Search results for "Radiant energy"

showing 10 items of 12 documents

Special needs and characteristic features of (photo)catalytic reactors with a review of the proposed Solutions

2019

Abstract In the present chapter, the analogies between photocatalytic systems and the systems where the more common thermally activated reactions take place are highlighted. The objective is to propose a unified approach for the analysis and the design, which, however, must take into account how and why photocatalytic reactors differ from reactors with thermal reactions. The necessity of absorbing photons to activate the photocatalytic process adds complexity to the system, but some approaches are presented to simplify the problems and make easier their solution.

Photo catalyticMaterials sciencebusiness.industryPhoton absorptionPhotocatalysiQuantum yield.Scientific methodThermalPhotocatalysisPhotocatalytic reactor engineeringProcess engineeringbusinessQuantum yieldRadiant energy transfer
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The Phenomenology of Elastic Energy Loss

2007

The unexpectedly strong suppression of high p_T heavy-quarks in heavy-ion collisions has given rise to the idea that partons propagating through a medium in addition to energy loss by induced radiation also undergo substantial energy loss due to elastic collisions. However, the precise magnitude of this elastic energy loss component is highly controversial. While it is for a parton inside a medium surprisingly difficult to define the difference between elastic and radiative processes rigorously, the main phenomenological difference is in the dependence of energy loss on in-medium pathlength: in a constant medium radiative energy loss is expected to grow quadratically with pathlength, elasti…

PhysicsQuarkNuclear and High Energy PhysicsHadronElastic energyRadiant energyFOS: Physical sciencesPartonElastic collisionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Path lengthQuantum electrodynamicsRadiative transferNuclear Experiment
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Thermal characterization of insulating materials

2018

Abstract The strict energy saving standards are based on the declared values of the materials, i.e. U-value, thermal conductivity or thermal capacity. To this end, proper knowledge of the thermophysical properties of the wall components is needed, especially with regard to new lightweight technologies that are being used in building construction/refurbishment, under the dynamic conditions of the Mediterranean climate, where one of most important parameters of building materials is their heat capacity because of the influence of solar radiation energy. With this regard, the actual heat capacity value, obtained in laboratory tests, is typically quite different from the nominal one. So, this p…

EngineeringSettore ING-IND/11 - Fisica Tecnica AmbientaleRenewable Energy Sustainability and the Environmentbusiness.industryPassive cooling020209 energyScale (chemistry)Lightweight wallMechanical engineeringRadiant energyThermal flux02 engineering and technologyHeat capacitySpecific heat capacityClimatic chamberCharacterization (materials science)Thermal conductivityHeat fluxThermal0202 electrical engineering electronic engineering information engineeringbusiness
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Distribution of radiative energy in ground fog

1970

This study deals with the distribution of solar and infrared radiation in a multiple scattering and absorbing fog consisting of water droplets and water vapor. An iterative solution of the radiative transfer equation, as formulated by Chandrasekhar (1960), is presented here, which is utilized to obtain radiative intensities, fluxes and their vertical divergence for the entire infrared spectrum. A sufficient number of sample computations is carried out also in the solar spectrum such as to verify the applicability of the numerical procedure for the entire heat spectrum. All calculations are made for two fog models, representing low and high fog for a liquid cloud water concentration of 0.1 g…

PhysicsAtmospheric Science010504 meteorology & atmospheric sciencesInfraredbusiness.industryScatteringRadiant energyGeneral MedicineOceanography01 natural sciencesSpectral lineComputational physicsFogOpticsAtmospheric radiative transfer codesRadiative transferbusinessWater vapor0105 earth and related environmental sciencesTellus A: Dynamic Meteorology and Oceanography
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The Flux Density of Radiation Energy Originating from the Circumsolar Sky Measured at Groundbased Stations

1983

The aim of this project was the measurement of the radiant energy flux provided by the diffuse radiation of the ring shaped area of the sky around the unmasked sun disk. More than 200 measurements of the irradiance of this circumsolar cloudy or cloudfree sky up to an angular radius of 10° had been taken at Mainz (FRG), Deuselbach (FRG) and Adrano (Sicily). The measurements show that the irradiance of the circumsolar sky radiation may reach an amount of more then 30 % of the direct solar irradiance at the observation site. This means, optical systems combining the direct solar radiation and the circumsolar radiation may compensate — at least partly — the extinction losses of the direct solar…

AtmosphereRadiant fluxExtinction (optical mineralogy)Skymedia_common.quotation_subjectIrradianceDiffuse sky radiationAstronomyEnvironmental scienceRadiant energyAtmospheric sciencesSolar irradiancemedia_common
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A reaction engineering approach to kinetic analysis of photocatalytic reactions in slurry systems

2016

Abstract The knowledge of the rate equation is fundamental for the assessment of the activity of the photocatalytic material and for the study, design and optimization of photocatalytic reactors. In the case of photocatalytic reactions, the local volumetric rate of photon absorption (LVRPA) affects the reaction rate and its inherently uneven distribution within a “slurry” reactor makes complex a correct kinetic analysis. In the present work it is shown which are the critical aspects of the kinetic analysis in slurry reactors and how to carry out photocatalytic experiments to minimize the misinterpretations of the experimental results. In particular, the influence of the type of illumination…

Work (thermodynamics)Settore ING-IND/25 - Impianti ChimiciKINETIC ANALYSIS02 engineering and technology010402 general chemistryKinetic energy01 natural sciencesCatalysisReaction ratePhotocatalysiPhysics::Chemical PhysicsAbsorption (electromagnetic radiation)Settore ING-IND/24 - Principi Di Ingegneria ChimicaChemical reaction engineeringChemistryPhotocatalysis Kinetic analysis UVA LED Rate of photon absorption Radiant energy transfer equationGeneral ChemistryMechanicsRate equation021001 nanoscience & nanotechnologyRADIANT ENERGY TRANSFER0104 chemical sciencesVolumetric flow rateUVA LEDSRate of photon absorptionSettore CHIM/03 - Chimica Generale E InorganicaSlurry0210 nano-technology
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Hard and soft probe - medium interactions in a 3D hydro+micro approach at RHIC

2007

We utilize a 3D hybrid hydro+micro model for a comprehensive and consistent description of soft and hard particle production in ultra-relativistic heavy-ion collisions at RHIC. In the soft sector we focus on the dynamics of (multi-)strange baryons, where a clear strangeness dependence of their collision rates and freeze-out is observed. In the hard sector we study the radiative energy loss of hard partons in a soft medium in the multiple soft scattering approximation. While the nuclear suppression factor $R_{AA}$ does not reflect the high quality of the medium description (except in a reduced systematic uncertainty in extracting the quenching power of the medium), the hydrodynamical model a…

QuenchingPhysicsNuclear and High Energy PhysicsNuclear Theory010308 nuclear & particles physicsScatteringPlane (geometry)Radiant energyFOS: Physical sciencesPartonStrangenessCollision01 natural sciencesBaryonNuclear physicsNuclear Theory (nucl-th)0103 physical sciences010306 general physicsNuclear Experiment
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A flux retrieval error behavior with CERES/TRMM data

2003

With the aid of CERES/TRMM (Clouds and the Earth's Radiant Energy System/Tropical Rainfall Measuring Mission) data, sampling problems that may impact the construction of anisotropic models have been investigated. We show the influence of the sun-orbit geometry, which causes a lack of measurements in forward and backward scattering directions at large viewing zenith angles, and how cloud properties retrieval algorithms as obtained from the Visible Infrared Scanner (VIRS) also affect sampling. We have also focused our attention on the dependency of the cloud cover retrieval algorithm with respect to the viewing zenith angle (VZA), showing that the shape of the cloud cover probability density …

GeographyMeteorologybusiness.industryCloud coverFluxSampling (statistics)Radiant energyProbability density functionCloud computingOrbital mechanicsbusinessZenithRemote sensingRemote Sensing of Clouds and the Atmosphere VII
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Analysis of broadband surface BRDFs derived from TOA SW CERES measurements for surfaces classified by the IGBP land cover

2012

Most studies on the reflectance properties of the Earth's surface are addressed estimating the bidirectional reflectance distribution function (BRDF) of high spatial resolution and high spectral resolution satellite measurements. This article assesses the development of broadband (BB) BRDFs from radiances corresponding to large footprints classified according to the International Geosphere-Biosphere Programme (IGBP) land-cover classification. Top-of-atmosphere (TOA) shortwave (SW) CERES (Clouds and the Earth's Radiant Energy System) measurements are employed to invert the bidirectional reflectance factor (BRF) Rahman–Pinty–Verstraete (RPV) model for regions identified with the same IGBP typ…

Atmospheric radiative transfer codesComputationParametric modelGeneral Earth and Planetary SciencesRadiant energyEnvironmental scienceBidirectional reflectance distribution functionLand coverSpectral resolutionAtmospheric sciencesShortwaveRemote sensingInternational Journal of Remote Sensing
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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