Search results for "Physics::Geophysics"

showing 10 items of 261 documents

Optical Frequency Combs Generated in Silica Microspheres in the Telecommunication C-, U-, and E-Bands

2021

Optical frequency combs (OFCs) generated in microresonators with whispering gallery modes are demanded for different applications including telecommunications. Extending operating spectral ranges is an important problem for wavelength-division multiplexing systems based on microresonators. We demonstrate experimentally three spectrally separated OFCs in the C-, U-, and E-bands in silica microspheres which, in principle, can be used for telecommunication applications. For qualitative explanation of the OFC generation in the sidebands, we calculated gain coefficients and gain bandwidths for degenerate four-wave mixing (FWM) processes. We also attained a regime when the pump frequency was in t…

Physics::OpticsSoliton (optics)MultiplexingPhysics::GeophysicsFour-wave mixingNonlinear Sciences::Adaptation and Self-Organizing Systemssilica microsphereDispersion (optics)Radiology Nuclear Medicine and imagingApplied optics. PhotonicsInstrumentationMixing (physics)PhysicsComputer simulationQuantitative Biology::Neurons and Cognitionbusiness.industryDegenerate energy levelsAtomic and Molecular Physics and OpticsTA1501-1820Raman OFCoptical frequency comb (OFC)Whispering-gallery wavefour-wave mixingTelecommunicationsbusinesssoliton-like spectrumPhotonics
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Cyclic fluctuations, climatic changes and role of noise in planktonic foraminifera in the Mediterranean Sea

2005

The study of Planktonic Foraminifera abundances permits to obtain climatic curves on the basis of percentage ratio between tropical and temperate/polar forms. Climatic changes were controlled by several phenomena as: (i) Milankovitch's cycles, produced by variations of astronomical parameters such as precession, obliquity and eccentricity; (ii) continental geodynamic evolution and orogenic belt; (iii) variations of atmospheric and oceanic currents; (iv) volcanic eruptions; (v) meteor impacts. But while astronomical parameters have a quasi-regular periodicity, the other phenomena can be considered as "noise signal" in natural systems. The interplay between cyclical astronomical variations, t…

Planktonic foraminiferaStochastic resonanceGeneral MathematicsGeneral Physics and AstronomyAtmospheric sciencesQuantitative Biology - Quantitative MethodsPhysics::GeophysicsForaminiferaMediterranean seaGlacial periodQuantitative Biology - Populations and EvolutionPlanktonic foraminifera; Climatic changes; Stochastic resonancePhysics::Atmospheric and Oceanic PhysicsQuantitative Methods (q-bio.QM)Milankovitch cyclesbiologyOcean currentPopulations and Evolution (q-bio.PE)biology.organism_classificationSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Climatic changeOceanographyFOS: Biological sciencesInterglacialPrecessionAstrophysics::Earth and Planetary AstrophysicsGeologyStochastic resonance
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Observation of the cosmic ray moon shadowing effect with the ARGO-YBJ experiment

2011

Cosmic rays are hampered by the Moon and a deficit in its direction is expected (the so-called Moon shadow). The Moon shadow is an important tool to determine the performance of an air shower array. Indeed, the westward displacement of the shadow center, due to the bending effect of the geomagnetic field on the propagation of cosmic rays, allows the setting of the absolute rigidity scale of the primary particles inducing the showers recorded by the detector. In addition, the shape of the shadow permits to determine the detector point spread function, while the position of the deficit at high energies allows the evaluation of its absolute pointing accuracy. In this paper we present the obser…

Point spread functionNuclear and High Energy PhysicsCosmic Rays Gamma Astronomy Extended Air ShowersAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodCosmic rayAstrophysics01 natural sciencesStandard deviationPhysics::GeophysicsRaggi cosmiciSettore FIS/05 - Astronomia E Astrofisicageomagnetic field0103 physical sciences010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsOmbra della lunaApparati di sciameDetectorSettore FIS/01 - Fisica SperimentaleMoon shadowAstronomyCosmic rayMagnetic fieldEarth's magnetic fieldAir shower13. Climate actionPhysics::Space Physics
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Adjoint-based inversion for porosity in shallow reservoirs using pseudo-transient solvers for non-linear hydro-mechanical processes

2020

Abstract Porous flow is of major importance in the shallow subsurface, since it directly impacts on reservoir-scale processes such as waste fluid sequestration or oil and gas exploration. Coupled and non-linear hydro-mechanical processes describe the motion of a low-viscous fluid interacting with a higher viscous porous rock matrix. This two-phase flow may trigger the initiation of solitary waves of porosity, further developing into vertical high-porosity pipes or chimneys. These preferred fluid escape features may lead to localised and fast vertical flow pathways potentially problematic in the case of for instance CO2 sequestration. Constraining the porosity and the non-linearly related pe…

PointwiseNumerical AnalysisPhysics and Astronomy (miscellaneous)Geophysical imagingApplied MathematicsFinite difference method010103 numerical & computational mathematicsMechanics01 natural sciencesPhysics::GeophysicsComputer Science ApplicationsPhysics::Fluid Dynamics010101 applied mathematicsComputational MathematicsNonlinear systemPermeability (earth sciences)Modeling and SimulationTwo-phase flow0101 mathematicsPorosityGradient descentGeologyJournal of Computational Physics
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Effects of Moisture and Stresses on the Structure and Properties of Polyester Resin

2004

The results of a complex study of structural changes in a cured Norpol 440 polyester resin under the action of damp environment and mechanical loading are presented. A considerable effect of absorbed moisture on the structure and some characteristics of the material is revealed by using thermophysical methods and X-ray diffractometry. The joint effect of moisture and mechanical stress is estimated by investigating the creep in stationary and nonstationary moisture conditions. The anisotropy of the material structure formed during creep is evaluated from the results of dilatometric measurements. It is found that the degree of anisotropy of the material after creep accompanied by moisture sor…

Polyester resinchemistry.chemical_classificationMaterials sciencePolymers and PlasticsMoistureGeneral MathematicsSorptionCondensed Matter PhysicsPhysics::GeophysicsBiomaterialsCreepchemistryMechanics of MaterialsSolid mechanicsCeramics and CompositesRelaxation (physics)Composite materialAnisotropyJoint (geology)Physics::Atmospheric and Oceanic PhysicsMechanics of Composite Materials
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Quasi-brittle porous material: Simulated effect of stochastic air void structure on compressive strength

2021

Abstract The effect of porosity comprised of spherical air voids on the compressive strength of quasi-brittle material was studied via simulations. The simulated porous structures were based on pore size distributions of two mortar samples measured by X-ray microtomography. While the simulation method set practical limits on the size of sample, the base of the statistics was established by simulating 128 small structures generated by sampling from pore structures of two mortars. By studying the application of the classical strength-porosity formulas to the simulated data, a new simple model was formed. A linear relationship was achieved between the cubic root of air void fraction (porosity)…

Pore sizeVoid (astronomy)Materials scienceScattering0211 other engineering and technologies02 engineering and technologyBuilding and Construction021001 nanoscience & nanotechnologyPhysics::GeophysicsCompressive strengthBrittlenessLinear relationship021105 building & constructionGeneral Materials ScienceComposite materialMortar0210 nano-technologyPorosityCement and Concrete Research
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The positioning system of the ANTARES Neutrino Telescope

2012

The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning sys…

Positioning systemDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Detector modelling and simulations II (electric fieldsDetector alignment and calibration methods (lasers sources particle-beams)01 natural sciencesTiming detectorshardwareDetector alignment and calibration methods010303 astronomy & astrophysicsInstrumentationDETECTOR ALIGMENTMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSOUND[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Orientation (computer vision)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsTriangulation (computer vision)particle-beams)GeodesyDETECTOR CONTROL SYSTEMDetector modelling and simulations II (electric fields charge transport multiplication and induction pulse formation electron emission etc)Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)sources[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pulse formationarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2DETECTOR MODELLING AND SIMULATIONSDetector modelling and simulations IIalgorithmsPhysics::Geophysics0103 physical sciences14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationetc)multiplication and inductionBuoyDetector control systems010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsMooringcharge transport[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Detector alignment and calibration methods (laserselectron emissionFISICA APLICADAdetector modelling and simulations ii (electric fields; antares neutrino telescope; multiplication and induction; charge transport; pulse formation; electron emission; etc); hardware; architecture; timing detectors; detector control systems (detector and experiment monitoring and slow-control systems; algorithms; databases); sources; detector alignment; calibration.; acoustic positioning; detector alignment and calibration methods (lasers; particle-beams)
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Constraining nonstandard neutrino-quark interactions with solar, reactor and accelerator data

2009

We present a reanalysis of nonstandard neutrino-down-quark interactions of electron and tau neutrinos using solar, reactor and accelerator data. In addition updating the analysis by including new solar data from SNO phase III and Borexino, as well as new KamLAND data and solar fluxes, a key role is played in our analysis by the combination of these results with the CHARM data. The latter allows us to better constrain the axial and axial-vector electron and tau-neutrino nonstandard interaction parameters characterizing the deviations from the Standard Model predictions.

QuarkHistoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhase (waves)FOS: Physical sciencesElectronEducationStandard ModelPhysics::GeophysicsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Charm (quantum number)Nuclear Experiment (nucl-ex)Neutrino oscillationNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)BorexinoSolar dataPhysicsNeutral currentHigh Energy Physics::PhenomenologyFísicaComputer Science ApplicationsHigh Energy Physics - PhenomenologyAstrophysics - Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentNeutrino
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Inter/intramolecular Cherenkov radiation energy transfer (CRET) from a fluorophore with a built-in radionuclide.

2014

The Cherenkov radiation (CR) from [(18)F]-FDG, [(177)Lu]-LuCl3 and [(90)Y]-YCl3 was detected and CR energy transfer (CRET) to several fluorophores was examined. Subsequent fluorescence emission was found to be a function of the position of absorption bands with respect to the CR peak, energy of emitted particles, radionuclide/fluorophore loading, and fluorophore brightness. A variant of the best fluorophore with a built-in radionuclide was synthesized to achieve inter- and intra-molecular CRET.

RadionuclideBrightnessFluorophoreChemistryAstrophysics::High Energy Astrophysical PhenomenaPhysics::Medical PhysicsMetals and AlloysAnalytical chemistryGeneral ChemistryFluorescenceCatalysisPhysics::GeophysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsPhysics::Popular Physicschemistry.chemical_compoundPhysics::Plasma PhysicsIntramolecular forceMaterials ChemistryCeramics and Composites[CHIM]Chemical Sciences[CHIM.OTHE]Chemical Sciences/OtherLuminescenceAbsorption (electromagnetic radiation)Cherenkov radiationChemical communications (Cambridge, England)
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Influence of spatial precipitation sampling on hydrological response at catchment scale

2014

Retrieving precipitation data from raingauge network is a classical and common practice in hydrology and climatology. These data represent the key input in hydrological modeling to reproduce, for example, the characteristics of a flood phenomenon. The accuracy of the model results is strongly dependent on the consistency of the monitoring network in terms of spatial scale, i.e. network density and location of raingauges, and time resolution. In this context, several studies have been carried out to analyze how the rainfall sampling influences the estimation of total runoff volume. The aim of this paper is to use a physically based and distributed-parameter hydrologic model to investigate ho…

Rain gaugeMeteorologyHydrological modellingSettore ICAR/02 - Costruzioni Idrauliche E Marittime E Idrologiahydrological modelSampling (statistics)Hydrographraingauges network; hydrological modelPhysics::GeophysicsRunoff modelClimatologySpatial ecologyEnvironmental ChemistryEnvironmental sciencePrecipitationraingauges networkVfloPhysics::Atmospheric and Oceanic PhysicsGeneral Environmental ScienceWater Science and TechnologyCivil and Structural Engineering
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