Search results for "Spectral"

showing 10 items of 3116 documents

Spectral anomalies in focused waves of different Fresnel numbers

2004

Light propagation induces remarkable changes in the spectrum of focused diffracted beams. We show that spectral changes take place in the vicinity of phase singularities in the focal region of spatially coherent, polychromatic spherical waves of different Fresnel numbers. Instead of the Debye formulation, we use the Kirchhoff integral to evaluate the focal field accurately. We find that as a result of a decrease in the Fresnel number, some cylindrical spectral switches are geometrically transformed into conical spectral switches.

PhysicsDiffractionFresnel zoneGeometrical opticsbusiness.industryFresnel zone antennaAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsFresnel integralAtomic and Molecular Physics and OpticsSpectral lineElectronic Optical and Magnetic MaterialsOpticsFresnel numberComputer Vision and Pattern RecognitionbusinessFresnel diffractionJournal of the Optical Society of America A
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Emitter-site specificity of hard x-ray photoelectron Kikuchi-diffraction

2020

New journal of physics 22(10), 103002 (1-13) (2020). doi:10.1088/1367-2630/abb68b

PhysicsDiffractionSiliconDopantX-rayGeneral Physics and Astronomychemistry.chemical_element01 natural sciencesMolecular physics530Spectral line010305 fluids & plasmaschemistryLattice (order)Interstitial defect0103 physical sciencesPhysics::Atomic and Molecular Clustersddc:530010306 general physicsBloch wave
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Spectral anomalies in supercontinuum focused waves

2006

The diffraction-induced spectral anomalies in the focal plane of an apertured spherical wave with supercontinuum flat-top power spectrum are investigated. Coherent broadband radiation (also incoherent white light) demonstrates a strong blue shift in the vicinity of the optical axis, and discrete spectral gaps with overall red shift arise out of this central region. Unlike narrow-band light, the spectral switch effect fades away with ultra-broad spectra.

PhysicsDiffractionWave propagationbusiness.industryPhysics::OpticsSpectral densityAtomic and Molecular Physics and OpticsSpectral lineElectronic Optical and Magnetic MaterialsSupercontinuumBlueshiftOptical axisCardinal pointOpticsElectrical and Electronic EngineeringPhysical and Theoretical ChemistrybusinessOptics Communications
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Achromatic diffraction of femtosecond light pulses

2003

Diffraction of electromagnetic waves in free space is a physical phenomenon that explicitly depends on the wavelength of light radiation. As an ultrashort-pulsed waveform consists of many frequency components that are coherently superposed, diffraction of a femtosecond pulse passing through an aperture radically differs from that under continuous wave (CW) monochromatic illumination. Note that the spectral width of a 5 fs pulsed beam is approximately 400 nm, which roughly corresponds to the entire visible spectrum bandwidth. The spectral distribution of the source results in the chromatic distortion, both lateral and axial, of the optical field diffracted by the aperture. This detrimental e…

PhysicsDiffractionWavelengthOpticsbusiness.industrySpectral widthFemtosecondFilament propagationTalbot effectPhysics::OpticsAcousto-opticsbusinessElectromagnetic radiationFrontiers in Optics
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A coupled-map model for the magnetotail current sheet

1999

A magnetic field model of the magnetotail current sheet in the form of a coupled-map lattice (CML) is presented. It is a continuously driven and based on the MHD diffusion equation. Solar wind vBs data (solar wind speed multiplied by the southward component of IMF) are used for driving the model, and it is shown to exhibit perturbations (avalanches) with power-law scalings in their distributions of duration and size. Such distributions may indicate self-organized critical (SOC) behavior. Furthermore, it is shown that the power spectra of the model outputs are of bicolor power-law form with different slopes for high and low frequencies. The model parameters determine the frequency of the bre…

PhysicsDiffusion equationSpectral densityGeophysicsPower lawSpectral lineComputational physicsMagnetic fieldCurrent sheetSolar windGeophysicsPhysics::Space PhysicsGeneral Earth and Planetary SciencesMagnetohydrodynamicsGeophysical Research Letters
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Transition from Prolate to Oblate to Triaxial Shapes in158Yb

1983

The decay of the entry states in ISIYb populated in the reactions of 149 MeV ,oNe with ,44Nd and lUNd has been investigated with a 4" multidetector system gated by a Ge counter. The average excitation energy, the ,.-ray spectra and the angular distribu tions as a function of multiplicity show several changes in the ,.-ray decay. These changes suggest a transition from prolate to particle aligned oblate connguration at low spin. At 1- 38-48 collective transitions with dipole and quad­ rupole component possibly built on high K single particle states are observed. Furthennore, above 1- 48 the dipole component disappears suggesting a further change toward more triaxial shape.

PhysicsDipoleOblate spheroidProlate spheroidAtomic physicsMultiplicity (chemistry)Condensed Matter PhysicsMathematical PhysicsAtomic and Molecular Physics and OpticsSpectral lineExcitationPhysica Scripta
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Fourier-transform spectroscopy and relativistic electronic structure calculation on the c3Σ+ state of KCs

2021

Abstract The Ti:Saphire laser operated within 13800 - 11800 cm − 1 range was used to excite the c 3 Σ + state of KCs molecule directly from the ground X 1 Σ + state. The laser-induced fluorescence (LIF) spectra of the c 3 Σ + → a 3 Σ + transition were recorded with Fourier-transform spectrometer within 8000 to 10000 cm − 1 range. Overall 673 rovibronic term values belonging to both e / f -components of the c 3 Σ + ( Ω = 1 ± ) state of 39 KCs, covering vibrational levels from v = 0 to about 45, and rotational levels J ∈ [ 11 , 149 ] were determined with the accuracy of about 0.01 cm − 1 ; among them 7 values for 41 KCs. The experimental term values with v ∈ [ 0 , 22 ] were involved in a dire…

PhysicsDipoleRadiationCoupled clusterMoleculeElectronic structureState (functional analysis)Atomic physicsPotential energySpectroscopyAtomic and Molecular Physics and OpticsSpectral lineFourier transform spectroscopyJournal of Quantitative Spectroscopy and Radiative Transfer
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Transfer reactions on light exotic nuclei studied with CHIMERA detector at LNS

2014

The kinematical coincidence method is used to extract angular distribution of elastic scattering and transfer reactions. The detected light particle energy spectra are used to extract the angular distribution with around 1° resolution in the Center of Mass (CM) system. Examples with 10Be beam are presented. In the case of proton scattering, γ-ray coincidences are used to discriminate excited levels population from elastic scattering. © Owned by the authors, published by EDP Sciences, 2014.

PhysicsElastic scatteringeducation.field_of_studyPhysicsQC1-999PopulationResolution (electron density)Nuclear reactionCoincidenceSpectral linePhysics and Astronomy (all)Transfer reactionsExcited stateCenter of massAtomic physicseducationBeam (structure)EPJ Web of Conferences
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On the soft excess in the x-ray spectrum of circinus X-1: Revisitation of the distance to circinus X-1

2005

We report on a 300 ks BeppoSAX (0.12-200 keV) observation of Circinus X-1 (Cir X-1) at phases between 0.62 and 0.84 and on a 90 ks BeppoSAX observation of Cir X-1 at phases 0.11-0.16. Using the canonical model adopted until now to fit the energy spectrum of this source, large residuals appear below 1 keV. These are well fitted using an equivalent hydrogen column of 0.66¿1022 cm-2, adding absorption edges of O VII, O VIII, and Ne IX in the spectra extracted from the observation at phases 0.62-0.84 and adding absorption edges of O VII, O VIII, Mg XI, and Mg XII and absorption lines of O VIII and Mg XII in the spectra extracted from the observation at phases 0.11-0.16. During the observation a…

PhysicsElectron densityAccretionAbsorption spectroscopyStars: Individual: Constellation Name: Circinus X-1Stars: individual (Circinus X-1)Accretion; Accretion Disks; Stars: Individual: Constellation Name: Circinus X-1; Stars: Neutron; X-Rays: Binaries; X-Rays: StarsX-rayAstronomy and Astrophysicsindividual (Circinus X-1); Stars: neutron; X-rays: binaries; X-rays: stars; Nuclear and High Energy Physics; Space and Planetary Science [Accretion accretion disks; Stars]AstrophysicsCompact starX-rays: binarieSpectral lineStars: neutronX-Rays: BinariesAccretion accretion diskSpace and Planetary ScienceIonizationAccretion DisksX-Rays: StarsCircinusX-rays: starAbsorption (logic)Nuclear and High Energy Physic
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Comparison of hydrogen Balmer-alpha Stark profiles measured at high electron densities with theoretical results

2005

Profiles of the H-alpha line calculated using the full computer simulation method (FCSM) and the standard theory (ST) agree excellently with a measured profile (at an electron density of Ne = 9.0 × 1016 cm−3 and temperature T = 12 600 K) in an argon–hydrogen (minority) arc plasma. Calculated widths (FCSM) and shifts (ST) also agree well with experimental data from flash-tube plasmas and gas-linear pinch plasmas. Some discrepancies are probably caused by experimental flaws. Our analysis of the so-called generalized theory (GT) shows that this theory is burdened with un-physical approximations, and consequently so are all subsequent modifications based on GT. It is shown that the so-called ac…

PhysicsElectron densityField (physics)Plasma parametersBalmer seriesElectronWarm dense matterCondensed Matter PhysicsSpectral lineAtomic and Molecular Physics and Opticssymbols.namesakesymbolsAtomic physicsLine (formation)Journal of Physics B: Atomic, Molecular and Optical Physics
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