Search results for "Radiative Transfer"

showing 10 items of 551 documents

Comparison of Thermal Infrared Emissivities Retrieved With the Two-Lid Box and the TES Methods With Laboratory Spectra

2009

Knowledge of surface emissivity in the thermal infrared (TIR) region is critical for determining the land surface temperature (LST) from remote-sensing measurements. If emissivity is not well determined, it can cause a significant systematic error in obtaining the LST. The main aim of this paper is to compare different methods for measuring accurate land surface emissivity in the field, namely, the box method and the temperature and emissivity separation (TES) algorithm. Field emissivities were compared with soil spectra from laboratory measurements. Emissivities were measured for the bands of a multispectral radiometer CE312-2 with effective wavelengths at 8.4, 8.7, 9.1, 10.6, and 11.3 mum…

WavelengthRadiometerMaterials scienceInfraredMultispectral imageEmissivityRadiative transferGeneral Earth and Planetary SciencesRadiometryElectrical and Electronic EngineeringAtmospheric opticsRemote sensingIEEE Transactions on Geoscience and Remote Sensing
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Guidelines for the assessment of the rate law of slurry photocatalytic reactions

2017

Abstract The assessment of the rate law of slurry photocatalytic reactions appears to be a hard task, mainly because in this type of reactions the average rate of reaction, which is experimentally observed in a real reactor, could be very different from the “true” (intrinsic) rate of reaction, which cannot be measured directly. In the present work, it is shown how a proper mathematical model allows the utilization of the differential and/or the integral methods of kinetic analysis. The mathematical model must take into account not only the momentum and the mass balances, but also the radiative transfer equation. However, the discrimination among different proposed kinetic laws remains diffi…

Work (thermodynamics)Formic acid02 engineering and technology010402 general chemistryKinetic energyKinetic analysi01 natural sciencesCatalysisCatalysiMomentumReaction ratePhotocatalysiRadiative transferOrganic chemistryAbsorption (electromagnetic radiation)ChemistryLangmuir-Hinshelwood kineticChemistry (all)General ChemistryRate equationMechanics021001 nanoscience & nanotechnology0104 chemical sciencesSlurry photocatalytic reactorMechanistic kinetic modelSlurry0210 nano-technology
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Two relaxation times and thermal nonlinear waves along wires with lateral heat exchange

2021

Abstract We propose a model for studying several nonlinear waves for heat transport along a cylindrical system with lateral non-linear heat transfer to the environment. We consider relaxational equations, each with its own relaxation time, for longitudinal heat transfer and for lateral heat transfer across the wall. We consider two kinds of nonlinear lateral heat transport: radiative heat transport, and flux-limited heat transport. This work generalizes our previous studies in which the relaxation time for the lateral heat transfer was considered equal to that of the longitudinal heat flux. We explore the influence of both relaxation times on the propagation speed of linear and nonlinear wa…

Work (thermodynamics)Materials scienceThermal solitonsRelaxation (NMR)Statistical and Nonlinear PhysicsMechanicsRadiant heatCondensed Matter Physics01 natural sciencesHeat waves010305 fluids & plasmasHeat flux saturationNonlinear systemHeat flux0103 physical sciencesThermalHeat exchangerHeat transferRadiative transferMaxwell–Cattaneo law010306 general physicsAuxiliary equation methodPhysica D: Nonlinear Phenomena
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The Be/X-ray transient 4U0115+63/V635 Cassiopeiae : II. Outburst mechanisms

2001

We present multi-wavelength long-term monitoring observations of V635 Cas, the optical counterpart to the transient X-ray pulsar 4U0115+63. The evolution of emission lines and photometric magnitudes indicates that the Be star undergoes relatively fast ( ~3 - 5yr) quasi-cyclic activity, losing and reforming its circumstellar disc. We show that the general optical, infrared and X-ray behaviour can be explained by the dynamical evolution of the viscous circumstellar disc around the Be star. After each disc-loss episode, the disc starts reforming and grows until it reaches the radius at which the resonant interaction of the neutron star truncates it. At some point, the disc becomes unstable to …

X-ray transientBe starAstrophysics::High Energy Astrophysical PhenomenaAstrophysicsNeutronUNESCO::ASTRONOMÍA Y ASTROFÍSICACircumstellar matter ; Emission-line ; Stars ; 4U 0115+63 ; Binaries ; Neutron ; X-rayX-rayPulsarRadiative transferAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics::Galaxy AstrophysicsPhysicsBinariesAstronomy and AstrophysicsRadiusCircumstellar matterStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Neutron starSpace and Planetary Science4U 0115+63PrecessionAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaEmission-line:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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New view of the corona of classical T Tauri stars: Effects of flaring activity in circumstellar disks

2019

Classical T Tauri stars (CTTSs) are young low-mass stellar objects accreting mass from their circumstellar disks. They are characterized by high levels of coronal activity as revealed by X-ray observations. This activity may affect the disk stability and the circumstellar environment. Here we investigate if an intense coronal activity due to flares occurring close to the accretion disk may perturb the inner disk stability, disrupt the inner part of the disk and, possibly, trigger accretion phenomena with rates comparable with those observed. We model a magnetized protostar surrounded by an accretion disk through 3D magnetohydrodinamic simulations. We explore cases characterized by a dipole …

Young stellar objectStars: flareAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesX-rays: starsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsaccretion accretion disk01 natural sciencesmagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferProtostarAstrophysics::Solar and Stellar AstrophysicsStars: coronae010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]accretion disksStellar magnetic fieldAstronomy and Astrophysics[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]CoronaAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsHeat flux13. Climate actionSpace and Planetary ScienceStars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysics
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Atomic transition probabilities for selected Yb II lines emitted from a ferroelectric plasma source

2010

The relative intensities of several hundred emission lines of Yb II between 200 nm and 900 nm were obtained with the use of ferroelectric plasma source. These relative intensities obtained for lines from 21 energy levels have been used to determine the line branching fractions, which have then been combined with accurate experimental radiative lifetime measurements to give absolute transition probabilities for 111 Yb II lines. The obtained values were compared with theoretical and experimental data taken from available literature.

YtterbiumChemistryBranching fractionRadiative transferchemistry.chemical_elementPlasmaEmission spectrumAtomic physicsInstrumentationFerroelectricitySpectroscopyAtomic and Molecular Physics and OpticsAnalytical ChemistrySpectrochimica Acta Part B: Atomic Spectroscopy
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On the radiative impact of aerosols on photolysis rates: comparison of simulations and observations in the Lampedusa island during the ChArMEx/ADRIME…

2016

The Mediterranean basin is characterized by large concentrations of aerosols from both natural and anthropogenic sources. These aerosols affect tropospheric photochemistry by modulating the photolytic rates. Three simulations of the atmospheric composition at basin scale have been performed with the CHIMERE chemistry-transport model for the period from 6 June to 15 July 2013 covered by the ADRIMED campaign, a campaign of intense measurements in the western Mediterranean basin. One simulation takes into account the radiative effect of the aerosols on photochemistry, the second one does not, and the third one is designed to quantify the model sensitivity to a bias in the ozone column. These s…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Atmospheric ScienceOzone010504 meteorology & atmospheric sciences010501 environmental sciencesMineral dustAtmospheric sciences01 natural scienceslcsh:QC1-999AERONETAerosolSun photometerlcsh:Chemistrychemistry.chemical_compoundMediterranean seachemistrylcsh:QD1-99913. Climate actionOzone layerRadiative transferEnvironmental science14. Life underwaterAtmospheric Science; EURO-MEDITERRANEAN REGION; MASS CLOSURE; TROPOSPHERIC CHEMISTRY; CHEMICAL-COMPOSITION; STRATOSPHERIC OZONE; ACCURATE SIMULATION; OPTICAL-PROPERTIES; SATELLITE DATA; DUST; MODELlcsh:Physics0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Airborne observations of far-infrared upwelling radiance in the Arctic

2016

Abstract. The first airborne measurements of the Far-InfraRed Radiometer (FIRR) were performed in April 2015 during the panarctic NETCARE campaign. Vertical profiles of spectral upwelling radiance in the range 8–50 μm were measured in clear and cloudy conditions from the surface up to 6 km. The clear-sky profiles highlight the strong dependence of radiative fluxes to the temperature inversion typical of the Arctic. Measurements acquired for total column water vapor from 1.5 to 10.5 mm also underline the sensitivity of the far-infrared greenhouse effect to specific humidity. The cloudy cases show that optically thin ice clouds increase the cooling rate of the atmosphere by a factor up to thr…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Atmospheric ScienceRadiometer010504 meteorology & atmospheric sciencesmedia_common.quotation_subjectAtmospheric sciences01 natural scienceslcsh:QC1-999lcsh:Chemistry010309 opticsAtmospherelcsh:QD1-999Arctic13. Climate actionSky0103 physical sciencesRadianceRadiative transferEnvironmental scienceRadiometrylcsh:PhysicsWater vapor0105 earth and related environmental sciencesmedia_commonRemote sensingAtmospheric Chemistry and Physics
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SNOM signal near plasmonic nanostructures: an analogy with fluorescence decays channels

2008

International audience; Scanning Near-field Optical Microscope (SNOM) is based on local excitations of nanostructures deposited on a substrate (illumination mode). Ideally, the local source behaves like a dipolar emitter so that the SNOM signal is strongly similar to the fluorescence decay rates of an excited molecule that would be located at the SNOM tip position. We present here how the SNOM signal near plasmonic nanostructures can be used to analyze radiative and non-radiative contribution to the fluorescence decay rate.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]HistologyMaterials science[SPI.OPTI] Engineering Sciences [physics]/Optics / Photonic[SPI.NANO] Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsPhysics::Optics02 engineering and technologySubstrate (electronics)01 natural sciencesSignalPathology and Forensic Medicinelaw.inventionGOLD NANORODSplasmonOpticsOptical microscopelaw0103 physical sciencesRadiative transferMODE[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics010306 general physicsPlasmon[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryGreen's dyadic021001 nanoscience & nanotechnologyFluorescenceSantennaDENSITY[SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic[ SPI.NANO ] Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsNear-field scanning optical microscopeNanorod[ SPI.OPTI ] Engineering Sciences [physics]/Optics / Photonicfluorescence decay rateSNOM0210 nano-technologybusiness
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Analysis of the Bloch mode spectra of surface polaritonic crystals in the weak and strong coupling regimes: grating-enhanced transmission at oblique …

2004

The Bloch mode spectrum of surface plasmon polaritons (SPPs) on a finite thickness metal film has been analyzed in the regimes of weak and strong coupling between SPP modes on the opposite film interfaces. The SPP mode dispersion and associated field distributions have been studied. The results have been applied to the description of the light transmission through thick and thin periodically structured metal films at oblique incidence. In contrast to normal incidence, all SPP Bloch modes on a grating structure participate in the resonant photon tunnelling leading to the transmission enhancement. However, at the angle of incidence corresponding to the crossing of different symmetry film SPP …

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Materials scienceCondensed matter physicsbusiness.industrySurface plasmonPhysics::OpticsGrating01 natural sciencesSurface plasmon polaritonOCIS codes: (240.6680) Surface plasmons; (050.0050) Diffraction and gratings; (240.7040)Atomic and Molecular Physics and Optics010309 opticsOpticsNegative refraction0103 physical sciencesDispersion (optics)Radiative transfer010306 general physicsbusinessQuantum tunnellingComputingMilieux_MISCELLANEOUSPhotonic crystal
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