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Titlebook: Godunov Methods; Theory and Applicati E. F. Toro Book 2001 Kluwer Academic / Plenum Publishers, New York 2001 Mathematica.algorithms.discre

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樓主: Amalgam
11#
發(fā)表于 2025-3-23 10:52:58 | 只看該作者
Hyperbolic-Elliptic Splitting for the Pseudo-Compressible Euler Equations,imilar decomposition for the incompressible equations is proposed. The artificial compressibility approach is used make the incompressible Euler equations hyperbolic in time. The canonical form of this pseudo-compressible system consists in an hyperbolic component corresponding to the convection of
12#
發(fā)表于 2025-3-23 16:40:48 | 只看該作者
Godunov Solution of Shallow Water Equations on Curvilinear and Quadtree Grids,ted and Cartesian quadtree grids. The shallow water equations are written in a new matrix-hyperbolic form suitable for spatially non-uniform bed profiles. The equations are discretised spatially using finite volumes and temporally using the fourth-order Runge-Kutta method. Convection terms are model
13#
發(fā)表于 2025-3-23 19:51:13 | 只看該作者
A Higher-Order-Accurate Reconstruction for the Computation of Compressible Flows on Cell-Vertex Tripwind discretization of the inviscid terms is obtained by using a new bi-linear reconstruction and a standard flux-difference-splitting scheme, whereas a standard central discretization is used for the viscous terms. The method is validated by computing the transonic inviscid flow in a two-dimension
14#
發(fā)表于 2025-3-24 01:12:34 | 只看該作者
15#
發(fā)表于 2025-3-24 02:39:19 | 只看該作者
16#
發(fā)表于 2025-3-24 08:41:25 | 只看該作者
s of difference schemes are consistent with the E-condition and discuss the quality of numerical result from the viewpoint of the E-condition. The consistency with E-condition gives the convergence proof in .∩.-category as well.
17#
發(fā)表于 2025-3-24 12:22:32 | 只看該作者
18#
發(fā)表于 2025-3-24 17:40:49 | 只看該作者
,Euklidische und unit?re R?ume (LA),ed energy deposition of ~ 10. - 10. erg/s within a 30° cone around the rotation axis of the progenitor star. The generated jet flow is strongly beamed ( ? few degrees) and reaches the surface of the stellar progenitor (r ≈ 310. cm) intact. At break-out the maximum Lorentz factor of the jet flow is a
19#
發(fā)表于 2025-3-24 19:58:09 | 只看該作者
,Zusammenfassungen und übersichten,iemann solvers for unsteady inviscid flows featuring shock-diffraction, multiple shock interactions and Richtmyer-Meshkov instability. The solvers have been used in conjunction with MUSCL interpolation for obtaining high resolution and a second-order accurate implicit-unfactored method. The latter p
20#
發(fā)表于 2025-3-24 23:09:17 | 只看該作者
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