Search results for "Spectral"

showing 10 items of 3116 documents

Unsupervised deep feature extraction of hyperspectral images

2014

This paper presents an effective unsupervised sparse feature learning algorithm to train deep convolutional networks on hyperspectral images. Deep convolutional hierarchical representations are learned and then used for pixel classification. Features in lower layers present less abstract representations of data, while higher layers represent more abstract and complex characteristics. We successfully illustrate the performance of the extracted representations in a challenging AVIRIS hyperspectral image classification problem, compared to standard dimensionality reduction methods like principal component analysis (PCA) and its kernel counterpart (kPCA). The proposed method largely outperforms…

PixelComputer sciencebusiness.industryDimensionality reductionFeature extractionHyperspectral imagingPattern recognitionDiscriminative modelKernel (image processing)Principal component analysisComputer visionArtificial intelligencebusinessFeature learning2014 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing (WHISPERS)
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A support vector domain method for change detection in multitemporal images

2010

This paper formulates the problem of distinguishing changed from unchanged pixels in multitemporal remote sensing images as a minimum enclosing ball (MEB) problem with changed pixels as target class. The definition of the sphere-shaped decision boundary with minimal volume that embraces changed pixels is approached in the context of the support vector formalism adopting a support vector domain description (SVDD) one-class classifier. SVDD maps the data into a high dimensional feature space where the spherical support of the high dimensional distribution of changed pixels is computed. Unlike the standard SVDD, the proposed formulation of the SVDD uses both target and outlier samples for defi…

PixelComputer sciencebusiness.industryFeature vectorComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONThresholdingMultispectral pattern recognitionSupport vector machineKernel methodArtificial IntelligenceComputer Science::Computer Vision and Pattern RecognitionSignal ProcessingOutlierDecision boundaryComputer visionComputer Vision and Pattern RecognitionArtificial intelligencebusinessSoftwareChange detectionPattern Recognition Letters
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Cluster kernels for semisupervised classification of VHR urban images

2009

In this paper, we present and apply a semisupervised support vector machine based on cluster kernels for the problem of very high resolution image classification. In the proposed setting, a base kernel working with labeled samples only is deformed by a likelihood kernel encoding similarities between unlabeled examples. The resulting kernel is used to train a standard support vector machine (SVM) classifier. Experiments carried out on very high resolution (VHR) multispectral and hyperspectral images using very few labeled examples show the relevancy of the method in the context of urban image classification. Its simplicity and the small number of parameters involved make it versatile and wor…

PixelContextual image classificationbusiness.industryMultispectral imageComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONHyperspectral imagingProbability density functionPattern recognitionSupport vector machineComputingMethodologies_PATTERNRECOGNITIONComputer Science::Computer Vision and Pattern RecognitionRadial basis function kernelArtificial intelligencebusinessClassifier (UML)Mathematics2009 Joint Urban Remote Sensing Event
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Spatial analysis of the homogeneity of the land surface temperature in three Spanish test sites

2015

Calibration and validation cal/val are key activities to test the data quality acquired from satellite-based instruments, as well as to report the accuracy of derived products such as the land surface temperature LST. Calibration of thermal infrared TIR data and validation of LST products at low spatial resolution requires the identification of large and homogeneous areas, which is a difficult task. In this work, spatial and temporal homogeneity of LST was analysed over three Spanish regions: the agricultural area of Barrax, Donana National Park, and Cabo de Gata Natural Park. For this purpose, very high spatial resolution approximately 3 m imagery acquired with the Airborne Hyperspectral S…

PixelMean squared errorHomogeneity (statistics)CalibrationGeneral Earth and Planetary SciencesEnvironmental scienceHyperspectral imagingSatelliteImage resolutionField (geography)Remote sensingInternational Journal of Remote Sensing
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<title>Spectral/spatial integration effects on information extraction from multispectral data: multiresolution approaches</title>

1995

New techniques for information extraction from multispectral data require physical modeling to understand the energy transfer at the atmosphere/surface interface and to develop appropriate inversion procedures, in combination with advanced processing techniques. A multi-step procedure is proposed in this work: the first step implies a binary decision about the second step to be applied in each case. If the pixel is considered as being a `pure' pixel, through a spectral/spatial classification procedure based on multiresolution techniques, then numerical inversion techniques, based on a multiple-scattering reflectance model, are used to extract parameters representing specific surface propert…

Pixelbusiness.industryBinary decision diagramComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONPattern recognitionAtmospheric modelcomputer.software_genreData modelingInformation extractionGeographyComputer Science::Computer Vision and Pattern RecognitionSpatial ecologyComputer visionArtificial intelligenceSpectral resolutionbusinessImage resolutioncomputerSPIE Proceedings
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Valence bands of poly(methylmethacrylate) and photoion emission in vacuum ultraviolet region

1992

Photoion and photoelectron yields were measured for poly(methylmethacrylate) in the photon energy region of 8–40 eV using synchrotron radiation. Further, the valence‐band structure was investigated with ultraviolet photoelectron spectra and valence effective Hamiltonian calculations. A significant difference was observed between the photon energy dependencies of photoion and photoelectron yields. The threshold energy for photoion emission was found to be 10.5 eV, while that for photoelectron emission was 8.5 eV, indicating holes created near the valence‐band top do not contribute to the ion emission. At the higher‐energy region, the ion emission efficiency was found to be enhanced in the ph…

PmmaValence BandsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomySynchrotron radiationPhotoelectron photoion coincidence spectroscopyAstrophysics::Cosmology and Extragalactic AstrophysicsPhoton energymedicine.disease_causeSpectral lineX-ray photoelectron spectroscopyEv Range 10−100:FÍSICA [UNESCO]medicinePmma ; Ion Emission ; Electron Emission ; Photoelectron Spectroscopy ; Ev Range 10−100 ; Valence Bands ; Band StructurePhysics::Atomic and Molecular ClustersIon EmissionPhysics::Atomic PhysicsElectron EmissionBand StructureAstrophysics::Galaxy AstrophysicsValence (chemistry)ChemistryPhotoelectron SpectroscopyUNESCO::FÍSICAThreshold energyAtomic physicsUltraviolet
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INTEGRAL/SPI ground calibration

2003

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, the spectral resolution and the angular resolution. Absolute determination of the effective area has been obtained from simulations and measurements. At 1 MeV, the effective area is 65 cm^2 for a point source on the optical axis, the spectral resolution ~2.3 keV. The angular resolution is better than 2.5 deg and the source separation capability about 1 deg. Some temperature dependant parameters will require permanent in-flight calibration.

Point source[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesInstrumentation ; Detectors ; Spectrographs ; Space vehicles ; Gamma rays ; ObservationsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrographs0103 physical sciencesCalibrationSource separationAngular resolutionSpectral resolutionspace vehicles: instrumentsInstrumentation010303 astronomy & astrophysicsObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]instrumentation: spectrographsPhysicsSpectrometer[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryinstrumentation: detectorsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAntenna apertureAstrophysics (astro-ph)DetectorsSpace vehiclesAstronomy and AstrophysicsOptical axisSpace and Planetary Sciencebusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]gamma rays: observations
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Flux and color variations of the quadruply imaged quasar HE 0435-1223

2011

aims: We present VRi photometric observations of the quadruply imaged quasar HE 0435-1223, carried out with the Danish 1.54m telescope at the La Silla Observatory. Our aim was to monitor and study the magnitudes and colors of each lensed component as a function of time. methods: We monitored the object during two seasons (2008 and 2009) in the VRi spectral bands, and reduced the data with two independent techniques: difference imaging and PSF (Point Spread Function) fitting.results: Between these two seasons, our results show an evident decrease in flux by ~0.2-0.4 magnitudes of the four lensed components in the three filters. We also found a significant increase (~0.05-0.015) in their V-R …

Point spread functionCosmology and Nongalactic Astrophysics (astro-ph.CO)FluxFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGravitational microlensing01 natural scienceslaw.inventionTelescopeSettore FIS/05 - Astronomia e AstrofisicaObservatorylaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsgeneral – gravitational lensing; weak – techniques: photometric [quasars]Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsphotometric [Techniques]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasargeneral [Quasars]Spectral bandsSpace and Planetary Scienceastro-ph.COAstrophysics::Earth and Planetary Astrophysicsweak [Gravitational lensing]Astrophysics - Cosmology and Nongalactic Astrophysics
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The ATHENA X-ray Integral Field Unit (X-IFU)

2018

Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States.

Point spread functionPhotonAstrophysics::High Energy Astrophysical PhenomenaField of viewAthena; Instrumentation; Space telescopes; X-ray Integral Field Unit; X-ray spectroscopy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringCondensed Matter PhysicLarge format01 natural sciences7. Clean energySpace telescopeslaw.inventionTelescopePhysics::Popular PhysicsSettore FIS/05 - Astronomia E AstrofisicaOpticslawPhysics::Plasma Physics0103 physical sciencesElectronicAthenaOptical and Magnetic MaterialsSpectral resolutionElectrical and Electronic Engineering010306 general physics010303 astronomy & astrophysicsInstrumentationPhysicsSpectrometerbusiness.industryElectronic Optical and Magnetic MaterialApplied MathematicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter Physics115 Astronomy Space sciencePhysics::History of PhysicsApplied MathematicSpace telescopeX-ray Integral Field UnitX-ray spectroscopybusiness
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2021

Abstract We propose a signal deconvolution procedure for imaging spectrometer data, where a measured point spread function (PSF) is deconvolved itself before being used for deconvolution of the signal. We evaluate the effectiveness of our procedure for improvement of the spatio-spectral signal, as well as our target application, i.e. estimation of sun-induced fluorescence (SIF). Imaging spectrometers are well established instruments for remote sensing. When used for scientific purposes these instruments are usually calibrated on a regular basis. In our case the point spread function of the optics is measured in an elaborate procedure with a tunable monochromator point light source. PSFs are…

Point spread functionmedicine.medical_specialtyComputer scienceWiener filterAstrophysics::Instrumentation and Methods for AstrophysicsImaging spectrometerSoil ScienceHyperspectral imagingGeologyPeak signal-to-noise ratioSpectral imagingsymbols.namesakesymbolsmedicineDeconvolutionComputers in Earth SciencesImage sensorAlgorithmRemote sensingRemote Sensing of Environment
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