Search results for "WAVES"

showing 10 items of 1766 documents

Analysis of FBG reflection spectra under uniform and non-uniform transverse loads

2019

Loads applied transversely on the external surface of waveguides change their circular cross-sectional geometry generating birefringence. Due to this effect the reflected spectrum of a Fibre Bragg grating (FBG) undergoes a splitting of the single peak of the Bragg wavelength. In this work, we employed the Transfer Matrix Method (TMM) for x- and y-polarized wave-modes to model the uniform FBG reflection spectra for uniform and non-uniform transverse loads. We also performed experimental measurements for two different transverse load scenarios. The load profiles chosen for these experiments were applied on the FBG sensor through a block of steel and a roll bearing pin. Then, the modelled and …

polarizationtransverse loadsMaterials scienceBirefringencebirefringencebusiness.industryPhysics::Opticsuniform FBGStructural Health Monitoring (SHM)uniform FBG birefringence transverse loads transfer matrix Structural Health Monitoring (SHM) polarization.Polarization (waves)Transfer matrixSpectral lineTransverse planeWavelengthOpticsFiber Bragg gratingtransfer matrixbusinessGLUESettore ING-IND/04 - Costruzioni E Strutture Aerospaziali
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Zewnątrzustrojowa Fala Uderzeniowa (ESW) jako alternatywna metoda wspomagająca terapię porażenia spastycznego mięśni kończyn w wyniku udaru mózgu - p…

2017

Zewnątrzustrojowa fala uderzeniowa (ESW – Extracorporeal Shock Wave) jest czynnikiem fizykalnym, którego zastosowanie kliniczne obserwowane jest w szerokiej gamie zaburzeń chorobowych, szczególnie dysfunkcji narządu ruchu. Obecnie zaobserwować można, iż lista wskazań do zabiegów ESW stale rośnie i obejmuje swym zasięgiem coraz to bardziej odmienne pod względem etiologii i patomechanizmu schorzenia ogólnoustrojowe. Niemniej jednak pamiętać należy, iż potencjalne mechanizmy biologiczne stymulacji ESW, warunkujące korzystne i pożądane efekty terapeutyczne, nie są jednoznacznie wyjaśnione. W świecie nauki w dalszym ciągu obserwowany jest brak niepodważalnych dowodów popartych zaawansowanymi bad…

post-stroke spasticitymuscles’ hypertonianeurorehabilitationpoudarowa spastycznośćprzegląd piśmiennictwaliterature reviewfizjoterapiashock wavesneurorehabilitacjahipertonia mięśniowaphysiotherapyfala uderzeniowaWiadomości Lekarskie
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Evaluation of Clutch Plate Integrity with Non-Destructive Methods

2009

Abstract Nondestructive evaluation (NDE) represents an important phase in the life cycle of a product to detect defects both in service and in production. NDE techniques most commonly used to detect surface defects are visual inspection and methods based on eddy current and ultrasound. Laser and non-contact sensors have been recently used to inspect ultrasonically without contact. Components with complex geometry are usually inspected combining several NDE techniques, or simply visually where analysis and evaluation of results are performed by an operator based on specific parameters of acceptance. This last method is currently used to inspect the clutch plates since their complex geometry,…

product life cycle product control laser ultrasound guided wavesSettore ING-IND/15 - Disegno E Metodi Dell'Ingegneria Industriale
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Numerical treatment of radiation processes in the internal shocks of magnetized relativistic outflows

2017

Los blázares son un tipo de núcleo activo de galaxia (AGN, por sus siglas en inglés) que se encuentran entre los objetos astrofísicos más energéticos y violentos, a la par de los brotes de rayos gamma (GRB por sus siglas en inglés). Los procesos físicos y, en particular, el escenario del chorro relativista en el que se genera la radiación ultraenergética detectada por observatorios terrestres y en órbita, han conseguido atraer la atención e interés de los astrónomos y astrofísicos desde su descubrimiento. En la presente tesis investigamos el modelo de choques internos (IS) cuya hipótesis consta del choque de dos capas de plasma con geometría cilíndrica, formando dos ondas de choque que atra…

radiation mechanisms: thermalradiation mechanisms: nonthermalradiative transferthermal [radiation mechanisms]numerical methodsgeneral [bl lacertae objects]nonthermal [radiation mechanisms]shock wavesUNESCO::ASTRONOMÍA Y ASTROFÍSICAmagnetohydrodynamics:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]bl lacertae objects: general
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Topological canal foliations

2019

Regular canal surfaces of $\mathbb{R}^3$ or $\mathbb{S}^3$ admit foliations by circles: the characteristic circles of the envelope. In order to build a foliation of $\mathbb{S}^3$ with leaves being canal surfaces, one has to relax the condition “canal” a little (“weak canal condition”) in order to accept isolated umbilics. Here, we define a topological condition which generalizes this “weak canal” condition imposed on leaves, and classify the foliations of compact orientable 3-manifolds we can obtain this way.

rational parametrizationsQuantitative Biology::Tissues and OrgansGeneral MathematicsPhysics::Medical PhysicssurfacesTopology01 natural sciencesQuantitative Biology::Cell Behavior0103 physical sciencesotorhinolaryngologic diseases57R30[MATH]Mathematics [math]0101 mathematicsMathematicsEnvelope (waves)griddlingQuantitative Biology::Molecular Networks010102 general mathematicsOrder (ring theory)53C12foliationFoliation (geology)sense organsMathematics::Differential Geometry010307 mathematical physicscanal surfaceJournal of the Mathematical Society of Japan
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Rotational effects on the oscillation frequencies of newly born proto-neutron stars

2003

In this paper we study the effects of rotation on the frequencies of the quasi-normal modes of a proto-neutron star (PNS) born in a gravitational collapse during the first minute of life. Our analysis starts a few tenths of seconds after the PNS formation, when the stellar evolution can be described by a sequence of equilibrium configurations. We use the evolutionary models developed by Pons et al. (1999; 2001) that describe how a non rotating star cools down and contracts while neutrino diffusion and thermalization processes dominate the stellar dynamics. For assigned values of the evolution time, we set the star into slow rotation and integrate the equations of stellar perturbations in th…

relativityFOS: Physical sciencesmethods : numericalAstrophysicsAstrophysicsInstabilitystars : oscillationsmethods: numericalstars: neutronstars: rotationstars : rotationStellar dynamicsGravitational collapseAstrophysics::Solar and Stellar AstrophysicsTime domainStellar evolutionPhysicsgravitational waves; methods : numerical; methods: numerical; relativity; stars : neutron; stars : oscillations; stars : rotation; stars: neutron; stars: oscillations; stars: rotationAstrophysics (astro-ph)Astronomy and Astrophysicsstars : neutronNeutron stargravitational wavesSpace and Planetary ScienceFrequency domainstars: oscillationsAstrophysics::Earth and Planetary AstrophysicsNeutrinoMonthly Notices of the Royal Astronomical Society
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8-parameter solutions of fifth order to the Johnson equation

2019

We give different representations of the solutions of the Johnson equation with parameters. First, an expression in terms of Fredholm determinants is given; we give also a representation of the solutions written as a quotient of wronskians of order 2N. These solutions of order N depend on 2N − 1 parameters. When one of these parameters tends to zero, we obtain N order rational solutions expressed as a quotient of two polyno-mials of degree 2N (N +1) in x, t and 4N (N +1) in y depending on 2N −2 parameters. Here, we explicitly construct the expressions of the rational solutions of order 5 depending on 8 real parameters and we study the patterns of their modulus in the plane (x, y) and their …

rogue waves PACS numbers : 33Q55ratio- nal solutionswronskiansrational solutions[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]Johnson equation4710A-[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]37K104735Fg4754BdFredholm determinants
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From first to fourth order rational solutions to the Boussinesq equation

2020

Rational solutions to the Boussinesq equation are constructed as a quotient of two polynomials in x and t. For each positive integer N , the numerator is a polynomial of degree N (N + 1) − 2 in x and t, while the denominator is a polynomial of degree N (N + 1) in x and t. So we obtain a hierarchy of rational solutions depending on an integer N called the order of the solution. We construct explicit expressions of these rational solutions for N = 1 to 4.

rogue waves PACS numbers : 33Q55rational solutions[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]4710A-[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]37K104735Fg4754BdBoussinesq equation
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Experimental Observation of a Large Low-Frequency Band Gap in a Polymer Waveguide

2018

The quest for large and low-frequency band gaps is one of the principal objectives pursued in a number of engineering applications, ranging from noise absorption to vibration control, and to seismic wave abatement. For this purpose, a plethora of complex architectures (including multiphase materials) and multiphysics approaches have been proposed in the past, often involving difficulties in their practical realization. To address the issue of proposing a material design that enables large band gaps using a simple configuration, in this study we propose an easy-to-manufacture design able to open large, low-frequency complete Lamb band gaps exploiting a suitable arrangement of masses and stif…

scanning laser Doppler vibrometerAbsorption (acoustics)Materials scienceBand gapAcousticsMaterials Science (miscellaneous)Vibration control02 engineering and technologyLow frequencyLamb band gaplcsh:Technology01 natural sciencesNoise (electronics)finite element simulationsLamb wavesphononic crystals and metamaterials; Lamb band gap; guided waves; finite element simulations; scanning laser Doppler vibrometer0103 physical sciencesCenter frequency010306 general physicsComputingMilieux_MISCELLANEOUS[PHYS]Physics [physics]guided waveslcsh:TIsotropyFinite element simulations; Guided waves; Lamb band gap; Phononic crystals and metamaterials; Scanning laser Doppler vibrometerphononic crystals and metamaterials021001 nanoscience & nanotechnology0210 nano-technology
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Fast changes in the morphology of the X-ray emitting shocks in HH 154

2006

Our recent second epoch Chandra observations have shown a fast morphological evolution of the X-ray source associated with the protostellar jet HH 154 (Fig.\ 1). We propose to study the evolution of the optical structures in the jet, specially the ones associated with the X-ray emission with a monitoring program of imaging narrow and broad band optical observations. We will determine the proper motions (and braking) of the optical knows associated with shock features and the evolution of their line luminosity and therefore their cooling time. These data, together with our past and future X-ray observations, constitute a fundamental input and constraint to our parallel program of ongoing hyd…

shock waves ISM: Herbig-Haro objects ISM: jets and outflows
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