Search results for " Magnetic field"

showing 10 items of 165 documents

STUDIO DI UNA FRIZIONE MAGNETOREOLOGICA PER AUTOVEICOLI

2013

Dopo un’accurata ricerca bibliografica sui fluidi magnetoreologici, il loro comportamento ed impiego, si è passati alla progettazione di una frizione magnetoreologica per autoveicoli. Considerando le caratteristiche di coppia trasmessa e potenza, il dispositivo è stato dimensionato tenendo presente i vincoli di ingombro del veicolo preso in esame. Sottoponendo il dispositivo ad analisi magnetostatica agli elementi finiti, si è determinato l’andamento delle linee di flusso del campo magnetico nel meato di fluido e nelle zone di maggior interesse, calcolando la coppia teoricamente trasmessa dall’innesto.È stato anche eseguito il confronto delle prestazionifra una frizione MR ed una frizione t…

Settore ING-IND/14 - Progettazione Meccanica E Costruzione Di MacchineAfter a thorough literature search on magnetorheological fluids their behavior and use it has gone to the design of a magnetorheological clutch for motor vehicles. Considering the characteristics of transmitted torque and power the device is dimensioned taking into account the constraints of space of the examined vehicle. Subjecting the device to magnetostatic finite element analysis it was determined the trend of the flow lines of the magnetic field in the gap of fluid and in areas of greater interest calculating the torque transmitted theoretically by the clutch. The performance comparison between a traditional clutch and a MR clutch was also performed pointing out that the MR clutch presents shorter response times with high energy savings. The study carried out shows that the device is well suited to a vehicle with automatic or robotic or otherwise with very short response times but requires a control system for the starting the vehicle.
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EPIDEMIOLOGICAL STUDIES ON POSSIBLE LONG-TERM EFFECTS OF EXTREMELY LOW FREQUENCIES ELECTRICAL AND MAGNETIC FIELDS

2008

Settore MED/42 - Igiene Generale E ApplicataELF LONG-TERM EFFECTS MAGNETIC FIELDS.
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Axisymmetric simulations of magnetorotational core collapse: approximate inclusion of general relativistic effects

2006

We continue our investigations of the magnetorotational collapse of stellar cores discussing simulations performed with a modified Newtonian gravitational potential that mimics general relativistic effects. The approximate TOV potential used in our simulations catches several features of fully relativistic simulations quite well. It is able to correctly reproduce the behavior of models which show a qualitative change both of the dynamics and the gravitational wave signal when switching from Newtonian to fully relativistic simulations. If this is not the case, the Newtonian and the approximate TOV models differ quantitatively. The collapse proceeds to higher densities with the approximate TO…

Shock waveMagnetohydrodynamics (MHD)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGravitational wavesGravitational potentialNewtonian fluidDifferential rotationPhysicsGravitational waveAstrophysics (astro-ph)Astronomy and AstrophysicsMechanicsNuclear matterStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Magnetic fieldSupernovaeSpace and Planetary ScienceMagnetic fieldsMagnetohydrodynamics (MHD) ; Gravitational waves ; Stars ; Magnetic fields ; SupernovaeUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaRelativistic quantum chemistry:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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On the Origin of Asymmetries in Bilateral Supernova Remnants

2007

AIMS: We investigate whether the morphology of bilateral supernova remnants (BSNRs) observed in the radio band is determined mainly either by a non-uniform interstellar medium (ISM) or by a non-uniform ambient magnetic field. METHODS: We perform 3-D MHD simulations of a spherical SNR shock propagating through a magnetized ISM. Two cases of shock propagation are considered: 1) through a gradient of ambient density with a uniform ambient magnetic field; 2) through a homogeneous medium with a gradient of ambient magnetic field strength. From the simulations, we synthesize the synchrotron radio emission, making different assumptions about the details of acceleration and injection of relativisti…

Shock wavePhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsElectronAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadio spectrumMagnetic fieldShock (mechanics)Interstellar mediumSupernovaSpace and Planetary Sciencemagnetohydrodynamics (MHD) – shock waves – ISM: supernova remnants – ISM: magnetic fields –MagnetohydrodynamicsAstrophysics::Galaxy Astrophysics
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Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment

2018

Monthly notices of the Royal Astronomical Society 479(3), 4253 - 4270 (2018). doi:10.1093/mnras/sty1750

Shock waveshock wave010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesISM: magnetic field0103 physical sciencesRadiative transferAdiabatic process010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicssupernova remnants [ISM]magnetic fields [ISM]Astronomy and Astrophysicsshock wavesAstronomy and Astrophysic520Magnetic fieldSupernovaSpace and Planetary Scienceddc:520Oblique shockMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Probing the radio emission from air showers with polarization measurements

2014

The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially wit…

SignalsAstronomy01 natural sciencesElectric fieldComputational physicsCosmic-raysComposition energy spectra and interactionscosmic rayRadio wavePhysicsEarth's magnetic fieldHigh Energy Astrophysical Phenomena (astro-ph.HE)Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsPolarization (waves)Polarization (waves)BolometersThunderstormsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCAMPO MAGNÉTICOradio emissionRadio waveNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerComposition energy spectra and interactions; Solar electromagnetic emission; BolometersAstrophysics::High Energy Astrophysical Phenomenainfrared submillimeter wave microwave and radiowave receivers and detectorsFieldFOS: Physical sciencesPierre Auger Observatory ; air shower ; radio emissionRadiationMonte-carlo SimulationsOpticsElectric field0103 physical sciencesddc:530Pierre auger observatory010306 general physicsPulsesInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industrySolar electromagnetic emissionFísicaOpticsDetectorComputational physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerEarth's magnetic fieldMagnetic fieldExperimental High Energy PhysicsbusinessCodalema
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Nuclear Magnetic Resonance for Cultural Heritage

2007

Abstract Nuclear magnetic resonance (NMR) portable devices are now being used for nondestructive in situ analysis of water content, pore space structure and protective treatment performance in porous media in the field of cultural heritage. It is a standard procedure to invert T 1 and T 2 relaxation data of fully water-saturated samples to get “pore size” distributions, but the use of T 2 requires great caution. It is well known that dephasing effects due to water molecule diffusion in a magnetic field gradient can affect transverse relaxation data, even if the smallest experimentally available half echo time τ is used in Carr–Purcell–Meiboom–Gill experiments. When a portable single-sided N…

Single-sided NMR deviceGeologic SedimentsPORE SIZE DISTRIBUTIONSMagnetic Resonance SpectroscopyTime FactorsField (physics)Scale (ratio)Surface PropertiesSample (material)DiffusionDephasingBiomedical EngineeringBiophysicsInhomogeneous magnetic fieldsDiffusionNuclear magnetic resonanceRadiology Nuclear Medicine and imagingNMR SINGLE-SIDEDChemistryConstruction MaterialsRelaxation (NMR)WaterPOROUS MEDIANMRArchaeologyNMR relaxationNuclear magnetic resonance in porous mediaPorous mediaNMR relaxationSingle-sided NMR deviceInhomogeneous magnetic fieldsCultural heritageCULTURAL HERITAGEPorous mediumPorosity
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Mean Interplanetary Magnetic Field Measurement Using the ARGO-YBJ Experiment

2011

The sun blocks cosmic ray particles from outside the solar system, forming a detectable shadow in the sky map of cosmic rays detected by the ARGO-YBJ experiment in Tibet. Because the cosmic ray particles are positive charged, the magnetic field between the sun and the earth deflects them from straight trajectories and results in a shift of the shadow from the true location of the sun. Here we show that the shift measures the intensity of the field which is transported by the solar wind from the sun to the earth.

Solar SystemField (physics)media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmagnetic fieldCosmic rayHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Settore FIS/05 - Astronomia E AstrofisicaShadowAstrophysics::Solar and Stellar AstrophysicsInterplanetary magnetic fieldcosmic raySolar and Stellar Astrophysics (astro-ph.SR)media_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsCosmic Rays Gamma Sources Extended Air Showers Solar windMagnetic fieldSolar windAstrophysics - Solar and Stellar Astrophysicssolar windSpace and Planetary ScienceSkyPhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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The polarimetric and helioseismic imager on solar orbiter

2020

This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from outside the Sun-Earth line. It is the key instrument meant to address the top-level science question: How does the solar dynamo work and drive connections between the Sun and the heliosphere? SO/PHI will also play an important role in answering the other top-level science questions of Solar Orbiter, as well as hosting the potential of a rich return in further science. SO/PHI measures the Zeeman effect and the Doppler shift in the FeI 617.3nm spectral line. To this end, the instrument carries out narrow-band imaging…

Solar Telescope010504 meteorology & atmospheric sciencesphotosphere [Sun]FiltegramsHighly elliptical orbitFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionTelescopeOrbiterPhotospherelaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHelioseismologySolar dynamo010303 astronomy & astrophysicsSun: magnetic fieldsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesSun: helioseismologyPhysics[PHYS]Physics [physics]PhotosphereEllipsometrypolarimeters [Instrumentation]Spacecraftbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyinstrumentation: polarimetersSun: photosphereHeliosismologiaAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestechniques: polarimetricmagnetic fields [Sun]Space and Planetary Sciencetechniques: imaging spectroscopyAstrophysics of Galaxies (astro-ph.GA)Physics::Space PhysicsHelioseismologyAstrophysics::Earth and Planetary AstrophysicsbusinessAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HeliosphereEl·lipsometria
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A prospective new diagnostic technique for distinguishing eruptive and noneruptive active regions

2019

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). This work used the DiRAC@Durham facility managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). The equipment was funded by BEIS capital funding via STFC capital grants ST/P002293/1, ST/R002371/1, and ST/S002502/1, Durham University and STFC operations grant ST/R000832/1. DiRAC is part of the National e-Infrastructure. S.L.Y. would like to acknowledge STFC for sup…

Solar coronal mass ejections (310)010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsSolar activityT-NDASLibrary scienceFOS: Physical sciencesSpace weather (2037)Solar coronaSolar activity (1475)Solar flares (1496)01 natural sciencesSolar coronal mass ejectionsSolar corona (1483)0103 physical sciencesmedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsQB AstronomyEuropean union010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesmedia_commonQBPhysicsEuropean researchSolar active region magnetic fieldsAstronomy and AstrophysicsSolar active region magnetic fields (1975)Solar magnetic fields (1503)Solar active regionsSolar active regions (1974)QC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSolar flaresSpace and Planetary SciencePhysics::Space Physics
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