A characteristic space-time conservation element and solution element method for conservation laws
A characteristic space-time conservation element and solution element method for conservation laws
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一种特征时空守恒元及守恒律解元法
DOI:
10.1016/j.jcp.2015.02.018
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发表时间:
2015-05
影响因子:
4.1
通讯作者:
Zhang De-Liang
中科院分区:
文献类型:
--
作者:
Shen Hua;Wen Chih-Yung;Zhang De-Liang
In this paper, an upwind space–time conservation element and solution element (CE/SE) method is developed to solve conservation laws. In the present method, the mesh quantity and spatial derivatives are the independent marching variables, which is consistent with the original CE/SE method proposed by Chang (1995)[5]. The staggered time marching strategy and the definition of conservation element (CE) also follow Chang's propositions. Nevertheless, the definition of solution element (SE) is modified from that of Chang. The numerical flux through the interface of two different conservation elements is not directly derived by a Taylor expansion in the reversed time direction as proposed by Chang, but determined by an upwind procedure. This modification does not change the local and global conservative features of the original method. Although, the time marching scheme of mesh variables is the same with the original method, the upwind fluxes are involved in the calculation of spatial derivatives, yielding a totally different approach from that of Chang's method. The upwind procedure breaks the space–time inversion invariance of the original scheme, so that the new scheme can be directly applied to capture discontinuities without spurious oscillations. In addition, the present method maintains low dissipation in a wide range of CFL number (from 10− 6 to 1). Furthermore, we extend the upwind CE/SE method to solve the Euler equations by adopting three different approximate Riemann solvers including Harten, Lax and van Leer (HLL) Riemann solver, contact discontinuity restoring HLLC Riemann solver and mathematically rigorous Roe Riemann solver. Extensive numerical examples are carried out to demonstrate the robustness of the present method. The numerical results show that the new CE/SE solvers perform improved resolutions.
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影响因子:
6.5
作者:
G. D. V. Albada;B. Leer;W. Roberts
通讯作者:
G. D. V. Albada;B. Leer;W. Roberts
影响因子:
2.2
作者:
E. Toro;M. Spruce;W. Speares
通讯作者:
E. Toro;M. Spruce;W. Speares
DOI:
10.2514/6.2005-4355
发表时间:
2013-07
期刊:
--
影响因子:
--
作者:
Sin-Chung Chang
通讯作者:
Sin-Chung Chang
影响因子:
10.2
作者:
A. Harten;P. Lax;B. Leer
通讯作者:
A. Harten;P. Lax;B. Leer
DOI:
10.1016/j.jcp.2011.06.018
发表时间:
2011-09
期刊:
J. Comput. Phys.
影响因子:
--
作者:
Wanai Li;Yu-xin Ren;Guodong Lei;H. Luo
通讯作者:
Wanai Li;Yu-xin Ren;Guodong Lei;H. Luo