Search results for "mass [neutrino]"

showing 10 items of 1841 documents

Optimal mass transportation for costs given by Finsler distances via p-Laplacian approximations

2016

Abstract In this paper we approximate a Kantorovich potential and a transport density for the mass transport problem of two measures (with the transport cost given by a Finsler distance), by taking limits, as p goes to infinity, to a family of variational problems of p-Laplacian type. We characterize the Euler–Lagrange equation associated to the variational Kantorovich problem. We also obtain different characterizations of the Kantorovich potentials and a Benamou–Brenier formula for the transport problem.

010101 applied mathematicsMass transportApplied Mathematics010102 general mathematicsp-LaplacianApplied mathematics0101 mathematicsMass transportation01 natural sciencesAnalysisMathematicsAdvances in Calculus of Variations
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Magnetic field control of gas-liquid mass transfer in ferrofluids

2020

Abstract Gas-liquid mass transfer plays a key role in a broad range of industrial processes. The magnetic field control over the morphology of the gas-liquid interface and solute transport is an attractive feature if it can be realized efficiently. However, the magnetic properties of typical liquids and gases are rather weak. The experimental investigation is carried out to evaluate the effect of the magnetic field, which is mediated by magnetic nanoparticles, on the gas-liquid mass exchange during the sparging run through a hydrocarbon ferrofluid. The results indicate that the gradient field is especially effective at controlling the gas-liquid contact volume: the foaming of the liquid dur…

010302 applied physicsRange (particle radiation)FerrofluidMaterials science02 engineering and technology021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesElectronic Optical and Magnetic MaterialsMagnetic fieldPhysics::Fluid DynamicsCondensed Matter::Soft Condensed MatterVolume (thermodynamics)Chemical physicsMass transfer0103 physical sciencesMagnetic nanoparticlesVector field0210 nano-technologySpargingJournal of Magnetism and Magnetic Materials
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Exposure to mercury among 9-year-old Spanish children: Associated factors and trend throughout childhood

2019

Mercury is considered a neurotoxicant and human exposure occurs mainly from the consumption of marine species. We aimed to describe total mercury concentrations (THg) and associated factors in 9-year old children, as well as to explore the trend in THg from 4 to 9 years of age. The study population consisted of 9-year-old children participating in the INMA (Environment and Childhood) birth cohort study in Valencia, Spain (n = 405, 2013–2014). THg in hair samples was measured by atomic absorption spectrometry at the age of 4 and 9 years. Sociodemographic and dietary data was obtained through questionnaires. Multiple linear regression was used to explore the association between THg and covari…

010504 meteorology & atmospheric sciencesChild Diet exposure Environmental exposure Mercury Postnatal exposure SpainDiet exposureMotherschemistry.chemical_elementFood Contamination010501 environmental sciences01 natural sciencesWorld healthCohort StudiesEnvironmental healthmedicineAnimalsHumansChildlcsh:Environmental sciences0105 earth and related environmental sciencesGeneral Environmental Sciencelcsh:GE1-350Pregnancybusiness.industryPostnatal exposureSwordfishFishesMercuryEnvironmental exposureEnvironmental exposuremedicine.diseaseConfidence intervalMercury (element)SeafoodchemistrySpainChild PreschoolMultivariate AnalysisLinear ModelsPopulation studyFemalebusinessBody mass indexHairEnvironment International
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Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011

2016

We present study of the complex event consisting of several solar wind transients detected by Advanced Composition Explorer (ACE) on 4 -- 7 August 2011, that caused a geomagnetic storm with Dst$=-$110 nT. The supposed coronal sources -- three flares and coronal mass ejections (CMEs) occurred on 2 -- 4 August 2011 in the active region (AR) 11261. To investigate the solar origin and formation of these transients we studied kinematic and thermodynamic properties of the expanding coronal structures using the Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) EUV images and the differential emission measure (DEM) diagnostics. The Helioseismic and Magnetic Imager (HMI) magnetic fie…

010504 meteorology & atmospheric sciencesMHDSolar windAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics01 natural sciencesPhysics - Space PhysicsModelsIonization0103 physical sciencesCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesGeomagnetic stormPhysicsAstronomy and Astrophysics3rd-DASPlasmaCoronaSpace Physics (physics.space-ph)Solar windQC PhysicsMagnetic field13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsCoronal mass ejectionsMagnetohydrodynamicsSolar Physics
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Ash-plume dynamics and eruption source parameters by infrasound and thermal imagery: The 2010 Eyjafjallajökull eruption

2013

During operational ash-cloud forecasting, prediction of ash concentration and total erupted mass directly depends on the determination of mass eruption rate (MER), which is typically inferred from plume height. Uncertainties for plume heights are large, especially for bent-over plumes in which the ascent dynamics are strongly affected by the surrounding wind field. Here we show how uncertainties can be reduced if MER is derived directly from geophysical observations of source dynamics. The combination of infrasound measurements and thermal camera imagery allows for the infrasonic type of source to be constrained (a dipole in this case) and for the plume exit velocity to be calculated (54–14…

010504 meteorology & atmospheric sciencesMeteorologyInfrasound Thermal cameras Volcanic Plume dynamicsInfrasoundPlume heightInfrasound010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesGeochemistry and PetrologyThermalEarth and Planetary Sciences (miscellaneous)ddc:5500105 earth and related environmental sciencesPlume heightLead (sea ice)Escape velocityPlumeGeophysics13. Climate actionSpace and Planetary ScienceParticle-size distributionEruption rateAsh eruptionsMass eruption rateGeology
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Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections.

2021

Geomagnetic storms are an important aspect of space weather and can result in significant impacts on space- and ground-based assets. The majority of strong storms are associated with the passage of interplanetary coronal mass ejections (ICMEs) in the near-Earth environment. In many cases, these ICMEs can be traced back unambiguously to a specific coronal mass ejection (CME) and solar activity on the frontside of the Sun. Hence, predicting the arrival of ICMEs at Earth from routine observations of CMEs and solar activity currently makes a major contribution to the forecasting of geomagnetic storms. However, it is clear that some ICMEs, which may also cause enhanced geomagnetic activity, cann…

010504 meteorology & atmospheric sciencesSpace weather01 natural scienceslaw.inventionDIMMINGSPhysics - Space PhysicslawRECONNECTIONCoronal mass ejectionQB Astronomy010303 astronomy & astrophysicsCoronagraphQCMISSIONQBSTREAMERSUN3rd-DASLow-coronal signaturesMagnetic StormsAstrophysics - Solar and Stellar AstrophysicsMagnetic stormsPhysical SciencesCURRENT SHEETSpace WeatherGeologyCoronal Mass EjectionsSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo CircumterrestreSpace weatherSOLAR-WIND HELIUMMAGNETIC CLOUDSFOS: Physical sciencesSolar cycle 24Astronomy & AstrophysicsArticleCurrent sheet0103 physical sciencesSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesGeomagnetic stormScience & TechnologyAstronomyAstronomy and AstrophysicsSpace Physics (physics.space-ph)EVOLUTIONEarth's magnetic fieldQC Physics13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Low-Coronal SignaturesCoronal mass ejectionsMAGNETOHYDRODYNAMIC MODELSInterplanetary spaceflightSpace science reviews
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A space weather tool for identifying eruptive active regions

2019

Funding: UK 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); UK STFC via the Consolidated Grant SMC1/YST025 and SMC1/YST037 (S.L.Y.); UK STFC and the ERC (SynergyGrant: WHOLE SUN, Grant Agreement No. 810218) for financial support (DHM). One of the main goals of solar physics is the timely identification of eruptive active regions. Space missions such as Solar Orbiter or future Space Weather forecasting missions would largely benefit from this achievement.Our aim is to produce a relatively simple technique that c…

010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsFOS: Physical sciencesSpace weather01 natural sciences3rd-NDASSolar coronal mass ejections0103 physical sciencesRegional sciencemedia_common.cataloged_instanceQB AstronomyEuropean union010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesmedia_commonQBPhysicsHorizon (archaeology)European researchAstronomy and AstrophysicsSolar active region magnetic fieldsSolar active regionsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test

2018

Context. The determination from coronagraphic observations of physical parameters of the plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our understanding of the origin and evolution of these phenomena. Aims. The aim of this work is to perform the first ever numerical simulations of a CME as it will be observed by future two-channel (visible light VL and UV Ly-α) coronagraphs, such as the Metis instrument on-board ESA-Solar Orbiter mission, or any other future coronagraphs with the same spectral band-passes. These simulations are then used to test and optimize the plasma diagnostic techniques to be applied to future observations of CMEs. Methods. The CME diagno…

010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)Plasma parametersT-NDASContext (language use)Astrophysics01 natural sciencessymbols.namesakeMethods: data analysis0103 physical sciencesRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]numerical [Methods]Methods: numericalAstronomy and AstrophysicsPlasmaSun: UV radiationPolarization (waves)coronal mass ejections (CMEs) [Sun]Computational physicsQC PhysicsPlasmasSpace and Planetary SciencePhysics::Space PhysicssymbolsMagnetohydrodynamicsDoppler effectAstronomy & Astrophysics
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Children’s exposure to polycyclic aromatic hydrocarbons in the Valencian Region (Spain): Urinary levels, predictors of exposure and risk assessment

2021

Polycyclic aromatic hydrocarbons (PAHs) are pollutants that are released into the environment during incomplete combustion of organic matter and which can have a negative effect on human health. PAHs enter the human body mostly through ingestion of food or inhalation of tobacco smoke. The purpose of the present study is to evaluate the internal levels of PAHs that children living in the Valencian Region (Spain) are exposed to. In total, we measured eleven biomarkers of exposure to naphthalene, fluorene, phenanthrene, pyrene, and benzo(a)pyrene in the urine of 566 children aged 5-12. The analytical method was based on a liquid-liquid extraction of the PAH metabolites from the urine samples, …

010504 meteorology & atmospheric sciencesUrine010501 environmental sciencesFluoreneUrineRisk Assessment01 natural sciencesTobacco smokeReference valueschemistry.chemical_compoundEnvironmental healthBenzo(a)pyreneHumansMedicineIngestionGE1-350ChildChildren0105 earth and related environmental sciencesGeneral Environmental Sciencebusiness.industryPhenanthrenePolycyclic aromatic hydrocarbonsHuman biomonitoringEnvironmental scienceschemistrySpainPyreneEnvironmental PollutantsbusinessRisk assessmentBody mass indexBiomarkersEnvironment International
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Models and data analysis tools for the Solar Orbiter mission

2020

All authors: Rouillard, A. P.; Pinto, R. F.; Vourlidas, A.; De Groof, A.; Thompson, W. T.; Bemporad, A.; Dolei, S.; Indurain, M.; Buchlin, E.; Sasso, C.; Spadaro, D.; Dalmasse, K.; Hirzberger, J.; Zouganelis, I.; Strugarek, A.; Brun, A. S.; Alexandre, M.; Berghmans, D.; Raouafi, N. E.; Wiegelmann, T.; Pagano, P.; Arge, C. N.; Nieves-Chinchilla, T.; Lavarra, M.; Poirier, N.; Amari, T.; Aran, A.; Andretta, V.; Antonucci, E.; Anastasiadis, A.; Auchère, F.; Bellot Rubio, L.; Nicula, B.; Bonnin, X.; Bouchemit, M.; Budnik, E.; Caminade, S.; Cecconi, B.; Carlyle, J.; Cernuda, I.; Davila, J. M.; Etesi, L.; Espinosa Lara, F.; Fedorov, A.; Fineschi, S.; Fludra, A.; Génot, V.; Georgoulis, M. K.; Gilbe…

010504 meteorology & atmospheric sciencescorona [Sun]Solar windAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]7. Clean energy01 natural scienceslaw.inventionData acquisitionlawCoronal mass ejectiongeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSun: magnetic fieldsQCComputingMilieux_MISCELLANEOUSQBPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]3rd-DASenergetic particlesSolar windCORONAL MASS EJECTIONSnumerical modelingmagnetic fields [Sun]solar windPhysics::Space PhysicsSystems engineeringAstrophysics::Earth and Planetary Astrophysicsatmosphere [Sun]fundamental parameters [Sun]Sun: generalFORCE-FREE FIELDSun: fundamental parametersSolar radiusContext (language use)STREAMER STRUCTUREOrbiter0103 physical sciencesOPTIMIZATION APPROACH[SDU.ASTR.SR] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]POLARIZATION MEASUREMENTSSun: Solar wind3-DIMENSIONAL STRUCTURE0105 earth and related environmental sciencesSpacecraftbusiness.industrySun: corona[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]solar coronaMAGNETIC-FLUX ROPESAstronomy and AstrophysicsSHOCKS DRIVEN115 Astronomy Space scienceSPECTRAL-LINESQC Physics13. Climate actionSpace and Planetary SciencebusinessHeliosphereSun: atmosphereELECTRON-DENSITY
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