Search results for "Magnetic Field"

showing 10 items of 1488 documents

The intensity contrast of solar photospheric faculae and network elements : II. Evolution over the rising phase of solar cycle 23

2006

We studied the radiative properties of small magnetic elements (active region faculae and the network) during the rising phase of solar cycle 23 from 1996 to 2001, determining their contrasts as a function of heliocentric angle, magnetogram signal, and the solar cycle phase. We combined near-simultaneous full disk images of the line-of-sight magnetic field and photospheric continuum intensity provided by the MDI instrument on board the SOHO spacecraft. Sorting the magnetogram signal into different ranges allowed us to distinguish between the contrast of different magnetic structures. We find that the contrast center-to-limb variation (CLV) of these small magnetic elements is independent of …

:ASTRONOMÍA Y ASTROFÍSICA::Sistema solar [UNESCO]PlagesFOS: Physical sciencesSolar cycle 23AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAFaculaeMagnetogramSun activityRadiative transferAstrophysics::Solar and Stellar AstrophysicsPhysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Sistema solarSpacecraftbusiness.industryAstrophysics (astro-ph)SunContrast (statistics)Astronomy and AstrophysicsMagnetic fluxMagnetic fieldOn boardSun activity ; Faculae ; Plages ; Sun ; Magnetic fieldsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsAstrophysics::Earth and Planetary Astrophysicsbusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Probing the Effects of Strong Electromagnetic Fields with Charge-Dependent Directed Flow in Pb-Pb Collisions at the LHC

2020

The first measurement at the LHC of charge-dependent directed flow ($v_{1}$) relative to the spectator plane is presented for Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV. Results are reported for charged hadrons and $\rm D^{0}$ mesons for the transverse momentum intervals $p_{\rm T}>0.2$ GeV/$c$ and $3<p_{\rm T}<$ 6 GeV/$c$ in the 5-40% and 10-40% centrality classes, respectively. The difference between the positively and negatively charged hadron $v_{1}$ has a positive slope as a function of pseudorapidity $\eta$, ${\rm d}\Delta{v_1}/{\rm d}\eta=$[1.68 $\pm$ 0.49 (stat.) $\pm$ 0.41 (syst.)] $\times 10^{-4}$. The same measurement for $\rm D^{0}$ and $\rm\bar{D}{}^0$ mesons yields a p…

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]heavy ion: scatteringflow: charge dependenceHadronGeneral Physics and Astronomyhiukkasfysiikkanucl-exmeson: yield01 natural sciencesHeavy ion experimentsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)electromagnetic field: highPb-Pb at LHC; flow[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Charm (quantum number)Nuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentMAGNETIC-FIELD; QCDQuantum chromodynamicsPhysicshigh [electromagnetic field]PhysicsMAGNETIC-FIELDVDP::Kjerne- og elementærpartikkelfysikk: 4313. Good healthquark gluon plasmaddc:PRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]CERN LHC CollVDP::Nuclear and elementary particle physics: 431charge dependence [flow]Pseudorapidityflowhadron: charged particlehadron: chargeParticle Physics - Experimentyield [meson]QuarkMesonFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]transverse momentumPhysics and Astronomy(all)spectator114 Physical sciencesNuclear physicsscattering [heavy ion]0103 physical sciencesPb-Pb at LHCRapidityNuclear Physics - Experimentddc:5305020 GeV-cms/nucleoncharged particle [hadron]010306 general physicsNuclear Physicshep-excharge dependenceHigh Energy Physics::PhenomenologysensitivityQCDNATURAL SCIENCES. Physics.rapidityspin (kvanttimekaniikka)Quark–gluon plasmaHigh Energy Physics::Experimentstrong electromagnetic fields ; Pb-Pb Collisionsexperimental results
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Magnetically Driven Swirling Flow Guided by Steady Magnetic Field and Imposed Rotation

1998

:NATURAL SCIENCES::Physics::Condensed matter physics::Magnetism [Research Subject Categories]Magnetic fieldSwirling flowsMagnetohidrodinamikaDisertācijaMagnetohydrodynamicMagnētiskais lauks
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X-rays from accretion shocks in classical T Tauri stars: 2D MHD modeling and the role of local absorption

2013

AbstractIn classical T Tauri stars (CTTS) strong shocks are formed where the accretion funnel impacts with the denser stellar chromosphere. Although current models of accretion provide a plausible global picture of this process, some fundamental aspects are still unclear: the observed X-ray luminosity in accretion shocks is order of magnitudes lower than predicted; the observed density and temperature structures of the hot post-shock region are puzzling and still unexplained by models.To address these issues we performed 2D MHD simulations describing an accretion stream impacting onto the chromosphere of a CTTS, exploring different configurations and strengths of the magnetic field. From th…

Accretion MHD Stars: pre-main sequence X-rays: starsPhysicsbusiness.product_categoryAstronomyAstronomy and AstrophysicsAstrophysicsViewing angleAccretion (astrophysics)Spectral lineMagnetic fieldT Tauri starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Sciencepre-main sequence X-rays: stars [Accretion MHD Stars]FunnelMagnetohydrodynamicsbusinessChromosphereProceedings of the International Astronomical Union
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Timing of the accreting millisecond pulsar IGR J17591-2342: evidence of spin-down during accretion

2020

We report on the phase-coherent timing analysis of the accreting millisecond X-ray pulsar IGR J17591-2342, using Neutron Star Interior Composition Explorer (NICER) data taken during the outburst of the source between 2018 August 15 and 2018 October 17. We obtain an updated orbital solution of the binary system. We investigate the evolution of the neutron star spin frequency during the outburst, reporting a refined estimate of the spin frequency and the first estimate of the spin frequency derivative ($\dot{\nu} \sim -7\times 10^{-14}$ Hz s$^{-1}$), confirmed independently from the modelling of the fundamental frequency and its first harmonic. We further investigate the evolution of the X-ra…

AccretionIGR J17591-2342Astrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesaccretion accretion disc stars: neutron X-rays: binaries010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Neutron Star Interior Composition Explorer010308 nuclear & particles physicsAstronomy and Astrophysicsneutron [Stars]Accretion (astrophysics)Magnetic fieldNeutron starAmplitudeSpace and Planetary Sciencebinaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsAccretion discAstrophysics - High Energy Astrophysical Phenomena
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First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon

2021

Full list of authors: Akiyama, Kazunori; Algaba, Juan Carlos; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Chesler, Paul M.; Cho, Ilje; Christian, Pierre; Conway, John E.…

AccretionKinoAstrophysics - astrophysics of galaxiesAstrophysics::High Energy Astrophysical PhenomenaAstronomy19641347FOS: Physical sciences479Astrophysics::Cosmology and Extragalactic AstrophysicsF500870126101 natural sciences7. Clean energyAstrophysics - high energy astrophysical phenomena994MagnetohydrodynamicsRelativistic jets 14 162 479 870 886 994 1964 1261 1278 1335 1347 13900103 physical sciencesJetsPolarimetryRadiative transferPlasma astrophysicsRadio jets010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics162High Energy Astrophysical Phenomena (astro-ph.HE)Physics1278Event horizons1335010308 nuclear & particles physicsBlack holesChatterjee14886Astronomy and AstrophysicsCreative commons139013. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Magnetic fieldsKerr black holesFish <Actinopterygii>Relativistic jetsHumanities
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Effects of an earth-strength magnetic field on pineal melatonin synthesis in pigeons

1987

Acetylserotonin O-Methyltransferasemedicine.medical_specialtyArylamine N-AcetyltransferaseChamp magnetiqueMethyltransferasesGeneral MedicineBiologyPineal GlandMagnetic fieldPineal melatoninMelatoninMagneticsPineal glandmedicine.anatomical_structureEndocrinologyAcetyltransferasesAcetylserotonin O-methyltransferaseInternal medicinemedicineAnimalsColumbidaeEcology Evolution Behavior and SystematicsMelatoninmedicine.drugNaturwissenschaften
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Exchange stiffness in the Co2FeSi Heusler compound

2009

Using Brillouin light scattering spectroscopy, we determine the spin-wave exchange stiffness D and the exchange constant A for thin films of the full Heusler compound Co2FeSi prepared by pulsed laser deposition. The thermal spin-wave spectra were measured in various magnetic fields, for different transferred spin-wave momenta, and for different film thicknesses. Fitting the observed spin-wave frequencies, we find an extraordinarily large value of

Acoustics and UltrasonicsCondensed matter physicsbusiness.industryChemistryIntermetallicengineering.materialCondensed Matter PhysicsHeusler compoundSpectral lineSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsPulsed laser depositionMagnetic fieldBrillouin zoneCondensed Matter::Materials ScienceOpticsSpin waveengineeringCondensed Matter::Strongly Correlated ElectronsThin filmbusinessJournal of Physics D: Applied Physics
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Coupling hydrodynamics and radiation calculations for star-jet interactions in active galactic nuclei

2016

Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Because of the complexity of jet-star interactions, the properties of the resulting emission are closely linked to those of the emitting flows. Aims. We simulate the interaction between a stellar wind and a relativistic extragalactic jet and use the hydrodynamic results to compute the non-thermal emission under different conditions. Methods. We performed relativistic axisymmetric hydrodynamical simulations of a relativistic jet interacting with a supersonic, non-relativistic stellar wind. We computed the corresponding streamlines out of the simulation results and calculated the injection, evolut…

Active galactic nucleusElectromagnetic spectrumAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsElectronAstrophysicsRadiation7. Clean energy01 natural sciencessymbols.namesake0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHidrodinàmica010308 nuclear & particles physicsAstronomy and AstrophysicsStarsEstelsMagnetic fieldParticle accelerationStars13. Climate actionSpace and Planetary ScienceHydrodynamicssymbolsDoppler effectAstronomy &amp; Astrophysics
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Magnetic In-Tube Solid Phase Microextraction

2012

We report a new in-tube solid phase microextraction approach named magnetic in-tube solid phase microextraction, magnetic-IT-SPME. Magnetic-IT-SPME has been developed, taking advantage of magnetic microfluidic principles with the aim to improve extraction efficiency of IT-SPME systems. First, a magnetic hybrid material formed by Fe(3)O(4) nanoparticles supported on SiO(2) was synthesized and immobilized in the surface of a bared fused silica capillary column to obtain a magnetic adsorbent extraction phase. The capillary column was placed inside a magnetic coil that allowed the application of a variable magnetic field. Acetylsalicylic acid, acetaminophen, atenolol, diclofenac, and ibuprofen …

AdsorptionChromatographyChemistryElectromagnetic coilPhase (matter)Extraction (chemistry)MicrofluidicsAnalytical chemistrySolid phase extractionSolid-phase microextractionAnalytical ChemistryMagnetic fieldAnalytical Chemistry
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