption near-edge-structure spectroscopy at oxygen K-edge (532 eV). A dramatic drop of the pre-edge peak intensity is observed in the Ni(c)Mg(1-c)O system upon dilution. It can be attributed to a decrease of 3d(8)(Ni(2+))-2p(O(2-)) mixing upon dilution with magnesium ions due to a decrease of the number of 3d vacancies as nickel ion is replaced by magnesium ion. Similarly, the decrease of the number of 4s and 4p vacancies also leads to a decrease of 4s4p(Ni(2+))-2p(O(2-)) hybridization, and hence a drop of intensities of features B and C. The features E and F are more…

ChemistrySpectrum AnalysisDrop (liquid)Analytical chemistrychemistry.chemical_elementSodium ChlorideOxygenAtomic and Molecular Physics and OpticsXANESAnalytical ChemistryDilutionOxygenSolutionsX-Ray DiffractionK-edgeNickelMagnesiumSpectroscopyInstrumentationMagnesium ionSpectroscopySolid solutionSpectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy
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Surface composition analysis during the oxidation of ferrites: A necessity

1998

The cationic composition of a titanium ferrite (Fe 2.5 Ti 0.5 O 4 ) has been followed by XPS during its oxidation in cation deficient phases (without crystallographic transformation) in order to reveal a dynamic segregation phenomenon. Indeed, during this oxidation, an important modification of the chemical composition of the first layers of the material has been revealed: below 350 °C, the titanium ferrites surface becomes richer in iron and poorer in titanium. But, if the reaction is extended above 400 °C, some titanium can move to the surface. This phenomenon has been interpreted on the basis of the differences of mobility of the different ions which are present in the material. Finally,…

ChemistrySpinelInorganic chemistryCationic polymerizationchemistry.chemical_elementComposition analysisengineering.materialCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsIonX-ray photoelectron spectroscopyengineeringFerrite (magnet)InstrumentationChemical compositionTitaniumThe European Physical Journal Applied Physics
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Thermal behaviour of anhydrous, dihydrate and (2/1) ethanol forms of 1-O-α-d-glucopyranosyl-d-mannitol

1998

Abstract The melting points of anhydrous 1-O-α- d -glucopyranosyl- d -mannitol, 1-O-α- d -glucopyranosyl- d -mannitol dihydrate and a new compound, 1-O-α- d -glucopyranosyl- d -mannitol-ethanol (2/1) were determined using differential scanning calorimetry. The melting onset values were 169.2 (3), 104.3 (18) and 158.7 (9), respectively, and the melting peak values were 171.4 (5), 107.9 (15) and 160.1 (6), respectively. 1-O-α- d -glucopyranosyl- d -mannitol dihydrate and 1-O-α- d -glucopyranosyl- d -mannitol-ethanol (2/1) decompose to anhydrous form when heated at slow heating rates. According to TG-FTIR measurements, 1-O-α- d -glucopyranosyl- d -mannitol-ethanol (2/1) lost its ethanol in the…

ChemistryThermal decompositionAnalytical chemistryCondensed Matter PhysicsThermogravimetryDifferential scanning calorimetrymedicineMelting pointAnhydrousMannitolPhysical and Theoretical ChemistryThermal analysisHydrateInstrumentationmedicine.drugThermochimica Acta
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Comparison of electron diffraction data from non-linear optically active organic DMABC crystals obtained at 100 and 300 kV

2000

During the recent past, we have synthesized a new class of molecules with intramolecular two-dimensional charge transfer upon excitation. The present report presents such a molecule, 2,6-bis(4-dimethylamino-benzylidene)-cyclohexanone (DMABC), with an unusually high value of the second-order non-linear optical (NLO) coefficients. In order to optimize the macroscopic NLO properties of the compounds, it is necessary to relate their first hyperpolarizability tensors at a molecular level to those at a crystal bulk level. This requires a complete structure determination and refinement. However, the growth of sufficiently large single crystals, which are needed for structural analysis and refineme…

Chemistrybusiness.industryDirect methodResolution (electron density)Ab initioHyperpolarizabilityAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsComputational physicsCrystalOpticsElectron diffractionDirect methodsTensorbusinessInstrumentationUltramicroscopy
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Effect of operation conditions of the drop-on-demand aerosol generator on aerosol characteristics: Pseudo-cinematographic and plasma mass spectrometr…

2014

Abstract The recently presented drop-on-demand (DOD) aerosol generator overcomes some of the drawbacks of pneumatic nebulization, as its aerosol is no longer generated by gas–liquid interaction. In the current study, an advanced imaging technique is presented, based on a CCD camera equipped with magnifying telecentric optics to allow for fast, automated and precise aerosol characterization as well as fundamental studies on the droplet generation processes by means of pseudo-cinematography. The DOD aerosol generator is thoroughly characterized regarding its droplet size distribution, which shows few distinct populations rather than a continuous distribution. Other important figures, such as …

Chemistrybusiness.industryDrop (liquid)Analytical chemistryPlasmaMass spectrometricAtomic and Molecular Physics and OpticsAnalytical ChemistryAerosolNebulizerOpticsOn demandAerosol generatorbusinessInstrumentationInductively coupled plasma mass spectrometrySpectroscopySpectrochimica Acta Part B: Atomic Spectroscopy
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Vertical and lateral drift corrections of scanning probe microscopy images

2010

A procedure is presented for image correction of scanning probe microscopy data that is distorted by linear thermal drift. The procedure is based on common ideas for drift correction, which the authors combine to a comprehensive step-by-step description of how to measure drift velocities in all three dimensions and how to correct the images using these velocities. The presented method does not require any knowledge about size or shape of the imaged structures. Thus, it is applicable to any type of scanning probe microscopy image, including images lacking periodic structures. Besides providing a simple, ready-to-use description of lateral and vertical drift correction, they derive all formul…

Chemistrybusiness.industryProcess Chemistry and Technologyscanning probe microscopyLinear driftLateral driftImage correction530Measure (mathematics)Surfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsScanning probe microscopyOpticsVertical driftThermalMaterials ChemistryElectrical and Electronic EngineeringbusinessInstrumentationJournal of Vacuum Science & Technology B, Nanotechnology and Microelectronics: Materials, Processing, Measurement, and Phenomena
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Application of infrared spectroscopy as Process Analytics Technology (PAT) approach in biodiesel production process utilizing Multivariate Curve Reso…

2019

Abstract Process Analytical Technology means at-line collection of analytical information from the process when the reaction is in progress. Obtained information enables process engineers to better control the Critical Process Parameters and direct the reaction to desirable routs. Near-infrared spectroscopy due to its analytical features, as well as the high capability of automation, versatile sampling and spectral acquisition methods is a useful tool in process monitoring when coupled to chemometrics. The Multiple Scatter Correction preprocessing technique and Alternative Least Square method can extract spectral and concentration information of a reaction mixture simultaneously, were emplo…

Chemistrybusiness.industryProcess analytical technologyNear-infrared spectroscopyProcess (computing)02 engineering and technologyWork in process010402 general chemistry021001 nanoscience & nanotechnology01 natural sciencesAutomationAtomic and Molecular Physics and Optics0104 chemical sciencesAnalytical ChemistryChemometricsBiodiesel production0210 nano-technologyBiological systembusinessSpectroscopyInstrumentationSpectroscopySpectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy
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Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

2023

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy $\gamma$-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs whi…

Cherenkov Telescope ArrayGamma rays: generalstatistical [methods]energy spectrumFOS: Physical sciencesVHESettore FIS/05 - Astronomia E Astrofisicacosmic raysMethods: data analysissupernovadata analysis [methods][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Cosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov Telescope Arra ; alactic Supernova Remnants ; PeVatrons ;Methods: statisticalgalactic PeVatronsHigh Energy Astrophysical Phenomena (astro-ph.HE)emission spectrum) supernovae: general [(stars]Astronomy and AstrophysicssensitivityobservatoryGalactic PeVatronscosmic radiationspectralgalaxyhadron(Stars:) supernovae: generalAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalgeneral [gamma rays]signature
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The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

2018

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the…

Cherenkov Telescope ArrayHigh-energy astrophysical phenomenaCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomyenergy resolution7. Clean energy01 natural sciencesSpace missionlaw.inventionIceCubeEinstein TelescopelawObservatoryLIGO010303 astronomy & astrophysicsKM3NeTPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Applied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionGamma-ray astronomyGamma-ray polarizationCondensed Matter Physicsphoton: energyobservatoryNuclear astrophysicsApace missionAstrophysics - High Energy Astrophysical Phenomenaperformancedetector: technologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstspace missionCompton and pair creation telescopeTelescope0103 physical sciencessupernovaElectroniccalorimetergamma ray: detectorOptical and Magnetic MaterialsKAGRAElectrical and Electronic Engineering010306 general physicsTime domain astronomyLISAGamma-ray astronomyEinstein TelescopeAstronomyInstitut für Physik und AstronomieTime-domain astronomyCherenkov Telescope ArraysensitivityLIGOmessengerKM3NeTVIRGO13. Climate actionCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineeringddc:520galaxyCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic Engineering[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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