Search results for "Shock"

showing 10 items of 1248 documents

Analysis of laser shock waves and resulting surface deformations in an Al-Cu-Li aluminium alloy

2012

Abstract Laser shock processing is now a recognized surface treatment for improving fatigue or corrosion behaviour of metallic materials through the generation of a compressive stress field. In turn, the analysis of shock wave propagation is of primary importance to predict numerically morphological and mechanical surface modifications. Considering experimental and numerical analyses of shock wave propagation, and surface deformations induced by single impacts, a 2050 aluminum alloy having different microstructures was investigated under laser-shock loading. In a first step, the evolution of shock wave attenuation and elastic precursor amplitude was correctly reproduced by finite element si…

Shock wavematière Condensée: Science des matériaux [Physique]Materials sciencechocMatériaux [Sciences de l'ingénieur]Acoustics and UltrasonicsField (physics)Constitutive equation02 engineering and technology01 natural sciences[SPI.MAT]Engineering Sciences [physics]/MaterialsResidual stress0103 physical sciencesComposite materialMécanique: Mécanique des matériaux [Sciences de l'ingénieur]010302 applied physicsaluminiumsimulation numérique021001 nanoscience & nanotechnologyCondensed Matter PhysicsMicrostructureFinite element methodSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsShock (mechanics)laserAmplitudeSIMULATION0210 nano-technology
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Überprüfung der Läsionsgefahr des N. ischiadicus des Kaninchens durch die Applikation niedrig- und mittelenergetischer extrakorporaler Stoßwellen

2008

Aim The aim of the study was to evaluate the likeliness for peripheral nerve lesions following extracorporeal shock wave application. Material and method 82 rabbit sciatic nerves were randomized to undergo low-energetic (0.08 mJ/mm2), middle-energetic (0.28 mJ/mm2) or no (controls) shock wave therapy. After 1 to 28 days an independent neuropathologist checked the specimen for signs of neural lesions. Results Only after 14 and 28 days vacuolic swelling of the axons was noted, somewhat pronounced in the middle-energetic group. In no case was there any disruption of the nerve's continuity. We did not observe any neurapraxia. Conclusion Shock wave application does not threaten peripheral nerve …

Shock wavemedicine.medical_specialtyLagomorphabiologybusiness.industryNeurapraxiabiology.organism_classificationmedicine.diseaseExtracorporealSurgeryLesionAnesthesiamedicineOrthopedics and Sports MedicineSurgeryHistopathologySciatic nervemedicine.symptombusinessComplicationZeitschrift für Orthopädie und ihre Grenzgebiete
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Electromagnetically generated extracorporeal shock waves for gallstone lithotripsy: in vitro experiments and clinical relevance.

1989

. First generation shock wave sources have been proved to disintegrate gallstones effectively, but they require the immersion of the patient's body in a tank of water. A recently developed second generation shock wave source (Siemens-Lithostar, Erlangen, FRG) generates shock waves electromagnetically. It presents several novel features. In particular the waterbath can be omitted and due to lower shock wave pressure general anaesthesia is not required. In vitro studies showed that 36 out of 38 gallstones (11–30 mm in diameter) could be disintegrated. Two concrements resisting lithotripsy were pure white cholesterol stones. Independent of shape, size, and composition (cholesterol or pigment) …

Shock wavemedicine.medical_specialtyMaterials sciencemedicine.medical_treatmentClinical BiochemistryGeneral MedicineGallstonesLithotripsyIn Vitro Techniquesmedicine.diseaseBiochemistryExtracorporeal shock wave lithotripsyExtracorporealFirst generationSurgeryMaximum diameterCholelithiasisLithotripsymedicineHumansTomography X-Ray ComputedElectromagnetic PhenomenaBiomedical engineeringEuropean journal of clinical investigation
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Extracorporeal Shock Wave Lithotripsy of Ureteral Stones: Clinical Experience and Experimental Findings

1986

AbstractESWL of impacted ureteral or caliceal stones is not as successful as expected. To study this problem a model for extracorporeal shock wave lithotripsy of ureteral stones has been designed. After initial fragmentation of the outer shell of impacted stones during the first series of shock wave application those fragments are kept in place by external mucosal contact, creating a lot of new interfaces.Absorption or reflection of shock wave energy within this fragmented shell seems to be responsible for the poor success rate in these cases. In regard to our experimental and clinical results we advise pushing ureteral stones back into the renal collecting system by means of a ureteral cat…

Shock wavemedicine.medical_specialtyUreteral Calculiurogenital systembusiness.industryUrologymedicine.medical_treatmentIn Vitro Techniquesurologic and male genital diseasesCollection systemExtracorporeal shock wave lithotripsyfemale genital diseases and pregnancy complicationsSurgeryModels StructuralKidney CalculiLithotripsymedicineHumansbusinessUrethral catheterJournal of Urology
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High-order regularization in lattice-Boltzmann equations

2017

A lattice-Boltzmann equation (LBE) is the discrete counterpart of a continuous kinetic model. It can be derived using a Hermite polynomial expansion for the velocity distribution function. Since LBEs are characterized by discrete, finite representations of the microscopic velocity space, the expansion must be truncated and the appropriate order of truncation depends on the hydrodynamic problem under investigation. Here we consider a particular truncation where the non-equilibrium distribution is expanded on a par with the equilibrium distribution, except that the diffusive parts of high-order nonequilibrium moments are filtered, i.e., only the corresponding advective parts are retained afte…

Shock waverecurrence relationspolynomialsComputational MechanicsLattice Boltzmann methods114 Physical sciences01 natural sciences010305 fluids & plasmassubspaces0103 physical sciences010306 general physicsFluid Flow and Transfer ProcessesPhysicstensor methods: shock tubesHermite polynomialsRecurrence relationta114AdvectionMechanical EngineeringpolynomitMathematical analysisCondensed Matter PhysicsDistribution functionMechanics of MaterialsRegularization (physics)shock tubes [tensor methods]Shear flowPhysics of Fluids
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Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment

2018

Monthly notices of the Royal Astronomical Society 479(3), 4253 - 4270 (2018). doi:10.1093/mnras/sty1750

Shock waveshock wave010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesISM: magnetic field0103 physical sciencesRadiative transferAdiabatic process010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicssupernova remnants [ISM]magnetic fields [ISM]Astronomy and Astrophysicsshock wavesAstronomy and Astrophysic520Magnetic fieldSupernovaSpace and Planetary Scienceddc:520Oblique shockMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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MODELING SNR CASSIOPEIA A from the SUPERNOVA EXPLOSION to ITS CURRENT AGE: The ROLE of POST-EXPLOSION ANISOTROPIES of EJECTA

2016

The remnants of core-collapse supernovae (SNe) have complex morphologies that may reflect asymmetries and structures developed during the progenitor SN explosion. Here we investigate how the morphology of the SNR Cassiopeia A (Cas A) reflects the characteristics of the progenitor SN with the aim to derive the energies and masses of the post-explosion anisotropies responsible for the observed spatial distribution of Fe and Si/S. We model the evolution of Cas A from the immediate aftermath of the progenitor SN to the three-dimensional interaction of the remnant with the surrounding medium. The post-explosion structure of the ejecta is described by small-scale clumping of material and larger-s…

Shock waveshock waveFOS: Physical sciencesCosmic rayAstrophysicsKinetic energy01 natural sciencessupernova remnants; shock waves; supernovae: individual (Cassiopeia A); Space and Planetary Science; Astronomy and Astrophysics [cosmic rays; hydrodynamics; instabilities; ISM]0103 physical sciencessupernovae: individual (Cassiopeia A)hydrodynamics instabilitiesAnisotropyEjecta010303 astronomy & astrophysicsCosmic rayscosmic rayISM: supernova remnantISM: supernova remnantshydrodynamicHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsinstabilitie010308 nuclear & particles physicsCosmic rays hydrodynamics instabilities ISM: supernova remnants shock waves;supernovae: individual (Cassiopeia A)Astronomy and Astrophysicsshock wavesCassiopeia ASupernovaSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Impact of self-steepening on incoherent dispersive spectral shocks and collapse-like spectral singularities

2014

International audience; Incoherent dispersive shock waves and collapselike singularities have been recently predicted to occur in the spectral evolution of an incoherent optical wave that propagates in a noninstantaneous nonlinear medium. Here we extend this work by considering the generalized nonlinear Schrödinger equation. We show that self-steepening significantly affects these incoherent spectral singularities: (i) It leads to a delay in the development of incoherent dispersive shocks, and (ii) it arrests the incoherent collapse singularity. Furthermore, we show that the spectral collapselike behavior can be exploited to achieve a significant enhancement (by two orders of magnitudes) of…

Shock wavespecklesIncoherent scatterDegree of coherencespeckles steepening shock waves01 natural sciencesNO010305 fluids & plasmasSingularity[ MATH.MATH-AP ] Mathematics [math]/Analysis of PDEs [math.AP][NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Quantum mechanicsNonlinear medium0103 physical sciences[MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP][ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]010306 general physicsPhysicsstatistical opticsshock wavesAtomic and Molecular Physics and Optics[MATH.MATH-PR]Mathematics [math]/Probability [math.PR]Nonlinear systemQuantum electrodynamicsGravitational singularitysteepening[ MATH.MATH-PR ] Mathematics [math]/Probability [math.PR]Coherence (physics)
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Laboratory evidence for asymmetric accretion structure upon slanted matter impact in young stars

2020

Aims. Investigating the process of matter accretion onto forming stars through scaled experiments in the laboratory is important in order to better understand star and planetary system formation and evolution. Such experiments can indeed complement observations by providing access to the processes with spatial and temporal resolution. A previous investigation revealed the existence of a two-component stream: a hot shell surrounding a cooler inner stream. The shell was formed by matter laterally ejected upon impact and refocused by the local magnetic field. That laboratory investigation was limited to normal incidence impacts. However, in young stellar objects, the complex structure of magne…

Shock wavestarsAccretionMagnetohydrodynamics (MHD)Young stellar objectFOS: Physical sciencesX-rays: starsAstrophysics01 natural sciencesShock wavesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsEjecta010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicspre-main sequence -X-raysAstronomy and AstrophysicsPlasmaPlanetary system[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]accretion disks -instabilities -magnetohydrodynamics (MHD) -shock waves -starsAccretion (astrophysics)StarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceInstabilitiesAccretion disksStars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Supernova 1987A: a Template to Link Supernovae to their Remnants

2015

The emission of supernova remnants reflects the properties of both the progenitor supernovae and the surrounding environment. The complex morphology of the remnants, however, hampers the disentanglement of the two contributions. Here we aim at identifying the imprint of SN 1987A on the X-ray emission of its remnant and at constraining the structure of the environment surrounding the supernova. We performed high-resolution hydrodynamic simulations describing SN 1987A soon after the core-collapse and the following three-dimensional expansion of its remnant between days 1 and 15000 after the supernova. We demonstrated that the physical model reproducing the main observables of SN 1987A during …

Shock wavesupernovae: individual (SN 1987A)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPower lawSpectral lineGravitational collapseAstrophysics::Solar and Stellar AstrophysicsHydrodynamics instabilities ISM: supernova remnants shock waves supernovae: individual (SN 1987A) X-rays: ISM.EjectaAstrophysics::Galaxy AstrophysicsISM: supernova remnantsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNebulaAstronomy and AstrophysicsObservableshock wavesX-rays: ISMhydrodynamics instabilities ISM: supernova remnants shock waves supernovae: individual: SN 1987A X-rays: ISMSupernovainstabilitiesSpace and Planetary ScienceHydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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