Search results for " Methods"

showing 10 items of 4102 documents

Multi-temporal and Multi-source Remote Sensing Image Classification by Nonlinear Relative Normalization

2016

Remote sensing image classification exploiting multiple sensors is a very challenging problem: data from different modalities are affected by spectral distortions and mis-alignments of all kinds, and this hampers re-using models built for one image to be used successfully in other scenes. In order to adapt and transfer models across image acquisitions, one must be able to cope with datasets that are not co-registered, acquired under different illumination and atmospheric conditions, by different sensors, and with scarce ground references. Traditionally, methods based on histogram matching have been used. However, they fail when densities have very different shapes or when there is no corres…

Signal Processing (eess.SP)FOS: Computer and information sciences010504 meteorology & atmospheric sciencesHyperspectral imagingComputer Vision and Pattern Recognition (cs.CV)0211 other engineering and technologiesNormalization (image processing)Computer Science - Computer Vision and Pattern Recognition02 engineering and technology3107 Atomic and Molecular Physics and Optics01 natural sciencesLaboratory of Geo-information Science and Remote SensingComputer vision910 Geography & travelMathematicsDomain adaptationContextual image classificationImage and Video Processing (eess.IV)1903 Computers in Earth SciencesPE&RCClassificationAtomic and Molecular Physics and OpticsComputer Science ApplicationsKernel method10122 Institute of GeographyKernel (image processing)Feature extractionFeature extractionVery high resolutionGraph-based methods1706 Computer Science ApplicationsFOS: Electrical engineering electronic engineering information engineeringLaboratorium voor Geo-informatiekunde en Remote SensingComputers in Earth SciencesElectrical Engineering and Systems Science - Signal ProcessingEngineering (miscellaneous)021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingManifold alignmentbusiness.industryNonlinear dimensionality reductionHistogram matchingKernel methodsPattern recognitionElectrical Engineering and Systems Science - Image and Video ProcessingManifold learningArtificial intelligence2201 Engineering (miscellaneous)businessISPRS Journal of Photogrammetry and Remote Sensing
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Secrecy analysis and learning-based optimization of cooperative NOMA SWIPT systems

2019

Non-orthogonal multiple access (NOMA) is considered to be one of the best candidates for future networks due to its ability to serve multiple users using the same resource block. Although early studies have focused on transmission reliability and energy efficiency, recent works are considering cooperation among the nodes. The cooperative NOMA techniques allow the user with a better channel (near user) to act as a relay between the source and the user experiencing poor channel (far user). This paper considers the link security aspect of energy harvesting cooperative NOMA users. In particular, the near user applies the decode-and-forward (DF) protocol for relaying the message of the source no…

Signal Processing (eess.SP)FOS: Computer and information sciencesComputer scienceDecode-and-forward (DF)050801 communication & media studies5G-tekniikkalaw.inventionNonorthogonal multiple access (NOMA)NomaComputer Science - Networking and Internet Architecturelangaton tiedonsiirto0508 media and communicationsoptimointiRelaylawRobustness (computer science)0502 economics and businessSecrecymedicineFOS: Electrical engineering electronic engineering information engineeringElectrical Engineering and Systems Science - Signal ProcessingtietoturvaNetworking and Internet Architecture (cs.NI)business.industryDeep learningPower-splitting05 social sciencesDeep learningmedicine.diseasekoneoppiminen050211 marketingArtificial intelligencebusinessDecoding methodsEfficient energy useComputer networkCommunication channel
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A probabilistic compressive sensing framework with applications to ultrasound signal processing

2019

Abstract The field of Compressive Sensing (CS) has provided algorithms to reconstruct signals from a much lower number of measurements than specified by the Nyquist-Shannon theorem. There are two fundamental concepts underpinning the field of CS. The first is the use of random transformations to project high-dimensional measurements onto a much lower-dimensional domain. The second is the use of sparse regression to reconstruct the original signal. This assumes that a sparse representation exists for this signal in some known domain, manifested by a dictionary. The original formulation for CS specifies the use of an l 1 penalised regression method, the Lasso. Whilst this has worked well in l…

Signal processing0209 industrial biotechnologyBayesian methodsComputer scienceTKAerospace Engineering02 engineering and technologycomputer.software_genre01 natural sciencesRelevance vector machineNDTSettore ING-IND/14 - Progettazione Meccanica E Costruzione Di Macchine020901 industrial engineering & automationLasso (statistics)0103 physical sciencesUltrasoundUncertainty quantification010301 acousticsSparse representationCivil and Structural EngineeringSignal processingSignal reconstructionMechanical EngineeringProbabilistic logicSparse approximationCompressive sensingComputer Science ApplicationsCompressed sensingControl and Systems EngineeringRelevance Vector MachineData miningcomputer
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A nonstationary model for the analysis of transient speech signals

1987

In this correspondence, a model is presented for the analysis of transient speech signals, which is based on a sum of the impulsive responses corresponding to a number of poles with time-dependent parameters. The aim of this analysis is to obtain discriminative features of the different transient elements of speech.

Signal processingComputer scienceSignal reconstructionSpeech recognitionSpeech processingsymbols.namesakeFourier transformDiscriminative modelComputer Science::SoundFrequency domainSignal ProcessingsymbolsTransient (oscillation)Decoding methodsIEEE Transactions on Acoustics, Speech, and Signal Processing
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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
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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
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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
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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
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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
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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
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