期刊文献+
共找到2篇文章
< 1 >
每页显示 20 50 100
Application of ADER Scheme in MHD Simulation 被引量:1
1
作者 ZHANG Yanyan FENG Xueshang +1 位作者 JIANG Chaowei ZHOU Yufen 《空间科学学报》 CAS CSCD 北大核心 2012年第2期170-181,共12页
The Arbitrary accuracy Derivatives Riemann problem method(ADER) scheme is a new high order numerical scheme based on the concept of finite volume integration,and it is very easy to be extended up to any order of space... The Arbitrary accuracy Derivatives Riemann problem method(ADER) scheme is a new high order numerical scheme based on the concept of finite volume integration,and it is very easy to be extended up to any order of space and time accuracy by using a Taylor time expansion at the cell interface position.So far the approach has been applied successfully to flow mechanics problems.Our objective here is to carry out the extension of multidimensional ADER schemes to multidimensional MHD systems of conservation laws by calculating several MHD problems in one and two dimensions: (ⅰ) Brio-Wu shock tube problem,(ⅱ) Dai-Woodward shock tube problem,(ⅲ) Orszag-Tang MHD vortex problem.The numerical results prove that the ADER scheme possesses the ability to solve MHD problem,remains high order accuracy both in space and time,keeps precise in capturing the shock.Meanwhile,the compared tests show that the ADER scheme can restrain the oscillation and obtain the high order non-oscillatory result. 展开更多
关键词 ADER scheme Generalized Riemann problem mhd numerical simulation HLL scheme
在线阅读 下载PDF
Numerical experiments of fast magnetic reconnection driven by the rapidly expanding plasma
2
作者 Shanshan Xu Jun Lin Zhixing Mei 《Science China(Physics,Mechanics & Astronomy)》 2025年第9期162-176,共15页
Three modes of magnetic reconnection,flux pile-up,Sonnerup,and hybrid,are examined in the context of driven magnetic reconnection via 2D and 2.5D magnetohydrodynamic(MHD)numerical simulations.They result from variance... Three modes of magnetic reconnection,flux pile-up,Sonnerup,and hybrid,are examined in the context of driven magnetic reconnection via 2D and 2.5D magnetohydrodynamic(MHD)numerical simulations.They result from variances in gas pressure and magnetic field strength in the reconnection inflow region.The simulation demonstrates that the Spitzer diffusion region of magnetic reconnection is not just an X-point;instead,it appears as a slim and elongated current sheet that creates two pairs of the slow-mode shock(SS)on either end.These shocks contribute to forming four boundaries that separate the inflow from the outflow.In the regions far from the Spitzer diffusion region,two sets of rotational discontinuity(RD)stand inside the SSs and form the combination of SS and RD structures.The RDs reverse the magnetic field inside the reconnection outflow region,and create a W-shaped magnetic field in that region.The scenario that the rotation of the magnetic field is not caused by an intermediate wave,and the SS is located outside the RD,is consistent with the inference of Priest(Mon.Not.R.Astron.Soc.159,389(1972)),and is contrary to that of Petschek and Thorne(Astrophys.J.147,1157(1967))and Vasyliunas(Rev.Geophys.Space Phys.13,303(1975)). 展开更多
关键词 magnetic reconnction shock waves mhd numerical simulation
原文传递
上一页 1 下一页 到第
使用帮助 返回顶部