Search results for "doppler"

showing 10 items of 637 documents

Dependence of the shapes of nonzero-field level-crossing signals in rubidium atoms on the laser frequency and power density

2013

We studied magneto-optical resonances caused by excited-state level crossings in a nonzero magnetic field. Experimental measurements were performed on the transitions of the ${D}_{2}$ line of rubidium. These measured signals were described by a theoretical model that takes into account all neighboring hyperfine transitions, the mixing of magnetic sublevels in an external magnetic field, the coherence properties of the exciting laser radiation, and the Doppler effect. Good agreement between the experimental measurements and the theoretical model could be achieved over a wide range of laser power densities. We further showed that the contrasts of the level-crossing peaks can be sensitive to c…

Physicschemistry.chemical_elementLaserAtomic and Molecular Physics and OpticsMagnetic fieldlaw.inventionRubidiumsymbols.namesakechemistrylawsymbolsPhysics::Atomic PhysicsLaser power scalingAtomic physicsHyperfine structureDoppler effectCoherence (physics)Doppler broadeningPhysical Review A
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Measuring the spin up of the Accreting Millisecond Pulsar XTE J1751-305

2007

We perform a timing analysis on RXTE data of the accreting millisecond pulsar XTE J1751-305 observed during the April 2002 outburst. After having corrected for Doppler effects on the pulse phases due to the orbital motion of the source, we performed a timing analysis on the phase delays, which gives, for the first time for this source, an estimate of the average spin frequency derivative = (3.7 +/- 1.0)E-13 Hz/s. We discuss the torque resulting from the spin-up of the neutron star deriving a dynamical estimate of the mass accretion rate and comparing it with the one obtained from X-ray flux. Constraints on the distance to the source are discussed, leading to a lower limit of \sim 6.7 kpc.

Physicspulsars: general pulsars: individual: XTE J1751-305 stars: magnetic fields stars: neutron X-rays: binariesAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)Static timing analysisFluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicssymbols.namesakeNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarOrbital motionsymbolsDoppler effectSpin-½
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A relativistically broadened iron line from an Accreting Millisecond Pulsar

2010

The capabilities of XMM-Newton have been fully exploited to detect a broadened iron Kα emission line from the 2.5 ms Accreting Millisecond Pulsar, SAX J1808.4-3658. The energy of the transition is compatible with fluorescence from neutral/lowly ionized iron. The observed large width (FWHM more than 1 keV) can be explained through Doppler and relativistic broadening from the inner rings of an accretion disc close to the NS. From a fit of the line shape with a diskline model we obtain an estimate of the inner disc radius of 18.0-5.6+7.6km for a 1.4 M⊙ neutron star. The disc is therefore truncated inside the corotation radius (31 km for SAX J1808.4-3658), in agreement with the observation of c…

PhysicsrelativityAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsRadiusAstrophysicsstars: pulsars: individual: SAX J1808.4-3658accretion accretion diskprofiles; relativity; stars: pulsars: individual: SAX J1808.4-3658; X-rays: binaries; Physics and Astronomy (all) [accretion accretion disks; line]X-rays: binarieNeutron starPhysics and Astronomy (all)Pulsarline: profileMillisecond pulsarAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsEmission spectrumAstrophysics::Galaxy AstrophysicsLine (formation)Doppler broadening
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Timing of the Accreting Millisecond Pulsar XTE J1814-338

2006

We present a precise timing analysis of the accreting millisecond pulsar XTE J1814-338 during its 2003 outburst, observed by RXTE. A full orbital solution is given for the first time; Doppler effects induced by the motion of the source in the binary system were corrected, leading to a refined estimate of the orbital period, P_orb=15388.7229(2)s, and of the projected semimajor axis, a sini/c= 390.633(9) lt-ms. We could then investigate the spin behaviour of the accreting compact object during the outburst. We report here a refined value of the spin frequency (nu=314.35610879(1) Hz) and the first estimate of the spin frequency derivative of this source while accreting (nu^dot=(-6.7 +/- 0.7) 1…

Physicsstars: magnetic fields stars: neutron pulsars: general pulsars: individual: XTE J1814-338 X-rays: binariesAccretion (meteorology)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesMagnetosphereAstronomy and AstrophysicsContext (language use)AstrophysicsCompact starOrbital periodAstrophysicssymbols.namesakeSpace and Planetary ScienceMillisecond pulsarsymbolsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsDoppler effectSpin-½
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INSTABILITIES IN DOPPLER BROADENED OPTICALLY PUMPED FAR-INFRARED LASERS

1988

Recently Weiss and Brock observed Lorenz-type chaos in the 81.5μm emission from an optically-pumped 14NH3 laser1. The theoretical interpretation of the experimental results is an open question, however. In fact, the Lorenz-Haken model refers to incoherently pumped lasers with homogeneously-broadened two-level active media2. Models based on (at least) a three-level system are needed to describe optically-pumped lasers, whose dynamics is known to reduce to that of the Lorez-Haken model under certain limiting conditions3. But these conditions are not met in the 14NH3 laser, and indeed theoretical predictions of a model for this laser, which considered a homogeneously-broadened three-level acti…

Physicssymbols.namesakeOpticsFar infraredlawbusiness.industryGeneral EngineeringsymbolsLaserbusinessDoppler effectlaw.inventionLe Journal de Physique Colloques
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Lifetime Measurements of Low-lying States in $^{73}$Ga and $^{70,72,74}$Zn Isotopes

2019

International audience; Lifetimes of low-lying states in 73Ga and 70,72,74Zn were measured using the Recoil Distance Doppler Shift (RDDS) method. These nuclei were produced in deep-inelastic reactions in inverse kinematics with a 208Pb beam impinging on a 76Ge target. Prompt γ rays were detected using the AGATA tracking array coupled to the VAMOS++ spectrometer. Lifetime of the 5/2 − state in 73Ga, measured for the first time, provides additional evidence for the existence of a 1/2 −, 3/2 − ground-state doublet. The lifetimes of the 4 + states in 70,72,74Zn were remeasured in an attempt to understand the discrepancies observed between earlier measurements. Our results are in agreement with …

Physicssymbols.namesakeRecoilIsotopeSpectrometersymbolsGeneral Physics and AstronomyAGATAAtomic physics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Tracking (particle physics)Doppler effectBeam (structure)
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Lifetime Measurements with the Doppler Shift Attenuation Method Using a Thick Homogeneous Production Target — Verification of the Method

2016

International audience; Doppler Shift Attenuation Method (DSAM) analysis of excited-state lifetimes normally employs thin production targets mounted on a thick stopper foil (“backing”) serving to slow down and stop the recoiling nuclei of interest in a well-defined manner. Use of a thick, homogeneous production target leads to a more complex analysis as it results in a substantial decrease in the energy of the incident projectile which traverses the target with an associated change in the production cross section of the residues as a function of penetration depth. Here, a DSAM lifetime analysis using a thick homogeneous target has been verified using the Doppler broadened lineshapes of γ ra…

Physicsta114Doppler Shift Attenuation Method010308 nuclear & particles physicsbusiness.industryAttenuationlifetime measurementGeneral Physics and Astronomy[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencessymbols.namesakeOpticsHomogeneous0103 physical sciencessymbols010306 general physicsbusinessDoppler effectFOIL method
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Exploring Training Options for RF Sensing Using CSI

2018

This work analyzes human behavior recognition approaches using WiFi channel state information from the perhaps less usual point of view of training and calibration needs. With the help of selected literature examples, as well as with more detailed experimental insights on our own Doppler spectrum-based approach for physical motion/presence/cardinality detection, we first classify the diverse forms of training so far employed into three main categories (trained, trained-once, and training-free). We further discuss under which conditions it is possible to move toward lighter forms of calibration or even succeed in devising fully untrained model-based solutions. Our take home messages are main…

Point (typography)Settore ING-INF/03 - TelecomunicazioniComputer Networks and CommunicationsCalibration (statistics)Computer sciencebusiness.industry010401 analytical chemistryBehavioural sciences020206 networking & telecommunications02 engineering and technologyMachine learningcomputer.software_genreTraining Wireless fidelity Calibration Doppler effect Behavioral sciences Radio frequency Sensors Channel state estimation01 natural sciencesTraining (civil)Motion (physics)0104 chemical sciencesComputer Science ApplicationsPersonalization0202 electrical engineering electronic engineering information engineeringArtificial intelligenceElectrical and Electronic EngineeringbusinesscomputerIEEE Communications Magazine
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Exceeding the resolving imaging power using environmental conditions

2007

We present two approaches that use the environmental conditions in order to exceed the classical Abbe's limit of resolution of an aperture-limited imaging system. At first we use water drops in order to improve the resolving capabilities of an imaging system using a time-multiplexing approach. The limit for the resolution improvement capabilities is equal to the size of the rain drops. The rain drops falling close to the imaged object act as a sparse and random high-resolution mask attached to it. By applying proper image processing, the center of each falling drop is located, and the parameters of the encoding grating are extracted from the captured set of images. The decoding is done digi…

Point spread functionSynthetic aperture radarComputer sciencebusiness.industryImage qualityMaterials Science (miscellaneous)Image processingGratingSuperresolutionIndustrial and Manufacturing Engineeringsymbols.namesakeOptical imagingOpticssymbolsBusiness and International ManagementbusinessDoppler effectApplied Optics
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Characterization of non-polar ZnO layers with positron annihilation spectroscopy

2008

We applied positron annihilation spectroscopy to study the effect of growth polarity on the vacancy defects in ZnO grown by metal-organic vapor phase deposition on sapphire. Both c-plane and a-plane ZnO layers were measured, and Zn vacancies were identified as the dominant defects detected by positrons. The results are qualitatively similar to those of earlier experiments in GaN. The Zn vacancy concentration decreases in c-plane ZnO by almost one order of magnitude (from high 10 cm−3 to low 10 cm−3) when the layer thickness is increased from 0.5 to 2 μm. Interestingly, in a-plane ZnO the Zn vacancy concentration is constant at a level of about 2×10 cm−3 in all the samples with thicknesses v…

PositronMaterials scienceVacancy defectAnnihilation radiationSapphireAnalytical chemistryGeneral Physics and AstronomyAnisotropyDeposition (law)Positron annihilation spectroscopyDoppler broadening
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