Search results for "Shock wave"

showing 10 items of 194 documents

Metastable oxygen atom velocity and temperature in supersonic CO2plasma expansions

2008

Radial and axial velocity distribution functions of metastable oxygen atoms were obtained by way of resonant laser induced fluorescence spectroscopy at 777.19 nm in rarefied supersonic plasma jets produced from pure CO2 and CO2–N2 gas mixtures. The N2 seeded fraction is 3% in volume in order to mimic the Martian atmosphere composition. The measured lineshapes allow computation of the mean radial velocity and the perpendicular temperature, with respect to the jet axis, as well as the mean axial velocity and the parallel temperature. With an arcjet plasma source input power of 6.5 kW, the metastable O(5S) atom axial velocity is around 4500 m s−1 and the atom perpendicular temperature reaches …

Shock waveThermal equilibriumJet (fluid)Acoustics and UltrasonicsChemistryPlasmaCondensed Matter PhysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsRadial velocityDistribution functionAtomSupersonic speedAtomic physicsJournal of Physics D: Applied Physics
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X-ray emission from the Vela SNR shock region: Spectral fitting with a non-equilibrium ionization model

1994

We report on the 5′ scale spectral analysis of the X‐ray emission from a region near the edge of the Vela SNR with a Non‐Equilibrium Ionization (NEI) model. We have found significant variations of temperature, density, ionization time and interstellar absorption. We have identified an overdense region with higher density and lower temperature than the surrounding medium. That can be interpreted as an ISM cloudlet recently shocked by the blast wave, not yet in thermal equilibrium. Our independent determination of the Vela SNR distance is in agreement with the most recent results based on ROSAT All‐Sky Survey data. Our analysis indicates the occurrence of fast electron‐ion energy equipartitio…

Shock waveThermal equilibriumPhysicsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsVelaNeonchemistryIonizationROSATElectron temperatureAstrophysics::Galaxy AstrophysicsBlast waveAIP Conference Proceedings
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Spectral long-range interaction of temporal incoherent solitons.

2014

We study the interaction of temporal incoherent solitons sustained by a highly noninstantaneous (Raman-like) nonlinear response. The incoherent solitons exhibit a nonmutual interaction, which can be either attractive or repulsive depending on their relative initial distance. The analysis reveals that incoherent solitons exhibit a long-range interaction in frequency space, which is in contrast with the expected spectral short-range interaction described by the usual approach based on the Raman-like spectral gain curve. Both phenomena of anomalous interaction and spectral long-range behavior of incoherent solitons are described in detail by a long-range Vlasov equation.

Shock waveWave propagationIncoherent scatter01 natural sciences010305 fluids & plasmassymbols.namesakeOptics[ MATH.MATH-AP ] Mathematics [math]/Analysis of PDEs [math.AP][NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Quantum mechanics0103 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 physicsDispersion (water waves)ComputingMilieux_MISCELLANEOUSPhysicsbusiness.industrystatistical opticsVlasov equationAtomic and Molecular Physics and Optics[MATH.MATH-PR]Mathematics [math]/Probability [math.PR]Nonlinear systemsymbolsbusiness[ MATH.MATH-PR ] Mathematics [math]/Probability [math.PR]Raman scatteringCoherence (physics)Optics letters
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Recollimation shocks in relativistic jets

2018

Recollimation shocks (RS) appear associated with relativistic flows propagating through pressure mismatched atmospheres. Astrophysical scenarios invoking the presence of such shocks include jets from AGNs and X-ray binaries and GRBs. We shall start reviewing the theoretical background behind the structure of RS in overpressured jets. Next, basing on numerical simulations, we will focus on the properties of RS in relativistic steady jets threaded by helical magnetic fields depending on the dominant type of energy. Synthetic radio maps from the simulation of the synchrotron emission for a selection of models in the context of parsec-scale extragalactic jets will also be discussed.© 2018 World…

Shock waveactive [Galaxies]Radio galaxyAstrophysics::High Energy Astrophysical PhenomenaContext (language use)Astrophysics01 natural sciencesShock wavesMagnetohydrodynamicsAstrophysical jet0103 physical sciencesRadiation mechanisms: nonthermal010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsMathematical PhysicsPhysicsnumerical [Methods]Methods: numericalComputer simulation010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarGalaxies: activenonthermal [Radiation mechanisms]Magnetic fieldGalaxies: jetsSpace and Planetary Sciencejets [Galaxies]MagnetohydrodynamicsInternational Journal of Modern Physics D
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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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