Search results for " sperimentale"

showing 10 items of 935 documents

Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory

2017

We report a multi-resolution search for anisotropies in the arrival directions of cosmic rays detected at the Pierre Auger Observatory with local zenith angles up to $80^\circ$ and energies in excess of 4 EeV ($4 \times 10^{18}$ eV). This search is conducted by measuring the angular power spectrum and performing a needlet wavelet analysis in two independent energy ranges. Both analyses are complementary since the angular power spectrum achieves a better performance in identifying large-scale patterns while the needlet wavelet analysis, considering the parameters used in this work, presents a higher efficiency in detecting smaller-scale anisotropies, potentially providing directional informa…

moment: dipoleAstronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray experiments; ultra high energy cosmic rays; Astronomy and AstrophysicsCosmic rayanisotropyultra high energy cosmic raysSURFACE DETECTOR01 natural sciencesLARGE-SCALE DISTRIBUTIONwaveletSEARCH0103 physical sciencesARRIVAL DIRECTIONSHigh Energy Physicscosmic radiation: UHEAnisotropy010303 astronomy & astrophysicsZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleSpectral densityAstronomy and AstrophysicsEEVASTROFÍSICAComputational physicsAugerCosmic ray experiments; ultra high energy cosmic raysobservatoryDipolecosmic ray experiments ultra high energy cosmic raysRESOLUTIONMoment (physics)Experimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGpower spectrum: angular dependenceARRAYcosmic ray experimentsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Lo sviluppo dell’intelligenza linguistica e della competenza comunicativa degli studenti universitari. Un esperimento Brain-Based in Dad

2021

Il contributo presenta l’utilizzo di un approccio di tipo Brainbased allo sviluppo dell’intelligenza linguistica e della correlata competenza linguistico-comunicativa, che ha permesso la sperimentazione di una batteria di attività di Brain Gym (Dennison & Dennison, 2008) nel contesto didattico universitario durante il periodo di Didattica a Distanza (DAD) imposta dalla pandemia da Covid-19. La DAD ha comportato una drastica limitazione di alcuni elementi considerati fondanti per lo sviluppo delle competenze linguistiche, espressive e comunicative quali la corporeità, il controllo visuo-acustico, i tempi d’attenzione, la gestualità, il contatto. Nella sua fase iniziale, la ricerca condot…

movimento.Distance Learninglinguistic-communicative skillmovement.Approccio Brain-basedDADBrain-based approachBrain GymSettore M-PED/04 - Pedagogia Sperimentalecompetenza linguistico-comunicativa
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Design and implementation of the AMIGA embedded system for data acquisition

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and admin-istrative staff in Malargtie. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energla Atomica, Agencia Nacional de Promocion Cientffica y Tec-nologica (ANPCyT) , Consejo Nacional de Investigaciones Cientfficas y Tecnicas (CONICET) , Gobierno de la Provincia de Mendoza, Municipalidad de Malargtie, NDM Holdings and Valle Las Leilas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho…

muon: showersDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Physics::Instrumentation and Detectorsdata acquisitionAstronomycosmic radiation: electromagnetic componentengineeringprimary [cosmic radiation]Particle detectors01 natural sciencesenergy: thresholdData acquisition concepthardwareInstrumentationMathematical Physicsshowers [muon]media_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEControl and monitor systems onlinePhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsthreshold [energy]16. Peace & justiceAugerelectromagnetic component [cosmic radiation]observatoryDetector control systems (detector andexperiment monitoring and slow-control systemslanguageupgradeAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)atmosphere [showers]Land accessarchitectureEuropean communityairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalgorithmsPolitical science0103 physical sciencesmedia_common.cataloged_instanceddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Control and monitor systems online; Data acquisition concepts; Detector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases); Particle detectorsEuropean union010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Ciencias Exactasscintillation countershowers: atmosphere010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsData acquisition conceptsFísicastabilitylanguage.human_languagecosmic radiation: primarymonitoringResearch councilExperimental High Energy PhysicsHigh Energy Physics::ExperimentControl and monitor systems on-linePortuguese[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HumanitiesRAIOS CÓSMICOSastro-ph.IM
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Calibration of the underground muon detector of the Pierre Auger Observatory

2021

To obtain direct measurements of the muon content of extensive air showers with energy above $10^{16.5}$ eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 $\mathrm{m^2}$-modules, each segmented into 64 scintillators coupled to silicon photomultipliers (SiPMs). Direct access to the shower muon content allows for the study of both of the composition of primary cosmic rays and of high-energy hadronic interactions in the forward direction. As the muon density can vary between tens of muons per m$^2$ close to the intersection of the shower axis with the ground to much less than one per m$^2$ when far away, the necessary bro…

muon: showersdata acquisitionPhysics::Instrumentation and DetectorsAstronomyDetector alignment and calibration methods (lasers sources particle-beams)primary [cosmic radiation]Particle detectors7. Clean energy01 natural sciencesEtc)030218 nuclear medicine & medical imaging0302 clinical medicinecalibration [detector]ObservatoryAPDsdetector: calibrationatmosphere [muon]InstrumentationPhoton detectors for UVshowers [muon]Mathematical PhysicsPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDsSi-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Particle-beams)Physicsenergy: highdetector [muon]EBCCDsPhysicselectronicsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSourcesSi-PMTsdetector: alignmentAugermuon: atmosphereobservatorydensity [muon]G-APDshigh [energy]Particle detectorAstrophysics - Instrumentation and Methods for Astrophysicsatmosphere [showers]Detector alignment and calibration methods (lasers sourcesparticle-beams)FOS: Physical sciencesCosmic rayScintillatorParticle detectorVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesOpticsSilicon photomultipliermuon: density0103 physical sciencesCalibrationddc:530photomultiplier: silicon[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610High Energy PhysicsCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)scintillation counterParticle detectors; Detector alignment and calibration methods (lasers sources particle-beams); Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Performance of High Energy Physics DetectorsPierre Auger ObservatoryMuonshowers: atmosphere010308 nuclear & particles physicsbusiness.industrymuon: detectorCCDscosmic radiation: primaryDetector alignment and calibration methods (lasersEMCCDsanalog-to-digital converterAPDs; CCDs; CMOS imagers; Detector alignment and calibration methods (lasers; EBCCDs; EMCCDs; Etc); G-APDs; Particle detectors; Particle-beams); Performance of High Energy Physics Detectors; Photon detectors for UV; Si-PMTs; Sources; Visible and IR photons (solid-state) (PIN diodesExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::Experimentphoton: detectorbusinessalignment [detector]RAIOS CÓSMICOSdetector [photon]astro-ph.IM
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Un caso di living archaeology: Bibracte ed il Museo della civiltà celtica

2005

musei indoor musealizzaione outdoor archeologia sperimentale living archaeologySettore ICAR/16 - Architettura Degli Interni E Allestimento
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La «communication» de l’art préhistorique: de la pratique didactique à la redécouverte de l’invisible

2009

Les sites préhistoriques peuvent devenir les instruments de la reconnaissance de l’identité d’une communauté par rapport à son territoire. Ce sont les spectateurs du lien existant entre facteurs visibles et invisibles à l’intérieur même des sites. En ce qui concerne les découvertes préhistoriques, on a conscience que le pouvoir de témoigner le plus fort est exprimé principalement par les formes primordiales d’art rupestre. Souvent s’imposent des solutions dans lesquelles la technique est « mise au service » de la préhistoire afin de la rendre accessible au public. Cette accessibilité se réalise à travers la création d’un pôle muséal. Avec les ateliers didactiques consacrés à l’« art rupestr…

musei preistoria comunicazione archeologicaSettore ICAR/16 - Architettura Degli Interni E Allestimentoparchi preistorici comunicazione archeologica musealizzazione open-air interni museali archeologia sperimentale didattica musealeArte Rupestre Museografia Archeologia sperimentale Identità territoriale Attività didattica
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Il reciprocal teaching nella formazione iniziale degli insegnanti di sostegno della scuola secondaria di primo e secondo grado

2022

Attraverso il presente contributo si vuole verificare se nell’ambito del percorso di Specializzazione per le attività di sostegno per la Scuola secondaria di primo e secondo grado dell’Università degli Studi di Palermo, un approccio sistematico basato sul Reciprocal Teaching, con 1203 futuri insegnanti di sostegno di scuola secondaria di primo e secondo grado e materiali didattici appositamente predisposti, possa favorire il miglioramento della comprensione attraverso la capacità di sintesi e lo sviluppo di abilità metacognitive. Il Reciprocal Teaching, tra le varie strategie metacognitive è stata riconosciuta come la più solida dal punto di visto teorico e quella supportata da maggiori evi…

mutual teachingmetacognitive strategiesfuturi insegnanti sostegnoText comprehensioninsegnamento reciprocofuture support teacherSettore M-PED/04 - Pedagogia SperimentaleComprensione del testostrategie metacognitive
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NANO-EMETTITORI NIR A BASE DI SILICE PER APPLICAZIONI IN-VIVO E RELATIVO PROCESSO DI PRODUZIONE

2010

Realizzazione di nano-sonde paramagnetiche e fosforescenti, ottenibili a partire da particelle nanometriche di silice mediante procedure di sintesi e arricchimento di O2 a seguito di opportuni trattamenti termici in ambiente controllato. Le nano-sonde così ottenute presentano emissioni nel vicino infrarosso (NIR), sono eccitabili nel visibile e nel NIR, e sono caratterizzate da un tempo di vita nell’ordine del secondo. Tali nano-sonde presentano un notevole potenziale scientifico e commerciale nel mercato della spettroscopia confocale per bio-imaging e nel mercato delle applicazioni medico-farmaceutiche di drug-labelling e drug-delivery.

nano siliceprobe fluorescenti probe magnetici applicazioni in vivoNano emettitoriSettore FIS/01 - Fisica Sperimentale
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Developing emergent literacy in infant schools: a laboratory experience for the construction of the written language

2017

Research, including the educational neuroscience, has highlighted the close relationship between emerging literacy and subsequent learning of reading and writing. Early verification of symbolic and linguistic skills is essential to support the development, and recovery strategies are to be prepared in case of early signs of difficulty. In some infant schools in the Palermo area we carried out a laboratory of the last 45 hours, according to a specific methodological setting, with a dual aim: a) developing the emerging areas of literacy in preschool, b) providing teachers with an objective approach to detect in children reading and writing readiness. The study investigated phonological, lexic…

narrazioneemerging skillsstorytellingemerging skillmetodo fonematicocompetenze emergentimedia digitalilcsh:LSettore M-PED/04 - Pedagogia Sperimentaledigital mediaSettore M-PED/03 - Didattica E Pedagogia Specialephonemic methodlcsh:EducationForm@re : Open Journal per la Formazione in Rete
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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