Search results for "methods [Diffusion Tensor Imaging]"

showing 10 items of 992 documents

White-light Fourier transformer with low chromatic aberration.

1992

A simple Fourier transformation system working with broadband parallel illumination is presented. The proposed setup, consisting of two on-axis zone plates and an achromatic objective, allows us to obtain the achromatic Fourier transform representation of the input at a finite distance with a low chromatic aberration. The discussion of the system, using the Fresnel diffraction theory, leads to an analytical expression to evaluate the transversal and longitudinal chromatic aberrations. It is shown that the resulting chromatic aberrations for typical values of the involved parameters are less than 1% over the entire visible spectrum.

PhysicsDiffractionGeometrical opticsbusiness.industryMaterials Science (miscellaneous)Astrophysics::Instrumentation and Methods for AstrophysicsIndustrial and Manufacturing Engineeringlaw.inventionsymbols.namesakeOpticsFourier transformlawAchromatic lensChromatic aberrationsymbolsPhysics::Accelerator PhysicsBusiness and International ManagementbusinessTransformerFresnel diffractionVisible spectrumApplied optics
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Scale-tunable optical correlation with natural light

2008

We describe two different scale-tunable optical correlators working under totally incoherent light. They behave as spatially incoherent wavelength-independent imaging systems with an achromatic point-spread function (PSF). In both cases it is possible to adapt the scale of the achromatic PSF, i.e., to modify the scaling factor of the PSF and preserve the chromatic compensation, by one's shifting the input along the optical axis. The remarkable properties of these systems allow us to carry out a scale-tunable color pattern-recognition experiment with natural light.

PhysicsDiffractionScale (ratio)Image qualitybusiness.industryMaterials Science (miscellaneous)Astrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsFunction (mathematics)Industrial and Manufacturing Engineeringlaw.inventionOptical axisOpticsAchromatic lenslawOptical correlatorChromatic scaleBusiness and International Managementbusiness
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Focal squeeze in axicons

2005

The on-axis irradiance distribution of a truncated conical wavefront is evaluated in terms of the Fresnel number of the focusing geometry. In agreement with geometrical optics, a focal line of increasing intensity is generated for extremely high Fresnel numbers. Otherwise clear deviations may be observed for the position of the maximum irradiance along the optical axis. A remarkable focal squeeze appears and, for decreasing Fresnel numbers, this effect manifests stronger. An analytical formula is provided for the fast evaluation of the focal squeeze.

PhysicsDiffractionWavefrontGeometrical opticsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsFresnel lensConical surfaceAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialslaw.inventionOptical axisOpticslawPosition (vector)Fresnel numberElectrical and Electronic EngineeringPhysical and Theoretical ChemistrybusinessOptics Communications
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Debye representation of dispersive focused waves

2006

We report on a matrix-based diffraction integral that evaluates the focal field of any diffraction-limited axisymmetric complex system. This diffraction formula is a generalization of the Debye integral applied to apertured focused beams, which may be accommodated to broadband problems. Longitudinal chromatic aberration may limit the convenience of the Debye formulation and, additionally, spatial boundaries of validity around the focal point are provided. Fresnel number is reformulated in order to guarantee that the focal region is entirely into the region of validity of the Debye approximation when the Fresnel number of the focusing geometry largely exceeds unity. We have applied the matri…

PhysicsDiffractionbusiness.industryParaxial approximationComplex systemRotational symmetryAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesPhysics::OpticsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsKirchhoff's diffraction formulasymbols.namesakeOpticssymbolsFresnel numberComputer Vision and Pattern RecognitionbusinessDiffraction gratingDebyeOptics (physics.optics)Physics - Optics
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An inquiry-based approach to Maxwell distribution: a case study with engineering students

2013

The concept of distribution is a fundamental component of statistical thinking. This paper describes a teaching approach for it that uses a specific activity related to the field of statistical mechanics. The concept of the velocity distribution of a particle system is dealt with using an inquiry-based approach involving an experimental examination of Maxwell’s distribution. Some outcomes of a teaching experiment held at the Faculty of Engineering of the University of Palermo, Italy are described.

PhysicsDistribution (number theory)Research in physics education Teaching methods and strategies Laboratory experiments and apparatus Laboratory course design organization and evaluationClassical statistical mechanicsSettore FIS/08 - Didattica E Storia Della Fisica05 social sciences050301 educationGeneral Physics and AstronomyStatistical mechanics01 natural sciencesMaxwell–Boltzmann distributionField (geography)symbols.namesakeTheoretical physicsStatistical thinkingComponent (UML)0103 physical sciencessymbolsMathematics education010306 general physics0503 educationEuropean Journal of Physics
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Coherence loss in phase-referenced VLBI observations

2010

Context. Phase-referencing is a standard calibration technique in radio interferometry, particularly suited for the detection of weak sources close to the sensitivity limits of the interferometers. However, effects from a changing atmosphere and inaccuracies in the correlator model may affect the phase-referenced images, and lead to wrong estimates of source flux densities and positions. A systematic observational study of signal decoherence in phase-referencing and its effects in the image plane has not been performed yet. Aims. We systematically studied how the signal coherence in Very-Long-Baseline-Interferometry (VLBI) observations is affected by a phase-reference calibration at differe…

PhysicsDynamic rangePhase (waves)Astrophysics::Instrumentation and Methods for AstrophysicsFluxAstronomy and AstrophysicsContext (language use)interferometers [Instrumentation]AstrophysicsAtmospheric effectsComputational physicsTechniques : interferometric; Atmospheric effects; Instrumentation : interferometersInterferometrySpace and Planetary ScienceVery-long-baseline interferometrySource separationinterferometric [Techniques]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]Coherence (physics)
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On the Measurements of Numerical Viscosity and Resistivity in Eulerian MHD Codes

2016

We propose a simple ansatz for estimating the value of the numerical resistivity and the numerical viscosity of any Eulerian MHD code. We test this ansatz with the help of simulations of the propagation of (magneto)sonic waves, Alfven waves, and the tearing mode instability using the MHD code Aenus. By comparing the simu- lation results with analytical solutions of the resistive-viscous MHD equations and an empirical ansatz for the growth rate of tearing modes we measure the numerical viscosity and resistivity of Aenus. The comparison shows that the fast-magnetosonic speed and wavelength are the characteristic velocity and length, respectively, of the aforementioned (relatively simple) syst…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsEulerian pathMechanicsCharacteristic velocity01 natural sciencesNumerical resistivityRiemann solver010305 fluids & plasmassymbols.namesakeViscosityAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetorotational instability0103 physical sciencessymbolsMagnetohydrodynamicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)AnsatzThe Astrophysical Journal Supplement Series
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High-visibility interference fringes with femtosecond laser radiation.

2009

We propose and experimentally demonstrate an interferometer for femtosecond pulses with spectral bandwidth about 100 nm. The scheme is based on a Michelson interferometer with a dispersion compensating module. A diffractive lens serves the purpose of equalizing the optical-path-length difference for a wide range of frequencies. In this way, it is possible to register high-contrast interference fringes with micrometric resolution over the whole area of a commercial CCD sensor for broadband femtosecond pulses.

PhysicsFemtosecond pulse shapingbusiness.industryLasersAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsMichelson interferometerEquipment DesignInterference (wave propagation)Atomic and Molecular Physics and Opticslaw.inventionEquipment Failure AnalysisInterferometryRefractometryOpticsInterferometrylawFemtosecondDispersion (optics)OptoelectronicsComputer-Aided DesignbusinessDiffraction gratingCoherence (physics)LensesOptics express
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Novel signatures of dark matter in laser-interferometric gravitational-wave detectors

2019

Dark matter may induce apparent temporal variations in the physical "constants", including the electromagnetic fine-structure constant and fermion masses. In particular, a coherently oscillating classical dark-matter field may induce apparent oscillations of physical constants in time, while the passage of macroscopic dark-matter objects (such as topological defects) may induce apparent transient variations in the physical constants. In this paper, we point out several new signatures of the aforementioned types of dark matter that can arise due to the geometric asymmetry created by the beam-splitter in a two-arm laser interferometer. These new signatures include dark-matter-induced time-var…

PhysicsField (physics)Gravitational wavebusiness.industryDark matterScalar (physics)FOS: Physical sciencesLIGOInterferometryHigh Energy Physics - PhenomenologyOpticsHigh Energy Physics - Phenomenology (hep-ph)HolometerKAGRAbusinessAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Optics (physics.optics)Physics - Optics
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Magnetic shielding of soft protons in future X-ray telescopes: the case of the ATHENA Wide Field Imager

2018

Both the interplanetary space and the Earth magnetosphere are populated by low energy ($\leq300$ keV) protons that are potentially able to scatter on the reflecting surface of Wolter-I optics of X-ray focusing telescopes and reach the focal plane. This phenomenon, depending on the X-ray instrumentation, can dramatically increase the background level, reducing the sensitivity or, in the most extreme cases, compromising the observation itself. The use of a magnetic diverter, deflecting protons away from the field of view, requires a detailed characterization of their angular and energy distribution when exiting the mirror. We present the first end-to-end Geant4 simulation of proton scattering…

PhysicsField (physics)ProtonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsMagnetosphereFOS: Physical sciencesAstronomy and AstrophysicsX-ray telescopeField of view01 natural sciencesComputational physicsMagnetic field010309 opticsCardinal pointSpace and Planetary Science0103 physical sciencesElectromagnetic shieldinginstrumentation: miscellaneous – telescopesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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