Search results for "computational"

showing 10 items of 5884 documents

3D MHD MODELING of TWISTED CORONAL LOOPS

2016

We perform MHD modeling of a single bright coronal loop to include the interaction with a non-uniform magnetic field. The field is stressed by random footpoint rotation in the central region and its energy is dissipated into heating by growing currents through anomalous magnetic diffusivity that switches on in the corona above a current density threshold. We model an entire single magnetic flux tube, in the solar atmosphere extending from the high-beta chromosphere to the low-beta corona through the steep transition region. The magnetic field expands from the chromosphere to the corona. The maximum resolution is ~30 km. We obtain an overall evolution typical of loop models and realistic loo…

Sun: activity; Sun: corona; Astronomy and Astrophysics; Space and Planetary Science010504 meteorology & atmospheric sciencescorona [Sun]Astrophysics::High Energy Astrophysical PhenomenaNDASFOS: Physical sciences01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaSun: activity0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsQB Astronomyactivity [Sun]010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesQBPhysicsFlux tubeSun: coronaAstronomy and AstrophysicsCoronal loopCoronaMagnetic fluxComputational physicsMagnetic fieldQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsMagnetic diffusivity
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Tracing the ICME plasma with a MHD simulation

2021

The determination of the chemical composition of interplanetary coronal mass ejection (ICME) plasma is an open issue. More specifically, it is not yet fully understood how remote sensing observations of the solar corona plasma during solar disturbances evolve into plasma properties measured in situ away from the Sun. The ambient conditions of the background interplanetary plasma are important for space weather because they influence the evolutions, arrival times, and geo-effectiveness of the disturbances. The Reverse In situ and MHD APproach (RIMAP) is a technique to reconstruct the heliosphere on the ecliptic plane (including the magnetic Parker spiral) directly from in situ measurements a…

Sun: coronal mass ejections (CMEs)FOS: Physical sciencesInterplanetary mediumAstrophysicsSpace weathermagnetohydrodynamics (MHD)Physics - Space PhysicsPhysics::Plasma PhysicsAstrophysics::Solar and Stellar AstrophysicsSun: abundancesSolar and Stellar Astrophysics (astro-ph.SR)PhysicsAstronomy and AstrophysicsPlasmasolar-terrestrial relationsSpace Physics (physics.space-ph)Physics - Plasma PhysicsComputational physicsPlasma Physics (physics.plasm-ph)Solar windAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsHeliospheric current sheetMagnetohydrodynamicsInterplanetary spaceflightHeliosphere
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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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Anhamonic finite temperature effects on the Raman and Infrared spectra to determine the crystal structure phase III of solid molecular hydrogen

2013

We present theoretical calculations of the Raman and IR spectra, as well as electronic properties at zero and finite temperature to elucidate the crystal structure of phase III of solid molecular hydrogen. We find that anharmonic finite temperature are particularly important and qualitatively influences the main conclusions. While P6$_3$/m is the most likely candidate for phase III at the nuclear ground state, at finite temperature the C2/c structure appears to be more suitable.

Superconductivity (cond-mat.supr-con)Chemical Physics (physics.chem-ph)Condensed Matter - Other Condensed MatterCondensed Matter - Materials ScienceCondensed Matter - SuperconductivityPhysics - Chemical PhysicsMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesComputational Physics (physics.comp-ph)Physics - Computational PhysicsOther Condensed Matter (cond-mat.other)
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Lifetime of the superconductive state in short and long Josephson junctions

2008

We study the transient statistical properties of short and long Josephson junctions under the influence of thermal and correlated fluctuations. In particular, we investigate the lifetime of the superconductive metastable state finding the presence of noise induced phenomena. For short Josephson junctions we investigate the lifetime as a function both of the frequency of the current driving signal and the noise intensity and we find how these noise-induced effects are modified by the presence of a correlated noise source. For long Josephson junctions we integrate numerically the sine-Gordon equation calculating the lifetime as a function of the length of the junction both for inhomogeneous a…

SuperconductivityPhysicsJosephson effectCondensed matter physicsCondensed Matter - SuperconductivityFOS: Physical sciencesBiasingCondensed Matter PhysicsSignalNoise (electronics)Settore FIS/03 - Fisica Della MateriaElectronic Optical and Magnetic MaterialsSuperconductivity (cond-mat.supr-con)MetastabilityCondensed Matter::SuperconductivityComputational methods in statistical physics and nonlinear dynamics Noise Fluctuations Josephson devices.Transient (oscillation)Maxima
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Quantum Monte Carlo Simulations of Models Related to High-Tc Superconductivity on a Transputer Network

1991

Much of the insight into the low temperature behaviour of two-dimensional quantum antiferromagnets has been recently obtained by extensive Monte Carlo. These models are relevant in the study of the magnetic behaviour of high Tc compounds containing copper-oxide layers. While of little technical importance, the physical properties of these models are certainly important for the understanding of the new type of behaviour that leads to superconductivity under certain conditions.

SuperconductivityPhysicsQuantum Monte CarloMonte Carlo methodGeneral Physics and AstronomyStatistical and Nonlinear PhysicsComputer Science ApplicationsComputational Theory and MathematicsDynamic Monte Carlo methodHigh tc superconductivityStatistical physicsQuantumMathematical PhysicsMonte Carlo molecular modelingTransputer networkInternational Journal of Modern Physics C
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G1-Blend between a Differentiable Superquadric of Revolution and a Plane or a Sphere Using Dupin Cyclides

2008

In this article, we present a method to perform G1-continuous blends between a differentiable superquadric of revolution and a plane or a sphere using Dupin cyclides. These blends are patches delimited by four lines of curvature. They allow to avoid parameterization problems that may occur when parametric surfaces are used. Rational quadratic Bezier curves are used to approximate the principal circles of the Dupin cyclide blends and thus a complex 3D problem is now reduced to a simpler 2D problem. We present the necessary conditions to be satisfied to create the blending patches and illustrate our approach by a number of superellipsoid/plane and superellipsoid/sphere blending examples.

SuperellipsoidParametric surfacePlane (geometry)Mathematical analysisDupin cyclideGeometryBézier curveDifferentiable functionCurvatureComputational geometryMathematics2008 IEEE International Conference on Signal Image Technology and Internet Based Systems
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Binding abilities of a chiral calix[4]resorcinarene: a polarimetric investigation on a complex case of study

2017

Polarimetry was used to investigate the binding abilities of a chiral calix[4]resorcinarene derivative, bearing L-proline subunits, towards a set of suitably selected organic guests. The simultaneous formation of 1:1 and 2:1 host–guest inclusion complexes was observed in several cases, depending on both the charge status of the host and the structure of the guest. Thus, the use of the polarimetric method was thoroughly revisited, in order to keep into account the occurrence of multiple equilibria. Our data indicate that the stability of the host–guest complexes is affected by an interplay between Coulomb interactions, π–π interactions, desolvation effects and entropy-unfavorable conformatio…

Supramolecular chemistryPolarimetryhost–guest complexes010402 general chemistry01 natural scienceshost-guest complexesFull Research Papersupramolecular chemistrylcsh:QD241-441chemistry.chemical_compoundlcsh:Organic chemistryComputational chemistryp-nitroanilinesDesolvationlcsh:Sciencepolarimetrycalix[4]resorcinarene010405 organic chemistryChemistryOrganic ChemistryHost-guest complexeSettore CHIM/06 - Chimica OrganicaResorcinarene0104 chemical sciencesChemistrylcsh:QP-nitroanilineDerivative (chemistry)Beilstein Journal of Organic Chemistry
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On the use of reduced active space in CASSCF calculations

2014

Abstract The complete active space self-consistent field (CASSCF) method is one of the most used approaches to explore theoretically non-adiabatic photochemical processes in medium-size molecular systems. It is also frequently utilized in direct dynamics studies because this method offers a reliable description of the electronic state mixing in the regions of surface crossings (conical intersections). In this context, however, the large computational demand required to perform such on-the-fly molecular dynamics simulations using CASSCF as the electronic structure method means that only relatively small active space can be handled (typically not more than 10 electrons distributed in 10 orbit…

Surface (mathematics)010304 chemical physicsField (physics)ChemistryContext (language use)Electronic structureConical surface010402 general chemistryCondensed Matter Physics01 natural sciencesBiochemistryMolecular physics0104 chemical sciencesMolecular dynamicsComputational chemistry0103 physical sciencesPotential energy surfaceComplete active spacePhysical and Theoretical Chemistryta116ComputingMilieux_MISCELLANEOUS
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Computation of the topological type of a real Riemann surface

2014

We present an algorithm for the computation of the topological type of a real compact Riemann surface associated to an algebraic curve, i.e., its genus and the properties of the set of fixed points of the anti-holomorphic involution τ \tau , namely, the number of its connected components, and whether this set divides the surface into one or two connected components. This is achieved by transforming an arbitrary canonical homology basis to a homology basis where the A \mathcal {A} -cycles are invariant under the anti-holomorphic involution  τ \tau .

Surface (mathematics)Algebra and Number TheoryApplied MathematicsRiemann surfaceMathematicsofComputing_GENERALHomology (mathematics)Type (model theory)TopologyComputational Mathematicssymbols.namesakeGenus (mathematics)symbolsAlgebraic curveCompact Riemann surfaceInvariant (mathematics)MathematicsMathematics of Computation
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