Search results for "Aga"

showing 10 items of 4366 documents

Wizja religii cesarstwa rzymskiego według Tertuliana na podstawie "Apologetyka"

2019

Artykuł prezentuje myśli Tertuliana na temat religii pogańskiej i chrześcijańskiej w Cesarstwie Rzymskim w II w., które zawarł w Apologetyku. W poszczególnych punktach artykułu są prezentowane porównania religii chrześcijańskiej z pogańską. Po przedstawieniu argumentów Tertuliana można stwierdzić, że nawołuje on wszystkich pogan, aby zostali chrześcijanami. Tylko w chrześcijaństwie odnajduje on prawdziwie Boga oraz czystość obyczajów, których nie ma w religiach pogańskich. Dzięki Tertulianowi poznajemy kształtowanie się chrześcijaństwa w dwóch pierwszych wiekach, a także kulty i obyczaje pogan.

"Apologetyk"chrześcijaństwopogaństworeligiaTertullianreligionpaganism"Apologeticum"TertulianChristianityStudia Teologiczno-Historyczne Śląska Opolskiego
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Discrete spectral incoherent solitons in nonlinear media with noninstantaneous response

2011

International audience; We show theoretically that nonlinear optical media characterized by a finite response time may support the existence of discrete spectral incoherent solitons. The structure of the soliton consists of three incoherent spectral bands that propagate in frequency space toward the low-frequency components in a discrete fashion and with a constant velocity. Discrete spectral incoherent solitons do not exhibit a confinement in the space-time domain, but exclusively in the frequency domain. The kinetic theory describes in detail all the essential properties of discrete spectral incoherent solitons: A quantitative agreement has been obtained between simulations of the kinetic…

01 natural sciencesoptical instabilitiesSchrödinger equation010309 opticssymbols.namesakeand lossesQuantum mechanics0103 physical sciencesDispersion (optics)Dynamics of nonlinear optical systemsOptical solitonssolitons010306 general physicsPropagationNonlinear Schrödinger equationNonlinear Sciences::Pattern Formation and SolitonsPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]and optical spatio-temporal dynamicsscatteringWave equationAtomic and Molecular Physics and OpticsSupercontinuumNonlinear systemFrequency domainsymbolsoptical chaos and complexitySolitonnonlinear guided waves
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Generalised bisection method for optimum ultrasonic ray tracing and focusing in multi-layered structures

2021

Ultrasonic testing has been used for many decades, proving itself very efficient for detecting defects in many industrial sectors. The desire to apply ultrasonic testing to geometrically complex structures, and to anisotropic, inhomogeneous materials, together with the advent of more powerful electronics and software, is constantly pushing the applicability of ultrasonic waves to their limits. General ray tracing models, suitable for calculating the proper incident angle of single element probes and the proper time delay of phased array, are currently required. They can support the development of new imaging techniques, as Full Matrix Capture and Total Focusing Method, and the execution of …

010302 applied physicsAcoustics and UltrasonicsComputer scienceIterative methodbusiness.industryTKComputationUltrasonic testing01 natural sciencesRay tracing (physics)Settore ING-IND/14 - Progettazione Meccanica E Costruzione Di MacchineSoftware0103 physical sciencesBisection methodUltrasonic wave propagation Ray tracing Mathematical modelling Bisection method Multi-layered structures Weld inspection CompositesA priori and a posterioriUltrasonic sensorbusiness010301 acousticsAlgorithmUltrasonics
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Savaime sklindančios aukštatemperatūrinės sintezės būdu gautų aliuminio oksinitrido miltelių ir jų keramikų optinės savybės

2021

The reported study was funded by RFBR according to the Research Project No. 19-08-00655. V.P. acknowledges the State Research Program ‘Aug-stas enerģijas fizika un paātrinātāju tehnoloģijas’ (Projekta Nr. VPP-IZM-CERN-2020/1-0002). The Institute of Solid State Physics, University of Latvia as the Center of Excellence has received funding from the H2020-WIDESPREAD-01-2016-2017-Teaming Phase2 under Grant Agreement No. 739508, Project CAMART2.

010302 applied physicsAluminium oxynitrideMaterials scienceAlONOptical propertiesAluminium oxynitrideSelf-propagating high-temperature synthesisGeneral Physics and AstronomyCombustion02 engineering and technology021001 nanoscience & nanotechnology01 natural scienceschemistry.chemical_compoundchemistryvisual_art0103 physical sciencesvisual_art.visual_art_medium:NATURAL SCIENCES [Research Subject Categories]Transparent ceramicsCeramicComposite material0210 nano-technologySelf-propagating high-temperature synthesis
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A multilayer model for self-propagating high-temperature synthesis of inter-metallic compounds

2007

International audience; Self-propagating high-temperature synthesis of intermetallic compounds is of wide interest. We consider reactions in a binary system in which the rise and fall of the temperature during the reaction is such that one of the reacting metals melts but not the other. For such a system, using the phase diagram of the binary system, we present a general theory that describes the reaction taking place in a single solid particle of one component surrounded by the melt of the second component. The theory gives us a set of kinetic equations that describe the propagation of the phase interfaces in the solid particle and the change in composition of the melt that surrounds it. I…

010302 applied physicsMaterials scienceComponent (thermodynamics)IntermetallicSelf-propagating high-temperature synthesisBinary compoundThermodynamics02 engineering and technology021001 nanoscience & nanotechnologySystem of linear equations01 natural sciencesSurfaces Coatings and Filmschemistry.chemical_compoundCrystallography[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]chemistryPhase (matter)0103 physical sciencesMaterials ChemistryBinary system[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Physical and Theoretical Chemistry0210 nano-technologyPhase diagram
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Stable and simple quantitative phase-contrast imaging by Fresnel biprism

2018

Digital holographic (DH) microscopy has grown into a powerful nondestructive technique for the real-time study of living cells including dynamic membrane changes and cell fluctuations in nanometer and sub-nanometer scales. The conventional DH microscopy configurations require a separately generated coherent reference wave that results in a low phase stability and a necessity to precisely adjust the intensity ratio between two overlapping beams. In this work, we present a compact, simple, and very stable common-path DH microscope, employing a self-referencing configuration. The microscope is implemented by a diode laser as the source and a Fresnel biprism for splitting and recombining the be…

010302 applied physicsMaterials scienceMicroscopePhysics and Astronomy (miscellaneous)business.industryPhase-contrast imagingHolographyÒpticaLaserInterference (wave propagation)Holographic interferometry01 natural scienceslaw.invention010309 opticsOptical axisMicroscòpiaOpticslaw0103 physical sciencesMicroscopybusinessApplied Physics Letters
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Broadband microwave emission spectrum associated with kinetic instabilities in minimum-B ECR plasmas

2017

Plasmas of electron cyclotron resonance ion sources (ECRISs) are prone to kinetic instabilities due to the resonant heating mechanism resulting in anisotropic electron velocity distribution. Frequently observed periodic oscillations of extracted ion beam current in the case of high plasma heating power and/or strong magnetic field have been proven to be caused by cyclotrontype instabilities leading to a notable reduction and temporal variation of highly charged ion production. Thus, investigations of such instabilities and techniques for their suppression have become important topics in ECRIS research. The microwave emission caused by the instabilities contains information on the electron e…

010302 applied physicsPhysicsRange (particle radiation)microwave sourcesIon sourcesIon beamta114Highly charged ionPlasmaAstrophysics::Cosmology and Extragalactic Astrophysicsplasma instabilitiesmagnetic fieldsCondensed Matter PhysicsPlasma oscillationmagneettikentät01 natural sciences7. Clean energyElectron cyclotron resonanceIonPhysics::Plasma Physicsmicrowave spectra0103 physical sciencesAtomic physics010306 general physicsMicrowave
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Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

2020

We present measurements of the large-scale cosmic-ray anisotropies in right ascension, using data collected by the surface detector array of the Pierre Auger Observatory over more than 14 years. We determine the equatorial dipole component, ~d⊥, through a Fourier analysis in right ascension that includes weights for each event so as to account for the main detector-induced systematic effects. For the energies at which the trigger efficiency of the array is small, the “East-West” method is employed. Besides using the data from the array with detectors separated by 1500 m, we also include data from the smaller but denser sub-array of detectors with 750 m separation, which allows us to extend …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsAstrophysicsanisotropy [cosmic radiation]Amplitude01 natural sciencessurface [detector]010303 astronomy & astrophysicsRight ascensionastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSGalactic CenterAstrophysics::Instrumentation and Methods for AstrophysicsCosmic RaysAugerobservatoryAmplitudePhysics::Space PhysicsAstrophysics - High Energy Astrophysical PhenomenaExtragalactic cosmic rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raycosmic radiation: anisotropyExtragalactic cosmic rayGalactic center0103 physical sciencesHigh Energy PhysicsPierre auger observatory0105 earth and related environmental sciencesPierre Auger Observatorydetector: surfaceFísicaAstronomy and AstrophysicsCosmic rayefficiency [trigger]GalaxyDipole* Automatic Keywords *Space and Planetary ScienceExperimental High Energy Physicstrigger: efficiencyddc:520galaxyDipoleObservatoryEnergy (signal processing)anisotropiesRight ascension[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)dipoleThe Astrophysical Journal
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Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart

2020

We study the impact of gas accretion on the orbital evolution of black-hole binaries initially at large separation in the band of the planned Laser Interferometer Space Antenna (LISA). We focus on two sources: (i)~stellar-origin black-hole binaries~(SOBHBs) that can migrate from the LISA band to the band of ground-based gravitational-wave observatories within weeks/months; and (ii) intermediate-mass black-hole binaries~(IMBHBs) in the LISA band only. Because of the large number of observable gravitational-wave cycles, the phase evolution of these systems needs to be modeled to great accuracy to avoid biasing the estimation of the source parameters. Accretion affects the gravitational-wave p…

010504 meteorology & atmospheric sciencesAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)Observableastro-ph.HE; astro-ph.HE; General Relativity and Quantum Cosmologygas: accretionblack holes gravitational wavesobservatoryInterferometrygravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenainterferometermedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational radiation: direct detectionelectromagnetic field: productionGeneral Relativity and Quantum Cosmologybinary: coalescencestatistical analysisSettore FIS/05 - Astronomia e Astrofisicagravitation: weak field0103 physical sciencesnumerical calculationsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLISAGravitational wavegravitational radiationOrder (ring theory)black hole: accretionAstronomy and Astrophysicsblack holesgravitational radiation detectorRedshiftBlack holeblack hole: binarySpace and Planetary ScienceSkygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray: detectorThe Astrophysical Journal
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X-ray emission from young brown dwarfs in the Orion Nebula Cluster

2005

We use the sensitive X-ray data from the Chandra Orion Ultradeep Project (COUP) to study the X-ray properties of 34 spectroscopically-identified brown dwarfs with near-infrared spectral types between M6 and M9 in the core of the Orion Nebula Cluster. Nine of the 34 objects are clearly detected as X-ray sources. The apparently low detection rate is in many cases related to the substantial extinction of these brown dwarfs; considering only the BDs with $A_V \leq 5$ mag, nearly half of the objects (7 out of 16) are detected in X-rays. Our 10-day long X-ray lightcurves of these objects exhibit strong variability, including numerous flares. While one of the objects was only detected during a sho…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)Brown dwarfFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStellar classificationAstrophysics01 natural sciencesSpectral linelaw.invention[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]law0103 physical sciencesOrion NebulaAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsEffective temperatureStarsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsFlare
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