Search results for "brightness"

showing 10 items of 162 documents

Color- and motion-specific units in the tectum opticum of goldfish

2016

Extracellular recordings were performed from 69 units at different depths between 50 and [Formula: see text]m below the surface of tectum opticum in goldfish. Using large field stimuli (86[Formula: see text] visual angle) of 21 colored HKS-papers we were able to record from 54 color-sensitive units. The colored papers were presented for 5[Formula: see text]s each. They were arranged in the sequence of the color circle in humans separated by gray of medium brightness. We found 22 units with best responses between orange, red and pink. About 12 of these red-sensitive units were of the opponent "red-ON/blue-green-OFF" type as found in retinal bipolar- and ganglion cells as well. Most of them w…

CombinatoricsPhysicsCommunicationBrightnessgenetic structuresColoredColor visionbusiness.industryGeneral NeuroscienceTectum opticumMotion visionGeneral MedicinebusinessJournal of Integrative Neuroscience
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New systems for extracting 3-D shape information from images

1993

Neural architectures may offer an adequate way to deal with early vision since they are able to learn shape features or classify unknown shapes, generalising the features of a few meaningful examples, with a low computational cost after the training phase. Two different neural approaches are proposed by the authors: the first one consists of a cascaded architecture made up by a first stage named BWE (Boundary Webs Extractor) which is aimed to extract a brightness gradient map from the image, followed by a backpropagation network that estimates the geometric parameters of the object parts present in the perceived scene. The second approach is based on the extraction of the boundary webs map …

Computer sciencebusiness.industryBoundary (topology)Pattern recognitionObject (computer science)BackpropagationExtractorImage (mathematics)SuperquadricsComputer visionArtificial intelligenceD-ShapeBrightness gradientbusiness
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Reduced efficiency roll-off in light-emitting diodes enabled by quantum dot–conducting polymer nanohybrids

2014

We demonstrate QLEDs implementing wider active layers (50 nm) based on QD–conducting polymer nanohybrids, which exhibit a stable operational device performance across a wide range of current densities and brightness. A comparative study reveals that the significant suppression of efficiency roll-off in the high current density regime is primarily attributed to a sufficient charge carrier distribution over the wider active layer and improved charge carrier balance within QDs enabled by the hybridization of QDs with conducting polymers. Utilization of this finding in future studies should greatly facilitate the development of high performance, stable QLEDs at high current density or luminance…

Conductive polymerchemistry.chemical_classificationBrightnessMaterials sciencebusiness.industryGeneral ChemistryPolymerLuminanceActive layerlaw.inventionchemistryQuantum dotlawMaterials ChemistryOptoelectronicsCharge carrierbusinessLight-emitting diodeJ. Mater. Chem. C
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Small-scale mixing processes enhancing troposphere-to-stratosphere transport by pyro-cumulonimbus storms

2007

Abstract. Deep convection induced by large forest fires is an efficient mechanism for transport of aerosol particles and trace gases into the upper troposphere and lower stratosphere (UT/LS). For many pyro-cumulonimbus clouds (pyroCbs) as well as other cases of severe convection without fire forcing, radiometric observations of cloud tops in the thermal infrared (IR) reveal characteristic structures, featuring a region of relatively high brightness temperatures (warm center) surrounded by a U-shaped region of low brightness temperatures. We performed a numerical simulation of a specific case study of pyroCb using a non-hydrostatic cloud resolving model with a two-moment cloud microphysics p…

ConvectionTropospherePhysicsAtmospheric ScienceBrightnessMeteorologyThermalGravity waveAtmospheric sciencesStratosphereTrace gasAerosolAtmospheric Chemistry and Physics
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Studies of Relativistic Jets in Active Galactic Nuclei with SKA

2014

Relativistic jets in active galactic nuclei (AGN) are among the most powerful astrophysical objects discovered to date. Indeed, jetted AGN studies have been considered a prominent science case for SKA, and were included in several different chapters of the previous SKA Science Book (Carilli & Rawlings 2004). Most of the fundamental questions about the physics of relativistic jets still remain unanswered, and await high-sensitivity radio instruments such as SKA to solve them. These questions will be addressed specially through analysis of the massive data sets arising from the deep, all-sky surveys (both total and polarimetric flux) from SKA1. Wide-field very-long-baseline-interferometri…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleus010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsJet (particle physics)01 natural sciencesAstrophysical jet0103 physical sciencesVery-long-baseline interferometryInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstrophysics - Astrophysics of GalaxiesGalaxyCharacterization (materials science)13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Brightness temperatureAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsProceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14)
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A simple model to estimate the daily value of the regional maximum evapotranspiration from satellite temperature and albedo images

1987

Abstract We have tried an adaptation of the radiation model proposed by FAO, applicable in any area, for the estimation of the regional maximum evapotranspiration, ET, from temperature and albedo images obtained from a satellite. This model is based on the relationships ETm = k cETo ETo = A + BR g + CR g Ta max where k c is the crop coefficient, ETo is the maximum evapotranspiration of the reference crop (green grass), Rg is the global radiation obtained from satellite albedo images, T a max is the maximum temperature of the air obtained from the near-midday satellite temperature and A, B and C are the empirical coefficients characteristic of each zone calculated for different intervals of …

Crop coefficientMeteorologyEvapotranspirationBrightness temperatureGeneral Earth and Planetary SciencesEnvironmental scienceValue (computer science)Relative humiditySatelliteAlbedoWind speedInternational Journal of Remote Sensing
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Enhancing TIR Image Resolution via Bayesian Smoothing for IRRISAT Irrigation Management Project

2013

Accurate estimation of physical quantities depends on the availability of High Resolution (HR) observations of the Earth surface. However, due to the unavoidable tradeoff between spatial and time resolution, the acquisition instants of HR data hardly coincides with those required by the estimation algorithms. A possible solution consists in constructing a synthetic HR observation at a given time k by exploiting Low Resolution (LR) and HR data acquired at different instants. In this work we recast this issue as a smoothing problem, thus focusing on cases in which observations acquired both before and after time k are available. The proposed approach is validated on a region of interest for t…

EstimationIrrigation Managementbusiness.industrySettore ICAR/02 - Costruzioni Idrauliche E Marittime E IdrologiaBrightness TemperatureBayesian SmoothingThermal SharpeningBayesian smoothingGeographyRegion of interestMultitemporal AnalysiKey (cryptography)thermal infraredComputer visionArtificial intelligencebusinessIrrigation managementImage resolutionAlgorithmMultisensor Data FusionSmoothingSettore ICAR/06 - Topografia E CartografiaPhysical quantity
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Optimizing colormaps with consideration for color vision deficiency to enable accurate interpretation of scientific data

2018

Color vision deficiency (CVD) affects more than 4% of the population and leads to a different visual perception of colors. Though this has been known for decades, colormaps with many colors across the visual spectra are often used to represent data, leading to the potential for misinterpretation or difficulty with interpretation by someone with this deficiency. Until the creation of the module presented here, there were no colormaps mathematically optimized for CVD using modern color appearance models. While there have been some attempts to make aesthetically pleasing or subjectively tolerable colormaps for those with CVD, our goal was to make optimized colormaps for the most accurate perce…

FOS: Computer and information sciences0301 basic medicineBrightnessVisual perceptionVisionComputer scienceComputer Vision and Pattern Recognition (cs.CV)Computer Science - Computer Vision and Pattern Recognitionlcsh:MedicineSocial SciencesColor Vision Defects01 natural sciencesMass SpectrometryAnalytical ChemistrySecondary Ion Mass SpectrometrySpectrum Analysis TechniquesMathematical and Statistical TechniquesPsychologyComputer visionlcsh:ScienceData ProcessingMultidisciplinaryPhysicsClassical MechanicsOther Quantitative Biology (q-bio.OT)Quantitative Biology - Other Quantitative BiologyChemistryPhysical SciencesRegression AnalysisSensory PerceptionInformation TechnologyStatistics (Mathematics)AlgorithmsColor PerceptionResearch ArticleComputer and Information SciencesColor visionColorFluid MechanicsLinear Regression AnalysisColor spaceResearch and Analysis MethodsContinuum Mechanics010309 optics03 medical and health sciencesSine Waves0103 physical sciencesHumansStatistical MethodsFluid FlowVision OcularHueColor Visionbusiness.industrylcsh:RBiology and Life SciencesFluid Dynamics030104 developmental biologyFOS: Biological scienceslcsh:QArtificial intelligencebusinessMathematical FunctionsMathematicsPhotic StimulationSoftwareNeurosciencePLOS ONE
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Dense matter with eXTP

2019

In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry (eXTP) mission for determining the nature of dense matter; neutron star cores host an extreme density regime which cannot be replicated in a terrestrial laboratory. The tightest statistical constraints on the dense matter equation of state will come from pulse profile modelling of accretion-powered pulsars, burst oscillation sources, and rotation-powered pulsars. Additional constraints will derive from spin measurements, burst spectra, and properties of the accretion flows in the vicinity of the neutron star. Under development by an international Consortium led by the Institute of High Energy Physics o…

GAMMA-RAY PULSARSdense matterAstrophysics::High Energy Astrophysical PhenomenaPolarimetryGeneral Physics and AstronomyFOS: Physical sciencesAstrophysicsNeutronBRIGHTNESS OSCILLATIONS7. Clean energy01 natural sciencesINNER ACCRETION DISKSSpectral lineX-raydense matter; equation of state; neutron; X-rays; Physics and Astronomy (all)Physics and Astronomy (all)Equacions d'estatneutronPulsar0103 physical sciencesMILLISECOND PULSARSX-raysNEUTRON-STARRADIUS CONSTRAINTS010306 general physics010303 astronomy & astrophysicsRELATIVISTIC IRON LINEequation of statePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)LIGHT CURVESNeutronsEquation of stateQUASI-PERIODIC OSCILLATIONSX-RaysStarke Wechselwirkung und exotische Kerne – Abteilung BlaumAstrophysics::Instrumentation and Methods for AstrophysicsEQUATION-OF-STATEAccretion (astrophysics)Neutron star:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Raigs XAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaDense matterDense matter
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Millimeter-VLBI observations of low-luminosity active galactic nuclei with source-frequency phase-referencing

2021

We report millimeter-VLBI results of low-luminosity active galactic nuclei (M 84 and M 87) up to 88 GHz with source-frequency phase-referencing observations. We detected the weak VLBI core and obtained the first image of M 84 at 88 GHz. The derived brightness temperature of M 84 core was about 7.2$\times$10$^9$ K, which could serve as a lower limit as the core down to 30 Schwarzschild radii was still un-resolved in our 88 GHz observations. We successfully determined the core-shifts of M 87 at 22-44 GHz and 44-88 GHz through source-frequency phase-referencing technique. The jet apex of M 87 could be deduced at about 46 $\mu$as upstream of the 43 GHz core from core-shift measurements. The est…

High Energy Astrophysical Phenomena (astro-ph.HE)Event Horizon TelescopePhysicsAstrofísicaActive galactic nucleusEvent horizonFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesLuminositySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Brightness temperatureVery-long-baseline interferometryMagnitude (astronomy)AstronomiaMillimeterAstrophysics - High Energy Astrophysical Phenomena
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