Search results for "Instrumentation"

showing 10 items of 4914 documents

Structure of N >= 126 nuclei produced in fragmentation of (238)U

2009

The nuclear structure of neutron‐rich N⩾126 nuclei have been investigated following their production via relativistic projectile fragmentation of a E/A = 1 GeV 238U beam on a Be target. The cocktail of secondary beam products were separated and identified using the GSI FRagment Separator (FRS). The nuclei of interest were implanted in a high‐granularity active stopper detector set‐up consisting of 6 double sided silicon strip detectors. The associated gamma‐ray transitions were detected with the RISING array, consisting of 15 Euroball cluster Ge‐detectors. Time‐correlated gamma decays from individually identified nuclear species have been recorded, allowing the clean identification of isome…

PhysicsNuclear reactionPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGamma rayParticle detectorSemiconductor detectorNuclear physicsUranium-238High Energy Physics::ExperimentGamma spectroscopyAtomic physicsNuclear ExperimentBeam (structure)Radioactive decay
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New High-Precision Measurement of the Reaction Rate of the 18O(p, α)15N Reaction via THM

2008

The 18O(p,alpha)15N reaction rate has been extracted by means of the Trojan-Horse method. For the first time the contribution of the 20-keV peak has been directly evaluated, giving a value about 35% larger than previously estimated. The present approach has allowed to improve the accuracy of a factor 8.5, as it is based on the measured strength instead of educated guesses or spectroscopic measurements. The contribution of the 90-keV resonance has been determined as well, which turned out to be of negligible importance to astrophysics.

PhysicsNuclear reactionabundances[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]InstrumentationAnalytical chemistryResonanceFOS: Physical sciencesnucleosynthesisAstronomy and Astrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex][PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]01 natural sciences3. Good healthReaction rateAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciences010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)nuclear reactions
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Modulational Instability and Stimulated Raman Scattering in Normally Dispersive Highly Birefringent Fibers

2001

Abstract The nonlinear interaction of two laser beams in normally dispersive highly birefringent optical fibers leads to a large set of fascinating physical effects such as modulational instability (MI) and stimulated Raman scattering (SRS). These two nonlinear phenomena have a positive role as a mechanism for the generation of short optical pulses and represent a drawback in fiber-optics transmissions. Indeed, we will show that an induced process of modulational instability may be exploited for the generation of THz train of vector dark solitons. The technique of frequency-resolved optical gating is used to completely characterize the intensity and phase of the dark soliton trains. On the …

PhysicsOptical fiberBirefringencebusiness.industryOrthogonal polarization spectral imagingTerahertz radiationPhase (waves)Physics::OpticsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialslaw.inventionsymbols.namesakeModulational instabilityOpticsControl and Systems EngineeringlawsymbolsSolitonElectrical and Electronic EngineeringbusinessInstrumentationRaman scatteringOptical Fiber Technology
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Actively Q-switched and modelocked all-fiber lasers

2010

Here we demonstrate active mode-locking (ML) and doubly-active Q-switching mode-locking (QML) of erbium-doped strictly all-fiber lasers. The active ML mechanism relies in the acoustooptic superlattice modulation (AOSLM) effect induced when longitudinal acoustic waves are launched along a fiber Bragg grating. In both regimes - ML as well as QML - we focus on the laser behavior when the AOSLM is driven by traveling acoustic waves, and next we compare these results with those obtained when the AOSLM is driven by standing acoustic waves. In the ML regime, optical pulses were obtained of 530 mW peak power, 700 ps temporal width, at a repetition rate of 4.1 MHz. On the other hand, in the QML regi…

PhysicsOptical fiberPhysics and Astronomy (miscellaneous)business.industryBragg's lawAcoustic waveLaserQ-switchinglaw.inventionOpticsFiber Bragg gratingMode-lockinglawFiber laserbusinessInstrumentationLaser Physics Letters
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Interdisciplinary experiments with polarized 3He

1998

Abstract Optical pumping of metastable 3 He atoms is a very efficient method to produce large quantities of nuclear spin-polarized 3 He. Recent developments in mechanical compression of the gas, its storage and transport allow for its flexible use in different fields of physics and applied science. Among these are (1) scattering experiments of polarized beams from polarized 3 He-targets, (2) 3 He as neutron spin filter to polarize neutron beams at research reactors, and (3) polarized 3 He gas inhaled into the lungs to perform magnetic resonance imaging. The paper discusses the different topics along with results obtained in a first round of experiments.

PhysicsOptical pumpingNuclear and High Energy PhysicsNeutron magnetic momentSpin polarizationScatteringMetastabilityMechanical compressionNeutronNeutron scatteringAtomic physicsInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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APXS and MIMOS IIA: Planetary and terrestrial applications

2011

Both Alpha Particle X-ray Spectrometer (APXS) and the Miniaturized Moessbauer Spectrometer (MIMOS II) have shown their performances in space missions and terrestrial applications. Taking advantage of the challenges of space missions both instruments have become very powerful tools, even small in mass and dimensions.

PhysicsOpticsBackscatterSpectrometerbusiness.industryPhysics::Space PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAlpha particleComputer Science::Computational GeometrybusinessSpace exploration2011 IEEE Nuclear Science Symposium Conference Record
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Recent developments at the RITU focal plane

2003

Several technical developments have recently taken place at the RITU [1] focal plane detector system. Due to these developments the gas-filled recoil separator RITU is now, in the best case, up to an order of magnitude more sensitive than before.

PhysicsOpticsCardinal pointPhysics::Instrumentation and Detectorsbusiness.industryFocal plane detectorbusinessRecoil separator
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Sensitivity and Efficiency of the INTEGRAL Imager

1995

A detailed simulation program of the INTEGRAL Imager has been written and implemented using the GEANT-3 Monte Carlo code. The expected detection efficiency and continuum sensitivity have been evaluated. The results obtained for the CsI configuration of the Imager are compared with those obtained with the new configuration which foresees a top plane made of CdTe solid state detector elements.

PhysicsOpticsPhysics::Instrumentation and Detectorsbusiness.industryMonte carlo codePlane (geometry)Monte Carlo methodContinuum (design consultancy)Solid state detectorSensitivity (control systems)business
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An optimized time screening algorithm for ROSAT PSPC and HRI observations

1998

We have developed a model-independent time screening optimization algorithm to cope with significant contamination spikes in the ROSAT PSPC/HRI bacground light-curves. The rejection criteria are based on the maximization of faint sources signal-to-noise ratio. The algorithm tuning parameters have been optimized through performing a wide set of runs on both simulated and real data. We have verified that the application of our selection criteria to the case of long exposure PSPC observations yields an increase of the number of faint sources ( SNR ) of up to 100% with a rejection of up to the 8% of the exposure time. At the same time, we obtain an average signal-to-noise ratio gain of 3% for t…

PhysicsOptimization algorithmbusiness.industryAstrophysics::High Energy Astrophysical PhenomenaDetectorGeneral Physics and AstronomyAstrophysicsMaximizationScreening algorithmOn boardOpticsROSATInstrumentation (computer programming)businessAlgorithmSelection (genetic algorithm)
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Effect of Acoustic Wave Reflections on Space Charge Measurements with PEA Method

2018

The Pulsed Electro-Acoustic (PEA) method is the most used technique for space charge detection in solid dielectrics. The methodology is largely employed in the field of High Voltage Direct Current (HVDC) transmission and is based on the detection of acoustic waves generated by charges vibration. One of the most common problems arising during the detection is the presence of multiple reflections taking place due to the presence of means discontinuity in the different PEA cell components. This reflection phenomenon, if not well taken into account, could cause incorrect interpretation of the PEA output signal. It is easy to understand that a simulation model is a basic tool to understand the w…

PhysicsPEA methodRenewable Energy Sustainability and the EnvironmentNumerical analysisAcousticsPEA modelEnergy Engineering and Power TechnologyComputer Science Applications1707 Computer Vision and Pattern RecognitionAcoustic waveDielectricsimulationSpace chargeIndustrial and Manufacturing EngineeringVibrationSettore ING-IND/31 - ElettrotecnicaComputer Networks and CommunicationTransduceracosutic waveArtificial IntelligenceHigh-voltage direct currentMATLABInstrumentationcomputercomputer.programming_language2018 IEEE 4th International Forum on Research and Technology for Society and Industry (RTSI)
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