Search results for "Shock wave"

showing 10 items of 194 documents

Low-frequency extracorporeal shock wave lithotripsy improves renal pelvic stone disintegration in a pig model.

2009

OBJECTIVE To compare disintegration rates for renal stones treated by 60 vs 120 shock waves (SW)/min at the same energy settings, using standardized validated artificial stones in a pig model. MATERIALS AND METHODS Gypsum artificial stones (13 × 6 mm) were inserted into the renal pelvis on either side of 12 anaesthetized pigs by open surgery. Extracorporeal SW lithotripsy (ESWL) was applied using a new electromagnetic lithotripter (Lithoskop®, Siemens AG Healthcare, Munich, Germany) at 60 and 120 SW/min; 3000 SW were applied to each kidney with the same energy settings. Stone fragments were collected after nephrectomy, passed through calibrated test sieves, and weighed. Fragment size catego…

Nephrologymedicine.medical_specialtyKidneybusiness.industrySwineUrologymedicine.medical_treatmentLithotripsymedicine.diseaseExtracorporeal shock wave lithotripsyNephrectomyExtracorporealSurgeryKidney Calculimedicine.anatomical_structureTreatment OutcomeInternal medicineLithotripsymedicineAnimalsNuclear medicinebusinessRenal pelvisKidney diseaseBJU international
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Surgical aspects of urolithiasis in children.

1991

Operative management of renal calculi has changed radically in the last decade. New operative techniques. the use of intra-operative ultrasound and Doppler sonography have even made possible the removal of complete staghorn calculi in short and kidney-preserving procedures. The introduction of percutaneous nephrolithotomy and stone extraction using a specially designed ureteroscope and, above all, the clinical application of extracorporeal shock wave lithotripsy have made stone surgery less invasive and have provided a higher rate of preservation of kidney function.

Nephrologymedicine.medical_specialtyURETEROSCOPEmedicine.diagnostic_testbusiness.industrymedicine.medical_treatmentUltrasoundEndoscopyLithotripsyExtracorporeal shock wave lithotripsySurgeryLithotomy positionEndoscopyKidney CalculiNephrologyInternal medicineLithotripsyPediatrics Perinatology and Child HealthPreoperative CaremedicineHumansUrinary CalculiPercutaneous nephrolithotomybusinessPediatric nephrology (Berlin, Germany)
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Extracorporeal shock wave lithotripsy (ESWL): alternatives and adjuvant procedures

1985

Within a short time, extensive statistics on ESWL have documented its efficiency in the treatment of most renal and ureteral stones. Approximately 20% of all stone patients, however, require additional or other forms of therapy, such as URS, PNL, or surgery. Up to now, the differential indications for these procedures have not been completely established. A crucial factor for successful application of ESWL is stone volume and localization. Large stones with a central stone mass may be successfully treated by combining ESWL and PNL, while surgery is still preferred in those with a peripheral stone mass.

Nephrologymedicine.medical_specialtybusiness.industryUrologymedicine.medical_treatmentInternal medicineUreteral stonemedicineShock wave lithotripsyLithotripsybusinessExtracorporeal shock wave lithotripsySurgeryWorld Journal of Urology
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Detailed characterization of laboratory magnetized super-critical collisionless shock and of the associated proton energization

2021

Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of nonthermal particles and high-energy radiation. In the absence of particle collisions in the system, theory shows that the interaction of an expanding plasma with a pre-existing electromagnetic structure (as in our case) is able to induce energy dissipation and allow shock formation. Shock formation can alternatively take place when two plasmas interact, through microscopic instabilities inducing electromagnetic fields that are able in turn to mediate energy dissipation and shock formation. Using our platform in which we couple a rapidly expanding plasma induced by high-power lasers (JLF/Titan…

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmagnetic fieldQC770-798shock waves01 natural sciencesAtomic and Molecular Physics and OpticsPhysics - Plasma Physics010305 fluids & plasmasPlasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E AstrofisicaNuclear Energy and Engineering[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesPhysics::Space PhysicsElectrical and Electronic Engineering010306 general physics
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Extracorporeal shock wave therapy as a potential therapeutic tool for breast cancer related lymphedema: a narrative review of in vitro, animal and cl…

2021

Background: The treatment of breast cancer related lymphedema (BCRL) focuses on the alleviation symptoms. One of the innovative, non-invasive therapies used for this condition is extracorporeal shock wave therapy (ESWT). Aim of the study: To review the available literature and evaluate the effectiveness of ESWT in the treatment of secondary lymphedema (in vitro works, animal experiments) and lymphedema associated with the treatment of breast cancer. Material and methods: The scientific literature review was conducted from October to December 2020. The review was carried out by searching scientifically recognized medical databases, including PubMed, MEDLINE and PEDro. Date restrictions were …

Oncologymedicine.medical_specialtylymphedema after breast cancerExtracorporeal shock wave therapybusiness.industryInternal medicineESWTmedicineshockwaveeffectivenessNarrative reviewbusinessBreast Cancer Related LymphedemaMedical Science Pulse
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Assessment of the fundamental flexural guided wave in cortical bone by an ultrasonic axial-transmission array transducer

2013

Abstract The fundamental flexural guided wave (FFGW), as modeled, for example, by the A0 Lamb mode, is a clinically useful indicator of cortical bone thickness. In the work described in this article, we tested so-called multiridge-based analysis, based on the crazy climber algorithm and short-time Fourier transform, for assessment of the FFGW component recorded by a clinical array transducer featuring a limited number of elements. Methods included numerical finite-element simulations and experiments in bone phantoms and human radius specimens ( n  = 41). The proposed approach enabled extraction of the FFGW component and determination of its group velocity. This group velocity was in good ag…

Pathologymedicine.medical_specialtyMaterials scienceLightAcoustics and UltrasonicsAcousticsTransducersBiophysicsModels BiologicalSensitivity and SpecificityHigh-Energy Shock Wavessymbols.namesakeFlexural strengthmedicineHumansScattering RadiationComputer SimulationRadiology Nuclear Medicine and imagingSensitivity (control systems)UltrasonographyGuided wave testingRadiological and Ultrasound Technologyta114Reproducibility of ResultsRadiusRadiusFourier transformmedicine.anatomical_structuresymbolsGroup velocityCortical boneUltrasonic sensorAlgorithmsUltrasound in Medicine and Biology
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Shock-cloud interaction in the Vela SNR II. Hydrodynamic model

2006

In the framework of the study of the X-ray and optical emission in supernova remnants we focus on an isolated X-ray knot in the northern rim of the Vela SNR (Vela FilD), whose X-ray emission has been studied and discussed in Paper I. We aim at understanding the physical origin of the X-ray and optical emission in FilD, at understanding the role of the different physical processes at work, and at obtaining a key for the interpretation of future X-ray observations of SNRs. To this end we have pursued an accurate ``forward'' modeling of the interaction of the Vela SNR shock with an ISM cloud. We perform hydrodynamic simulations and we directly compare the observables synthesized from the simul…

PhysicsAstrophysics::High Energy Astrophysical PhenomenacloudsISMAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysicsThermal conductionVelaAstrophysicsSpectral lineindividual objectVela SNRISMShock wavesSupernovakinematics and dynamicsISMsupernova remnantKnot (unit)Space and Planetary ScienceThermalIntercloudHydrodynamicsISMAstrophysics::Galaxy Astrophysics
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X-rays from protostellar jets: emission from continuous flows

2006

Recently X-ray emission from protostellar jets has been detected with both XMM-Newton and Chandra satellites, but the physical mechanism which can give rise to this emission is still unclear. We performed an extensive exploration of a wide space of the main parameters influencing the jet/ambient interaction. Aims include: 1) to constrain the jet/ambient interaction regimes leading to the X-ray emission observed in Herbig-Haro objects in terms of the emission by a shock forming at the interaction front between a continuous supersonic jet and the surrounding medium; 2) to derive detailed predictions to be compared with optical and X-ray observations of protostellar jets; 3) to get insight int…

PhysicsJet (fluid)Proper motionShock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsSpace (mathematics)Thermal conductionSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceRadiative transferHerbig-Haro objects ISM: jets and outflows X-rays: ISM [shock waves ISM]Astrophysics::Solar and Stellar AstrophysicsSupersonic speedCylindrical coordinate systemshock waves ISM: Herbig-Haro objects ISM: jets and outflows X-rays: ISMAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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Numerical study of a multiscale expansion of the Korteweg de Vries equation and Painlev\'e-II equation

2007

The Cauchy problem for the Korteweg de Vries (KdV) equation with small dispersion of order $\e^2$, $\e\ll 1$, is characterized by the appearance of a zone of rapid modulated oscillations. These oscillations are approximately described by the elliptic solution of KdV where the amplitude, wave-number and frequency are not constant but evolve according to the Whitham equations. Whereas the difference between the KdV and the asymptotic solution decreases as $\epsilon$ in the interior of the Whitham oscillatory zone, it is known to be only of order $\epsilon^{1/3}$ near the leading edge of this zone. To obtain a more accurate description near the leading edge of the oscillatory zone we present a…

PhysicsLeading edgeSmall dispersion limitComputer Science::Information RetrievalGeneral MathematicsMathematical analysisGeneral EngineeringMathematics::Analysis of PDEsGeneral Physics and AstronomyNonlinear equationsDispersive partial differential equationShock wavesAmplitudeNonlinear Sciences::Exactly Solvable and Integrable SystemsInitial value problemWavenumberDispersive shockDispersion (water waves)Constant (mathematics)Korteweg–de Vries equationDevries equationAsymptoticsSettore MAT/07 - Fisica MatematicaNonlinear Sciences::Pattern Formation and SolitonsMathematical Physics
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On the existence of a reverse shock in magnetized gamma-ray burst ejecta

2007

The role of magnetic fields in gamma-ray burst (GRB) flows remains controversial. The study of the early afterglow phases and, in particular, of the reverse shock dynamics and associated emission offers a promising probe of the magnetization of the ejecta. In this paper, we derive the conditions for the existence of a reverse shock in arbitrarily magnetized ejecta that decelerate and interact with the circumburst medium. Both constant and wind-like density profiles are considered. We show, in contrast to previous estimates, that ejecta with magnetization σ0 >∼ 1 are not crossed by a reverse shock for a large fraction of the parameter space relevant to GRB flows. Allowing for shell spreading…

PhysicsMagnetohydrodynamics (MHD)Astrophysics::High Energy Astrophysical PhenomenaAstronomy and AstrophysicsAstrophysicsParameter spaceUNESCO::ASTRONOMÍA Y ASTROFÍSICAShock (mechanics)Magnetic fieldAfterglowShock wavesMagnetizationGamma rays : bursts; Magnetohydrodynamics (MHD); Shock wavesbursts [Gamma rays]Space and Planetary ScienceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicasEjectaGamma-ray burstAstrophysics::Galaxy Astrophysics:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]
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