Search results for "VIEWING ANGLE"

showing 10 items of 36 documents

On the angular variation of thermal infrared emissivity of inorganic soils

2012

[1] Land surface temperature (LST), a key parameter for many environmental studies, can be most readily estimated by using thermal infrared (TIR) sensors onboard satellites. Accurate LST are contingent upon simultaneously accurate estimates of land surface emissivity (e), which depend on sensor viewing angle and the anisotropy of optical and structural properties of surfaces. In the case of inorganic bare soils (IBS), there are still few data that quantify emissivity angular effects. The present work deals with the angular variation of TIR emissivity for twelve IBS types, representative of nine of the twelve soil textures found on Earth according to United States Department of Agriculture c…

Atmospheric ScienceMaterials scienceEcologyIsotropyPaleontologySoil ScienceMineralogyForestryAquatic ScienceOceanographyViewing angleGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyInfrared windowEarth and Planetary Sciences (miscellaneous)EmissivityNadirOutgoing longwave radiationAnisotropyWater vaporEarth-Surface ProcessesWater Science and TechnologyRemote sensingJournal of Geophysical Research: Atmospheres
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Radiative Flux Estimation from a Broadband Radiometer Using Synthetic Angular Models in the EarthCARE Mission Framework. Part II: Evaluation

2012

AbstractThe instantaneous top-of-atmosphere (TOA) radiance-to-flux conversion for the broadband radiometer (BBR) on board the Earth Clouds, Aerosols, and Radiation Explorer (EarthCARE) was assessed in Part I of this paper, by developing theoretical angular distribution models (ADMs) specifically designed for the instrument viewing configuration. This paper validates the BBR ADMs by comparing derived flux estimates with flux retrievals obtained from the Clouds and the Earth’s Radiant Energy System (CERES) Terra models. A CERES BBR-like database is employed in the assessment, which is an optimum dataset to validate the BBR algorithms and to determine the benefits of the multiangular conversio…

Atmospheric ScienceRadiation fluxRadiative fluxRadiometerMeteorologyRadiative transferRadianceRadiant energyEnvironmental scienceShortwave radiationViewing angleRemote sensingJournal of Applied Meteorology and Climatology
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Flux retrieval optimization with a nonscanner along-track broadband radiometer

2003

[1] The theoretical behavior of broadband flux retrieval is analyzed with the aid of a radiance field database. Several angular inversion models are developed for different viewing configurations, with special emphasis in a nonscanner along-track design concept. Results show that the performance of these angular models depends on the viewing zenith angle (VZA). When cloud cover is predominant within the observed scene, VZAs around 55° (shortwave) and 50° (longwave) minimize the error when deriving fluxes. These results might help in the design of future missions where the main idea is to obtain accurate instantaneous measurements of top of atmosphere reflected and emitted fluxes. Such measu…

Atmospheric ScienceRadiometerEcologyMeteorologyCloud coverLongwavePaleontologySoil ScienceForestryAquatic ScienceOceanographyViewing angleGeophysicsLidarSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)RadianceEnvironmental scienceShortwaveZenithEarth-Surface ProcessesWater Science and TechnologyRemote sensing
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Image simulation of geostationary sensor dedicated to ocean color

2010

A method of image simulation of geostationary sensor dedicated to ocean color for open water (case1) and coastal water (case2) is presented in this paper. This method uses HYDROLIGHT to model the radiative transfer in order to obtain the water surface radiance. MeRIS level 3 products have been used for input water components to provide a realistic spatial distribution. The atmospheric radiative transfer model and the sensor model finely lead to satellite remote sensing images. This system allows to evaluate the dynamic range of BOA and TOA radiances depending on solar and viewing angles in operational situation and latter their influence on water composition retrieval.

Atmospheric radiative transfer codesMeteorologyOcean colorRadianceGeostationary orbitRadiative transferHyperspectral imagingEnvironmental scienceAtmospheric modelViewing angleRemote sensing2010 2nd Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing
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Relativistic beaming and gamma-ray brightness of blazars

2009

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA images from the MOJAVE program with millimetre-wavelength flux density monitoring data from Metsahovi Radio Observatory, we estimate the jet Doppler factors, Lorentz factors, and viewing angles for a sample of 62 blazars. We study the trends in these quantities between the sources which were detected in gamma-rays by the Fermi Large Area Telescope (LAT) during its first three months of science operations and those which were not detected. The LAT-detected blaz…

BrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenajets [galaxies]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionTelescopesymbols.namesakeRelativistic beaminglawquasars: general0103 physical sciencesBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physicsGamma rayAstronomy and Astrophysicsgalaxies: jetsViewing angle:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Lorentz factorSpace and Planetary Scienceactive [galaxies]BL Lacertae objectssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAstrophysics - High Energy Astrophysical Phenomenagalaxies: active; ; ; BL Lacertae objects : generalFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Chess recognition using 3D patterned illumination camera

2021

Computer Vision has been applied to augment traditional board games such as Chess for a number of reasons. While augmented reality enhances the gaming experience, the required additional hardware (e.g. head gear) is still not widely accepted in everyday leisure activities, and therefore, camera based methods have been developed to interface the computer with the real-life chess board. However, traditional 2D camera approaches suffer from ill-defined environmental conditions (lighting, viewing angle) and are therefore severely limited in their application. To answer this issue, we have incorporated a consumer-grade depth camera based on patterned illumination. We could show that in combinati…

Computer programComputer sciencebusiness.industryHead (linguistics)Interface (computing)ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONComputingMilieux_PERSONALCOMPUTINGRGB color modelAugmented realityComputer visionArtificial intelligenceViewing anglebusinessThirteenth International Conference on Machine Vision
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Full-parallax 3D display from stereo-hybrid 3D camera system

2018

Abstract In this paper, we propose an innovative approach for the production of the microimages ready to display onto an integral-imaging monitor. Our main contribution is using a stereo-hybrid 3D camera system, which is used for picking up a 3D data pair and composing a denser point cloud. However, there is an intrinsic difficulty in the fact that hybrid sensors have dissimilarities and therefore should be equalized. Handled data facilitate to generating an integral image after projecting computationally the information through a virtual pinhole array. We illustrate this procedure with some imaging experiments that provide microimages with enhanced quality. After projection of such microim…

Computer sciencePoint cloudComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION02 engineering and technologyStereo display01 natural sciences010309 opticsComputer graphics (images)0103 physical sciences0202 electrical engineering electronic engineering information engineeringComputer visionElectrical and Electronic EngineeringProjection (set theory)Integral imagingbusiness.industryMechanical EngineeringÒpticaViewing angleAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materials3d camera020201 artificial intelligence & image processingPinhole (optics)Artificial intelligenceParallaxbusinessOptics and Lasers in Engineering
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A possible jet precession in the periodic quasar B0605-085

2010

The quasar B0605-085 (OH 010) shows a hint for probable periodical variability in the radio total flux-density light curves. We study the possible periodicity of B0605-085 in the total flux-density, spectra and opacity changes in order to compare it with jet kinematics on parsec scales. We have analyzed archival total flux-density variability at ten frequencies (408 MHz, 4.8 GHz, 6.7 GHz, 8 GHz, 10.7 GHz, 14.5 GHz, 22 GHz, 37 GHz, 90 GHz, and 230 GHz) together with the archival high-resolution very long baseline interferometry data at 15 GHz from the MOJAVE monitoring campaign. Using the Fourier transform and discrete autocorrelation methods we have searched for periods in the total flux-de…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleusOpacityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsViewing angleLight curveAstrophysics - Astrophysics of GalaxiesSpectral lineInterferometrySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Very-long-baseline interferometryAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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Integral Imaging Monitors with an Enlarged Viewing Angle

2015

Enlarging the horizontal viewing angle is an important feature of integral imaging monitors. Thus far, the horizontal viewing angle has been enlarged in different ways, such as by changing the size of the elemental images or by tilting the lens array in the capture and reconstruction stages. However, these methods are limited by the microlenses used in the capture stage and by the fact that the images obtained cannot be easily projected into different displays. In this study, we upgrade our previously reported method, called SPOC 2.0. In particular, our new approach, which can be called SPOC 2.1, enlarges the viewing angle by increasing the density of the elemental images in the horizontal …

Integral imagingComputer Networks and CommunicationsComputer sciencebusiness.industryThree dimensional displayViewing angleComputational photographyTransformation (function)Feature (computer vision)Media TechnologyComputer visionArtificial intelligenceElectrical and Electronic EngineeringbusinessLens arrayInformation SystemsJournal of information and communication convergence engineering
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Extended View Angle Integral Imaging 3D Display using Smart Pseudoscopic-to-orthoscopic Conversion with Head Tracking

2016

We overview a head tracking integral imaging display using the smart pseudoscopic-to-orthoscopic conversion method. The crosstalk for a large viewing angle in integral imaging is eliminated by generating a new set of elemental images.

Integral imagingComputer sciencebusiness.industryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONHead trackingStereo displayViewing angleCrosstalkOpticsConversion methodComputer visionArtificial intelligenceView angleImage sensorbusinessImaging and Applied Optics 2016
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