Search results for " Conduction"

showing 10 items of 373 documents

Accretion shock on CTTSs and its X-ray emission

2009

High spectral resolution X-ray observations of classical T Tauri stars (CTTSs) demonstrate the presence of plasma at T~2-3×10^6 K and ne~10^11-10^13 cm-3. Stationary models suggest that this emission is due to shock-heated accreting material. We address this issue by a 1-D hydrodynamic model of the impact of the accretion flow onto a chromosphere of a CTTS with the aim of investigating the stability of accretion shock and the role of the chromosphere. Our simulations include the effects of gravity, radiative losses from optically thin plasma, the thermal conduction and a detailed modeling of the stellar chromosphere. Here we present the results of a simulation based on the parameters of the…

Shock wavePhysicsPlanetary bow shocksAstrophysics::High Energy Astrophysical Phenomenainterplanetary shocksPlasmaAstrophysicsNumerical approximation and analysisThermal conductionAccretion (astrophysics)T Tauri starSettore FIS/05 - Astronomia E AstrofisicaX-ray emission spectra and fluorescenceRadiative transferHydrodynamicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsSpectral resolutionChromosphereAstrophysics::Galaxy Astrophysics
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Crushing of interstellar gas clouds in supernova remnants II. X-ray emission

2006

AIMS. We study and discuss the time-dependent X-ray emission predicted by hydrodynamic modeling of the interaction of a SNR shock wave with an interstellar gas cloud. The scope includes: 1) to study the correspondence between modeled and X-ray emitting structures, 2) to explore two different physical regimes in which either thermal conduction or radiative cooling plays a dominant role, and 3) to investigate the effects of the physical processes at work on the emission of the shocked cloud in the two different regimes. METHODS. We use a detailed hydrodynamic model, including thermal conduction and radiation, and explore two cases characterized by different Mach numbers of the primary shock: …

Shock wavePhysicsRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and Astrophysicsshock wavesAstrophysicsRadiationThermal conductionAstrophysicsISM: cloudsCoronaX-rays: ISMShock (mechanics)Supernovasymbols.namesakeMach numberSpace and Planetary SciencehydrodynamicssymbolsAstrophysics::Galaxy AstrophysicsISM: supernova remnants
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Hydrodynamic Modeling of Accretion Impacts in Classical T Tauri Stars: Radiative Heating of the Pre-shock Plasma

2016

Context. It is generally accepted that, in classical T Tauri stars, the plasma from the circumstellar disc accretes onto the stellar surface with free-fall velocity and the impact generates a shock. The impact region is expected to contribute to emission in different spectral bands; many studies have confirmed that the X-rays arise from the post-shock plasma but, otherwise, there are no studies in the literature investigating the origin of the observed UV emission which is apparently correlated to accretion. Aims: We investigated the effect of radiative heating of the infalling material by the post-shock plasma at the base of the accretion stream, with the aim to identify in which region a …

Shock waveRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAccretion accretion diskSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsX-rays: starIrradiationEmission spectrum010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsHydrodynamicPlasmaAstronomy and AstrophysicThermal conductionAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsShock waveSpace and Planetary ScienceStars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysics
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Quantification of synchronization during atrial fibrillation by Shannon entropy: Validation in patients and computer model of atrial arrhythmias

2005

Atrial fibrillation (AF), a cardiac arrhythmia classically described as completely desynchronized, is now known to show a certain amount of synchronized electrical activity. In the present work a new method for quantifying the level of synchronization of the electrical activity recorded in pairs of atrial sites during atrial fibrillation is presented. A synchronization index (Sy) was defined by quantifying the degree of complexity of the distribution of the time delays between sites by Shannon entropy estimation. The capability of Sy to discriminate different AF types in patients was assessed on a database of 60 pairs of endocardial recordings from a multipolar basket catheter. The analysis…

Signal processingmedicine.medical_specialtyTime delaysPhysiologyEntropyBiomedical EngineeringBiophysicsSensitivity and SpecificitySynchronizationHeart Conduction SystemArrhythmia (mechanisms)Internal medicinePhysiology (medical)medicineHumansIn patientDiagnosis Computer-AssistedMathematicsBody Surface Potential MappingModels CardiovascularCardiac arrhythmiaReproducibility of ResultsAtrial fibrillationAtrial arrhythmiasComputer simulationmedicine.diseaseAtrial fibrillationElectrophysiologyElectrophysiologymedicine.anatomical_structureBiophysicCardiologyRight atriumAlgorithms
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New experiment to model self-organized critical transport and accumulation of melt and hydrocarbons from their source rocks

2001

A new, simple, and easily reproducible experiment was designed to simulate the production, accumulation, and transport of melt within rock. The transport was found to be of the self-organized critical type. The emergence of self-organized criticality is explained by the availability of hydrofracture propagation as a rapid or ballistic transport mechanism. This mechanism also serves as a mechanism for stepwise accumulation. These findings are confirmed by a numerical model, which shows the emergence of self-organized critical behavior when Darcian transport cannot accommodate transport and the dormant transport mechanism of hydrofracture propagation is activated. Ballistic and self-organized…

Source rockBallistic conductionGeologyGeotechnical engineeringPetrologyGeologyGeology
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Resolving the Fundamentals of Magnetotransport in Metals with Ultrafast Terahertz Spectroscopy

2016

Using terahertz spectroscopy we directly resolved the fundamentals of spin-dependent conductivity in ferromagnetic metals. We quantified the differences in conduction by Fermi-level electrons with opposite spins on the sub-100 fs timescale of electron momentum scattering.

SpinsFerromagnetismCondensed matter physicsScatteringChemistryCondensed Matter::Strongly Correlated ElectronsElectronConductivityThermal conductionTerahertz spectroscopy and technologyMagnetic fieldInternational Conference on Ultrafast Phenomena
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On a set of data for the membrane potential in a neuron

2006

We consider a set of data where the membrane potential in a pyramidal neuron is measured almost continuously in time, under varying experimental conditions. We use nonparametric estimates for the diffusion coefficient and the drift in view to contribute to the discussion which type of diffusion process is suitable to model the membrane potential in a neuron (more exactly: in a particular type of neuron under particular experimental conditions).

Statistics and ProbabilityModels NeurologicalNeural ConductionAction PotentialsTetrodotoxinType (model theory)Statistics NonparametricGeneral Biochemistry Genetics and Molecular BiologyMembrane PotentialsSet (abstract data type)MiceStatisticsAnimalsDiffusion (business)MathematicsCerebral CortexNeuronsMembrane potentialStochastic ProcessesQuantitative Biology::Neurons and CognitionGeneral Immunology and MicrobiologyStochastic processPyramidal CellsApplied MathematicsNonparametric statisticsGeneral MedicineElectrophysiologyElectrophysiologynervous systemDiffusion processModeling and SimulationPotassiumGeneral Agricultural and Biological SciencesBiological systemAlgorithmsMathematical Biosciences
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Comment on "Ecological importance of the thermal emissivity of avian eggshells".

2012

Eggshell emissivity must be known to determine accurately the cooling rate of avian eggs when the parent, after heating by conduction during the incubation, is temporarily absent. We estimate possible values of eggshell emissivities from in-situ measurements and spectral libraries. Emissivity is near to 1 (probably higher than 0.95) and therefore its effect on cooling rate may be negligible, with differences between the temperature of the egg assuming a value of e=0.95 and that of a blackbody (e=1) below 0.2 °C.

Statistics and ProbabilityThermal infraredMaterials scienceGeneral Immunology and MicrobiologyEcologyApplied MathematicsGeneral MedicineThermal conductionModels BiologicalGeneral Biochemistry Genetics and Molecular BiologyBirdsEgg ShellCooling rateThermal radiationModeling and SimulationEmissivityAnimalsBlack-body radiationEggshellGeneral Agricultural and Biological SciencesBody Temperature RegulationJournal of theoretical biology
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A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method

2021

We have demonstrated that the Transition Region Adaptive Conduction (TRAC) method permits fast and accurate numerical solutions of the field-aligned hydrodynamic equations, successfully removing the influence of numerical resolution on the coronal density response to impulsive heating. This is achieved by adjusting the parallel thermal conductivity, radiative loss, and heating rates to broaden the transition region (TR), below a global cutoff temperature, so that the steep gradients are spatially resolved even when using coarse numerical grids. Implementing the original 1D formulation of TRAC in multi-dimensional magnetohydrodynamic (MHD) models would require tracing a large number of magne…

Sun: flaresMagnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencescorona [Sun]Field lineNDASFOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencestransition region [Sun]0103 physical sciencesRadiative transferQB AstronomyMagnetohydrodynamic driveflares hydrodynamics [Sun]Sun: transition region010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencescomputer.programming_languageQBPhysicsSun: coronaSun: chromosphereAstronomy and AstrophysicsTRACCoronal loopThermal conductionComputational physicsMagnetic fieldQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHydrodynamicsMagnetohydrodynamicscomputerSettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo Circumterrestre
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Development of an Inductive NIS Thermometer

2012

We have studied an inductive readout for normal metal-insulator-superconductor (NIS) tunnel junctions by using on-chip planar inductors and a DC SQUID (superconducting quantum interference device) to develop a sensitive and fast thermometer for studies of nanoscale heat conduction and bolometry. Our initial results show the feasibility of the concept, with a good sensitivity for temperatures below 1 K for aluminum as the superconductor when voltage biased close to the superconductor energy gap. peerReviewed

SuperconductivityHistoryMaterials sciencesuprajohtavuusbusiness.industryBand gapElectrical engineeringThermal conductionCondensed Matter::Mesoscopic Systems and Quantum Hall EffectComputer Science ApplicationsEducationTunnel junctionThermometerCondensed Matter::SuperconductivityInstrumentation and measurementPlanar inductorOptoelectronicsbusinessSensitivity (electronics)Voltage
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