An approximate Riemann solver for relativistic magnetohydrodynamics

被引：30
|
作者：
Koldoba, AV
Kuznetsov, OA
Ustyugova, GV
机构：
[1] Inst Math Modelling, Moscow 125047, Russia
[2] MV Keldysh Appl Math Inst, Moscow 125047, Russia
[3] Russian Acad Sci, Inst Astron, Moscow, Russia
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2002年 / 333卷 / 04期
关键词：
MHD; relativity; shock waves; methods : numerical;
D O I：
10.1046/j.1365-8711.2002.05474.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A Godunov-type scheme for relativistic magnetohydrodynamic (MHD) equations is developed. We consider the Maxwell equations and dynamic equations for a gas with perfect conductivity in hyperbolic form as was suggested by van Putten. To calculate the fluxes of conservative variables through cells' interfaces we suggest an algorithm for the solution of the linearized Riemann problem. 'Primitive' variables are calculated by solving a non-linear system using the Newton method.
引用
收藏
页码：932 / 942
页数：11
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