Search results for "Dual"

showing 10 items of 2547 documents

International Legal Approaches to Waste Water Discharges. Opening speech

2002

En este discurso inaugural, realizo una introducción a la frustrante situación jurídica en la que se encuentran las descargas de aguas residuales a nivel internacional. Las descargas de aguas residuales son la mayor fuente de contaminación marina y, en consecuencia, ellas representan el mayor riesgo actual para la protección del medio ambiente marino. In this opening speech, I make an introduction to the disappointing legal situation of waste water discharges at international level. Waste water discharges is the main source of marine pollution and, therefore, they represent the major current risk to the protection of the marine environment.

Waste water dischargesProtección del medio ambiente marinoContaminación marina:CIENCIAS JURÍDICAS Y DERECHO [UNESCO]Marine pollutionUNESCO::CIENCIAS JURÍDICAS Y DERECHODescargas de aguas residualesProtection of the marine environment
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On the FE codes capability for tool temperature calculation in machining processes

2006

Abstract The applications of numerical simulation to machining processes have been more and more growing in the last years: today a quite effective predictive capability has been reached, at least as far as global cutting variables (for instance cutting forces) are concerned. On the other hand, the capability to predict local cutting variables (i.e. pressure on the tool, temperature distribution, residual stresses in the machined surface) has to be heavily improved and verified. At the same time, effective experimental procedures for validating numerical results have to be developed. In this work two different approaches were implemented for temperature measuring: a thermocouple based appro…

Work (thermodynamics)EngineeringComputer simulationbusiness.industryMetals and AlloysMechanical engineeringIndustrial and Manufacturing EngineeringFinite element methodComputer Science ApplicationsMachined surfaceMachiningThermocoupleResidual stressModeling and SimulationThermalCeramics and Compositesbusiness
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Calibration and simulation of ASM2d at different temperatures in a phosphorous removal pilot plant

2006

In this work, an organic and nutrient removal pilot plant was used to study the temperature influence on phosphorus accumulating organisms. Three experiments were carried out at 13, 20 and 24.5 degrees C, achieving a high phosphorus removal percentage in all cases. The ASM2d model was calibrated at 13 and 20 degrees C and the Arrhenius equation constant was obtained for phosphorus removal processes showing that the temperature influences on the biological phosphorus removal subprocesses in a different degree. The 24.5 degrees C experiment was simulated using the model parameters obtained by means of the Arrhenius equation. The simulation results for the three experiments showed good corresp…

Work (thermodynamics)Environmental Engineeringchemistry.chemical_elementPilot ProjectsSoil scienceWater PurificationDegree (temperature)symbols.namesakeNutrientCalibrationWater Science and TechnologyArrhenius equationSewagePhosphorusTemperatureEnvironmental engineeringAigües residuals EliminacióPhosphorusModels StructuralPilot plantEnhanced biological phosphorus removalchemistryCalibrationsymbolsEnvironmental scienceAigües residuals Plantes de tractament
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On the mechanisms involved in the tensile strength of a dissimilar Ti6Al4V/316L laser welded assembly

2021

International audience; The aim of the present work is to analyze the thermomechanical behavior of dissimilar laser seams by means of FE modeling. The case of a Ti6Al4V/316L assembly with vanadium insert was considered. Effective mechanical properties of the main materials and cords were first estimated from NHT measurements. Modeling of the double pass laser welding process was performed first by considering shrinking of the two weld seams during manufacturing, to get the residual stress state in the welded assembly. Modeling of the tensile test was performed in a second step to study the assembly behavior during loading. In these modeling results, the mesh was the cross-section of the mic…

Work (thermodynamics)Materials scienceComputational Mechanicstensile load02 engineering and technologyWelding01 natural scienceslaw.inventionStress (mechanics)[SPI]Engineering Sciences [physics]lawResidual stress316L stainless steel0103 physical sciencesUltimate tensile strengthMaterials Chemistryvanadium insertComposite materialFEM modelingTensile testing010302 applied physicsdissimilar weldingMetals and AlloysTi6Al4VTitanium alloyLaser beam welding021001 nanoscience & nanotechnologylaserMechanics of Materialsresidual stresses0210 nano-technology
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Impact of Superfinish Turning on Surface Integrity of Pure Copper

2011

Abstract The presented study deals with comprehension of relationships between machining cutting conditions and physical-chemical properties linked with surface integrity. A multi-physics model is presented to calculate residual stress, temperature and dislocation fields in the machined material. This model includes both thermal-mechanical, structural evolution and dynamic recristallisation approaches. The model was applied to pure copper after superfinish turning. Good agreement was found between numerical values and experimental ones. This paper also presents a work on the impact of mechanical and microstructural changes induced by machining on the electrochemical behaviour and corrosion …

Work (thermodynamics)Materials scienceMetallurgyCorrosion resistancechemistry.chemical_elementGeneral MedicineCopperStructural evolutionCorrosionSurface integrityMachiningchemistryResidual stressSuperfinish turningDislocationEngineering(all)Surface integrityProcedia Engineering
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The BeppoSAX 0.1 - 18 keV Spectrum of the Bright Atoll Source GX 9+1: an Indication of the Source Distance

2005

We report the results of a long, 350 ks, BeppoSAX observation of the bright atoll source GX 9+1 in the 0.12 - 18 keV energy range. During this observation GX 9+1 showed a large count rate variability in its lightcurve. From its color - color diagram we selected six zones and extracted the source energy spectrum from each zone. We find that the model, composed of a blackbody plus a Comptonized component absorbed by an equivalent hydrogen column of similar to 1.4 x 10(22) cm(-2), fits the spectra in the energy range 1 - 18 keV well; however, below 1 keV a soft excess is present. We find that the spectrum of GX 9+1, in the 0.12 - 18 keV energy range, is well fitted by the model above, if we us…

X-ray : binariestars : individual : GX 9+1X-ray : generalaccretion accretion discs; stars : individual : GX 9+1; stars : neutron; X-ray : stars; X-ray : binaries; X-ray : general:accretion accretion discX-ray : starstars : neutron
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Broadband observations of the X-ray burster 4U1705-44 with Beppo SAX

2016

4U 1705-44 is one of the most-studied type I X-ray burster and Atoll sources. This source represents a perfect candidate to test different models proposed to self-consistently track the physical changes occurring between different spectral states because it shows clear spectral state transitions. The broadband coverage, the sensitivity and energy resolution of the BeppoSAX satellite offers the opportunity to disentangle the components that form the total X-ray spectrum and to study their changes according to the spectral state. Using two BeppoSAX observations carried out in August and October 2000, respectively, for a total effective exposure time of about 100 ks, we study the spectral evol…

X-ray bursterAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsX-rays: general01 natural sciencesSpectral lineAccretion accretion diskStars: individual: 4U 1705-44Settore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBlack-body radiationX-rays: star010303 astronomy & astrophysicsLine (formation)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicX-rays: binarieStars: neutronNeutron starSpace and Planetary ScienceReflection (physics)individual: 4U 1705-44; Stars: neutron; X-rays: binaries; X-rays: general; X-rays: stars; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Stars]Astrophysics - High Energy Astrophysical Phenomena
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Towards purely inorganic clusters in medicine: Biocompatible divalent cations as counterions of cobaltabis(dicarbollide) and its iodinated derivatives

2021

Monovalent cations, Cs+, and alkylammonium ([NR4]+) salts have traditionally been used to precipitate the anions of boranes, carborane and metallocarborane clusters. In contrast, in the body and in living organisms in general, divalent cations have a special relevance. In this work, we isolate for the first time the cobaltabis(dicarbollide) salts of the biocompatible divalent cations of biological importance that can have application both in biology and in materials science. The preparation of Ca2+, Mg2+ and Fe2+ salts of anionic iodinated nido-[C2B9H12]− and cobaltabis(dicarbollide) as well as its di-, tetra- and octa-iodinated derivatives are reported. Ca2+ and Mg2+ are hard Lewis acids a…

X-ray contrastanionitDual-actionBoranesBiochemistryDivalentjodiInorganic Chemistrychemistry.chemical_compoundBone biomaterialsPolymer chemistryMaterials ChemistryAcetoneMoleculeLewis acids and basesPhysical and Theoretical Chemistrychemistry.chemical_classificationkalsiumChemistrydual-action biocompatibleOrganic ChemistrykationitSmall moleculeBiocompatibleX-ray contrastCarboraneCalciumMetallacarboranesCounterionbiomateriaalitIodine
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First observations of the X-ray transient EXO 2030+375 with IBIS/ISGRI

2003

We present a first INTEGRAL observation of the 42s transient X-ray pulsar EXO 2030+375 with IBIS/ISGRI. The source was detected during Cyg X-1 observations in December 2002. We analyzed observations during the outburst period from 9 to 21 December 2002 with a total exposure time of ~770 kiloseconds. EXO 2030+375 was almost always detected during single ~30 minute exposures in the 18-45 energy bands. The source light curve shows the characteristic outburst shape observed in this source.

X-ray transientFOS: Physical sciencesIndividualAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsGamma rays ; Observations ; X-rays ; Individual ; EXO 2030+375 ; Telescopes ; INTEGRAL ; IBISPulsarX-raysObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]PhysicsIbisEXO 2030+375biologyINTEGRALUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAstrophysics (astro-ph)Astronomy and Astrophysicsbiology.organism_classificationLight curveSpace and Planetary ScienceIBIS:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Telescopes
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Tracking the evolution of the accretion flow in MAXI J1820+070 during its hard state with the JED-SAD model

2021

X-ray binaries in outburst typically show two canonical X-ray spectral states, i.e. hard and soft states, in which the physical properties of the accretion flow and of the jet are known to change. Recently, the JED-SAD paradigm has been proposed for black hole X-ray binaries, aimed to address the accretion-ejection interplay in these systems. According to this model, the accretion flow is composed by an outer standard Shakura-Sunyaev disk (SAD) and an inner hot Jet Emitting Disk (JED). The JED produces both the hard X-ray emission, effectively playing the role of the hot corona, and the radio jets. In this paper, we use the JED-SAD model to describe the evolution of the accretion flow in th…

X-rays: AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesX-rays: Accretion disksSpectral lineX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesThick disk010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Accretion (meteorology)010308 nuclear & particles physicsaccretion disksAstronomy and AstrophysicsRadiusX-rays: individuals: MAXI J1820+070CoronaBlack holeISM: jets and outflowsSpace and Planetary ScienceReflection (physics)Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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