Search results for "interferometry"

showing 10 items of 343 documents

First hints of pressure waves in a helical extragalactic jet: S5~0836+710

2014

One of the open questions in extragalactic jet Astrophysics is related to the nature of the observed radio jet, namely whether it traces a pattern or the flow structure itself. In this paper I summarize the evidence collected for the presence of waves in extragalactic jets. The evidence points towards the peak of emission in helical jets corresponding to pressure-maxima of a wave that is generated within the core region and propagates downstream. Making use of a number of very long baseline interferometry (VLBI) observations of the radio jet in the quasar S5~0836+710 at different frequencies and epochs, Perucho et al. (2012) were able to observe wave-like behavior within the observed radio-…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsHelicityCore (optical fiber)Physical structureFlow (mathematics)lcsh:TA1-2040Very-long-baseline interferometryGeneral Earth and Planetary Scienceslcsh:Engineering (General). Civil engineering (General)Astrophysics - High Energy Astrophysical PhenomenaGeneral Environmental ScienceAstrophysics - Cosmology and Nongalactic Astrophysics
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Apparent superluminal core expansion and limb brightening in the candidate neutrino blazar TXS 0506+056

2019

IceCube has reported a very-high-energy neutrino (IceCube-170922A) in a region containing the blazar TXS 0506+056. Correlated {\gamma}-ray activity has led to the first high-probability association of a high-energy neutrino with an extragalactic source. This blazar has been found to be in a radio outburst during the neutrino event. We have performed target-of-opportunity VLBI imaging observations at 43 GHz frequency with the VLBA two and eight months, respectively, after the neutrino event. We produced two images of TXS 0506+056 with angular resolutions of (0.2x1.1) mas and (0.2x0.5) mas, respectively. The source shows a compact, high brightness temperature core (albeit not approaching the …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Superluminal motion010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Astrophysics of GalaxiesGalaxyNeutrino detectorSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesVery-long-baseline interferometryNeutrinoBlazarAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsVery Long Baseline Array
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Two-particle correlations in pp, (p)over-bar(p)over-bar and (KSKS0)-K-0 pairs from hadronic Z decays

2005

Two-particle correlations in pp, and pairs have been studied in hadronic Z decays recorded at LEP with the ALEPH detector. The correlations were measured as a function of the four-momentum difference Q of the pair. For pp, pairs a depletion of events is observed in the region , and for pairs an enhancement of events is observed in the region . These features are consistent with expectations from Fermi–Dirac and Bose–Einstein statistics, respectively.

INTERFERENCEINTERFEROMETRYZ(0) DECAYSBOSE-EINSTEIN CORRELATIONSLEPANNIHILATIONALEPHDETECTORMESONSMULTIPLE PRODUCTION
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Bose-Einstein correlations in W-pair decays with an event-mixing technique

2005

Bose-Einstein correlations in W-pair decays are studied using data collected by the ALEPH detector at LEP at e+e- centre-of-mass energies from 183 to 209 GeV. The analysis is based on the comparison of WW→qq̄qq̄ events to "mixed" events constructed with the hadronic part of WW→qq̄ℓν events. The data are in agreement with the hypothesis that Bose-Einstein correlations are present only for pions from the same W decay. The JETSET model with Bose-Einstein correlations between pions from different W bosons is disfavoured.

INTERFEROMETRYPHYSICSCOLLISIONSE+E-ANNIHILATIONSE(+)E(-)2-DIMENSIONAL ANALYSISHADRONSLEPZ(0)PEAK
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Analysis of an interferometric optical fibre detection technique applied to silicon vibrating sensors

1987

A simple and accurate analysis of a single-mode optical fibre interferometric displacement detection technique is resented. This analysis is in good agreement with experimental measurements, and shows that angular alignment between the fibre and the sensor is the most critical parameter.

ImaginationMaterials scienceOptical fiberSiliconbusiness.industrymedia_common.quotation_subjectchemistry.chemical_elementÒpticaVibracióDisplacement (vector)law.inventionVibrationInterferometryOpticsCritical parameterchemistrylawVibration measurementElectrical and Electronic Engineeringbusinessmedia_common
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Spectral evolution simulation on leading multi-socket, multicore platforms

2011

Spectral evolution simulations based on the observed Very Long Baseline Interferometry (VLBI) radio-maps are of paramount importance to understand the nature of extragalactic objects in astrophysics. This work analyzes the performance and scaling of a spectral evolution algorithm on three leading multi-socket, multi-core architectures. We evaluate three parallel models with different levels of data-sharing: a sharing approach, a privatizing approach and a hybrid approach. Our experiments show that the data-privatizing model is reasonably efficient on medium scale multi-socket, multi-core systems (up to 48 cores) while regardless algorithmic and scheduling optimizations, sharing approach is …

Instruction setMulti-core processorSpectral evolutionComputer scienceDistributed computingScalabilityVery-long-baseline interferometryScalingScheduling (computing)2011 18th International Conference on High Performance Computing
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Measurements of anterior chamber depth, white-to-white distance, anterior chamber angle, and pupil diameter using two Scheimpflug imaging devices.

2014

Purpose: To compare the ocular anterior chamber depth, white-to-white distance, anterior chamber angle, and pupil diameter, as measured with two different Scheimpflug imaging devices. Methods: This transversal study included 80 right eyes from 80 subjects aged from 20 to 40 years. Their spherical equivalents ranged from -4.25 to +1.00 diopters (D). Each eye's anterior chamber depth, white-to-white distance, anterior chamber angle, and pupil diameter, were measured for far vision using both the Galilei G4 (double Scheimpflug camera) and the Pentacam HR (single Scheimpflug camera) systems. Results: Mean anterior chamber depths were calculated as 3.12 ± 0.23 mm and 3.19 ± 0.24 mm when measured…

InterferometriaAdultAnterior ChamberScheimpflug principlePhotography/methodsPupil diameterIrisPupila/fisiologiaDiagnostic Techniques OphthalmologicalAnterior chamber anglePupilYoung AdultOpticsAnterior chamber/pathologyImaging Three-Dimensionallcsh:OphthalmologymedicineDiagnostic techniques ophthalmologicalPhotographyHumansPentacam hrDioptrePhysicsWhite to whitemedicine.diagnostic_testbusiness.industryPupilGeneral MedicineTécnicas de diagnóstico oftalmológicoCorneal topographyeye diseasesOphthalmologyInterferometryCâmara anterior/patologialcsh:RE1-994Fotografia/métodosTopografia da córneasense organsCorneal topographyPupil/physiologybusinessNuclear medicineArquivos brasileiros de oftalmologia
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Medida da profundidade da câmara anterior, distância branco a branco, ângulo da câmara anterior e diâmetro pupilar usando dois dispositivos de imagen…

2014

Purpose: To compare the ocular anterior chamber depth, white-to-white distance, anterior chamber angle, and pupil diameter, as measured with two different Scheimpflug imaging devices. Methods: This transversal study included 80 right eyes from 80 subjects aged from 20 to 40 years. Their spherical equivalents ranged from -4.25 to +1.00 diopters (D). Each eye's anterior chamber depth, white-to-white distance, anterior chamber angle, and pupil diameter, were measured for far vision using both the Galilei G4 (double Scheimpflug camera) and the Pentacam HR (single Scheimpflug camera) systems. Results: Mean anterior chamber depths were calculated as 3.12 ± 0.23 mm and 3.19 ± 0.24 mm when measured…

InterferometriaAnterior chamber/pathologyInterferometryCâmara anterior/patologiaPhotography/methodsFotografia/métodosDiagnostic techniques ophthalmologicalTopografia da córneaCorneal topographyPupil/physiologyPupila/fisiologiaTécnicas de diagnóstico oftalmológico
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Current modulation induced stability in laser diode under high optical feedback strength

2021

The back-reflection of emitted laser beam (optical feedback, also know as selfmixing) from various external interfaces are sufficient to cause instability, and prohibiting its use in various fields such as communication, spectroscopy, imaging to name a few. So it is desirable to study the laser dynamics and the conditions causing it to be stable in spite of strong optical feedback. With the aid of mathematical formulation, simulation and backed by experimental evidences, it is demonstrated that the frequency deviation of the laser emission due to current (intensity) modulation alters the dynamic state and boundary conditions of the system such that even under large optical feedback strength…

InterferometriaMaterials scienceGeneral Computer ScienceIntensity modulationPhysics::Optics02 engineering and technology01 natural scienceslaw.inventionSemiconductor laser theory010309 optics020210 optoelectronics & photonicsOpticslaw0103 physical sciences0202 electrical engineering electronic engineering information engineeringGeneral Materials ScienceOptical feedbackLaser diodebusiness.industryGeneral EngineeringFrequency deviationLaserSpectrum analysisAnàlisi espectralself-mixing interferometryVDP::Teknologi: 500InterferometrySelf-mixing interferometryModulation:Ciències de la visió [Àrees temàtiques de la UPC]frequency coefficientlcsh:Electrical engineering. Electronics. Nuclear engineeringFrequency coefficientbusinessSelf-mixing interferometryIntensity modulationFrequency modulationlcsh:TK1-9971intensity modulation
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Variability and polarization in the inner jet of 3C 395

2001

We present new results on the parsec-scale jet of the quasar 3C395, derived from VLBI polarization sensitive observations made in 1995.91 and 1998.50 at 8.4, 15.4 and 22.2 GHz. The observations show a complex one-sided jet extending up to 20 mas, with a projected magnetic field essentially aligned with the radio jet. The emission is strongly dominated, in total intensity and polarization, by the core and the inner jet region (of ~3 mas length). We have studied the details of this dominant region finding clear structural variations during this ~2.5 years period, in contrast with the apparent quietness of the jet structure inferred from lower resolution VLBI observations. We observe the eject…

InterferometricAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAsymbols.namesakeFaraday effectVery-long-baseline interferometryJetsPhysicsIndividual galaxiesAstrophysics (astro-ph)Active Galaxies ; Individual galaxies ; 3C 395 ; Jets ; Radio continuum ; InterferometricAstronomy and AstrophysicsQuasarPolarization (waves):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Magnetic fieldRadio continuumPolarization sensitiveSpace and Planetary Science3C 395symbolsDegree of polarizationUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaActive Galaxies:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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