Search results for "Brightness"

showing 10 items of 162 documents

Surface temperature in the context of FLuorescence EXplorer (FLEX) mission

2007

It has been demonstrated that the spectrum of fluorescence emission is dependent on leaf temperature, thus there is a need for thermal information in order to interpret fluorescence signals. Temperature is also related to transpiration and stomata closure, which affects CO2 uptake and fluorescence. Therefore temperature measurements help to confirm the trends observed in fluorescence measurements. While fluorescence is immediately and uniquely related to photosynthesis, temperature provides additional information about plant status and instantaneous energy/water fluxes between plants and the atmosphere. The objective of this paper is to demonstrate the role of surface temperature in the con…

BrightnessPlanetary boundary layerMeasuring instrumentEmissivityRadiometryContext (language use)Atmospheric temperatureTemperature measurementRemote sensing2007 IEEE International Geoscience and Remote Sensing Symposium
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A generalized soil-adjusted vegetation index

2002

Operational monitoring of vegetative cover by remote sensing currently involves the utilisation of vegetation indices (VIs), most of them being functions of the reflectance in red (R) and near-infrared (NIR) spectral bands. A generalized soil-adjusted vegetation index (GESAVI), theoretically based on a simple vegetation canopy model, is introduced. It is defined in terms of the soil line parameters (A and B) as: GESAVI=(NIRBRA)/(R+Z), where Z is related to the red reflectance at the cross point between the soil line and vegetation isolines. As Z is a soil adjustment coefficient, this new index can be considered as belonging to the SAVI family. In order to analyze the GESAVI sensitivity to s…

BrightnessSoil ScienceGeologyRadiosity (computer graphics)Enhanced vegetation indexSpectral bandsLand coverComputers in Earth SciencesVegetation IndexNormalized Difference Vegetation IndexSoil colorRemote sensingMathematicsRemote Sensing of Environment
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Comparison of measured brightness temperatures from SMOS with modelled ones from ORCHIDEE and H-TESSEL over the Iberian Peninsula

2017

19 pges, 10 figures, 6 tables

BrightnessState variable010504 meteorology & atmospheric sciences0211 other engineering and technologies[SDU.STU]Sciences of the Universe [physics]/Earth SciencesEmpirical orthogonal functions02 engineering and technologyAtmospheric scienceslcsh:Technology01 natural scienceslcsh:TD1-1066Atmospheric radiative transfer codesPeninsulalcsh:Environmental technology. Sanitary engineeringlcsh:Environmental sciencesRetrieval algorithm021101 geological & geomatics engineering0105 earth and related environmental scienceslcsh:GE1-350geographygeography.geographical_feature_categorylcsh:Tlcsh:Geography. Anthropology. RecreationCiències de la terralcsh:G[SDU]Sciences of the Universe [physics]Brightness temperatureRadiometryEnvironmental scienceImatges Processament Tècniques digitals
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Microwave and optical data fusion for global mapping of soil moisture at high resolution

2018

After more than 8 years in orbit the Soil Moisture and Ocean Salinity (SMOS) satellite is still in good health and several algorithms for improving its spatial resolution have been proposed and validated in a variety of catchments. However, none of them has yet been applied at the global scale. In this article we present: i) a review of the latest SMOS-BEC downscaling algorithm, which allows for its global application using an adaptive moving window and ii) a thorough validation of the resulting maps over two in-situ networks: REMEDHUS in Spain and OzNet in Australia. The proposed algorithm combines SMOS brightness temperatures (at ~40 km spatial resolution), and MODIS-derived Land Surface …

BrightnessTeledetecció010504 meteorology & atmospheric sciences0211 other engineering and technologies02 engineering and technology01 natural sciences:Enginyeria agroalimentària::Ciències de la terra i de la vida::Edafologia [Àrees temàtiques de la UPC]In-situ stationsDownscalingImage resolutionWater content021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingAdaptive moving windowRemote sensing:Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Teledetecció [Àrees temàtiques de la UPC]Orbit (dynamics)Environmental scienceERA5SatelliteSoil moistureSòls -- HumitatScale (map)MicrowaveDownscalingSMOS
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Corresponding-pair procedure: a new approach to simulation of dichromatic color perception.

2004

The dichromatic color appearance of a chromatic stimulus T can be described if a stimulus S is found that verifies that a normal observer experiences the same sensation viewing S as a dichromat viewing T. If dichromatic and normal versions of the same color vision model are available, S can be computed by applying the inverse of the normal model to the descriptors of T obtained with the dichromatic model. We give analytical form to this algorithm, which we call the corresponding-pair procedure. The analytical form highlights the requisites that a color vision model must verify for this procedure to be used. To show the capabilities of the method, we apply the algorithm to different color vi…

BrightnessVisual perceptionComputer sciencebusiness.industryColor visionColor normalizationComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONColor balanceColor spaceAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsColor modelOpticsComputer visionComputer Vision and Pattern RecognitionChromatic scaleArtificial intelligencebusinessJournal of the Optical Society of America. A, Optics, image science, and vision
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Lit environments quality: A software for the analysis of luminance maps obtained with the HDR imaging technique

2013

Abstract Energy performance of lighting systems has assumed a significant role in the assessment of buildings’ consumptions and consequently lighting design is aimed to reduce installed power but at the same time to achieve an excellent lighting quality both for visual and health purposes. Lighting design is nowadays essentially based on illuminance values on visual tasks and surrounding areas, but today designers’ and researchers’ interest is focused on the analysis of luminance maps obtained through video luminance meters or with numeric simulation tools. Luminance maps availability focus the attention on a more accurate study of the light reaching the eyes (luminance), rather than on the…

Brightnessbusiness.industryComputer scienceMechanical Engineeringmedia_common.quotation_subjectIlluminanceBuilding and ConstructionEnergy savingsLuminanceSoftwareLit environments' perceptionBrightneHDR imagingComputer graphics (images)Quality (business)Computer visionArtificial intelligenceSensitivity (control systems)Electrical and Electronic EngineeringbusinessFocus (optics)Energy (signal processing)Civil and Structural Engineeringmedia_commonLuminance Maps Analysi
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BALDONE 1.2M TELESCOPE PLATE ARCHIVE - HIDDEN RESERVES OF THE FON PROJECT

2018

The plate archive of the 1.2 m Baldone telescope (Latvia) has approximately 780 and 4660 astronegatives exposed in 1967-1993 in the U (ZU21 + UG1 filter plates) and V (A600N + ZS17 filter films) closed to Johnson system U and V passbands. Digitization of astronegatives is carried out using the Epson Expression 10000XL scanner, the scanning mode is 1200 or 2400 dpi, each field covers 19 square degrees of sky.  The plates and films are scanned at the Baldone Observatory, processing of digitized scans is carried out by the observers in Baldone, at the Research Institute "Mykolaiv Astronomical Observatory" and at the Main Astronomical Observatory of the National Academy of Sciences of Ukraine. …

Brightnesseducation.field_of_studylcsh:AstronomyPopulationAstronomyAstrometrylaw.inventionlcsh:QB1-991Photometry (optics)TelescopeStarsObservatorylawscanning; processing of digitized plates; FON project; astrometry; photometry; data analysiseducationGeologyOpen clusterOdessa Astronomical Publications
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UV-PHOTOMETRY WITH THE 1.2 M SCHMIDT TELESCOPE IN BALDONE

2016

TheUniversityofLatvia's Institute of astronomy possesses a collection of 22 thousand photographic plates taken by the1.2 mSchmidt telescope located at the Baldone observatory. Among others, there are 767 astronegatives in this collection obtained in 314 sky areas using the Johnson U-filter. The field of view of each negative covers 19 square degrees. The plate scale is 72”/mm. The digitizing of the UV-collection has started in June 2016 with EPSON EXPRESSION 10000XL flatbed scanner. The general aim of the digitizing is to obtain UV-magnitudes and positions of all objects registered on the plates. Up to date near a half of the UV-collection is digitized. 24 digitized MEGA program plates of t…

Brightnesslcsh:Astronomymedia_common.quotation_subjectAstronomyField of viewSchmidt cameralaw.inventionPhotometry (optics)Telescopelcsh:QB1-991Starsdigital image processing; ultraviolet; star cataloguesSkylawObservatoryGeologymedia_commonOdessa Astronomical Publications
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Revealing the structure of the lensed quasar Q 0957+561. I. Accretion disk size

2021

We thank the anonymous referee for the helpful comments, and constructive remarks on this manuscript. We thank the GLENDAMA project for making publicly available the monitoring data of Q 0957+561. C.F. gratefully acknowledges the financial support from Tel Aviv University and University of Haifa through a DFG grant HA3555-14/1. E.M. and J.A.M are supported by the Spanish MINECO with the grants AYA2016- 79104-C3-1-P and AYA2016-79104-C3-3-P. J.A.M. is also supported from the Generalitat Valenciana project of excellence Prometeo/2020/085. J.J.V. is supported by the project AYA2017-84897-P financed by the Spanish Ministerio de Economia y Competividad and by the Fondo Europeo de Desarrollo Regi…

Brightnessmagnificationtime-delayFOS: Physical sciencesAstrophysicsgravitational lensing: microAstrophysics::Cosmology and Extragalactic AstrophysicsGravitational microlensingvlbi observationsmicro [Gravitational lensing]accretionpeculiar velocityindividual: Q 0957+561 [Quasars]Astrophysics::Galaxy AstrophysicsPhysicsquasars: individual: q 0957+561robust determinationaccretion disksvelocity dispersionq0957+561Astronomy and AstrophysicsQuasarAccretion accretion disksLight curveAstrophysics - Astrophysics of GalaxiesGalaxyAccretion (astrophysics)StarsGravitational lensdark-matterx-raySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary Astrophysicsoptical continuum emission
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Brightness and contrast do not affect visually induced motion sickness in a passively-flown fixed-base flight simulator

2016

Abstract Background Visually Induced Motion Sickness (VIMS) or simulator sickness is often elicited by a visual stimulus that lacks the appropriate vestibular or proprioceptive feedback. In this study, we chose to investigate the effects of brightness and contrast of the visual scene on VIMS. Hypothesis We hypothesized that visual environments differing in brightness or contrast would differentially induce VIMS. The symptoms of VIMS should be most severe for the combination of high brightness and high contrast and conversely lowest for the low brightness and low contrast condition. Methods 33 healthy subjects were tested in a fixed-base flight simulator. Each subject flew in four consecutiv…

Brightnessmedicine.medical_specialtygenetic structuresStimulus (physiology)AudiologyFlight simulator03 medical and health sciences0302 clinical medicineMedicine0501 psychology and cognitive sciencesComputer visionElectrical and Electronic Engineering050107 human factorsFixed baseVestibular systemProprioceptionbusiness.industry05 social sciencesbiochemical phenomena metabolism and nutritionbacterial infections and mycosesmedicine.diseaseHuman-Computer InteractionMotion sicknessHardware and ArchitectureSimulator sicknessArtificial intelligencebusiness030217 neurology & neurosurgeryDisplays
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