Search results for "Magneto"

showing 10 items of 919 documents

The force-free twisted magnetosphere of a neutron star

2016

We present a detailed analysis of the properties of twisted, force-free magnetospheres of non-rotating neutron stars, which are of interest in the modelling of magnetar properties and evolution. In our models the magnetic field smoothly matches to a current-free (vacuum) solution at some large external radius, and they are specifically built to avoid pathological surface currents at any of the interfaces. By exploring a large range of parameters, we find a few remarkable general trends. We find that the total dipolar moment can be increased by up to $40\%$ with respect to a vacuum model with the same surface magnetic field, due to the contribution of magnetospheric currents to the global ma…

MHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMagnetosphere7. Clean energy01 natural sciences010305 fluids & plasmasNuclear physicsmagnetars [Stars]0103 physical sciencesmedia_common.cataloged_instanceCost actionEuropean union010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)media_commonAstronomía y AstrofísicaHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and Astrophysicsneutron [Stars]Magnetic fieldNeutron starAstrophysics - Solar and Stellar AstrophysicsWork (electrical)Space and Planetary ScienceMagnetic fieldsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Instability of relativistic sheared jets and distinction between FRI and FRII sources

2002

We investigate the shear-driven instability of nonmagnetic relativistic jets with the bulk velocity, V , dependent on the cylindric radius, r. It is shown that instability can arise for any dependence of the velocity (or the Lorentz factor that is the same) on r. The shear-driven instability can e ectively operate in the whole volume of a jet. The growth time can be shorter than that of the Kelvin-Helmholtz instability. The considered instability leads to a turbulization of jets and can account for a distiction between the jets in the FRI and FRII sources. Urpin, V., Vadim.Urpin@uv.es

MHDAstrophysics::High Energy Astrophysical PhenomenaJets and outflowsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAInstabilityMHD ; Instabilities ; ISM ; Jets and outflows ; Galaxiessymbols.namesakeAstrophysical jetComputer Science::DatabasesISMPhysicsJet (fluid)Astronomy and AstrophysicsRadiusGalaxies:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Growth timeLorentz factorSpace and Planetary ScienceInstabilitiessymbolsBulk velocityUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaMagnetohydrodynamics:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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How to form a millisecond magnetar? Magnetic field amplification in protoneutron stars

2017

Extremely strong magnetic fields of the order of $10^{15}\,{\rm G}$ are required to explain the properties of magnetars, the most magnetic neutron stars. Such a strong magnetic field is expected to play an important role for the dynamics of core-collapse supernovae, and in the presence of rapid rotation may power superluminous supernovae and hypernovae associated to long gamma-ray bursts. The origin of these strong magnetic fields remains, however, obscure and most likely requires an amplification over many orders of magnitude in the protoneutron star. One of the most promising agents is the magnetorotational instability (MRI), which can in principle amplify exponentially fast a weak initia…

MHD[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsmagnetic fieldsMagnetar01 natural sciencesstars: neutronsupernovae: generalstars: rotation0103 physical sciencesstars: magnetic fieldsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMillisecond010308 nuclear & particles physicsAstronomy and AstrophysicsMagnetic fieldStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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MITC FINITE ELEMENTS FOR MAGNETO-ELECTRO-ELASTIC PLATES BASED ON EQUIVALENT SINGLE-LAYER THEORY

2013

Finite elements for magneto-electro-elastic laminated plates are formulated. They are based on an equivalent single-layer model, which assumes the first order shear deformation theory and quasi-static behavior for the electric and magnetic fields. To infer the plate model, the electro-magnetic state is firstly determined and condensed to the the mechanical primary variables, namely the generalized displacements. In turn, this result is used into the layers constitutive law to obtain the equivalent single-layer laminate constitutive relationship that expresses the plate mechanical stress resultants in terms of the generalized displacements taking the magneto-electro-elastic couplings into ac…

MITC Finite ElementSettore ING-IND/04 - Costruzioni E Strutture AerospazialiMultilayered plateMagneto-electro-elastic structure
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Electric field modification of magnetotransport in Ni thin films on (011) PMN-PT piezosubstrates

2015

This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared in Appl. Phys. Lett. 106, 062404 (2015) and may be found at https://doi.org/10.1063/1.4907775 This study reports the magnetotransport and magnetic properties of 20 nm-thick polycrystalline Ni films deposited by magnetron sputtering on unpoled piezoelectric (011) [PbMg1/3Nb2/3O3]0.68-[PbTiO3]0.32 (PMN-PT) substrates. The longitudinal magnetoresistance (MR) of the Ni films on (011) PMN-PT, measured at room temperature in the magnetic field range of −0.3 T < μ0H < 0.3 T, is found to depend on the crystallographic direction and polarization state …

Magnetic anisotropyMaterials sciencePhysics and Astronomy (miscellaneous)Condensed matter physicsMagnetoresistanceRemanenceElectric fieldPolingddc:530Sputter depositionThin filmMagnetic fieldBIFEO3
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Magnetic Anisotropy Engineering in Thin Film Ni Nanostructures by Magnetoelastic Coupling

2014

Magnetic anisotropyNanostructureMaterials scienceCondensed matter physics530 PhysicsGeneral Physics and AstronomyThin film530 PhysikMagnetoelastic couplingPhysical Review Applied
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Phase separated Cu@Fe3O4 heterodimer nanoparticles from organometallic reactants

2011

Cu@Fe3O4 heteroparticles with distinct morphologies were synthesized from organometallic reactants. The shape of the magnetic domains could be controlled by the solvent and reaction conditions. They display magnetic and optical properties that are useful for simultaneous magnetic and optical detection. After functionalization, the Cu@Fe3O4 heterodimers become water soluble. The morphology, structure, magnetic and optical properties of the as-synthesized heterodimer nanoparticles were characterized using transmission electron microscopy (TEM), X-ray diffraction (XRD), mossbauer spectroscopy, superconducting quantum interference device (SQUID) magnetometry, and dark field imaging. A special a…

Magnetic domainMagnetometerChemistryNanoparticleGeneral Chemistryequipment and suppliesDark field microscopylaw.inventionSQUIDCrystallographylawTransmission electron microscopyPhase (matter)Mössbauer spectroscopyMaterials Chemistryhuman activitiesJournal of Materials Chemistry
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New ultraportable data logger to perform magnetic surveys

2019

This article presents the realization of a device for magnetic surveys It is a flexible, user-reprogramable, lightweight, and compact tool that can be easily integrated with aerial and marine drones. The device can accurately measure the local magnetic anomalies. It is based on the Atmega 2560 microcontroller and a digital 3-axis fluxgate magnetometer.

Magnetic domaingeophysicMagnetometerbusiness.industryComputer scienceUAV010401 analytical chemistryElectrical engineeringMeasure (physics)Magnetic separationmagnetic surveyComputerApplications_COMPUTERSINOTHERSYSTEMS010502 geochemistry & geophysics01 natural sciences0104 chemical scienceslaw.inventionMicrocontrollerlawROVData loggerMagnetic anomalybusinessRealization (systems)0105 earth and related environmental sciences
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Search for Magnetic Monopoles with the MoEDAL Forward Trapping Detector in 13 TeV Proton-Proton Collisions at the LHC

2017

MoEDAL is designed to identify new physics in the form of long-lived highly-ionising particles produced in high-energy LHC collisions. Its arrays of plastic nuclear-track detectors and aluminium trapping volumes provide two independent passive detection techniques. We present here the results of a first search for magnetic monopole production in 13 TeV proton-proton collisions using the trapping technique, extending a previous publication with 8 TeV data during LHC run-1. A total of 222 kg of MoEDAL trapping detector samples was exposed in the forward region and analysed by searching for induced persistent currents after passage through a superconducting magnetometer. Magnetic charges excee…

Magnetic monopolesProtonMagnetismPhysics beyond the Standard ModelGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - Experimentlaw.inventionCOLLIDERHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)STOPPING-POWERlawPhysics02 Physical SciencesLarge Hadron ColliderSTABLE MASSIVE PARTICLESPhysicsMagnetismDrell–Yan processhep-phPersistent currents3. Good healthHigh Energy Physics - PhenomenologyPhysical SciencesELECTROWEAK MONOPOLEParticle Physics - ExperimentGeneral PhysicsMagnetometerPhysics MultidisciplinaryMagnetic monopoleFOS: Physical sciencesNuclear track detector114 Physical sciencesNuclear physicsPhysics and Astronomy (all)Tellurium compoundsHigh energy physics Magnetism Magnetometers Highly ionizing particles Magnetic charges Magnetic monopoles Nuclear track detector Passive detection Persistent currents Proton proton collisions Trapping techniques Tellurium compounds0103 physical sciencesHigh energy physics010306 general physicsColliderIONIZING PARTICLESScience & TechnologyProton proton collisionshep-ex010308 nuclear & particles physicsMagnetometers Highly ionizing particlesMagnetic chargesTrapping techniquesPassive detectionSTATES
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&lt;title&gt;Influence of strong static magnetic field on human cancer HT 1080 cells&lt;/title&gt;

2001

The aim of this study was to investigate strong uniform magnetic field influence on the human cancer cells HT 1080. The cells were treated with magnetic field of intensity 1,16 Tesla and with anticancer agent - cis-platinum 0.025 mg/ml or vincristinum 2-3 ng/ml. The intact and the treated cell samples were incubated in a medium with acridine orange (AO). The magnetic field after 15 minutes of influence significantly increased cytoplasmic red fluorescence. Increased AO accumulation in lysosomes suggested to cancer cell metabolic activity stimulation.© (2001) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.

MagnetismAcridine orangeCancerMagnetostaticsmedicine.diseasechemistry.chemical_compoundNuclear magnetic resonancechemistryCytoplasmCancer cellBiophysicsmedicinehuman activitiesHuman cancerTreated cellSPIE Proceedings
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