Search results for "MAGNETIC FIELD"

showing 10 items of 1488 documents

On numerical simulation of electromagnetic field effects in the combustion process

2018

This paper deals with a simplified model taking into account the interplay of compressible, laminar, axisymmetric flow and the electrodynamical effects due to Lorentz force’s action on the combustion process in a cylindrical pipe. The combustion process with Arrhenius kinetics is modelled by a single step exothermic chemical reaction of fuel and oxidant. We analyze non-stationary PDEs with 6 unknown functions: the 3 components of velocity, density, concentration of fuel and temperature. For pressure the ideal gas law is used. For the inviscid flow approximation ADI method is used. Some numerical results are presented.

Exothermic reactionElectromagnetic fieldMaterials science01 natural sciences010305 fluids & plasmasPhysics::Fluid Dynamicssymbols.namesakeLorentz forceInviscid flow0103 physical sciencesQA1-9390101 mathematicsPhysics::Chemical PhysicsIdeal gas law010102 general mathematicsaxisymmetric flowArrhenius kineticsLaminar flowMechanicslaminarAlternating direction implicit methodModeling and SimulationCompressibilitysymbolsLorentz forceAnalysisMathematicscompressibleMathematical Modelling and Analysis
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Magnetic field dynamos and magnetically triggered flow instabilities

2017

The project A2 of the LIMTECH Alliance aimed at a better understanding of those magnetohydrodynamic instabilities that are relevant for the generation and the action of cosmic magnetic fields. These comprise the hydromagnetic dynamo effect and various magnetically triggered flow instabilities, such as the magnetorotational instability and the Tayler instability. The project was intended to support the experimental capabilities to become available in the framework of the DREsden Sodium facility for DYNamo and thermohydraulic studies (DRESDYN). An associated starting grant was focused on the dimensioning of a liquid metal experiment on the newly found magnetic destabilization of rotating flow…

F300FOS: Physical sciencesF5007. Clean energy01 natural sciencesInstability010305 fluids & plasmasPhysics - GeophysicsMagnetorotational instability0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic drive[NLIN]Nonlinear Sciences [physics]010306 general physicsPhysics[PHYS]Physics [physics]Fluid Dynamics (physics.flu-dyn)MechanicsPhysics - Fluid Dynamics[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Magnetic fieldGeophysics (physics.geo-ph)Shear (sheet metal)Flow (mathematics)Dynamo theory[NLIN.NLIN-CD]Nonlinear Sciences [physics]/Chaotic Dynamics [nlin.CD][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Dynamo
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Modelling of asymmetric nanojets in coronal loops

2021

Context. Observations of reconnection jets in the solar corona are emerging as a possible diagnostic for studying highly elusive coronal heating. Such jets, and in particular those termed nanojets, can be observed in coronal loops and have been linked to nanoflares. However, while models successfully describe the bilateral post-reconnection magnetic slingshot effect that leads to the jets, observations reveal that nanojets are unidirectional or highly asymmetric, with only the jet travelling inward with respect to the coronal loop’s curvature being clearly observed. Aims. The aim of this work is to address the role of the curvature of the coronal loop in the generation and evolution of asym…

F300media_common.quotation_subjectFOS: Physical sciencesAstrophysicsF500magnetic fieldsCurvaturemagnetohydrodynamics (MHD)AsymmetryAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic driveSolar and Stellar Astrophysics (astro-ph.SR)media_commonPhysicsJet (fluid)SunAstronomy and AstrophysicsMechanicsCoronal loopNanoflaresMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceatmospherePhysics::Space PhysicsMagnetohydrodynamicscoronaSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo Circumterrestre
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Gain, detuning, and radiation patterns of nanoparticle optical antennas

2008

International audience; For their capability to localize and redirect electromagnetic field, metal nanoparticles have been recently viewed as efficient nanoantenna operating in the optical regime. In this article, we experimentally investigated the optical responses of coupled gold antenna pairs and measured the critical parameters defining antenna characteristics: resonant frequencies and bandwidths, detuning and gains, and radiation patterns.

FAR-FIELDElectromagnetic fieldPLASMONIC NANOPARTICLEPhysics::OpticsNanoparticle02 engineering and technologySILVER NANOPARTICLESRadiation01 natural sciencesNANOANTENNASOptics[ PHYS.COND.CM-MSQHE ] Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall]0103 physical sciencesSCATTERING[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics010306 general physicsMetal nanoparticles[PHYS.COND.CM-MSQHE]Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryRESONANCE021001 nanoscience & nanotechnologyCondensed Matter PhysicsDIMERSElectronic Optical and Magnetic MaterialsSINGLE[SPI.OPTI]Engineering Sciences [physics]/Optics / PhotonicQuasiparticleOptoelectronics[ SPI.NANO ] Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics[ SPI.OPTI ] Engineering Sciences [physics]/Optics / PhotonicAntenna (radio)EMISSION0210 nano-technologybusinessNEAR-FIELDPhysical Review B
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

2016

We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles ra…

FLUORESCENCE YIELDAstronomymagnetic monopolemagnetic fieldAstrophysics7. Clean energy01 natural sciencesObservatoryUHE Cosmic Raysair-showerMonte Carlo010303 astronomy & astrophysicsMagnetic Monopolesmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicscritical phenomenaFLUORESCENCE YIELD; ENERGY LOSS; DETECTORAugerMagnetic fieldobservatoryLorentz factorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical Phenomenaspatial distribution [showers]LorentzENERGY LOSSatmosphere [showers]energyFLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]airmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Magnetic monopoleFOS: Physical sciencesCosmic rayNuclear physicssymbols.namesakecosmic rays0103 physical sciencesddc:530High Energy PhysicsDETECTORCiencias Exactasfluorescence [detector]Pierre Auger Observatorybackground010308 nuclear & particles physicsFísicaASTROFÍSICAUniversefluxultrarelativistic magnetic monopolesAir shower13. Climate actionExperimental High Energy PhysicsrelativisticgalaxyENERGY-LOSS
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Generation of energy selective excitations in quantum hall edge states

2011

We operate an on-demand source of single electrons in high perpendicular magnetic fields up to 30T, corresponding to a filling factor below 1/3. The device extracts and emits single charges at a tunable energy from and to a two-dimensional electron gas, brought into well defined integer and fractional quantum Hall (QH) states. It can therefore be used for sensitive electrical transport studies, e.g. of excitations and relaxation processes in QH edge states.

FOS: Physical sciences02 engineering and technologyElectronCorrelated Electron Systems / High Field Magnet Laboratory (HFML)Quantum Hall effect7. Clean energy01 natural sciences0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Materials ChemistryPerpendicularElectrical and Electronic EngineeringWell-defined010306 general physicsPhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsFilling factorRelaxation (NMR)021001 nanoscience & nanotechnologyCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSING0210 nano-technologyFermi gas
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Time-dependent transport in Aharonov–Bohm interferometers

2010

A numerical approach is employed to explain transport characteristics in realistic, quantum Hall based Aharonov-Bohm interferometers. First, the spatial distribution of incompressible strips, and thus the current channels, are obtained applying a self-consistent Thomas-Fermi method to a realistic heterostructure under quantized Hall conditions. Second, the time-dependent Schr\"odinger equation is solved for electrons injected in the current channels. Distinctive Aharonov-Bohm oscillations are found as a function of the magnetic flux. The oscillation amplitude strongly depends on the mutual distance between the transport channels and on their width. At an optimal distance the amplitude and t…

FOS: Physical sciencesGeneral Physics and AstronomyFlux02 engineering and technologySTRIPSElectronQuantum Hall effect01 natural sciencesSchrödinger equationlaw.inventionCondensed Matter - Strongly Correlated Electronssymbols.namesakelawMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciences010306 general physicsPhysicsStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - Mesoscale and Nanoscale PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall Effect021001 nanoscience & nanotechnologyMagnetic fluxMagnetic fieldAmplitudeQuantum electrodynamicssymbols0210 nano-technologyNew Journal of Physics
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Faraday patterns in bose-Einstein condensates.

2002

Temporal periodic modulation of the interatomic s-wave scattering length in Bose-Einstein condensates is shown to excite subharmonic patterns of atom density through a parametric resonance. The dominating wavelength of the spatial structures is shown to be primarily selected by the excitation frequency but also affected by the depth of the spatial modulation via a nonlinear resonance. These phenomena represent macroscopic quantum analogues of the Faraday waves excited in vertically shaken liquids.

FOS: Physical sciencesGeneral Physics and AstronomyPattern formationPattern Formation and Solitons (nlin.PS)Resonance (particle physics)law.inventionFaraday wavesymbols.namesakelawQuantum mechanicsFaraday effectFaraday cageFeshbach resonanceCondensed Matter - Statistical MechanicsPhysicsCondensed Matter::Quantum GasesStatistical Mechanics (cond-mat.stat-mech)Condensed matter physicsScatteringCondensed Matter::OtherResonanceScattering lengthNonlinear Sciences - Pattern Formation and SolitonsSymmetry (physics)Magnetic fieldModulationNonlinear resonanceExcited statesymbolsDissipative systemState of matterAtomic physicsParametric oscillatorExcitationBose–Einstein condensatePhysical review letters
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Variable X-ray emission from the accretion shock in the classical T Tauri star V2129 Ophiuchi

2011

The soft X-ray emission from high density plasma in CTTS is associated with the accretion process. It is still unclear whether this high density cool plasma is heated in the accretion shock, or if it is coronal plasma fed/modified by the accretion process. We conducted a coordinated quasi-simultaneous optical and X-ray observing campaign of the CTTS V2129 Oph (Chandra/HETGS data to constrain the X-ray emitting plasma components, and optical observations to constrain the characteristics of accretion and magnetic field). We analyze a 200 ks Chandra/HETGS observation of V2129 Oph, subdivided into two 100 ks segments, corresponding to two different phases within one stellar rotation. The X-ray …

FOS: Physical sciencesstars: variables:X-rays: starsmagnetic fieldAstrophysicsstars: pre-main sequenceT Tauricircumstellar matterlaw.inventionX-raycircumstellar matter stars: coronae stars: individual: V2129 Oph stars: pre-main sequence X-rays: stars stars: variables: T Tauri Herbig Ae/BeSettore FIS/05 - Astronomia E AstrofisicaaccretionlawSolar and Stellar Astrophysics (astro-ph.SR)Physicsstars: coronaeLine-of-sight[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Stellar rotationHerbig Ae/Bestars: individual: V2129Astronomy and AstrophysicsPlasmaCoronal loopAccretion (astrophysics)Magnetic fieldT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science[SDU]Sciences of the Universe [physics]stellar activityOphFlare
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Faraday effect in magnetic fluids at a frequency 10GHz

2002

Abstract This work presents some results of observed Faraday effect in magnetic fluids in the centimetric region of the electromagnetic spectrum. The effect is observed when a transversal electric wave of mode H11 propagates in the circular waveguide with a magnetic fluid. The constant magnetic field was applied along the waveguide. Magnetic fluids with different concentrations of magnetite core nanoparticles suspended in tetradecane (C14H30) are used in the magnetic fields from 0 to 1500 Oe. A 160° rotation of wave polarization is obtained for a 200 mm sample.

FerrofluidMaterials scienceCondensed matter physicsElectromagnetic spectrumbusiness.industryCondensed Matter PhysicsMagneto-optic effectElectronic Optical and Magnetic Materialslaw.inventionMagnetic fieldsymbols.namesakeOpticslawFaraday effectsymbolsbusinessFaraday rotatorWaveguideMicrowaveJournal of Magnetism and Magnetic Materials
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