Search results for "SPECTRA"

showing 10 items of 3542 documents

Orientation dependence of high-order harmonic generation in molecules

2003

We present two- and three-dimensional model calculations of high-order harmonic generation in ${\mathrm{H}}_{2}^{+}.$ The harmonic spectra exhibit clear signatures of intramolecular interference. An interference minimum appears at a harmonic order that depends on the molecular orientation. Harmonic generation in three-center molecules is studied on the basis of two-dimensional calculations for a ${\mathrm{H}}_{3}^{2+}$ model system. From analytical considerations, the orientation dependence of the harmonic intensities in three-center molecules exhibits a double minimum due to intramolecular interference. In the numerical results, the double minimum is broadened into a single wide minimum. T…

PhysicsLinear polarizationIntramolecular forceMoleculeHigh harmonic generationSurface second harmonic generationElliptical polarizationAtomic physicsPolarization (waves)GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Atomic and Molecular Physics and OpticsSpectral linePhysical Review A
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On X-ray Optical Depth in the Coronae of Active Stars

2007

We have investigated the optical thickness of the coronal plasma through the analysis of high-resolution X-ray spectra of a large sample of active stars observed with the High Energy Transmission Grating Spectrometer on Chandra. In particular, we probed for the presence of significant resonant scattering in the strong Lyman series lines arising from hydrogen-like oxygen and neon ions. The active RS CVn-type binaries II Peg and IM Peg and the single M dwarf EV Lac show significant optical depth. For these active coronae, the Lya/Lyb ratios are significantly depleted as compared with theoretical predictions and with the same ratios observed in similar active stars. Interpreting these decremen…

PhysicsLyman seriesAstrophysics (astro-ph)chemistry.chemical_elementFluxFOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsradiative transfer — stars: coronae — stars: late-type — X-rays: starsSpectral linesymbols.namesakeStarsNeonchemistrySpace and Planetary SciencesymbolsAstrophysics::Solar and Stellar AstrophysicsOptical depthLine (formation)
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Retrieval of sun-induced fluorescence using advanced spectral fitting methods

2015

Abstract The FLuorescence EXplorer (FLEX) satellite mission, candidate of ESA's 8th Earth Explorer program, is explicitly optimized for detecting the sun-induced fluorescence emitted by plants. It will allow consistent measurements around the O2-B (687 nm) and O2-A (760 nm) bands, related to the red and far-red fluorescence emission peaks respectively, the photochemical reflectance index, and the structural-chemical state variables of the canopy. The sun-induced fluorescence signal, overlapped to the surface reflected radiance, can be accurately retrieved by employing the powerful spectral fitting technique. In this framework, a set of fluorescence retrieval algorithms optimized for FLEX ar…

PhysicsMETIS-314125Spectrometerbusiness.industryRetrieval algorithmSpectral fitting methodSoil ScienceGeologyFull fluorescence spectrumPhotochemical Reflectance IndexFluorescenceSpectral linen/a OA procedureFLEX missionOpticsSun-induced fluorescenceRadianceRadiative transferSatelliteComputers in Earth SciencesbusinessAbsorption (electromagnetic radiation)Remote sensing
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High-resolution laser spectroscopy of Al27–32

2021

Hyperfine spectra of $^\text{27-32}$Al ($Z=13$) have been measured at the ISOLDE-CERN facility via collinear laser spectroscopy using the $3s^23p\ ^2\text{P}^\text{o} _{3/2}\rightarrow 3s^24s\ ^2\text{S}_{1/2}$ atomic transition. For the first time, mean-square charge radii of radioactive aluminum isotopes have been determined alongside the previously unknown magnetic dipole moment of $^{29}$Al and electric quadrupole moments of $^{29,30}$Al. A potentially reduced charge radius at $N=19$ may suggest an effect of the $N=20$ shell closure, which is visible in the Al chain, contrary to other isotopic chains in the $sd$ shell. The experimental results are compared to theoretical calculations in…

PhysicsMagnetic moment010308 nuclear & particles physicsCharge (physics)7. Clean energy01 natural sciencesSpectral lineCharge radius0103 physical sciencesQuadrupoleAtomic physics010306 general physicsSpectroscopyMagnetic dipoleHyperfine structurePhysical Review C
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Electromagnetic Multipole Moments and Transitions

2007

In the preceding chapter we constructed and discussed the simplest possible nuclear wave functions. This construction was done at the mean-field level. No account was taken of configuration mixing caused by the nuclear residual interaction. These simple wave functions produce degeneracies in energy spectra. This is contrary to experimental data, so improved wave functions are called for.

PhysicsMagnetic momentSimple (abstract algebra)Quantum electrodynamicsMultipole expansionResidualWave functionEnergy (signal processing)Mixing (physics)Spectral line
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Accessing fast magnetization dynamics by XPEEM: Status and perspectives

2006

Abstract Being already well established as a versatile technique for high-resolution static magnetic domain imaging, X-ray photoemission electron microscopy (XPEEM) is now also capturing the field of time-resolved magnetic investigations. Using appropriate operation modes at synchrotron radiation sources, a time resolution of 10 ps and less can be achieved in recent magnetodynamics studies, giving access even to phenomena involving precessional processes.

PhysicsMagnetization dynamicsPhotoemission electron microscopyMagnetizationNuclear magnetic resonanceField (physics)Magnetic domainTime resolved spectraSynchrotron radiationTime resolutionCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsComputational physicsJournal of Magnetism and Magnetic Materials
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Mass number scaling in ultra-relativistic nuclear collisions from a hydrodynamical approach

1998

We study the different nucleus-nucleus collisions, O+Au, S+S, S+Ag, S+Au and Pb+Pb, at the CERN-SPS energy in a one-fluid hydrodynamical approach using a parametrization based on baryon stopping in terms of the thickness of colliding nuclei. Good agreement with measured particle spectra is achieved. We deduce the mass number scaling behaviour of the initial energy density. We find that the equilibration time is nearly independent of the size of the colliding nuclei.

PhysicsMass numberNuclear TheoryPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsNuclear TheoryFOS: Physical sciencesSpectral lineNuclear Theory (nucl-th)Nuclear physicsBaryonBaryon densityEnergy densityParticleHigh Energy Physics::ExperimentAtomic physicsNuclear ExperimentEngineering (miscellaneous)ParametrizationScalingThe European Physical Journal C
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Photoproduction of high-energy neutrons in thick targets by electrons in the energy range 150 to 270 MeV

1973

Photoneutron spectra with energies greater than 12 MeV produced by electrons incident on a thick lead target have been measured for primary electron energies between 150 and 266 MeV and at a fixed angle of 90 ° to the beam axis. Measurements of the neutron yield have furthermore been performed at a primary energy of 234 MeV as a function of target depth for the same lead target and as a function of the mass number for C, Al, Cu, Cd and Pb targets. The results were obtained with three independent neutron detectors: two proton recoil counters and one time-of-flight set-up. The high-energy regions of the spectra are compared with the predictions of the phenomenological quasi-deuteron model and…

PhysicsMass numberNuclear and High Energy PhysicsRange (particle radiation)Nuclear TheoryGeneral Physics and AstronomyElectronSpectral lineNuclear physicsPionNuclear fusionNeutron detectionNeutronNuclear ExperimentZeitschrift für Physik
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O(αs)corrections to the correlator of finite mass baryon currents

2000

We present analytical next-to-leading order results for the correlator of baryonic currents at the three-loop level with one finite mass quark. We obtain the massless and the HQET limit of the correlator from the general formula as particular cases. We also give explicit expressions for the moments of the spectral density.

PhysicsMassless particleQuantum chromodynamicsBaryonQuarkNuclear and High Energy PhysicsParticle physicsQuantum electrodynamicsHigh Energy Physics::PhenomenologyHyperonSpectral densityLimit (mathematics)Spectral methodPhysical Review D
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SHIFT AND WIDTH OF HeII LINES

1998

Abstract Based on a quantum statistical many-particle theory, the shift and the width of some He II lines have been evaluated. Ion dynamics have been treated within the model microfield method. Furthermore, fine structure splitting has been taken into account in order to check whether this effect is the cause for the existing large discrepancies between theoretical and experimental line widths. Besides the electronic contributions to the line shift, the shift due to the inhomogeneities of the ionic microfield as well as that due to the quadratic Stark effect has been included.

PhysicsMaterials scienceRadiationIonic bondingSpectral shiftAtomic and Molecular Physics and OpticsLine shiftIonsymbols.namesakeQuadratic equationStark effectHelium ionssymbolsFine structureEmission spectrumAtomic physicsQuantumSpectroscopyLine (formation)Journal of Quantitative Spectroscopy and Radiative Transfer
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