Search results for "methods [Diffusion Tensor Imaging]"

showing 10 items of 992 documents

High-contrast white-light Lau fringes

2004

We present a new optical assembly with which to achieve Lau fringes with totally incoherent illumination. Gratinglike codification of the spatially incoherent source combined with an achromatic Fresnel diffraction setup allows us to achieve Lau fringe-pattern visibility of almost 100% with broadband light. The white-light character to our proposed setup is in stark contrast to previous monochromatic implementations. Potential implications of this fact are identified.

DiffractionPhysicsbusiness.industrymedia_common.quotation_subjectVisibility (geometry)Astrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsPhysical opticsAtomic and Molecular Physics and Opticslaw.inventionOpticsAchromatic lenslawContrast (vision)Physics::Atomic PhysicsMonochromatic colorbusinessDiffraction gratingFresnel diffractionmedia_commonOptics Letters
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Effective Fresnel-number concept for evaluating the relative focal shift in focused beams

1998

We report on an analytical formulation, based on the concept of effective Fresnel number, to evaluate in a simple way the relative focal shift of rotationally nonsymmetric scalar fields that have geometrical focus and moderate Fresnel number. To illustrate our approach, certain previously known results and also some new focusing setups are analytically examined.

DiffractionWavefrontPhysicsFresnel zoneGeometrical opticsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsScalar (physics)Atomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsOpticsFresnel numberComputer Vision and Pattern RecognitionFocus (optics)businessFresnel diffractionJournal of the Optical Society of America A
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Performance analysis of optical imaging systems based on the fractional fourier transform

1998

Some image quality parameters, such as the Strehl ratio and the optical transfer function, are analysed in the generalized phase-space, or x-p domain, of the fractional Fourier transform associated with a modified one-dimensional pupil function. Some experimental results together with computer simulations are performed which illustrate the tolerance to defocus of different apertures.

Discrete-time Fourier transformStrehl ratioIngenieríaDiscrete Fourier transformsymbols.namesakePupil functionOpticsOptical transfer functionPupil functionComputer Science::Distributed Parallel and Cluster ComputingCiencias ExactasPhysicsbusiness.industryPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsShort-time Fourier transformStrehl ratioOpticsDiscrete Fourier transformFourier analysisAtomic and Molecular Physics and OpticsFractional Fourier transformFractional Fourier transformOptical transfer functionFourier analysisShort-time Fourier transformsymbolsbusinessDiscrete-time Fourier transformJournal of Modern Optics
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Nonlinear dynamics of a two-photon Fabry–Pérot laser

2000

Abstract The steady-state emission, stability and temporal dynamics of a single-mode two-photon laser with a Fabry–Perot cavity is investigated and compared with that of a ring-cavity laser. It is found that the Fabry–Perot cavity makes the laser less efficient than the ring cavity because of spatial hole burning, but the domain of stability is larger for the Fabry–Perot laser. The intensity and phase dynamics are numerically investigated and distinctive features are found in the phase dynamics as compared with one-photon lasers.

Distributed feedback laserMaterials sciencePhysics::Instrumentation and Detectorsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsInjection seederLaserAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsIntensity (physics)law.inventionNonlinear systemOpticsTwo-photon excitation microscopylawPhysics::Atomic PhysicsLaser power scalingElectrical and Electronic EngineeringPhysical and Theoretical ChemistrybusinessFabry–Pérot interferometerOptics Communications
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Observational Approach and Perspective

1983

Well you did not cover more than half of my planned talk! (laughter). Let me comment on interferometric techniques, in particular speckle imaging which you mentioned. Doing speckle imaging with the largest telescopes now available will not give you better than the theoretical resolving power of the telescope. With a 4m telescope that is about 30 marc sec in the visible. That happens to be the radius of the supergiant Betelguese. So you are not going to achieve much with speckle imaging on these stars. One technique which has not been adequately exploited is that of lunar occultation which can give much better angular resolution than speckle, of the order of 2-3 marc sec. By using suitably c…

Dwarf starComputer scienceAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyOccultationlaw.inventionTelescopeSpeckle patternInterferometryStarslawAstrophysics::Solar and Stellar AstrophysicsAngular resolutionAstrophysics::Earth and Planetary AstrophysicsSpeckle imagingAstrophysics::Galaxy Astrophysics
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Massive evaluation and analysis of Poincar�� recurrences on grids of initial data: a tool to map chaotic diffusion

2020

We present a novel numerical method aimed to characterize global behaviour, in particular chaotic diffusion, in dynamical systems. It is based on an analysis of the Poincar\'e recurrence statistics on massive grids of initial data or values of parameters. We concentrate on Hamiltonian systems, featuring the method separately for the cases of bounded and non-bounded phase spaces. The embodiments of the method in each of the cases are specific. We compare the performances of the proposed Poincar\'e recurrence method (PRM) and the custom Lyapunov exponent (LE) methods and show that they expose the global dynamics almost identically. However, a major advantage of the new method over the known g…

Dynamical systems theoryComputer scienceChaoticGeneral Physics and AstronomyFOS: Physical sciencesLyapunov exponent01 natural sciences010305 fluids & plasmasHamiltonian systemsymbols.namesakeSimple (abstract algebra)0103 physical sciencesApplied mathematicsDiffusion (business)010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ComputingMilieux_MISCELLANEOUSEarth and Planetary Astrophysics (astro-ph.EP)Numerical analysisNonlinear Sciences - Chaotic DynamicsHardware and ArchitectureBounded functionsymbolsChaotic Dynamics (nlin.CD)Astrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Earth and Planetary Astrophysics
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Lidar : traitement avancé des données et interprétation archéologique - cours 2016

2016

Détection[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[INFO.INFO-TI] Computer Science [cs]/Image Processing [eess.IV]archéologie[SHS.GEO] Humanities and Social Sciences/Geography[SHS.STAT] Humanities and Social Sciences/Methods and statisticsTélédétection par lidarmodèle numérique de terrainlidar
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Les déterminants des compétences sociales des élèves de cycle III

2016

Les différences de réussite à l’école primaire traditionnellement étudiées par les chercheurs en éducation peuvent être analysées à la lumière des compétences et plus particulièrement des compétences sociales. Champ théorique encore en construction, les compétences sociales deviennent tout de même un « incontournable » pour les acteurs du système éducatif et pour la recherche en sciences de l’éducation. Par une approche pluridisciplinaire, cet article propose d’étudier quels sont les déterminants des compétences sociales à l’aide d’indicateurs sociodémographiques et scolaires largement empruntés dans les modèles d’explication des différences de réussite, auxquels sont associées des mesures …

DéterminantCompétence sociale[SHS.EDU]Humanities and Social Sciences/Education[SHS.EDU] Humanities and Social Sciences/Educationlearners' skills and behaviours[ SHS.EDU ] Humanities and Social Sciences/EducationGeneral Medicineimage de soihigher and university educationmethods and tools [pedagogy]famille et éducationrelationship to knowledge and cultureenseignement supérieur et universitairePolitical scienceEnseignement élémentaireméthodes et outils [pédagogie ]geography (teaching/education/relationship)ÉlèveFrancecompétences et comportements des apprenantsself-imagerapport au savoir et à la cultureHumanitiesfamily and educationgéographie (enseignement/éducation/rapport à)
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The MOBI-Kids Study Protocol: Challenges in Assessing Childhood and Adolescent Exposure to Electromagnetic Fields from Wireless Telecommunication Tec…

2014

The rapid increase in mobile phone use in young people has generated concern about possible health effects of exposure to radiofrequency (RF) and extremely low frequency (ELF) electromagnetic fields (EMF). MOBI-Kids, a multinational case–control study, investigates the potential effects of childhood and adolescent exposure to EMF from mobile communications technologies on brain tumor risk in 14 countries. The study, which aims to include approximately 1,000 brain tumor cases aged 10–24 years and two individually matched controls for each case, follows a common protocol and builds upon the methodological experience of the INTERPHONE study. The design and conduct of a study on EMF exposure an…

ELF–EMFmedia_common.quotation_subjectPopulationInternet privacyBrain tumorSocio-culturalecomputer.software_genreAdolescentsBrain tumors03 medical and health sciences0302 clinical medicineEconomicaMethods ArticlemedicineWirelessMobile phones030212 general & internal medicineeducationAssociation (psychology)Childrenmedia_commonTumorsSelection biasProtocol (science)education.field_of_studybusiness.industrylcsh:Public aspects of medicinePublic Health Environmental and Occupational HealthELF-EMFAmbientaleTumors en els infantslcsh:RA1-1270medicine.diseaseTelèfon mòbil i adolescents3. Good healthCervell Localització de funcionsMobile phoneTelèfon mòbil030220 oncology & carcinogenesisadolescentMobile telephonyData miningPublic HealthRF-EMFbusinesscomputerbrain tumor
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IPHAS-selected classical Be stars

2016

We present a semi-automatic procedure to obtain fundamental physical parameters and distances of classical Be (CBe) stars, based on the Barbier-Chalonge-Divan (BCD) spectrophotometric system. Our aim is to apply this procedure to a large sample of CBe stars detected by the IPHAS photometric survey, to determine their fundamental physical parameters and to explore their suitability as galactic structure tracers. In this paper we describe the methodology used and the validation of the procedure by comparing our results with those obtained from different independent astrophysical techniques for subsamples of stars in common with other studies. We also present a test case study of the galactic …

Early type starsAstrophysics and AstronomyPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsStellar distanceAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital Librariesobservational astronomyStellar AstronomyEarly-type starsBe starsAstrophysics::Solar and Stellar AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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