Search results for "Visible"

showing 10 items of 351 documents

Low-dimensional non-toxic A 3 Bi 2 X 9 compounds synthesized by a dry mechanochemical route with tunable visible photoluminescence at room temperature

2019

We have synthesized fifteen inorganic and hybrid organic-inorganic non-toxic A3Bi2X9 compounds (A = K+, Rb+, Cs+, CH3NH3+ and HC(NH2)2+; X = I−, Br−, Cl−) through dry mechanochemistry. We demonstrate that this synthetic method is very well suited to prepare compounds from poorly soluble precursors, allowing thus the preparation of so far unreported compounds. X-ray diffraction analysis demonstrates the high crystallinity of the so-formed ternary bismuth halides. Furthermore, we show that, through substitution of the A-cation and X-anion, the bandgap of these compounds can be tuned to absorb throughout the whole visible spectrum. As-prepared powders of Cs3Bi2Br9 and Cs3Bi2I9 without any pass…

PhotoluminescenceMaterials scienceBand gapHalidechemistry.chemical_element02 engineering and technologyGeneral ChemistryQuímica010402 general chemistry021001 nanoscience & nanotechnologyPhotochemistry01 natural sciences0104 chemical sciencesBismuthCrystallinitychemistryMechanochemistryMaterials Chemistry0210 nano-technologyTernary operationMaterialsVisible spectrumJournal of Materials Chemistry C
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Charge reconstruction in large-area photomultipliers

2018

Large-area PhotoMultiplier Tubes (PMT) allow to efficiently instrument Liquid Scintillator (LS) neutrino detectors, where large target masses are pivotal to compensate for neutrinos' extremely elusive nature. Depending on the detector light yield, several scintillation photons stemming from the same neutrino interaction are likely to hit a single PMT in a few tens/hundreds of nanoseconds, resulting in several photoelectrons (PEs) to pile-up at the PMT anode. In such scenario, the signal generated by each PE is entangled to the others, and an accurate PMT charge reconstruction becomes challenging. This manuscript describes an experimental method able to address the PMT charge reconstruction …

PhotomultiplierLiquid detectorsvisible and IR photons (vacuum) (photomultipliers HPDs others)Physics - Instrumentation and Detectorsgas and liquid scintillators)Physics::Instrumentation and DetectorsPhoton detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others)FOS: Physical sciencesvisible and IR photons (vacuum) (photomultipliers HPDsScintillatorvisible and IR photons (vacuum) (photomultipliers01 natural sciencesParticle detectorNOsymbols.namesakeOptics0103 physical sciencesCalorimeter methods010306 general physicsInstrumentationPhoton detectors for UVMathematical PhysicsPhysicsscintillation and light emission processes (solid gas and liquid scintillators)010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleWiener filterDetectorReconstruction algorithmScintillators scintillation and light emission processes (solid gas and liquid scintillators)Instrumentation and Detectors (physics.ins-det)Scintillatorscintillation and light emission processes (solidCalorimeter methods; Liquid detectors; Photon detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others); Scintillators scintillation and light emission processes (solid gas and liquid scintillators)Photon detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others)Neutrino detectorHPDsCalorimeter methodScintillatorsScintillators scintillation and light emission processes (solid gas and liquid scintillators)symbolsLiquid detectorCalorimeter methods; Liquid detectors; Photon detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others); Scintillators scintillation and light emission processes (solid gas and liquid scintillators)Deconvolutionbusinessothers)scintillation and light emission processes (solid gas and liquid scintillators)
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A laser-based system for a fast and accurate measurement of gain and linearity of photomultipliers

2018

This paper describes a method for the measurement of gain and linearity of photomultipliers (PMTs). Gain and linearity are two fundamental parameters to use properly a PMT in several physics experiments. In the developed system light is laser generated and adressed to the PMT through a set of optical fibers. The data acquisition system consists in a commercial 16 channel digitizer coupled to a custom front-end board. With the chosen digitizer the system is scalable to test up to 16 PMTs, with the aid of a light distribution system and a multi-channel version of the front-end board. Data analysis is performed by a custom acquisition software. A 1.5» Hamamatsu PMT is used to validate the syst…

PhotomultiplierOptical fiberMaterials scienceDistribution (number theory)Fiber Laservisible and IR photons (vacuum) (photomultipliers01 natural sciencesAnalogue electronic circuit030218 nuclear medicine & medical imaginglaw.invention03 medical and health sciences0302 clinical medicineData acquisitionOpticslawFront-end electronics for detector readout0103 physical sciencesPhoton detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others); Front-end electronics for detector readout; Analogue electronic circuits; Fiber LasersPhoton detectors for UVInstrumentationMathematical PhysicsFiber LasersData processing010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleLinearityLaserPhoton detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others)HPDsAnalogue electronic circuitsothers)businessJournal of Instrumentation
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A precise photometric ratio via laser excitation of the sodium layer - I. One-photon excitation using 342.78 nm light

2020

The largest uncertainty on measurements of dark energy using type Ia supernovae is presently due to systematics from photometry; specifically to the relative uncertainty on photometry as a function of wavelength in the optical spectrum. We show that a precise constraint on relative photometry between the visible and near-infrared can be achieved in upcoming surveys (such as in LSST at the Vera C. Rubin Observatory) via a mountaintop-located laser source tuned to the 342.78 nm vacuum excitation wavelength of neutral sodium atoms. Using a high-power (500 W) laser modified from laser guide star studies, this excitation will produce an artificial star (which we term a "laser photometric ratio s…

PhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicslaw.inventionPhotometry (optics)techniques: photometricOpticslawAstrophysics::Solar and Stellar Astrophysicsdark energyInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsPhysicsbusiness.industrymethods:observationalAstrophysics::Instrumentation and Methods for AstrophysicsSodium layerAstronomy and AstrophysicstelescopesLaser[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]instrumentation: miscellaneousWavelengthLaser guide starSpace and Planetary Science[SDU]Sciences of the Universe [physics]instrumentation:miscellaneousmethods: observationalbusinesstechniques:photometricAstrophysics - Instrumentation and Methods for AstrophysicsExcitationVisible spectrumAstrophysics - Cosmology and Nongalactic Astrophysics
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Effect of quantized conductivity on the anomalous photon emission radiated from atomic-size point contacts

2019

We observe anomalous visible to near-infrared electromagnetic radiation emitted from electrically driven atomic-size point contacts. We show that the number of photons released strongly depends on the quantized conductance steps of the contact. Counter-intuitively, the light intensity features an exponential decay dependence with the injected electrical power. We propose an analytical model for the light emission considering an out-of-equilibrium electron distribution. We treat photon emission as bremsstrahlung process resulting from hot electrons colliding with the metal boundary and a find qualitative accord with the experimental data.

PhotonQC1-999FOS: Physical sciences02 engineering and technologybremsstrahlung01 natural sciences7. Clean energyElectromagnetic radiationelectromigrationMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciences[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]Electrical and Electronic EngineeringExponential decay010306 general physicsPhysicsCondensed Matter - Mesoscale and Nanoscale Physicsquantized conductivityPhysicsBremsstrahlungConductancevisible light emission021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsLight intensityAtomic radiuspoint contactLight emissionAtomic physics0210 nano-technologyOptics (physics.optics)BiotechnologyPhysics - Optics
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Dependence of polytetrafluoroethylene reflectance on thickness at visible and ultraviolet wavelengths in air

2020

[EN] Polytetrafluoroethylene (PTFE) is an excellent diffuse reflector widely used in light collection systems for particle physics experiments. However, the reflectance of PTFE is a function of its thickness. In this work, we investigate this dependence in air for light of wavelengths 260 nm and 450 nm using two complementary methods. We find that PTFE reflectance for thicknesses from 5 mm to 10 mm ranges from 92.5% to 94.5% at 450 nm, and from 90.0% to 92.0% at 260 nm We also see that the reflectance of PIFE of a given thickness can vary by as much as 2.7% within the same piece of material. Finally, we show that placing a specular reflector behind the PTFE can recover the loss of reflectan…

Physics - Instrumentation and DetectorsFOS: Physical sciencesLibrary science7. Clean energy01 natural sciences030218 nuclear medicine & medical imagingSynthetic materialsTECNOLOGIA ELECTRONICA03 medical and health sciences0302 clinical medicinePolitical science0103 physical sciencesmedia_common.cataloged_instanceEuropean unionInstrumentationUltraviolet radiationMathematical Physicsmedia_common010308 nuclear & particles physicsEuropean researchTime projection Chambers (TPC)Instrumentation and Detectors (physics.ins-det)Visible radiationDouble-beta decay detectorsReflectivityDetector design and construction technologies and materialsNational laboratory
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Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina -Comision Nacional de Energia Atomica; Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT); Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargue; NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia -the Australian Research Council; Braz…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyPerformance of High Energy Physics Detector01 natural sciences7. Clean energyEtc)030218 nuclear medicine & medical imaging0302 clinical medicineFront-end electronics for detector readoutAPDsInstrumentationphysics.ins-detPhoton detectors for UVMathematical PhysicsInstrumentation et méthodes en physiqueEBCCDsVisible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)electronicsSettore FIS/01 - Fisica SperimentaleCalibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UVPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsInstrumentation and Detectors (physics.ins-det)charged particleAPDs; Calibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UV; CCDs; Cluster finding; CMOS imagers; EBCCDs; EMCCDs; Etc); Front-end electronics for detector readout; Pattern recognition; G-APDs; Si-PMTs; Visible and IR photons (solid-state) (PIN diodesAugerobservatorydensity [muon]Pattern recognition cluster finding calibration and fitting methodG-APDsChristian ministryupgradeddc:620Astrophysics - Instrumentation and Methods for Astrophysicsperformanceatmosphere [showers]Land accessCherenkov counter: waterairAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesPolitical sciencePattern recognition0103 physical sciencesmuon: densityFront-end electronics for detector readout; Pattern recognitionphotomultiplier: siliconHigh Energy Physicscosmic radiation: UHE[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610CMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Engineering & allied operationsscintillation counterCalibration and fitting methodsshowers: atmosphere010308 nuclear & particles physicswater [Cherenkov counter]Cluster findingAutres mathématiquesCCDsEMCCDsResearch councilefficiencyExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::ExperimentHumanitiesRAIOS CÓSMICOSastro-ph.IM
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The first coronal mass ejection observed in both visible-light and UV HI Ly-α channels of the Metis coronagraph on board Solar Orbiter

2021

Context.The Metis coronagraph on board Solar Orbiter offers a new view of coronal mass ejections (CMEs), observing them for the first time with simultaneous images acquired with a broad-band filter in the visible-light interval and with a narrow-band filter around the H ILy-αline at 121.567 nm, the so-called Metis UV channel.Aims.We show the first Metis observations of a CME, obtained on 16 and 17 January 2021. The event was also observed by the EUI/FSI imager on board Solar Orbiter, as well as by other space-based coronagraphs, such as STEREO-A/COR2 and SOHO/LASCO/C2, whose images are combined here with Metis data.Methods.Different images are analysed here to reconstruct the 3D orientation…

Physics010504 meteorology & atmospheric sciences[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Sun: coronaSun: coronal mass ejections (CMEs)Astronomy and AstrophysicsAstrophysicsAlpha (navigation)Sun: UV radiation01 natural scienceslaw.inventionOn boardOrbiterSpace and Planetary Sciencelaw0103 physical sciencesCoronal mass ejectionMetis010303 astronomy & astrophysicsCoronagraphSun: atmosphere0105 earth and related environmental sciencesVisible spectrumSun: atmosphere – Sun: corona – Sun: UV radiation – Sun: coronal mass ejections (CMEs)
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White-light Fourier transformer with low chromatic aberration.

1992

A simple Fourier transformation system working with broadband parallel illumination is presented. The proposed setup, consisting of two on-axis zone plates and an achromatic objective, allows us to obtain the achromatic Fourier transform representation of the input at a finite distance with a low chromatic aberration. The discussion of the system, using the Fresnel diffraction theory, leads to an analytical expression to evaluate the transversal and longitudinal chromatic aberrations. It is shown that the resulting chromatic aberrations for typical values of the involved parameters are less than 1% over the entire visible spectrum.

PhysicsDiffractionGeometrical opticsbusiness.industryMaterials Science (miscellaneous)Astrophysics::Instrumentation and Methods for AstrophysicsIndustrial and Manufacturing Engineeringlaw.inventionsymbols.namesakeOpticsFourier transformlawAchromatic lensChromatic aberrationsymbolsPhysics::Accelerator PhysicsBusiness and International ManagementbusinessTransformerFresnel diffractionVisible spectrumApplied optics
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All-incoherent dispersion-compensated optical correlator

2007

We report on a simple, spatially incoherent, wavelength-independent imaging system that, in contrast to the conventional case, exhibits a dispersion-compensated point-spread function. Our hybrid (diffractive-refractive) three-lens imaging configuration thus acts as an all-incoherent dispersion-compensated optical irradiance correlator. So the optical arrangement is well adapted to processing color information (both spatially and temporally incoherent) under natural illumination.

PhysicsDiffractionbusiness.industrymedia_common.quotation_subjectIrradiancePhysics::OpticsAtomic and Molecular Physics and OpticsPtychographyOpticsDispersion (optics)Optical correlatorContrast (vision)businessFresnel diffractionmedia_commonVisible spectrum
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