Search results for "Absorption"

showing 10 items of 2701 documents

Temperature dependence of the rate constant of hydrogen isotope interactions with a lithium capillary-porous system under reactor irradiation

2013

Abstract Experiments with a sample of a lithium capillary-porous system (CPS) were performed at the reactor IVG-1.M of the Institute of Atomic Energy NNC RK to study the effects of neutron irradiation on the parameters of hydrogen isotope interactions with a lithium CPS. The absorption technique was used during the experiments, and this technique allowed the temperature dependences of the hydrogen isotope interaction rate constants with the lithium CPS to be obtained under various reactor powers. The obtained dependencies were used to determine the main interaction parameters: the activation energies and the pre-exponents of the Arrhenius dependence of the hydrogen interaction rate constant…

Arrhenius equationMaterials scienceHydrogenCapillary actionMechanical EngineeringDivertortechnology industry and agricultureAnalytical chemistrychemistry.chemical_elementcomplex mixturessymbols.namesakeReaction rate constantNuclear Energy and EngineeringchemistrysymbolsAstrophysics::Solar and Stellar AstrophysicsComputer Science::Programming LanguagesGeneral Materials ScienceLithiumPhysics::Atomic PhysicsIrradiationAbsorption (chemistry)Civil and Structural EngineeringFusion Engineering and Design
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Characterization of water mobility in dry and wetted roasted coffee using low-field proton nuclear magnetic resonance

2007

Abstract Roasted and ground coffee was studied by low-field 1 H nuclear magnetic resonance at various water contents and temperatures. The spin–spin relaxation times ( T 2 ) were measured with single pulse free induction decay (FID) and Carr–Purcell–Meiboom–Gill (CPMG) sequences. Four relaxing components were distinguished: the solid population was observed with FID sequence at T 2s ∼9 μs; the other three populations, measured with the CPMG sequence, corresponded to an apolar phase, the coffee oil, and two polar phases. The two polar populations, observed at T 2m ∼6 ms and ∼27 ms (for coffee with 50% water content at 90 °C) were attributed to water in cell wall polymers and in water filling…

Arrhenius equationeducation.field_of_studyAbsorption of waterChemistryPopulationAnalytical chemistryFree induction decaySpin–spin relaxationsymbols.namesakesymbolsProton NMRPolareducationWater contentFood ScienceJournal of Food Engineering
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Development of Eco-Friendly and Self-Cleaning Lime-Pozzolan Plasters for Bio-Construction and Cultural Heritage

2020

Summarization: Nowadays, the design and use of multi-functional mortars has increased significantly, with interesting applications in the green building and cultural heritage conservation sectors. A key point for a correct adoption of these innovative materials is their behavior along time and their resistance to the weathering. The objective of this project was to define the performance and durability of innovative mortars, in order to use them correctly and to avoid irreparable damage over time. For the development of this project, lime–metakaolin and hydraulic lime–metakaolin based mortars (hereinafter called A, B), as well as A and B with the addition of nano-TiO2 and perlite (hereinaft…

Artificial ageingAbsorption of waterenergy efficient mortars; photocatalytic; cultural heritage; bio architecture; nano-titanium dioxide; artificial ageing; self-cleaning0211 other engineering and technologiesPhotocatalytic02 engineering and technologyengineering.materialnano-titanium dioxidelcsh:TH1-9745Nano-titanium dioxideenergy efficient mortarenergy efficient mortarsBio architectureFlexural strength021105 building & constructionArchitectureartificial ageingCivil and Structural EngineeringLimeEnvironmental engineeringBuilding and ConstructionPozzolancultural heritage021001 nanoscience & nanotechnologyphotocatalyticEnvironmentally friendlyDurabilitySettore ICAR/12 - Tecnologia Dell'ArchitetturaCultural heritageengineeringPerlitebio architectureEnvironmental scienceMortar0210 nano-technologySelf-cleaningself-cleaningEnergy efficient mortarslcsh:Building constructionBuildings
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Beta Decay Studies of Neutron Rich Nuclei Using Total Absorption Gamma-ray Spectroscopy and Delayed Neutron Measurements

2010

International audience; A complete characterisation of the β-decay of neutron-rich nuclei can be obtained from the measurement of β-delayed gamma rays and, whenever the process is energetically possible, β-delayed neutrons. The accurate determination of the β-intensity distribution and the β-delayed neutron emission probability is of great relevance in the fields of reactor technology and nuclear astrophysics. A programme for combined measurements using the total absorption gamma-ray spectroscopy technique and both neutron counters and neutron time-of-flight spectrometers is presented.

Astrofísica nuclearNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and AstronomyBeta decayNeutron scattering[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesNuclear physicsPrompt neutronNuclear Technology0103 physical sciencesNuclear AstrophysicsNeutron cross sectionNeutronDelayed neutrons emission010306 general physicsNuclear ExperimentSpectroscopyPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Total Absorption Gamma-Rayta114010308 nuclear & particles physicsRadioactivitat betaNeutron stimulated emission computed tomographyBeta DecayDelayed Neutron Emission3. Good healthNeutron Detectors23.40.Bw 29.30.KvNuclear astrophysicsPrompt neutronsDelayed neutronNeutron activation
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A possible cyclotron resonance scattering feature near 0.7 keV in X1822-371

2015

We analyse all available X-ray observations of X1822-371 made with XMM-Newton, Chandra, Suzaku and INTEGRAL satellites. The observations were not simultaneous. The Suzaku and INTEGRAL broad band energy coverage allows us to constrain the spectral shape of the continuum emission well. We use the model already proposed for this source, consisting of a Comptonised component absorbed by interstellar matter and partially absorbed by local neutral matter, and we added a Gaussian feature in absorption at $\sim 0.7$ keV. This addition significantly improves the fit and flattens the residuals between 0.6 and 0.8 keV. We interpret the Gaussian feature in absorption as a cyclotron resonant scattering …

Astrophysics::High Energy Astrophysical PhenomenaCyclotron resonanceFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-rays: generalLuminositysymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaAccretion accretion diskAstrophysics::Solar and Stellar AstrophysicsAbsorption (logic)Continuum (set theory)Astrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Stars: magnetic fieldStars: individual: X1822-371Astronomy and AstrophysicsRadiusAstronomy and AstrophysicX-rays: binarieInterstellar mediumNeutron starSpace and Planetary ScienceEddington luminositysymbolsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Study of the reflection spectrum of the LMXB 4U 1702-429

2016

The source 4U 1702-429 (Ara X-1) is a low-mass X-ray binary system hosting a neutron star. Albeit the source is quite bright ( $\sim10^{37}$ erg s$^{-1}$) its broadband spectrum has never been studied. Neither dips nor eclipses have been observed in the light curve suggesting that its inclination angle is smaller than 60$^{\circ}$.We analysed the broadband spectrum of 4U 1702-429 in the 0.3-60 keV energy range, using XMM-Newton and INTEGRAL data, to constrain its Compton reflection component if it is present. After excluding the three time intervals in which three type-I X-ray bursts occurred, we fitted the joint XMM-Newton and INTEGRAL spectra obtained from simultaneous observations. A bro…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral lineAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaIonization0103 physical sciencesStars: individual: 4U 1702-429Emission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsindividual: 4U 1702-429; Stars: neutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Stars]PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieAccretion (astrophysics)Stars: neutronNeutron starAbsorption edgeSpace and Planetary ScienceElectron temperatureAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Effects of radiation in accretion regions of classical T Tauri stars

2019

Models and observations indicate that the impact of matter accreting onto the surface of young stars produces regions at the base of accretion columns, in which optically thin and thick plasma components coexist. Thus an accurate description of these impacts requires to account for the effects of absorption and emission of radiation. We study the effects of radiation emerging from shock-heated plasma in impact regions on the structure of the pre-shock downfalling material. We investigate if a significant absorption of radiation occurs and if it leads to a pre-shock heating of the accreting gas. We developed a radiation hydrodynamics model describing an accretion column impacting onto the su…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsradiation: dynamics01 natural sciencesaccretion0103 physical sciencesThermalRadiative transferAstrophysics::Solar and Stellar Astrophysics010306 general physicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsultraviolet: starsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsstars: variables: T Tauristars: formationaccretion disksHerbig Ae/BeAstronomy and AstrophysicsPlasmaThermal conductionAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomena
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TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

2013

The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence le…

Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectFOS: Physical sciencesFluxField of viewAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGamma rays: general – surveys01 natural sciencesDeclination0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsgeneral – su [gamma rays]Air showerExtragalactic background light13. Climate actionSpace and Planetary ScienceSkygeneral – surveys [Gamma rays]Astrophysics - High Energy Astrophysical Phenomena
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Analysis of the aerosol radiative forcing over a Mediterranean urban coastal site

2014

Abstract The aerosol radiative forcing for the period 2003–2011 has been analyzed in Burjassot, Spain, an urban coastal site on the western Mediterranean, using measurements of global solar irradiance and aerosol properties, as well as simulated data. The aerosol radiative forcing was calculated at 5 minute intervals, and then integrated over 24 h to obtain daily mean values for 200 complete days under cloud-free skies. The monthly mean values of the aerosol radiative forcing showed a clear variation during the year, associated to the annual variability of the aerosol optical depth at 500 nm, ranging from − 6 to − 29 Wm− 2 at the surface, and from − 1.5 to − 3.9 Wm− 2 at the top of the atmo…

AtmosphereMediterranean climateCloud forcingAtmospheric ScienceAerosol radiative forcingClimatologyEnvironmental scienceRadiative forcingAbsorption (electromagnetic radiation)Solar irradianceAtmospheric sciencesAerosolAtmospheric Research
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Atmospheric water vapour content retrieval from visible and thermal data in the framework of the DAISEX campaigns

2005

In this paper three methods are presented that retrieve the atmospheric water vapour from DAIS (digital airborne imaging spectrometer) data in the framework of the DAISEX (DAIS Experiment) campaigns carried out by ESA (European Space Agency). The three methodologies analysed in the paper are: (i) the ratio technique, in which the water vapour is obtained from visible and near‐infrared bands; (ii) the split‐window technique; and (iii) the split‐window covariance‐variance ratio technique, in which the water vapour content is retrieved from thermal infrared bands. A comparison between the atmospheric water vapour content extracted from the DAIS images using these techniques and that obtained f…

AtmosphereMeteorologyThermalImaging spectrometerAtmospheric correctionGeneral Earth and Planetary SciencesAtmospheric water vapourEnvironmental scienceDaisAbsorption (electromagnetic radiation)Water vaporRemote sensingInternational Journal of Remote Sensing
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