Search results for " Magnetic field"

showing 10 items of 165 documents

Dynamics of a flexible ferromagnetic filament in a rotating magnetic field.

2017

Flexible magnetic filaments have garnered considerable attention as prospective materials for the creation of different microdevices. We describe a theoretical model of a ferromagnetic filament and derive its equations of motion by variational techniques. The numerical algorithm used to solve the filament dynamics in magnetic fields of different configurations is described. It is found that in a rotating field the filament transitions between synchronous and asynchronous regimes with respect to the rotating field, similarly to a rigid magnetic dipole. The mean angular velocity of the filament is well described by a relation valid for a rigid magnetic dipole with quantitative differences att…

PhysicsRotating magnetic fieldCondensed matter physicsField (physics)Equations of motionAngular velocity02 engineering and technology021001 nanoscience & nanotechnology01 natural sciences010305 fluids & plasmasMagnetic fieldQuantitative Biology::Subcellular ProcessesProtein filamentFerromagnetism0103 physical sciences0210 nano-technologyMagnetic dipolePhysical review. E
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3D motion of flexible ferromagnetic filaments under a rotating magnetic field.

2020

Ferromagnetic filaments in a rotating magnetic field are studied both numerically and experimentally. The filaments are made from micron-sized ferromagnetic particles linked with DNA strands. It is found that at low frequencies of the rotating field a filament rotates synchronously with the field and beyond a critical frequency it undergoes a transition to a three dimensional regime. In this regime the tips of the filament rotate synchronously with the field on circular trajectories in the plane parallel to the plane of the rotating field. The characteristics of this motion found numerically match the experimental data and allow us to obtain the physical properties of such filaments. We als…

PhysicsRotating magnetic fieldCondensed matter physicsField (physics)Plane (geometry)FOS: Physical sciences02 engineering and technologyGeneral ChemistryCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesRodQuantitative Biology::Cell BehaviorProtein filamentQuantitative Biology::Subcellular ProcessesFerromagnetismCritical frequency0103 physical sciencesSoft Condensed Matter (cond-mat.soft)010306 general physics0210 nano-technologyMixing (physics)Soft matter
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Bending of ferrofluid droplet in rotating magnetic field

1999

Abstract This paper presents results concerning 2D ferrofluid droplet motion at high values of magnetic field and frequencies above a critical one with respect to droplet ability to follow field rotation. The boundary element method is used to solve 2D equations of a magnetic field and Stokes flow problems. If the viscosity of the ferrofluid is larger than that of the surrounding fluid, droplet exhibits bending, forming “S-shape”. Fluid flow inside the droplet is analyzed and the main stages of periodical rotation of a droplet are reported.

PhysicsRotating magnetic fieldFerrofluidField (physics)MechanicsStokes flowCondensed Matter PhysicsRotationElectronic Optical and Magnetic MaterialsMagnetic fieldPhysics::Fluid DynamicsViscosityClassical mechanicsPhysics::Atomic and Molecular ClustersFluid dynamicsJournal of Magnetism and Magnetic Materials
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Three-dimensional dynamics of a particle with a finite energy of magnetic anisotropy in a rotating magnetic field.

2013

A model of a single ferromagnetic particle with a finite coupling energy of the magnetic moment with the body of the particle is formulated, and regimes of its motion in a rotating magnetic field are investigated. Regimes are possible that are synchronous and asynchronous with the field. In a synchronous regime the easy axis of the particle is in the plane of the rotating magnetic field at low frequencies (a planar regime) and on the cone at high frequencies (a precession regime). The stability of these regimes is investigated, and it is shown that the precession regime is stable for field strengths below the critical value. In a particular range of field strength value, irreversible jumps …

PhysicsRotating magnetic fieldMagnetic anisotropyNuclear magnetic resonanceCondensed matter physicsMagnetic energyDemagnetizing fieldField strengthMagnetic pressureMagnetic dipoleMagnetosphere particle motionPhysical review. E, Statistical, nonlinear, and soft matter physics
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Diffusion in active magnetic colloids

2013

Abstract Properties of active colloids of circle swimmers are reviewed. As a particular example of active magnetic colloids the magnetotactic bacteria under the action of a rotating magnetic field is considered. The relation for a diffusion coefficient due to the random switching of the direction of rotation of their rotary motors is derived on the basis of the master equation. The obtained relation is confirmed by the direct numerical simulation of random trajectory of a magnetotactic bacterium under the action of the Poisson type internal noise due to the random switching of rotary motors. The results obtained are in qualitative and quantitative agreement with the available experimental r…

PhysicsRotating magnetic fieldMagnetotactic bacteriaStatistical Mechanics (cond-mat.stat-mech)Direct numerical simulationFOS: Physical sciencesCondensed Matter - Soft Condensed MatterCondensed Matter PhysicsRotation01 natural sciences6. Clean waterAction (physics)010305 fluids & plasmasElectronic Optical and Magnetic MaterialsQuantitative Biology::Cell BehaviorQuantitative Biology::Subcellular ProcessesClassical mechanics0103 physical sciencesMaster equationTrajectorySoft Condensed Matter (cond-mat.soft)Diffusion (business)010306 general physicsCondensed Matter - Statistical MechanicsJournal of Magnetism and Magnetic Materials
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BeppoSAX serendipitous discovery of the X-ray pulsar SAX J1802.7-2017

2003

We report on the serendipitous discovery of a new X-ray source, SAX J1802.7-2017, ~22' away from the bright X-ray source GX 9+1, during a BeppoSAX observation of the latter source on 2001 September 16-20. SAX J1802.7-2017 remained undetected in the first 50 ks of observation; the source count rate in the following ~300 ks ranged between 0.04 c/s and 0.28 c/s, corresponding to an averaged 0.1-10 keV flux of 3.6 10^{-11} ergs cm^{-2} s^{-1}. We performed a timing analysis and found that SAX J1802.7-2017 has a pulse period of 139.612 s, a projected semimajor axis of a_x sin i ~ 70 lt-s, an orbital period of ~4.6 days, and a mass function f(M) ~ 17 Msun. The new source is thus an accreting X-ra…

PhysicsSemi-major axisAstrophysics (astro-ph)FluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsOrbital periodPulse periodSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceHigh massStars: Pulsars: General Stars: Pulsars: Individual: Alphanumeric: SAX J1802.7-2017 Stars: Magnetic Fields Stars: Neutron X-Rays: BinariesX-ray pulsar
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Thermal conduction and modeling of static stellar coronal loops

1993

We have modeled stellar coronal loops in static conditions for a wide range of loop length, plasma pressure at the base of the loop and stellar surface gravity, so as to describe physical conditions that can occur in coronae of stars ranging from low mass dwarfs to giants as well as on a significant fraction of the Main-Sequence stars.

PhysicsStellar magnetic fieldAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCoronal loopAstrophysicsSolar physicsSurface gravityStarsSpace and Planetary ScienceStellar mass lossPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics::Galaxy AstrophysicsMain sequenceSolar Physics
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Coronal Magnetic Field Measurements Through Quasi-Transverse Propagation

2004

The QT-propagation of microwaves as a means to measure coronal magnetic fields and the inversion of circular polarization as an observational proof of the QT-propagation are discussed. The first part of the chapter briefly outlines the relevant geometry and mathematical relations. Then the state of the art in the coronal magnetography and some possibilities are demonstrated. We discuss use of the technique for coronal magnetography and give some estimates concerning the coronal magnetography with the forthcoming Frequency Agile Solar Radiotelescope.

PhysicsTransverse planeSolar windPhysics::Space PhysicsStellar magnetic fieldAstrophysics::Solar and Stellar AstrophysicsAstronomyMagnetic reconnectionCoronal loopCoronaCoronal radiative lossesComputational physicsNanoflares
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Vibration Detector based on GMR Sensors

2007

Up to now, vibrations have been mostly sensed by measuring displacement, velocity and acceleration. The most common types of vibration sensors are piezoelectric, capacitive, null-balance, strain gage, optoelectronic, resonance beam or piezoresistive. We present a low cost and low power vibration detector based on the measurement of magnetic field variations induced in a recent SS501 GMR magnetic sensor, which has never been applied for that. Vibrations on small ferromagnetic pieces disturb the Earth's magnetic field. These weak perturbations can be detected and measured over the assumed constant Earth's magnetic field, which is uniform over a wide area. A novel array configuration of 3 half…

PhysicsVibrationEarth's magnetic fieldMagnetoresistancebusiness.industryCapacitive sensingAcousticsDetectorElectrical engineeringbusinessPiezoresistive effectStrain gaugeMagnetic field2007 IEEE Instrumentation & Measurement Technology Conference IMTC 2007
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High X-Ray Luminosity from Dynamo Stars

1981

In the present work we intend to show that a stellar dynamo mechanism can produce high X-ray luminosities and also give account for modulation periods of the order thousand seconds or larger.

PhysicsX-ray bursterAstrophysics::High Energy Astrophysical PhenomenaStellar rotationStellar magnetic fieldAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLuminosityStarsDynamo theoryAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Galaxy AstrophysicsMain sequenceDynamo
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