Search results for "asma"

showing 10 items of 4204 documents

Gravity effects on mixing with magnetic micro-convection in microfluidics.

2018

Mixing remains an important problem for development of successful microfluidic and lab-on-a-chip devices, where simple and predictable systems are particularly interesting. One is magnetic micro-convection, an instability happening on the interface of miscible magnetic and non-magnetic fluids in a Hele-Shaw cell under applied field. Previous work proved that Brinkman model quantitatively explains the experiments. However, a gravity caused convective motion complicated the tests. Here we first improve the experimental system to exclude the gravitational convective motion. Afterwards, we observe and quantify how gravity and laminar flow play an important role in stabilizing the perturbations …

ConvectionGravity (chemistry)Field (physics)BiophysicsFOS: Physical sciences02 engineering and technologyCondensed Matter - Soft Condensed Matter01 natural sciencesInstability010305 fluids & plasmasGravitationPhysics::Fluid Dynamics0103 physical sciencesGeneral Materials ScienceCritical fieldMixing (physics)PhysicsFluid Dynamics (physics.flu-dyn)Laminar flowSurfaces and InterfacesGeneral ChemistryMechanicsPhysics - Fluid Dynamics021001 nanoscience & nanotechnologySoft Condensed Matter (cond-mat.soft)0210 nano-technologyBiotechnologyThe European physical journal. E, Soft matter
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Influence of Skin Depth on Convective Heat Transfer in Induction Heating

2017

International audience; We investigate convection driven by induction heating of a horizontal fluid layer using direct numerical simulations (DNS). This problem is of particular interest in the context of nuclear severe accident mastering. In a real severe accident, the molten core is subjected to homogeneous internal sources resulting from nuclear disintegrations. This situation is mimicked in the laboratory using induction heating as the internal source. In induction heating, however, heat sources are localized in the skin layer. Consequently, this concentration of heat may modify the flow and wall heat transfer compared to the case of homogeneous internal sources. DNS are carried out for…

ConvectionInduction heatingConvective heat transferMHDDNS020209 energyMécanique des fluidesFlow (psychology)General Physics and AstronomyThermodynamicsContext (language use)02 engineering and technology01 natural sciences010305 fluids & plasmas[CHIM.GENI]Chemical Sciences/Chemical engineering0103 physical sciences0202 electrical engineering electronic engineering information engineeringThermal convectionNumerical simulationsElectrical and Electronic EngineeringInduction heatingCritical heat fluxChemistryMechanicsCore (optical fiber)Heat transfer
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On the impact of the heat transfer modelling approach on the prediction of EU-DEMO WCLL breeding blanket thermal performances

2020

Abstract The Water-Cooled Lithium-Lead Breeding Blanket is a key component of a fusion power plant, in charge of ensure Tritium production, shield Vacuum Vessel and magnets and remove the heat power deposited by radiation and particles arising from plasma. The last function is fulfilled by First Wall and Breeding Zone independent cooling systems. Several layouts of BZ coolant system have been investigated in the last years to identify a configuration that might guarantee EUROFER temperature below the limit (550 °C) and good thermal-hydraulic performances (i.e. water outlet temperature of 328 °C). A research activity is conducted to study and compare different modelling approaches to simulat…

ConvectionLiquid metalMaterials scienceNuclear engineeringBlanket engineeringBlanket7. Clean energy01 natural sciences010305 fluids & plasmasBreeder (animal)0103 physical sciencesGeneral Materials Science010306 general physicsSettore ING-IND/19 - Impianti NucleariCivil and Structural EngineeringFEMFinite volume methodWCLL; CFD; FEM; breeding blanket; blanket engineeringMechanical EngineeringFinite element methodCoolantWCLLNuclear Energy and EngineeringHeat transferBreeding blanketCFD
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Magnetic field emergence in mesogranular-sized exploding granules observed with SUNRISE/IMaX data

2011

We report on magnetic field emergences covering significant areas of exploding granules. The balloon-borne mission SUNRISE provided high spatial and temporal resolution images of the solar photosphere. Continuum images, longitudinal and transverse magnetic field maps and Dopplergrams obtained by IMaX onboard SUNRISE are analyzed by Local Correlation Traking (LCT), divergence calculation and time slices, Stokes inversions and numerical simulations are also employed. We characterize two mesogranular-scale exploding granules where $\sim$ 10$^{18}$ Mx of magnetic flux emerges. The emergence of weak unipolar longitudinal fields ($\sim$100 G) start with a single visible magnetic polarity, occupyi…

ConvectionPhysicsAdvectionFOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceTemporal resolutionSunriseAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsSolar and Stellar Astrophysics (astro-ph.SR)
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Convectively driven vortex flows in the Sun

2008

We have discovered small whirlpools in the Sun, with a size similar to the terrestrial hurricanes (<~0.5 Mm). The theory of solar convection predicts them, but they had remained elusive so far. The vortex flows are created at the downdrafts where the plasma returns to the solar interior after cooling down, and we detect them because some magnetic bright points (BPs) follow a logarithmic spiral in their way to be engulfed by a downdraft. Our disk center observations show 0.009 vortexes per Mm^2, with a lifetime of the order of 5 min, and with no preferred sense of rotation. They are not evenly spread out over the surface, but they seem to trace the supergranulation and the mesogranulation. T…

ConvectionPhysicsAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsAstrophysicsRotationVortexSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsSupergranulationAstrophysics::Earth and Planetary AstrophysicsLogarithmic spiralCooling down
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Modeling X-ray emission from stellar coronae

2008

By extrapolating from observationally derived surface magnetograms of low-mass stars we construct models of their coronal magnetic fields and compare the 3D field geometry with axial multipoles. AB Dor, which has a radiative core, has a very complex field, whereas V374 Peg, which is completely convective, has a simple dipolar field. We calculate global X-ray emission measures assuming that the plasma trapped along the coronal loops is in hydrostatic equilibrium and compare the differences between assuming isothermal coronae, or by considering a loop temperature profiles. Our preliminary results suggest that the non-isothermal model works well for the complex field of AB Dor, but not for the…

ConvectionPhysicsopacity and line formation Magnetic and electric fieldField (physics)Astrophysics (astro-ph)FOS: Physical sciencesCoronal loopAstrophysicsPlasmapolarization of starlightAstrophysicsMagnetic fieldlaw.inventionStarsSettore FIS/05 - Astronomia E Astrofisicaradiative transferlawX-ray emission spectra and fluorescence Stellar atmospheresRadiative transferAstrophysics::Solar and Stellar AstrophysicsHydrostatic equilibrium
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Evolution of small-scale magnetic elements in the vicinity of granular-size swirl convective motions

2014

Advances in solar instrumentation have led to a widespread usage of time series to study the dynamics of solar features, specially at small spatial scales and at very fast cadences. Physical processes at such scales are determinant as building blocks for many others occurring from the lower to the upper layers of the solar atmosphere and beyond, ultimately for understanding the bigger picture of solar activity. Ground-based (SST) and space-borne (Hinode) high-resolution solar data are analyzed in a quiet Sun region displaying negative polarity small-scale magnetic concentrations and a cluster of bright points observed in G-band and Ca II H images. The studied region is characterized by the …

ConvectionPolarity (physics)GranulationInstrumentationCiencias FísicasFOS: Physical sciencesScale (descriptive set theory)AstrophysicsConvectionCiencias de la Tierra y relacionadas con el Medio Ambiente//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/1.5 [https]PhotosphereCluster (physics)Astrophysics::Solar and Stellar AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]PlasmaVortexAstronomíaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetic fieldsAstrophysics::Earth and Planetary AstrophysicsMeteorología y Ciencias AtmosféricasIntensity (heat transfer)CIENCIAS NATURALES Y EXACTAS
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In-flight temperature of solid micrometric powders during cold spray additive manufacturing

2020

Abstract During cold dynamic gas spray additive manufacturing, the thermal field within particles is generally simplified by a state of an instantaneous uniform distribution over the particle's media at any position inside and outside the De-Laval nozzle. This paper addresses critical discussions using analytical and computational analysis of the transient heat transfer within the solid particles due to the convective exchange with the flowing gas. An analytical criterion depicts conditions of instantaneous uniform temperature over the range of typical cold spray data including various particle thermal conductivity, particle size range, dragging velocities, gas nature and gas setting condit…

ConvectionRange (particle radiation)Materials science020209 energyGeneral EngineeringGas dynamic cold spray02 engineering and technologyMechanicsCondensed Matter PhysicsResidence time (fluid dynamics)01 natural sciences010305 fluids & plasmasTemperature gradient[SPI]Engineering Sciences [physics]Thermal conductivity0103 physical sciences0202 electrical engineering electronic engineering information engineeringParticleParticle size
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Effects of Red Cell Spacing and Red Cell Movement Upon Oxygen Release Under Conditions of Maximally Working Skeletal Muscle

1989

The impacts of the particulate nature of blood upon capillary O 2 release have been studied extensively by Federspiel and Sarelius [8] and by Federspiel and Popel [9]. The latter authors found that the O 2 flux out of a capillary decreases rapidly as intracapillary red blood cell spacing increases. The O 2 flux out of a single RBC, however, is enhanced as long as the inter-erythrocytic plasma gap does not exceed the “zone-of-influence” of a single RBC, which they determined to be about 1 capillary diameter. In their model, they considered spherical red cells contained in a cylindrical tube filled with plasma, on the lateral surface of which a boundary Po 2 was specified. Based on earlier st…

ConvectionRed CellLateral surfaceChemistryCapillary actionFluxchemistry.chemical_elementPlasmaAnatomyOxygenRed blood cellmedicine.anatomical_structuremedicineBiophysics
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Impacts of Varying Concentrations of Cloud Condensation Nuclei on Deep Convective Cloud Updrafts—A Multimodel Assessment

2021

AbstractThis study presents results from a model intercomparison project, focusing on the range of responses in deep convective cloud updrafts to varying cloud condensation nuclei (CCN) concentrations among seven state-of-the-art cloud-resolving models. Simulations of scattered convective clouds near Houston, Texas, are conducted, after being initialized with both relatively low and high CCN concentrations. Deep convective updrafts are identified, and trends in the updraft intensity and frequency are assessed. The factors contributing to the vertical velocity tendencies are examined to identify the physical processes associated with the CCN-induced updraft changes. The models show several c…

Convection[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereAtmospheric ScienceBuoyancy010504 meteorology & atmospheric sciencesPerturbation (astronomy)engineering.materialAtmospheric sciences01 natural sciences010305 fluids & plasmasTroposphere13. Climate action0103 physical sciencesConvective cloudengineeringCloud condensation nucleiEnvironmental scienceIntensity (heat transfer)Pressure gradient0105 earth and related environmental sciences
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