Search results for "Cardinal point"

showing 10 items of 69 documents

Uncertainty quantification on a spatial Markov-chain model for the progression of skin cancer

2019

AbstractA spatial Markov-chain model is formulated for the progression of skin cancer. The model is based on the division of the computational domain into nodal points, that can be in a binary state: either in ‘cancer state’ or in ‘non-cancer state’. The model assigns probabilities for the non-reversible transition from ‘non-cancer’ state to the ‘cancer state’ that depend on the states of the neighbouring nodes. The likelihood of transition further depends on the life burden intensity of the UV-rays that the skin is exposed to. The probabilistic nature of the process and the uncertainty in the input data is assessed by the use of Monte Carlo simulations. A good fit between experiments on mi…

65C05Skin NeoplasmsComputer scienceQuantitative Biology::Tissues and OrgansMarkovin ketjut0206 medical engineeringMonte Carlo methodPhysics::Medical PhysicsBinary number02 engineering and technologyArticleihosyöpä03 medical and health sciencesMicemedicineAnimalsHumansComputer SimulationStatistical physicsUncertainty quantification60J20stokastiset prosessit030304 developmental biologyProbability0303 health sciencesMarkov chainApplied MathematicsProbabilistic logicUncertaintyState (functional analysis)medicine.disease020601 biomedical engineeringAgricultural and Biological Sciences (miscellaneous)Markov ChainsCardinal pointModeling and Simulation65C40Disease Progressionmatemaattiset mallitSkin cancerMonte Carlo MethodJournal of Mathematical Biology
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The cryogenic anticoincidence detector for ATHENA-XMS: preliminary results from the new prototype

2012

ATHENA has been the re-scoped IXO mission, and one of the foreseen focal plane instrument was the X-ray Microcalorimeter Spectrometer (XMS) working in the energy range 0.3-10 keV, which was a kilo-pixel array based on TES (Transition Edge Sensor) detectors. The need of an anticoincidence (AC) detector is legitimated by the results performed with GEANT4 simulations about the impact of the non x-ray background onto XMS at L2 orbit (REQ. < 0.02 cts/cm2/s/keV). Our consortium has both developed and tested several samples, with increasing area, in order to match the large area of the XMS (64 mm2). Here we show the preliminary results from the last prototype. The results achieved in this work off…

Anticoincidence detectorLow temperature DetectorAnticoincidence detectorsAstrophysicsOrbital mechanicslaw.inventionOpticslawElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringAnticoincidence detectors; High Energy Astrophysics; Low temperature Detectors; TES; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringPhysicsLow temperature DetectorsSpectrometerbusiness.industryApplied MathematicsElectronic Optical and Magnetic MaterialBolometerDetectorComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsApplied MathematicCardinal pointMillimeterSatelliteTransition edge sensorHigh Energy AstrophysicbusinessTESHigh Energy AstrophysicsSPIE Proceedings
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Visegrad Euroscepticism: Discursive Nodal Points in Eurosceptic Discourses Surrounding External Actions of the European Union

2018

Increasing support for Eurosceptic parties and movements can be observed in the European Union’s (EU) member states since 2009, when the economic crisis heavily affected the continent. This process has happened also within Central and Eastern European countries, especially in Poland, the Czech Republic, Slovakia and Hungary (collectively referred to as the Visegrad Group countries, or V4 for short). The goal of this paper is an analysis of far-right Eurosceptic politicians and their attitudes towards EU external actions. Using the Thomas Diez concept of discursive nodal points (DNPs) and examining European Parliament (EP) debates, literature about V4 Euroscepticism and media reports, this p…

Cardinal pointSociology and Political ScienceEU`s external actionPolitical economyPolitical sciencePolitical Science and International RelationsEuroscepticismmedia_common.cataloged_instanceConstructivismEuropean unionfar-rightVisegradmedia_commonOn-line Journal Modelling the New Europe
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Optical See-Through Head-Mounted Displays With Short Focal Distance: Conditions for Mitigating Parallax-Related Registration Error

2020

Optical see-through (OST) augmented reality head-mounted displays are quickly emerging as a key asset in several application fields but their ability to profitably assist high precision activities in the peripersonal space is still sub-optimal due to the calibration procedure required to properly model the user's viewpoint through the see-through display. In this work, we demonstrate the beneficial impact, on the parallax-related AR misregistration, of the use of optical see-through displays whose optical engines collimate the computer-generated image at a depth close to the fixation point of the user in the peripersonal space. To estimate the projection parameters of the OST display for a …

Computer sciencelcsh:Mechanical engineering and machineryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION01 natural sciencesCollimated lightlcsh:QA75.5-76.95Rendering (computer graphics)010309 opticsArtificial Intelligenceregistration0103 physical sciencesFocal lengthComputer visionlcsh:TJ1-1570Original Research010302 applied physicsRobotics and AIbusiness.industryoptical see-through displayscalibrationFixation pointaugmented realityComputer Science ApplicationsPhotogrammetryCardinal pointparallax related errorAugmented realityArtificial intelligencelcsh:Electronic computers. Computer scienceParallaxbusinessFrontiers in Robotics and AI
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Structural modelling and mechanical tests supporting the design of the ATHENA X-IFU thermal filters and WFI optical blocking filter

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. ATHENA is a Large high energy astrophysics space mission selected by ESA in the Cosmic Vision 2015-2025 Science Program. It will be equipped with two interchangeable focal plane detectors: the X-Ray Integral Field Unit (X-IFU) and the Wide Field Imager (WFI). Both detectors require x-ray transparent filters to fully exploit their sensitivity. In order to maximize the X-ray tra…

Cosmic VisionComputer scienceCondensed Matter PhysicBlocking (statistics)01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaWFI0103 physical sciencesSensitivity (control systems)Aerospace engineeringElectrical and Electronic Engineering010306 general physicsFEAX-IFU010308 nuclear & particles physicsbusiness.industryFilterElectronic Optical and Magnetic MaterialDetectorComputer Science Applications1707 Computer Vision and Pattern RecognitionTransparency (human–computer interaction)ATHENAVibrationApplied MathematicCardinal pointFilter (video)X-Raybusiness
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The TES-based cryogenic anticoincidence detector for IXO: First results from large area prototypes

2010

The technique which combines high resolution spectroscopy with imaging capability is a powerful tool to extract fundamental information in X-ray Astrophysics and Cosmology. TES (Transition Edge Sensors)-based microcalorimeters match at best the requirements for doing fine spectroscopy and imaging of both bright (high count rate) and faint (poor signal-to-noise ratio) sources. For this reason they are considered among the most promising detectors for the next high energy space missions and are being developed for use on the focal plane of the IXO (International X-ray Observatory) mission. In order to achieve the required signal-to-noise ratio for faint or diffuse sources it is necessary to r…

Cryogenic Detectors; IXO; SQUID; TES; X-ray; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringCryogenic DetectorsSQUIDSpace explorationX-raySignal-to-noise ratioOpticsSettore FIS/05 - Astronomia E AstrofisicaObservatoryElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringPhysicsSpectrometerPixelbusiness.industryApplied MathematicsDetectorPulse durationComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCardinal pointIXObusinessTES Cryogenic Detectors X-ray SQUID IXOTES
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The focal plane assembly for the Athena X-ray Integral Field Unit instrument

2016

This paper summarizes a preliminary design concept for the focal plane assembly of the X-ray Integral Field Unit on the Athena spacecraft, an imaging microcalorimeter that will enable high spectral resolution imaging and point-source spectroscopy. The instrument's sensor array will be a ~ 3840-pixel transition edge sensor (TES) microcalorimeter array, with a frequency domain multiplexed SQUID readout system allowing this large-format sensor array to be operated within the thermal constraints of the instrument's cryogenic system. A second TES detector will be operated in close proximity to the sensor array to detect cosmic rays and secondary particles passing through the sensor array for off…

CryostatPhysics::Instrumentation and DetectorsAperture01 natural sciencesfrequency division multiplexingfocal plane assemblySettore FIS/05 - Astronomia E AstrofisicaOpticsSensor array0103 physical sciencesElectronicSQUID amplifierAthenaOptical and Magnetic MaterialsElectrical and Electronic Engineeringta216010306 general physicsta113010302 applied physicsPhysicsX-IFUta114ta213business.industryStray lightApplied Mathematicstransition edge sensorDetectorAstrophysics::Instrumentation and Methods for AstrophysicsX-ray microcalorimeterComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCardinal pointElectromagnetic shieldingcryogenic anti-coincidence detectorX-ray microcalorimeter transition edge sensor cryogenic anti-coincidence detector SQUID amplifier frequency division multiplexing Athena X-IFU focal plane assemblyTransition edge sensorbusinessAthena; cryogenic anti-coincidence detector; focal plane assembly; frequency division multiplexing; SQUID amplifier; transition edge sensor; X-IFU; X-ray microcalorimeter; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringSPIE Proceedings
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Thermal Filters for the ATHENA X-IFU: Ongoing Activities Toward the Conceptual Design

2016

ATHENA is the L2 mission selected by ESA to pursue the science theme “Hot and Energetic Universe.” One of the two focal plane instruments is the X-ray Integral Field Unit, an array of TES microcalorimeters operated at T $$<$$ 100 mK. To allow the X-ray photons focused by the telescope to reach the detector, windows have to be opened on the cryostat thermal shields. X-ray transparent filters need to be mounted on these open windows to attenuate the IR radiation from warm surfaces, to attenuate RF electromagnetic interferences on TES sensors and SQUID electronics, and to protect the detector from contamination. This paper reviews the ongoing activities driving the design of the X-IFU thermal …

CryostatX-ray AstronomyAtomic and Molecular Physics and OpticATHENA; Thermal Filters; X-IFU; X-ray Astronomy; Condensed Matter Physics; Atomic and Molecular Physics and Optics; Materials Science (all)ShieldsCondensed Matter Physic01 natural sciencesThermal Filterlaw.invention010309 opticsTelescopeATHENA; Thermal Filters; X-IFU; X-ray Astronomy; Atomic and Molecular Physics and Optics; Materials Science (all); Condensed Matter PhysicsOpticsSettore FIS/05 - Astronomia E AstrofisicaConceptual designlawAtomic and Molecular Physics0103 physical sciencesGeneral Materials ScienceElectronics010303 astronomy & astrophysicsThermal FiltersPhysicsX-ray astronomyX-IFUbusiness.industryDetectorCondensed Matter PhysicsAtomic and Molecular Physics and OpticsATHENACardinal pointMaterials Science (all)and Opticsbusiness
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Third-harmonic light polarization control in magnetically resonant silicon metasurfaces

2021

Nonlinear metasurfaces have become prominent tools for controlling and engineering light at the nanoscale. Usually, the polarization of the total generated third harmonic is studied. However, diffraction orders may present different polarizations. Here, we design an high quality factor silicon metasurface for third harmonic generation and perform back focal plane imaging of the diffraction orders, which present a rich variety of polarization states. Our results demonstrate the possibility of tailoring the polarization of the generated nonlinear diffraction orders paving the way to a higher degree of wavefront control.

DiffractionEBLSiliconthird harmonic wave front control diffraction orders polarizationFOS: Physical scienceschemistry.chemical_elementPhysics::Optics02 engineering and technology01 natural sciences010309 opticsQuality (physics)Optics0103 physical sciencesnonlinear diffractionWavefrontPhysicsbusiness.industryNonlinear opticsSettore ING-INF/02 - Campi Elettromagnetici021001 nanoscience & nanotechnologyPolarization (waves)Atomic and Molecular Physics and OpticsNonlinear systemmetasurfaceCardinal pointchemistry0210 nano-technologybusinessthird harmonicOptics (physics.optics)Physics - Optics
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Focal plane array infrared camera transfer function calculation and image restoration

2004

Infrared images often present distortions induced by the measurement system. Image processing is thus an essential part of infrared measurements. A distortion model based on a convolution product is presented. The analytical form of the convolution kernel has been obtained from an image formation theory, along with an analysis of the sampling of the focal plane array camera detector's matrix. Image restoration is an ill-posed problem, and its solution can be obtained using regularization methods. In this work, image restoration is performed using a variation of Tikhonov regularization that makes use of the particular form of the convolution kernel matrix, which is built as a block-circulant…

DiffractionImage formationDiagonal formComputer sciencebusiness.industryDetectorGeneral EngineeringImage processingRegularization (mathematics)Atomic and Molecular Physics and OpticsConvolutionTikhonov regularizationMatrix (mathematics)Cardinal pointKernel (image processing)DistortionComputer visionArtificial intelligencebusinessImage restorationOptical Engineering
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