Search results for "modeling"

showing 10 items of 4489 documents

Classes of orbits in the main problem of satellite theory

1986

We consider the main problem in satellite theory restricted to the polar plane. For suitable values of the energy the system has two unstable periodic orbits. We classify the trajectories in terms of their ultimate behavior with respect these periodic orbits in: oscillating, asymptotic and capture orbits. We study the energy level set and the existence and properties of the mentioned types of motion.

PhysicsApplied MathematicsMotion (geometry)Astronomy and AstrophysicsCollisionCelestial mechanicsComputational MathematicsLevel setClassical mechanicsSpace and Planetary ScienceModeling and SimulationOrbit (dynamics)SatellitePolar planeMathematical PhysicsEnergy (signal processing)Celestial Mechanics
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Dipole soliton solution for the homogeneous high-order nonlinear Schrödinger equation with cubic–quintic–septic non-Kerr terms

2015

Abstract We consider a high-order nonlinear Schrodinger equation with third- and fourth-order dispersions, cubic–quintic–septic nonlinearities, self-steepening, and instantaneous Raman response. This equation models describes ultra-short optical pulse propagation in highly-nonlinear media. The ansatz solution of Choudhuri and Porsezian (in Ref. [16]) is adapted to investigate solutions composed of the product of bright and dark solitary waves. Parametric conditions for the existence of the derived soliton solutions are given and their stabilities are numerically discussed. These exact solutions provide insight into balance mechanisms between several high-order nonlinearities of different na…

PhysicsApplied MathematicsSoliton (optics)Quintic functionDipolesymbols.namesakeClassical mechanicsModeling and SimulationProduct (mathematics)Quantum mechanicssymbolsRaman spectroscopyNonlinear Schrödinger equationParametric statisticsAnsatzApplied Mathematical Modelling
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Probing the internal solar magnetic field through g-modes

2006

The observation of g-mode candidates by the SoHO mission opens the possibility of probing the internal structure of the solar radiative zone (RZ) and the solar core more directly than possible via the use of the p-mode helioseismology data. We study the effect of rotation and RZ magnetic fields on g-mode frequencies. Using a self-consistent static MHD magnetic field model we show that a 1% g-mode frequency shift with respect to the Solar Seismic Model (SSeM) prediction, currently hinted in the GOLF data, can be obtained for magnetic fields as low as 300 kG, for current measured modes of radial order n=-20. On the other hand, we also argue that a similar shift for the case of the low order g…

PhysicsAstrophysics (astro-ph)Frequency shiftFOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsRotationAstrophysicsRadiation zoneMagnetic fieldComputational physicsSolar coreSpace and Planetary ScienceSeismic modelingPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsHelioseismologyMagnetohydrodynamics
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On the effect of damping on dispersion curves in plates

2013

AbstractThis paper presents a study on quantitative prediction and understanding of time-harmonic wave characteristics in damped plates. Material dissipation is modelled by using complex-valued velocities of free dilatation and shear waves in an unbounded volume. As a numerical example, solution of the classical Rayleigh–Lamb problem for a viscoelastic plate is presented to illustrate and discuss the role of dissipation in the cut-off phenomenon and in the phenomenon of veering for dispersion curves. These phenomena are explained in more detail considering a simple model, which allows accurate asymptotic analysis of the perturbation of dispersion curves in the regions of cut-off and veering.

PhysicsAsymptotic analysisShear wavesMechanical EngineeringApplied MathematicsPerturbation (astronomy)ViscoelasticityMechanicsDispersionDissipationCondensed Matter PhysicsCoupled waveguideViscoelasticityRayleigh–Lamb problemMaterials Science(all)Mechanics of MaterialsModeling and SimulationModelling and SimulationGuided wavesGeneral Materials ScienceDispersion (water waves)International Journal of Solids and Structures
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Flare diagnostics from loop modeling of a stellar flare observed with XMM-Newton

2006

Abstract XMM-Newton data of an X-ray flare observed on Proxima Centauri provide detailed and challenging constraints for flare modeling. The comparison of the data with the results of time-dependent hydrodynamic loop modeling of this flare allows us to constrain not only the loop morphology, but also the details of the heating function. The results show that even a complex flare event like this can be described with a relatively few – though constrained – components: two loop systems, i.e., a single loop and an arcade, and two heat components, an intense pulse probably located at the loop footpoints followed by a low gradual decay distributed in the coronal part of the loop. The similarity …

PhysicsAtmospheric ScienceSolar flareStars: X-raysAstrophysics::High Energy Astrophysical PhenomenaFlare starAerospace EngineeringAstronomyAstronomy and AstrophysicsAstrophysicsPulse (physics)law.inventionStars: flaresLoop (topology)GeophysicsSpace and Planetary SciencelawPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsGeneral Earth and Planetary SciencesStars: coronaeLoop modelingSingle loopEvent (particle physics)Flare
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A Brightening Coronal Loop Observed byTRACE. II. Loop Modeling and Constraints on Heating

2000

This is the second of two papers dedicated to the brightening of a coronal loop observed by the Transition Region and Coronal Explorer (TRACE) on 1998 June 26; it aims at hydrodynamic modeling of the brightening. Since the loop geometry is practically unchanged during the brightening, the evolution of the plasma confined in the loop is described with a one-dimensional hydrodynamic time-dependent numerical model, and from the results the emission along the loop in the TRACE 171 A band is synthesized. The information from Paper I is used to derive the geometry and the initial configuration of the loop as well as for comparison with the results of the model. The modeling is focused to determin…

PhysicsBrightnessPhase (waves)Gamma rayAstronomy and AstrophysicsPlasmaAstrophysicsCoronal loopComputational physicsLoop (topology)Space and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsLoop modelingConstant (mathematics)The Astrophysical Journal
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Balance equation of generalised sub-grid scale (SGS) turbulent kinetic energy in a new tensorial dynamic mixed SGS model

2000

A new dynamic model is proposed in which the eddy viscosity is defined as a symmetric second rank tensor, proportional to the product of a turbulent length scale with an ellipsoid of turbulent velocity scales. The employed definition of the eddy viscosity allows to remove the local balance assumption of the SGS turbulent kinetic energy formulated in all the dynamic Smagorinsky-type SGS models. Furthermore, because of the tensorial structure of the eddy viscosity the alignment assumption between the principal axes of the SGS turbulent stress tensor and the resolved strain-rate tensor is equally removed, an assumption which is employed in the scalar eddy viscosity SGS models. The proposed mod…

PhysicsCauchy stress tensorTurbulenceScalar (physics)Turbulence modelingGeneral Physics and AstronomyMaxwell stress tensorMechanicsPhysics::Fluid DynamicsMechanics of MaterialsTurbulence kinetic energyGeneral Materials ScienceStatistical physicsTensorLarge eddy simulation
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Lack of long-range order in confined two-dimensional model colloidal crystals.

2006

We investigate the nature of the ordered phase for a model of colloidal particles confined within a quasi-one-dimensional (Q1D) strip between two parallel boundaries, or walls, separated a distance $D$ in two dimensions (2D). Using Monte Carlo simulations we find that at densities typical of the bulk 2D triangular solid the order in the D1D strip is determined by the nature of the boundaries. While the order is enhanced for a suitably corrugated boundary potential, for a uniformly repulsive smooth boundary potential ordering normal to the walls is enhanced (``layering''), but destroyed parallel to the wall.

PhysicsColloidRange (particle radiation)Condensed matter physicsBoundary potentialPhase (matter)Monte Carlo methodOrder (ring theory)Dimensional modelingColloidal crystalPhysical review. E, Statistical, nonlinear, and soft matter physics
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Simple sampling Monte Carlo methods

2005

PhysicsComputer scienceMonte Carlo methodSampling (statistics)Markov chain Monte CarloHybrid Monte Carlosymbols.namesakeSimple (abstract algebra)symbolsDynamic Monte Carlo methodMonte Carlo integrationMonte Carlo method in statistical physicsQuasi-Monte Carlo methodStatistical physicsMonte Carlo molecular modeling
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Limits of lateral expansion in two-dimensional materials with line defects

2021

The flexibility of two-dimensional (2D) materials enables static and dynamic ripples that are known to cause lateral contraction, shrinking of the material boundary. However, the limits of 2D materials' \emph{lateral expansion} are unknown. Therefore, here we discuss the limits of intrinsic lateral expansion of 2D materials that are modified by compressive line defects. Using thin sheet elasticity theory and sequential multiscale modeling, we find that the lateral expansion is inevitably limited by the onset of rippling. The maximum lateral expansion $\chi_{max}\approx 2.1\cdot t^2\sigma_d$, governed by the elastic thickness $t$ and the defect density $\sigma_d$, remains typically well belo…

PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsPhysics and Astronomy (miscellaneous)Condensed matter physicsBoundary (topology)SigmaFOS: Physical sciencesApproxLateral expansionMultiscale modelingkimmoisuusStrain engineeringRipplingMesoscale and Nanoscale Physics (cond-mat.mes-hall)grafeeniGeneral Materials SciencesimulointiohutkalvotContraction (operator theory)
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