Search results for "SCAD"

showing 10 items of 348 documents

Universal spectral dynamics of modulation instability : theory, simulation, experiment

2011

A central process of nonlinear fibre optics is modulation instability (MI), where weak perturbations on a continuous wave are amplified to generate a parametric cascade of spectral sidebands. Although studied for many years, it has only been recently appreciated that MI dynamics can be described analytically by Akhmediev breather (AB) solutions to the nonlinear Schrodinger equation (NLSE) [1]. This has led to important results, including the first observation of the Peregrine Soliton [2]. AB theory has also shown that the spectral amplitudes at the peak of the MI gain curve yield a characteristic log-triangular spectrum, providing new insight into the initial phase of supercontinuum generat…

Physics[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Breather01 natural sciencesInstabilitySupercontinuumSchrödinger equation010309 opticssymbols.namesakeCascadeQuantum mechanics0103 physical sciencesModulation (music)symbolsPeregrine solitonStatistical physics010306 general physicsNonlinear Schrödinger equation
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Atomic Coherence Effects in Doppler-Broadened Three-Level Systems with Standing-Wave Drive

2001

We study atomic coherence effects (e.g., electromagnetically induced transparency, EIT, and amplification without inversion, AWI) for a probe travelling-wave (TW) laser field in closed Doppler-broadened three-level systems driven by a standingwave (SW) laser field of moderate intensity (its Rabi frequencies are smaller than the Doppler width of the driven transition). We show that probe windows of transparency occur only for values of the probe to drive field frequency ratio R close to half integer values. For optical transitions and typical values of Doppler broadening for atoms in a vapor cell, we show that for R > 1 a SW drive field is appreciably more efficient than a TW drive in induci…

Physicsbusiness.industryElectromagnetically induced transparencyLaserAtomic coherencelaw.inventionStanding wavesymbols.namesakeOpticsCascadelawsymbolsHalf-integerPhysics::Atomic PhysicsAtomic physicsbusinessDoppler effectDoppler broadening
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Cascade coherence transfer and magneto-optical resonances at 455 nm excitation of Cesium

2010

We present and experimental and theoretical study of nonlinear magneto-optical resonances observed in the fluorescence to the ground state from the 7P_{3/2} state of cesium, which was populated directly by laser radiation at 455 nm, and from the 6P_{1/2} and 6P_{3/2} states, which were populated via cascade transitions that started from the 7P_{3/2} state and passed through various intermediate states. The laser-induced fluorescence (LIF) was observed as the magnetic field was scanned through zero. Signals were recorded for the two orthogonal, linearly polarized components of the LIF. We compared the measured signals with the results of calculations from a model that was based on the optica…

Physicsbusiness.industryLinear polarizationAtomic Physics (physics.atom-ph)FOS: Physical sciencesLaserAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsMagnetic fieldlaw.inventionPhysics - Atomic Physicssymbols.namesakeOpticsCascadelawsymbolsPhysics::Atomic PhysicsElectrical and Electronic EngineeringPhysical and Theoretical ChemistryAtomic physicsbusinessGround stateDoppler effectExcitationCoherence (physics)
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Type-II intermittency in a cascade laser model

2005

PhysicslawCascadeIntermittencyAtomic physicsLaserlaw.invention
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Master equation for cascade quantum channels: a collisional approach

2012

It has been recently shown that collisional models can be used to derive a general form for the master equations which describe the reduced time evolution of a composite multipartite quantum system, whose components "propagate" in an environmental medium which induces correlations among them via a cascade mechanism. Here we analyze the fundamental assumptions of this approach showing how some of them can be lifted when passing into a proper interaction picture representation.

Physicsopen quantum systems quantum correlation collision modelQuantum PhysicsOpen quantum systems dynamicTime evolutionQuantum channelsFOS: Physical sciencesCondensed Matter PhysicsAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della MateriaMultipartiteClassical mechanicsCascadeInteraction pictureMaster equationQuantum systemQuantum InformationRepresentation (mathematics)Quantum Physics (quant-ph)Quantum
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The exposure of the hybrid detector of the Pierre Auger Observatory

2010

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ‘‘hybrid” detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data coll…

Physics::Instrumentation and DetectorsAstronomy01 natural sciencesCoincidenceAugerFluorescence detectorData acquisitionAuger experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsFÍSICA DE PARTÍCULASSettore INF/01 - InformaticaCascada atmosférica extensaPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger Observatoryultra high energy cosmic rays; Pierre Auger Observatory; extensive air showers; trigger; exposure; fluorescence detector; hybridENERGY-SPECTRUMRadiación cósmicaSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaFísica nuclearAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaExtensive air showerMeasure (physics)FOS: Physical sciencesCosmic rayCosmic RayFluorescence spectroscopyUltra high energy cosmic rayExposureNuclear physicsOpticsSHOWERS0103 physical sciencesExtensive air showers010306 general physicsCiencias ExactasPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaAstronomy and AstrophysicsUltra high energy cosmic raysHybrid[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]fluxTriggerExperimental High Energy PhysicsbusinessSYSTEMAstroparticle Physics
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Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

2018

With the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60 and 84. In contrast to air showers with more vertical incidence, these inclined air showers illuminate large ground areas of several km2 with radio signals detectable in the 30 to 80 MHz band. A comparison of the measured radio-signal amplitudes with Monte Carlo simulations of a subset of 50 events for which we reconstruct the energy using the Auger surface detector shows agreement within the uncertainties of the current analysis. As expected for forward-beamed radio emission undergoing no significant absorption or sc…

Physics::Instrumentation and DetectorsAstronomyengineering01 natural sciencesultra high energy cosmic rayAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)cosmic ray experiments; cosmic rays detectors; ultra high energy cosmic rays; Astronomy and Astrophysics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Cosmic ray experiments cosmic rays detectors ultra high energy cosmic rays Astronomy and Astrophysics.Absorption (electromagnetic radiation)Physicsradio waveSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETORESCOSMIC-RAYSAugerobservatoryAmplitudecosmic rays detectorsAstrophysics - Instrumentation and Methods for Astrophysicsnumerical calculations: Monte CarloairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentultra high energy cosmic rayscascade: electromagneticOptics0103 physical sciencesHigh Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]cosmic rays detector010306 general physicscosmic ray experiments cosmic rays detectors ultra high energy cosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithAstrophysiquePierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryScatteringhep-exdetector: surfacescatteringAstronomy and AstrophysicsAstronomieAir showerExperimental High Energy PhysicsARRAYHigh Energy Physics::Experimentcosmic ray experimentscosmic ray experiments; cosmic rays detectors; ultra high energy cosmic raysEMISSIONbusinessabsorptionastro-ph.IM
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

2020

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers.

Physics::Instrumentation and DetectorsAstronomyprimary [cosmic radiation]01 natural sciences030218 nuclear medicine & medical imagingAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinesurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Data Processing; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of High Energy Physics DetectorsInstrumentationMathematical PhysicsData Processing; Large detector systems for particle and astroparticle physics; Largedetector-systems performance; Performance of High Energy Physics DetectorsLarge detector-systems performanceHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEInstrumentation et méthodes en physiqueData ProcessingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugercascadeobservatoryCascadeLargedetector-systems performanceddc:620Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airAstrophysics::High Energy Astrophysical PhenomenawaterFOS: Physical sciencesCosmic rayAtmosphere03 medical and health sciencesOptics0103 physical sciencesHigh Energy Physics14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithEngineering & allied operationsPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryhep-exdetector: surfaceLarge detector systems for particle and astroparticle physicsAutres mathématiquescosmic radiation: primaryCherenkov counterExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentPerformance of High Energy Physics Detectorsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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Innovative Computational Approach to Harmonic Mitigation for Seven-level Cascaded H-Bridge Inverters

2020

Low frequency modulation strategies are a good solution to increase the energy conversion efficiency in high power applications. The paper is devoted to presents an innovative way to low order harmonics mitigation for seven-level Cascaded H-Bridge Inverters. In particular, this approach is based on the mitigation of selected harmonics without solve non-linear equations for an extended range of the fundamental amplitude. In fact, in real-Time operation to evaluate the control angles the polynomial equations have been identified. Through circuit simulation analysis in MatLab/PLECS environment, the effectiveness of the harmonic mitigation method has been tested and compared with theoretical re…

PolynomialComputer science020209 energy020208 electrical & electronic engineeringEnergy conversion efficiencyElectrical Drive02 engineering and technologySettore ING-IND/32 - Convertitori Macchine E Azionamenti ElettriciH bridgePower (physics)Settore ING-IND/31 - ElettrotecnicaAmplitudeHarmonics0202 electrical engineering electronic engineering information engineeringElectronic engineeringRange (statistics)Selective Harmonic MitigationMATLABCascaded H-Bridge InverterscomputerSoft Switching Modulation Techniquescomputer.programming_language2020 Fifteenth International Conference on Ecological Vehicles and Renewable Energies (EVER)
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Novel Computational Method for Harmonic Mitigation for Three-phase Five-level Cascaded H-Bridge Inverter

2018

The efficiency of the system is a very important parameter for high power electrical drives applications,. Moreover, in the system the efficiency of the power converter play a fundamental role and for this reason, the soft switching modulation techniques represent the best choice. This paper presents a novel computational method for harmonic mitigation on the output voltage of a five-level, three-phase Cascaded H-Bridge Inverter without solving non-linear equations. Through this simple approach the Working Areas have been identified in which the harmonics reference have minimum amplitude possible. Moreover, polynomial equations to evaluate the control angels have been found. In this way, th…

PolynomialComputer scienceEnergy Engineering and Power TechnologyCascaded H-Bridge multilevel inverterPower (physics)Harmonic analysisselective harmonic mitigationNonlinear systemComputer Networks and CommunicationThree-phaseArtificial IntelligenceControl theoryHarmonicsInverterhigh power applicationSafety Risk Reliability and QualityMATLABcomputercomputer.programming_language
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