Search results for "HYDRODYNAMICS"

showing 10 items of 390 documents

Computational fluid dynamics of the ascending aorta before the onset of type A aortic dissection.

2016

We performed a pre-dissection computational fluid analysis of an ascending aortic aneurysm associated with unicuspid aortic valve. The analysis showed an abnormal helical flow pattern inside the aneurysm and an increased wall stress on the right postero-lateral wall of the ascending aorta. These values were largely higher than the theoretical cut-off for aortic wall dissection, their topographic distribution followed the intimal tear site as subsequently diagnosed by computed tomography scan and confirmed during the operation for dissection repair.

Pulmonary and Respiratory MedicineAdultMalemedicine.medical_specialty0206 medical engineeringBlood Pressure02 engineering and technologyDissection (medical)030204 cardiovascular system & hematologyAortographyComputer03 medical and health sciencesAortic aneurysm0302 clinical medicineAneurysmAneurysm Dissectingmedicine.arteryInternal medicineAscending aortamedicineHumansComputer SimulationAortaAortic dissectionAortabusiness.industryModels CardiovascularSettore ING-IND/34 - Bioingegneria IndustrialeHydrodynamicGeneral Medicinemedicine.disease020601 biomedical engineeringUnicuspid aortic valveAortic wallAortic AneurysmAortic Dissectioncardiovascular systemCardiologyHydrodynamicsSurgeryStress MechanicalCardiology and Cardiovascular MedicinebusinessTomography X-Ray ComputedBlood Flow VelocityHumanEuropean journal of cardio-thoracic surgery : official journal of the European Association for Cardio-thoracic Surgery
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Magnetohydrodynamic simulations of the ejection of a magnetic flux rope

2013

Context. Coronal mass ejections (CME's) are one of the most violent phenomena found on the Sun. One model to explain their occurrence is the flux rope ejection model. In this model, magnetic flux ropes form slowly over time periods of days to weeks. They then lose equilibrium and are ejected from the solar corona over a few hours. The contrasting time scales of formation and ejection pose a serious problem for numerical simulations. Aims: We simulate the whole life span of a flux rope from slow formation to rapid ejection and investigate whether magnetic flux ropes formed from a continuous magnetic field distribution, during a quasi-static evolution, can erupt to produce a CME. Methods: To …

Q ScienceMagnetohydrodynamics (MHD)coronal mass ejections [Sun]010504 meteorology & atmospheric sciencescorona [Sun]FluxAstrophysicsmagnetic fields01 natural sciencesmagnetohydrodynamics (MHD)0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsSun: coronal mass ejectionsSun: coronaQSunAstronomy and AstrophysicsCoronal loopCoronaMagnetic fluxNanoflares13. Climate actionSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsCoronal mass ejectionsCoronaMagnetohydrodynamicsRope
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On a radiating fluid in a general relativistic context

2006

A model for the radiation hydrodynamics in general relativity is analyzed, describing the gravitational collapse and supernovae explosion. As these physical phenomena can be assumed spherically symmetric, the equations of motion for a unique fluid, representing the interaction between matter and radiation, are written in a spherical symmetric space-time with respect to a comoving frame. The system is completed by using the Eddington closure, assuming a local thermodynamical equilibrium for the radiation field. The resulting system is analyzed by the Lie symmetry approach and a reduction to an ODEs system is obtained. Numerical simulations of the solutions are performed, showing a realistic …

Radiation hydrodynamics Lie symmetries Exact solutions
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X-ray emitting MHD accretion shocks in classical T Tauri stars. Case for moderate to high plasma-beta values

2009

AIMS. We investigate the stability and dynamics of accretion shocks in CTTSs, considering the case of beta >= 1 in the post-shock region. In these cases the 1D approximation is not valid and a multi-dimensional MHD approach is necessary. METHODS. We model an accretion stream propagating through the atmosphere of a CTTS and impacting onto its chromosphere, by performing 2D axisymmetric MHD simulations. The model takes into account the stellar magnetic field, the gravity, the radiative cooling, and the thermal conduction (including the effects of heat flux saturation). RESULTS. The dynamics and stability of the accretion shock strongly depends on the plasma beta. In the case of shocks with…

Radiative coolingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesX-rays: starsAstrophysicsstars: pre-main sequenceInstabilitymagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics::Solar and Stellar AstrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)accretion accretion disksStellar magnetic fieldStellar atmosphereAstronomy and Astrophysicsshock wavesAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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A numerical meshless particle method in solving the magnetoencephalography forward problem

2012

In this paper, a numerical meshless particle method is presented in order to solve the magnetoencephalography forward problem for analyzing the complex activation patterns in the human brain. The forward problem is devoted to compute the scalp potential and magnetic field distribution generated by a set of current sources representing the neural activity, and in this paper, it has been approached by means of the smoothed particle hydrodynamics method suitably handled. The Poisson equation generated by the quasi-stationary Maxwell's curl equations, by assuming Neumann boundary conditions has been considered, and the current sources have been simulated by current dipoles. The adopted meshless…

Regularized meshless methodSingular boundary methodComputer Science ApplicationsSmoothed-particle hydrodynamicssymbols.namesakeClassical mechanicsMaxwell's equationsMesh generationModeling and SimulationNeumann boundary conditionsymbolsApplied mathematicsElectrical and Electronic EngineeringPoisson's equationBoundary element methodMathematicsInternational Journal of Numerical Modelling: Electronic Networks, Devices and Fields
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Laboratory disruption of scaled astrophysical outflows by a misaligned magnetic field

2021

The shaping of astrophysical outflows into bright, dense, and collimated jets due to magnetic pressure is here investigated using laboratory experiments. Here we look at the impact on jet collimation of a misalignment between the outflow, as it stems from the source, and the magnetic field. For small misalignments, a magnetic nozzle forms and redirects the outflow in a collimated jet. For growing misalignments, this nozzle becomes increasingly asymmetric, disrupting jet formation. Our results thus suggest outflow/magnetic field misalignment to be a plausible key process regulating jet collimation in a variety of objects from our Sun’s outflows to extragalatic jets. Furthermore, they provide…

ScienceAstrophysics::High Energy Astrophysical PhenomenaNozzleoutflows magnetohydrodynamics(MHD) shockwaves astrophysical jetsGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciencesArticleGeneral Biochemistry Genetics and Molecular BiologyCollimated lightSettore FIS/05 - Astronomia E AstrofisicaAmbient field0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetic pressure010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsLaboratory astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)MultidisciplinaryQLaser-produced plasmasGeneral ChemistryPhysics - Plasma PhysicsMagnetic fieldPlasma Physics (physics.plasm-ph)Astrophysics - Solar and Stellar AstrophysicsPhysics::Accelerator PhysicsOutflowHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Modeling Transit Flow Through Port Gates and Connecting Channel in Baltic Sea—Liepaja Port—Liepaja Lake System

2021

This study investigates a water transport features by extending Copernicus Marine Environment Service (CMEMS) to the Liepaja coast-port-channel-lake system with a two-way nested model. The Liepaja lake and Liepaja port are connected by Trade channel. The Liepaja port has three gates—the openings in wave breakers connecting the port aquatory with the Baltic sea. Each of gates has a corresponding dredged channel for securing the navigation. A hydrodynamic model is set up to study the flow and water level in this system. The area of the port gates, port and Trade channel are resolved by 33 m grid. The model results are verified against currents and sea level observations inside/outside port, T…

Seiche010504 meteorology & atmospheric sciencesScienceOcean EngineeringQH1-199.5Aquatic ScienceOceanography01 natural sciencestransit currents in portsport hydrodynamicsport seichesUnderwatertwo-way nesting0105 earth and related environmental sciencesWater Science and TechnologygeographyGlobal and Planetary ChangeWater transportgeography.geographical_feature_category010505 oceanographyQFetchOcean currentGeneral. Including nature conservation geographical distributionPort (computer networking)Water levelOceanographycoastal modelingGeologyChannel (geography)Frontiers in Marine Science
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Gelation of smectic liquid crystal phases with photosensitive gel forming agents.

2020

This paper studies the potential of 3 newly synthesized low molecular weight gelling agents (2 of them with azo groups) with the semicarbazide group as a H-bonding motif to gel the smectic phase of a commercial chiral smectic C material. To detect gelation two methods were used: the stabilization of the director pattern, which measures the interaction of the physical gel network with the LC-director, and the suppression of the onset of electrohydrodynamic instabilities, which measures the increase of viscosity. Special emphasis was put on the influence of the photochemical - isomerization of the gelling agents on gelation.From the stabilization of the director pattern an elastic component c…

SemicarbazidePhotoisomerizationChemistryGeneral ChemistryCondensed Matter PhysicsGel formingViscositychemistry.chemical_compoundChemical engineeringLiquid crystalPhase (matter)Organic chemistryElectrohydrodynamicsIsomerizationSoft matter
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Exploiting Numerical Behaviors in SPH.

2010

Smoothed Particle Hydrodynamics is a meshless particle method able to evaluate unknown field functions and relative differential operators. This evaluation is done by performing an integral representation based on a suitable smoothing kernel function which, in the discrete formulation, involves a set of particles scattered in the problem domain. Two fundamental aspects strongly characterizing the development of the method are the smoothing kernel function and the particle distribution. Their choice could lead to the so-called particle inconsistency problem causing a loose of accuracy in the approximation; several corrective strategies can be adopted to overcome this problem. This paper focu…

Series (mathematics)Applied MathematicsMeshless particle methodconsistency restoringfunction approximationGeneral ChemistryFunction (mathematics)smoothed particle hydrodinamics methodSmoothed-particle hydrodynamicsSettore MAT/08 - Analisi NumericaFunction approximationDistribution (mathematics)Kernel methodProblem domainCalculusApplied mathematicsparticle distributionSmoothingMathematics
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Tracking multiple pathways of waste from a northern bluefin tuna farm in a marine-coastal area.

2011

Aquaculture of bluefin tuna in Mediterranean coastal waters has generated growing concern about the negative environmental effects. In the present isotopic study we examined the dispersal and fate of organic matter derived from a Mediterranean tuna farm in the surrounding environment. An overall enrichment in the heavy nitrogen isotope was found in the feed and in farmed tunas, indicating the input of isotopically traceable organic matter in the system. Waste was clearly traceable in the water column up to 1000 m from the cages, while only slight accumulation occurred in the sediment just below the cages. Waste was isotopically shown also to contribute to the diet of demersal and benthopela…

Settore BIO/07 - EcologiaGeologic SedimentsAquacultureAquatic ScienceOceanographyDemersal zoneMass SpectrometryDemersal fishWater columnAquacultureAnimalsOrganic matterSeawaterchemistry.chemical_classificationWaste ProductsAnalysis of VariancebiologyNitrogen Isotopesbusiness.industryTunaGeneral MedicineBiodegradable wastebiology.organism_classificationPollutionFisheryOceanographychemistryBenthic zoneaquaculture nitrogen stable isotopes Thunnus thynnus organic waste MediterraneanHydrodynamicsEnvironmental sciencebusinessTunaMarine environmental research
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