Results 11 to 20 of about 1,497,004 (325)

Numerical simulations of sunspots [PDF]

open access: yesProceedings of the International Astronomical Union, 2006
AbstractThe origin, structure and evolution of sunspots are investigated using a numerical model. The compressible MHD equations are solved with physical parameter values that approximate the top layer of the solar convection zone. A three dimensional (3D) numerical code is used to solve the set of equations in cylindrical geometry, with the numerical ...
Alistair Rucklidge   +2 more
openaire   +6 more sources

Numerical Simulations of Generic Singularities [PDF]

open access: yesPhysical Review Letters, 2004
typos ...
A. Rendall   +5 more
openaire   +4 more sources

Numerical simulations of bouncing jets [PDF]

open access: yesInternational Journal for Numerical Methods in Fluids, 2015
SummaryBouncing jets are fascinating phenomenon occurring under certain conditions when a jet impinges on a free surface. This effect is observed when the fluid is Newtonian and the jet falls in a bath undergoing a solid motion. It occurs also for non‐Newtonian fluids when the jets fall in a vessel at rest containing the same fluid.
Bonito, Andrea   +2 more
openaire   +7 more sources

In-shock cooling in numerical simulations [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2002
We model a one-dimensional shock-tube using smoothed particle hydrodynamics and investigate the consequences of having finite shock-width in numerical simulations. We investigate the cooling of gas during passage through the shock for different cooling regimes. For a shock temperature of 10^5K, the maximum temperature of the gas is much reduced and the
Peter A. Thomas, Roger M. Hutchings
openaire   +7 more sources

Numerical Simulations of Turbulent Combustion

open access: yesFluids, 2020
Turbulent burning of gaseous fuels is widely used for energy conversion in stationary power generation, e.g., gas turbines, land transportation, e.g., piston engines, and aviation, e.g., aero‐engine afterburners[...]
Andrei N. Lipatnikov
doaj   +1 more source

Numerical simulations of wave breaking [PDF]

open access: yesESAIM: Mathematical Modelling and Numerical Analysis, 2005
This paper is devoted to the numerical simulation of wave breaking. It presents the results of a numerical workshop that was held during the conference LOMA04. The objective is to compare several mathematical models (compressible or incompressible) and associated numerical methods to compute the flow field during a wave breaking over a reef.
Helluy, Philippe   +12 more
openaire   +5 more sources

Differential Models, Numerical Simulations and Applications

open access: yesAxioms, 2021
Differential models, numerical methods and computer simulations play a fundamental role in applied sciences. Since most of the differential models inspired by real world applications have no analytical solutions, the development of numerical methods and ...
Gabriella Bretti
doaj   +1 more source

Analysis of the inadequacy of determining the spectral characteristics of optical fibre periodic structures by way of numerical modelling

open access: yesMetrology and Measurement Systems, 2020
As part of the work, the error level of simulations of uniform optical-fibre Bragg gratings was determined using the transitionmatrixmethod. The errorswere established by comparing the transmission characteristics of the structures obtained by simulation
Stępniak Piotr, Kisała Piotr
doaj   +1 more source

An approach to consider the arterial residual stresses in modelling of a patient-specific artery

open access: yesAdvances in Mechanical Engineering, 2016
In this work, the residual stress state of a human common carotid artery is predicted using the so-called thermomechanical analogy approach. The purpose of the approach is to enable consistent mapping of residual stresses and the respective configuration
Janez Urevc   +3 more
doaj   +1 more source

Numerical Simulations of M51 [PDF]

open access: yesSymposium - International Astronomical Union, 1999
No conference on the interaction of galaxies would be complete without a contribution on M51 (NGC5194) and its companion NGC5195. Much observational and theoretical work has been carried out to try to understand this interacting pair, and to elucidate the morphological features and weak AGN which are thought to be the result of the interaction.
Andrew Nelson, Mario Antonioletti
openaire   +2 more sources

Home - About - Disclaimer - Privacy