Search results for "FLOWS"

showing 10 items of 148 documents

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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The diagnostic potential of Fe lines applied to protostellar jets

2013

We investigate the diagnostic capabilities of the iron lines for tracing the physical conditions of the shock-excited gas in jets driven by pre-main sequence stars. We have analyzed the 300-2500 nm X-shooter spectra of two jets driven by the pre-main sequence stars ESO-Halpha 574 and Par-Lup 3-4. Both spectra are very rich in [FeII] lines over the whole spectral range; in addition, lines from [FeIII] are detected in the ESO-H\alpha 574 spectrum. NLTE codes along with codes for the ionization equilibrium are used to derive the gas excitation conditions of electron temperature and density, and fractional ionization. The iron gas-phase abundance is provided by comparing the iron lines emissivi…

PhysicsJet (fluid)Range (particle radiation)ISM: individual objects: ESO-Hα 574 Par-Lup 3-4 ISM: jets and outflows ISM: lines and bands stars: pre-main sequenceFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesSpectral lineStarsindividual objects: ESO-Hα 574 Par-Lup 3-4 ISM: jets and outflows ISM: lines and bands stars: pre-main sequence [ISM]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceIonizationAstrophysics of Galaxies (astro-ph.GA)EmissivityElectron temperatureAtomic physicsExcitationSolar and Stellar Astrophysics (astro-ph.SR)
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Effects of roughness on particle dynamics in turbulent channel flows: a DNS analysis

2014

AbstractDeposition and resuspension mechanisms in particle-laden turbulent flows are dominated by the coherent structures arising in the wall region. These turbulent structures, which control the turbulent regeneration cycles, are affected by the roughness of the wall. The particle-laden turbulent flow in a channel bounded by irregular two-dimensional rough surfaces is analysed. The behaviour of dilute dispersions of heavy particles is analysed using direct numerical simulations (DNS) to calculate the three-dimensional turbulent flow and Lagrangian tracking to describe the turbophoretic effect associated with two-phase turbulent flows in a complex wall-bounded domain. Turbophoresis is inves…

PhysicsParticle statisticsTurbulenceMechanical Engineeringmedia_common.quotation_subjectParticle-laden flowsProbability density functionMechanicsCondensed Matter PhysicsTracking (particle physics)Inertiamultiphase and particle-laden flows particle/fluid flows turbulent flowsPhysics::Fluid DynamicsMechanics of MaterialsParticleParticle velocitymedia_commonJournal of Fluid Mechanics
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Distributed correlations and information flows within a hybrid multipartite quantum-classical system

2015

Understanding the non-Markovian mechanisms underlying the revivals of quantum entanglement in the presence of classical environments is central in the theory of quantum information. Tentative interpretations have been given by either the role of the environment as a control device or the concept of hidden entanglement. We address this issue from an information-theoretic point of view. To this aim, we consider a paradigmatic tripartite system, already realized in the laboratory, made of two independent qubits and a random classical field locally interacting with one qubit alone. We study the dynamical relationship between the two-qubit entanglement and the genuine tripartite correlations of …

PhysicsQuantum PhysicsQuantum decoherenceInformation flowClassical environmentNon-MarkovianityFOS: Physical sciencesQuantum correlationQuantum PhysicsQuantum entanglementINFORMAÇÃO QUÂNTICASquashed entanglementMultipartite entanglementSettore FIS/03 - Fisica Della MateriaAtomic and Molecular Physics and OpticsMultipartiteOpen quantum systems; Classical environment; Quantum correlations; Information flows; Non-MarkovianityOpen quantum systemQuantum mechanicsQubitStatistical physicsQuantum informationQuantum Physics (quant-ph)Quantum
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A numerical study of postshock oscillations in slowly moving shock waves

2003

Abstract Godunov-type methods and other shock capturing schemes can display pathological behavior in certain flow situations. This paper discusses the numerical anomaly associated to slowly moving shocks. We present a series of numerical experiments that illustrate the formation and propagation of this pathology, and allows us to establish some conclusions and question some previous conjectures for the source of the numerical noise. A simple diagnosis on an explicit Steger-Warming scheme shows that some intermediate states in the first time steps deviate from the true direction and contaminate the flow structure. A remedy is presented in the form of a new flux split method with an entropy i…

PhysicsShock capturing schemesSlowly moving shocksMechanicsMoving shockFlux split methodsComputational MathematicsNonlinear systems of conservation lawsNumerical noiseComputational Theory and MathematicsModeling and SimulationModelling and SimulationCompressible flowsEntropy (energy dispersal)Computers & Mathematics with Applications
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Discussion of "preliminary Study of Surface Hydraulic Jumps" by S. Ahmed, Y. Ye, H. Liu, and N. Rajaratnam

2020

In this paper the results of Preliminary Study of Surface Hydraulic Jumps” by S. Ahmed, Y. Ye, H. Liu, and N. Rajaratnam are discussed

PhysicsSurface (mathematics)hydraulic jump open channel flowsSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-ForestaliGeometryAgricultural and Biological Sciences (miscellaneous)Hydraulic jumpWater Science and TechnologyCivil and Structural Engineering
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An X-shooter survey of star forming regions: Low-mass stars and sub-stellar objects

2011

We present preliminary results of our X-shooter survey in star forming regions. In this contribution we focus on sub-samples of young stellar and sub-stellar objects (YSOs) in the Lupus star forming region and in the TW Hya association. We show that the X-shooter spectra are suitable for conducting several parallel studies such as YSO + disk fundamental parameters, accretion and outflow activity in the very low-mass (VLM) and sub-stellar regimes, as well as magnetic activity in young VLM YSOs, and Li abundance determinations. The capabilities of X-shooter in terms of wide spectral coverage, resolution and limiting magnitudes, allow us to assess simultaneously the accretion/outflow, magnetic…

PhysicsYoung stellar objectBrown dwarfAstronomyAstronomy and AstrophysicsAstrophysicsAccretion (astrophysics)Spectral lineT Tauri starStarsaccretion accretion disks ISM: jets and outflows stars: formation stars: low-mass brown dwarfs stars: pre-main sequence T Tauri starsSpace and Planetary ScienceOutflowLow Massjets and outflows stars: formation stars: low-mass brown dwarfs stars: pre-main sequence T Tauri stars [accretion accretion disks ISM]
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Hyper-concentrated flow and surface velocity estimation by digital imaging technique: a study case

2015

This paper investigates the utility of digital imaging technique for performing surface velocity measurements of hyper-concentrated flows. The analysis is conducted with the aid of data collected in a scale laboratory flume constructed at the Hydraulic laboratory of the Department of Civil, Environmental, Aerospatial and of Materials Engineering (DICAM) – University of Palermo (Italy). In particular the present paper describes the setup of a laboratory test and the applicability of a fully digital imaging approach.

Predictions hyper-concentrated flows flow velocity experiments digital measurementsSettore ICAR/01 - Idraulica
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Risk Management Optimization for Sovereign Debt Restructuring

2015

Abstract Debt restructuring is one of the policy tools available for resolving sovereign debt crises and, while unorthodox, it is not uncommon. We propose a scenario analysis for debt sustainability and integrate it with scenario optimization for risk management in restructuring sovereign debt. The scenario dynamics of debt-to-GDP ratio are used to define a tail risk measure, termed conditional Debt-at-Risk. A multi-period stochastic programming model minimizes the expected cost of debt financing subject to risk limits. It provides an operational model to handle significant aspects of debt restructuring: it collects all debt issues in a common framework, and can include contingent claims, m…

RestructuringFinancial economicsmedia_common.quotation_subjectGeography Planning and DevelopmentRecourse debtDebt-to-GDP ratioMonetary economicsDevelopmentportfolio optimizationstochastic programmingsovereign debtSettore SECS-S/06 -Metodi Mat. dell'Economia e d. Scienze Attuariali e Finanz.Debt0502 economics and businessEconomics050207 economicsDebt levels and flowsRisk managementmedia_common050208 financebusiness.industryconditional Value-at-RiskValue-at-RiskRisk metric05 social sciencesscenario analysiGreek crisiExternal debtExpected shortfallDebt restructuringdebt restructuringInternal debtPortfolio optimizationbusinessGeneral Economics Econometrics and FinanceValue at riskSenior debtJournal of Globalization and Development
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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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