Search results for "LABOR"

showing 10 items of 3876 documents

Chemical Evolution of Interstellar Methanol Ice Analogs upon Ultraviolet Irradiation: The Role of the Substrate

2018

An important issue in the chemistry of interstellar ices is the role of dust materials. In this work, we study the effect of an amorphous water-rich magnesium silicate deposited onto ZnSe windows on the chemical evolution of ultraviolet-irradiated methanol ices. For comparison, we also irradiate similar ices deposited onto bare ZnSe windows. Silicates are produced at relatively low temperatures exploiting a sol-gel technique. The chemical composition of the synthesized material reflects the forsterite stoichiometry. Si-OH groups and magnesium carbonates are incorporated during the process. The results show that the substrate material does affect the chemical evolution of the ice. In particu…

PhysicsAstrochemistryastrochemistryExtinction (astronomy)methods: laboratory: molecularSubstrate (chemistry)Astronomy and AstrophysicsISM: moleculeAstronomy and AstrophysicPhotochemistryultraviolet: ISM01 natural sciencesChemical evolutionchemistry.chemical_compoundchemistrySpace and Planetary Science0103 physical sciencesUltraviolet irradiationdust extinctionMethanol010306 general physics010303 astronomy & astrophysicsThe Astrophysical Journal
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SOFT X-RAY IRRADIATION OF PURE CARBON MONOXIDE INTERSTELLAR ICE ANALOGUES

2012

There is an increasing evidence for the existence of large organic molecules in the interstellar and circumstellar medium. Very few among such species are readily formed in conventional gas-phase chemistry under typical conditions of interstellar clouds. Attention has therefore focused on interstellar ices as a potential source of these relatively complex species. Laboratory experiments show that irradiation of interstellar ice analogues by fast particles or ultraviolet radiation can induce significant chemical complexity. However, stars are sources of intense X-rays at almost every stage of their formation and evolution. Such radiation may thus provide chemical changes in regions where ult…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaInterstellar icePhotodissociationInterstellar cloudAstronomy and AstrophysicsAstrophysicsRadiationmolecules | X-rays: ISM | methods: laboratory [ISM]Starschemistry.chemical_compoundSettore FIS/05 - Astronomia E AstrofisicachemistrySpace and Planetary ScienceISM: molecules | X-rays: ISM | methods: laboratoryAstrophysics::Earth and Planetary AstrophysicsIrradiationAstrophysics::Galaxy AstrophysicsOrder of magnitudeCarbon monoxide
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Characterization of a Be(p,xn) Neutron Source for Fission Yields Measurements

2013

We report on measurements performed at The Svedberg Laboratory (TSL) to characterize a proton-neutron converter for independent fission yield studies at the IGISOL-JYFLTRAP facility (Jyv\"askyl\"a, Finland). A 30 MeV proton beam impinged on a 5 mm water-cooled Beryllium target. Two independent experimental techniques have been used to measure the neutron spectrum: a Time of Flight (TOF) system used to estimate the high-energy contribution, and a Bonner Sphere Spectrometer able to provide precise results from thermal energies up to 20 MeV. An overlap between the energy regions covered by the two systems will permit a cross-check of the results from the different techniques. In this paper, th…

PhysicsBonner sphereNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsSpectrometerta114010308 nuclear & particles physicsFissionNuclear TheoryNuclear dataFOS: Physical sciencesFission product yieldInstrumentation and Detectors (physics.ins-det)7. Clean energy01 natural sciencesThe Svedberg LaboratoryNuclear physics0103 physical sciencesNeutron sourceNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentNuclear Data Sheets
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An inquiry-based approach to Maxwell distribution: a case study with engineering students

2013

The concept of distribution is a fundamental component of statistical thinking. This paper describes a teaching approach for it that uses a specific activity related to the field of statistical mechanics. The concept of the velocity distribution of a particle system is dealt with using an inquiry-based approach involving an experimental examination of Maxwell’s distribution. Some outcomes of a teaching experiment held at the Faculty of Engineering of the University of Palermo, Italy are described.

PhysicsDistribution (number theory)Research in physics education Teaching methods and strategies Laboratory experiments and apparatus Laboratory course design organization and evaluationClassical statistical mechanicsSettore FIS/08 - Didattica E Storia Della Fisica05 social sciences050301 educationGeneral Physics and AstronomyStatistical mechanics01 natural sciencesMaxwell–Boltzmann distributionField (geography)symbols.namesakeTheoretical physicsStatistical thinkingComponent (UML)0103 physical sciencessymbolsMathematics education010306 general physics0503 educationEuropean Journal of Physics
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Which Reaches the Bottom First?

2008

A well-known classroom demonstration involves the rolling of hollow and solid objects down an incline.1 The fact that the objects roll at different rates can be used as a starting point in introducing students to rotational dynamics and rotational kinetic energy. In this paper we describe a simple quantitative version of the demonstration that is suitable for use as a laboratory experiment.

PhysicsFísicaGeneral Physics and AstronomyMechanical engineeringCiència ExperimentsCiència EnsenyamentEducationRotational energyMomentumAccelerationClassical mechanicsSimple (abstract algebra)Point (geometry)Laboratory experimentRotational dynamicsEnergy (signal processing)The Physics Teacher
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Non-thermal processes in coronae and beyond

2013

This contribution summarizes the splinter session “Non-thermal processes in coronae and beyond” held at the Cool Stars 17 workshop in Barcelona in 2012. It covers new developments in high energy non-thermal effects in the Earth's exosphere, solar and stellar flares, the diffuse emission in star forming regions and reviews the state and the challenges of the underlying atomic databases. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

PhysicsHigh energyStarsSolar flareSpace and Planetary ScienceThermalAstronomyAstronomy and AstrophysicsMethods laboratoryExosphereAtomic dataAstronomische Nachrichten
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βdecay of102Y produced in projectile fission of238U

2012

The population of 102Zr following the β decay of 102Y produced in the projectile fission of 238U at the GSI facility in Darmstadt, Germany has been studied. 102Y is known to ß decay into 102Zr via two states, one of high spin and the other low spin. These states preferentially populate different levels in the 102Zr daughter. In this paper the intensities of transitions in 102Zr observed are compared with those from the decay of the low-spin level studied at the TRISTAN facility at Brookhaven National Laboratory and of the high-spin level studied at the JOSEF separator at the Kernforschungsanlage Jülich.

PhysicsHistoryeducation.field_of_studyCluster decayFissionProjectilePopulationBeta decayddc:Computer Science ApplicationsEducationNuclear physicsSubatomic PhysicsHigh Energy Physics::ExperimentAtomic physicsNuclear ExperimentSpin (physics)National laboratoryeducationJournal of Physics: Conference Series
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From led light signboards to the Planck’s constant

2018

Recent studies have highlighted an alarming decline in young people’s interest towards the study of scientific subjects, often considered interesting but not easily understood and appreciated by students. In particular, the introduction of Modern Physics (MP) key-topics at secondary school level is a difficult and complex task because MP involves abstract ideas and requires a strong mathematical background. In this communication we present and discuss the results of an inquiry-based teaching/learning path aimed at surmounting the difficulties of an exclusively theoretical approach to the introduction of MP topics. In particular, we planned and realized an inquiry-driven learning environment…

PhysicsHistorysymbols.namesakeQuantum electrodynamicsSettore FIS/08 - Didattica E Storia Della FisicasymbolsModern Physics teaching Laboratory Inquiry-based approach Critical thinkingPlanckConstant (mathematics)Settore FIS/03 - Fisica Della MateriaSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Computer Science ApplicationsEducation
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Influence of the input-stage architecture on the in-laboratory test of a mid-infrared interferometer: application to the ALOHA up-conversion interfer…

2020

ABSTRACT In the framework of the Astronomical Light Optical Hybrid Analysis (ALOHA) laboratory mid-infrared (MIR) up-conversion fibred interferometer in the L band, we report on the influence of the input-stage architecture. Using an amplitude division set-up in the visible or near-infrared is a straightforward choice in most cases. In the MIR context, the results are slightly different and we show that a wavefront division set-up is needed. These in-laboratory principle experiments allow us to measure a reliable 88 per cent instrumental contrast with high flux and to obtain fringes from faint sources at 3.5 μm with a spectral bandwith of 37 nm converted to 817 nm. An equivalent limiting L-…

PhysicsL bandbusiness.industryMid infraredAstronomy and Astrophysics01 natural sciencesInterferometryLaboratory testOpticsSpace and Planetary ScienceAloha0103 physical sciencesUp conversionStage (hydrology)010306 general physicsbusiness010303 astronomy & astrophysicsMonthly Notices of the Royal Astronomical Society
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Emission-Line Intensity Ratios in F[CLC]e[/CLC] [CSC]xvii[/CSC] Observed with a Microcalorimeter on an Electron Beam Ion Trap

2000

We report new observations of emission line intensity ratios of Fe XVII under controlled experimental conditions, using the National Institute of Standards and Technology electron beam ion trap (EBIT) with a microcalorimeter detector. We compare our observations with collisional-radiative models using atomic data computed in distorted wave and R-matrix approximations, which follow the transfer of the polarization of level populations through radiative cascades. Our results for the intensity ratio of the 2p6 1S0-2p53d 1P1 15.014 A line to the 2p6 1S0-2p53d 3D1 15.265 A line are 2.94 ± 0.18 and 2.50 ± 0.13 at beam energies of 900 and 1250 eV, respectively. These results are not consistent wit…

PhysicsMethods: laboratorySun: coronaDetectorTechniques: spectroscopicAstronomy and Astrophysicslaboratory; Stars: individual (Capella); Sun: corona; Techniques: spectroscopic; X-rays: general [Atomic data; Methods]PlasmaX-rays: generalIntensity ratioPolarization (waves)IonSettore FIS/05 - Astronomia E AstrofisicaStars: individual (Capella)Space and Planetary ScienceRadiative transferEmission spectrumAtomic physicsAtomic dataElectron beam ion trapThe Astrophysical Journal
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