Search results for "reflection"

showing 10 items of 645 documents

Hyperspectral imager calibration using ceramic color tiles (Conference Presentation)

2019

Sets of chromatic and neutral ceramic tiles are widely used as measurement standards for reflectance factors in color applications. The usual instrument for color measurements is a spectrophotometer that measures the tiles using either a 0:45 or 45:0 illumination and viewing geometry, or with an integrating sphere in order to measure the reflectance factor in either specular excluded or specular included conditions. Having the corresponding measurements of the tile set from a calibrated instrument, systematic errors in the instrument under study can be diagnosed and corrected using a model of the errors and fitting it to the difference in measurements. One such is the Berns-Petersen model, …

WavelengthIntegrating sphereComputer sciencevisual_artvisual_art.visual_art_mediumHyperspectral imagingChromatic scaleSpecular reflectionTileImage sensorImage resolutionRemote sensingModeling Aspects in Optical Metrology VII
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Mode family analysis for PMMA WGM micro resonators using spot intensity changes

2021

The whispering gallery modes (WGM) micro resonators are based on elliptical objects, which can be made from optically transparent materials, The geometry of the object enables optical wave circulating inside the ellipse using total internal reflection. If there is a monochromatic light source with constant intensity to the ellipse, constructive interference may be observed. Poly methyl methacrylate acrylic (PMMA) WGM micro resonators are commercially available with typical optical quality factor of 103-104. These could limit problems with WGM micro resonator expensive manufacturing. Thanks to advances in high resolution image processing, read-outs using spectroscopy (single photo detector) …

WavelengthResonatorTotal internal reflectionMaterials scienceOpticsbusiness.industryPhotodetectorImage processingWhispering-gallery wavebusinessRefractive indexVertical-cavity surface-emitting laserLaser Resonators, Microresonators, and Beam Control XXIII
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Magneto-optical effects in multilayers illuminated by total internal reflection

1999

This paper describes the magneto-optical effects of metallic multilayers under the condition of total internal reflection. In the framework of Green’s dyadic technique, we detail a practical and at time-consuming scheme to compute accurately the optical properties of anisotropic multilayers deposited on a substrate. We present numerical simulations which account for the variation of the angle of incidence at a fixed wavelength and for the variation of the wavelength at fixed angle of incidence. The Kerr rotation is found to increase significantly around the critical angle for total reflection. We also discuss the importance of plasmon effects in the structure of the Kerr rotation spectra. @…

WavelengthTotal internal reflectionMaterials scienceOpticsAngle of incidence (optics)business.industryPhysics::OpticsSubstrate (electronics)businessAnisotropyRotationPlasmonSpectral linePhysical Review B
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Ultraviolet reflection and predation risk in diurnal and nocturnal Lepidoptera

2004

According to our extensive data on Lepidoptera (883 species), UV wing patterns are almost three times more common in nocturnal than in diurnal Lepidoptera. This might be due to predation, because the primary diurnal predators, birds, utilize UV light in foraging and even prefer UV-reflecting prey. To test this hypothesis, we conducted a field experiment with tethered living moths whose wings were artificially manipulated to reflect (UV+, reflection at UV wavelength: 15%) or absorb (UV - ) UV light, keeping longer wavelengths identical. Thus, any difference found in survival rates would be the result of the difference in wing patterns in UV spectrum. Significantly more UV+ moths th…

WingEcologyField experimentPrey detectionForagingNocturnalBiologymedicine.disease_causePredationLepidoptera genitaliaLepidoptera; predation; prey detection; ultraviolet reflectionmedicineAnimal Science and ZoologyEcology Evolution Behavior and SystematicsUltravioletBehavioral Ecology
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Broadband observations of the X-ray burster 4U1705-44 with Beppo SAX

2016

4U 1705-44 is one of the most-studied type I X-ray burster and Atoll sources. This source represents a perfect candidate to test different models proposed to self-consistently track the physical changes occurring between different spectral states because it shows clear spectral state transitions. The broadband coverage, the sensitivity and energy resolution of the BeppoSAX satellite offers the opportunity to disentangle the components that form the total X-ray spectrum and to study their changes according to the spectral state. Using two BeppoSAX observations carried out in August and October 2000, respectively, for a total effective exposure time of about 100 ks, we study the spectral evol…

X-ray bursterAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsX-rays: general01 natural sciencesSpectral lineAccretion accretion diskStars: individual: 4U 1705-44Settore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBlack-body radiationX-rays: star010303 astronomy & astrophysicsLine (formation)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicX-rays: binarieStars: neutronNeutron starSpace and Planetary ScienceReflection (physics)individual: 4U 1705-44; Stars: neutron; X-rays: binaries; X-rays: general; X-rays: stars; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Stars]Astrophysics - High Energy Astrophysical Phenomena
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Thin plastic foil X-ray optics with spiral geometry

2007

Winding a plastic foil ribbon into spiral cylinder or spiral cones we can design and build single or multiple reflection X-ray grazing incidence focusing optics with potential applications in Astronomy as well as experimental physics. The use of thin plastic foils from common industrial applications and of a mounting technique which does not require the construction of mandrels make these optics very cost effective. A spiral geometry focusing optic produces an annular image of a point source with the angular size of the annulus depending mainly on the pitch of the winding and the focal length. We use a ray-tracing code to evaluate the performances of cylindrical, and double conical spiral g…

X-ray instrumentation; grazing incidence opticsPhysicsbusiness.industryX-ray opticsGeometryConical surfaceOpticsX-ray instrumentationX-ray instrumentation grazing incidence opticsgrazing incidence opticsAnnulus (firestop)Reflection (physics)Focal lengthCylinderRay tracing (graphics)businessSpiralSPIE Proceedings
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Tracking the evolution of the accretion flow in MAXI J1820+070 during its hard state with the JED-SAD model

2021

X-ray binaries in outburst typically show two canonical X-ray spectral states, i.e. hard and soft states, in which the physical properties of the accretion flow and of the jet are known to change. Recently, the JED-SAD paradigm has been proposed for black hole X-ray binaries, aimed to address the accretion-ejection interplay in these systems. According to this model, the accretion flow is composed by an outer standard Shakura-Sunyaev disk (SAD) and an inner hot Jet Emitting Disk (JED). The JED produces both the hard X-ray emission, effectively playing the role of the hot corona, and the radio jets. In this paper, we use the JED-SAD model to describe the evolution of the accretion flow in th…

X-rays: AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesX-rays: Accretion disksSpectral lineX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesThick disk010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Accretion (meteorology)010308 nuclear & particles physicsaccretion disksAstronomy and AstrophysicsRadiusX-rays: individuals: MAXI J1820+070CoronaBlack holeISM: jets and outflowsSpace and Planetary ScienceReflection (physics)Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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Determination at low ppm levels of dithiocarbamate residues in foodstuff by vapour phase-liquid phase microextraction-infrared spectroscopy

2010

Abstract A methodology based on the vapour phase (VP) generation of carbon disulphide from non-volatile dithiocarbamate compounds has been developed for determination of pesticide residues in foodstuff at low ppm levels. The method involves a selective reaction combined with liquid phase microextraction (LPME) and transmission infrared measurements. The use of a home made transmission cell improved the detection limits (LOD) compared to the use of attenuated total reflectance measurements by a factor of approximately 80. Using the most appropriate experimental conditions for the CS2 generation and LPME preconcentration, the precision of the methodology, expressed as the relative standard de…

ZinebDetection limitchemistry.chemical_classificationResidue (complex analysis)ChromatographySpectrophotometry InfraredChemistryPesticide ResiduesAnalytical chemistryInfrared spectroscopyChemical FractionationMass spectrometryBiochemistryEthylenebis(dithiocarbamates)Gas Chromatography-Mass SpectrometryAnalytical ChemistryLimit of DetectionAttenuated total reflectionManebEnvironmental ChemistryGas chromatographyGas chromatography–mass spectrometryDithiocarbamateFood AnalysisSpectroscopyAnalytica Chimica Acta
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Manufactured object sub-segmentation based on reflection motion estimation

2015

International audience; In computer vision, reflection is a long-standing problem, it covers image textures, makes original color difficult to recognize, complicates the understanding of the scene. Most of the time, it is considered as “noise”. Many methods are proposed in order to reduce or delete the reflection effects in the image, but generally, the performances are not quite satisfactory. While instead of working on “de-noising”, we propose a method to take advantage of moving reflections that can be used for different computer vision applications. For instance, the segmentation of reflective manufactured objects is presented in this paper. We focus on tracking reflection components an…

[ INFO.INFO-TS ] Computer Science [cs]/Signal and Image ProcessingSegmentation-based object categorizationbusiness.industryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONScale-space segmentationPattern recognition02 engineering and technologyImage segmentation01 natural sciencesScale space010309 opticsImage texture[INFO.INFO-TS]Computer Science [cs]/Signal and Image ProcessingRegion growingMotion estimation0103 physical sciences0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingComputer visionArtificial intelligenceReflection (computer graphics)businessMathematics
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A Hard Look at the Neutron Stars and Accretion Disks in 4U 1636-53, GX 17+2, and 4U 1705-44 with NuStar

2017

We present $\emph{NuSTAR}$ observations of neutron star (NS) low-mass X-ray binaries: 4U 1636-53, GX 17+2, and 4U 1705-44. We observed 4U 1636-53 in the hard state, with an Eddington fraction, $F_{\mathrm{Edd}}$, of 0.01; GX 17+2 and 4U 1705-44 were in the soft state with fractions of 0.57 and 0.10, respectively. Each spectrum shows evidence for a relativistically broadened Fe K$_{\alpha}$ line. Through accretion disk reflection modeling, we constrain the radius of the inner disk in 4U 1636-53 to be $R_{in}=1.03\pm0.03$ ISCO (innermost stable circular orbit) assuming a dimensionless spin parameter $a_{*}=cJ/GM^{2}=0.0$, and $R_{in}=1.08\pm0.06$ ISCO for $a_{*}=0.3$ (errors quoted at 1 $\sig…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesAstrophysics01 natural sciencesstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesaccretion accretion disks stars: neutron X-rays: binaries X-rays: individual: 4U 1636-53 GX 17+2 4U 1705-44010303 astronomy & astrophysicsLine (formation)Spin-½PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsEquation of state (cosmology)neutron X-rays: binaries X-rays: individual: 4U 1636-53 GX 17+2 4U 1705-44 [accretion accretion disks stars]accretion disksAstronomy and AstrophysicsRadiusNeutron starReflection (mathematics)Space and Planetary Science[SDU]Sciences of the Universe [physics]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-rays: individualDimensionless quantity
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