Search results for "Magnetic flux"

showing 10 items of 80 documents

Design and experimental validation of a magnetic device for stem cell culture.

2020

Cell culture of bone and tendon tissues requires mechanical stimulation of the cells in order to mimic their physiological state. In the present work, a device has been conceived and developed to generate a controlled magnetic field with a homogeneous gradient in the working space. The design requirement was to maximize the magnetic flux gradient, assuring a minimum magnetizing value in a 15 mm × 15 mm working area, which highly increases the normal operating range of this sort of devices. The objective is to use the machine for two types of biological tests: magnetic irradiation of biological samples and force generation on paramagnetic particles embedded in scaffolds for cell culture. The…

010302 applied physicsElectromagnetic fieldMaterials scienceStem CellsCell Culture TechniquesExperimental validationEquipment Designequipment and supplies01 natural sciencesMagnetic flux010305 fluids & plasmasMagnetic fieldMagnetic FieldsCell cultureDental pulp stem cells0103 physical sciencesMagnetic nanoparticlesIrradiationInstrumentationhuman activitiesBiomedical engineeringThe Review of scientific instruments
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A tale of two emergences: Sunrise II observations of emergence sites in a solar active region

2017

R. Centeno et. al.

010504 meteorology & atmospheric sciencesField (physics)photosphere [Sun]Field lineFOS: Physical sciencesFluxchromosphere [Sun]Astrophysicspolarimetric [Techniques]01 natural sciences0103 physical sciencesSunrise010303 astronomy & astrophysicsChromosphereSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSunspotsSun: chromosphereTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic reconnectionMagnetic fluxMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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Magnetic shuffling of coronal downdrafts

2017

Channelled fragmented downflows are ubiquitous in magnetized atmospheres, and have been recently addressed from an observation after a solar eruption. We study the possible back-effect of the magnetic field on the propagation of confined flows. We compare two 3D MHD simulations of dense supersonic plasma blobs downfalling along a coronal magnetic flux tube. In one, the blobs move strictly along the field lines; in the other, the initial velocity of the blobs is not perfectly aligned to the magnetic field and the field is weaker. The aligned blobs remain compact while flowing along the tube, with the generated shocks. The misaligned blobs are disrupted and merged by the chaotic shuffling of …

010504 meteorology & atmospheric sciencesField lineAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsSun:corona01 natural sciencesAlfvén waveSettore FIS/05 - Astronomia E AstrofisicaPhysics::Plasma Physics0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar flareAstronomy and AstrophysicsSun:activityPlasmaMagnetic fluxAccretion (astrophysics)Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsmagnetohydrodynamics
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Spectropolarimetric evidence for a siphon flow along an emerging magnetic flux tube

2016

©2017 The American Astronomical Society. All rights reserved.We study the dynamics and topology of an emerging magnetic flux concentration using high spatial resolution spectropolarimetric data acquired with the Imaging Magnetograph eXperiment on board the sunrise balloon-borne solar observatory. We obtain the full vector magnetic field and the line of sight (LOS) velocity through inversions of the Fe i line at 525.02 nm with the SPINOR code. The derived vector magnetic field is used to trace magnetic field lines. Two magnetic flux concentrations with different polarities and LOS velocities are found to be connected by a group of arch-shaped magnetic field lines. The positive polarity footp…

010504 meteorology & atmospheric sciencesPolarity (physics)photosphere [Sun]FOS: Physical sciencesAstrophysicspolarimetric [Techniques]01 natural sciencesMethods: observational0103 physical sciencesSunriseAstrophysics::Solar and Stellar Astrophysicsobservational [Methods]010303 astronomy & astrophysicsSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsSolar observatoryPolarity symbolsTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsFlow (mathematics)magnetic fields [Sun]Space and Planetary Science
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The intensity contrast of solar photospheric faculae and network elements : II. Evolution over the rising phase of solar cycle 23

2006

We studied the radiative properties of small magnetic elements (active region faculae and the network) during the rising phase of solar cycle 23 from 1996 to 2001, determining their contrasts as a function of heliocentric angle, magnetogram signal, and the solar cycle phase. We combined near-simultaneous full disk images of the line-of-sight magnetic field and photospheric continuum intensity provided by the MDI instrument on board the SOHO spacecraft. Sorting the magnetogram signal into different ranges allowed us to distinguish between the contrast of different magnetic structures. We find that the contrast center-to-limb variation (CLV) of these small magnetic elements is independent of …

:ASTRONOMÍA Y ASTROFÍSICA::Sistema solar [UNESCO]PlagesFOS: Physical sciencesSolar cycle 23AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAFaculaeMagnetogramSun activityRadiative transferAstrophysics::Solar and Stellar AstrophysicsPhysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Sistema solarSpacecraftbusiness.industryAstrophysics (astro-ph)SunContrast (statistics)Astronomy and AstrophysicsMagnetic fluxMagnetic fieldOn boardSun activity ; Faculae ; Plages ; Sun ; Magnetic fieldsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsAstrophysics::Earth and Planetary Astrophysicsbusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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3‐D CALCULATION OF ZERO‐COMPONENT FLUX IN THREE‐PHASE THREE‐COLUMN TRANSFORMER

1994

The paper discusses the problem of space distribution of zero‐component magnetic flux generated in three‐column transformer. For 3‐D magnetic field calculation the method of integral equations was used. The numerical calculations were made for physical model of the transformer and compared with experimental results. The accuracy of the calculations of the magnetic field, achieved in the work, proves that the modelling may be used as a computer aided designing tool.

Applied MathematicsMechanicsIntegral equationMagnetic fluxComputer Science ApplicationsMagnetic fieldlaw.inventionComputational Theory and MathematicsThree-phaselawElectronic engineeringComputer-aidedElectrical and Electronic EngineeringTransformerMathematicsCOMPEL - The international journal for computation and mathematics in electrical and electronic engineering
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A Targeted Search for Point Sources of EeV Neutrons

2014

A flux of neutrons from an astrophysical source in the Galaxy can be detected in the Pierre Auger Observatory as an excess of cosmic-ray air showers arriving from the direction of the source. To avoid the statistical penalty for making many trials, classes of objects are tested in combinations as nine “target sets”, in addition to the search for a neutron flux from the Galactic Center or from the Galactic Plane. Within a target set, each candidate source is weighted in proportion to its electromagnetic flux, its exposure to the Auger Observatory, and its flux attenuation factor due to neutron decay. These searches do not find evidence for a neutron flux from any class of candidate sources. …

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesGalaxy: diskcosmic raysNeutron fluxObservatory0103 physical sciencesdata analysis [methods]Neutron010306 general physics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Galactic CenterPierre Auger Observatory; cosmic ray; neutronsAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsGalactic planemethods: data analysisMagnetic fluxGalaxyAstronomíaSpace and Planetary ScienceExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGddc:520Física nuclearAstrophysics - High Energy Astrophysical Phenomenadisk [Galaxy]
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A new technique for observationally derived boundary conditions for space weather

2018

This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 647214). D.H.M. would like to thank STFC and the Leverhulme Trust for their financial support. ARY was supported by STFC consortium grant ST/N000781/1 to the universities of Dundee and Durham. Context.  In recent years, space weather research has focused on developing modelling techniques to predict the arrival time and properties of coronal mass ejections (CMEs) at the Earth. The aim of this paper is to propose a new modelling technique suitable for the next generation of Space Weather predictive tools that is both efficie…

Atmospheric Science010504 meteorology & atmospheric sciencesMHDNDASWeather forecastingFluxFOS: Physical sciencesContext (language use)Space weatherlcsh:QC851-999computer.software_genre01 natural sciencesSolar Corona0103 physical sciencesCMECoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsBoundary value problemQA010303 astronomy & astrophysicsR2CSolar and Stellar Astrophysics (astro-ph.SR)QB0105 earth and related environmental sciencesPhysicssolar CoronaMechanicsMagnetic fluxAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary SciencePhysics::Space Physicslcsh:Meteorology. ClimatologyMagnetohydrodynamicsBDCcomputerJournal of Space Weather and Space Climate
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State Space-Vector Model of Linear Induction Motors including End-Effects and Iron Losses Part I: Theoretical Analysis

2020

This is the first part of the article, divided into two parts, dealing with the definition of a space-vector dynamic model of the linear induction motor (LIM) taking into consideration both the dynamic end-effects and the iron losses and its offline identification. This first part specifically treats the theoretical formulation of this model, which has been expressed in a state form, so to be, in perspective, suitably adopted for developing novel nonlinear control techniques, nonlinear observers as well as electrical losses minimization techniques. Besides the formulation of the dynamic model in space-vector state form, a steady-state analysis is proposed, highlighting the combined effects …

Computer sciencestate modelend-effectsNonlinear controlIndustrial and Manufacturing EngineeringMagnetic fluxEnd-effectIdentification (information)Nonlinear systemPerspective (geometry)Settore ING-INF/04 - AutomaticaControl and Systems EngineeringControl theoryLinear induction motorspace vectorState spacelinear induction motor (LIM)MinificationElectrical and Electronic Engineering
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Exploring helical phases of matter in bosonic ladders

2020

Ladder models of ultracold atoms offer a versatile platform for the experimental and theoretical study of different phenomena and phases of matter linked to the interplay between artificial gauge fields and interactions. Strongly correlated helical states are known to appear for specific ratios of the particle and magnetic flux densities and they can often be interpreted as a one-dimensional limit of fractional quantum Hall states, thus being called pretopological. Their signatures, however, are typically hard to observe due to the small gaps characterizing these states. Here we investigate bosonic ladder models at filling factor 1. Based on bosonization, renormalization group and matrix pr…

Condensed Matter::Quantum GasesPhysicsQuantum PhysicsParticle numberCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)FOS: Physical sciencesMagnetic fluxCondensed Matter - Strongly Correlated ElectronsQuantum Gases (cond-mat.quant-gas)Condensed Matter::Strongly Correlated Electronsddc:530Physics::Atomic PhysicsCondensed Matter - Quantum GasesQuantum Physics (quant-ph)
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