Search results for " Instrumentation."

showing 10 items of 712 documents

The positioning system of the ANTARES Neutrino Telescope

2012

The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning sys…

Positioning systemDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Detector modelling and simulations II (electric fieldsDetector alignment and calibration methods (lasers sources particle-beams)01 natural sciencesTiming detectorshardwareDetector alignment and calibration methods010303 astronomy & astrophysicsInstrumentationDETECTOR ALIGMENTMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSOUND[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Orientation (computer vision)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsTriangulation (computer vision)particle-beams)GeodesyDETECTOR CONTROL SYSTEMDetector modelling and simulations II (electric fields charge transport multiplication and induction pulse formation electron emission etc)Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)sources[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pulse formationarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2DETECTOR MODELLING AND SIMULATIONSDetector modelling and simulations IIalgorithmsPhysics::Geophysics0103 physical sciences14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationetc)multiplication and inductionBuoyDetector control systems010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsMooringcharge transport[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Detector alignment and calibration methods (laserselectron emissionFISICA APLICADAdetector modelling and simulations ii (electric fields; antares neutrino telescope; multiplication and induction; charge transport; pulse formation; electron emission; etc); hardware; architecture; timing detectors; detector control systems (detector and experiment monitoring and slow-control systems; algorithms; databases); sources; detector alignment; calibration.; acoustic positioning; detector alignment and calibration methods (lasers; particle-beams)
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Master's level education in biomedical optics: four-year experience at the University of Latvia

2000

Pilot program for Master's studies on Biomedical Optics has been developed and launched at University of Latvia in 1995. The Curriculum contains several basic subjects like Fundamentals of Biomedical Optics, Medical Lightguides, Anatomy and Physiology, Lasers and Non-coherent Light Sources, Optical Instrumentation for Healthcare, Optical Methods for Patient Treatment, Basic Physics, etc. Special English Terminology and Laboratory-Clinical Praxis are also involved, and the Master Theses is the final step for the degree award. Following one four-year teaching experience, some observations, conclusions and eventual future activities are discussed.

Praxisbusiness.industrymedia_common.quotation_subjecteducationOptical instrumentationeye diseasesTerminologyOpticsHealth careMedicineMaster sPilot programSpecial EnglishbusinessCurriculummedia_commonSPIE Proceedings
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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

2019

The determination of the primary energy of extensive air showers using the fluorescence detection technique requires an estimation of the energy carried away by particles that do not deposit all their energy in the atmosphere. This estimation is typically made using Monte Carlo simulations and thus depends on the assumed primary particle mass and on model predictions for neutrino and muon production. In this work we present a new method to obtain the invisible energy from events detected by the Pierre Auger Observatory. The method uses measurements of the muon number at ground level, and it allows us to significantly reduce the systematic uncertainties related to the mass composition and th…

Primary energyAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodHadronFOS: Physical sciencesCosmic rayultra high energy cosmic rays01 natural sciencesNuclear physicscosmic rays0103 physical sciencesExperiments in gravityddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGénéralitésDETETORESMODEL13. Climate actioncosmic rays detectors ultra high energy cosmic raysExperimental High Energy Physicscosmic rays detectorsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyEnergy (signal processing)Physical Review D
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Approaches to evaluate the virtual instrumentation measurement uncertainties

2002

This paper deals with the metrological characterization of virtual instruments. After a brief description of the features, the components and the working principle of the virtual instruments and the various uncertainty sources are analyzed. Then, two methods to evaluate the uncertainty of the measurement results are presented: a numerical method simulating the physical process of the A/D conversion, and an approximated theoretical method applying the "uncertainty propagation law" of the "guide to the expression of uncertainty in measurement." With both methods, the combined standard uncertainty of the measurement result is obtained, starting from the standard uncertainty generated by each s…

Propagation of uncertaintyComputer simulationVirtual instrumentationEstimation theoryComputer scienceNumerical analysisProcess (computing)Control engineeringMetrologyMeasurement uncertaintySensitivity analysisElectrical and Electronic EngineeringInstrumentationUncertainty analysisIMTC 2001. Proceedings of the 18th IEEE Instrumentation and Measurement Technology Conference. Rediscovering Measurement in the Age of Informatics (Cat. No.01CH 37188)
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Measurement uncertainty estimation of a virtual instrument

2002

The law of uncertainty propagation is applied to a PC-based virtual instrument. According to the "guide to the expression of uncertainty in measurement", the measuring model and the various sources of uncertainty have been taken into account. The expressions of the combined output uncertainty in various basic digital signal processing blocks, are obtained starting from each input sample absolute accuracy, without taking into account the parameters which regard the overall behavior of an acquisition board, such as the effective number of bits. In order to verify this procedure, the results obtained by means of the theoretical analysis, are compared with the ones obtained from numerical simul…

Propagation of uncertaintyData acquisitionVirtual instrumentationComputer simulationbusiness.industryComputer scienceMeasurement uncertaintySensitivity analysisbusinessDigital signal processingUncertainty analysisSimulationProceedings of the 17th IEEE Instrumentation and Measurement Technology Conference [Cat. No. 00CH37066]
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The High A(V) Quasar Survey: Reddened quasi-stellar objects selected from optical/near-infrared photometry - II

2014

Quasi-stellar objects (QSOs) whose spectral energy distributions (SEDs) are reddened by dust either in their host galaxies or in intervening absorber galaxies are to a large degree missed by optical color selection criteria like the one used by the Sloan Digital Sky Survey (SDSS). To overcome this bias against red QSOs, we employ a combined optical and near-infrared color selection. In this paper, we present a spectroscopic follow-up campaign of a sample of red candidate QSOs which were selected from the SDSS and the UKIRT Infrared Deep Sky Survey (UKIDSS). The spectroscopic data and SDSS/UKIDSS photometry are supplemented by mid-infrared photometry from the Wide-field Infrared Survey Explo…

QSOSCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectYoung stellar objectgalaxies: activeFOS: Physical sciencesgalaxies: active; quasars: absorption lines; quasars: general; Space and Planetary Science; Astronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPhotometry (optics)quasars: general0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsLarge Magellanic CloudInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshiftGalaxyquasars: absorption linesSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Impact of Helium Ion Implantation Dose and Annealing on Dense Near-Surface Layers of NV Centers

2022

A. Berzins acknowledges support from Latvian Council of Science project lzp-2021/1-0379, “A novel solution for high magnetic field and high electric current stabilization using color centers in diamond,” and LLC “MikroTik” donation project, administered by the UoL foundation, “Improvement of Magnetic field imaging system” for the opportunity to significantly improve experimental setup as well as “Simulations for stimulation of science” for the opportunity to acquire COMSOL license. I. Fescenko acknowledges support from ERAF project 1.1.1.5/20/A/001, and I.F. and A.B. acknowledge support from LLC “MikroTik” donation project “Annealing furnace for the development of new nanometer-sized sensor…

Quantum PhysicsCondensed Matter - Materials Sciencenitrogen-vacancy centers; He ion implantation; diamond annealing; dense NV layersPhysics - Instrumentation and DetectorsCondensed Matter - Mesoscale and Nanoscale PhysicsGeneral Chemical Engineeringdiamond annealingMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciences:NATURAL SCIENCES::Physics [Research Subject Categories]Instrumentation and Detectors (physics.ins-det)nitrogen-vacancy centersHe ion implantationMesoscale and Nanoscale Physics (cond-mat.mes-hall)General Materials Sciencedense NV layersQuantum Physics (quant-ph)Nanomaterials
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Search for Axionlike Dark Matter Using Solid-State Nuclear Magnetic Resonance.

2021

Physical review letters 126(14), 141802 (2021). doi:10.1103/PhysRevLett.126.141802

Quantum chromodynamicsPhysicsPhysics - Instrumentation and DetectorsNeutron electric dipole momentRelaxation (NMR)FOS: Physical sciencesGeneral Physics and AstronomyInstrumentation and Detectors (physics.ins-det)Coupling (probability)01 natural sciences530High Energy Physics - ExperimentCondensed Matter - Other Condensed MatterHigh Energy Physics - Experiment (hep-ex)Electric dipole moment0103 physical sciencesddc:530Atomic physics010306 general physicsSpin (physics)AxionExcitationOther Condensed Matter (cond-mat.other)Physical review letters
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The SPEDE spectrometer

2017

8 pags., 10 figs., 2 tabs.

Radioactive ion beamsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsElectron spectrometerPhysics::Instrumentation and DetectorsFOS: Physical sciencesElectronnucl-ex7. Clean energy01 natural sciencesMomentumNuclear physicsInternal conversion0103 physical sciencesNuclear Physics - ExperimentDetectors and Experimental TechniquesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear Experimentphysics.ins-detPhysicsLarge Hadron ColliderSpectrometer010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Magnetic fieldPhysics::Accelerator Physics
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A new off-line ion source facility at IGISOL

2019

An off-line ion source station has been commissioned at the IGISOL (Ion Guide Isotope Separator On-Line) facility. It offers the infrastructure needed to produce stable ion beams from three off-line ion sources in parallel with the radioactive ion beams produced from the IGISOL target chamber. This has resulted in improved feasibility for new experiments by offering reference ions for Penning-trap mass measurements, laser spectroscopy and atom trap experiments.

Radioactive ion beamsNuclear and High Energy PhysicsTechnologyPhysics - Instrumentation and DetectorsMaterials sciencetutkimuslaitteetFOS: Physical sciencesSeparator (oil production)Physics Atomic Molecular & Chemical01 natural sciencesIonNuclear physicsPhysics::Plasma Physics0103 physical sciencesAtomPhysics::Atomic PhysicsIGISOLNuclear Experiment (nucl-ex)Nuclear Experiment010306 general physicsSpectroscopyNuclear Science & TechnologyDischarge ion sourceNuclear ExperimentInstrumentationInstruments & InstrumentationScience & TechnologyIsotope010308 nuclear & particles physicsPhysicsInstrumentation and Detectors (physics.ins-det)Ion sourcePhysics NuclearPhysical SciencesPhysics::Accelerator PhysicsydinfysiikkaOff lineSurface ion source
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