Search results for "hydrodynamic"

showing 10 items of 530 documents

Accretion disk coronae of intermediate polar cataclysmic variables

2017

Context. Intermediate polar cataclysmic variables (IPCV) contain a magnetic, rotating white dwarf surrounded by a magnetically truncated accretion disk. To explain their strong flickering X-ray emission, accretion has been successfully taken into account. Nevertheless, observations suggest that accretion phenomena might not be the only process behind it. An intense flaring activity occurring on the surface of the disk may generate a corona, contribute to the thermal X-ray emission, and influence the system stability. Aims. Our purposes are: investigating the formation of an extended corona above the accretion disk, due to an intense flaring activity occurring on the disk surface; studying t…

Magnetohydrodynamics (MHD)Stars: flareAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMagnetosphereAstrophysics01 natural scienceslaw.inventionAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaIntermediate polarlaw0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar AstrophysicsStars: coronaeX-rays: star0101 mathematics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNovae cataclysmic variableWhite dwarfAstronomy and AstrophysicsAstronomy and AstrophysicThermal conductionAccretion (astrophysics)010101 applied mathematicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaFlareAstronomy & Astrophysics
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Accretion disk coronae of Intermediate Polar Cataclysmic Variables: 3D MagnetoHydroDynamic modeling and thermal X-ray emission

Intermediate Polar Cataclysmic Variables (IPCVs), also known as DQ Her stars after their prototype, are cataclysmic variable stars characterized by the presence of an accreting, magnetic, rapidly rotating white dwarf surrounded by an accretion disk magnetically truncated by the inner magnetosphere of the star. These objects exhibit a magnetic field of the order of few MG, able to disrupt the inner part of the disk but not strong enough to inhibit the formation of a disk. These stars show a strong X-ray emission with a stochastic pulsation that in some cases arise in the inner part of the disk. However, the observations of the X-ray luminosity for these objects do not match the expected valu…

Magnetohydrodynamics (MHD)Stars: novae cataclysmic variableStars: flareStars: coronaeX-rays: starsAccretion accretion discnovae cataclysmic variables; Stars: flare; Magnetohydrodynamics (MHD); Accretion accretion discs; Stars: stars [Stars]
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Total and linearly polarized synchrotron emission from overpressured magnetized relativistic jets

2018

We present relativistic magnetohydrodynamic (RMHD) simulations of stationary overpressured magnetized relativistic jets, which are characterized by their dominant type of energy: internal, kinetic, or magnetic. Each model is threaded by a helical magnetic field with a pitch angle of 45° and features a series of recollimation shocks produced by the initial pressure mismatch, whose strength and number varies as a function of the dominant type of energy. We perform a study of the polarization signatures from these models by integrating the radiative transfer equations for synchrotron radiation using as inputs the RMHD solutions. These simulations show a top-down emission asymmetry produced by …

Magnetohydrodynamics (MHD)active [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies [Radio continuum]01 natural sciencesRadio continuum: galaxiesNuclear physicsAstrophysical jet0103 physical sciences010306 general physics010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)polarizationnumerical [Methods]Methods: numericalLinear polarizationAstronomy and AstrophysicsGalaxies: activePolarization (waves)Synchrotron emissionGalaxies: jetsSpace and Planetary Sciencejets [Galaxies]Astrophysics - High Energy Astrophysical Phenomena
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Contribution of phase-mixing of Alfvén waves to coronal heating in multi-harmonic loop oscillations

2018

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’s Horizon 2020 research and innovation program ( grant agreement No. 647214). This work is supported by the European Research Council under the SeismoSun Research Project No. 321141 (DJP). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 724326). This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf o…

Magnetohydrodynamics (MHD)corona [Sun]010504 meteorology & atmospheric sciencesAstrophysics7. Clean energy01 natural sciencesCoronal heatingQB AstronomyRESONANT ABSORPTIONAstrophysics::Solar and Stellar AstrophysicsQASun: magnetic fields010303 astronomy & astrophysicsQCQBSun: helioseismologymedia_commonPhysicsoscillations [Sun]European researchAstrophysics::Instrumentation and Methods for AstrophysicsKINK OSCILLATIONSmagnetic fields [Sun]MHD WAVESAstrophysics - Solar and Stellar AstrophysicsPhysical SciencesPhysics::Space Physicsatmosphere [Sun]INSTABILITYDirac (software)NDASTRACELibrary scienceAstronomy & AstrophysicsComputer Science::Digital Librariesmagnetohydrodynamics (MHD)0103 physical sciencesmedia_common.cataloged_instancewavesQA Mathematicshelioseismology [Sun]Sun: oscillationsEuropean unionPhase mixing0105 earth and related environmental sciencesScience & TechnologySun: coronaSEISMOLOGYAstronomy and AstrophysicsPhysics::History of PhysicsQC PhysicsSpace and Planetary ScienceWavesTRANSVERSE OSCILLATIONSAstronomy & Astrophysics
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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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Profesors Gunārs Sermons: biobibliogrāfiskais rādītājs

1994

Biobibliogrāfiskajā rādītājā ietverti tehnisko zinātņu doktora, profesora Gunāra Sermona publicētie darbi no 1958. līdz 1994.gadam, kā ari literatūra par viņu.

Magnetohydrodynamics - bibliographical indexЭлектромагнетизм - библиографический указательProfessors of the Latvian University:NATURAL SCIENCES::Physics [Research Subject Categories]Fizika - bibliogrāfiskais rādītājsElectromagnetism - bibliographical indexBiobibliogrāfiskie rādītājiMagnetohidrodinamika - bibliogrāfiskais rādītājsHistory of the University of LatviaМагнитогидродинамика - библиографический указательFizikas zinātņu profesori Latvijas UnivesitātēLatvijas Universitātes vēstureLatvijas Universitātes profesoriElektromagnētisms - bibliogrāfiskais rādītājs
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Исследование некоторых видов неоднородных МГД-течений в применении к задачам управления потоками жидкого металла

1973

Magnetohydrodynamics:NATURAL SCIENCES::Physics::Condensed matter physics::Magnetism [Research Subject Categories]Жидкие металлыМагнитогидродинамикаMagnetohidrodinamikaЭлектромагнитная гидродинамикаМагнитогидродинамические теченияŠķidrie metāli
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High Performance Computing on the COMETA Grid Infrastructure

2008

We present the High Performance Computing (HPC) projects jointly developed at the INAF - Osservatorio Astronomico di Palermo and at the DSFA - Universita` di Palermo which benefits of the Grid infrastructure of COMETA. We have contributed to setup the infrastructure in order to run HPC applications on the Grid. We report on our experience regarding to porting HPC applications to the Grid and to the first HPC simulations performed. The most demanding simulations describe the interaction of a magnetized supernova shock wave with an interstellar gas cloud. We discuss the resources required for the simulations, the performance and the scalability of our code on the Grid, and present first resul…

MagnetohydrodynamicsSettore FIS/05 - Astronomia E AstrofisicaHigh Performance ComputingHydrodynamicsAstrophysics
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Studying Closed Hydrodynamic Models of "In Vivo" DNA Perfusion in Pig Liver for Gene Therapy Translation to Humans.

2016

17 páginas, 6 figuras. En la versión online contiene 3 figuras y 1 tabla en información suplemetaria

Male0301 basic medicineSwineCardiovascular ProceduresGenetic enhancementProtein ExpressionCellGene ExpressionMetal Nanoparticleslcsh:MedicineVascular SurgeryBiochemistryTranslational Research BiomedicalMice0302 clinical medicinePig ModelsGene expressionMedicine and Health SciencesTransgeneslcsh:ScienceMammalsMultidisciplinaryPhysicsGene Transfer TechniquesClassical MechanicsAgricultureAnimal ModelsPerfusionmedicine.anatomical_structureLivermedicine.veinOrgan SpecificityNaked DNA030220 oncology & carcinogenesisVertebratesPhysical SciencesFemalePerfusionPlasmidsResearch ArticleLivestockSurgical and Invasive Medical ProceduresFluid MechanicsBiologyGene deliveryResearch and Analysis MethodsContinuum MechanicsInferior vena cavaCatheterizationGene Delivery03 medical and health sciencesModel OrganismsIn vivoGene Expression and Vector TechniquesmedicineAnimalsHumansMolecular Biology TechniquesMolecular BiologyMolecular Biology Assays and Analysis TechniquesPlasma Proteinslcsh:ROrganismsBiology and Life SciencesProteinsFluid DynamicsDNAGenetic TherapyMolecular biology030104 developmental biologyalpha 1-AntitrypsinAmniotesHydrodynamicslcsh:QGoldPLoS ONE
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