Search results for " Radiation."

showing 10 items of 2788 documents

Compensation of Oxygen Transmittance Effects for Proximal Sensing Retrieval of Canopy–Leaving Sun–Induced Chlorophyll Fluorescence

2018

Estimates of Sun–Induced vegetation chlorophyll Fluorescence (SIF) using remote sensing techniques are commonly determined by exploiting solar and/or telluric absorption features. When SIF is retrieved in the strong oxygen (O 2 ) absorption features, atmospheric effects must always be compensated. Whereas correction of atmospheric effects is a standard airborne or satellite data processing step, there is no consensus regarding whether it is required for SIF proximal–sensing measurements nor what is the best strategy to be followed. Thus, by using simulated data, this work provides a comprehensive analysis about how atmospheric effects impact SIF estimations on proximal sensing, regarding: (…

1171 GeosciencesFLUXspectral fitting method (SFM)AIRBORNE010504 meteorology & atmospheric sciencesScience0211 other engineering and technologiesFlux02 engineering and technologyfraunhofer line discriminator (FLD)Surface pressure01 natural sciencesO2 transmittanceAtmospheric radiative transfer codesatmospheric pressureFIELD SPECTROSCOPYTransmittanceAstrophysics::Solar and Stellar AstrophysicsSPACESpectral resolutionAbsorption (electromagnetic radiation)021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingproximal sensing4112 Forestrysun-induced chlorophyll fluorescence (SIF)Atmospheric pressureSTRESS DETECTIONPHOTOSYNTHESISQAtmospheric correctionO-2 transmittanceair temperatureREFLECTANCEsun–induced chlorophyll fluorescence (SIF)Physics::Space Physicssun–induced chlorophyll fluorescence (SIF); proximal sensing; O<sub>2</sub> transmittance; fraunhofer line discriminator (FLD); spectral fitting method (SFM); air temperature; atmospheric pressureLUMINESCENCEGeneral Earth and Planetary SciencesEnvironmental scienceABSORPTION-BANDSAstrophysics::Earth and Planetary AstrophysicsVEGETATIONRemote Sensing
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Errors and uncertainties introduced by a regional climate model in climate impact assessments: example of crop yield simulations in West Africa

2015

16 pages; International audience; The challenge of estimating the potential impacts of climate change has led to an increasing use of dynamical downscaling to produce fine spatial-scale climate projections for impact assessments. In this work, we analyze if and to what extent the bias in the simulated crop yield can be reduced by using the Weather Research and Forecasting (WRF) regional climate model to downscale ERA-Interim (European Centre for Medium-Range Weather Forecasts (ECMWF) Re-Analysis) rainfall and radiation data. Then, we evaluate the uncertainties resulting from both the choice of the physical parameterizations of the WRF model and its internal variability. Impact assessments w…

2. Zero hungerMeteorologyRenewable Energy Sustainability and the EnvironmentImpact assessmentcrop modelregional climate modelYield (finance)WRFPublic Health Environmental and Occupational HealthClimate changeSARRA-H15. Life on land13. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyClimatologyWeather Research and Forecasting ModelWest AfricaEnvironmental scienceClimate modelPrecipitationShortwave radiation[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyEPICGeneral Environmental ScienceDownscaling
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Irradiated silicon detectors for HL-LHC: Characterization and simulations

2012

283 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear, de la Universidad de Valencia. Fecha de lectura: 18 julio 2012.

:FÍSICA::Física de altas energías [UNESCO]UNESCO::FÍSICA::Física del estado sólido ::Semiconductores:FÍSICA::Física del estado sólido ::Semiconductores [UNESCO]High Energy Physics; ATLAS; Silicon Detectors; Radiation Damage;UNESCO::FÍSICA::Física de altas energíasHigh Energy PhysicsATLASDetectors and Experimental TechniquesRadiation DamageSilicon Detectors
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Decorated pottery study: Analysis of pigments by x-ray absorbance spectroscopy measurements

2007

Characterization of pigments on decorated pottery fragments has been fully carried out by nondestructive x-ray absorbance spectroscopy (XAS). The samples were a series of pottery shards excavated from the archeological site of Caltagirone (Sicily, Italy), a well-known ceramic production center. Aesthetical criteria and morphological observations allowed us to attribute the samples to quite different historical periods, starting from the 18th century B.C. up to the 16th century A.D. An extensive time interval led us to suppose that different materials and techniques were used for the production of the ceramic paste and also for the preparation of pigments. XAS measurements were performed at …

ABSORPTION FINE-STRUCTUREX-ray absorption spectroscopyMaterials scienceExtended X-ray absorption fine structureAbsorption spectroscopyIDENTIFICATIONXASXAFSx-ray absorbance spectroscopy; XANES; EXAFS; pottery shardsXRFAnalytical chemistryGeneral Physics and AstronomyCOPPERXANESEXAFS XANES pigment potterypigmentvisual_artvisual_art.visual_art_mediumpigment; XRF; XASPotteryCeramicAbsorption (electromagnetic radiation)SpectroscopyRAMAN MICROSCOPY
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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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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Pressure dependence of the optical properties of wurtzite and rock-salt Zn1–xCoxO thin films

2007

In this paper we investigate the electronic structure of Zn 1-x Co x O by means of optical absorption measurements under pressure. Thin films of Zn 1-x Co x O with different Co content (from 1 to 30%) were prepared by pulsed laser deposition on mica substrates. Absorption spectra exhibit three main features that are clearly correlated to the Co content in the films: (i) absorption peaks in the infrared associated to crystal-field-split internal transitions in the Co 3d shell, with very small pressure coefficients due to their atomic character; (ii) a broad absorption band below the fundamental edge associated to charge transfer transitions, that exhibit relatively large pressure coefficient…

Absorption edgeAbsorption spectroscopyChemistryAbsorption bandPhase (matter)Analytical chemistryThin filmCondensed Matter PhysicsAbsorption (electromagnetic radiation)Electronic Optical and Magnetic MaterialsWurtzite crystal structurePulsed laser depositionphysica status solidi (b)
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X-ray CT imaging as a scientific tool to study the capillary water absorption in sedimentary rocks used in cultural heritages

2009

This paper proposes the X-Ray CT imaging as appropriate tool for investigating the capillary water absorption in sedimentary rocks. This technique, in fact, provides information useful for deeping the knowledge about of the porosity and the kinetics of the water capillary absorption in porous materials. The possibility to improve in non invasive manner, the understanding of this phenomenon, constitutes a fundamental aspect to take actions in the restoration and conservation of lapideous artifact and monuments from cultural heritages. The investigated sedimentary rocks come from different Sicilian quarries and were used for the building of the Greek temples in the archaeological areas of Agr…

Absorption of waterGeographyRegion of interestX-ray CT cultural heritagesCapillary water absorptionMineralogySedimentary rockWettingPorosityPorous mediumAbsorption (electromagnetic radiation)SPIE Proceedings
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Ab Initio Studies of Triplet-State Properties for Organic Semiconductor Molecules

2012

Triplet–triplet annihilation (TTA) leads to a reduced efficiency of organic light-emitting diodes (OLEDs) at high current densities. Spacial confinement of the triplet excitons, which is mainly dependent on triplet energy differences, can reduce the TTA rate. Therefore, a deliberate choice of the organic semiconductor materials with particular attention to their triplet energies can help to considerably increase the device efficiency. Organic solid-state lasers are, on the other hand, efficiently quenched by singlet–triplet annihilation (STA), which is closely related to the triplet–triplet absorption of the organic semiconductors. To establish a useful set of parameters related to the proc…

Absorption spectroscopyChemistryExcitonAb initio02 engineering and technology010402 general chemistry021001 nanoscience & nanotechnology7. Clean energy01 natural sciences0104 chemical sciencesSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsOrganic semiconductorGeneral EnergyChemical physicsComputational chemistryOLEDMoleculePhysical and Theoretical ChemistryTriplet state0210 nano-technologyAbsorption (electromagnetic radiation)The Journal of Physical Chemistry C
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Line intensities of CH3D in the Triad region: 6–10μm

2004

Abstract Line intensities of the three lowest fundamentals of the 12CH3D Triad are modeled with an RMS of 3.2% using over 2100 observed values retrieved by multispectrum fitting of enriched sample spectra recorded with two Fourier transform spectrometers. The band strengths of the Triad in units of 10−18 cm−1/(molecule cm−2) at 296 K are, respectively, 2.33 for ν6 (E) at 1161 cm−1, 1.75 for ν3 (A1) at 1307 cm−1 and 0.571 for ν5 (E) at 1472 cm−1. The total calculated absorption arising from 12CH3D Triad fundamentals is 4.65×10−18 cm−1/(molecule cm−2) at 296 K. In addition, some 740 intensities of nine hotbands are fitted to 8.1%; most of the hotband measurements belong to 2ν6−ν6 and ν3+ν6−ν3…

Absorption spectroscopyChemistryOrganic ChemistryFourier transform spectrometersAnalytical chemistrySpectral responseTriad (anatomy)Spectral lineAnalytical ChemistryInorganic Chemistrymedicine.anatomical_structuremedicineMoleculeAbsorption (electromagnetic radiation)SpectroscopyLine (formation)Journal of Molecular Structure
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