Search results for "Magneto"

showing 10 items of 919 documents

Constraints on the local interstellar magnetic field from non-thermal emission of SN1006

2011

The synchrotron radio morphology of bilateral supernova remnants depends on the mechanisms of particle acceleration and on the viewing geometry. However, unlike X-ray and $\gamma$-ray morphologies, the radio emission does not depend on the cut-off region of the parent electron population, making it a simpler and more straightforward tool to investigate the physics of cosmic ray production in SNRs. Our aim is to derive from the radio morphology tight constraints on the direction of the local magnetic field and its gradient, and on the obliquity dependence of the electron injection efficiency. We perform a set of 3D MHD simulations describing the expansion of a spherical SNR through a magneti…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsshock waveField (physics)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsCosmic rayField strengthAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalactic planeGalaxyMagnetic fieldSupernovaSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomenaacceleration of particleAstrophysics::Galaxy AstrophysicsISM: supernova remnantsAstronomy & Astrophysics
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ROLE OF EJECTA CLUMPING AND BACK-REACTION OF ACCELERATED COSMIC RAYS IN THE EVOLUTION OF TYPE Ia SUPERNOVA REMNANTS

2012

We investigate the role played by initial clumping of ejecta and by efficient acceleration of cosmic rays (CRs) in determining the density structure of the post-shock region of a Type Ia supernova remnant (SNR) through detailed 3D MHD modeling. Our model describes the expansion of a SNR through a magnetized interstellar medium (ISM), including the initial clumping of ejecta and the effects on shock dynamics due to back-reaction of accelerated CRs. The model predictions are compared to the observations of SN 1006. We found that the back-reaction of accelerated CRs alone cannot reproduce the observed separation between the forward shock (FS) and the contact discontinuity (CD) unless the energ…

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsCosmic rayAstrophysicsShock (mechanics)cosmic rays instabilities ISM: supernova remnants magnetohydrodynamics: MHD shock waves supernovae: individual: SN 1006Interstellar mediumSupernovaSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaEjectaSupernova remnantAstrophysics::Galaxy AstrophysicsThe Astrophysical Journal
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Chirality transfer and chiral turbulence in gauge theories

2020

Chirality transfer between fermions and gauge fields plays a crucial role for understanding the dynamics of anomalous transport phenomena such as the Chiral Magnetic Effect. In this proceeding we present a first principles study of these processes based on classical-statistical real-time lattice simulations of strongly coupled QED $(e^2N_f=64)$. Our simulations demonstrate that a chirality imbalance in the fermion sector triggers chiral plasma instabilities in the gauge field sector, which ultimately lead to the generation of long range helical magnetic fields via a self-similar turbulent cascade of the magnetic helicity.

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::Latticechiral plasma instabilitiesFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Magnetic helicity0103 physical sciencesGauge theory010306 general physicsPhysicsChirality transferchiral turbulence010308 nuclear & particles physicsmagnetogensisHigh Energy Physics::PhenomenologyFermionPlasmaMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)CascadeQuantum electrodynamicsChirality (chemistry)Transport phenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Magnetization relaxation in YBCO films with improved supercurrent transport properties

2010

The relaxation of the irreversible magnetization in optimally doped YBCO films with natural and artificial pinning centres was measured in zero-field cooling conditions using SQUID magnetometry. The external magnetic field H was oriented along the c axis. An appropriate method for the determination of the characteristic vortex pinning energy from the normalized vortex-creep activation energy is discussed. This is based on the existence of a crossover elastic (collective) vortex creep at low temperatures T – plastic vortex creep at high T, caused by the T dependent macroscopic currents induced in the sample during magnetization measurements.

HistoryMaterials scienceCondensed matter physicsMagnetometerRelaxation (NMR)Computer Science ApplicationsEducationMagnetic fieldlaw.inventionVortexSQUIDMagnetizationCreeplawCondensed Matter::SuperconductivityPinning forceJournal of Physics: Conference Series
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An iterative based approach for hysteresis parameters estimation in Magnetorheological dampers

2012

The following work entails the problem of regenerating the hysteresis loop in the Magnetorheological (MR) dampers. The collected data from tests are not sufficient neither efficient for designing optimal controls compensating for the hysteresis in the dampers. This work presents an iterative based approach for estimating the hysteresis parameters, the method however can be generalized for different kind of dampers or actuators hence the hysteresis loop can be generalized using available test data. Some assumptions can be introduced in order to facilitate the underlines of the parameters estimation, one of the assumptions in this work is to use predetermined hysteresis parameters and regener…

HysteresisControl theoryEstimation theoryIterative methodComputer scienceMagnetorheological fluidParticle swarm optimizationMagnetorheological damperDamperTest data2012 6th IEEE INTERNATIONAL CONFERENCE INTELLIGENT SYSTEMS
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Firefly optimization used to identify hysteresis parameter on rotational MR-damper

2014

In his paper the physical properties and mathematical models of a semi-active magnetorheological (MR) damper is studied. The considered models are the Dahl model and Bouc-Wen model. The parameters for these models are found by using a firefly optimization algorithm that minimizes the difference between experimental and simulated data. The objective of his paper is to compare different mathematical MR-damper models with the experimental data. The simulation results illustrate he effectiveness of he proposed optimization algorithm.

HysteresisShock absorberEngineeringMathematical modelControl theorybusiness.industryMagnetorheological fluidExperimental dataTorquebusinessDamperData modeling2014 International Conference on Mechatronics and Control (ICMC)
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Numerical simulation of unsteady MHD flows and applications

2009

International audience; We present a robust numerical method for solving the compressible Ideal Magneto-Hydrodynamic equations. It is based on the Residual Distribution (RD) algorithms already successfully tested in many problems. We adapted the scheme to the multi-dimensional unsteady MHD model. The constraint ∇ · B = 0 is enforced by the use a Generalized Lagrange Multiplier (GLM) technique. First, we present this complete system and the keys to get its eigensystem, as we may need it in the algorithm. Next, we introduce the numerical scheme built in order to get a compressible, unsteady and implicit solver which has good shock-capturing properties and is second-order accurate at the conve…

Ideal (set theory)Computer simulationComputer scienceNumerical analysisGeneral Physics and AstronomySolver01 natural sciences010305 fluids & plasmasConstraint (information theory)symbols.namesakeLagrange multiplier0103 physical sciencesCompressibilitysymbols[INFO.INFO-DC] Computer Science [cs]/Distributed Parallel and Cluster Computing [cs.DC]Applied mathematicsElectrical and Electronic EngineeringMagnetohydrodynamics[INFO.INFO-DC]Computer Science [cs]/Distributed Parallel and Cluster Computing [cs.DC]010306 general physics
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Feasibility study for a nanosatellite-based instrument for in-situ measurements of radio noise

2015

The radio environment on the earth is heavily affected by manmade sources such as radio transmissions, radars, and the like. The effect is particularly strong at MF frequencies and below, since the signals can propagate large distances via ionospheric bounce. Terrestrial magnetometer measurements have long been used to predict the Kp index, which is related to radio transmission at these ranges. Space weather measurements and models can also predict propagation of MF signals on the ground.

In situRadio transmissionMeteorologyMagnetometerlawPhysics::Space PhysicsEnvironmental scienceSpace weatherIonospherePhysics::GeophysicsRadio waveRemote sensinglaw.invention2015 1st URSI Atlantic Radio Science Conference (URSI AT-RASC)
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Maiņstrāvas magnētiskā lauka mērīšana augstas temperatūras apstākļos izmantojot spolītes ar ferīta serdi

2015

Šī darba mērķis ir izpētīt spolītes ar ferīta serdi. Mērīšanai izmantot mainīgu magnētisko lauku. Mērījumi veikti ar vairākām spolītēm, lai novērtētu, cik uzticama būtu šāda veida mērīšana. Darbā apskatīti sekojoši jautājumi: •spolīšu inducētais spriegums dažāda stipruma ārējos magnētiskajos laukos, tā forma; •spolīšu inducētais spriegums pie dažādiem leņķiem pret magnētiskā lauka līnijām; •spolīšu inducētais spriegums pie dažādām temperatūrām; •spolīšu kritiskā temperatūra. Rezultāti tiek salīdzināti ar teorētiskajiem datiem un izdarīti secinājumi par to vai šīs spolītes un šāda metode ir noderīga LU FI patreizējos un nākotnes projektos.

Indukcijas spoleMagnetohidrodinamikaInducētais spriegumsFizikaMagnētiskais lauks
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Compensating for instantaneous signal mixing in transfer entropy analysis of neurobiological time series

2013

The transfer entropy (TE) has recently emerged as a nonlinear model-free tool, framed in information theory, to detect directed interactions in coupled processes. Unfortunately, when applied to neurobiological time series TE is biased by signal cross-talk due to volume conduction. To compensate for this bias, in this study we introduce a modified TE measure which accounts for possible instantaneous effects between the analyzed time series. The new measure, denoted as compensated TE (cTE), is tested on simulated time series reproducing conditions typical of neuroscience applications, and on real magnetoencephalographic (MEG) multi-trial data measured during a visuo-tactile cognitive experime…

Information transferTime FactorsComputer scienceEntropySpeech recognitionBiomedical EngineeringHealth InformaticsInformation theoryEntropy (classical thermodynamics)medicineHumansEntropy (information theory)Computer SimulationNervous System Physiological PhenomenaEntropy (energy dispersal)Entropy (arrow of time)Visual Cortex1707Entropy (statistical thermodynamics)MagnetoencephalographySignal Processing Computer-AssistedSomatosensory CortexNonlinear systemVisual cortexmedicine.anatomical_structureSignal ProcessingSettore ING-INF/06 - Bioingegneria Elettronica E InformaticaTransfer entropyAlgorithmEntropy (order and disorder)
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