Search results for "methods [Diffusion Tensor Imaging]"

showing 10 items of 992 documents

Amplitude modulation technique for designing metalenses with apodized and enhanced resolution focal spots

2017

Abstract In this paper we show that engineering both phase and amplitude of the scattered light can be employed in designing metalenses with either higher resolution or apodized focal spots. C-shaped split-ring micro-resonators (CSRRs) with different geometrical parameters are selected to have a full control of amplitude and phase. While phase engineering is necessary for light focusing, amplitude modulation of the scattered wave can be applied to characterize the focal point properties such as resolution gain and sidelobe level. We show that both axial and transverse resolution improvement or apodization is possible in the far-field region by applying proper amplitude function. Amplitude m…

PhysicsFocal pointbusiness.industryResolution (electron density)Astrophysics::Instrumentation and Methods for AstrophysicsPhase (waves)02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materials010309 opticsAmplitude modulationAmplitudeOpticsApodization0103 physical sciencesElectrical and Electronic EngineeringPhysical and Theoretical Chemistry0210 nano-technologybusinessLithographyPhase modulationOptics Communications
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On-axis diffractional behavior of two-dimensional pupils

2010

We show that, at any Fresnel number, a suitable one-dimensional Fourier transform relates the complex-amplitude distribution along the optical axis with the zero-order circular harmonic of the amplitude transmittance of a two-dimensional diffracting screen. First, our general result is applied to recognize that any rationally nonsymmetric screen generates an axial-irradiance distribution that exhibits focal shift. In this way we identify a wide set of two-dimensional screens that produce the same focal shift as that produced by the clear circular aperture. Second, we identify several apodizers for shaping the axial-amplitude distribution. We discuss some examples for achieving high-precisio…

PhysicsFresnel zoneAperturebusiness.industryMaterials Science (miscellaneous)Astrophysics::Instrumentation and Methods for AstrophysicsFresnel integralIndustrial and Manufacturing EngineeringOptical axissymbols.namesakeOpticsFourier transformApodizationsymbolsFresnel numberBusiness and International ManagementFocus (optics)businessApplied Optics
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Strehl ratio versus defocus for noncentrally obscured pupils.

1994

We discuss from the viewpoint of the Strehl ratio versus defocus, or the normalized axial-irradiance distribution, the influence of decentering the dark mask of an annular pupil. Our treatment, which is valid for pupil apertures with any Fresnel number, permits us to infer that the axial behavior of a noncentrally obscured pupil is equivalent to that of an apodizer with continuous amplitude variations. Hence the Strehl ratio versus defocus of an optical system can be shaped by use of noncentered dark masks that act as continuous gray apodizers. Several numerically evaluated examples are presented.

PhysicsFresnel zoneSpatial filterImage qualitybusiness.industryMaterials Science (miscellaneous)Astrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsStrehl ratioIndustrial and Manufacturing EngineeringPupilAmplitudeOpticsFresnel numberBusiness and International ManagementbusinessApplied optics
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Focal-shift formula in apodized nontelecentric focusing systems

2007

A single analytical formulation for evaluating the focal shift in any apodized nontelecentric focusing setup is reported. The formulation is also useful in the case of imaged paraxial beams. We show explicitly that the magnitude of the focal shift is determined by only one parameter that depends on the effective width of the pupil filter and its axial position. To illustrate our approach we examine different focusing setups.

PhysicsGeometrical opticsbusiness.industryParaxial approximationAstrophysics::Instrumentation and Methods for AstrophysicsFilter (signal processing)Atomic and Molecular Physics and OpticsOpticsApodizationPosition (vector)Systems designFresnel numberbusinessFresnel diffractionOptics Letters
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OCTOCAM: A fast multichannel imager and spectrograph for the 10.4m GTC

2010

OCTOCAM is a multi-channel imager and spectrograph that has been proposed for the 10.4m GTC telescope. It will use dichroics to split the incoming light to produce simultaneous observations in 8 different bands, ranging from the ultraviolet to the near-infrared. The imaging mode will have a field of view of 2' x 2' in u, g, r, i, z, J, H and Ks bands, whereas the long-slit spectroscopic mode will cover the complete range from 4,000 to 23,000 {\AA} with a resolution of 700 - 1,700 (depending on the arm and slit width). An additional mode, using an image slicer, will deliver a spectral resolution of over 3,000. As a further feature, it will use state of the art detectors to reach high readout…

PhysicsGran Telescopio Canariasbusiness.industryResolution (electron density)Near-infrared spectroscopyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesField of viewlaw.inventionTelescopeOpticslawObservatorySpectral resolutionbusinessAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Spectrograph
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Denoising of gravitational wave signals via dictionary learning algorithms

2016

Gravitational wave astronomy has become a reality after the historical detections accomplished during the first observing run of the two advanced LIGO detectors. In the following years, the number of detections is expected to increase significantly with the full commissioning of the advanced LIGO, advanced Virgo and KAGRA detectors. The development of sophisticated data analysis techniques to improve the opportunities of detection for low signal-to-noise-ratio events is, hence, a most crucial effort. In this paper, we present one such technique, dictionary-learning algorithms, which have been extensively developed in the last few years and successfully applied mostly in the context of image…

PhysicsGravitational-wave observatoryEinstein Telescope010308 nuclear & particles physicsGravitational waveFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGravitational-wave astronomyGeneral Relativity and Quantum CosmologyLIGONumerical relativityBinary black hole0103 physical sciencesKAGRAAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)AlgorithmPhysical Review D
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A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes

2021

Code comparisons are a valuable tool for the verification of supernova simulation codes and the quantification of model uncertainties. Here we present a first comparison of axisymmetric magnetohydrodynamic (MHD) supernova simulations with the CoCoNuT-FMT and Aenus-Alcar codes, which use distinct methods for treating the MHD induction equation and the neutrino transport. We run two sets of simulations of a rapidly rotating 35M gamma-ray burst progenitor model with different choices for the initial field strength, namely 10^12 G for the maximum poloidal and toroidal field in the strong-field case and 10^10 G in the weak-field case. We also investigate the influence of the Riemann solver and t…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSupernovaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetohydrodynamic driveMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)
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Diffusivity in force-free simulations of global magnetospheres

2021

Abstract: Assuming that the numerical diffusivity triggered by violations of the force-free electrodynamics constraints is a proxy for the physical resistivity, we examine its impact on the overall dynamics of force-free aligned pulsar magnetospheres endowed with an equatorial current sheet. We assess the constraint violations as a diffusivity source. The effects of modifications on electric fields used to restore force-free conditions are not confined to the equatorial current sheet, but modify the magnetospheric dynamics on timescales shorter than the pulsar rotational period. These corrections propagate especially via a channel that was unexplored, namely, changes induced to the electric…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFluxCharge densityFOS: Physical sciencesAstronomy and AstrophysicsThermal diffusivityLuminositysymbols.namesakeCurrent sheetMaxwell's equationsPulsarSpace and Planetary ScienceQuantum electrodynamicsPoynting vectorsymbolsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Relativistic Magnetohydrodynamics: Renormalized eigenvectors and full wave decomposition Riemann solver

2010

We obtain renormalized sets of right and left eigenvectors of the flux vector Jacobians of the relativistic MHD equations, which are regular and span a complete basis in any physical state including degenerate ones. The renormalization procedure relies on the characterization of the degeneracy types in terms of the normal and tangential components of the magnetic field to the wavefront in the fluid rest frame. Proper expressions of the renormalized eigenvectors in conserved variables are obtained through the corresponding matrix transformations. Our work completes previous analysis that present different sets of right eigenvectors for non-degenerate and degenerate states, and can be seen as…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Degenerate energy levelsFOS: Physical sciencesAstronomy and AstrophysicsSolverRest frameRiemann solverRenormalizationsymbols.namesakeTransformation matrixSpace and Planetary SciencesymbolsApplied mathematicsDegeneracy (mathematics)Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaInstrumentation and Methods for Astrophysics (astro-ph.IM)Eigenvalues and eigenvectorsAstrophysics - Cosmology and Nongalactic Astrophysics
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3HWC: The Third HAWC Catalog of Very-High-Energy Gamma-ray Sources

2020

We present a new catalog of TeV gamma-ray sources using 1523 days of data from the High Altitude Water Cherenkov (HAWC) observatory. The catalog represents the most sensitive survey of the Northern gamma-ray sky at energies above several TeV, with three times the exposure compared to the previous HAWC catalog, 2HWC. We report 65 sources detected at $\geq$ 5 sigma significance, along with the positions and spectral fits for each source. The catalog contains eight sources that have no counterpart in the 2HWC catalog, but are within $1^\circ$ of previously detected TeV emitters, and twenty sources that are more than $1^\circ$ away from any previously detected TeV source. Of these twenty new so…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)High energyHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGamma-ray astronomyAstrophysics::Cosmology and Extragalactic AstrophysicsPulsarSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy Astrophysics
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