An Approximate Riemann Solver for Ideal Magnetohydrodynamics
β Scribed by Wenlong Dai; Paul R. Woodward
- Publisher
- Elsevier Science
- Year
- 1994
- Tongue
- English
- Weight
- 877 KB
- Volume
- 111
- Category
- Article
- ISSN
- 0021-9991
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β¦ Synopsis
To construct numerical schemes of the Godunov type for solving magnetohydrodynamical (MHO) problems, an approximate method of solving the MHD Riemann problem is required in order to calculate the time-averaged fluxes at the interfaces of numerical zones. Such an MHD Riemann solver is presented here which treats alf waves entanating from the initial discontinuity as themselves discontinuous. Ihus shock jump romditions aro used for tirefactions, which limits the applicability of this work to weak rarefactions, the case most important for computation. The soletions from our approximate MHD Riamn solver consist of two fast waves (either shock or rarefaction) two rotational discontinuities, two rarefaction waves (either shock or rarefaction ), and one contact discontinuity for a general MHD Riemann problem. In order to display rotational discontinuities, a three-component model is necessary. Only under very limited circumstances is there no rotational discontinuity involved and thus the two component approximation may be used in the MHD Riemann problem. The solutions of the MHD Riemann problem in the shock tube problem which generates the compound wave in the earlier work contain two fast rarefaction waves, two slow shocks, one contact discontinuity, and one rotational discontinuity in our formalism. 'c) 1994 Academic Press, Inc.
π SIMILAR VOLUMES
In this paper, we adapt to the ideal 1D lagrangian MHD equations a class of numerical schemes of order one in time and space presented in an earlier paper and applied to the gas dynamics system. They use some properties of systems of conservation laws with zero entropy flux which describe fluid mode
For simplicity we will restrict the following presentation to flows with statistically two space dimensions, i.e., a variable vector W = (Ο, ΟU, ΟV, Ο E, Ο R 11 , Ο R 22 , Ο R 33 , Ο R 12 ) t , such that we can write the system in matrix-vector notation