Search results for " polar"

showing 10 items of 1091 documents

Power monitoring in dielectric-loaded surface plasmon-polariton waveguides

2011

We report on propagating mode power monitoring in dielectric-loaded surface plasmon-polariton waveguides (DLSPPWs) by measuring the resistance of gold stripes supporting the DLSPPW mode propagation. Inevitable absorption of the DLSPPW mode in metal causes an increase in the stripe temperature and, thereby, in its resistance whose variations are monitored with an external Wheatstone bridge being accurately balanced in the absence of radiation in a waveguide. The investigated waveguide configuration consists of a 1-µm-thick and 10-µm-wide polymer ridges tapered laterally to a 1-µm-wide ridge placed on a 50-nm-thin and 4-µm-wide gold stripe, all supported by a magnesium fluoride substrate. Usi…

Magnesium fluorideMaterials scienceWheatstone bridgebusiness.industrySurface plasmonPhotonic integrated circuitBiasingSurface plasmon polaritonAtomic and Molecular Physics and Opticslaw.inventionchemistry.chemical_compoundOpticschemistrylawbusinessAbsorption (electromagnetic radiation)Waveguide
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Fiber-coupled dielectric-loaded plasmonic waveguides.

2010

Fiber in- and out-coupling of radiation guided by dielectric-loaded surface plasmon-polariton waveguides (DLSPPWs) is realized using intermediate tapered dielectric waveguides. The waveguide structures fabricated by large-scale UV-lithography consist of 1-microm-thick polymer ridges tapered from 10-microm-wide ridges deposited directly on a magnesium fluoride substrate to 1-microm-wide ridges placed on a 50-nm-thick and 100-microm-wide gold stripe. Using fiber-to-fiber transmission measurements at telecom wavelengths, the performance of straight and bent DLSPPWs is characterized demonstrating the overall insertion loss below 24 dB, half of which is attributed to the DLSPPW loss of propagati…

Magnesium fluorideMaterials sciencebusiness.industrySurface plasmonPhotonic integrated circuitSubstrate (electronics)DielectricSurface plasmon polaritonAtomic and Molecular Physics and Opticslaw.inventionchemistry.chemical_compoundOpticschemistrylawInsertion lossbusinessWaveguideOptics express
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Precise measurement of 1H 90° pulse in solid-state NMR spectroscopy for complex and heterogeneous molecular systems

2007

The 90 degrees pulse calibration is essential in NMR spectroscopy to prevent artefacts in the liquid state or to enhance cross-polarization efficiency in the solid state. We verified pulse-angle (PA) errors due to circuit impedances in solid-state NMR and suggested a possible solution to prevent the inconvenience of PA errors. The classic pulse sequences used to calibrate (1)H 90 degrees pulse lengths by direct detection of protons or by cross-polarization were modified in order to replace single (1)H pulses with (1)H pulse trains. Pulse trains were found to decrease the effect of PA imperfections in the calibration of basic pulses (i.e. 90 degrees and 180 degrees ) for a number of organic …

Magnetic Resonance SpectroscopyMagic angleChemistrySettore AGR/13 - Chimica AgrariaAnalytical chemistryReproducibility of ResultsNuclear magnetic resonance spectroscopyBiochemistryAnalytical ChemistryPulse (physics)Liquid stateSolid-state nuclear magnetic resonanceCalibrationCross polarization magic angle spinning NMR 1H 90° pulse Pulse calibration Circuit impedance Complex molecular systemsCalibrationSpectroscopyElectrical impedanceAnalytical and Bioanalytical Chemistry
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Water dynamics and its role in structural hysteresis of dissolved organic matter

2016

Knowledge of structural dynamics of dissolved organic matter (DOM) is of paramount importance for understanding DOM stability and role in the fate of solubilized organic and inorganic compounds (e.g., nutrients and pollutants), either in soils or aquatic systems. In this study, fast field cycling (FFC) (1)H NMR relaxometry was applied to elucidate structural dynamics of terrestrial DOM, represented by two structurally contrasting DOM models such as Suwanee River (SRFA) and Pahokee peat (PPFA) fulvic acids purchased by the International Humic Substance Society. Measurement of NMR relaxation rate of water protons in heating-cooling cycles revealed structural hysteresis in both fulvic acids. I…

Magnetic Resonance SpectroscopyrelaxometrySettore AGR/13 - Chimica Agraria010501 environmental sciences01 natural scienceshumic substanceSoilRiversDissolved organic carbonEnvironmental ChemistryReactivity (chemistry)Benzopyrans0105 earth and related environmental sciencesChemistryHydrogen bondwater histeresiChemical polarityTemperatureSoil chemistryWaterHydrogen Bonding04 agricultural and veterinary sciencesGeneral ChemistryNuclear magnetic resonance spectroscopyEnvironmental chemistrySoil water040103 agronomy & agricultureProton NMR0401 agriculture forestry and fisheriesHydrophobic and Hydrophilic Interactions
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Photoinduced magnetization wave in diluted magnetic semiconductors

2006

We derive an evolutional equation incorporating the processes of spin-polarization transfer from an electron to a magnetic ion subsystem of a diluted magnetic semiconductor along with spin-lattice relaxation and spatial spin diffusion. Above equation has been obtained for nonequilibrium magnetization due to exchange scattering of photoexcited charge carriers by magnetic ions. We show that the mechanism of a band gap narrowing due to exchange scattering requires relatively low optical power to reach an optical bistability for pump frequency range close to crystal band gap. In a bulk crystal, only relatively small local area with essential magnetization enhancement can absorb optical power, t…

Magnetic anisotropyMagnetizationCondensed matter physicsSpin polarizationMagnetismBand gapChemistryRelaxation (NMR)Magnetic semiconductorOrbital magnetizationSPIE Proceedings
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Optical magnetic circular dichroism in threshold photoemission from a magnetite thin film

2011

Threshold photoemission excited by polarization-modulated ultraviolet femtosecond laser light is exploited for phase-sensitive detection of magnetic circular dichroism (MCD) for a magnetite thin film. Magnetite (Fe(3)O(4)) shows a magnetic circular dichroism of ∼(4.5 ± 0.3) × 10(-3) for perpendicularly incident circularly polarized light and a magnetization vector switched parallel and antiparallel to the helicity vector by an external magnetic field. The asymmetry in threshold photoemission is discussed in comparison to the magneto-optical Kerr effect. The optical MCD contrast in threshold photoemission will provide a basis for future laboratory photoemission studies on magnetic surfaces.

Magnetic circular dichroismChemistryInverse photoemission spectroscopyAnalytical chemistryPhysics::OpticsAngle-resolved photoemission spectroscopyCondensed Matter PhysicsMolecular physicsMagnetic fieldCondensed Matter::Materials ScienceMagnetizationX-ray magnetic circular dichroismCondensed Matter::SuperconductivityVibrational circular dichroismGeneral Materials ScienceCircular polarizationJournal of Physics: Condensed Matter
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Spin orbit torque switching in Ta/CoFeB/MgO without longitudinal fields

2015

Intense investigations are carried out on novel magnetic materials systems with perpendicular magnetic anisotropy (PMA), where new spin-orbit effects occur due to structural inversion asymmetry (SIA). So called spin-orbit torques (SOTs), have been observed for the first time in PMA nano-structures with SIA, when an electric current is injected [1-3], leading to ultra-efficient current-induced domain wall motion and current-induced magnetization switching [2,3].

MagnetizationMagnetic anisotropyMaterials scienceMagnetic domainCondensed matter physicsSpin polarizationDemagnetizing fieldMagnetic particle inspectionSingle domainMagnetic dipole2015 IEEE Magnetics Conference (INTERMAG)
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First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-correlation Analysis

2019

The determination of the speed of Coronal Mass Ejections (CMEs) is usually done by tracking brighter features (such as the CME front and core) in visible light coronagraphic images and by deriving unidimensional profiles of the CME speed as a function of altitude or time. Nevertheless, CMEs are usually characterized by the presence of significant density inhomogeneities propagating outward with different radial and latitudinal projected speeds, resulting in a complex evolution eventually forming the Interplanetary CME. In this work, we demonstrate for the first time how coronagraphic image sequences can be analyzed with cross-correlation technique to derive 2D maps of the almost instantaneo…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesDistribution (number theory)Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicspolarimetric [Techniques]magnetohydrodynamics (MHD)01 natural sciences0103 physical sciencesCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysicsmedia_common.cataloged_instanceEuropean uniondata analysis [Methods]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QCQB0105 earth and related environmental sciencesmedia_commonPhysicsUV radiation [Sun]Horizon (archaeology)Cross correlation analysisDASAstronomy and AstrophysicsSun: UV radiationmethods: data analysiscoronal mass ejections (CMEs) [Sun]techniques: polarimetricQC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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A new MHD-assisted Stokes inversion technique

2016

©2017 The American Astronomical Society. All rights reserved. We present a new method of Stokes inversion of spectropolarimetric data and evaluate it by taking the example of a Sunrise/IMaX observation. An archive of synthetic Stokes profiles is obtained by the spectral synthesis of state-of-the-art magnetohydrodynamics (MHD) simulations and a realistic degradation to the level of the observed data. The definition of a merit function allows the archive to be searched for the synthetic Stokes profiles that best match the observed profiles. In contrast to traditional Stokes inversion codes, which solve the Unno–Rachkovsky equations for the polarized radiative transfer numerically and fit the …

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesphotosphere [Sun]FOS: Physical sciencesTechniques: spectroscopicAstrophysicspolarimetric [Techniques]01 natural sciencesspectroscopic [Techniques]0103 physical sciencesMerit functionRadiative transferInitial value problemAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsRelaxation processTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsInversion (meteorology)Computational physicsmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSolar timeMagnetohydrodynamics
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Accretion disk coronae of intermediate polar cataclysmic variables

2017

Context. Intermediate polar cataclysmic variables (IPCV) contain a magnetic, rotating white dwarf surrounded by a magnetically truncated accretion disk. To explain their strong flickering X-ray emission, accretion has been successfully taken into account. Nevertheless, observations suggest that accretion phenomena might not be the only process behind it. An intense flaring activity occurring on the surface of the disk may generate a corona, contribute to the thermal X-ray emission, and influence the system stability. Aims. Our purposes are: investigating the formation of an extended corona above the accretion disk, due to an intense flaring activity occurring on the disk surface; studying t…

Magnetohydrodynamics (MHD)Stars: flareAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMagnetosphereAstrophysics01 natural scienceslaw.inventionAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaIntermediate polarlaw0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar AstrophysicsStars: coronaeX-rays: star0101 mathematics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNovae cataclysmic variableWhite dwarfAstronomy and AstrophysicsAstronomy and AstrophysicThermal conductionAccretion (astrophysics)010101 applied mathematicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaFlareAstronomy & Astrophysics
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