Search results for "mass [target]"

showing 10 items of 514 documents

Superconducting Solenoid System with Adjustable Shielding Factor for Precision Measurements of the Properties of the Antiproton

2019

Physical review applied 12(4), 044012 (2019). doi:10.1103/PhysRevApplied.12.044012

MAGNETIC-MOMENTSpeichertechnik - Abteilung BlaumPenning trapNuclear engineeringGeneral Physics and Astronomy02 engineering and technologyPROTON53001 natural sciencesNoise (electronics)Physics AppliedTrap (computing)External magnetic field0103 physical sciencesPENNING TRAP TECHNIQUEFACILITYddc:530Physics::Atomic PhysicsSolenoidsDetectors and Experimental TechniquesNuclear Experiment010306 general physicsSuperconductivityPhysicsScience & TechnologyLarge Hadron ColliderPhysics021001 nanoscience & nanotechnologyMagnetic fieldElectromagnetic coilAntiprotonPhysical SciencesMagnetic momentsElectromagnetic shieldingPhysics::Accelerator PhysicsCharge-to-mass ratiosDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikATOMIC MASSPARTICLE0210 nano-technologyMASS MEASUREMENTSPhysical Review Applied
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A DERIVATION OF THE VLASOV-NAVIER-STOKES MODEL FOR AEROSOL FLOWS FROM KINETIC THEORY

2016

This article proposes a derivation of the Vlasov-Navier-Stokes system for spray/aerosol flows. The distribution function of the dispersed phase is governed by a Vlasov-equation, while the velocity field of the propellant satisfies the Navier-Stokes equations for incompressible fluids. The dynamics of the dispersed phase and of the propellant are coupled through the drag force exerted by the propellant on the dispersed phase. We present a formal derivation of this model from a multiphase Boltzmann system for a binary gaseous mixture, involving the droplets/dust particles in the dispersed phase as one species, and the gas molecules as the other species. Under suitable assumptions on the colli…

MSC: 35Q20 35B25 (82C40 76T15 76D05)aerosolVlasov-Navier-Stokes systemGeneral Mathematics01 natural sciencesPhysics::Fluid DynamicsBoltzmann equationsymbols.namesakeMathematics - Analysis of PDEsThermal velocityPhase (matter)35Q20 35B25 (82C40 76T15 76D05)SpraysFOS: Mathematics[MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP]0101 mathematicsSettore MAT/07 - Fisica MatematicaPhysicsPropellantAerosolsGas mixtureApplied Mathematics010102 general mathematicsMechanicsMass ratioBoltzmann equationAerosol010101 applied mathematicsDistribution functionsprayBoltzmann constantsymbolsHydrodynamic limitAnalysis of PDEs (math.AP)
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First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-correlation Analysis

2019

The determination of the speed of Coronal Mass Ejections (CMEs) is usually done by tracking brighter features (such as the CME front and core) in visible light coronagraphic images and by deriving unidimensional profiles of the CME speed as a function of altitude or time. Nevertheless, CMEs are usually characterized by the presence of significant density inhomogeneities propagating outward with different radial and latitudinal projected speeds, resulting in a complex evolution eventually forming the Interplanetary CME. In this work, we demonstrate for the first time how coronagraphic image sequences can be analyzed with cross-correlation technique to derive 2D maps of the almost instantaneo…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesDistribution (number theory)Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicspolarimetric [Techniques]magnetohydrodynamics (MHD)01 natural sciences0103 physical sciencesCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysicsmedia_common.cataloged_instanceEuropean uniondata analysis [Methods]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QCQB0105 earth and related environmental sciencesmedia_commonPhysicsUV radiation [Sun]Horizon (archaeology)Cross correlation analysisDASAstronomy and AstrophysicsSun: UV radiationmethods: data analysiscoronal mass ejections (CMEs) [Sun]techniques: polarimetricQC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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Hydrogen non-equilibrium ionisation effects in coronal mass ejections

2020

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). D.H.M. would like to thank both the UK STFC and the ERC (Synergy grant: WHOLE SUN, grant Agreement No. 810218) for financial support. D.H.M. and P.P. would like to thank STFC for IAA funding under grant number SMC1-XAS012. This work used the DiRAC@Durham facility man-aged by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk. The equipment was funded by BEIS capital fundin…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesHydrogenSun: coronal mass ejections (CMEs)FOS: Physical scienceschemistry.chemical_elementAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences7. Clean energycoronal mass ejections (CMEs) [un]Ionization0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]Sun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]Sun: coronaAstronomy and Astrophysics3rd-DASPlasmaMagnetic fluxSolar windQC PhysicsAstrophysics - Solar and Stellar AstrophysicschemistrySpace and Planetary SciencePhysics::Space PhysicsPlasma diagnosticsMagnetohydrodynamicsAstronomy & Astrophysics
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Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations

2021

Coronal mass ejections (CMEs) that exhibit weak or no eruption signatures in the low corona, known as stealth CMEs, are problematic as upon arrival at Earth they can lead to geomagnetic disturbances that were not predicted by space weather forecasters. We investigate the origin and eruption of a stealth event that occurred on 2015 January 3 that was responsible for a strong geomagnetic storm upon its arrival at Earth. To simulate the coronal magnetic field and plasma parameters of the eruption we use a coupled approach. This approach combines an evolutionary nonlinear force-free field model of the global corona with a MHD simulation. The combined simulation approach accurately reproduces th…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysics01 natural sciencesPhysics::GeophysicsAeronauticsMethods: data analysis0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar Astrophysicsdata analysis [Methods]Sun: magnetic fields010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)QB0105 earth and related environmental sciencesPhysicsAstronomy and Astrophysics3rd-DAScoronal mass ejections (CMEs) [Sun]QC PhysicsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstronomy & Astrophysics
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Effect of gravitational stratification on the propagation of a CME

2013

Our aim is to study the role of gravitational stratification on the propagation of CMEs. In particular, we assess how it influences the speed and shape of CMEs and under what conditions the flux rope ejection becomes a CME or when it is quenched. We ran a set of MHD simulations that adopt an eruptive initial magnetic configuration that has already been shown to be suitable for a flux rope ejection. We varied the temperature of the backgroud corona and the intensity of the initial magnetic field to tune the gravitational stratification and the amount of ejected magnetic flux. We used an automatic technique to track the expansion and the propagation of the magnetic flux rope in the MHD simula…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]Sun: coronal mass ejections (CMEs)Stratification (water)FOS: Physical sciencesAstrophysics01 natural sciencesmagnetohydrodynamics (MHD)Physics - Space Physics0103 physical sciencesGravitational stratificationCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsFlux rope ejectionSolar and Stellar Astrophysics (astro-ph.SR)QB0105 earth and related environmental sciencesPhysicsCoronal mass ejections (CMEs)Sun: coronaAstronomy and AstrophysicsPlasmaCoronaMagnetic fluxSpace Physics (physics.space-ph)coronal mass ejections (CMEs) [Sun]Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsRope
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Simulating AIA observations of a flux rope ejection

2014

D.H.M. would like to thank STFC, the Leverhulme Trust and the European Commission’s Seventh Framework Programme (FP7/2007-2013) for their financial support. P.P. would like to thank the European Commission’s Seventh Framework Programme (FP7/2007-2013) under grant agreement SWIFF (project 263340, http://www.swiff.eu) and STFC for financial support. These results were obtained in the framework of the projects GOA/2009-009 (KU Leuven), G.0729.11 (FWO-Vlaanderen) and C 90347 (ESA Prodex 9). The research leading to these results has also received funding from the European Commission’s Seventh Framework Programme (FP7/2007-2013) under the grant agreements SOLSPANET (project No. 269299, http:// ww…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicsmagnetohydrodynamics (MHD)7. Clean energyProminencesObservatoryRadiative transferQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsQASun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsUV radiation [Sun]Line-of-sightSun: coronaAstronomy and AstrophysicsPlasmaSun: UV radiationCoronacoronal mass ejections (CMEs) [Sun]Magnetic fluxSun: filamentsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]13. Climate actionSpace and Planetary ScienceExtreme ultravioletPhysics::Space Physicsfilaments prominences [Sun]Rope
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Future capabilities of CME polarimetric 3D reconstructions with the METIS instrument: A numerical test

2015

D.H.M. would like to thank STFC and the Leverhulme Trust for their financial support. P.P. would like to thank STFC and the Leverhulme Trust. The computational work for this paper was carried out on the joint STFC and SFC (SRIF) funded cluster at the University of St Andrews (Scotland, UK). Context. Understanding the 3D structure of coronal mass ejections (CMEs) is crucial for understanding the nature and origin of solar eruptions. However, owing to the optical thinness of the solar corona we can only observe the line of sight integrated emission. As a consequence the resulting projection effects hide the true 3D structure of CMEs. To derive information on the 3D structure of CMEs from whit…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)Sun: filaments prominencesNDASFOS: Physical sciencesLibrary scienceAstrophysicspolarimetric [Techniques]MetisQB AstronomyAstrophysics::Solar and Stellar AstrophysicsNumerical testsQCSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsSun: coronaTechniques: polarimetricAstronomy and Astrophysicscoronal mass ejections (CMEs) [Sun]QC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physicsfilaments prominences [Sun]
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Medical Support for Children's Mass Gatherings

2003

AbstractIntroduction:Medical care must be well-planned for mass gatherings. Events such as fairs, concerts, parades, and rallies cause many people to gather in one place, increasing the chance of injuries and for the development of a disaster. In this study, the level and quality of medical care were evaluated at a mass gathering of approximately 100,000 children. The event was a television-sponsored fun fair.Methods:Every patient contact was documented on printed forms, including data such as the number of patients treated, gender of the patients, presence or absence of a parental escort, time distribution of patient contacts, the diagnoses for the patient contacts, specific therapies appl…

MaleEmergency Medical ServicesPediatricsmedicine.medical_specialtyAdolescentChild Health ServicesPoison controlEmergency NursingSuicide preventionOccupational safety and healthGermanyMass gatheringInjury preventionmedicineHumansMedical diagnosisChildEmergency TreatmentParentingbusiness.industryMajor traumamedicine.diseaseAnniversaries and Special EventsCrowdingOutcome and Process Assessment Health CareTransportation of PatientsEmergency medicineEmergency MedicineFemaleEmergenciesHeadachesmedicine.symptombusinessMass BehaviorTotal Quality ManagementPrehospital and Disaster Medicine
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Lower limb muscle strength and muscle mass are associated with incident symptomatic knee osteoarthritis: a Longitudinal Cohort Study

2021

Recent literature suggests that sarcopenia, often represented by low lower limbs muscle mass and strength, can be considered a potential risk factor for knee osteoarthritis (OA), but the available literature is still limited. We therefore aimed to investigate whether sarcopenia is associated with a higher risk of radiographic (ROA) and symptomatic knee OA (SxOA) in a large cohort of North American people in the context of the OA initiative. Sarcopenia at baseline was diagnosed in case of low skeletal muscle mass (i.e., lower skeletal mass index) and poor performance in the chair stands test. The outcomes of interest for this study included ROA (radiographical osteoarthritis) if a knee devel…

MaleSarcopeniaEndocrinology Diabetes and MetabolismDiseases of the endocrine glands. Clinical endocrinologyCohort Studiesolder peoplesarcopeniaEndocrinologyRisk Factorsosteoarthritis of the kneeOsteoarthritisepidemiology; muscle mass and function; older people; osteoarthritis of the knee; sarcopenia; Aged; Body Composition; Cohort Studies; Female; Humans; Longitudinal Studies; Male; Middle Aged; Muscle Strength; Muscle Skeletal; Osteoarthritis Knee; Risk Factors; Sarcopenia; United StatesHumansKneeLongitudinal StudiesMuscle StrengthMuscle Skeletalmuscle mass and functionOriginal ResearchAgedddc:616SkeletalOsteoarthritis KneeMiddle AgedRC648-665musculoskeletal systemUnited StatesBody CompositionMuscleFemaleepidemiologyepidemiology muscle mass and function older people osteoarthritis of the knee Aged Body Composition Cohort Studies Female Humans Longitudinal Studies Male Middle Aged Muscle Strength Muscle Skeletal Osteoarthritis Knee Risk Factors Sarcopeniahuman activities
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