Search results for "methods [Combined Modality Therapy]"

showing 10 items of 254 documents

'School adopts an experiment': the magnetic levitation of superconductors

2010

The event 'School adopts an experiment' is an event targeted at high schools and secondary schools. It is based on a tight and direct collaboration between researchers and school students and teachers. Several schools were involved in the event by 'adopting' an experiment in physics research laboratories. Groups of selected students were first trained by university researchers, then they demonstrated the experiments to other students and teachers during the event. Students who adopted an experiment acquired knowledge of the subjects connected with the experiment in a most impressive way compared with the usual didactics at school. Further positive points were: (i) to establish a close and d…

Physics educationLaboratory experiments and apparatuEvent (relativity)Physics educationComputingMilieux_COMPUTERSANDEDUCATIONMathematics educationGeneral Physics and AstronomySuperconducting magnets magnetic levitationSecondary schoolEducation and communication.Magnetic levitationTeaching methods and strategieEducation
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'School adopts an experiment': the photoluminescence in extra-virgin olive oil and in tonic water

2011

We report a laboratory activity, carried out along with high- and secondary-school students, that can be done to increase the interest of the young in scientific studies. Groups of selected students ‘adopted’ experiments at physics research laboratories, under the guidance of university researchers. Subsequently, the students demonstrated the experiments to the public at large during the annual science festival organized in Palermo by the association PalermoScienza, in collaboration with the University of Palermo. Experiments on the magnetic levitation of superconductors and on the photoluminescence of several substances were proposed. We discuss the experiment on photoluminescence as a cas…

Physics education; Teaching methods and strategies; Fluorescence and phosphorescence spectraPhysicsScience instructionPhysics educationTeaching methodPhysics educationGeneral Physics and AstronomyTeaching methods and strategieEducationTonic waterfoodMathematics educationfood.beverageFluorescence and phosphorescence spectraOlive oil
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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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Search for pulsations at high radio frequencies from accreting millisecond X-ray pulsars in quiescence

2010

It is commonly believed that millisecond radio pulsars have been spun up by transfer of matter and angular momentum from a low-mass companion during an X-ray active mass transfer phase. A subclass of low-mass X-ray binaries is that of the accreting millisecond X-ray pulsars, transient systems that show periods of X-ray quiescence during which radio emission could switch on. The aim of this work is to search for millisecond pulsations from three accreting millisecond X-ray pulsars, XTE J1751-305, XTE J1814-338, and SAX J1808.4-3658, observed during their quiescent X-ray phases at high radio frequencies (5 - 8 GHz) in order to overcome the problem of the free-free absorption due to the matter…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLuminosityInterstellar medium85-05pulsars general methods data analysis methods observational stars neutron X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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On Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

2010

X-ray charge-coupled devices (CCDs) are the workhorse detectors of modern X-ray astronomy. Typically covering the 0.3-10.0 keV energy range, CCDs are able to detect photoelectric absorption edges and K shell lines from most abundant metals. New CCDs also offer resolutions of 30-50 (E/dE), which is sufficient to detect lines in hot plasmas and to resolve many lines shaped by dynamical processes in accretion flows. The spectral capabilities of X-ray CCDs have been particularly important in detecting relativistic emission lines from the inner disks around accreting neutron stars and black holes. One drawback of X-ray CCDs is that spectra can be distorted by photon "pile-up", wherein two or mor…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhotonSpectrometerAstrophysics::High Energy Astrophysical PhenomenaElectron shellFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyRelativistic diskSpectral lineaccretion accretion disks black hole physics instrumentation spectrographs methods analytical X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceEmission spectrumAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSpectroscopyAstrophysics::Galaxy Astrophysics
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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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Some analytical considerations on two-scale relations

1994

Scaling functions that generate a multiresolution analysis (MRA) satisfy, among other conditions, the so-called «two-scale relation» (TSR). In this paper we discuss a number of properties that follow from the TSR alone, independently of any MRA: position of zeros (mainly for continuous scaling functions), existence theorems (using fixed point and eigenvalue arguments) and orthogonality relation between integer translates. © 1994 Società Italiana di Fisica.

PhysicsMathematics::Functional AnalysisScale (ratio)mathematical methods in physicsFixed pointIntegerProbability theoryOrthogonalityPosition (vector)Computer Science::Computer Vision and Pattern RecognitionQuantum mechanicsApplied mathematicsSettore MAT/07 - Fisica MatematicaScalingEigenvalues and eigenvectorsIl Nuovo Cimento B
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Time characteristics of Lévy flights in a steep potential well

2013

Using the method previously developed for ordinary Brownian diffusion, we derive a new formula to calculate the correlation time of stationary Lévy flights in a steep potential well. For the symmetric quartic potential, we obtain the exact expression of the correlation time of steady-state Lévy flights with index α = 1. The correlation time of stationary Lévy flights decreases with an increasing noise intensity and steepness of potential well.

PhysicsMathematics::ProbabilityLévy flightQuartic functionGeneral Physics and AstronomyNoise intensityGeneral Materials ScienceLévy flights Kolmogorov equation Frcational Fokker-Planck equation Stochastic Dynamics (theory) Methods of Stochastic Analysis Exact resultsStatistical physicsPhysical and Theoretical ChemistrySettore FIS/03 - Fisica Della MateriaBrownian motionThe European Physical Journal Special Topics
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Low energy collective modes of deformed superfluid nuclei within the finite amplitude method

2013

Background: The major challenge for nuclear theory is to describe and predict global properties and collective modes of atomic nuclei. Of particular interest is the response of the nucleus to a time-dependent external field that impacts the low-energy multipole and beta-decay strength. Purpose: We propose a method to compute low-lying collective modes in deformed nuclei within the finite amplitude method (FAM) based on the quasiparticle random-phase approximation (QRPA). By using the analytic property of the response function, we find the QRPA amplitudes by computing the residua of the FAM amplitudes by means of a contour integration around the QRPA poles in a complex frequency plane. Metho…

PhysicsNuclear and High Energy Physicsta114Nuclear TheoryIsoscalarNuclear TheoryMagnetic monopoleFOS: Physical sciencesMethods of contour integrationNuclear Theory (nucl-th)Matrix (mathematics)Classical mechanicsQuantum mechanicsAtomic nucleusQuasiparticleMultipole expansionNuclear ExperimentNuclear density
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Kinematics of Magnetic Bright Features in the Solar Photosphere

2016

S. Jafarzadeh et. al.

PhysicsPhotospherephotosphere [Sun]FOS: Physical sciencesSun: photosphereAstronomy and AstrophysicsSolar photosphereAstrophysicsKinematics01 natural sciencesMethods observationalmagnetic fields [Sun]Methods: observationalAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsobservational [Methods]010306 general physics010303 astronomy & astrophysicsSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)
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