Search results for "Synchro"

showing 10 items of 886 documents

Hydrodynamic synchronization of pairs of puller type magnetotactic bacteria in a high frequency rotating magnetic field.

2019

Ensembles of magnetotactic bacteria are known to interact hydrodynamically and form swarms under the influence of external magnetic fields. We describe the synchronization of puller type magnetotactic bacteria in a rotating magnetic field by representing the bacteria as hydrodynamic force dipoles. Numerical simulations show that at moderate values of the hydrodynamic interaction parameter large ensembles of asynchronously rotating bacteria randomly eject propagating doublets of synchronized bacteria. We quantitatively analyze the dynamics of the doublets and show that an important role in the formation of these propagating structures is played by the parameters characterizing the possible t…

PhysicsPhysics::Biological PhysicsRotating magnetic fieldMagnetotactic bacteriaDynamics (mechanics)02 engineering and technologyGeneral ChemistryType (model theory)010402 general chemistry021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesQuantitative Biology::Cell Behavior0104 chemical sciencesMagnetic fieldQuantitative Biology::Subcellular ProcessesSynchronization (alternating current)DipoleChemical physics0210 nano-technologySoft matter
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New results from testing of coplanar-grid CdZnTe detectors

2005

New results from studies of coplanar-grid CdZnTe (CZT) detectors are presented. The coplanar-grid detectors were investigated by using a highly collimated X-ray beam available at Brookhaven's National Synchrotron Light Source and by applying a pulse-shape analysis. The coplanar-grid detector operates as a single-carrier device. Despite the fact that its operational principle is well known and has been investigated by many groups in the past, we found some new details that may explain the performance limits of these types of devices. The experimental results have been confirmed by extensive computer modeling.

PhysicsPhysics::Instrumentation and Detectorsbusiness.industryDetectorSynchrotron radiationParticle acceleratorGridCollimated lightParticle detectorlaw.inventionNational Synchrotron Light SourceOpticslawbusinessBeam (structure)Hard X-Ray and Gamma-Ray Detector Physics VII
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2021

Several techniques are under development for image-guidance in particle therapy. Positron (β+) emission tomography (PET) is in use since many years, because accelerated ions generate positron-emitting isotopes by nuclear fragmentation in the human body. In heavy ion therapy, a major part of the PET signals is produced by β+-emitters generated via projectile fragmentation. A much higher intensity for the PET signal can be obtained using β+-radioactive beams directly for treatment. This idea has always been hampered by the low intensity of the secondary beams, produced by fragmentation of the primary, stable beams. With the intensity upgrade of the SIS-18 synchrotron and the isotopic separati…

PhysicsRadioactive ion beamsCancer ResearchParticle therapyProtonIsotopemedicine.medical_treatmentSynchrotron030218 nuclear medicine & medical imaginglaw.inventionIonNuclear physics03 medical and health sciences0302 clinical medicinePositronOncologyFragmentation (mass spectrometry)law030220 oncology & carcinogenesismedicineFrontiers in Oncology
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CERN's longest serving experimental facility

2004

The On-Line Isotope Separator ISOLDE has operated continuously at CERN since 1967. Today ISOLDE and its Post accelerator REX-ISOLDE, dedicated to the production of a large variety of radioactive ion beams with energies from 1 keV/u up to 3.1 MeV/u, are used for a great number of different experiments in the fields of nuclear and atomic physics, nuclear astrophysics, material physics and life sciences. The facility, originally located at the CERNs first accelerator Synchrocyclotron (SC), has been located at the Proton-Synchrotron Booster (PSB) since 1992. Long and outstanding operation of ISOLDE has had important impact on the evolution of nuclear physics and its applications. ISOLDE has bee…

PhysicsRadioactive ion beamsNuclear physicsLarge Hadron ColliderSynchrocyclotronEarly startNuclear astrophysicsGeneral Physics and AstronomyMaterial physicsPhysics Reports
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An RMHD study of transition between prompt and afterglow GRB phases

2008

We study the afterglow phases of a GRB through relativistic magnetohydrodynamic simulations. The evolution of a relativistic shell propagating into a homogeneous external medium is followed. We focus on the effect of the magnetization of the ejecta on the initial phases of the ejecta-external medium interaction. In particular we are studying the condition for the existence of a reverse shock into the ejecta, the timescale for the transfer of the energy from the shell to the shocked medium and the resulting multiwavelength light curves. To this end, we have developed a novel scheme to include non-thermal processeses which is coupled to the relativistic magnetohydrodynamic code MRGENESIS in o…

PhysicsShock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Shell (structure)Synchrotron radiationFOS: Physical sciencesAstrophysicsLight curveAstrophysicsAfterglowMagnetohydrodynamic driveGamma-ray burstEjectaAstrophysics::Galaxy Astrophysics
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A method for computing synchrotron and inverse-Compton emission from hydrodynamic simulations of supernova remnants

2015

Abstract The observational signature of supernova remnants (SNRs) is very complex, in terms of both their geometrical shape and their spectral properties, dominated by non-thermal synchrotron and inverse-Compton scattering. We propose a post-processing method to analyse the broad-band emission of SNRs based on three-dimensional hydrodynamical simulations. From the hydrodynamical data, we estimate the distribution of non-thermal electrons accelerated at the shock wave and follow the subsequent evolution as they lose or gain energy by adiabatic expansion or compression and emit energy by radiation. As a first test case, we use a simulation of a bipolar supernova expanding into a cloudy medium…

PhysicsShock waveNuclear and High Energy PhysicsRadiationScatteringAstrophysics::High Energy Astrophysical PhenomenaInverseAstrophysicsElectronRadiation01 natural sciencesSynchrotronlaw.inventionSupernovalaw0103 physical sciences010306 general physicsAdiabatic process010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Density Physics
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Analysis of Torque Developed in Axial Flux, Single-Phase Brushless DC Motor With Salient-Pole Stator

2004

An analysis of the torque developed by a single-phase disc brushless permanent magnet motor with salient-pole stator is presented. The machine represents a new family of brushless disc motors with the starting torque issue appearing to be most challenging. To produce a starting torque, the permanent magnets on one of the rotor discs are distributed nonuniformly. However, this significantly distorts a shape of the cogging torque versus rotational angle characteristic which, in turn, affects a waveform of the overall torque. A three-dimensional (3-D) finite-element model is used for the purpose of determining of angular variations of the torque developed by the motor. To find how the torque v…

PhysicsStall torqueTorque motorCogging torqueEnergy Engineering and Power TechnologyControl engineeringQuantitative Biology::Subcellular ProcessesTorque limiterDirect torque controlControl theoryTorque sensorAstrophysics::Earth and Planetary AstrophysicsElectrical and Electronic EngineeringDamping torqueSynchronous motorIEEE Transactions on Energy Conversion
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Star network synchronization led by strong coupling-induced frequency squeezing

2017

We consider a star network consisting of N oscillators coupled to a central one which in turn is coupled to an infinite set of oscillators (reservoir), which makes it leaking. Two of the N + 1 normal modes are dissipating, while the remaining N - 1 lie in a frequency range which is more and more squeezed as the coupling strengths increase, which realizes synchronization of the single parts of the system.

PhysicsStar networkInfinite setRange (particle radiation)Quantum PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciFOS: Physical sciencesdissipationDissipationCondensed Matter Physics01 natural sciencesSettore FIS/03 - Fisica Della MateriaAtomic and Molecular Physics and Optics010305 fluids & plasmasSynchronization (alternating current)Coupling (physics)Normal modeQuantum mechanics0103 physical sciencesTurn (geometry)star network010306 general physicsQuantum Physics (quant-ph)synchronizationMathematical Physics
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Design and Performance of a High Temperature Superconducting Axial Flux Generator

2013

In this paper, a high temperature axial flux (HTSAF) generator is presented. In this generator the excitation of the generator is obtained by using some high temperature superconducting magnets. In order to reduce the negative effects of vibrations, the excitation is located on the stationary part of the generator. Starting, running and endurance tests of the machine are presented.

PhysicsSuperconductivityGenerator (computer programming)Superconducting electric machineMechanicsSuperconducting magnetPermanent magnet synchronous generatorSuperconducting magnetic energy storageTerms—Superconducting materials magnetic materials electric machines power systemsElectronic Optical and Magnetic Materialslaw.inventionNuclear magnetic resonancelawMagnetElectrical and Electronic EngineeringExcitationIEEE Transactions on Magnetics
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Multi-Wavelength VLA Observations of the Young Supernova SN 1993J

2003

We present continuum VLA measurements of SN1993J in M81 taken on 17 and 21 December 2000, about 2820 days after the supernova explosion, spanning the frequency range from 0.32 to 14.9 GHz. These observations aimed at discerning the main absorbing processes acting in SN1993J at late epochs. We discuss three models for the late radio emission of SN1993J: (i) a simple power-law spectrum, (ii) a power-law spectrum free-free absorbed by a screen of homogeneously distributed ionized gas, and (iii) a power-law spectrum free-free absorbed by a “clumpy” medium. We find that the best fit to the data is yielded by a power-law spectrum free-free absorbed by either a homogeneous, or a clumpy, distributi…

PhysicsSupernovaSpectral indexlawIonizationRadiative transferAstronomyPlasmaAstrophysicsElectronSynchrotronRadio spectrumlaw.invention
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