Search results for "Adiabatic process"

showing 10 items of 237 documents

ADIABATIC COOLING OF IONS IN THE PENNING TRAP

1991

An ion cloud in a Penning trap can be cooled by adiabatic expansion by reducing the trap's magnetic and electric fields. We treat the ion cloud as a classical gas and obtain the relations between the temperature and the trapping fields. This cooling method may be useful in trapping and cooling of antiprotons with the aim of measuring the gravitational accleration of anti-protons and other experiments on heavy ions.

Condensed Matter::Quantum GasesPhysicsTrappingPenning trapAtomic and Molecular Physics and OpticsIonMagnetic trapElectric fieldPhysics::Atomic PhysicsIon trapAtomic physicsNuclear ExperimentAdiabatic processDoppler cooling
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Towards the origin of the shear force in near-field microscopy

2001

The shear force from a gold or a graphite sample acting on an approaching near-field optical probe is studied in detail. The adiabatic and dissipative contributions to the force are clearly distinguished by monitoring the amplitude as well as the phase of the tip vibration when the tip approaches the surfaces. We also take into account that not only the damping and the resonance frequency but also the mass of the system changes when the tip approaches the surface. The relative strength of the contributions to the force varies differently but characteristically with the distance of the two samples, starting at a much larger distance in the case of graphite. The adiabatic contribution is lar…

Condensed matter physicsbusiness.industryChemistryElectrostatic force microscopeShear forceGeneral EngineeringGeneral Physics and AstronomyAtomic force acoustic microscopyConductive atomic force microscopyOpticsAmplitudeNear-field scanning optical microscopeAdiabatic processbusinessNon-contact atomic force microscopy
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Observed and Simulated Variability of Droplet Spectral Dispersion in Convective Clouds Over the Amazon

2021

In this study, the variability of the spectral dispersion of droplet size distributions (DSDs) in convective clouds is investigated. Analyses are based on aircraft measurements of growing cumuli near the Amazon basin, and on numerical simulations of an idealized ice‐free cumulus. In cleaner clouds, the relative dispersion ϵ, defined as the ratio of the standard deviation to the mean value of the droplet diameter, is negatively correlated with the ratio of the cloud water content (qc) to the adiabatic liquid water content (qa), while no strong correlation between ϵ and qc/qa is seen in polluted clouds. Bin microphysics numerical simulations suggest that these contrasting behaviors are associ…

ConvectionAtmospheric ScienceAmazon rainforestaerosolcloudsSpectral dispersionMICROFÍSICA DE NUVENSAtmospheric sciencesdroplet spectumStandard deviationGeophysicsddc:551.5Space and Planetary ScienceLiquid water contentEarth and Planetary Sciences (miscellaneous)Environmental sciencedispersionAdiabatic processDroplet sizeWater contentPhysics::Atmospheric and Oceanic Physics
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Cloud droplet formation at the base of tropical convective clouds: closure between modeling and measurement results of ACRIDICON–CHUVA

2021

Aerosol–cloud interactions contribute to the large uncertainties in current estimates of climate forcing. We investigated the effect of aerosol particles on cloud droplet formation by model calculations and aircraft measurements over the Amazon and over the western tropical Atlantic during the ACRIDICON–CHUVA campaign in September 2014. On the HALO (High Altitude Long Range Research) research aircraft, cloud droplet number concentrations (Nd) were measured near the base of clean and polluted growing convective cumuli using a cloud combination probe (CCP) and a cloud and aerosol spectrometer (CAS-DPOL). An adiabatic parcel model was used to perform cloud droplet number closure studies for fl…

ConvectionAtmospheric ScienceRange (particle radiation)010504 meteorology & atmospheric sciencesSpectrometerPhysicsQC1-999Radiative forcingTropical Atlantic010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesCondensation particle counterAerosolChemistry13. Climate actionComputer Science::Programming LanguagesEnvironmental science[CHIM]Chemical Sciences14. Life underwaterAdiabatic processQD1-999Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciences
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Comparing parameterized versus measured microphysical properties of tropical convective cloud bases during the ACRIDICON–CHUVA campaign

2017

The objective of this study is to validate parameterizations that were recently developed for satellite retrievals of cloud condensation nuclei supersaturation spectra, NCCN(S), at cloud base alongside more traditional parameterizations connecting NCCN(S) with cloud base updrafts and drop concentrations. This was based on the HALO aircraft measurements during the ACRIDICON–CHUVA campaign over the Amazon region, which took place in September 2014. The properties of convective clouds were measured with a cloud combination probe (CCP), a cloud and aerosol spectrometer (CAS-DPOL), and a CCN counter onboard the HALO aircraft. An intercomparison of the cloud drop size distributions (DSDs) and the…

ConvectionAtmospheric Sciencecould condenstion nuclei010504 meteorology & atmospheric sciencesMeteorologysupersaturationCloud computing010502 geochemistry & geophysicsAtmospheric sciences01 natural scienceslcsh:ChemistryCloud baseCloud condensation nucleicloudWolkenphysikAdiabatic processupdraftAstrophysics::Galaxy AstrophysicsPhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesbusiness.industryDrop (liquid)CASlcsh:QC1-999Aerosollcsh:QD1-999Environmental scienceHalobusinesslcsh:Physics
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Numerical investigation of thermomagnetic convection in a heated cylinder under the magnetic field of a solenoid

2011

The main objective of this paper is the numerical investigation of the process of thermomagnetic convection of a special temperature sensitive ferrofluid. The fluid is studied in a cylindrical domain, with constant temperatures on the top and bottom ends and adiabatic boundary conditions on the sidewalls. The thermomagnetic convection is generated by a non-uniform constant magnetic field of a solenoid, which is placed in a hollow area inside the domain. It has been found that the efficiency of convective heat transfer in such a set-up can be increased up to sevenfold by magnetic field within the studied range of parameters.

ConvectionFerrofluidConvective heat transferChemistryThermodynamicsSolenoidThermomagnetic convectionMechanicsCondensed Matter PhysicsMagnetic fieldPhysics::Fluid DynamicsHeat transferGeneral Materials ScienceAdiabatic processJournal of Physics: Condensed Matter
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Viscous dissipation and thermoconvective instabilities in a horizontal porous channel heated from below

2010

Accepted version of av article from the journal: International Journal of Thermal Sciences. Published version available on Science Direct: http://dx.doi.org/10.1016/j.ijthermalsci.2009.10.010 A linear stability analysis of the basic uniform flow in a horizontal porous channel with a rectangular cross section is carried out. The thermal boundary conditions at the impermeable channel walls are: uniform incoming heat flux at the bottom wall, uniform temperature at the top wall, adiabatic lateral walls. Thermoconvective instabilities are caused by the incoming heat flux at the bottom wall and by the internal viscous heating. Linear stability against transverse or longitudinal roll disturbances …

ConvectionVDP::Mathematics and natural science: 400::Mathematics: 410::Applied mathematics: 413Darcy's lawMaterials scienceLINEAR STABILITYGeneral EngineeringThermodynamicsMechanicsCondensed Matter PhysicsInstabilityVISCOUS DISSIPATIONPhysics::Fluid DynamicsHeat fluxPOROUS MEDIUMCONVECTIVE ROLLSHeat transferPotential flowVDP::Technology: 500::Materials science and engineering: 520Adiabatic processDARCY'S LAWLinear stability
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Onset of convection in a porous rectangular channel with external heat transfer to upper and lower fluid environments

2012

Published version of an article in the journal: Transport in Porous Media. Also available from the publisher at: http://dx.doi.org/10.1007/s11242-012-0018-9 The conditions for the onset of convection in a horizontal rectangular channel filled with a fluid saturated porous medium are studied. The vertical sidewalls are assumed to be impermeable and adiabatic. The horizontal upper and lower boundary walls are considered as impermeable and subject to external heat transfer, modelled through a third-kind boundary condition on the temperature field. The external fluid environments above and below the channel, kept at different temperatures, provide the heating-from-below mechanism which may lead…

ConvectionVDP::Mathematics and natural science: 400::Mathematics: 410::Applied mathematics: 413Materials scienceDarcy's lawBiot numberGeneral Chemical EngineeringThermodynamicsMechanicsCatalysisPhysics::Fluid Dynamicsanalytical solutionDarcy’s lawHeat transferBoundary value problemVDP::Technology: 500::Materials science and engineering: 520Porous mediumAdiabatic processrectangular porous channelDarcy–Bénard problemLongitudinal wavelinear stabilitythird-kind temperature conditions
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Primordial dark matter from curvature induced symmetry breaking

2020

We demonstrate that adiabatic dark matter can be generated by gravity induced symmetry breaking during inflation. We study a $Z_2$ symmetric scalar singlet that couples to other fields only through gravity and for which the symmetry is broken by the spacetime curvature during inflation when the non-minimal coupling $\xi$ is negative. We find that the symmetry breaking leads to the formation of adiabatic dark matter with the observed abundance for the singlet mass $m\sim{\rm MeV}$ and $|\xi|\sim 1$.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCurvature01 natural sciences114 Physical sciencessymmetry breakingGeneral Relativity and Quantum Cosmologypimeä aineGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesprimordial dark matterSymmetry breakinginflationAdiabatic processMathematical physicsPhysicsInflation (cosmology)symmetriadark matter theory010308 nuclear & particles physicsAstronomy and AstrophysicsCoupling (probability)Symmetry (physics)quantum field theory on curved spaceHigh Energy Physics - PhenomenologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample

2018

The hot plasma in galaxy clusters is expected to be heated to high temperatures through shocks and adiabatic compression. The thermodynamical properties of the gas encode information on the processes leading to the thermalization of the gas in the cluster's potential well as well as non-gravitational processes such as gas cooling, AGN feedback and kinetic energy. In this work we present the radial profiles of the thermodynamic properties of the intracluster medium (ICM) out to the virial radius for a sample of 12 galaxy clusters selected from the Planck all-sky survey. We determine the universal profiles of gas density, temperature, pressure, and entropy over more than two decades in radius…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)galaxies: clusters: intracluster mediumDark matterPopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesdark matterVirial theoremsymbols.namesakeIntracluster medium0103 physical sciencesGravitational collapsePlanckAdiabatic processeducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Settore FIS/05010308 nuclear & particles physicsThermodynamical quantitiesAstronomy and AstrophysicsX-rays: galaxies: clusters; dark matter; galaxies: clusters: intracluster medium; galaxies: clusters: general; Thermodynamical quantitiesgalaxies: clusters: general13. Climate actionSpace and Planetary ScienceX-rays: galaxies: clustersastro-ph.COsymbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsAstronomy & Astrophysics
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