Search results for "methods [Diffusion Tensor Imaging]"

showing 10 items of 992 documents

Deep-learning based reconstruction of the shower maximum X max using the water-Cherenkov detectors of the Pierre Auger Observatory

2021

The atmospheric depth of the air shower maximum $X_{\mathrm{max}}$ is an observable commonly used for the determination of the nuclear mass composition of ultra-high energy cosmic rays. Direct measurements of $X_{\mathrm{max}}$ are performed using observations of the longitudinal shower development with fluorescence telescopes. At the same time, several methods have been proposed for an indirect estimation of $X_{\mathrm{max}}$ from the characteristics of the shower particles registered with surface detector arrays. In this paper, we present a deep neural network (DNN) for the estimation of $X_{\mathrm{max}}$. The reconstruction relies on the signals induced by shower particles in the groun…

showers: energylongitudinal [showers]interaction: modelPhysics::Instrumentation and DetectorsAstronomyCalibration and fitting methods; Cluster finding; Data analysis; Large detector systems for particle and astroparticle physics; Particle identification methods; Pattern recognition01 natural sciencesHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)Particle identification methodscluster findingsurface [detector]ObservatoryLarge detector systemsInstrumentationMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsPattern recognition cluster finding calibration and fitting methodsPhysicsSettore FIS/01 - Fisica Sperimentalemodel [interaction]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsData analysicalibration and fitting methodsenergy [showers]AugerobservatoryPattern recognition cluster finding calibration and fitting methodastroparticle physicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airneural networkAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Data analysisFOS: Physical sciences610Cosmic raydetector: fluorescencePattern recognition0103 physical sciencesddc:530High Energy Physicsddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]cosmic radiation: UHEstructureparticle physicsnetwork: performance010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Ciencias ExactasCherenkov radiationfluorescence [detector]Pierre Auger ObservatoryCalibration and fitting methodsmass spectrum [nucleus]showers: atmospheredetector: surfacehep-ex010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsCluster findingFísicaresolutioncalibrationComputational physicsperformance [network]Cherenkov counterAir showerLarge detector systems for particle and astroparticle physicExperimental High Energy PhysicsHigh Energy Physics::Experimentnucleus: mass spectrumshowers: longitudinalRAIOS CÓSMICOSEnergy (signal processing)astro-ph.IM
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A Telemetry, Tracking, and Command Antennas System for Small-Satellite Applications

2019

Circularly polarized (CP) antennas are used in space applications for telemetry tracking and command (TT&amp

small satellitesComputer Networks and CommunicationsFrequency bandTT&amplcsh:TK7800-836002 engineering and technologyTracking (particle physics)circular patchOpticsCircular patch; Circular polarization; Small satellites; TT&CComputer Science::Systems and ControlCTelemetryTelecommunications link0202 electrical engineering electronic engineering information engineeringElectrical and Electronic EngineeringCircular polarizationComputer Science::Information TheoryPatch antennaPhysicsbusiness.industryAxial ratio020208 electrical & electronic engineeringlcsh:ElectronicsAstrophysics::Instrumentation and Methods for Astrophysics020206 networking & telecommunicationsHardware and ArchitectureControl and Systems EngineeringPhysics::Space PhysicsSignal Processingcircular polarizationAntenna (radio)businessSmall satelliteElectronics
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Metodologiczne aspekty badań regionu śląskiego w okresie międzywojennym z socjologicznej perspektywy

2021

The paper demonstrates the methodologic aspect of the Polish sociologic research on the Silesian region in the interwar period. Referring to pre-sociologic and sociologic research, it depicts the methodologic foundations and intellectual perspectives that were conceptualised by ludwik krzy-wicki and constitute the cognitive basis for the construction of the knowledge about Silesia – they are defined as the object analysis current and the subject analysis current. The article illustrates the evolution of research methods – from the questionnaire technique, via the existing materials analy-sis, to Florian Znaniecki’s id method and the monographic method used in field research. it touches upon…

socio-geographic currentmetody i techniki badawczeresearch methods and techniquesmetodologianurt socjograficznypersonal ID methodSilesiamethodologymetoda dokumentów osobistychmetoda monograficznaŚląskmonographic methodStudia Śląskie
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On-Orbit Degradation of Solar Instruments

2013

International audience; We present the lessons learned about the degradation observed in several space solar missions, based on contributions at the Workshop about On-Orbit Degradation of Solar and Space Weather Instruments that took place at the Solar Terrestrial Centre of Excellence (Royal Observatory of Belgium) in Brussels on 3 May 2012. The aim of this workshop was to open discussions related to the degradation observed in Sun-observing instruments exposed to the effects of the space environment. This article summarizes the various lessons learned and offers recommendations to reduce or correct expected degradation with the goal of increasing the useful lifespan of future and ongoing s…

solar instruments[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010504 meteorology & atmospheric sciencesFOS: Physical sciencesSolar missionSpace weatherSpace (commercial competition)7. Clean energy01 natural sciencesSpace explorationDegradationContaminationObservatory0103 physical sciencesAerospace engineeringInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesbusiness.industryAstronomy and Astrophysicscon- taminationcalibrationspace environment[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceOrbit (dynamics)Environmental scienceAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSpace environmentDegradation (telecommunications)SOLAR PHYSICS
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La modélisation de l'information spatio-temporelle

2012

spatial dynamicsdynamiques spatiales[SHS.STAT]Humanities and Social Sciences/Methods and statistics[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistoryespace-tempsfonctions urbainesspaceHistorical sciencestemporalitémodellingurban functionspace-timeespace[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and PrehistorycityGeographical information systemtempsSystème d'information géographique[SHS.STAT] Humanities and Social Sciences/Methods and statisticsvilleSciences historiques[ SHS.STAT ] Humanities and Social Sciences/Methods and statisticstimemodélisation
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Understanding Urban Fabric with the OH_FET model based on Social Use, Space and Time

2008

The proposed principle for understanding the urban fabric is based on considering the town as a set of complex objects, taking a systemic approach. The town system used to study the urban fabric over large time spans is composed of three sub-systems relating to historical objects from the level of the excavation to that of the former urban space: function (social use), space (location, surface area and morphology) and time (dating, duration and chronology). The historical object is the analytical unit of the space studied. It is the Cartesian product of the three sets, Social use, Space and Time, from which it stems. On the basis of this process, the Historical Object (OH) is broken down in…

spatial dynamicshistorical sciences[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SHS.STAT]Humanities and Social Sciences/Methods and statistics[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistoryspacemodellingurban functioncity[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and Prehistory[SHS.STAT] Humanities and Social Sciences/Methods and statisticsGIS and cartographySurvey and excavationsSpace-time[ SHS.STAT ] Humanities and Social Sciences/Methods and statisticstimegeographical information system
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Methods for territorial intelligence

2006

Quantitative methods which are used by social sciences for thirty years can provide tools to help territorial actors better managing their territories. This short paper outlines an inventory of the kinds of methods that are usable within this framework.

spatial simulation[SHS.STAT]Humanities and Social Sciences/Methods and statistics[SHS.GEO] Humanities and Social Sciences/Geographysimulation spatialeinferential methodsexploratory methods[SHS.GEO]Humanities and Social Sciences/Geographyméthodes confirmatoires[ SHS.HISPHILSO ] Humanities and Social Sciences/History Philosophy and Sociology of Sciences[ SHS.GEO ] Humanities and Social Sciences/Geography[SHS.HISPHILSO]Humanities and Social Sciences/History Philosophy and Sociology of Sciencesméthodes exploratoires[SHS.HISPHILSO] Humanities and Social Sciences/History Philosophy and Sociology of Sciences[SHS.STAT] Humanities and Social Sciences/Methods and statisticsterritorial intelligence[ SHS.STAT ] Humanities and Social Sciences/Methods and statisticsIntelligence territorialeComputingMilieux_MISCELLANEOUS
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The Gaia-ESO Public Spectroscopic Survey

2012

The Gaia-ESO Public Spectroscopic Survey has begun and will obtain high quality spectroscopy of some 100000 Milky Way stars, in the field and in open clusters, down to magnitude 19, systematically covering all the major components of the Milky Way. This survey will provide the first homogeneous overview of the distributions of kinematics and chemical element abundances in the Galaxy. The motivation, organisation and implementation of the Gaia-ESO Survey are described, emphasising the complementarity with the ESA Gaia mission. Spectra from the very first observing run of the survey are presented.

spectroscopy stars kinematics abundancesSettore FIS/05 - Astronomia E AstrofisicaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy Astrophysics
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Characterization of a CZT focal plane small prototype for hard X-ray telescope

2005

The promise of good energy and spatial resolution coupled with high efficiency and room temperature operation has fuelled a large international effort to develop cadmium zinc telluride (CZT) for hard X-ray applications. We are involved on the development of a hard X-ray telescope based on multilayer optics and focal plane detector operative in the 10-80 keV energy range. This telescope requires a high efficiency focal plane providing both fine spatial resolution and spectroscopy with a compact and robust design. This paper reports preliminary results on the characterization both in spectroscopic and spatial response of two small pixellated CZT detectors (10times10times1 mm3 and 10times10tim…

spectroscopyNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsX-ray telescopeParticle detectorlaw.inventionTelescopechemistry.chemical_compoundOpticslawElectronicsElectrical and Electronic EngineeringImage resolutionPhysicsPixelbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsCadmium zinc tellurideCZTCardinal pointNuclear Energy and Engineeringchemistrypixel detectorfocal planehard X-rayOptoelectronicsbusinessIEEE Transactions on Nuclear Science
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THE ALHAMBRA SURVEY: EVOLUTION OF GALAXY SPECTRAL SEGREGATION

2016

arXiv:1601.03668v1

statistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of universeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesMethods statisticalGalaxies: distances and redshiftsMethods: data analysis0103 physical sciencesdistances and redshifts [Galaxies]observations [Cosmology]data analysis [Methods]010303 astronomy & astrophysicsMethods: statisticalAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsCosmology: observationsFísicaAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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