Search results for " rays"

showing 10 items of 520 documents

Enhanced field-of-view integral imaging display using multi-Köhler illumination.

2014

A common drawback in 3D integral imaging displays is the appearance of pseudoimages beyond the viewing angle. These pseudoimages appear when the light rays coming from each elemental image are not passing through the corresponding microlens, and a set of barriers must be used to avoid this flipping effect. We present a pure optical arrangement based on Köhler illumination to generate these barriers thus avoiding the pseudoimages. The proposed system does not use additional lenses to project the elemental images, so no optical aberrations are introduced. As an added benefit, Köhler illumination provides a higher contrast 3D display. This work was supported in part by the Plan Nacional I + D …

3-D displayslight raysField of viewStereo displaySensitivity and SpecificityOpticsImaging Three-DimensionalImage Interpretation Computer-AssistedKöhler illuminationLightingviewing angleoptical arrangementPhysicsMicrolensIntegral imagingbusiness.industryReproducibility of ResultsViewing angleImage EnhancementRayAtomic and Molecular Physics and Opticsintegral imagingLight intensity3D integral imagingfield of viewselemental imagesbusinessArtifactsAlgorithmsOptics express
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Study of cosmic ray events with high muon multiplicity using the ALICE detector at the CERN Large Hadron Collider

2016

ALICE is one of four large experiments at the CERN Large Hadron Collider near Geneva, specially designed to study particle production in ultra-relativistic heavy-ion collisions. Located 52 meters underground with 28 meters of overburden rock, it has also been used to detect muons produced by cosmic ray interactions in the upper atmosphere. In this paper, we present the multiplicity distribution of these atmospheric muons and its comparison with Monte Carlo simulations. This analysis exploits the large size and excellent tracking capability of the ALICE Time Projection Chamber. A special emphasis is given to the study of high multiplicity events containing more than 100 reconstructed muons a…

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Physics::Instrumentation and Detectorshigh muon multiplicity01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICECERN[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)Nuclear Experimentcosmic rayPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Large Hadron ColliderDetectorVDP::Kjerne- og elementærpartikkelfysikk: 431ENERGY-SPECTRUMPRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]VDP::Nuclear and elementary particle physics: 431ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGcosmic rays detectorsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics and Astronomy[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FOS: Physical sciencescosmic ray experimentCosmic ray[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]EXTENSIVE AIR-SHOWERScosmic ray ; high muon multiplicity ; ALICE ; CERNBUNDLES114 Physical sciencesREGIONNuclear physicsALICE detectorcosmic rays0103 physical sciencesMultiplicity (chemistry)cosmic rays detector010306 general physicsatmospheric muonsMuon010308 nuclear & particles physicscosmic ray experiments; cosmic rays detectors;EXTENSIVE AIR-SHOWERS; ENERGY-SPECTRUM; BUNDLES; REGION; LEPAstronomy and AstrophysicsLEP115 Astronomy Space scienceNATURAL SCIENCES. Physics.13. Climate actioncosmic ray experiments; cosmic rays detectors; Astronomy and AstrophysicsHigh Energy Physics::Experimentcosmic ray experiments
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

2011

The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies $E>E_{th}=5.5\times 10^{19}$ eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at $E>E_{th}$ are heavy nuclei with charge $Z$, the proton component of the sources should lead to excesses in the same regions at energies $E/Z$. We here report the lack of anisotropies in these directions at energies above $E_{th}/Z$ (for illustrative values of $Z=6,\ 13,\ 26$). If the anisotropies above $E_{th}$ are du…

ACTIVE GALACTIC NUCLEI[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ProtonAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentAcceleration (differential geometry)Cosmic rayultra high energy cosmic rays; cosmic ray experimentsultra high energy cosmic rays7. Clean energy01 natural sciencesultra high energy cosmic rayAugerNuclear physics0103 physical sciencesUltra-high-energy cosmic ray010306 general physicsAnisotropyNuclear ExperimentDETECTORHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaCharge (physics)Astronomy and Astrophysics13. Climate actionExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaJournal of Cosmology and Astroparticle Physics
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First Multi-wavelength Campaign on the Gamma-ray-loud Active Galaxy IC 310

2017

The extragalactic VHE gamma-ray sky is rich in blazars. These are jetted active galactic nuclei viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a larger angle are known so far to emit above 100 GeV. Multi-wavelength studies of such objects up to the highest energies provide new insights into the particle and radiation processes of active galactic nuclei. We report the results from the first multi-wavelength campaign observing the TeV detected nucleus of the active galaxy IC 310, whose jet is observed at a moderate viewing angle of 10 deg - 20 deg. The multi-instrument campaign was conducted between 2012 Nov. and 2013 Jan., and involved observations with MAG…

Active galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesEnergy fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxies: active; Galaxies: individual: IC 310; Gamma rays: galaxies; Astronomy and Astrophysics; Space and Planetary Science01 natural scienceslaw.inventionlawGalaxies: individual: IC 3100103 physical sciencesindividual: IC 310 [galaxies]Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgalaxie [Gamma rays]010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsGalaxies: activeAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesSynchrotrongamma rays: galaxies ; galaxies: active ; individual (IC 310)Gamma rays: galaxiesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)active [galaxies]galaxies [gamma rays]ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGSpectral energy distributionddc:520Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeFlare
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Long-term monitoring of mrk 501 for its very high energy γ emission and a flare in 2011 october

2012

"As one of the brightest active blazars in both X-ray and very high energy γ -ray bands, Mrk 501, is very useful for" "physics associated with jets from active galactic nuclei. The ARGO-YBJ experiment has monitored Mrk 501 for γ - rays above 0.3 TeV since 2007 November. The largest flare since 2005 was observed from 2011 October and lasted until about 2012 April. In this paper, a detailed analysis of this event is reported. During the brightest γ -ray flaring episodes from 2011 October 17 to November 22, an excess of the event rate over 6σ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the γ -ray flux above 1 TeV by a factor of 6.6 ± 2.2 from its steady…

Active galactic nucleusactive" ["galaxies]Astrophysics::High Energy Astrophysical PhenomenaFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencesBlazar010303 astronomy & astrophysicsPhysicsindividual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermal [BL Lacertae objects]" "general" ["gamma rays]010308 nuclear & particles physicsBL Lacertae objects: individual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermalSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsQuasarGalaxyindividual (Markarian 501)" ["BL Lacertae objects]13. Climate actionSpace and Planetary ScienceSpectral energy distributionFlare
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Effects of Infrared-A Irradiation on Skin: Discrepancies in Published Data Highlight the Need for an Exact Consideration of Physical and Photobiologi…

2010

Skin exposure to infrared (IR) radiation should be limited in terms of irradiance, exposure time and frequency in order to avoid acute or chronic damage. Recommendations aimed at protecting humans from the risks of skin exposure to IR (e.g. ICNIRP, ACGIH) are only defined in terms of acute effects (e.g. heat pain and cardiovascular collapse), whereas the actual exposure conditions (e.g. spectral distribution, exposure geometry, frequency and number of exposures, thermal exchange with the environment, metabolic energy production and regulatory responses) are not taken into consideration. Since the IR component of solar radiation reaching the Earth's surface is mainly IR-A, and considering th…

Acute effectsMetabolic energyInfrared RaysInfraredChemistrySkin exposureHeat painGeneral MedicineModels TheoreticalRadiationModels BiologicalBiochemistryBiophysical PhenomenaPhotobiologyLawTissue damageHumansIrradiationPhysical and Theoretical ChemistrySkinPhotochemistry and Photobiology
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Response of membrane-bound ATPase of Micrococcus luteus to heat and ultraviolet light.

1976

It is shown that the properties of ATPase (EC 3.6.1.3) of Micrococcus luteus depend only to some extent on the state of the membrane to which it is attached. Its interaction with the membrane appears to be largely controlled by polar forces. It is shown, however, that the UV-sensitivity of the membrane-bound ATPase is also significantly influenced by the state of membrane lipids.

Adenosine TriphosphatasesRadiationHot TemperatureMembranesbiologyChemistryMembrane boundUltraviolet RaysMembrane lipidsATPaseBiophysicsMicrococcusDose-Response Relationship RadiationPhospholipasebiology.organism_classificationMicrococcusRadiation EffectsMembraneBiochemistryPhospholipasesUltraviolet lightbiology.proteinMicrococcus luteusGeneral Environmental ScienceRadiation and environmental biophysics
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Spectral Transmission of the Human Crystalline Lens in Adult and Elderly Persons: Color and Total Transmission of Visible Light

2012

Purpose To experimentally measure the spectral transmission of human crystalline lenses belonging to adult and elderly persons, and to determine the color and total transmission of visible light of such crystalline lenses. Methods The spectral transmission curve of 32 human crystalline lenses was measured using a PerkinElmer 800UV/VIS spectrometer. Total transmission of visible light and the chromatic coordinates of these crystalline lenses were determined from these curves for solar illumination. Results The crystalline lens that filters UV and its transmission in the visible spectrum decreases with age; such a decrease is greater for short wavelengths. The total transmission of visible li…

AdultMaleAgingMaterials scienceUltraviolet RaysColorMineralogylaw.inventionOpticsElderly personslawLens CrystallineTransmittanceHumansChromatic scaleAgedSunlightSpectrometerbusiness.industrySpectrum AnalysisMiddle Agedeye diseasesLens (optics)WavelengthSunlightFemalesense organsbusinessPhotic StimulationVisible spectrumInvestigative Opthalmology & Visual Science
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In vivo release of non-neuronal acetylcholine from human skin by dermal microdialysis: Effects of sunlight, UV-A and tactile stimulus

2007

Non-neuronal acetylcholine (ACh) is expressed in epithelial, endothelial and immune cells. For example, the in vivo release of ACh from the human skin pretreated with botulinum toxin has recently been demonstrated. In the present experiments the effects of light (sunlight and solar radiation by a commercial UV-A applier) and of a tactile stimulus on the release of non-neuronal ACh were investigated. Release of ACh from the proximal and distal shin, i.e. anterior tibial region, was measured by dermal microdialysis in 20 min samples over a time period of at least 140 min. Control experiments were performed in a dark room throughout. In some experiments volunteers were exposed to sunshine (80-…

AdultMaleMicrodialysisTime FactorsInjections IntradermalUltraviolet RaysMicrodialysisHuman skinStimulus (physiology)General Biochemistry Genetics and Molecular BiologyIn vivoPhysical StimulationmedicineHumansGeneral Pharmacology Toxicology and PharmaceuticsSkinNeuronsSunlightChemistryGeneral MedicineAnatomyAcetylcholineNon neuronal acetylcholineDermal microdialysisSunlightBiophysicsFemaleAcetylcholinemedicine.drugLife Sciences
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