Search results for "Instrumentation"

showing 10 items of 4914 documents

Phase error analysis of clipped waveforms in surface topography measurement using projected fringes

2021

Abstract When working with the method of projected fringes outside the optical laboratory one often encounters the problem of uncontrollable ambient light. This might cause saturation of the camera which in turn results in clipping of the fringes. Since standard theories describing phase-shifting techniques assume the projected fringes to be purely sinusoidal, such clipping will result in measurement error. In this paper a detailed analysis of this problem is given, and relations between phase errors, the amount of fringe clipping and the number of phase steps are found. Moreover, the phase difference between the clipped and the unclipped fringes is described. This investigation is based on…

Signal processingProjected fringesOptical metrology3-D measurementPhase (waves)ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION02 engineering and technology01 natural sciencesGeneralLiterature_MISCELLANEOUS010309 opticssymbols.namesakeOpticsClipping (photography)0103 physical sciencesWaveformProfilometryElectrical and Electronic EngineeringPhysical and Theoretical ChemistryPhase shiftMathematicsSignal processingObservational errorbusiness.industryPhasorAstrophysics::Instrumentation and Methods for Astrophysics021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsFourier analysisPhasor diagramsElectronic Optical and Magnetic MaterialsVDP::Teknologi: 500Fourier transformFourier analysissymbols0210 nano-technologybusiness
researchProduct

Multiple-Output Walsh Function Generation for Minimum Orthogonality Error

1978

A hazard-free multiple-output Walsh function generator is presented which requires a minimum amount of hardware and is as fast as the integrated logic family employed for the implementation. However, the main characteristic of the instrument is the optimum performance from the viewpoint of the orthogonality of the function generated, as it is shown by the experimental verifications reported.

Signal processingSignal generatorComputer scienceFast Fourier transformLogic familyOrthogonal functionsOrthogonality principleFunction (mathematics)Logic synthesisOrthogonalityWalsh functionBinary codeElectrical and Electronic EngineeringInstrumentationAlgorithmIEEE Transactions on Instrumentation and Measurement
researchProduct

A Hybrid Frequency-Space Approach for Shape Measurement by Shadow Moiré Technique with Carrier Fringe Pattern

2006

In this paper, a novel methodology to process fringe pattern is presented. The core of the signal processing technique is the use of the direction information, a modulo 2pi quantity that locally informs about the direction along which fringes grow with maximum rate. By using this information, it was possible to perform adaptive, direction- and orientation-based operations on fringe images in order to remove unwanted effects, to enhance the contrast and to extract the phase information encoded. The method has been applied on shadow moire interferograms with carrier fringes in order to measure the surface of small objects. The developed algorithm allows to process fringes whose phase informat…

Signal processingbusiness.industryComputer scienceAstrophysics::Instrumentation and Methods for AstrophysicsPhase (waves)Process (computing)Image processingAdaptive filtersymbols.namesakeOpticsFourier transformsymbolsDemodulationHilbert transformbusiness2006 IEEE Instrumentation and Measurement Technology Conference Proceedings
researchProduct

A Direction/Orientation-Based Method for Shape Measurement by Shadow MoirÉ

2008

In this paper, a methodology to process fringe patterns is presented. The core of the signal processing technique is the use of the direction information, which is a modulo quantity that locally indicates the direction along which fringes grow at a maximum rate. By using this information, it was possible to perform adaptive and direction/orientation-based operations on fringe images to remove unwanted effects (mainly distortions at the image borders), to enhance the contrast, and to extract the phase information encoded. The method has been applied on shadow-moire interferograms with carrier fringes in order to measure the surface of small objects. The developed algorithm allows processing …

Signal processingbusiness.industryOrientation (computer vision)Computer sciencePhase distortionAstrophysics::Instrumentation and Methods for AstrophysicsPhase (waves)Process (computing)Adaptive filtersymbols.namesakeOpticsFourier transformsymbolsElectrical and Electronic EngineeringbusinessInstrumentationIEEE Transactions on Instrumentation and Measurement
researchProduct

Probing the radio emission from air showers with polarization measurements

2014

The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially wit…

SignalsAstronomy01 natural sciencesElectric fieldComputational physicsCosmic-raysComposition energy spectra and interactionscosmic rayRadio wavePhysicsEarth's magnetic fieldHigh Energy Astrophysical Phenomena (astro-ph.HE)Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsPolarization (waves)Polarization (waves)BolometersThunderstormsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCAMPO MAGNÉTICOradio emissionRadio waveNuclear and High Energy Physics[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]Air showerComposition energy spectra and interactions; Solar electromagnetic emission; BolometersAstrophysics::High Energy Astrophysical Phenomenainfrared submillimeter wave microwave and radiowave receivers and detectorsFieldFOS: Physical sciencesPierre Auger Observatory ; air shower ; radio emissionRadiationMonte-carlo SimulationsOpticsElectric field0103 physical sciencesddc:530Pierre auger observatory010306 general physicsPulsesInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industrySolar electromagnetic emissionFísicaOpticsDetectorComputational physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerEarth's magnetic fieldMagnetic fieldExperimental High Energy PhysicsbusinessCodalema
researchProduct

Background studies for acoustic neutrino detection at the South Pole

2011

The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method to measure the tiny flux of cosmogenic neutrinos expected on Earth. The energy threshold for this process depends strongly on the absolute noise level in the target material. The South Pole Acoustic Test Setup (SPATS), deployed in the upper part of four boreholes of the IceCube Neutrino Observatory, has monitored the noise in Antarctic ice at the geographic South Pole for more than two years down to 500 m depth. The noise is very stable and Gaussian distributed. Lacking an in-situ calibration up to now, laboratory measurements have been used to estimate the absolute noise level in the 10 to …

SignalsTELESCOPEAbsolute noise levelAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstrophysics7. Clean energy01 natural sciencesIceCube Neutrino Observatorylaw.inventionIceCubeTelescopeAbsolute noise level; Acoustic neutrino detection; Neutrino flux limitNeutrino flux limitlawSIGNALS0103 physical sciencesWATERDetection theory010306 general physicsTelescopeInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsAcoustic neutrino detector010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsWaterAstronomy and AstrophysicsGeodesyAcoustic neutrino detectionNoiseNeutrino detectorPhysics and Astronomy13. Climate actionddc:540NeutrinoAstrophysics - Instrumentation and Methods for Astrophysics
researchProduct

The Large Area Detector onboard the eXTP mission

2018

The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS) and China National Space Administration (CNSA) currently performing an extended phase A study and proposed for a launch by 2025 in a low-earth orbit. The eXTP scientific payload envisages a suite of instruments (Spectroscopy Focusing Array, Polarimetry Focusing Array, Large Area Detector and Wide Field Monitor) offering unprecedented simultaneous wide-band X-ray spectral, timing and polarimetry sensitivity. A large European consortium is contributing to the eXTP study and it is expected to provide key hardware elements, including a Large Area Detector (LAD). The LAD instrumen…

Silicon detectorX-ray AstronomyComputer sciencecapillary platePolarimetryFOS: Physical sciencesField of viewContext (language use)Condensed Matter Physic01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesElectroniccapillary plates; Silicon detectors; Timing; X-ray Astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringTimingOptical and Magnetic MaterialsAerospace engineeringSpectral resolutionElectrical and Electronic Engineering010306 general physicscapillary plates; Silicon detectors; Timing; X-ray Astronomy; astro-ph.IM; astro-ph.IM; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringInstrumentation and Methods for Astrophysics (astro-ph.IM)X-ray astronomycapillary plates010308 nuclear & particles physicsbusiness.industryPayloadElectronic Optical and Magnetic MaterialApplied MathematicsDetectorAntenna apertureComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsApplied MathematicSilicon detectorsAstrophysics - Instrumentation and Methods for Astrophysicsbusinessastro-ph.IM
researchProduct

Determination of molecular stopping cross section of 12C, 16O, 28Si, 35Cl, 58Ni, 79Br, and 127I in silicon nitride

2015

Abstract Silicon nitride is a technologically important material in a range of applications due to a combination of important properties. Ion beam analysis techniques, and in particular, heavy ion elastic recoil detection analysis can be used to determine the stoichiometry of silicon nitride films, which often deviates from the ideal Si3N4, as well as the content of impurities such as hydrogen, even in the presence of other materials or in a matrix containing heavier elements. Accurate quantification of IBA results depends on the basic data used in the data analysis. Quantitative depth profiling relies on the knowledge of the stopping power cross sections of the materials studied for the io…

Silicon nitrideNuclear and High Energy PhysicsIon beam analysisMaterials scienceta114HydrogenIon beam analysischemistry.chemical_elementHeavy ionsIonElastic recoil detectionchemistry.chemical_compoundchemistrySilicon nitrideImpurityThin filmAtomic physicsStopping powerInstrumentationStoichiometryNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
researchProduct

Measurements of Silicon Photomultipliers Responsivity in Continuous Wave Regime

2013

We report on the electrical and optical characterization, in continuous wave regime, of a novel class of silicon photomultipliers fabricated in standard planar technology on a silicon p-type substrate. Responsivity measurements, performed with an incident optical power down to tenths of picowatts, at different reverse bias voltages and on a broad (340–820 nm) spectrum, will be shown and discussed. The device temperature was monitored, allowing us to give a physical interpretation of the measurements. The obtained results demonstrate that such novel silicon photomultipliers are suitable as sensitive power meters for low photon fluxes.

Silicon photonicsMaterials scienceSiliconPhysics::Instrumentation and Detectorsbusiness.industryHybrid silicon laserchemistry.chemical_elementSettore ING-INF/02 - Campi ElettromagneticiOptical powerSubstrate (electronics)Settore ING-INF/01 - ElettronicaElectronic Optical and Magnetic MaterialsResponsivityOpticsSilicon photomultiplierchemistryOptoelectronicsContinuous waveAvalanche photodiode (APD) photodetector responsivity silicon photomultiplier (SiPM) single-photon avalanche diode (SPAD)Electrical and Electronic EngineeringbusinessIEEE Transactions on Electron Devices
researchProduct

Baseline design of the filters for the LAD detector on board LOFT

2014

The Large Observatory for X-ray Timing (LOFT) was one of the M3 missions selected for the phase A study in the ESA's Cosmic Vision program. LOFT is designed to perform high-time-resolution X-ray observations of black holes and neutron stars. The main instrument on the LOFT payload is the Large Area Detector (LAD), a collimated experiment with a nominal effective area of ~10 m 2 @ 8 keV, and a spectral resolution of ~240 eV in the energy band 2-30 keV. These performances are achieved covering a large collecting area with more than 2000 large-area Silicon Drift Detectors (SDDs) each one coupled to a collimator based on lead-glass micro-channel plates. In order to reduce the thermal load onto …

SiliconCosmic VisionPhysics - Instrumentation and DetectorsSpectral resolutionSilicon drift detectorVisionAstrophysics::High Energy Astrophysical PhenomenaCollimatorsObservatoriesFOS: Physical sciencesCollimated lightlaw.inventionSettore FIS/05 - Astronomia E AstrofisicaOpticsObservatorylawX-raysSpectral resolutionphysics.ins-detInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsEquipment and servicesLead glassSensorsbusiness.industryDetectorAntenna apertureAstrophysics::Instrumentation and Methods for AstrophysicsCollimatorInstrumentation and Detectors (physics.ins-det)Microchannel platesbusinessAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
researchProduct