Search results for "MAGNETIC FIELD"

showing 10 items of 1488 documents

New view of the corona of classical T Tauri stars: Effects of flaring activity in circumstellar disks

2019

Classical T Tauri stars (CTTSs) are young low-mass stellar objects accreting mass from their circumstellar disks. They are characterized by high levels of coronal activity as revealed by X-ray observations. This activity may affect the disk stability and the circumstellar environment. Here we investigate if an intense coronal activity due to flares occurring close to the accretion disk may perturb the inner disk stability, disrupt the inner part of the disk and, possibly, trigger accretion phenomena with rates comparable with those observed. We model a magnetized protostar surrounded by an accretion disk through 3D magnetohydrodinamic simulations. We explore cases characterized by a dipole …

Young stellar objectStars: flareAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesX-rays: starsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsaccretion accretion disk01 natural sciencesmagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferProtostarAstrophysics::Solar and Stellar AstrophysicsStars: coronae010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]accretion disksStellar magnetic fieldAstronomy and Astrophysics[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]CoronaAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsHeat flux13. Climate actionSpace and Planetary ScienceStars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysics
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SELECTIVE AMPLIFICATION OF NARROW RESONANCE FORMED IN TRANSMISSION SPECTRUM OF Rb NANO-CELL IN MAGNETIC FIELD

2012

Recently it was shown that "λ-Zeeman Technique" (λ-ZT) is a convenient tool to study individual transitions between the Zeeman sublevels of hyperfine levels in an external magnetic field. λ-ZT is based on resonant transmission spectrum of nanometric thin cell (NTC) of thickness L = λ, where λ is the resonant wavelength 794 nm for Rb D1 line. Narrow velocity selective optical pumping (VSOP) resonances in the transmission spectrum of the NTC are split into several components in a magnetic field. Examination of VSOP resonances allows one to identify and investigate an atomic transition in the range of magnetic fields 10 - 5000 G. Here we present a new method for selective addressing of VSOP r…

Zeeman effect[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]ChemistryRb atomResonancemagnetic fieldVSOP01 natural sciencesnarrow optical resonanceMagnetic field010309 opticsOptical pumpingWavelengthsymbols.namesake[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencessymbolsPhysics::Atomic PhysicsAtomic physics010306 general physicsHyperfine structureLine (formation)nano-metric thin cell
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Polarization transfer via field sweeping in parahydrogen-enhanced nuclear magnetic resonance.

2019

<div><br></div><div><table><tr><td>We show that in a spin system of two magnetically inequivalent protons coupled to a heteronucleus such as 13C, an adiabatic magnetic field sweep, passing through zero field, transfers proton singlet order into magnetization of the coupled heteronucleus. This effect is potentially useful in parahydrogen-enhanced nuclear magnetic resonance, and is demonstrated on singlet-hyperpolarized [1-13C]maleic acid, which is prepared via the reaction between [1-13C]acetylene dicarboxylic acid and para-enriched hydrogen gas. The magnetic field sweeps are of microtesla amplitudes, and have durations on the order of seconds. We sh…

Zero field NMRMaterials science010304 chemical physicsMaleic acidHydrogenField (physics)ProtonGeneral Physics and Astronomychemistry.chemical_element010402 general chemistryPolarization (waves)Spin isomers of hydrogen01 natural sciences0104 chemical sciencesMagnetic fieldchemistry.chemical_compoundMagnetizationNuclear magnetic resonancechemistry0103 physical sciencesSinglet statePhysical and Theoretical ChemistryThe Journal of chemical physics
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Hyperfine Paschen-Back regime realized in Rb nanocell

2012

A simple and efficient scheme based on one-dimensional nanometric thin cell filled with Rb and strong permanent ring magnets allowed direct observation of hyperfine Paschen-Back regime on D1 line in 0.5 - 0.7 T magnetic field. Experimental results are perfectly consistent with the theory. In particular, with sigma+ laser excitation, the slopes of B-field dependence of frequency shift for all the 10 individual transitions of 85,87Rb are the same and equal to 18.6 MHz/mT. Possible applications for magnetometry with submicron spatial resolution and tunable atomic frequency references are discussed.

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Atomic Physics (physics.atom-ph)MagnetometerFOS: Physical sciences01 natural sciencesPhysics - Atomic Physicslaw.invention010309 optics[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesOCIS codes: 020.1335 300.6360010306 general physicsHyperfine structure[PHYS.QPHY] Physics [physics]/Quantum Physics [quant-ph]Line (formation)PhysicsNanocellLaserRubidiumAtomic and Molecular Physics and OpticsMagnetic fieldnanocellMagnetHyperfineAtomic physicsPaschen-BackExcitation
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Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

2011

We present the results of an analysis of data recorded at the Pierre Auger Observatory in which we search for groups of directionally-aligned events (or ‘multiplets’) which exhibit a correlation between arrival direc- tion and the inverse of the energy. These signatures are expected from sets of events coming from the same source after having been deflected by intervening coherent magnetic fields. The observation of several events from the same source would open the possibility to accurately reconstruct the position of the source and also measure the integral of the component of the magnetic field orthogonal to the trajectory of the cos- mic rays. We describe the largest multiplets found an…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Field (physics)Astronomyultra-high energy cosmic rays; Pierre Auger Observatory; arrival directionsFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesCosmic RayAugerPosition (vector)0103 physical sciencesFIELDPierre auger observatory010303 astronomy & astrophysicsUltra-high energy cosmic rayDETECTORCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysicsArrival directions010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsIsotropyFísicaAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysMagnetic fieldExperimental High Energy PhysicsData analysisComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSArrival directionUltra-High Energy Cosmic Ray
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Results of a self-triggered prototype system for radio-detection of extensive air showers at the Pierre Auger Observatory

2012

We describe the experimental setup and the results of RAuger, a small radio-antenna array, consisting of three fully autonomous and self-triggered radio-detection stations, installed close to the center of the Surface Detector (SD) of the Pierre Auger Observatory in Argentina. The setup has been designed for the detection of the electric field strength of air showers initiated by ultra-high energy cosmic rays, without using an auxiliary trigger from another detection system. Installed in December 2006, RAuger was terminated in May 2010 after 65 registered coincidences with the SD. The sky map in local angular coordinates (i.e., zenith and azimuth angles) of these events reveals a strong azi…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]self-triggergeomagnetic effect.media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray01 natural sciencesElectric field0103 physical sciencesextensive air showers010306 general physicsCosmic raysInstrumentationMathematical PhysicsZenithmedia_commonPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsCosmic rayextensive air showerAntennas; Large detector systems for particle and astroparticle physics3. Good healthComputational physicsAzimuthEarth's magnetic fieldSkyAntennasAstrophysics - High Energy Astrophysical Phenomenaradio-detection
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The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory

2011

We present a comprehensive study of the influence of the geomagnetic field on the energy estimation of extensive air showers with a zenith angle smaller than $60^\circ$, detected at the Pierre Auger Observatory. The geomagnetic field induces an azimuthal modulation of the estimated energy of cosmic rays up to the ~2% level at large zenith angles. We present a method to account for this modulation of the reconstructed energy. We analyse the effect of the modulation on large scale anisotropy searches in the arrival direction distributions of cosmic rays. At a given energy, the geomagnetic effect is shown to induce a pseudo-dipolar pattern at the percent level in the declination distribution t…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentCosmic rayAstrophysicsultra high energy cosmic raysEXTENSIVE AIR-SHOWERS01 natural sciencesDeclinationultra high energy cosmic ray0103 physical sciencescosmic rays detectors; cosmic ray experiments; ultra high energy cosmic rayscosmic rays detectorAnisotropyInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsZenithParticle detectors.Pierre Auger ObservatoryPhysics010308 nuclear & particles physicsPhysicsOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AzimuthMODELEarth's magnetic fieldPhysics::Space PhysicsLarge detector systems for particle and astroparticle physicARRAYFísica nuclearcosmic rays detectorscosmic ray experimentsAstrophysics - Instrumentation and Methods for AstrophysicsEnergy (signal processing)Cherenkov detectorJournal of Cosmology and Astroparticle Physics
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Plasma diagnostic tools for ECR ion sources : What can we learn from these experiments for the next generation sources

2019

International audience; The order-of-magnitude performance leaps of ECR ion sources over the past decades result from improvements to the magnetic plasma confinement, increases in the microwave heating frequency, and techniques to stabilize the plasma at high densities. Parallel to the technical development of the ion sources themselves, significant effort has been directed into the development of their plasma diagnostic tools. We review the recent results of Electron Cyclotron Resonance Ion Source (ECRIS) plasma diagnostics highlighting a number of selected examples of plasma density, electron energy distribution, and ion confinement time measurements, obtained mostly with the second-gener…

[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Solenoidmagnetic fieldshiukkaskiihdyttimetplasmafysiikka7. Clean energy01 natural sciencesbremsstrahlungElectron cyclotron resonance010305 fluids & plasmasIonoptical emission spectroscopySuperposition principleion sourcesPhysics::Plasma Physics0103 physical sciencesInstrumentation010302 applied physicsPhysics[PHYS]Physics [physics]plasma confinementplasma properties and parametersplasma diagnosticssyklotronitplasma heatingPlasmaIon sourceComputational physicsMagnetic fieldPlasma diagnostics
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Swarming of micron-sized hematite cubes in a rotating magnetic field -- Experiments

2020

Energy input by under-field rotation of particles drives the systems to emergent non-equilibrium states. Here we investigate the suspension of rotating magnetic cubes. Micron-sized hematite cubes are synthesized and observed microscopically. When exposed to a rotating magnetic field, they form rotating swarms that interact with each other like liquid droplets. We describe the swarming behaviour and its limits and characterize swarm size and angular velocity dependence on magnetic field strength and frequency. A quantitative agreement with a theoretical model is found for the angular velocity of swarms as a function of field frequency. It is interesting to note that hematite particles with p…

[PHYS]Physics [physics]010302 applied physicsRotating magnetic fieldMaterials scienceSwarming (honey bee)Swarm behaviourFOS: Physical sciencesAngular velocity02 engineering and technologyField frequencyHematiteCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesMolecular physicsElectronic Optical and Magnetic MaterialsMagnetic fieldvisual_art0103 physical sciencesvisual_art.visual_art_medium[CHIM]Chemical SciencesMagnetic nanoparticlesSoft Condensed Matter (cond-mat.soft)0210 nano-technology
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Field-Induced Slow Magnetic Relaxation in a Six-Coordinate Mononuclear Cobalt(II) Complex with a Positive Anisotropy

2012

International audience; The novel mononuclear Co(II) complex cis-[Co-II(dmphen)(2)(NCS)(2)]center dot 0.25EtOH (1) (dmphen = 2,9-dimethyl-1,10-phenanthroline) features a highly rhombically distorted octahedral environment that is responsible for the strong positive axial and rhombic magnetic anisotropy of the high-spin Co-II ion (D = +98 cm(-1) and E = +8.4 cm(-1)). Slow magnetic relaxation effects were observed for 1 in the presence of a dc magnetic field, constituting the first example of field-induced single-molecule magnet behavior in a mononuclear six-coordinate Co(II) complex with a transverse anisotropy energy barrier.

[PHYS]Physics [physics]Anisotropy energy010405 organic chemistrychemistry.chemical_elementGeneral Chemistry010402 general chemistry01 natural sciencesBiochemistryCatalysis3. Good health0104 chemical sciencesMagnetic fieldIonCrystallographyMagnetic anisotropyColloid and Surface ChemistryNuclear magnetic resonancechemistryOctahedronMagnetAnisotropyCobalt
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