Characteristic analysis of a complex two-dimensional magnetohydrodynamic bow shock flow with steady compound shocks
- 19 February 1999
- journal article
- conference paper
- Published by AIP Publishing in Physics of Plasmas
- Vol. 6 (3) , 954-969
- https://doi.org/10.1063/1.873336
Abstract
A simple, compact, and systematic derivation is given of the characteristic properties of the magnetohydrodynamic (MHD) equations with two independent variables (time-dependent MHD in the plane and steady MHD in the plane), based on the symmetrizable Galilean invariant form of the equations and using a matrix approach. A numerically obtained stationary planar field-aligned MHD bow shock flow with interacting shocks is then analyzed in terms of hyperbolic and elliptic regions, steady characteristics, limiting lines, and allowed shock transitions. With the help of this analysis, a wave structure present in the bow shock flow can be interpreted as a double steady compound shock. This interpretation is based on the complete analogy demonstrated in our analysis, between the characteristic structure of this novel steady compound shock and the characteristic structure of the well-known time-dependent MHD compound shock.
Keywords
This publication has 31 references indexed in Scilit:
- Complex magnetohydrodynamic bow shock topology in field-aligned low-β flow around a perfectly conducting cylinderPhysics of Plasmas, 1998
- Heliosphere in the magnetized local interstellar medium: Results of a three‐dimensional MHD simulationJournal of Geophysical Research, 1998
- Dynamics of hot filaments in a tokamak plasmaJournal of Plasma Physics, 1998
- On the relation of limiting characteristics to critical surfaces in magnetohydrodynamic flowsMonthly Notices of the Royal Astronomical Society, 1996
- Solar activity and the coronaSolar Physics, 1996
- Damping of global Alfven waves in tokamaks due to resonant absorptionPlasma Physics and Controlled Fusion, 1992
- Magnetohydrodynamic solar/stellar wind modelsComputer Physics Reports, 1990
- Axisymmetric ideal MHD stellar wind flowJournal of Geophysical Research, 1978
- Reducible Problems in Magneto-Fluid Dynamic Steady FlowsReviews of Modern Physics, 1960
- Hydromagnetic Plane Steady Flow in Compressible Ionized GasesProgress of Theoretical Physics, 1959