Search results for "MAGNETIC FIELD"

showing 10 items of 1488 documents

Thermodiffusion anisotropy under a magnetic field in ionic liquid-based ferrofluids

2021

International audience; Ferrofluids based on maghemite nanoparticles (NPs), typically 10 nm in diameter, are dispersed in an ionic liquid (1-ethyl 3-methylimidazolium bistriflimide - EMIM-TFSI). The average interparticle interaction is found to be repulsive by small angle scattering of X-rays and of neutrons, with a second virial coefficient A2 = 7.3. A moderately concentrated sample at Φ = 5.95 vol% is probed by forced Rayleigh scattering under an applied magnetic field (up to H = 100 kA m-1) from room temperature up to T = 460 K. Irrespective of the values of H and T, the NPs in this study are always found to migrate towards the cold region. The in-field anisotropy of the mass diffusion c…

[PHYS]Physics [physics]FerrofluidMaterials scienceCondensed matter physics02 engineering and technologyGeneral Chemistry010402 general chemistry021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciences0104 chemical sciencesMagnetic fieldchemistry.chemical_compoundDipolechemistryVirial coefficientIonic liquidBistriflimideSmall-angle scattering0210 nano-technologyAnisotropySoft Matter
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Nonlinear electrostatic oscillations in a cold magnetized electron-positron plasma

2017

We study the spatio-temporal evolution of the nonlinear electrostatic oscillations in a cold magnetized electron-positron (e-p) plasma using both analytics and simulations. Using a perturbative method we demonstrate that the nonlinear solutions change significantly when a pure electrostatic mode is excited at the linear level instead of a mixed upper-hybrid and zero-frequency mode that is considered in a recent study. The pure electrostatic oscillations undergo phase mixing nonlinearly. However, the presence of the magnetic field significantly delays the phase-mixing compared to that observed in the corresponding unmagnetized plasma. Using 1D PIC simulations we then analyze the damping of t…

[PHYS]Physics [physics]PhysicsFOS: Physical sciencesElectronPlasmaCondensed Matter PhysicsPlasma oscillationLower hybrid oscillation01 natural sciencesPhysics - Plasma Physics010305 fluids & plasmasMagnetic fieldPlasma Physics (physics.plasm-ph)Two-stream instabilityPhysics::Plasma Physics[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Upper hybrid oscillation0103 physical sciencesAstrophysical plasmaAtomic physics010306 general physicsComputingMilieux_MISCELLANEOUSPhysics of Plasmas
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Optical force rectifiers based on PT-symmetric metasurfaces

2018

We introduce here the concept of optical force rectifier based on parity-time symmetric metasurfaces. Directly linked to the properties of non-Hermitian systems engineered by balanced loss and gain constituents, we show that light can exert asymmetric pulling or pushing forces on metasurfaces depending on the direction of the impinging light. This generates a complete force rectification in the vicinity of the exceptional point. Our findings have the potential to spark the design of applications in optical manipulation where the forces, strictly speaking, act unidirectionally. R.A. and B.G. would like to acknowledge financial support from the Max Planck Society. J.C. acknowledges the suppor…

[SPI.ACOU]Engineering Sciences [physics]/Acoustics [physics.class-ph]PhysicsElectromagnetic field calculationsMaterialesExceptional pointbusiness.industryOptical forceFísicaPhysics::Optics02 engineering and technology021001 nanoscience & nanotechnology01 natural sciences[SPI.MAT]Engineering Sciences [physics]/MaterialsRectifierRectificationMetamaterials0103 physical sciencesSpark (mathematics)OptoelectronicsElectrónica[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics010306 general physics0210 nano-technologybusinessPhysical Review B
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The magnetosphere of the close accreting PMS binary V4046 Sgr

2013

V4046 Sagittarii AB is a close short-period classical T Tauri binary. It is a circularised and synchronised system accreting from a circumbinary disk. In 2009 it was observed as part of a coordinated program involving near-simultaneous spectropolarimetric observations with ESPaDOnS at the Canada-France-Hawai'i Telescope and high-resolution X-ray observations with XMM-Newton. Magnetic maps of each star were derived from Zeeman-Doppler imaging. After briefly highlighting the most significant observational findings, we present a preliminary 3D model of the binary magnetosphere constructed from the magnetic maps using a newly developed binary magnetic field extrapolation code. The large-scale f…

accretion young starsQC1-999Astrophysics::High Energy Astrophysical PhenomenaMagnetosphereBinary numberFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionTelescopeSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Physics010308 nuclear & particles physicsPhysicsMagnetic fieldDipoleStarsT Tauri starQC PhysicsAstrophysics - Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsCircumbinary planet
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VLBA polarimetric monitoring of 3C 111

2018

Context. While studies of large samples of jets of active galactic nuclei (AGN) are important in order to establish a global picture, dedicated single-source studies are an invaluable tool for probing crucial processes within jets on parsec scales. These processes involve in particular the formation and geometry of the jet magnetic field as well as the flow itself. Aims. We aim to better understand the dynamics within relativistic magneto-hydrodynamical flows in the extreme environment and close vicinity of supermassive black holes. Methods. We analyze the peculiar radio galaxy 3C 111, for which long-Term polarimetric observations are available. We make use of the high spatial resolution of…

active [Galaxies]Radio galaxyAstrophysics::High Energy Astrophysical PhenomenaeducationFOS: Physical sciencesAstrophysicsgalaxies [Radio continuum]Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesgalaxies: individual: 3C 111Coincident0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsSupermassive black holepolarizationGalaxies: magnetic fields010308 nuclear & particles physicsmagnetic fields [Galaxies]Astronomy and AstrophysicsGalaxies: activePolarization (waves)Astrophysics - Astrophysics of GalaxiesMonitoring programMagnetic fieldTransverse planeindividual: 3C 111 [galaxies]Space and Planetary ScienceGalaxies: jetsBrightness temperatureAstrophysics of Galaxies (astro-ph.GA)jets [Galaxies]
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Extremely low frequency electromagnetic fields (ELF-EMFs) induce in vitro angiogenesis process in human endothelial cells.

2008

Effects of extremely low frequency (ELF) electromagnetic fields (EMFs) on activation of angiogenesis were analysed using cultured umbilical human vein endothelial cells (HUVECs). The cultures were exposed to a sinusoidal EMF to intensity of 1 mT, 50 Hz for up to 12 h. EMFs increased the degree of endothelial cell proliferation and tubule formation, coupled by an acceleration in the process of wound healing. Since this process is physiologically accompanied by a large modification in the structural organization of actin and focal adhesions, we analyzed the rearrangement of some cytoskeleton elements demonstrating a major reorganization of the fibres and of the focal adhesion complexes after …

animal structuresCytoskeleton organizationPhysiologyAngiogenesisBiophysicsNeovascularization PhysiologicBiologyRadiation DosageFocal adhesionElectromagnetic FieldsEndothelial cellElectricityHumansRadiology Nuclear Medicine and imagingTherapeutic angiogenesisCytoskeletonCells CulturedEndothelial CellsDose-Response Relationship RadiationGeneral MedicineCell biologyEndothelial stem cellAngiogenesiSignal transductionWound healingExtremely low frequency electromagnetic fieldsBioelectromagnetics
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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Contribution of observed multi frequency spectrum of Alfvén waves to coronal heating

2019

Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves carry enough energy to maintain the thermal structure of the solar corona, it is not clear whether such energy can be efficiently and effectively converted into heating. Phase-mixing of Alfvén waves is considered a candidate mechanism, as it can develop transverse gradient where magnetic energy can be converted into thermal energy. However, phase-mixing is a process that crucially depends on the amplitude and period of the transverse oscillations, and only recently have we obtained a complete measurement of the power spectrum for transverse oscillations in the corona. Aims. We aim to investig…

atmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]T-NDASContext (language use)Astrophysics01 natural sciences03 medical and health sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsSun: oscillationsQASun: magnetic fields010303 astronomy & astrophysicsQCQB030304 developmental biologyPhysics0303 health sciencesMagnetic energySun: coronaoscillations [Sun]Spectral densityAstronomy and AstrophysicsTransverse waveCoronal loopComputational physicsTransverse planeQC PhysicsAmplitudemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsSun: atmosphereAstronomy & Astrophysics
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Solar Coronal Loops Associated with Small-scale Mixed Polarity Surface Magnetic Fields

2017

L. P. Chitta et. al.

atmosphere [Sun]corona [Sun]010504 meteorology & atmospheric sciencesphotosphere [Sun]Polarity (physics)FOS: Physical sciencesFluxAstrophysics01 natural sciencesAtmosphereObservatory0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsPhotosphereSun: coronaSun: photosphereAstronomy and AstrophysicsCoronal loopMagnetic fluxMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsSun: atmosphere
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ELEKTROMAGNĒTISKI IETEKMĒTU HIDRODINAMISKO PROCESU EKSPERIMENTĀLI PĒTĪJUMI ŠĶIDRU METĀLU NOSLĒGTOS TILPUMOS

2014

Elektroniskā versija nesatur pielikumus

augstfrekvences magnētiskais lauksFizika materiālzinātne matemātika un statistikaŠķidrumu un gāzu mehānikamagnetic fieldfluid dynamicshigh frequencyšķidri metāliFizika astronomija un mehānikathermoelectricityMagnetohydrodynamicstermokapilārā konvekcijaMagnetohidrodinamikathermocapillary convectiontermoelektrībaFizikaliquid metals
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