Search results for "Hydrostatic equilibrium"

showing 6 items of 26 documents

Macroscopic capillarity without a constitutive capillary pressure function

2006

This paper challenges the foundations of the macroscopic capillary pressure concept. The capillary pressure function, as it is traditionally assumed in the constitutive theory of two-phase immiscible displacement in porous media, relates the pressure difference between nonwetting and wetting fluid to the saturation of the wetting fluid. The traditional capillary pressure function neglects the fundamental difference between percolating and nonpercolating fluid regions as first emphasized in R. Hilfer [Macroscopic equations of motion for two phase flow in porous media, Phys. Rev. E 58 (1998) 2090]. The theoretical approach proposed here starts from residual saturations as the volume fractions…

Statistics and ProbabilityCapillary pressureMaterials scienceCapillary actionMultiphase flowThermodynamicsMechanicsCondensed Matter PhysicsCapillary numberlaw.inventionPhysics::Fluid DynamicslawTwo-phase flowHydrostatic equilibriumPorous mediumQuasistatic processPhysica A: Statistical Mechanics and its Applications
researchProduct

Numerical and experimental study of hydrostatic displacement machine

2012

This paper presents a simulation tool to determine the structural deflections and corresponding leakage flow in a hydrostatic displacement motor. The simulation tool is applied to a new motor principle that is categorized as an extreme low-speed high-torque motor with dimensions that calls for attention to the volumetric efficiency. To counteract structural deflections the motor is equipped with compensation pressure volumes that may be used to limit the leakage flow across the end faces of the circular rotor. This leakage flow is investigated by solving Reynolds equation for the pressure distribution across both end faces. The fluid pressure is combined with structural calculations in a fl…

Volumetric efficiencyEngineeringbusiness.industryMechanical EngineeringGeneral Physics and AstronomyLeakage flowStructural engineeringHigh torqueReynolds equationlaw.inventionPhysics::Fluid DynamicsLow speedlawFluid–structure interactionHydrostatic equilibriumbusinessLeakage (electronics)
researchProduct

Numerical and Experimental Study of Friction Loss in Hydrostatic Motor

2012

Published version of an article in the journal: Modeling, Identification and Control. Also available from the publisher at: http://dx.doi.org/10.4173/mic.2012.3.2 Open access This paper presents a numerical and experimental study of the losses in a hydrostatic motor principle. The motor is designed so that the structural deflections and lubricating regimes between moving surfaces and, subsequently, the leakage and friction losses, can be controlled during operation. This is done by means of additional pressure volumes that influence the stator deflection. These pressures are referred to as compensation pressures and the main emphasis is on friction or torque loss modeling of the motor as a …

experimental verificationEngineeringbusiness.industryVDP::Technology: 500Mechanical engineeringFriction losslcsh:QA75.5-76.95hydrostatic motorComputer Science Applicationslaw.inventionmixed lubricationIdentification (information)Control and Systems EngineeringlawModeling and Simulationlcsh:Electronic computers. Computer scienceHydrostatic equilibriumbusinessSoftwarefriction loss
researchProduct

Observational Results On The Influence Of Surface Layer Stability And Inversion Entrainment On Surface Layer Marine Aerosol Number Density (1 Microme…

1983

Wind speed and relative humidity have been the physical variables used in empirical expressions for equilibrium marine aerosol distributions. Recent formulations, which include the role of hydrostatic stability because it influences turbulent transport and entrainment of clear air from aloft, are examined on the basis of 1 um radius aerosol number density values. The aerosol data were collected along with a quite complete meteorological data set in the Northeast Atlantic during the international Joint Air Sea Interaction Experiment (JASIN-78). The 1 um number density values are normalized for generation and relative humidity influences, and analyses are performed to gain reasonable assuranc…

food.ingredientNumber densitySea saltGeneral EngineeringHumidityAtmospheric sciencesAtomic and Molecular Physics and Opticslaw.inventionAerosolBoundary layerfoodlawEnvironmental scienceRelative humiditySurface layerHydrostatic equilibriumOptical Engineering
researchProduct

The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the Intracluster Medium out to $R_{200}$ in Abell 2319

2018

We present the joint analysis of the X-ray and SZ signals in A2319, the galaxy cluster with the highest signal-to-noise ratio in Planck maps and that has been surveyed within our XMM Cluster Outskirts Project (X-COP). We recover the thermodynamical profiles by the geometrical deprojection of the X-ray surface brightness, of the SZ comptonization parameter, and an accurate and robust spectroscopic measurements of the temperature. We resolve the clumpiness of the density to be below 20 per cent demonstrating that most of this clumpiness originates from the ongoing merger and can be associated to large-scale inhomogeneities. This analysis is done in azimuthally averaged radial bins and in eigh…

galaxies: clusters: general ; galaxies: clusters: intracluster medium – X-rays; galaxies: clusters – intergalactic mediumgalaxies: clusters: intracluster medium – X-raysCosmology and Nongalactic Astrophysics (astro-ph.CO)galaxies: clusters: intracluster medium[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionlawIntracluster medium0103 physical sciencesROSATCluster (physics)Surface brightnessTotal pressure010303 astronomy & astrophysicsGalaxy clusterComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgalaxies: clusters – intergalactic medium[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsSettore FIS/05Astronomy and AstrophysicsAstronomy and AstrophysicX-rays: galaxies: clusterGalaxySpace and Planetary Sciencegalaxies: clusters: generalX-rays: galaxies: clustersintergalactic mediumHydrostatic equilibrium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Non-thermal pressure support in X-COP galaxy clusters

2018

Galaxy clusters are the endpoints of structure formation and are continuously growing through the merging and accretion of smaller structures. Numerical simulations predict that a fraction of their energy content is not yet thermalized, mainly in the form of kinetic motions (turbulence, bulk motions). Measuring the level of non-thermal pressure support is necessary to understand the processes leading to the virialization of the gas within the potential well of the main halo and to calibrate the biases in hydrostatic mass estimates. We present high-quality measurements of hydrostatic masses and intracluster gas fraction out to the virial radius for a sample of 12 nearby clusters with availab…

galaxies: clusters: intracluster mediumStructure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Cosmic microwave backgroundFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesVirial theoremCosmologylaw.inventionsymbols.namesakelaw0103 physical sciencesPlanck010303 astronomy & astrophysicsGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Settore FIS/05010308 nuclear & particles physicsComputer Science::Information RetrievalAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusters; large-scale structure of Universe; galaxies: clusters: intracluster medium; galaxies: clusters: generalgalaxies: clusters: generalSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)symbolslarge-scale structure of UniverseHaloHydrostatic equilibriumAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-rays: galaxies: clusters - Galaxies: clusters: general - Galaxies: groups: general - Galaxies: clusters: intracluster medium - cosmology: large-scale structureAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct